FN Thomson Reuters Web of Science™ VR 1.0 PT J AU Dordevic, SV van der Marel, D Homes, CC AF Dordevic, S. V. van der Marel, D. Homes, C. C. TI Fate of quasiparticles in the superconducting state SO PHYSICAL REVIEW B LA English DT Article ID CONDUCTIVITY; ELECTRODYNAMICS; METALS AB Quasiparticle properties in the superconducting state are masked by the superfluid and are not directly accessible to infrared spectroscopy. We show how one can use a Kramers-Kronig transformation to separate the quasiparticle from superfluid response and extract intrinsic quasiparticle properties in the superconducting state. We also address the issue of a narrow quasiparticle peak observed in microwave measurements, and demonstrate how it can be combined with infrared measurements to obtain a unified picture of electrodynamic properties of cuprate superconductors. C1 [Dordevic, S. V.] Univ Akron, Dept Phys, Akron, OH 44325 USA. [Dordevic, S. V.; van der Marel, D.] Univ Geneva, Dept Phys Mat Condensee, CH-1211 Geneva 4, Switzerland. [Homes, C. C.] Brookhaven Natl Lab, Condensed Matter Phys & Mat Sci Dept, Upton, NY 11973 USA. RP Dordevic, SV (reprint author), Univ Akron, Dept Phys, Akron, OH 44325 USA. EM dsasa@uakron.edu RI van der Marel, Dirk/G-4618-2012 OI van der Marel, Dirk/0000-0001-5266-9847 FU Swiss National Science Foundation (SNSF) [200020-140761] FX This work was supported by the Swiss National Science Foundation (SNSF) through Grant No. 200020-140761. NR 20 TC 1 Z9 1 U1 0 U2 10 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1098-0121 EI 1550-235X J9 PHYS REV B JI Phys. Rev. B PD NOV 17 PY 2014 VL 90 IS 17 AR 174508 DI 10.1103/PhysRevB.90.174508 PG 6 WC Physics, Condensed Matter SC Physics GA AU5HU UT WOS:000345638400008 ER PT J AU Forst, M Frano, A Kaiser, S Mankowsky, R Hunt, CR Turner, JJ Dakovski, GL Minitti, MP Robinson, J Loew, T Le Tacon, M Keimer, B Hill, JP Cavalleri, A Dhesi, SS AF Foerst, M. Frano, A. Kaiser, S. Mankowsky, R. Hunt, C. R. Turner, J. J. Dakovski, G. L. Minitti, M. P. Robinson, J. Loew, T. Le Tacon, M. Keimer, B. Hill, J. P. Cavalleri, A. Dhesi, S. S. TI Femtosecond x rays link melting of charge-density wave correlations and light-enhanced coherent transport in YBa2Cu3O6.6 SO PHYSICAL REVIEW B LA English DT Article ID ORDER; SUPERCONDUCTIVITY; FLUCTUATIONS; PSEUDOGAP AB We use femtosecond resonant soft x-ray diffraction to measure the optically stimulated ultrafast changes of charge-density wave correlations in underdoped YBa2Cu3O6.6. We find that when coherent interlayer transport is enhanced by optical excitation of the apical oxygen distortions, at least 50% of the in-plane charge-density wave order is melted. These results indicate that charge ordering and superconductivity may be competing up to the charge ordering transition temperature, with the latter becoming a hidden phase that is accessible only by nonlinear phonon excitation. C1 [Foerst, M.; Kaiser, S.; Mankowsky, R.; Hunt, C. R.; Cavalleri, A.] Max Planck Inst Struct & Dynam Matter, D-22761 Hamburg, Germany. [Foerst, M.; Kaiser, S.; Mankowsky, R.; Hunt, C. R.; Cavalleri, A.] Ctr Free Electron Laser Sci, D-22761 Hamburg, Germany. [Frano, A.; Loew, T.; Le Tacon, M.; Keimer, B.] Max Planck Inst Solid State Res, D-70569 Stuttgart, Germany. [Frano, A.] Helmholtz Zentrum Berlin Mat & Energie, D-12489 Berlin, Germany. [Hunt, C. R.] Univ Illinois, Dept Phys, Urbana, IL 61802 USA. [Turner, J. J.; Dakovski, G. L.; Minitti, M. P.; Robinson, J.] Natl Accelerator Lab, Stanford Linear Accelerator Ctr, Linac Coherent Light Source, Menlo Pk, CA 94025 USA. [Hill, J. P.] Brookhaven Natl Lab, Condensed Matter Phys & Mat Sci Dept, Upton, NY 11973 USA. [Cavalleri, A.] Univ Oxford, Dept Phys, Clarendon Lab, Oxford OX1 3PU, England. [Dhesi, S. S.] Diamond Light Source, Didcot OX11 0QX, Oxon, England. RP Forst, M (reprint author), Max Planck Inst Struct & Dynam Matter, D-22761 Hamburg, Germany. RI Forst, Michael/D-8924-2012; Kaiser, Stefan/B-7788-2008; Le Tacon, Mathieu/D-8023-2011 OI Kaiser, Stefan/0000-0001-9862-2788; Le Tacon, Mathieu/0000-0002-5838-3724 FU LCLS; University of Hamburg through the BMBF [FSP 301]; Center for Free Electron Laser Science (CFEL); European Research Council under the European Union's Seventh Framework Programme (FP7)/ERC [319286]; Department of Energy, Division of Materials Science and Engineering [DE-AC02-98CH10886]; Stanford University, through the Stanford Institute for Materials Energy Sciences (SIMES); Lawrence Berkeley National Laboratory (LBNL) [DE-AC02-05CH11231] FX Portions of this research were carried out on the SXR Instrument at the Linac Coherent Light Source (LCLS), a division of SLAC National Accelerator Laboratory and an Office of Science user facility operated by Stanford University for the U.S. Department of Energy. The SXR Instrument is funded by a consortium whose membership includes the LCLS, Stanford University, through the Stanford Institute for Materials Energy Sciences (SIMES), Lawrence Berkeley National Laboratory (LBNL, Contract No. DE-AC02-05CH11231), University of Hamburg through the BMBF priority program FSP 301, and the Center for Free Electron Laser Science (CFEL). The research leading to these results has received funding from the European Research Council under the European Union's Seventh Framework Programme (FP7/2007-2013)/ERC Grant Agreement No. 319286 (Q-MAC). Work at Brookhaven National Laboratory was funded by the Department of Energy, Division of Materials Science and Engineering, under Contract No. DE-AC02-98CH10886. NR 25 TC 18 Z9 18 U1 2 U2 28 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1098-0121 EI 1550-235X J9 PHYS REV B JI Phys. Rev. B PD NOV 17 PY 2014 VL 90 IS 18 AR 184514 DI 10.1103/PhysRevB.90.184514 PG 4 WC Physics, Condensed Matter SC Physics GA AU5IQ UT WOS:000345640600007 ER PT J AU Lemery, F Piot, P AF Lemery, F. Piot, P. TI Ballistic bunching of photoinjected electron bunches with dielectric-lined waveguides SO PHYSICAL REVIEW SPECIAL TOPICS-ACCELERATORS AND BEAMS LA English DT Article ID WAKE-FIELD; ACCELERATION; LASER; BEAM; COMPRESSION; GUN AB We describe a simple technique to passively bunch non-ultra-relativistic (less than or similar to 10 MeV) electron bunches produced in conventional photoinjectors. The scheme employs a dielectric-lined waveguide located downstream of the electron source to impress an energy modulation on a picosecond bunch. The energy modulation is then converted into a density modulation via ballistic bunching. The method is shown to support the generation of subpicosecond bunch trains with multi-kA peak currents. The relatively simple technique is expected to find applications in compact, accelerator-based, light sources and advanced beam-driven accelerator methods. C1 [Lemery, F.; Piot, P.] No Illinois Univ, Northern Illinois Ctr Accelerator & Detector Dev, De Kalb, IL 60115 USA. [Lemery, F.; Piot, P.] No Illinois Univ, Dept Phys, De Kalb, IL 60115 USA. [Piot, P.] Fermilab Natl Accelerator Lab, Accelerator Phys Ctr, Batavia, IL 60510 USA. RP Lemery, F (reprint author), No Illinois Univ, Northern Illinois Ctr Accelerator & Detector Dev, De Kalb, IL 60115 USA. OI piot, philippe/0000-0002-4799-292X FU Defense Threat Reduction Agency, Basic Research Award [HDTRA1-10-1-0051]; Department of Energy [DE-FG02-08ER41532, DE-SC0011831]; Northern Illinois University; DOE [DE-AC02-07CH11359] FX This work was supported by the Defense Threat Reduction Agency, Basic Research Award No. HDTRA1-10-1-0051, to Northern Illinois University and by the Department of Energy Contracts No. DE-FG02-08ER41532 and No. DE-SC0011831 with Northern Illinois University. P. P. is partially supported by DOE Contract No. DE-AC02-07CH11359 to the Fermi research alliance LLC. NR 51 TC 4 Z9 4 U1 0 U2 4 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1098-4402 J9 PHYS REV SPEC TOP-AC JI Phys. Rev. Spec. Top.-Accel. Beams PD NOV 17 PY 2014 VL 17 IS 11 AR 112804 DI 10.1103/PhysRevSTAB.17.112804 PG 10 WC Physics, Nuclear; Physics, Particles & Fields SC Physics GA AU6DH UT WOS:000345692500002 ER PT J AU Han, R Ha, JW Xiao, CX Pei, YC Qi, ZY Dong, B Bormann, NL Huang, WY Fang, N AF Han, Rui Ha, Ji Won Xiao, Chaoxian Pei, Yuchen Qi, Zhiyuan Dong, Bin Bormann, Nicholas L. Huang, Wenyu Fang, Ning TI Geometry-Assisted Three-Dimensional Superlocalization Imaging of Single-Molecule Catalysis on Modular Multilayer Nanocatalysts SO ANGEWANDTE CHEMIE-INTERNATIONAL EDITION LA English DT Article DE heterogeneous catalysis; mesoporous silica; multilayer nanocatalysts; platinum; three-dimensional imaging ID CORE-SHELL NANOCATALYSTS; FLUORESCENCE MICROSCOPY; PROPANE DEHYDROGENATION; CARBON NANOTUBES; CRYSTAL SURFACES; IN-SITU; SILICA; ELECTRON; NANOCRYSTALS; REACTIVITY AB To establish the structure-catalytic property relationships of heterogeneous catalysts, a detailed characterization of the three-dimensional (3D) distribution of active sites on a single catalyst is essential. Single-particle catalysis of a modular multilayer catalytic platform that consists of a solid silica core, a mesoporous silica shell, and uniformly distributed Pt nanoparticles sandwiched in between these layers is presented. The first 3D high-resolution super-localization imaging of single fluorescent molecules produced at active sites on the core-shell model nanocatalysts is demonstrated. The 3D mapping is aided by the well-defined geometry and a correlation study in scanning electron microscopy and total internal reflection fluorescence and scattering microscopy. This approach can be generalized to study other nano- and mesoscale structures. C1 [Han, Rui; Ha, Ji Won; Xiao, Chaoxian; Pei, Yuchen; Qi, Zhiyuan; Dong, Bin; Bormann, Nicholas L.; Huang, Wenyu; Fang, Ning] Iowa State Univ, Ames Lab, USDA, Ames, IA 50011 USA. [Han, Rui; Ha, Ji Won; Xiao, Chaoxian; Pei, Yuchen; Qi, Zhiyuan; Dong, Bin; Bormann, Nicholas L.; Huang, Wenyu; Fang, Ning] Iowa State Univ, Dept Chem, Ames, IA 50011 USA. [Ha, Ji Won] Northwestern Univ, Dept Chem, Evanston, IL 60208 USA. RP Huang, WY (reprint author), Iowa State Univ, Ames Lab, USDA, Ames, IA 50011 USA. EM whuang@iastate.edu; nfang@iastate.edu RI Xiao, Chaoxian/E-7339-2013; Huang, Wenyu/L-3784-2014 OI Xiao, Chaoxian/0000-0002-4012-0539; Huang, Wenyu/0000-0003-2327-7259 FU Iowa State University; Ames Laboratory (Royalty Account); U.S. Department of Energy by Iowa State University [DE-AC02-07CH11358] FX This work was supported by U.S. Department of Energy, Office of Basic Energy Sciences, Chemical Sciences, Geosciences, and Biosciences Division (instrument development) and by the Laboratory Directed Research and Development (LDRD) program of the Ames Laboratory (catalysis, platform synthesis). W. H. also thanks Iowa State University and the Ames Laboratory (Royalty Account) for startup funds. The Ames Laboratory is operated for the U.S. Department of Energy by Iowa State University under contract no. DE-AC02-07CH11358. NR 44 TC 8 Z9 8 U1 9 U2 57 PU WILEY-V C H VERLAG GMBH PI WEINHEIM PA BOSCHSTRASSE 12, D-69469 WEINHEIM, GERMANY SN 1433-7851 EI 1521-3773 J9 ANGEW CHEM INT EDIT JI Angew. Chem.-Int. Edit. PD NOV 17 PY 2014 VL 53 IS 47 BP 12865 EP 12869 DI 10.1002/anie.201407140 PG 5 WC Chemistry, Multidisciplinary SC Chemistry GA AT2UY UT WOS:000344793400034 PM 25257929 ER PT J AU Gleber, SC Wojcik, M Liu, J Roehrig, C Cummings, M Vila-Comamala, J Li, K Lai, B Shu, DM Vogt, S AF Gleber, Sophie-Charlotte Wojcik, Michael Liu, Jie Roehrig, Chris Cummings, Marvin Vila-Comamala, Joan Li, Kenan Lai, Barry Shu, Deming Vogt, Stefan TI Fresnel zone plate stacking in the intermediate field for high efficiency focusing in the hard X-ray regime SO OPTICS EXPRESS LA English DT Article ID MICROSCOPY; RESOLUTION; OPTICS AB Focusing efficiency of Fresnel zone plates (FZPs) for X-rays depends on zone height, while the achievable spatial resolution depends on the width of the finest zones. FZPs with optimal efficiency and sub-100-nm spatial resolution require high aspect ratio structures which are difficult to fabricate with current technology especially for the hard X-ray regime. A possible solution is to stack several zone plates. To increase the number of FZPs within one stack, we first demonstrate intermediate-field stacking and apply this method by stacks of up to five FZPs with adjusted diameters. Approaching the respective optimum zone height, we maximized efficiencies for high resolution focusing at three different energies, 10, 11.8, and 25 keV. (C)2014 Optical Society of America C1 [Gleber, Sophie-Charlotte; Wojcik, Michael; Liu, Jie; Roehrig, Chris; Cummings, Marvin; Vila-Comamala, Joan; Lai, Barry; Shu, Deming; Vogt, Stefan] Argonne Natl Lab, Argonne, IL 60439 USA. [Li, Kenan] Northwestern Univ, Evanston, IL 60208 USA. RP Gleber, SC (reprint author), Argonne Natl Lab, 9700 S Cass Ave, Argonne, IL 60439 USA. EM gleber@aps.anl.gov RI Vila-Comamala, Joan/E-2106-2017 FU U.S. Department of Energy (DOE) Office of Science; U.S. DOE [DE-AC02-06CH11357] FX We would like to acknowledge Liliana Stan, Leonidas E. Ocola and Ed Wrobel with their assistance during the research presented. Data was collected on beamlines 2-ID-D and 2-ID-E at the Advanced Photon Source, Argonne National Laboratory. Use of the Advanced Photon Source, an Office of Science User Facility operated for the U.S. Department of Energy (DOE) Office of Science by Argonne National Laboratory, and Center for Nanoscale Materials was supported by the U.S. DOE under Contract No. DE-AC02-06CH11357. NR 27 TC 8 Z9 8 U1 0 U2 9 PU OPTICAL SOC AMER PI WASHINGTON PA 2010 MASSACHUSETTS AVE NW, WASHINGTON, DC 20036 USA SN 1094-4087 J9 OPT EXPRESS JI Opt. Express PD NOV 17 PY 2014 VL 22 IS 23 BP 28142 EP 28153 DI 10.1364/OE.22.028142 PG 12 WC Optics SC Optics GA AT9TI UT WOS:000345268500035 PM 25402054 ER PT J AU Huang, ZX Droulias, S Koschny, T Soukoulis, CM AF Huang, Zhixiang Droulias, Sotiris Koschny, Thomas Soukoulis, Costas M. TI Mechanism of the metallic metamaterials coupled to the gain material SO OPTICS EXPRESS LA English DT Article ID INDEX AB We present evidence of strong coupling between the gain material and the metallic metamaterials. It is of vital importance to understand the mechanism of the coupling of metamaterials with the gain medium. Using a four-level gain system, the numerical pump-probe experiments are performed in several configurations (split-ring resonators (SRRs), inverse SRRs and fishnets) of metamaterials, demonstrating reduction of the resonator damping in all cases and hence the possibility for loss compensation. We find that the differential transmittance Delta T/T can be negative in different SRR configurations, such as SRRs on the top of the gain substrate, gain in the SRR gap and gain covering the SRR structure, while in the fishnet metamaterial with gain Delta T/T is positive. (C) 2014 Optical Society of America C1 [Huang, Zhixiang; Koschny, Thomas; Soukoulis, Costas M.] Iowa State Univ, Dept Phys & Astron, Ames, IA 50011 USA. [Huang, Zhixiang; Koschny, Thomas; Soukoulis, Costas M.] Iowa State Univ, Ames Lab, Ames, IA 50011 USA. [Huang, Zhixiang] Anhui Univ, Key Lab Intelligent Comp & Signal Proc, Hefei 230039, Peoples R China. [Droulias, Sotiris; Soukoulis, Costas M.] FORTH, Inst Elect Struct & Laser, Iraklion 71110, Greece. RP Droulias, S (reprint author), FORTH, Inst Elect Struct & Laser, Iraklion 71110, Greece. EM sdroulias@iesl.forth.gr RI Huang, Zhixiang/C-3416-2014; Soukoulis, Costas/A-5295-2008 OI Huang, Zhixiang/0000-0002-8023-9075; FU U.S. Dept. of Energy, Basic Energy Science, Materials Science and Engineering [DE-AC02-07CH11358]; European Research Council under the ERC Advanced Grant [320081] FX Work at Ames Lab was partially supported by the U.S. Dept. of Energy, Basic Energy Science, Materials Science and Engineering, Contract no. DE-AC02-07CH11358. Simulation work at FORTH (theory) was supported by the European Research Council under the ERC Advanced Grant no. 320081 (PHOTOMETA). NR 22 TC 3 Z9 3 U1 2 U2 42 PU OPTICAL SOC AMER PI WASHINGTON PA 2010 MASSACHUSETTS AVE NW, WASHINGTON, DC 20036 USA SN 1094-4087 J9 OPT EXPRESS JI Opt. Express PD NOV 17 PY 2014 VL 22 IS 23 BP 28596 EP 28605 DI 10.1364/OE.22.028596 PG 10 WC Optics SC Optics GA AT9TI UT WOS:000345268500082 PM 25402101 ER PT J AU Demos, SG Ehnnann, PR Qiu, SR Schaffers, KI Suratwala, TI AF Demos, Stavros G. Ehnnann, Paul R. Qiu, S. Roger Schaffers, Kathleen I. Suratwala, Tayyab I. TI Dynamics of defects in Ce3+ doped silica affecting its performance as protective filter in ultraviolet high-power lasers SO OPTICS EXPRESS LA English DT Article ID SPECTROSCOPIC PROPERTIES; PHOSPHATE-GLASSES; CERIUM; ABSORPTION; FLUORESCENCE; EFFICIENT; BORATE AB We investigate defects forming in Ce3+-doped fused silica samples following exposure to nanosecond ultraviolet laser pulses and their relaxation as a function of time and exposure to low intensity light at different wavelengths. A subset of these defects are responsible for inducing absorption in the visible and near infrared spectral range, which is of critical importance for the use of this material as ultraviolet light absorbing filter in high power laser systems. The dependence of the induced absorption as a function of laser fluence and methods to most efficiently mitigate this effect are presented. Experiments simulating the operation of the material as a UV protection filter for high power laser systems were performed in order to determine limitations and practical operational conditions. (C) 2014 Optical Society of America C1 [Demos, Stavros G.; Ehnnann, Paul R.; Qiu, S. Roger; Schaffers, Kathleen I.; Suratwala, Tayyab I.] Lawrence Livermore Natl Lab, Livermore, CA 94551 USA. RP Demos, SG (reprint author), Lawrence Livermore Natl Lab, 7000 East Ave, Livermore, CA 94551 USA. EM demos1@llnl.gov FU U.S. Department of Energy by Lawrence Livermore National Laboratory [DE-AC52-07NA27344, LLNL-JRNL-439171] FX This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344. LLNL-JRNL-439171. We thank Raluca A. Negres and Mary A. Norton for helping with execution of experiments. The authors also wish to acknowledge Asahi Glass Company (AGC) and Heraeus Quartz America for contributing the Ce:Silica glass samples that were studied in this work. NR 24 TC 3 Z9 3 U1 4 U2 19 PU OPTICAL SOC AMER PI WASHINGTON PA 2010 MASSACHUSETTS AVE NW, WASHINGTON, DC 20036 USA SN 1094-4087 J9 OPT EXPRESS JI Opt. Express PD NOV 17 PY 2014 VL 22 IS 23 BP 28798 EP 28809 DI 10.1364/OE.22.028798 PG 12 WC Optics SC Optics GA AT9TI UT WOS:000345268500100 PM 25402119 ER PT J AU Liao, ZM Raymond, B Gaylord, J Fallejo, R Bude, J Wegner, P AF Liao, Zhi M. Raymond, B. Gaylord, J. Fallejo, R. Bude, J. Wegner, P. TI Damage modeling and statistical analysis of optics damage performance in MJ-class laser systems SO OPTICS EXPRESS LA English DT Article ID FUSED-SILICA OPTICS; GROWTH; NIF; MITIGATION AB Modeling the lifetime of a fused silica optic is described for a multiple beam, MJ-class laser system. This entails combining optic processing data along with laser shot data to account for complete history of optic processing and shot exposure. Integrating with online inspection data allows for the construction of a performance metric to describe how an optic performs with respect to the model. This methodology helps to validate the damage model as well as allows strategic planning and identifying potential hidden parameters that are affecting the optic's performance. (C) 2014 Optical Society of America C1 [Liao, Zhi M.; Raymond, B.; Gaylord, J.; Fallejo, R.; Bude, J.; Wegner, P.] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA. RP Liao, ZM (reprint author), Lawrence Livermore Natl Lab, 7000 East Ave, Livermore, CA 94550 USA. EM zman@llnl.gov FU U.S. Department of Energy by Lawrence Livermore National Laboratory [DE-AC52-07NA27344]; LLNL office of LDRD [LLNL-JRNL-660594] FX The authors would like to acknowledge our wonderful colleagues at NIF for their contributions: Kris Fury for editing, T. Suratwala, M. Nostrand, P. Whitman for helpful discussions; W. Carr, D. Cross, M. Negres, M. Norton, and OSL team for all the offline damage data and rules that are the heart of the damage model, and finally M. Spaeth for setting us on this path so many years ago. This work is performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344 and funded through LLNL office of LDRD. (LLNL-JRNL-660594) NR 20 TC 6 Z9 7 U1 0 U2 16 PU OPTICAL SOC AMER PI WASHINGTON PA 2010 MASSACHUSETTS AVE NW, WASHINGTON, DC 20036 USA SN 1094-4087 J9 OPT EXPRESS JI Opt. Express PD NOV 17 PY 2014 VL 22 IS 23 BP 28845 EP 28856 DI 10.1364/OE.22.028845 PG 12 WC Optics SC Optics GA AT9TI UT WOS:000345268500105 PM 25402124 ER PT J AU Eftink, BP Mara, NA Kingstedt, OT Safarik, DJ Lambros, J Robertson, IM AF Eftink, B. P. Mara, N. A. Kingstedt, O. T. Safarik, D. J. Lambros, J. Robertson, I. M. TI Anomalous deformation twinning in coarse-grained Cu in Ag60Cu40 composites under high strain-rate compressive loading SO MATERIALS SCIENCE AND ENGINEERING A-STRUCTURAL MATERIALS PROPERTIES MICROSTRUCTURE AND PROCESSING LA English DT Article DE Twinning; Copper; Silver; Slip ID ROOM-TEMPERATURE; EUTECTIC ALLOY; FCC METALS; COPPER; AG; SLIP; INTERFACES; STRENGTH; BOUNDARIES; LAMELLAE AB The deformation response of a directionally solidified Ag60Cu40 eutectic alloy with a cube-on-cube orientation relationship between Ag and Cu subjected to high strain-rate 10(3) s(-1) compressive loading was examined. Loading at 45 degrees and 90 degrees to the growth axis, near [001] and [11 (1) over bar] local crystal orientations, respectively, resulted in deformation twinning and dislocation slip in both Ag and Cu under conditions where deformation twinning would not normally be expected in Cu. In contrast, loading at 0 degrees and 90 degrees to the growth axis, near < 101 > local crystal orientations, resulted in the primary deformation mode being dislocation slip. These results are interpreted in terms of the influence of loading axis with respect to the local crystal orientation in the directionally solidified alloy and on slip transmission from Ag into Cu. (C) 2014 Elsevier B.V. All rights reserved. C1 [Eftink, B. P.] Univ Illinois, Dept Mat Sci & Engn, Urbana, IL 61801 USA. [Mara, N. A.] Los Alamos Natl Lab, MPA CINT, Los Alamos, NM 87545 USA. [Kingstedt, O. T.; Lambros, J.] Univ Illinois, Dept Aerosp Engn, Urbana, IL 61801 USA. [Safarik, D. J.] Los Alamos Natl Lab, MST 6, Los Alamos, NM 87545 USA. [Robertson, I. M.] Univ Wisconsin, Dept Mat Sci & Engn, Madison, WI 53706 USA. RP Eftink, BP (reprint author), Univ Illinois, Dept Mat Sci & Engn, Urbana, IL 61801 USA. EM beftink2@illinois.edu RI Mara, Nathan/J-4509-2014; OI Safarik, Douglas/0000-0001-8648-9377 FU National Nuclear Security Administration of the Department of Energy [DE-FG52-09NA29463]; National Nuclear Security Administration of the U.S. Department of Energy [DE-AC52-06NA25396] FX This work was performed, in part, at the University of Illinois Urbana-Champaign by a grant from the National Nuclear Security Administration of the Department of Energy under contract DE-FG52-09NA29463. This work was also performed, in part, at the Center for Integrated Nanotechnologies, an Office of Science User Facility operated for the U.S. Department of Energy (DOE) Office of Science. Los Alamos National Laboratory, an affirmative action equal opportunity employer, is operated by Los Alamos National Security, LLC, for the National Nuclear Security Administration of the U.S. Department of Energy under contract DE-AC52-06NA25396. Compression testing assistance was provided by the Advanced Materials Testing and Evolution Laboratory (AMTEL) through Dr. Gavin Horn, Fire Service Institute, University of Illinois at Urbana-Champaign. Electron Microscopy was carried out in the Frederick Seitz Materials Research Laboratory Central Facilities at the University of Illinois in addition to the Electron Microscopy Laboratory at Los Alamos National Laboratory. NR 39 TC 4 Z9 4 U1 3 U2 18 PU ELSEVIER SCIENCE SA PI LAUSANNE PA PO BOX 564, 1001 LAUSANNE, SWITZERLAND SN 0921-5093 EI 1873-4936 J9 MAT SCI ENG A-STRUCT JI Mater. Sci. Eng. A-Struct. Mater. Prop. Microstruct. Process. PD NOV 17 PY 2014 VL 618 BP 254 EP 261 DI 10.1016/j.msea.2014.08.082 PG 8 WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Metallurgy & Metallurgical Engineering SC Science & Technology - Other Topics; Materials Science; Metallurgy & Metallurgical Engineering GA AS7MG UT WOS:000344439500031 ER PT J AU Stinson, JL Kathmann, SM Ford, IJ AF Stinson, Jake L. Kathmann, Shawn M. Ford, Ian J. TI Dynamical consequences of a constraint on the Langevin thermostat in molecular cluster simulation SO MOLECULAR PHYSICS LA English DT Article DE Langevin thermostat; small system; constraints AB We investigate some unusual behaviour observed while performing molecular dynamics simulations of small molecular clusters using a constrained Langevin thermostat. Atoms appear to be thermalised to different temperatures that depend on their mass and on the total number of particles in the system. The deviation from the zeroth law of thermodynamics can be considerable for small systems of heavy and light particles. We trace this behaviour to the absence of thermal noise acting on the centre of mass of the system. This is demonstrated by solving the stochastic dynamics for the constrained thermostat and comparing the results with simulation data. By removing the constraint, the Langevin thermostat may be restored to its intended behaviour. We also investigate a Langevin thermostat constrained to have zero total force acting on its centre of mass, and find similar deficiencies. C1 [Stinson, Jake L.; Ford, Ian J.] UCL, Dept Phys & Astron, London, England. [Stinson, Jake L.; Ford, Ian J.] UCL, London Ctr Nanotechnol, London, England. [Kathmann, Shawn M.] Pacific NW Natl Lab, Div Phys Sci, Richland, WA 99352 USA. RP Stinson, JL (reprint author), UCL, Dept Phys & Astron, London, England. EM j.stinson@ucl.ac.uk FU U.S. Department of Energy, Office of Basic Energy Sciences, Division of Chemical Sciences, Geosciences, and Biosciences; Pacific Northwest National Laboratory; IMPACT scheme at University College London FX We thank Ilian Todorov for assistance and comments. S. M. Kathmann was supported by the U.S. Department of Energy, Office of Basic Energy Sciences, Division of Chemical Sciences, Geosciences, and Biosciences. J.L. Stinson acknowledges Pacific Northwest National Laboratory and the IMPACT scheme at University College London for funding. We thank an anonymous referee for drawing our attention to the use of Gauss' principle of least constraint. NR 6 TC 0 Z9 0 U1 0 U2 4 PU TAYLOR & FRANCIS LTD PI ABINGDON PA 4 PARK SQUARE, MILTON PARK, ABINGDON OX14 4RN, OXON, ENGLAND SN 0026-8976 EI 1362-3028 J9 MOL PHYS JI Mol. Phys. PD NOV 17 PY 2014 VL 112 IS 22 BP 2920 EP 2923 DI 10.1080/00268976.2014.917732 PG 4 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AT9UU UT WOS:000345272700005 ER PT J AU Hagos, S Feng, Z Burleyson, CD Lim, KSS Long, CN Wu, D Thompson, G AF Hagos, Samson Feng, Zhe Burleyson, Casey D. Lim, Kyo-Sun Sunny Long, Charles N. Wu, Di Thompson, Greg TI Evaluation of convection-permitting model simulations of cloud populations associated with the Madden-Julian Oscillation using data collected during the AMIE/DYNAMO field campaign SO JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES LA English DT Article DE dynamo; cold pools; s-pol radar; cloud permitting; tropical convection; Madden-Julian oscillation ID MICROPHYSICS PARAMETERIZATION; PART I; RESOLVING MODEL; CLIMATE MODELS; RADAR; PRECIPITATION; ORGANIZATION; EXPLICIT; SCHEME; SNOW AB Regional convection-permitting model simulations of cloud populations observed during the 2011 Atmospheric Radiation Measurement (ARM) Madden-Julian Oscillation Investigation Experiment/Dynamics of the Madden-Julian Oscillation Experiment (AMIE/DYNAMO) field campaign are evaluated against ground-based radar and ship-based observations. Sensitivity of model simulated reflectivity, surface rain rate, and cold pool statistics to variations of raindrop breakup/self-collection parameters in four state-of-the-art two-moment bulk microphysics schemes in the Weather Research and Forecasting (WRF) model is examined. The model simulations generally overestimate reflectivity from large and deep convective cells, and underestimate stratiform rain and the frequency of cold pools. In the sensitivity experiments, introduction of more aggressive raindrop breakup or decreasing the self-collection efficiency increases the cold pool occurrence frequency in all of the simulations, and slightly reduces the reflectivity and precipitation statistics bias in some schemes but has little effect on the overall mean surface precipitation. Both the radar observations and model simulations of cloud populations show an approximate power law relationship between convective echo-top height and equivalent convective cell radius. C1 [Hagos, Samson; Feng, Zhe; Burleyson, Casey D.; Lim, Kyo-Sun Sunny; Long, Charles N.] Pacific NW Natl Lab, Richland, WA 99352 USA. [Wu, Di] NASA, Goddard Space Flight Ctr, Mesoscale Atmospher Processes Lab, Greenbelt, MD 20771 USA. [Wu, Di] Sci Syst & Applicat Inc, Lanham, MD USA. [Thompson, Greg] Natl Ctr Atmospher Res, Boulder, CO 80307 USA. RP Hagos, S (reprint author), Pacific NW Natl Lab, Richland, WA 99352 USA. EM samson.hagos@pnnl.gov RI Lim, Kyo-Sun/I-3811-2012; Burleyson, Casey/F-1833-2016; Feng, Zhe/E-1877-2015 OI Burleyson, Casey/0000-0001-6218-9361; Feng, Zhe/0000-0002-7540-9017 FU Office of Biological and Environmental Research of the U.S. Department of Energy (DOE) as part of the Regional and Global Climate Modeling Program; Office of Biological and Environmental Research of the U.S. Department of Energy (DOE) as part of the Atmospheric System Research Program; DOE by Battelle Memorial Institute [DE-AC06-76RLO 1830] FX The authors thank Yun Qian for his comments and suggestions. The data for this paper are available at NCAR's Earth Observing Laboratory's DYNAMO Data Catalogue https://www.eol.ucar.edu/field_projects/dynamo. The data set names are, R/V Roger Revelle Flux, Near-Surface Meteorology, and Navigation Data and S-PolKa Radar, fully corrected, merged, final moments data in cfRadial format. The S-Polka data were regridded by Stacy Brodzik (brodzik@atmos.washington.edu) at the University of Washington. This research is based on work supported by the Office of Biological and Environmental Research of the U.S. Department of Energy (DOE) as part of the Regional and Global Climate Modeling Program and Atmospheric System Research Program. Computing resources for the simulations are provided by the National Energy Research Scientific Computing Center (NERSC) and Oak Ridge Leadership Computing Facility (OLCF). The Pacific Northwest National Laboratory is operated for DOE by Battelle Memorial Institute under contract DE-AC06-76RLO 1830. NR 39 TC 11 Z9 11 U1 2 U2 6 PU AMER GEOPHYSICAL UNION PI WASHINGTON PA 2000 FLORIDA AVE NW, WASHINGTON, DC 20009 USA SN 2169-897X EI 2169-8996 J9 J GEOPHYS RES-ATMOS JI J. Geophys. Res.-Atmos. PD NOV 16 PY 2014 VL 119 IS 21 BP 12052 EP 12068 DI 10.1002/2014JD022143 PG 17 WC Meteorology & Atmospheric Sciences SC Meteorology & Atmospheric Sciences GA AU6EQ UT WOS:000345696600031 ER PT J AU Niemann, C Gekelman, W Constantin, CG Everson, ET Schaeffer, DB Bondarenko, AS Clark, SE Winske, D Vincena, S Van Compernolle, B Pribyl, P AF Niemann, C. Gekelman, W. Constantin, C. G. Everson, E. T. Schaeffer, D. B. Bondarenko, A. S. Clark, S. E. Winske, D. Vincena, S. Van Compernolle, B. Pribyl, P. TI Observation of collisionless shocks in a large current-free laboratory plasma SO GEOPHYSICAL RESEARCH LETTERS LA English DT Article ID EXPANSION; DESIGN AB We report the first measurements of the formation and structure of a magnetized collisionless shock by a laser-driven magnetic piston in a current-free laboratory plasma. This new class of experiments combines a high-energy laser system and a large magnetized plasma to transfer energy from a laser plasma plume to the ambient ions through collisionless coupling, until a self-sustained M-A similar to 2 magnetosonic shock separates from the piston. The ambient plasma is highly magnetized, current free, and large enough (17 m x 0.6 m) to support Alfven waves. Magnetic field measurements of the structure and evolution of the shock are consistent with two-dimensional hybrid simulations, which show Larmor coupling between the debris and ambient ions and the presence of reflected ions, which provide the dissipation. The measured shock formation time confirms predictions from computational work. C1 [Niemann, C.; Gekelman, W.; Constantin, C. G.; Everson, E. T.; Schaeffer, D. B.; Bondarenko, A. S.; Clark, S. E.; Vincena, S.; Van Compernolle, B.; Pribyl, P.] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA. [Winske, D.] Los Alamos Natl Lab, Los Alamos, NM USA. RP Niemann, C (reprint author), Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA. EM cniemann@ucla.edu OI Van Compernolle, Bart/0000-0002-5853-6233 FU Defense Threat Reduction Agency [HDTRA1-12-1-0024]; DOE Office of Science Early Career Research Program [E-FOA-0000395]; DOE/NSF FX This work was supported by the Defense Threat Reduction Agency under contract HDTRA1-12-1-0024 and the DOE Office of Science Early Career Research Program (E-FOA-0000395). The experiments were performed at the UCLA Basic Plasma Science Facility (BaPSF) supported by DOE/NSF. NR 23 TC 10 Z9 10 U1 1 U2 20 PU AMER GEOPHYSICAL UNION PI WASHINGTON PA 2000 FLORIDA AVE NW, WASHINGTON, DC 20009 USA SN 0094-8276 EI 1944-8007 J9 GEOPHYS RES LETT JI Geophys. Res. Lett. PD NOV 16 PY 2014 VL 41 IS 21 BP 7413 EP 7418 DI 10.1002/2014GL061820 PG 6 WC Geosciences, Multidisciplinary SC Geology GA AU3MT UT WOS:000345518300001 ER PT J AU Airapetian, A Akopov, N Akopov, Z Augustyniak, W Avetissian, A Blok, HP Borissov, A Bryzgalov, V Capiluppi, M Capitani, GP Cisbani, E Ciullo, G Contalbrigo, M Dalpiaz, PF Deconinck, W De Leo, R De Sanctis, E Diefenthaler, M Di Nezza, P Duren, M Ehrenfried, M Elbakian, G Ellinghaus, F Etzelmuller, E Fabbri, R Felawka, L Frullani, S Gabbert, D Gapienko, G Gapienko, V Garibaldi, F Gavrilov, G Gharibyan, V Hartig, M Hasch, D Holler, Y Hristova, I Ivanilov, A Jackson, HE Joosten, S Kaiser, R Karyan, G Keri, T Kinney, E Kisselev, A Korotkov, V Kozlov, V Kravchenko, P Krivokhijine, VG Lagamba, L Lapikas, L Lehmann, I Lenisa, P Lorenzon, W Ma, BQ Mahon, D Manaenkov, SI Mao, Y Marianski, B Marukyan, H Movsisyan, A Murray, M Naryshkin, Y Nass, A Nowak, WD Pappalardo, LL Perez-Benito, R Petrosyan, A Reimer, PE Reolon, AR Riedl, C Rith, K Rostomyan, A Ryckbosch, D Schafer, A Schnell, G Schuller, KP Seitz, B Shibata, TA Stahl, M Stancari, M Statera, M Steffens, E Steijger, JJM Taroian, S Terkulov, A Truty, R Trzcinski, A Tytgat, M Van Haarlem, Y VanHulse, C Vikhrov, V Vilardi, I Wang, S Yaschenko, S Yen, S Zeiler, D Zihlmann, B Zupranski, P AF Airapetian, A. Akopov, N. Akopov, Z. Augustyniak, W. Avetissian, A. Blok, H. P. Borissov, A. Bryzgalov, V. Capiluppi, M. Capitani, G. P. Cisbani, E. Ciullo, G. Contalbrigo, M. Dalpiaz, P. F. Deconinck, W. De Leo, R. De Sanctis, E. Diefenthaler, M. Di Nezza, P. Dueren, M. Ehrenfried, M. Elbakian, G. Ellinghaus, F. Etzelmueller, E. Fabbri, R. Felawka, L. Frullani, S. Gabbert, D. Gapienko, G. Gapienko, V. Garibaldi, F. Gavrilov, G. Gharibyan, V. Hartig, M. Hasch, D. Holler, Y. Hristova, I. Ivanilov, A. Jackson, H. E. Joosten, S. Kaiser, R. Karyan, G. Keri, T. Kinney, E. Kisselev, A. Korotkov, V. Kozlov, V. Kravchenko, P. Krivokhijine, V. G. Lagamba, L. Lapikas, L. Lehmann, I. Lenisa, P. Lorenzon, W. Ma, B. -Q. Mahon, D. Manaenkov, S. I. Mao, Y. Marianski, B. Marukyan, H. Movsisyan, A. Murray, M. Naryshkin, Y. Nass, A. Nowak, W. -D. Pappalardo, L. L. Perez-Benito, R. Petrosyan, A. Reimer, P. E. Reolon, A. R. Riedl, C. Rith, K. Rostomyan, A. Ryckbosch, D. Schaefer, A. Schnell, G. Schueller, K. P. Seitz, B. Shibata, T. -A. Stahl, M. Stancari, M. Statera, M. Steffens, E. Steijger, J. J. M. Taroian, S. Terkulov, A. Truty, R. Trzcinski, A. Tytgat, M. Van Haarlem, Y. VanHulse, C. Vikhrov, V. Vilardi, I. Wang, S. Yaschenko, S. Yen, S. Zeiler, D. Zihlmann, B. Zupranski, P. TI Spin density matrix elements in exclusive omega electroproduction on H-1 and H-2 targets at 27.5 GeV beam energy SO EUROPEAN PHYSICAL JOURNAL C LA English DT Article ID VECTOR-MESON LEPTOPRODUCTION; VIRTUAL COMPTON-SCATTERING; PARTON DISTRIBUTIONS; QCD AB Exclusive electroproduction of. mesons on unpolarized hydrogen and deuterium targets is studied in the kinematic region of Q(2) > 1.0 GeV2, 3.0 GeV < W < 6.3 GeV, and -t ' < 0.2 GeV2. Results on the angular distribution of the omega meson, including its decay products, are presented. The data were accumulated with the HER-MES forward spectrometer during the 1996-2007 running period using the 27.6 GeV longitudinally polarized electron or positron beam of HERA. The determination of the virtual-photon longitudinal-to-transverse cross-section ratio reveals that a considerable part of the cross section arises from transversely polarized photons. Spin density matrix elements are presented in projections of Q(2) or -t '. Violation of s-channel helicity conservation is observed for some of these elements. Asizable contribution from unnatural-parity-exchange amplitudes is found and the phase shift between those amplitudes that describe transverse omega production by longitudinal and transverse virtual photons,gamma(L)* -> omega(T) and gamma(T)* -> omega(T), is determined for the first time. A hierarchy of helicity amplitudes is established, which mainly means that the unnatural-parity-exchange amplitude describing the gamma(T)* -> omega(T) transition dominates over the two natural-parity-exchange amplitudes describing the gamma(L)* -> omega(L) and gamma(T)* -> omega(T) transitions, with the latter two being of similar magnitude. Good agreement is found between the HERMES proton data and results of a pQCD-inspired phenomenological model that includes pion-pole contributions, which are of unnatural parity. C1 [Jackson, H. E.; Reimer, P. E.] Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA. [De Leo, R.; Lagamba, L.; Vilardi, I.] Ist Nazl Fis Nucl, Sez Bari, I-70124 Bari, Italy. [Ma, B. -Q.; Mao, Y.; Wang, S.] Peking Univ, Sch Phys, Beijing 100871, Peoples R China. [Schnell, G.; VanHulse, C.] Univ,Basque Country UPV EHU, Dept Theoret Phys, Bilbao 48080, Spain. [Schnell, G.] Basque Fdn Sci, Ikerbasque, Bilbao 48013, Spain. [Ellinghaus, F.; Kinney, E.] Univ Colorado, Nucl Phys Lab, Boulder, CO 80309 USA. [Akopov, Z.; Borissov, A.; Deconinck, W.; Gavrilov, G.; Hartig, M.; Holler, Y.; Rostomyan, A.; Schueller, K. P.; Yaschenko, S.; Zihlmann, B.] DESY, D-22603 Hamburg, Germany. [Fabbri, R.; Gabbert, D.; Hristova, I.; Nowak, W. -D.; Riedl, C.] DESY, D-15738 Zeuthen, Germany. [Krivokhijine, V. G.] Joint Inst Nucl Res, Dubna 141980, Russia. [Diefenthaler, M.; Nass, A.; Rith, K.; Steffens, E.; Yaschenko, S.; Zeiler, D.] Univ Erlangen Nurnberg, Inst Phys, D-91058 Erlangen, Germany. [Capiluppi, M.; Ciullo, G.; Contalbrigo, M.; Dalpiaz, P. F.; Lenisa, P.; Movsisyan, A.; Pappalardo, L. L.; Stancari, M.; Statera, M.] Ist Nazl Fis Nucl, Sez Ferrara, I-44122 Ferrara, Italy. [Capiluppi, M.; Ciullo, G.; Dalpiaz, P. F.; Lenisa, P.; Pappalardo, L. L.; Stancari, M.; Statera, M.] Univ Ferrara, Dipartimento Fis & Sci Terra, I-44122 Ferrara, Italy. [Capitani, G. P.; De Sanctis, E.; Di Nezza, P.; Hasch, D.; Reolon, A. R.] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy. [Joosten, S.; Ryckbosch, D.; Schnell, G.; Tytgat, M.; Van Haarlem, Y.; VanHulse, C.] Univ Ghent, Dept Phys & Astron, B-9000 Ghent, Belgium. [Airapetian, A.; Dueren, M.; Ehrenfried, M.; Etzelmueller, E.; Keri, T.; Perez-Benito, R.; Stahl, M.] Univ Giessen, Inst Phys 2, D-35392 Giessen, Germany. [Kaiser, R.; Lehmann, I.; Mahon, D.; Murray, M.; Seitz, B.] Univ Glasgow, Sch Phys & Astron, SUPA, Glasgow G12 8QQ, Lanark, Scotland. [Diefenthaler, M.; Joosten, S.; Riedl, C.; Truty, R.] Univ Illinois, Dept Phys, Urbana, IL 61801 USA. [Airapetian, A.; Lorenzon, W.] Univ Michigan, Randall Lab Phys, Ann Arbor, MI 48109 USA. [Kozlov, V.; Terkulov, A.] PN Lebedev Phys Inst, Moscow 117924, Russia. [Blok, H. P.; Lapikas, L.; Steijger, J. J. M.] Natl Inst Subat Phys Nikhef, NL-1009 DB Amsterdam, Netherlands. [Gavrilov, G.; Kisselev, A.; Kravchenko, P.; Manaenkov, S. I.; Naryshkin, Y.; Vikhrov, V.] BP Konstantinov Petersburg Nucl Phys Inst, Gatchina 188300, Leningrad Regio, Russia. [Bryzgalov, V.; Gapienko, G.; Gapienko, V.; Ivanilov, A.; Korotkov, V.] Inst High Energy Phys, Protvino 142281, Moscow Region, Russia. [Schaefer, A.] Univ Regensburg, Inst Theoret Phys, D-93040 Regensburg, Germany. [Cisbani, E.; Frullani, S.; Garibaldi, F.] Ist Nazl Fis Nucl, Grp Collegato Sanita, I-00161 Rome, Italy. [Cisbani, E.; Frullani, S.; Garibaldi, F.] Ist Super Sanita, I-00161 Rome, Italy. [Felawka, L.; Gavrilov, G.; Yen, S.] TRIUMF, Vancouver, BC V6T 2A3, Canada. [Shibata, T. -A.] Tokyo Inst Technol, Dept Phys, Tokyo 152, Japan. [Blok, H. P.] Vrije Univ Amsterdam, Dept Phys & Astron, NL-1081 HV Amsterdam, Netherlands. [Augustyniak, W.; Marianski, B.; Trzcinski, A.; Zupranski, P.] Natl Ctr Nucl Res, PL-00689 Warsaw, Poland. [Akopov, N.; Avetissian, A.; Elbakian, G.; Gharibyan, V.; Karyan, G.; Marukyan, H.; Movsisyan, A.; Petrosyan, A.; Taroian, S.] Yerevan Phys Inst, Yerevan 375036, Armenia. RP Airapetian, A (reprint author), Univ Giessen, Inst Phys 2, D-35392 Giessen, Germany. EM gunar.schnell@desy.de RI Cisbani, Evaristo/C-9249-2011; Kozlov, Valentin/M-8000-2015; Terkulov, Adel/M-8581-2015 OI Cisbani, Evaristo/0000-0002-6774-8473; FU SCOAP3 / License Version CC BY 4.0 FX Funded by SCOAP3 / License Version CC BY 4.0. NR 28 TC 9 Z9 9 U1 3 U2 11 PU SPRINGER PI NEW YORK PA 233 SPRING ST, NEW YORK, NY 10013 USA SN 1434-6044 EI 1434-6052 J9 EUR PHYS J C JI Eur. Phys. J. C PD NOV 15 PY 2014 VL 74 IS 11 AR 3110 DI 10.1140/epjc/s10052-014-3110-1 PG 25 WC Physics, Particles & Fields SC Physics GA AX8OZ UT WOS:000347169800001 ER PT J AU Cernuschi, F Bison, P Sun, JG AF Cernuschi, F. Bison, P. Sun, J. G. TI Thermal diffusivity of TBC: Results of a small round robin test and considerations about the effect of the surface preparation and the measuring approach SO SURFACE & COATINGS TECHNOLOGY LA English DT Article DE Thermal barrier coatings; Thermal diffusivity; Blackening layer; Thermographic technique ID SPRAYED ZIRCONIA COATINGS; BARRIER COATINGS; MICROSTRUCTURAL CHARACTERIZATION; THERMOPHYSICAL PROPERTIES; HEAT-TREATMENT; LASER FLASH; CONDUCTIVITY AB Among the techniques used to measure the thermal diffusivity of TBC, the Laser Flash is a standard. Nonetheless, this technique shows two main limitations related to the size and the well-defined geometry of the specimens. Furthermore the most reliable data can be typically obtained only on freestanding coatings. On the contrary, other photothermal and thermographic techniques in reflection configuration (the same side is heated and temperature detected) can overcome these limitations. One aspect, only partially studied in the literature, is common to most of the photothermal and thermographic techniques. It concerns the effect of the blackening coating used for guaranteeing the absorption of the heating radiation just within a very shallow outer layer and to make opaque the TBC in the sensitivity range of the IR detector/camera. For this purpose, an inter-laboratory round robin has been promoted for comparing the thermal diffusivity in dependency of the blackening layer deposition technique, the TBC microstructure (in particular porous APS, columnar EB-PVD and PS-PVD (TM)) and the three different experimental set-ups in terms of spectral range and frame rate of the IR cameras, heating source and data reduction. (C) 2014 Elsevier B.V. All rights reserved. C1 [Cernuschi, F.] RSE, I-20134 Milan, Italy. [Bison, P.] CNR ITC, I-35127 Padua, Italy. [Sun, J. G.] Argonne Natl Lab, Argonne, IL 60439 USA. RP Cernuschi, F (reprint author), RSE, Via Rubattino 54, I-20134 Milan, Italy. EM federico.cernuschi@rse-web.it OI Bison, Paolo/0000-0002-8984-1994 FU RSE; Ministry of Economic Development - General Directorate for Nuclear Energy, Renewable Energy and Energy Efficiency; U.S. Department of Energy, Office of Fossil Energy, Advanced Research and Technology Development/Materials Program; EU [AST4-CT-2005-516149] FX The work at RSE has been partially financed by the Research Fund for the Italian Electrical System under the Contract Agreement between RSE (formerly known as ERSE) and the Ministry of Economic Development - General Directorate for Nuclear Energy, Renewable Energy and Energy Efficiency stipulated on July 29, 2009 in compliance with the Decree of March 19, 2009.; The work at Argonne was sponsored by the U.S. Department of Energy, Office of Fossil Energy, Advanced Research and Technology Development/Materials Program.; Some samples used within this work have been manufactured in the frame of the EU project TOPPCOAT Project No. AST4-CT-2005-516149. NR 42 TC 3 Z9 3 U1 2 U2 16 PU ELSEVIER SCIENCE SA PI LAUSANNE PA PO BOX 564, 1001 LAUSANNE, SWITZERLAND SN 0257-8972 J9 SURF COAT TECH JI Surf. Coat. Technol. PD NOV 15 PY 2014 VL 258 BP 284 EP 292 DI 10.1016/j.surfcoat.2014.09.011 PG 9 WC Materials Science, Coatings & Films; Physics, Applied SC Materials Science; Physics GA AX4HW UT WOS:000346895000035 ER PT J AU Nordhorn, C Mucke, R Unocic, KA Lance, MJ Pint, BA Vassen, R AF Nordhorn, Christian Muecke, Robert Unocic, Kinga A. Lance, Michael J. Pint, Bruce A. Vassen, Robert TI Effects of thermal cycling parameters on residual stresses in alumina scales of CoNiCrAlY and NiCoCrAlY bond coats SO SURFACE & COATINGS TECHNOLOGY LA English DT Article DE Photo-stimulated luminescence-spectroscopy; Thermally grown oxide; MCrAlY bond coats; Finite-element analysis; Mechanical stress ID BARRIER COATINGS; WATER-VAPOR; PHOTOLUMINESCENCE PIEZOSPECTROSCOPY; OXIDATION BEHAVIOR; GROWN OXIDE; SYSTEMS; TBCS; DURABILITY; MECHANISMS; LIFETIME AB Furnace cycling experiments were performed on free-standing high-velocity oxygen-fuel bond coat samples to investigate the effect of material composition, surface texture, and cycling conditions on the average stresses in the formed oxide scales after cooling. The oxide scale thicknesses were determined by SEM image analyses and information about the stresses were acquired by photo-stimulated luminescence-spectroscopy. Additionally, the scale thickness dependent stress fields were calculated in finite-element analyses including approximation functions for the surface roughness derived on the basis of profilometry data. The evolution of the average residual stress as a function of oxide scale thickness was subject to stochastic fluctuations predominantly caused by local scale spallations. In comparison to the supplemental modeling results, thermal stresses due to mismatch of thermal expansion coefficients are identified as the main contribution to the residual stresses. The theoretical results emphasize that analyses of spectroscopic data acquired for average stress investigations of alumina scales rely on detailed information about microstructural features. (C) 2014 Elsevier B.V. All rights reserved. C1 [Nordhorn, Christian; Muecke, Robert; Vassen, Robert] Forschungszentrum Julich, IEK 1, D-52428 Julich, Germany. [Unocic, Kinga A.; Lance, Michael J.; Pint, Bruce A.] Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37831 USA. RP Nordhorn, C (reprint author), Forschungszentrum Julich, IEK 1, Wilhelm Johnen Str, D-52428 Julich, Germany. EM c.nordhorn@fz-juelich.de RI Pint, Bruce/A-8435-2008; Lance, Michael/I-8417-2016 OI Pint, Bruce/0000-0002-9165-3335; Lance, Michael/0000-0001-5167-5452 FU U.S. Department of Energy, Office of Coal and Power R&D, Office of Fossil Energy FX The authors gratefully acknowledge the support of D. Sebold for SEM work at Julich, G.W. Garner at ORNL for assistance with the thermal cycling experiments, and T.M. Lowe and T. Jordan for assistance with the experimental work at ORNL. The experimental work at ORNL was supported by the U.S. Department of Energy, Office of Coal and Power R&D, Office of Fossil Energy. NR 29 TC 2 Z9 2 U1 4 U2 30 PU ELSEVIER SCIENCE SA PI LAUSANNE PA PO BOX 564, 1001 LAUSANNE, SWITZERLAND SN 0257-8972 J9 SURF COAT TECH JI Surf. Coat. Technol. PD NOV 15 PY 2014 VL 258 BP 608 EP 614 DI 10.1016/j.surfcoat.2014.08.028 PG 7 WC Materials Science, Coatings & Films; Physics, Applied SC Materials Science; Physics GA AX4HW UT WOS:000346895000074 ER PT J AU Tripathy, PK Wurth, LA Dufek, EJ Gutknecht, TY Gese, NJ Hahn, PA Frank, SM Fredrickson, GL Herring, JS AF Tripathy, Prabhat K. Wurth, Laura A. Dufek, Eric J. Gutknecht, Toni Y. Gese, Natalie J. Hahn, Paula A. Frank, Steven M. Fredrickson, Guy L. Herring, J. Stephen TI Aluminum electroplating on steel from a fused bromide electrolyte SO SURFACE & COATINGS TECHNOLOGY LA English DT Article DE Bromide plating bath; Functional electrolyte; Aluminum electro-coating; Current density; Coating morphology ID MOLTEN-SALT; CORROSION-RESISTANCE; STAINLESS-STEEL; ELECTRODEPOSITION; ALCL3-NACL-KCL; DEPOSITION; SUBSTRATE; CHLORIDE; SURFACE; FILMS AB A quaternary bromide bath (LiBr-KBr-CsBr-AlBr3) was used to electro-coat aluminum on steel substrates. The electrolyte was prepared by the addition of AlBr3 into the eutectic LiBr-KBr-CsBr melt. A smooth, thick, adherent and shiny aluminum coating could be obtained with 80 wt.% AlBr3 in the ternary melt. The SEM photographs of the coated surfaces suggest the formation of thick and dense coatings with good aluminum coverage. Both salt immersion and open circuit potential measurement suggested that the coatings did display a good corrosion-resistance behavior. Annealing of the coated surfaces, prior to corrosion tests, suggested the robustness of the metallic aluminum coating in preventing the corrosion of the steel surfaces. Studies also indicated that the quaternary bromide plating bath can potentially provide a better aluminum coating on both ferrous and non-ferrous metals, including complex surfaces/geometries. Published by Elsevier B.V. C1 [Tripathy, Prabhat K.; Gese, Natalie J.; Frank, Steven M.; Fredrickson, Guy L.] Idaho Natl Lab, Separat Dept, Nucl Sci & Technol Directorate, Idaho Falls, ID 83415 USA. [Wurth, Laura A.] ZAF Energy Syst Inc, Columbia Falls, MT 59912 USA. [Dufek, Eric J.] Idaho Natl Lab, Biol & Chem Proc Dept, Energy & Environm Sci & Technol Directorate, Idaho Falls, ID 83415 USA. [Gutknecht, Toni Y.] Chalmers, S-41296 Gothenburg, Sweden. [Hahn, Paula A.] Idaho Natl Lab, Chem & Radiat Measurement Dept, Energy & Environm Sci & Technol Directorate, Idaho Falls, ID 83415 USA. [Herring, J. Stephen] Idaho Natl Lab, Nucl Sci & Technol Directorate, Nucl & Sci Engn Dept, Idaho Falls, ID 83415 USA. RP Tripathy, PK (reprint author), Idaho Natl Lab, Separat Dept, Nucl Sci & Technol Directorate, POB 1625, Idaho Falls, ID 83415 USA. EM Prabhat.Tripathy@inl.gov RI Dufek, Eric/B-8847-2017; Frank, Steven/B-9046-2017 OI Dufek, Eric/0000-0003-4802-1997; Frank, Steven/0000-0001-8259-6722 FU Idaho National Laboratory Directed Research and Development Program under DOE Idaho Operations Office; US Department of Energy [DE-AC07-05ID14517] FX The authors gratefully acknowledge the Idaho National Laboratory Directed Research and Development Program under DOE Idaho Operations Office for supporting the present research and development program. The manuscript was authorized by Battelle Energy Alliances under the contract No. DE-AC07-05ID14517, with the US Department of Energy, for publication. The US government retains and the publisher, by accepting the manuscript for publication, acknowledges that the US government retains a non-exclusive, paid up irrevocable worldwide license to publish or reproduce the published form of this manuscript or allow others to do so for United States Government purposes. NR 36 TC 0 Z9 0 U1 4 U2 22 PU ELSEVIER SCIENCE SA PI LAUSANNE PA PO BOX 564, 1001 LAUSANNE, SWITZERLAND SN 0257-8972 J9 SURF COAT TECH JI Surf. Coat. Technol. PD NOV 15 PY 2014 VL 258 BP 652 EP 663 DI 10.1016/j.surfcoat.2014.08.021 PG 12 WC Materials Science, Coatings & Films; Physics, Applied SC Materials Science; Physics GA AX4HW UT WOS:000346895000080 ER PT J AU Garcin, E Seeger, F Quintyn, R Tanimoto, A Williams, G Tainer, J Wysocki, V AF Garcin, Elsa Seeger, Franziska Quintyn, Royston Tanimoto, Akiko Williams, Gareth Tainer, John Wysocki, Vicki TI Interfacial residues promote an optimal alignment of the catalytic center in soluble guanylate cyclase SO NITRIC OXIDE-BIOLOGY AND CHEMISTRY LA English DT Meeting Abstract DE Soluble guanylate cyclase; Enzyme mechanism; Regulation; X-ray crystallography; Conformational changes; Domain-domain interactions C1 [Garcin, Elsa; Seeger, Franziska] Univ Maryland Baltimore Cty, Baltimore, MD 21228 USA. [Quintyn, Royston; Tanimoto, Akiko; Wysocki, Vicki] Ohio State Univ, Columbus, OH 43210 USA. [Williams, Gareth] Lawrence Berkeley Natl Lab, Berkeley, CA USA. NR 0 TC 0 Z9 0 U1 0 U2 2 PU ACADEMIC PRESS INC ELSEVIER SCIENCE PI SAN DIEGO PA 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA SN 1089-8603 EI 1089-8611 J9 NITRIC OXIDE-BIOL CH JI Nitric Oxide-Biol. Chem. PD NOV 15 PY 2014 VL 42 MA 2012-1 BP 112 EP 112 DI 10.1016/j.niox.2014.09.042 PG 1 WC Biochemistry & Molecular Biology; Cell Biology SC Biochemistry & Molecular Biology; Cell Biology GA AU7XZ UT WOS:000345812900049 ER PT J AU Garcin, E Seeger, F Quintyn, R Tanimoto, A Williams, G Tainer, J Wysocki, V AF Garcin, Elsa Seeger, Franziska Quintyn, Royston Tanimoto, Akiko Williams, Gareth Tainer, John Wysocki, Vicki TI Interfacial residues promote an optimal alignment of the catalytic center in soluble guanylate cyclase SO NITRIC OXIDE-BIOLOGY AND CHEMISTRY LA English DT Meeting Abstract DE Soluble guanylate cyclase; Enzyme mechanism; Regulation; X-ray crystallography; Conformational changes; Domain-domain interactions C1 [Garcin, Elsa; Seeger, Franziska] Univ Maryland Baltimore Cty, Baltimore, MD 21228 USA. [Quintyn, Royston; Tanimoto, Akiko; Wysocki, Vicki] Ohio State Univ, Columbus, OH 43210 USA. [Williams, Gareth] Lawrence Berkeley Natl Lab, Berkeley, CA USA. NR 0 TC 0 Z9 0 U1 0 U2 1 PU ACADEMIC PRESS INC ELSEVIER SCIENCE PI SAN DIEGO PA 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA SN 1089-8603 EI 1089-8611 J9 NITRIC OXIDE-BIOL CH JI Nitric Oxide-Biol. Chem. PD NOV 15 PY 2014 VL 42 MA P216 BP 152 EP 153 DI 10.1016/j.niox.2014.09.156 PG 2 WC Biochemistry & Molecular Biology; Cell Biology SC Biochemistry & Molecular Biology; Cell Biology GA AU7XZ UT WOS:000345812900163 ER PT J AU Krot, AN Nagashima, K Wasserburg, GJ Huss, GR Papanastassiou, D Davis, AM Hutcheon, ID Bizzarro, M AF Krot, Alexander N. Nagashima, Kazuhide Wasserburg, Gerald J. Huss, Gary R. Papanastassiou, Dimitri Davis, Andrew M. Hutcheon, Ian D. Bizzarro, Martin TI Calcium-aluminum-rich inclusions with fractionation and unknown nuclear effects (FUN CAIs): I. Mineralogy, petrology, and oxygen isotopic compositions SO GEOCHIMICA ET COSMOCHIMICA ACTA LA English DT Article ID UNUSUAL ALLENDE INCLUSION; EARLY SOLAR-SYSTEM; REFRACTORY INCLUSIONS; CARBONACEOUS CHONDRITES; PROTOPLANETARY DISK; MELILITE CRYSTALS; TRACE-ELEMENT; CV3 CHONDRITE; HETEROGENEOUS DISTRIBUTION; CAAL2SI2O8 POLYMORPHS AB We present a detailed characterization of the mineralogy, petrology, and oxygen isotopic compositions of twelve FUN CAIs, including C1 and EK1-4-1 from Allende (CV), that were previously shown to have large isotopic fractionation patterns for magnesium and oxygen, and large isotopic anomalies of several elements. The other samples show more modest patterns of isotopic fractionation and have smaller but significant isotopic anomalies. All FUN CAIs studied are coarse-grained igneous inclusions: Type B, forsterite-bearing Type B, compact Type A, and hibonite-rich. Some inclusions consist of two mineralogically distinct lithologies, forsterite-rich and forsterite-free/poor. All the CV FUN CAIs experienced postcrystallization open-system iron-alkali-halogen metasomatic alteration resulting in the formation of secondary minerals commonly observed in non-FUN CAIs from CV chondrites. The CR FUN CAI GG#3 shows no evidence for alteration. In all samples, clear evidence of oxygen isotopic fractionation was found. Most samples were initially O-16-rich. On a three-oxygen isotope diagram, various minerals in each FUN CAI (spinel, forsterite, hibonite, dmisteinbergite, most fassaite grains, and melilite (only in GG#3)), define mass-dependent fractionation lines with a similar slope of similar to 0.5. The different inclusions have different Delta O-17 values ranging from similar to-25 parts per thousand to similar to-16 parts per thousand. Melilite and plagioclase in the CV FUN CAIs have O-16-poor compositions (Delta O-17 similar to-3 parts per thousand) and plot near the intercept of the Allende CAI line and the terrestrial fractionation line. We infer that mass-dependent fractionation effects of oxygen isotopes in FUN CAI minerals are due to evaporation during melt crystallization. Differences in Delta O-17 values of mass-dependent fractionation lines defined by minerals in individual FUN CAIs are inferred to reflect differences in Delta O-17 values of their precursors. Differences in delta O-18 values of minerals defining the mass-dependent fractionation lines in several FUN CAIs are consistent with their inferred crystallization sequence, suggesting these minerals crystallized during melt evaporation. In other FUN CAIs, no clear correlation between delta O-18 values of individual minerals and their inferred crystallization sequence is observed, possibly indicating gas-melt back reaction and oxygen-isotope exchange in a O-16-rich gaseous reservoir. After oxygen-isotope fractionation, some FUN CAIs could have experienced partial melting and gas-melt oxygen-isotope exchange in a O-16-poor gaseous reservoir that resulted in crystallization of O-16-depleted fassaite, melilite and plagioclase. The final oxygen isotopic compositions of melilite and plagioclase in the CV FUN CAIs may have been established on the CV parent asteroid as a result of isotope exchange with a O-16-poor fluid during hydrothermal alteration. We conclude that FUN CAIs are part of a general family of refractory inclusions showing various degrees of fractionation effects due to evaporative processes superimposed on sampling of isotopically heterogeneous material. These processes have been experienced both by FUN and non-FUN igneous CAIs. Generally, the inclusions identified as FUN show larger isotope fractionation effects than non-FUN CAIs. There is a wide spread in UN isotopic anomalies in a large number of CAIs not exhibiting large fractionation effects in oxygen, magnesium, and silicon. The question of why some FUN CAIs show more extreme UN isotopic effects is attributed by us to limited sampling and not a special source of isotopically anomalous material. We consider the majority of igneous CAIs to be the result of several stages of thermal processing (evaporation, condensation, and melting) of aggregates of solid precursors composed of incompletely isotopically homogenized materials. The unknown nuclear effects in CAIs are common to both FUN and non-FUN CAIs, and are not a special characteristic of FUN inclusions but represent the spectrum of results from sampling a very heterogeneous medium in the accreting Solar System. (C) 2014 Elsevier Ltd. All rights reserved. C1 [Krot, Alexander N.; Nagashima, Kazuhide; Wasserburg, Gerald J.; Huss, Gary R.] Univ Hawaii Manoa, Sch Ocean & Earth Sci & Technol, Hawaii Inst Geophys & Planetol, Honolulu, HI 96822 USA. [Wasserburg, Gerald J.; Papanastassiou, Dimitri] CALTECH, Lunat Asylum, Pasadena, CA 91125 USA. [Papanastassiou, Dimitri] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA. [Davis, Andrew M.] Lawrence Livermore Natl Lab, Glenn Seaborg Inst, Livermore, CA 94551 USA. [Hutcheon, Ian D.] Univ Chicago, Enrico Fermi Inst, Dept Geophys Sci, Chicago, IL 60637 USA. [Hutcheon, Ian D.] Univ Chicago, Chicago Ctr Cosmochem, Chicago, IL 60637 USA. [Bizzarro, Martin] Univ Copenhagen, Ctr Star & Planet Format, Geol Museum, DK-1350 Copenhagen, Denmark. RP Krot, AN (reprint author), Univ Hawaii Manoa, Sch Ocean & Earth Sci & Technol, Hawaii Inst Geophys & Planetol, Honolulu, HI 96822 USA. EM sasha@higp.hawaii.edu RI Bizzarro, Martin/I-8701-2012 OI Bizzarro, Martin/0000-0001-9966-2124 FU NASA [NNX10AH76G, NNX12AJ01G, NNX08AG58G, NNH10AO48I]; Danish National Research Foundation [DNRF97] FX We thank Dr. Hisayoshi Yurimoto, the anonymous reviewer, and Dr. Sara S. Russell for useful comments and suggestions. Editorial handling of the manuscript by S. S. Russell is highly appreciated.. This work was supported by NASA grants NNX10AH76G and NNX12AJ01G (A. N. Krot, P. I.), NNX08AG58G (G. R. Huss, P. I.), and NNH10AO48I (I. D. Hutcheon, P. I.). The Centre for Star and Planet Formation is financed by the Danish National Research Foundation (Grant DNRF97). This is Hawai'i Institute of Geophysics and Planetology publication XXXX and School of Ocean and Earth Science and Technology publication XXXX. NR 110 TC 12 Z9 12 U1 4 U2 22 PU PERGAMON-ELSEVIER SCIENCE LTD PI OXFORD PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, ENGLAND SN 0016-7037 EI 1872-9533 J9 GEOCHIM COSMOCHIM AC JI Geochim. Cosmochim. Acta PD NOV 15 PY 2014 VL 145 BP 206 EP 247 DI 10.1016/j.gca.2014.09.027 PG 42 WC Geochemistry & Geophysics SC Geochemistry & Geophysics GA AT4XO UT WOS:000344945800012 ER PT J AU Yan, HP Park, C Ahn, G Hong, S Keane, DT Kenney-Benson, C Chow, P Xiao, YM Shen, GY AF Yan, Hongping Park, Changyong Ahn, Gun Hong, Seungbum Keane, Denis T. Kenney-Benson, Curtis Chow, Paul Xiao, Yuming Shen, Guoyin TI Termination and hydration of forsteritic olivine (010) surface SO GEOCHIMICA ET COSMOCHIMICA ACTA LA English DT Article ID X-RAY REFLECTIVITY; CRYSTAL TRUNCATION RODS; ATOMIC-FORCE MICROSCOPY; DISSOLUTION KINETICS; COMPUTER-SIMULATION; OCEANIC PERIDOTITES; HYDROGEN GENERATION; WATER; TEMPERATURE; SERPENTINIZATION AB Termination and hydration of the forsteritic (Fo90Fa10) olivine (010) surface have been investigated with high-resolution specular X-ray reflectivity and Atomic Force Microscopy. The surface was prepared by polishing a naturally grown {010} face, from which we found the polished surface in acidic (pH 3.5) alumina suspension exhibits regular steps while the basic (pH 9.5) silica polished surface is irregularly roughened, indicating there are two distinguishable mechanochemical processes for the surface dissolution. The quantitative interpretation of the regular steps from the alumina-polished surface suggests that the observed step heights correspond to multiples of crystallographic unit cell. Only this atomically terraced surface is investigated with the high-resolution X-ray reflectivity (HRXR) to determine the surface termination and hydration. The basic silica paste polished surface turned out too rough to measure with X-ray reflectivity. HRXR reveals that the alumina polished olivine (0 1 0) surface in pure water is terminated at a plane including half-occupied metal ion sites (M1), an oxygen vacancy site, and a silicate tetrahedral unit with one of its apices pointing outward with respect to the surface. An ideal termination with the oxygen vacancy would fulfill the stoichiometry of the formula unit; however, in the observation, the vacancy site is filled by an adsorbed water species and about a quarter of the remaining metal ions are further depleted. The terminating plane generates two distinct atomic layers in the laterally averaged electron density profile, on which two highly ordered adsorbed water layers are formed. The first layer formation is likely through the direct interaction with the M1 plane and the second layer is likely through the hydrogen bonding interaction with the first water layer. With this multilayered adsorbed water structure, the surface metal ion is partially hydrated by the vacancy-filling water species and adsorbed water molecules. The bulk water links to these distinct adsorbed water layers, with weak density oscillations that almost completely damp out after the first bulk water layer. The total thickness of the layered water structure including the two distinct adsorbed layers and the first layer of bulk water is slightly less than 1 nm, which corresponds to roughly three molecular layers of water. These results describe the steric constraints of the surface metal ion hydration and the iron redox environment during water-olivine interactions in this particular crystallographic orientation. (C) 2014 Elsevier Ltd. All rights reserved. C1 [Yan, Hongping; Park, Changyong; Kenney-Benson, Curtis; Chow, Paul; Xiao, Yuming; Shen, Guoyin] Carnegie Inst Sci, HPCAT, Geophys Lab, Argonne, IL 60439 USA. [Ahn, Gun; Hong, Seungbum] Argonne Natl Lab, Div Mat Sci, Argonne, IL 60439 USA. [Keane, Denis T.] Northwestern Univ, Dept Mat Sci & Engn, Evanston, IL 60208 USA. RP Yan, HP (reprint author), Carnegie Inst Sci, HPCAT, Geophys Lab, 9700 South Cass Ave,434E, Argonne, IL 60439 USA. EM hyan@carnegiescience.edu; cpark@carnegiescience.edu RI Hong, Seungbum/B-7708-2009; Park, Changyong/A-8544-2008; OI Hong, Seungbum/0000-0002-2667-1983; Park, Changyong/0000-0002-3363-5788; Yan, Hongping/0000-0001-6235-4523 FU Alfred P. Sloan Foundation in the United States; High-Pressure Collaborative Access Team (HPCAT); DOE-NNSA [DE-NA0001974]; DOE-BES [DE-FG02-99ER45775, DE-AC02-06CH11357]; NSF; E.I. DuPont de Nemours Co.; Dow Chemical Company; Northwestern University; Carnegie/DOE Alliance Center (CDAC); U.S. Department of Energy, Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division [DE-AC02-06CH11357] FX This work is a part of the Deep Carbon Observatory-Deep Energy project, supported by the Alfred P. Sloan Foundation in the United States. H. Yan is partially supported by the High-Pressure Collaborative Access Team (HPCAT). HPCAT is supported by DOE-NNSA under Award No. DE-NA0001974 and DOE-BES under Award no. DE-FG02-99ER45775, with partial instrumental funding by NSF. Portions of this work were performed at the DuPont-Northwestern-Dow Collaborative Access Team (DND-CAT) located at Sector 5 of the Advanced Photon Source (APS). DND-CAT is supported by E.I. DuPont de Nemours & Co., The Dow Chemical Company and Northwestern University. Some preliminary tests were performed at the HPCAT 16ID-D beamline through the auspices of Carnegie/DOE Alliance Center (CDAC) for the beamtime. APS is supported by DOE-BES, under Contract No. DE-AC02-06CH11357. AFM experiments conducted at Materials Science Division, Argonne National Laboratory by G. Ahn and S. Hong were supported by the U.S. Department of Energy, Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division under Contract No. DE-AC02-06CH11357. NR 51 TC 2 Z9 2 U1 2 U2 19 PU PERGAMON-ELSEVIER SCIENCE LTD PI OXFORD PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, ENGLAND SN 0016-7037 EI 1872-9533 J9 GEOCHIM COSMOCHIM AC JI Geochim. Cosmochim. Acta PD NOV 15 PY 2014 VL 145 BP 268 EP 280 DI 10.1016/j.gca.2014.09.005 PG 13 WC Geochemistry & Geophysics SC Geochemistry & Geophysics GA AT4XO UT WOS:000344945800014 ER PT J AU Anderson, B Venus, G Ott, D Divliansky, I Dawson, JW Drachenberg, DR Messerly, MJ Pax, PH Tassano, JB Glebov, LB AF Anderson, B. Venus, G. Ott, D. Divliansky, I. Dawson, J. W. Drachenberg, D. R. Messerly, M. J. Pax, P. H. Tassano, J. B. Glebov, L. B. TI Fundamental mode operation of a ribbon fiber laser by way of volume Bragg gratings SO OPTICS LETTERS LA English DT Article ID OPTICAL PARAMETRIC OSCILLATOR; HIGH-ORDER MODE; NARROW-BAND; POWER AB Selection of the fundamental mode of an active large mode area "ribbon" fiber laser with core dimensions of 107.8 mu m by 8.3 mu m was produced by a transmitting Bragg grating (TBG) in a free-space resonator. The multimode performance of the original laser was characterized to have an M-2 of 11.3 with an absorbed power slope efficiency of 76%. With the TBG aligned to provide maximum diffraction efficiency for the fundamental mode, the M-2 improved to 1.45 at an absorbed power slope efficiency of 54% and enhanced the brightness by 5.1 times. (C) 2014 Optical Society of America. C1 [Anderson, B.; Venus, G.; Ott, D.; Divliansky, I.; Glebov, L. B.] Univ Cent Florida, Coll Opt & Photon, CREOL, Orlando, FL 32816 USA. [Dawson, J. W.; Drachenberg, D. R.; Messerly, M. J.; Pax, P. H.; Tassano, J. B.] Lawrence Livermore Natl Lab, Livermore, CA 94551 USA. RP Anderson, B (reprint author), Univ Cent Florida, Coll Opt & Photon, CREOL, POB 162700, Orlando, FL 32816 USA. EM bmanders@knights.ucf.edu RI Divliansky, Ivan/D-4869-2011; OI Ott, Daniel/0000-0001-5221-8819 FU ARO; HEL-JTO [W911NF-10-1-0441]; Directed Energy Professional Society (DEPS) FX This work was supported by the ARO and HEL-JTO contract W911NF-10-1-0441. The author B. Anderson would like to acknowledge the support of the Directed Energy Professional Society (DEPS) graduate student scholarship. NR 16 TC 6 Z9 6 U1 0 U2 8 PU OPTICAL SOC AMER PI WASHINGTON PA 2010 MASSACHUSETTS AVE NW, WASHINGTON, DC 20036 USA SN 0146-9592 EI 1539-4794 J9 OPT LETT JI Opt. Lett. PD NOV 15 PY 2014 VL 39 IS 22 BP 6498 EP 6500 DI 10.1364/OL.39.006498 PG 3 WC Optics SC Optics GA AT5MB UT WOS:000344986000036 PM 25490503 ER PT J AU Otterstrom, N Pooser, RC Lawrie, BJ AF Otterstrom, N. Pooser, R. C. Lawrie, B. J. TI Nonlinear optical magnetometry with accessible in situ optical squeezing SO OPTICS LETTERS LA English DT Article ID RUBIDIUM VAPOR; ATOMIC MAGNETOMETER; QUANTUM-NOISE; COHERENCE; LIGHT AB We demonstrate compact and accessible squeezed-light magnetometry using four-wave mixing in a single hot rubidium vapor cell. The strong intrinsic coherence of the four-wave mixing process results in nonlinear magneto-optical rotation (NMOR) on each mode of a two-mode relative-intensity squeezed state. This framework enables 4.7 dB of quantum noise reduction while the opposing polarization rotation signals of the probe and conjugate fields add to increase the total signal to noise ratio. (C) 2014 Optical Society of America C1 [Otterstrom, N.] Brigham Young Univ, Dept Phys & Astron, Provo, UT 84602 USA. [Otterstrom, N.; Pooser, R. C.; Lawrie, B. J.] Oak Ridge Natl Lab, Computat Sci & Engn Div, Quantum Informat Sci Grp, Oak Ridge, TN 37830 USA. RP Lawrie, BJ (reprint author), Oak Ridge Natl Lab, Computat Sci & Engn Div, Quantum Informat Sci Grp, Oak Ridge, TN 37830 USA. EM lawriebj@ornl.gov RI Lawrie, Benjamin/B-7182-2016 OI Pooser, Raphael/0000-0002-2922-453X; Lawrie, Benjamin/0000-0003-1431-066X NR 30 TC 8 Z9 8 U1 5 U2 18 PU OPTICAL SOC AMER PI WASHINGTON PA 2010 MASSACHUSETTS AVE NW, WASHINGTON, DC 20036 USA SN 0146-9592 EI 1539-4794 J9 OPT LETT JI Opt. Lett. PD NOV 15 PY 2014 VL 39 IS 22 BP 6533 EP 6536 DI 10.1364/OL.39.006533 PG 4 WC Optics SC Optics GA AT5MB UT WOS:000344986000045 PM 25490512 ER PT J AU Cai, ZB Meyer, HM Ma, C Chi, MF Luo, HM Qu, J AF Cai, Zhen-Bing Meyer, Harry M., III Ma, Cheng Chi, Miaofang Luo, Huimin Qu, Jun TI Comparison of the tribological behavior of steel-steel and Si3N4-steel contacts in lubricants with ZDDP or ionic liquid SO WEAR LA English DT Article DE ZDDP; Oil-soluble ionic liquid; Anti-wear additive; Wear mechanism; Tribofilm ID OIL; ADDITIVES; FRICTION; FILMS AB Tribological evaluations were conducted on lubricating base oils of different viscosity grades with and without an anti-wear (AW) additive in lubricating steel-steel and ceramic-steel contacts. Two AW additives were applied: a conventional secondary zinc dialkyldithiophosphate (ZDDP) and an oilmiscible phosphonium-phosphate ionic liquid (IL). Tests were carried out using reciprocating ball-on-flat sliding at room temperature. The flat material was AISI A2 tool steel, and the ball material was either AISI 52100 bearing steel or silicon nitride. Four lubricants were tested: Chevron SAE 15W40 and 0W30 base oils, and the 0W30 base oil plus 1 wt% ZDDP or IL For the steel-steel contact, the lower-viscosity 0W30 base oil resulted in a higher wear rate than did the 15W40 base oil, as expected. Both the ZDDP and the IL substantially reduced wear, and the IL-additized 0W30 base oil was the best performer. For the ceramic-steel contact, the ZDDP provided moderate wear protection for both ball and flat. In contrast, the IL reduced the steel flat wear more effectively but increased the ceramic ball wear rate. Crosssectional transmission electron microscopy (TEM) examination and x-ray photoelectron spectroscopy (XPS) chemical analysis were used to reveal the thickness, nanostructure, and composition of the tribofilms formed by ZDDP and IL on the steel and silicon nitride surfaces. (C) 2014 Elsevier B.V. All rights reserved. C1 [Cai, Zhen-Bing] Southwest Jiaotong Univ, Tribol Res Inst, Key Lab Adv Technol Mat, Chengdu 610031, Peoples R China. [Cai, Zhen-Bing; Meyer, Harry M., III; Ma, Cheng; Chi, Miaofang; Qu, Jun] Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37831 USA. [Luo, Huimin] Oak Ridge Natl Lab, Energy & Transportat Sci Div, Oak Ridge, TN 37831 USA. RP Qu, J (reprint author), Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37831 USA. EM qujn@ornl.gov RI Ma, Cheng/C-9120-2014; Chi, Miaofang/Q-2489-2015; OI Chi, Miaofang/0000-0003-0764-1567; Qu, Jun/0000-0001-9466-3179 FU Vehicle Technologies Office, Office of Energy Efficiency and Renewable Energy, US Department of Energy (DOE); DOE Office of Basic Energy Sciences FX The authors thank Dr. E.A. Bardasz of Lubrizol Corporation for providing the ZDDP. And thank D.W. Coffey and Dr. Y. Zhou of ORNL for TEM sample preparation and partial XPS analysis, respectively. This research was sponsored by The Vehicle Technologies Office, Office of Energy Efficiency and Renewable Energy, US Department of Energy (DOE). The characterization work was supported in part by ORNL's SHaRE User Facility, which is sponsored by The DOE Office of Basic Energy Sciences. NR 20 TC 12 Z9 12 U1 5 U2 37 PU ELSEVIER SCIENCE SA PI LAUSANNE PA PO BOX 564, 1001 LAUSANNE, SWITZERLAND SN 0043-1648 EI 1873-2577 J9 WEAR JI Wear PD NOV 15 PY 2014 VL 319 IS 1-2 BP 172 EP 183 DI 10.1016/j.wear.2014.08.002 PG 12 WC Engineering, Mechanical; Materials Science, Multidisciplinary SC Engineering; Materials Science GA AT6PP UT WOS:000345061600019 ER PT J AU Ryb, U Matmon, A Erel, Y Haviv, I Benedetti, L Hidy, AJ AF Ryb, U. Matmon, A. Erel, Y. Haviv, I. Benedetti, L. Hidy, A. J. TI Styles and rates of long-term denudation in carbonate terrains under a Mediterranean to hyper-arid climatic gradient SO EARTH AND PLANETARY SCIENCE LETTERS LA English DT Article DE denudation; chemical weathering; erosion; carbonate terrains; climatic gradient; Cl-36 ID CHEMICAL-WEATHERING RATES; SITU-PRODUCED BE-10; DEAD-SEA RIFT; COSMOGENIC CL-36; LANDSCAPE EVOLUTION; DRAINAGE BASINS; EROSION RATES; KARST AREAS; LIMESTONE; NUCLIDES AB Carbonate minerals, unlike silicates, have the potential to dissolve almost completely and with high efficiency. Thus, in carbonate terrains denudation rate and style (the governing process of denudation, mechanical or chemical) should be more sensitive to climatic forcing. Using Cl-36 measurements in 39 carbonate bedrock and sediment samples, we calculate long-term denudation rates across a sharp climatic gradient from Mediterranean to hyper-arid conditions. Our samples were collected along the Arugot watershed, which drains the eastern flank of the Judea Range (central Israel) to the Dead Sea and is characterized by a pronounced rain shadow. Denudation rates of flat-lying bedrock outcrops sampled along interfluves differ by an order of magnitude from similar to 20 mm ka(-1) in the Mediterranean zone to 1-3 mm ka(-1) in the hyper-arid zone. These rates are strongly correlated with precipitation, and thus reflect the importance of carbonate mineral dissolution in the overall denudation process. In contrast, denudation rates of steep bedrock surfaces depend on the hillslope gradient, but only in the hyper-arid climate zone, indicating that mechanical processes dominate the overall hillslope denudation within this zone. The dominance of slope-dependent mechanical erosion in the hyper-arid zone is also reflected by an increase in spatially-average denudation rates from 17-19 mm ka(-1) in the Mediterranean-semi-arid zones to 21-25 mm ka(-1) in the hyper-arid zone. These higher rates are attributed to clast contribution from steep slopes under arid climate. This suggests an increased importance of mechanical processes to the overall denudation in the hyper-arid zone. We demonstrate that the transition between chemically-dominated denudation to mechanically-dominated denudation occurs between 100 and 200 mm of mean annual precipitation. Long-term denudation rates across the Judea Range indicate that between Mediterranean and hyper-arid climates, chemical weathering rates are limited by precipitation. Nevertheless, in more humid climates, chemical weathering rates are apparently limited by the rates of carbonate mineral dissolution. This study demonstrates that carbonate terrains have the capacity to shift between mechanically and chemically dominated denudation in response to changes in precipitation. Similar transitions in response to changes in temperature or the level of tectonic activity have been previously reported. We suggest that the abrupt nature of such transitions can be primarily attributed to the efficiency of carbonate dissolution processes and the competition between surface and subsurface drainage systems in carbonate terrains. (C) 2014 Elsevier B.V. All rights reserved. C1 [Ryb, U.; Matmon, A.; Erel, Y.] Fredy & Nadine Herrmann Inst Earth Sci, IL-91904 Jerusalem, Israel. [Haviv, I.] Ben Gurion Univ Negev, Dept Geol & Environm Sci, IL-84105 Beer Sheva, Israel. [Benedetti, L.] Aix Marseille Univ, Ctr Rech & Enseignement Gosci Environm CEREGE, Inst Rech Dev, Coll France,Technopole Arbois,CNRS,UM 34, F-13545 Aix En Provence, France. [Hidy, A. J.] Lawrence Livermore Natl Lab, CAMS, Livermore, CA 94550 USA. RP Ryb, U (reprint author), Fredy & Nadine Herrmann Inst Earth Sci, Admond J Safra Campus, IL-91904 Jerusalem, Israel. FU Kaye-Einstein fellowship; Israel Science Foundation [50/10] FX The authors wish to thank D. Palchan, M. Davis, U. Davidovich, and Y. Goldsmith for their assistance in the field, to S. Mazze, S. Vainer, and A. Paldor for assisting in preparing the samples for 36Cl analyses, and to the staff of ASTER-CEREGE for AMS measurements. We thank five anonymous reviewers for their critical and detailed reviews. We also thank the Kaye-Einstein fellowship for their support during this study. This study was funded by Israel Science Foundation grant 50/10. This is LLNL-JRNL-658044. NR 75 TC 10 Z9 10 U1 2 U2 14 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0012-821X EI 1385-013X J9 EARTH PLANET SC LETT JI Earth Planet. Sci. Lett. PD NOV 15 PY 2014 VL 406 BP 142 EP 152 DI 10.1016/j.epsl.2014.09.008 PG 11 WC Geochemistry & Geophysics SC Geochemistry & Geophysics GA AS3YO UT WOS:000344211200015 ER PT J AU Syverson, DD Pester, NJ Craddock, PR Seyfried, WE AF Syverson, Drew D. Pester, Nicholas J. Craddock, Paul R. Seyfried, William E., Jr. TI Fe isotope fractionation during phase separation in the NaCl-H2O system: An experimental study with implications for seafloor hydrothermal vents SO EARTH AND PLANETARY SCIENCE LETTERS LA English DT Article DE Fe isotope fractionation; phase separation; mid-ocean ridge hydrothermal processes ID MID-ATLANTIC RIDGE; EAST PACIFIC RISE; IN-SITU XAS; CHLORIDE COMPLEXES; FLUIDS; IRON; SPECIATION; BENEATH; FIELD AB Phase separation has been proposed as a possible mechanism contributing to the Fe isotope composition of hydrothermal fluids at mid-ocean ridges. The uncertainty results largely from the emphasis on field data that can involve competing processes that obscure cause and effect of any one process. To better understand the potential significance of phase separation in the NaCl-Fe-H2O system on Fe isotope fractionation, temperature and pressure of a Fe-bearing NaCl fluid in a titanium flow reactor were carefully adjusted to produce vapor +/- liquid +/- halite, while the Fe isotope composition between coexisting phases was monitored. Two different P-T regions were emphasized: (1) 424-420 degrees C, 35.2-31.5 MPa; and (2) 464-466 degrees C, 29.8-24.7 MPa. Both regions were chosen to simulate the range of physical conditions that are experienced by hydrothermal fluids at mid-ocean ridges (MORs). Decompression induced phase separation in both P-T regions results in the vapor phase becoming enriched in the heavier isotopes of Fe, as the Fe/Cl ratio decreases. The coexisting NaCl-rich liquid phase remains essentially constant with respect to Fe/CI ratio and Fe isotope composition. Coinciding with the lowest vapor chlorinity in the vapor-liquid stability field, the Fe/Cl ratio of the vapor abruptly increases, while the Fe isotope fractionation between the vapor and liquid (10(3) ln alpha(56/54)(V/L)) reached a maximum value of +0.145 +/- 0.048 parts per thousand). Subsequently, Fe isotope fractionation decreased upon transition into the vapor-halite stability field (P-T region 2). We infer that the observed Fe isotope fractionation between vapor +/- liquid +/- halite is caused by differences in Fe speciation among coexisting chloride-bearing phases. The experimental study confirms for the first time that measurable Fe isotope variability can result from phase separation in high temperature hydrothermal systems. The species-dependent Fe isotope fractionation reported here is small relative to predicted mineral-mineral and mineral-fluid fractionations, especially if redox effects are involved as might occur during vent fluid-seawater mixing reactions and/or magmatic activity associated with seafloor eruptive episodes. (C) 2014 Elsevier B.V. All rights reserved. C1 [Syverson, Drew D.; Pester, Nicholas J.; Seyfried, William E., Jr.] Univ Minnesota, Dept Earth Sci, Minneapolis, MN 55455 USA. [Craddock, Paul R.] Univ Chicago, Dept Geophys Sci, Chicago, IL 60637 USA. [Craddock, Paul R.] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA. [Pester, Nicholas J.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Earth Sci, Berkeley, CA 94720 USA. [Craddock, Paul R.] Schlumberger Doll Res Ctr, Cambridge, MA 02139 USA. RP Syverson, DD (reprint author), Univ Minnesota, Dept Earth Sci, 310 Pillsbury Dr SE, Minneapolis, MN 55455 USA. EM syve0063@umn.edu RI Pester, Nicholas/G-2424-2015; OI Pester, Nicholas/0000-0002-1852-6663; Syverson, Drew/0000-0003-2838-1522; Craddock, Paul/0000-0003-4702-0204 FU NSF grants OCE [0751771, 1061308, 1232704]; University of Minnesota FX The authors would like to thank the two anonymous reviewers and the associate editor, Dr. Bernard Marty, for their constructive comments, which made this paper undoubtedly more clear. We would also like to thank Rick Knurr (U. of MN) for providing detailed chemical analyses of the fluid samples provided. The authors are grateful for the funding provided by the NSF grants OCE #0751771, 1061308, and 1232704 (WES). The corresponding author (DDS) also acknowledges funding awarded by the University of Minnesota through the Doctoral Fellowship during a portion of this research. NR 52 TC 4 Z9 4 U1 6 U2 30 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0012-821X EI 1385-013X J9 EARTH PLANET SC LETT JI Earth Planet. Sci. Lett. PD NOV 15 PY 2014 VL 406 BP 223 EP 232 DI 10.1016/j.epsl.2014.09.020 PG 10 WC Geochemistry & Geophysics SC Geochemistry & Geophysics GA AS3YO UT WOS:000344211200022 ER PT J AU Litombe, NE Bollinger, AT Hoffman, JE Bozovic, I AF Litombe, N. E. Bollinger, A. T. Hoffman, J. E. Bozovic, I. TI La2-xSrxCuO4 superconductor nanowire devices SO PHYSICA C-SUPERCONDUCTIVITY AND ITS APPLICATIONS LA English DT Article DE La2-xSrxCuO4; Nanowire; Fabrication; ALL-MBE; Lithography; Critical current ID TEMPERATURE; MAGNETORESISTANCE AB La2-xSrxCuO4 nanowire devices have been fabricated and characterized using electrical transport measurements. Nanowires with widths down to 80 nm are patterned using high-resolution electron beam lithography. However, the narrowest nanowires show incomplete superconducting transitions with some residual resistance at T = 4 K. Here, we report on the refinement of the fabrication process to achieve narrower nanowire devices with complete superconducting transitions, opening the path to the study of novel physics arising from dimension-limited superconductivity on the nanoscale. (C) 2014 Elsevier B.V. All rights reserved. C1 [Litombe, N. E.; Hoffman, J. E.] Harvard Univ, Cambridge, MA 02138 USA. [Litombe, N. E.; Bollinger, A. T.; Bozovic, I.] Brookhaven Natl Lab, Upton, NY 11973 USA. RP Bozovic, I (reprint author), Brookhaven Natl Lab, Upton, NY 11973 USA. EM bozovic@bnl.gov RI Hoffman, Jennifer/H-4334-2011 OI Hoffman, Jennifer/0000-0003-2752-5379 FU U.S. Department of Energy, Office of Basic Energy Sciences, Materials Sciences and Engineering Division; U.S. Department of Energy, Office of Basic Energy Sciences [DE-AC02-98CH10886] FX Research supported by the U.S. Department of Energy, Office of Basic Energy Sciences, Materials Sciences and Engineering Division. E-beam lithography was carried out at the Center for Functional Nanomaterials, Brookhaven National Laboratory, supported by the U.S. Department of Energy, Office of Basic Energy Sciences, under Contract No. DE-AC02-98CH10886. NR 22 TC 2 Z9 2 U1 2 U2 25 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0921-4534 EI 1873-2143 J9 PHYSICA C JI Physica C PD NOV 15 PY 2014 VL 506 SI SI BP 169 EP 173 DI 10.1016/j.physc.2014.06.010 PG 5 WC Physics, Applied SC Physics GA AS4JD UT WOS:000344240100028 ER PT J AU Kresin, V Ovchinnikov, Y AF Kresin, Vladimir Ovchinnikov, Yurii TI Superconducting state of metallic nanoclusters and Josephson tunneling networks SO PHYSICA C-SUPERCONDUCTIVITY AND ITS APPLICATIONS LA English DT Article DE Nanoclusters; Energy shells; Observables; Networks; Synchronization ID JUNCTION ARRAYS; CLUSTERS; TEMPERATURE AB Metallic nanoclusters form a new family of high temperature superconductors. In principle, the value of T-C can be raised up to room temperature. In addition, one can observe the Josephson tunneling between two clusters. One can build the nanocluster-based tunneling network capable to transfer a macroscopic supercurrent at high temperatures. Such a network can be synchronized and radiate as single junction. Published by Elsevier B.V. C1 [Kresin, Vladimir] Univ Calif Berkeley, Lawrence Berkeley Lab, Berkeley, CA 94720 USA. [Ovchinnikov, Yurii] RAN, L Landau Inst Theoret Phys, Moscow 117334, Russia. RP Kresin, V (reprint author), Univ Calif Berkeley, Lawrence Berkeley Lab, Berkeley, CA 94720 USA. EM vzkresin@lbl.gov NR 32 TC 0 Z9 0 U1 2 U2 11 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0921-4534 EI 1873-2143 J9 PHYSICA C JI Physica C PD NOV 15 PY 2014 VL 506 SI SI BP 201 EP 206 DI 10.1016/j.physc.2014.06.001 PG 6 WC Physics, Applied SC Physics GA AS4JD UT WOS:000344240100034 ER PT J AU Sun, ZJ Wells, D Segebade, C Quigley, K Chemerisov, S AF Sun, Z. J. Wells, D. Segebade, C. Quigley, K. Chemerisov, S. TI A comparison of various procedures in photon activation analysis with the same irradiation setup SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION B-BEAM INTERACTIONS WITH MATERIALS AND ATOMS LA English DT Article DE Photon activation analysis; Quasi-absolute method; Monte Carlo simulation; LINAC ID NEUTRON; SAMPLES AB A sample of known elemental concentrations was activated in the bremsstrahlung photon beam which was created by a pulsed electron LINAC. Several procedures of photon activation analysis, including those applied with/without reference material and with/without photon flux monitor, were conducted to make a comparison of their precision and accuracy in practice. Experimental results have indicated that: (1) relative procedures usually produce better outcome despite that the absolute measurement is straightforward and eliminate the assistance of reference materials; (2) among relative procedures, the method with internal flux monitor yields higher quality of the analytical results. In the article, the pros and cons of each procedure are discussed as well. (C) 2014 Elsevier B.V. All rights reserved. C1 [Sun, Z. J.; Quigley, K.; Chemerisov, S.] Argonne Natl Lab, Chem Sci & Engn Div, Argonne, IL 60439 USA. [Wells, D.] South Dakota Sch Mines & Technol, Dept Phys, Rapid City, SD 57701 USA. [Segebade, C.] Idaho State Univ, Idaho Accelerator Ctr, Pocatello, ID 83209 USA. RP Sun, ZJ (reprint author), Argonne Natl Lab, Chem Sci & Engn Div, 9700 S Cass Ave, Argonne, IL 60439 USA. FU U.S. Department of Energy, National Nuclear Security Administration's (NNSA's) Office of Defense Nuclear Nonproliferation [DE-AC02-06CH11357] FX This work is supported by the U.S. Department of Energy, National Nuclear Security Administration's (NNSA's) Office of Defense Nuclear Nonproliferation, under Contract DE-AC02-06CH11357. Argonne National Laboratory is operated for the U.S. Department of Energy by UChicago Argonne, LLC. The U.S. Government retains for itself, and others acting on its behalf, a paid-up nonexclusive, irrevocable worldwide license in said article to reproduce, prepare derivative works, distribute copies to the public, and perform publicly and display publicly, by or on behalf of the Government. NR 29 TC 4 Z9 4 U1 2 U2 13 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0168-583X EI 1872-9584 J9 NUCL INSTRUM METH B JI Nucl. Instrum. Methods Phys. Res. Sect. B-Beam Interact. Mater. Atoms PD NOV 15 PY 2014 VL 339 BP 53 EP 57 DI 10.1016/j.nimb.2014.08.021 PG 5 WC Instruments & Instrumentation; Nuclear Science & Technology; Physics, Atomic, Molecular & Chemical; Physics, Nuclear SC Instruments & Instrumentation; Nuclear Science & Technology; Physics GA AR7UP UT WOS:000343785500010 ER PT J AU Bannister, ME Hijazi, H Meyer, HM Cianciolo, V Meyer, FW AF Bannister, M. E. Hijazi, H. Meyer, H. M., III Cianciolo, V. Meyer, F. W. TI Surface-conductivity enhancement of PMMA by keV-energy metal-ion implantation SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION B-BEAM INTERACTIONS WITH MATERIALS AND ATOMS LA English DT Article DE Surface conductivity; Metal-ion implantation; Polymer; Tungsten ID SYSTEMS; FILMS AB An experiment has been proposed to measure the neutron electric dipole moment (nEDM) with high precision at the Oak Ridge National Laboratory (ORNL) Spallation Neutron Source. One of the requirements of this experiment is the development of PMMA (Lucite) material with a sufficiently conductive surface to permit its use as a high-voltage electrode while immersed in liquid He. At the ORNL Multicharged Ion Research Facility, an R&D activity is under way to achieve suitable surface conductivity in poly-methyl methacrylate (PMMA) using metal ion implantation. The metal implantation is performed using an electron-cyclotron-resonance (ECR) ion source and a recently developed beam line deceleration module that is capable of providing high flux beams for implantation at energies as low as a few tens of eV. The latter is essential for reaching implantation fluences exceeding 1 x 10(16) cm(-2), where typical percolation thresholds in polymers have been reported. In this contribution, we report results on initial implantation of Lucite by Ti and W beams with keV energies to average fluences in the range 0.5-6.2 x 10(16) cm(-2). Initial measurements of surface-resistivity changes are reported as function of implantation fluence, energy, and sample temperature. We also report X-ray photoelectron spectroscopy (XPS) surface and depth profiling measurements of the ion implanted samples, to identify possible correlations between the near surface and depth resolved implanted W concentrations and the measured surface resistivities. (C) 2014 Elsevier B.V. All rights reserved. C1 [Bannister, M. E.; Hijazi, H.; Meyer, H. M., III; Cianciolo, V.; Meyer, F. W.] Oak Ridge Natl Lab, Oak Ridge, TN 37831 USA. RP Meyer, FW (reprint author), Oak Ridge Natl Lab, Oak Ridge, TN 37831 USA. EM meyerfw@ornl.gov FU LDRD Program of Oak Ridge National Laboratory for the U.S. Department of Energy; Oak Ridge National Laboratory's Shared Research Equipment (ShaRE) User Program - Office of Basic Energy Sciences, U.S. Department of Energy FX This research was sponsored by the LDRD Program of Oak Ridge National Laboratory, managed by UT-Battelle, LLC, for the U.S. Department of Energy. HH was appointed through the ORNL Postdoctoral Research Associates Program administered jointly by Oak Ridge Institute of Science and Education (ORISE), Oak Ridge Associated Universities (ORAU) and Oak Ridge National Laboratory (ORNL). XPS instrument supported by Oak Ridge National Laboratory's Shared Research Equipment (ShaRE) User Program, which is sponsored by the Office of Basic Energy Sciences, U.S. Department of Energy. NR 14 TC 5 Z9 5 U1 4 U2 17 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0168-583X EI 1872-9584 J9 NUCL INSTRUM METH B JI Nucl. Instrum. Methods Phys. Res. Sect. B-Beam Interact. Mater. Atoms PD NOV 15 PY 2014 VL 339 BP 75 EP 84 DI 10.1016/j.nimb.2014.02.133 PG 10 WC Instruments & Instrumentation; Nuclear Science & Technology; Physics, Atomic, Molecular & Chemical; Physics, Nuclear SC Instruments & Instrumentation; Nuclear Science & Technology; Physics GA AR7UP UT WOS:000343785500014 ER PT J AU Kim, Y Ban, KY Kuciauskas, D Dippo, PC Honsberg, CB AF Kim, Yeongho Ban, Keun-Yong Kuciauskas, Darius Dippo, Patricia C. Honsberg, Christiana B. TI Effect of silicon delta-doping density on optical properties of type-II InAs/GaAsSb quantum dots SO JOURNAL OF CRYSTAL GROWTH LA English DT Article DE Low dimensional structures; Molecular beans epitaxy; Antimonides; Semiconducting III-V materials ID PHOTOLUMINESCENCE; SEMICONDUCTORS; LAYER AB We have investigated the optical properties of type-II InAs/GaAs0.83Sb0.17 quantum dots (QDs) with different silicon delta-doping densities of 5 x 10(11)), 5 x 10 and 2 x 10(12) cm(-2) using photoluminescence (PL). The PL spectra of the QD ground state (GS) emission peaks for the samples are blueshifted at a slower rate with increasing the doping density due to the enhanced radiative recombination rate of the carriers. The PL intensity ratio of the GS emission to the first excited state emission increases with the doping density, which is indicative of the faster radiative recombination at the GS subbands with the doping density. The redshift rate of the GS emissions becomes faster at a high temperature (> 130 K) as the doping density increases up to 5 x 10(11) cm(-2) resulting from the quantum confined Stark effect by the electric field of the ionized dopants, and decreases at an increased doping density of 2 x 10(12) cm(-2) due to the enhanced QD size uniformity. Time-resolved PL exhibits that the QD sample doped at 5 x 10(10) cm(-2) has a longer total radiative lifetime than the undopal sample, and a further increase in the doping density to 2 x 10(12) cm(-2) decreases the lifetime due to the enhancement of the radiative recombination through fast carrier relaxation. (C) 2014 Elsevier B.V. All rights reserved. C1 [Kim, Yeongho; Ban, Keun-Yong; Honsberg, Christiana B.] Arizona State Univ, Dept Elect Engn, Tempe, AZ 85287 USA. [Kuciauskas, Darius; Dippo, Patricia C.] Natl Renewable Energy Lab, Golden, CO 80401 USA. RP Kim, Y (reprint author), Arizona State Univ, Dept Elect Engn, Tempe, AZ 85287 USA. EM ykim172@asu.edu FU National Science Foundation (NSF); U.S. Department of Energy (DOE) under NSF CA [EEC-1041895]; National Renewable Energy Laboratory as a part of the Non-Proprietary Partnering Program [De-AC36-08-GO28308]; U.S. Department of Energy FX This material is based upon work primarily supported by the National Science Foundation (NSF) and the U.S. Department of Energy (DOE) under NSF CA No. EEC-1041895. Any opinions, findings and conclusions or recommendations expressed in this material are those of the authors and do not necessarily reflect those of NSF or DOE. This work was supported by the National Renewable Energy Laboratory as a part of the Non-Proprietary Partnering Program under Contract No. De-AC36-08-GO28308 with the U.S. Department of Energy. NR 21 TC 2 Z9 2 U1 0 U2 17 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0022-0248 EI 1873-5002 J9 J CRYST GROWTH JI J. Cryst. Growth PD NOV 15 PY 2014 VL 406 BP 68 EP 71 DI 10.1016/j.jcrysgro.2014.08.009 PG 4 WC Crystallography; Materials Science, Multidisciplinary; Physics, Applied SC Crystallography; Materials Science; Physics GA AQ8QC UT WOS:000343092800012 ER PT J AU Dalai, AK Wang, Y AF Dalai, Ajay K. Wang, Yong TI Preface for the special Issue: Sustainable Fuels and Chemicals SO CATALYSIS TODAY LA English DT Editorial Material C1 [Dalai, Ajay K.] Univ Saskatchewan, Coll Engn, Dept Chem & Biol Engn, Catalysis & Chem React Engn Lab, Saskatoon, SK S7N 5A9, Canada. [Wang, Yong] Washington State Univ, Voiland Sch Chem Engn & Bioengn, Pacific NW Natl Lab, Inst Integrated Catalysis, Richland, WA 99354 USA. RP Dalai, AK (reprint author), Univ Saskatchewan, Coll Engn, Dept Chem & Biol Engn, Catalysis & Chem React Engn Lab, Saskatoon, SK S7N 5A9, Canada. EM akd983@campus.usask.ca NR 0 TC 0 Z9 0 U1 1 U2 5 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0920-5861 EI 1873-4308 J9 CATAL TODAY JI Catal. Today PD NOV 15 PY 2014 VL 237 BP 1 EP 2 DI 10.1016/j.cattod.2014.08.004 PG 2 WC Chemistry, Applied; Chemistry, Physical; Engineering, Chemical SC Chemistry; Engineering GA AP2BR UT WOS:000341877900001 ER PT J AU Wang, H Lu, JL Marshall, CL Elam, JW Miller, JT Liu, HB Enterkin, JA Kennedy, RM Stair, PC Poeppelmeier, KR Marks, LD AF Wang, Hui Lu, Junling Marshall, Christopher L. Elam, Jeffrey W. Miller, Jeffrey T. Liu, HongBo Enterkin, James A. Kennedy, Robert M. Stair, Peter C. Poeppelmeier, Kenneth R. Marks, Laurence D. TI In situ XANES study of methanol decomposition and partial oxidation to syn-gas over supported Pt catalyst on SrTiO3 nanocubes SO CATALYSIS TODAY LA English DT Article DE Methanol; Decomposition; Partial oxidation; In situ XANES; SrTiO3 nanocuboid; Platinum nanoparticle ID HYDROGEN-PRODUCTION; TEMPERATURE; PT/AL2O3; PRETREATMENT AB A catalyst of Pt nanoparticles was prepared by atomic layer deposition on SrTiO3 nanocuboids and tested for methanol decomposition and partial oxidation. The catalyst had uniform nanoparticle size of 1.58 +/- 0.37 nm and a Pt (1 1 1) surface. In situ X-ray absorption near-edge spectroscopy (XANES) measured in a temperature-programmed reduction showed that the Pt particles were easily reduced. However, the as-received catalyst, a reduced catalyst, and an oxidized catalyst all had catalytic activity, differing slightly in methanol conversion and product selectivity. In situ XANES also revealed that CO adsorbed on the Pt sites was the only observed surface species during both methanol decomposition and partial oxidation. It seemed that the breakage of CH and OH bonds overwhelmingly occurred once methanol was adsorbed, forming H-2 and adsorbed CO. The latter was then released from the catalyst surface or was oxidized to CO2 when O-2 was present. (C) 2014 Elsevier B.V. All rights reserved. C1 [Wang, Hui; Marshall, Christopher L.; Miller, Jeffrey T.; Liu, HongBo] Chem Sci & Engn Div, Argonne, IL 60439 USA. [Lu, Junling; Elam, Jeffrey W.] Argonne Natl Lab, Div Energy Syst, Argonne, IL 60439 USA. [Wang, Hui] Univ Saskatchewan, Dept Chem & Biol Engn, Saskatoon, SK S7N 5A9, Canada. [Enterkin, James A.; Kennedy, Robert M.; Poeppelmeier, Kenneth R.] Northwestern Univ, Dept Chem, Evanston, IL 60208 USA. [Marks, Laurence D.] Northwestern Univ, Dept Mat Sci, Evanston, IL 60208 USA. RP Marshall, CL (reprint author), Chem Sci & Engn Div, Argonne, IL 60439 USA. EM marshall@anl.gov RI ID, MRCAT/G-7586-2011; Lu, Junling/F-3791-2010; Marks, Laurence/B-7527-2009; Marshall, Christopher/D-1493-2015 OI Lu, Junling/0000-0002-7371-8414; Marshall, Christopher/0000-0002-1285-7648 FU Institute for Atom-efficient Chemical Transformations (IACT), an Energy Frontier Research Center - U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences; University of Saskatchewan; Argonne National Laboratory FX This material is based upon work supported as part of the Institute for Atom-efficient Chemical Transformations (IACT), an Energy Frontier Research Center funded by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences. Support for H. Wang was provided by the University of Saskatchewan and Argonne National Laboratory. NR 21 TC 5 Z9 5 U1 7 U2 86 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0920-5861 EI 1873-4308 J9 CATAL TODAY JI Catal. Today PD NOV 15 PY 2014 VL 237 BP 71 EP 79 DI 10.1016/j.cattod.2014.02.008 PG 9 WC Chemistry, Applied; Chemistry, Physical; Engineering, Chemical SC Chemistry; Engineering GA AP2BR UT WOS:000341877900010 ER PT J AU Ramasamy, KK Wang, Y AF Ramasamy, Karthikeyan K. Wang, Yong TI Ethanol conversion to hydrocarbons on HZSM-5: Effect of reaction conditions and Si/Al ratio on the product distributions SO CATALYSIS TODAY LA English DT Article DE HZSM-5; Si/Al ratio; Ethanol to hydrocarbon; Coke deposition; WHSV ID ZEOLITE CATALYSTS; AQUEOUS-ETHANOL; COKE FORMATION; METHANOL; DEACTIVATION; H-ZSM-5; MECHANISM; TRANSFORMATION; COKING; ZSM-5 AB The Conversion of ethanol to hydrocarbon over HZSM-5 zeolite with different Si/Al ratios was investigated under various reaction conditions. The catalyst with a higher Si/Al ratio (low acid density) deactivated faster and generated more unsaturated compounds at a similar time-on-stream. Temperature affects the catalytic activity with respect to liquid hydrocarbon generation and the hydrocarbon product composition. At lower temperatures (similar to 300 degrees C), the catalyst deactivated faster with respect to the liquid hydrocarbon formation. Higher temperatures (similar to 400 degrees C) reduced the formation of liquid range hydrocarbons and formed more gaseous fractions. Weight hourly space velocity was also found to affect product selectivity with higher weight hourly space velocity leading to a higher extent of ethylene formation. The experimental results were analyzed in terms of the product composition and the coke content with respect to catalyst time-on-stream and compared with the catalyst lifetime with respect to the variables tested on the conversion of ethanol to hydrocarbon. (C) 2014 Elsevier B.V. All rights reserved. C1 [Ramasamy, Karthikeyan K.; Wang, Yong] Pacific NW Natl Lab, Inst Integrated Catalysis, Richland, WA 99354 USA. [Ramasamy, Karthikeyan K.; Wang, Yong] Washington State Univ, Voiland Sch Chem Engn & Bioengn, Pullman, WA 99163 USA. RP Ramasamy, KK (reprint author), Pacific NW Natl Lab, 902 Battelle Blvd, Richland, WA 99352 USA. EM karthi@pnnl.gov; yong.wang@pnnl.gov RI Ramasamy, karthikeyan/H-9981-2014 FU U.S. Department of Energy's Bioenergy Technologies Office; Laboratory Directed Research and Development program at Pacific Northwest National Laboratory; Battelle Memorial Institute for the U.S. Department of Energy [DE-AC05-76RL01830] FX This work was supported by the U.S. Department of Energy's Bioenergy Technologies Office. The authors also thank the Laboratory Directed Research and Development program at Pacific Northwest National Laboratory for funding the project. Pacific Northwest National Laboratory is operated by the Battelle Memorial Institute for the U.S. Department of Energy under contract no. DE-AC05-76RL01830. NR 32 TC 16 Z9 18 U1 3 U2 59 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0920-5861 EI 1873-4308 J9 CATAL TODAY JI Catal. Today PD NOV 15 PY 2014 VL 237 BP 89 EP 99 DI 10.1016/j.cattod.2014.02.044 PG 11 WC Chemistry, Applied; Chemistry, Physical; Engineering, Chemical SC Chemistry; Engineering GA AP2BR UT WOS:000341877900012 ER PT J AU Marin-Flores, OG Karim, AM Wang, Y AF Marin-Flores, Oscar G. Karim, Ayman M. Wang, Yong TI Role of tungsten in the aqueous phase hydrodeoxygenation of ethylene glycol on tungstated zirconia supported palladium SO CATALYSIS TODAY LA English DT Article DE Palladium; Tungstated zirconia; Aqueous phase hydrodeoxygenation; Aqueous phase reforming; Ethylene glycol ID LIGNOCELLULOSIC BIOMASS; PD CLUSTERS; CATALYSTS; ACIDITY; CONVERSION; CHEMICALS; ZEOLITES; SORBITOL; SILICA; OXIDE AB The focus of the present work was specifically on the elucidation of the role played by tungsten on the catalytic activity and selectivity of tungstated zirconia supported palladium (Pd-mWZ) for the aqueous phase hydrodeoxygenation (APHDO) of ethylene glycol (EG). Zirconia supported palladium (Pd-mZ) was used as reference. The catalysts were prepared via incipient wet impregnation and characterized using X-ray diffraction (XRD), temperature-programmed reduction (TPR), CO pulse chemisorption, CO-DRIFTS, ammonia temperature-programmed desorption (NH3-TPD) and pyridine adsorption. The presence of W results in larger Pd particles on supported Pd catalysts, i.e., 0.9 and 6.1 nm Pd particles are for Pd-mZ and Pd-mWZ, respectively. The catalytic activity measurements show that the overall intrinsic activity of Pd-particles on mWZ is 1.9 times higher than on mZ. APHDO process appears to be highly favored on Pd-mWZ whereas Pd-mZ exhibits a higher selectivity for reforming. This difference in terms of selectivity seems to be related to the high concentration of Bronsted acid sites and electron-deficient Pd species present on Pd-mWZ. (C) 2014 Elsevier B.V. All rights reserved. C1 [Marin-Flores, Oscar G.; Wang, Yong] Washington State Univ, Gene & Linda Voiland Sch Chem Engn & Bioengn, Pullman, WA 99164 USA. [Karim, Ayman M.; Wang, Yong] Pacific NW Natl Lab, Inst Integrated Catalysis, Richland, WA 99352 USA. RP Karim, AM (reprint author), Pacific NW Natl Lab, Inst Integrated Catalysis, Richland, WA 99352 USA. EM ayman.karim@pnnl.gov; wang42@wsu.edu RI Karim, Ayman/G-6176-2012 OI Karim, Ayman/0000-0001-7449-542X FU National Advanced Biofuels Consortium (NABC), Department of Energy's Office of Biomass Program; Battelle for the United States Department of Energy [DE-AC05-76RL01830] FX We would like to acknowledge Virent for their initial work on Pd/W-ZrO2 for HDO of polyols, and we would like to thank Dr. Randy Cortright, Ms. Liz Woods and Mr. Brian Blank for numerous invaluable discussions and suggestions. We acknowledge the financial support from the National Advanced Biofuels Consortium (NABC) which is funded by the Department of Energy's Office of Biomass Program with recovery act funds. The Pacific Northwest National Laboratory is operated by Battelle for the United States Department of Energy under Contract DE-AC05-76RL01830. NR 34 TC 3 Z9 3 U1 4 U2 62 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0920-5861 EI 1873-4308 J9 CATAL TODAY JI Catal. Today PD NOV 15 PY 2014 VL 237 BP 118 EP 124 DI 10.1016/j.cattod.2014.03.068 PG 7 WC Chemistry, Applied; Chemistry, Physical; Engineering, Chemical SC Chemistry; Engineering GA AP2BR UT WOS:000341877900015 ER PT J AU Wickramanayake, S Hopkinson, D Myers, C Hong, L Feng, J Seol, Y Plasynski, D Zeh, M Luebke, D AF Wickramanayake, Shan Hopkinson, David Myers, Christina Hong, Lei Feng, Jie Seol, Yongkoo Plasynski, Devon Zeh, Matthew Luebke, David TI Mechanically robust hollow fiber supported ionic liquid membranes for CO2 separation applications SO JOURNAL OF MEMBRANE SCIENCE LA English DT Article DE Torlon; Matrimid; Hollow fiber; Ionic liquid; Strength ID CARBON-DIOXIDE; MICROFILTRATION MEMBRANES; ELECTRON-MICROGRAPHS; IMAGE-ANALYSIS; PERMEABILITY AB Polymeric hollow fiber supported ionic liquid membranes (SILMs) were fabricated utilizing Matrimid (R) and Torlon (R) as the supporting structure and the ionic liquid (IL) 1-hexyl-3-methylimidalzolium bis(trifluoromethylsulfonyl)imide ([C(6)mim][Tf2N]) as the gas transport media. This IL served as a baseline while the polymer and the fiber pore morphology were varied in order to optimize the support structure. By using sufficiently high fiber porosity, and thus maximizing the IL content of the membrane, it was found that the permeance and selectivity for CO2/H-2 separation were comparable for both Matrimid (R) and Torlon (R) supports. However, the mechanical strength of Matrimid (R) supports was low when saturated with IL Therefore Torlon (R) fibers were subsequently investigated because of the higher strength of this material. Molecular modeling was used to investigate the source of the increased strength of Torlon (R), and it was found that the polymer chains in Torlon (R) Lend to interlock with each other to a greater degree than Matrimid (R). Also, the IL [C(6)mim][Tf2N] has less interaction with Torlon (R) than with Matrimid (R). In this work the permeance and selectivity for CO2/H-2 of these hollow fiber SILMs are reported, as well as the tensile strength, Young's modulus, and glass transition temperature. Threshold image analysis was used to determine the volume fractions of polymer, macro-voids, and micro-voids. X-ray computed tomography scanning was used to non-destructively evaluate the location of IL within the fiber wall. (C) 2014 Elsevier B.V. All rights reserved. C1 [Wickramanayake, Shan; Hopkinson, David; Myers, Christina; Hong, Lei; Feng, Jie; Seol, Yongkoo; Plasynski, Devon; Zeh, Matthew; Luebke, David] Natl Energy Technol Lab, Pittsburgh, PA 15236 USA. [Wickramanayake, Shan; Hong, Lei] URS Energy & Construct, Pittsburgh, PA 15236 USA. [Feng, Jie; Plasynski, Devon; Zeh, Matthew] Oak Ridge Inst Sci & Educ, Pittsburgh, PA 15236 USA. RP Wickramanayake, S (reprint author), URS Energy & Construct, 626 Cochrans Mill Rd, Pittsburgh, PA 15236 USA. EM shan.wickramanayake@urs.com FU U.S. Department of Energy National Energy Technology Laboratory under the FY14 Carbon Capture field work proposal; agency of the United States Government FX We gratefully acknowledge funding and support from the U.S. Department of Energy National Energy Technology Laboratory under the FY14 Carbon Capture field work proposal. This report was prepared as an account of work sponsored by an agency of the United States Government, Neither the United States Government nor any agency thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe on privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof. The views and opinions of authors expressed herein do not necessarily state or reflect those of the United States Government or any agency thereof. NR 27 TC 7 Z9 7 U1 7 U2 120 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0376-7388 EI 1873-3123 J9 J MEMBRANE SCI JI J. Membr. Sci. PD NOV 15 PY 2014 VL 470 BP 52 EP 59 DI 10.1016/j.memsci.2014.07.015 PG 8 WC Engineering, Chemical; Polymer Science SC Engineering; Polymer Science GA AO2IB UT WOS:000341141800006 ER PT J AU Mulvenna, RA Weidman, JL Jing, BX Pople, JA Zhu, YX Boudouris, BW Phillip, WA AF Mulvenna, Ryan A. Weidman, Jacob L. Jing, Benxin Pople, John A. Zhu, Yingxi Boudouris, Bryan W. Phillip, William A. TI Tunable nanoporous membranes with chemically-tailored pore walls from triblock polymer templates SO JOURNAL OF MEMBRANE SCIENCE LA English DT Article DE PI-PS-PUMA triblock polymers; RAFT polymerization; Self-assembly and non-solvent induced; phase separation (SNIPS); Nanofiltration; Ultrafiltration ID LIVING RADICAL POLYMERIZATION; BLOCK-COPOLYMER MEMBRANES; ULTRAFILTRATION MEMBRANES; NANOFILTRATION MEMBRANES; FILTRATION MEMBRANES; WATER FILTRATION; PHASE-INVERSION; THIN-FILMS; PERFORMANCE; SEPARATION AB Membranes derived from sell assembled block polymers have shown promise as highly selective and highly permeable filters, but the complex synthetic routes and limited pore functionalities of existing systems need to be improved if these materials are to serve as a platform for the next generation of nanostructured membranes. Here, the facile synthesis of a polyisoprene-b-polystyrene-b-poly(N,N-dimethylacrylamide) (PI-PS-PDMA) triblock polymer using a controlled reversible addition fragmentation chain transfer (RAFT) polymerization mechanism is reported. This material is then processed into a membrane using a self assembly and non solvent induced phase separation (SNIPS) technique, which creates an asymmetric, porous structure consisting of a selective layer that contains a high density of PDMA-lined pores (9.4 x 10(13) pores m(-2)) with an average diameter of 8.1 nm, as determined using solute rejection tests. Solvent Bow experiments demonstrate that the PI-PS-PDMA membrane has a pH independent permeability of 6 L m(-2) h(-1) bar(-1). The PDMA moiety lining the pore walls is converted, through simple hydrolysis in the solid stare, to yield a poly(acrylic acid)-lined (PAA-lined) structure. The permeability of the PI-PS-PAA membrane is pH dependent, and ranges from 0.6 L m(-2) h(-1) bar(-1) for solutions with a pH greater than 4 to 16 L m(-2) h-(1) bar(-1) for a solution at pH 1. Solute rejection tests demonstrated a pore size of 3.4 nm for the PI-PS-PAA membrane, which is the smallest pore size reported to date for membranes fabricated horn self-assembled block polymers. The Facile synthesis of the PI-PS-PDMA material, the scalable SNIPS membrane fabrication protocol, and the simple conversion chemistry of the pore functionality demonstrate that these nanostructured membranes are a strong platform for applications within the range of water purification, pharmaceutical separations, sensors, and drug delivery. (C) 2014 Elsevier B.V. All rights reserved. C1 [Mulvenna, Ryan A.; Boudouris, Bryan W.] Purdue Univ, Sch Chem Engn, W Lafayette, IN 47907 USA. [Weidman, Jacob L.; Jing, Benxin; Zhu, Yingxi; Phillip, William A.] Univ Notre Dame, Dept Chem & Biomol Engn, Notre Dame, IN 46556 USA. [Pople, John A.] SLAC, Stanford Synchrotron Radiat Lightsource, Menlo Pk, CA 94025 USA. RP Boudouris, BW (reprint author), Purdue Univ, Sch Chem Engn, 480 Stadium Mall Dr, W Lafayette, IN 47907 USA. EM boudouris@purdue.edu; wphillip@nd.edu RI Jing, Benxin/I-4944-2014 OI Jing, Benxin/0000-0002-8400-1937 FU Ralph W. and Grace M. Showalter Research Trust Award at Purdue University; Indiana Clinical and Translational Sciences Institute; National Institutes of Health, National Center for Advancing Translational Sciences, Clinical and Translational Sciences Award through the Collaboration in Translational Research (CTR) Pilot Program [TR000006] FX We gratefully acknowledge support from the Ralph W. and Grace M. Showalter Research Trust Award at Purdue University, Portions of this work were made possible with support from the Indiana Clinical and Translational Sciences Institute funded, in part by Grant number TR000006 (Project Manager: Dr. Thomas Sors) from the National Institutes of Health, National Center for Advancing Translational Sciences, Clinical and Translational Sciences Award through the Collaboration in Translational Research (CTR) Pilot Program. Portions of this research were carried out at the Stanford Synchrotron Radiation Lightsource, a Directorate of SLAC National Accelerator and an Office of Science User Facility operated for the U.S. Department of Energy Office of Science by Stanford University. Portions of this research were also performed with the equipment from the Center for Environmental Science and Technology (CEST) at Notre Dame and Notre Dame Integrated Imaging Facility (NDIIF). NR 53 TC 25 Z9 25 U1 12 U2 145 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0376-7388 EI 1873-3123 J9 J MEMBRANE SCI JI J. Membr. Sci. PD NOV 15 PY 2014 VL 470 BP 246 EP 256 DI 10.1016/j.memsci.2014.07.021 PG 11 WC Engineering, Chemical; Polymer Science SC Engineering; Polymer Science GA AO2IB UT WOS:000341141800026 ER PT J AU Ramirez, AI Aggarwal, SK Som, S Rutter, TP Longman, DE AF Ramirez, A. I. Aggarwal, S. K. Som, S. Rutter, T. P. Longman, D. E. TI Effects of blending a heavy alcohol (C20H40O with diesel in a heavy-duty compression-ignition engine SO FUEL LA English DT Article DE Second-generation biofuel; In-cylinder endoscopy; Bio-derived alcohol; Cavitation modeling; CO and NOx measurements ID BIODIESEL FUELS; EMISSIONS; OIL; COMBUSTION; PERFORMANCE; SPRAY AB There is an extensive worldwide search for alternate fuels that can displace fossil-based resources, yet still fit within existing infrastructure. At Argonne National Laboratory, strains of fuel have been designed that are generated by photosynthetic bacteria, eventually producing a heavy alcohol called phytol (C20H40O). Phytol's physical and chemical properties (cetane number, heat of combustion, heat of vaporization, density, surface tension, etc.) correspond in magnitude to those of diesel fuel, suggesting that phytol might be a good blending agent in compression ignition (CI) engine applications. The main objective of this study is to investigate the feasibility of using phytol as a blending agent with diesel. Three phytol-diesel blends were chosen for evaluation: P5, P10, and P20 (5%, 10%, and 20% phytol by volume). The fuel blends were extensively analyzed to determine their chemical and physical properties, with mostly comparable values, excepting viscosity and vapor pressure. In order to understand the effects of higher viscosity phytol in the fuel injector, three-dimensional simulations of transient, turbulent nozzle flow compared the injection and cavitation characteristics of the various blends. Specifically, area and discharge coefficients and mass flow rates of diesel and phytol blends were compared under corresponding engine operating conditions. Experimental research was performed using a single-cylinder engine under conventional operating conditions to gather comparative performance and emissions characteristics of the various blends of phytol and diesel. The influence of the fuel's chemical composition on performance and emission characteristics was captured by executing an injection timing sweep. Combustion characteristics such as the in-cylinder pressure trace were comparable for the diesel and all the blends with phytol at each of the injection timings. The diesel/phytol blends show similar emissions characteristics as the diesel. The combustion event was depicted by performing high-speed, natural luminosity endoscopic imaging. The conclusion is that phytol may be a suitable blending agent with diesel fuel for CI applications. Published by Elsevier Ltd. C1 [Ramirez, A. I.; Aggarwal, S. K.] Univ Illinois, Dept Mech & Ind Engn, Chicago, IL 60680 USA. [Som, S.; Rutter, T. P.; Longman, D. E.] Argonne Natl Lab, Ctr Transportat Res, Argonne, IL 60439 USA. RP Ramirez, AI (reprint author), Univ Illinois, Dept Mech & Ind Engn, Chicago, IL 60680 USA. EM aramir12@uic.edu FU Argonne, a U.S. Department of Energy Office of Science laboratory [DE-AC02-06CH11357]; DOE's Office of Vehicle Technologies, Office of Energy Efficiency and Renewable Energy [DE-AC02-06CH11357] FX The submitted manuscript has been created by UChicago Argonne, LLC, operator of Argonne National Laboratory (Argonne). Argonne, a U.S. Department of Energy Office of Science laboratory, is operated under Contract No. DE-AC02-06CH11357. The U.S. Government retains for itself, and others acting on its behalf, a paid-up, nonexclusive, irrevocable worldwide license in said article to reproduce, prepare derivative works, distribute copies to the public, and perform publicly and display publicly, by or on behalf of the Government.; This research was funded by DOE's Office of Vehicle Technologies, Office of Energy Efficiency and Renewable Energy under Contract No. DE-AC02-06CH11357. The authors wish to thank Kevin Stork, program manager at DOE, for his support. NR 52 TC 4 Z9 4 U1 0 U2 41 PU ELSEVIER SCI LTD PI OXFORD PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, OXON, ENGLAND SN 0016-2361 EI 1873-7153 J9 FUEL JI Fuel PD NOV 15 PY 2014 VL 136 BP 89 EP 102 DI 10.1016/j.fuel.2014.06.039 PG 14 WC Energy & Fuels; Engineering, Chemical SC Energy & Fuels; Engineering GA AO4JC UT WOS:000341302300011 ER PT J AU Bhavsar, S Tackett, B Veser, G AF Bhavsar, Saurabh Tackett, Brian Veser, Goetz TI Evaluation of iron- and manganese-based mono- and mixed-metallic oxygen carriers for chemical looping combustion SO FUEL LA English DT Article DE Chemical looping combustion; CO2 capture; Iron; Manganese; Mixed oxides ID FLUIDIZED-BED; CO2 CAPTURE; UNCOUPLING CLOU; SOLID FUELS; OXIDES; METHANE; REACTOR; GAS; CLC; OXIDATION AB Chemical looping combustion (CLC) is an emerging technology for clean combustion of fossil fuels with inherent CO2 capture. In the present work, we investigate the use of iron and manganese based mixed oxides (MnxFe1 (x)-CeO2)supported on CeO2 as oxygen carriers in CLC. The low cost and low toxicity of iron and manganese make them interesting candidates for CLC, but both mono-metallic carriers suffer from issues of low reactivity, and manganese is additionally prone to form undesired spinel structures with typical oxide supports. Mono-and bimetallic oxygen carriers were synthesized across the entire spectrum of compositions from pure Mn to pure Fe (with x = 0, 0.1, 0.33, 0.5, 0.8, 0.9, 1), characterized, and tested in thermogravimetric and fixed-bed reactor studies using H-2 and CH4 as fuels. We find that the use of ceria as support results in stable operation for all compositions of the metal phase, including pure Mn. Bimetallic carriers with high Fe content, which contain a FeMnO3 phase, exhibit an unusual, reversible de-alloying/re-alloying behavior during cyclic redox operation, which precludes any synergistic effects between the two metals and results in slowed reduction kinetics. However, Mn-rich carriers show a pronounced increase in carrier reactivity and selectivity for total oxidation of methane due to the addition of small amounts of Fe, indicating the promise of appropriately designed FeMn carriers as low-cost, environmentally benign oxygen carrier materials for chemical looping combustion. (C) 2014 Elsevier Ltd. All rights reserved. C1 [Bhavsar, Saurabh; Tackett, Brian; Veser, Goetz] Univ Pittsburgh, Swanson Sch Engn, Dept Chem Engn, Pittsburgh, PA 15261 USA. [Bhavsar, Saurabh; Veser, Goetz] US DOE, Natl Energy Technol Lab, Pittsburgh, PA USA. RP Veser, G (reprint author), Univ Pittsburgh, Swanson Sch Engn, Dept Chem Engn, Pittsburgh, PA 15261 USA. EM gveser@pitt.edu FU U.S. Department of Energy's National Energy Technology Laboratory's on-going research under the RDS [DE-AC26-04NT41817]; National Science Foundation (CBET) [1159853]; University of Pittsburgh's Mascaro Center for Sustainable Innovation FX This technical effort was performed in support of the U.S. Department of Energy's National Energy Technology Laboratory's on-going research under the RDS contract DE-AC26-04NT41817. Furthermore, financial support by the National Science Foundation (CBET # 1159853) and by the University of Pittsburgh's Mascaro Center for Sustainable Innovation is gratefully acknowledged. Finally, we would like to thank Prashant Kumta and Karan Kadakia for their help with Rietveld analysis. NR 53 TC 14 Z9 14 U1 9 U2 83 PU ELSEVIER SCI LTD PI OXFORD PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, OXON, ENGLAND SN 0016-2361 EI 1873-7153 J9 FUEL JI Fuel PD NOV 15 PY 2014 VL 136 BP 268 EP 279 DI 10.1016/j.fuel.2014.07.068 PG 12 WC Energy & Fuels; Engineering, Chemical SC Energy & Fuels; Engineering GA AO4JC UT WOS:000341302300033 ER PT J AU Hyman, JD Winter, CL AF Hyman, Jeffrey D. Winter, C. Larrabee TI Stochastic generation of explicit pore structures by thresholding Gaussian random fields SO JOURNAL OF COMPUTATIONAL PHYSICS LA English DT Article DE Porous media; Stochastic methods; Minkowski functionals; Direct numerical simulation ID STRONGLY CORRELATED SYSTEMS; POROUS-MEDIA; FLOW; PERCOLATION; BOUNDARY; SIMULATIONS; GEOMETRIES; HEART; MODEL AB We provide a description and computational investigation of an efficient method to stochastically generate realistic pore structures. Smolarkiewicz and Winter introduced this specific method in pores resolving simulation of Darcy flows (Smolarkiewicz and Winter, 2010 [1]) without giving a complete formal description or analysis of the method, or indicating how to control the parameterization of the ensemble. We address both issues in this paper. The method consists of two steps. First, a realization of a correlated Gaussian field, or topography, is produced by convolving a prescribed kernel with an initial field of independent, identically distributed random variables. The intrinsic length scales of the kernel determine the correlation structure of the topography. Next, a sample pore space is generated by applying a level threshold to the Gaussian field realization: points are assigned to the void phase or the solid phase depending on whether the topography over them is above or below the threshold. Hence, the topology and geometry of the pore space depend on the form of the kernel and the level threshold. Manipulating these two user prescribed quantities allows good control of pore space observables, in particular the Minkowski functionals. Extensions of the method to generate media with multiple pore structures and preferential flow directions are also discussed. To demonstrate its usefulness, the method is used to generate a pore space with physical and hydrological properties similar to a sample of Berea sandstone. (C) 2014 Elsevier Inc. All rights reserved. C1 [Hyman, Jeffrey D.; Winter, C. Larrabee] Univ Arizona, Program Appl Math, Tucson, AZ 85721 USA. [Hyman, Jeffrey D.] Los Alamos Natl Lab, Computat Earth Sci Earth & Environm Sci EES 16, Los Alamos, NM 87544 USA. [Hyman, Jeffrey D.] Los Alamos Natl Lab, Ctr Nonlinear Studies, Los Alamos, NM 87544 USA. [Winter, C. Larrabee] Univ Arizona, Dept Hydrol & Water Resources, Tucson, AZ 85721 USA. RP Hyman, JD (reprint author), Univ Arizona, Program Appl Math, Tucson, AZ 85721 USA. EM jhyman@lanl.gov; winter@email.arizona.edu OI Hyman, Jeffrey /0000-0002-4224-2847 FU U.S. Department of Energy [DE-AC52-06NA25396] FX We thank M. Zhang for providing the sample of Berea sandstone, J.M. Hyman, A. Guadagnini and C. M. Newman for several insightful discussions and encouragement, and B. Berman for helping with image processing. We gratefully acknowledge the support of the U.S. Department of Energy through the LANL/LDRD Program for this work (Grant no. DE-AC52-06NA25396). NR 56 TC 3 Z9 3 U1 3 U2 29 PU ACADEMIC PRESS INC ELSEVIER SCIENCE PI SAN DIEGO PA 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA SN 0021-9991 EI 1090-2716 J9 J COMPUT PHYS JI J. Comput. Phys. PD NOV 15 PY 2014 VL 277 BP 16 EP 31 DI 10.1016/j.jcp.2014.07.046 PG 16 WC Computer Science, Interdisciplinary Applications; Physics, Mathematical SC Computer Science; Physics GA AO4LV UT WOS:000341311000002 ER PT J AU Vogman, GV Colella, P Shumlak, U AF Vogman, G. V. Colella, P. Shumlak, U. TI Dory-Guest-Harris instability as a benchmark for continuum kinetic Vlasov-Poisson simulations of magnetized plasmas SO JOURNAL OF COMPUTATIONAL PHYSICS LA English DT Article DE Vlasov-Poisson; Dory-Guest-Harris instability; Plasma kinetic theory; Continuum kinetic benchmark; Electrostatic waves in magnetized plasma; Phase space ID SEMI-LAGRANGIAN METHOD; MAXWELL SYSTEM; PERPENDICULAR PROPAGATION; WEIBEL INSTABILITY; NUMERICAL SCHEME; WAVES; EQUATION; INTEGRATION; SPACE; FIELD AB The Dory-Guest-Harris instability is demonstrated to be a well-suited benchmark for continuum kinetic Vlasov-Poisson algorithms. The instability is a special case of perpendicularly-propagating kinetic electrostatic waves in a warm uniformly magnetized plasma. A complete derivation of the closed-form linear theory dispersion relation for the instability is presented. The electric field growth rates and oscillation frequencies specified by the dispersion relation provide concrete measures against which simulation results can be quantitatively compared. A fourth-order continuum kinetic algorithm is benchmarked against the instability, and is demonstrated to have good convergence properties and close agreement with theoretical growth rate and oscillation frequency predictions. Second-order accurate simulations are also shown to be consistent with theoretical predictions, but require higher resolution for convergence. The Dory-Guest-Harris instability benchmark extends the scope of current standard test problems by providing a substantive means of validating continuum kinetic simulations of magnetized plasmas in higher-dimensional 3D (x, v(x), v(y)) phase space. The linear theory analysis, initial conditions, algorithm description, and comparisons between theoretical predictions and simulation results are presented. (C) 2014 Elsevier Inc. All rights reserved. C1 [Vogman, G. V.] Univ Calif Berkeley, Appl Sci & Technol Program, Berkeley, CA 94720 USA. [Colella, P.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Computat Res Div, Berkeley, CA 94720 USA. [Colella, P.] Univ Calif Berkeley, Dept Elect Engn & Comp Sci, Berkeley, CA 94720 USA. [Shumlak, U.] Univ Washington, Aerosp & Energet Res Program, Seattle, WA 98195 USA. RP Vogman, GV (reprint author), Univ Calif Berkeley, Appl Sci & Technol Program, Berkeley, CA 94720 USA. OI Shumlak, Uri/0000-0002-2918-5446 FU Department of Energy Office of Science Graduate Fellowship Program (DOE SCGF); Office of Advanced Scientific Computing Research of the US Department of Energy [DE-AC02-05CH11231]; United States Air Force Office of Scientific Research [FA9550-11-1-0167] FX This research was supported by an award from the Department of Energy Office of Science Graduate Fellowship Program (DOE SCGF), agrant from the Office of Advanced Scientific Computing Research of the US Department of Energy under Contract Number DE-AC02-05CH11231, and a grant from the United States Air Force Office of Scientific Research under grant number FA9550-11-1-0167. NR 51 TC 1 Z9 1 U1 0 U2 9 PU ACADEMIC PRESS INC ELSEVIER SCIENCE PI SAN DIEGO PA 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA SN 0021-9991 EI 1090-2716 J9 J COMPUT PHYS JI J. Comput. Phys. PD NOV 15 PY 2014 VL 277 BP 101 EP 120 DI 10.1016/j.jcp.2014.08.014 PG 20 WC Computer Science, Interdisciplinary Applications; Physics, Mathematical SC Computer Science; Physics GA AO4LV UT WOS:000341311000006 ER PT J AU Plunkett, P Hu, J Siefert, C Atzberger, PJ AF Plunkett, Pat Hu, Jonathan Siefert, Christopher Atzberger, Paul J. TI Spatially adaptive stochastic methods for fluid-structure interactions subject to thermal fluctuations in domains with complex geometries SO JOURNAL OF COMPUTATIONAL PHYSICS LA English DT Article DE Stochastic Eulerian Lagrangian method; Immersed boundary method; Adaptive numerical methods; Multigrid; Stochastic numerical methods; Stochastic partial differential equations ID IMMERSED BOUNDARY METHOD; NAVIER-STOKES EQUATIONS; MONTE-CARLO METHOD; HYDRODYNAMIC INTERACTION; MULTIQUADRATIC ACTIONS; PROJECTION METHOD; DYNAMICS; PARTICLES; VERSION; BODIES AB We develop stochastic mixed finite element methods for spatially adaptive simulations of fluid-structure interactions when subject to thermal fluctuations. To account for thermal fluctuations, we introduce a discrete fluctuation-dissipation balance condition to develop compatible stochastic driving fields for our discretization. We perform analysis that shows our condition is sufficient to ensure results consistent with statistical mechanics. We show the Gibbs-Boltzmann distribution is invariant under the stochastic dynamics of the semi-discretization. To generate efficiently the required stochastic driving fields, we develop a Gibbs sampler based on iterative methods and multigrid to generate fields with O (N) computational complexity. Our stochastic methods provide an alternative to uniform discretizations on periodic domains that rely on Fast Fourier Transforms. To demonstrate in practice our stochastic computational methods, we investigate within channel geometries having internal obstacles and no-slip walls how the mobility/diffusivity of particles depends on location. Our methods extend the applicability of fluctuating hydrodynamic approaches by allowing for spatially adaptive resolution of the mechanics and for domains that have complex geometries relevant in many applications. (C) 2014 Elsevier Inc. All rights reserved. C1 [Plunkett, Pat; Atzberger, Paul J.] Univ Calif Santa Barbara, Dept Math, Santa Barbara, CA 93106 USA. [Hu, Jonathan; Siefert, Christopher] Sandia Natl Labs, Livermore, CA 94550 USA. RP Atzberger, PJ (reprint author), Univ Calif Santa Barbara, Dept Math, Santa Barbara, CA 93106 USA. EM atzberg@math.ucsb.edu FU DOE ASCR [CM4]; NSF [DMS-0956210]; W. M. Keck Foundation FX The authors would like to acknowledge support from DOE ASCR CM4. The author P. J. A. acknowledges support from research grant NSF CAREER DMS-0956210 and W. M. Keck Foundation. The Trilinos packages ML and Epetra were used for the application simulations. The authors thank Alexander Roma, Boyce Griffith, Mike Parks, and Micheal Minion for helpful suggestions. NR 51 TC 6 Z9 6 U1 1 U2 24 PU ACADEMIC PRESS INC ELSEVIER SCIENCE PI SAN DIEGO PA 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA SN 0021-9991 EI 1090-2716 J9 J COMPUT PHYS JI J. Comput. Phys. PD NOV 15 PY 2014 VL 277 BP 121 EP 137 DI 10.1016/j.jcp.2014.07.051 PG 17 WC Computer Science, Interdisciplinary Applications; Physics, Mathematical SC Computer Science; Physics GA AO4LV UT WOS:000341311000007 ER PT J AU Long, AR Gentile, NA Palmer, TS AF Long, A. R. Gentile, N. A. Palmer, T. S. TI The iterative thermal emission method: A more implicit modification of IMC SO JOURNAL OF COMPUTATIONAL PHYSICS LA English DT Article DE Thermal radiative transfer; Implicit Monte Carlo ID MONTE-CARLO METHOD; RADIATIVE-TRANSFER; TIME AB For over 40 years, the Implicit Monte Carlo (IMC) method has been used to solve challenging problems in thermal radiative transfer. These problems typically contain regions that are optically thick and diffusive, as a consequence of the high degree of "pseudo-scattering" introduced to model the absorption and reemission of photons from a tightly-coupled, radiating material. IMC has several well-known features that could be improved: a) it can be prohibitively computationally expensive, b) it introduces statistical noise into the material and radiation temperatures, which may be problematic in multiphysics simulations, and c) under certain conditions, solutions can be nonphysical, in that they violate a maximum principle, where IMC-calculated temperatures can be greater than the maximum temperature used to drive the problem. We have developed a variant of IMC called iterative thermal emission IMC, which is designed to have a reduced parameter space in which the maximum principle is violated. ITE IMC is a more implicit version of IMC in that it uses the information obtained from a series of IMC photon histories to improve the estimate for the end of time step material temperature during a time step. A better estimate of the end of time step material temperature allows for a more implicit estimate of other temperature-dependent quantities: opacity, heat capacity, Fleck factor (probability that a photon absorbed during a time step is not reemitted) and the Planckian emission source. We have verified the ITE IMC method against 0-D and 1-D analytic solutions and problems from the literature. These results are compared with traditional IMC. We perform an infinite medium stability analysis of ITE IMC and show that it is slightly more numerically stable than traditional IMC. We find that significantly larger time steps can be used with ITE IMC without violating the maximum principle, especially in problems with non-linear material properties. The ITE IMC method does however yield solutions with larger variance because each sub-step uses a different Fleck factor (even at equilibrium). (C) 2014 Elsevier Inc. All rights reserved. C1 [Long, A. R.] Texas A&M Univ, Dept Nucl Engn, College Stn, TX 77843 USA. [Gentile, N. A.] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA. [Palmer, T. S.] Oregon State Univ, Corvallis, OR 97333 USA. RP Long, AR (reprint author), Texas A&M Univ, Dept Nucl Engn, 3133 TAMU, College Stn, TX 77843 USA. EM arlong.ne@tamu.edu NR 22 TC 2 Z9 2 U1 1 U2 9 PU ACADEMIC PRESS INC ELSEVIER SCIENCE PI SAN DIEGO PA 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA SN 0021-9991 EI 1090-2716 J9 J COMPUT PHYS JI J. Comput. Phys. PD NOV 15 PY 2014 VL 277 BP 228 EP 247 DI 10.1016/j.jcp.2014.08.017 PG 20 WC Computer Science, Interdisciplinary Applications; Physics, Mathematical SC Computer Science; Physics GA AO4LV UT WOS:000341311000011 ER PT J AU Gupta, S Suresh, KG Nigam, AK Mudryk, Y Paudyal, D Pecharsky, VK Gschneidner, KA AF Gupta, Sachin Suresh, K. G. Nigam, A. K. Mudryk, Y. Paudyal, D. Pecharsky, V. K. Gschneidner, K. A., Jr. TI The nature of the first order isostructural transition in GdRhSn SO JOURNAL OF ALLOYS AND COMPOUNDS LA English DT Article DE Rare earth intermetallic; Iso-structural transition; Magnetocaloric effect ID SN-119 MOSSBAUER-SPECTROSCOPY; MAGNETIC PHASE-TRANSITIONS; GDPDAL SINGLE-CRYSTALS; STANNIDES RERHSN RE; ELECTRONIC-STRUCTURE; TBRHSN; DYRHSN; ANOMALIES; TRANSPORT; HORHSN AB We present structural, magnetic, thermal, magnetocaloric, and electrical transport properties of polycrystalline GdRhSn. Magnetization data show that it orders antiferromagnetically at T-N = 16.2 K. The compound has the ZrNiAl type hexagonal crystal structure at room temperature and undergoes a first order iso-structural transition in the paramagnetic state at 245 K. The unit cell volume change at the transition is small (-0.07%) but discontinuous, in agreement with the first-order nature of the transition observed by magnetic, transport, and heat capacity measurements. The anisotropic changes of the lattice parameters are Delta alpha/alpha = 0.28% and Delta c/c = 0.64% on cooling. A substantial change in the 4f and conduction electron hybridization, giving rise to an increased integrated DOS, occurs when the high temperature phase transforms to the low temperature phase. A moderate magnetocaloric effect at T-N (Delta S-M = 6.5 J/kg K and Delta T-ad = 4.5 K for Delta H = 50 kOe) has been measured using both magnetization and heat capacity data. (C) 2014 Elsevier B.V. All rights reserved. C1 [Gupta, Sachin; Suresh, K. G.] Indian Inst Technol, Dept Phys, Bombay 400076, Maharashtra, India. [Nigam, A. K.] Tata Inst Fundamental Res, Bombay 400005, Maharashtra, India. [Mudryk, Y.; Paudyal, D.; Pecharsky, V. K.; Gschneidner, K. A., Jr.] Iowa State Univ, Ames Lab, Ames, IA 50011 USA. [Pecharsky, V. K.; Gschneidner, K. A., Jr.] Iowa State Univ, Dept Mat Sci & Engn, Ames, IA 50011 USA. RP Suresh, KG (reprint author), Indian Inst Technol, Dept Phys, Bombay 400076, Maharashtra, India. EM suresh@phy.iitb.ac.in RI Gupta, Sachin/G-4793-2013 OI Gupta, Sachin/0000-0002-2407-5555 FU CSIR, New Delhi; Iowa State University of Science and Technology for the US Department of Energy [DE-AC02-07CH11358]; Office of Basic Energy Sciences, Materials Sciences Division of the Office of Science, US Department of Energy FX SG would like to thank CSIR, New Delhi for granting senior research fellowship. The Ames Laboratory is operated by Iowa State University of Science and Technology for the US Department of Energy under contract No. DE-AC02-07CH11358. Work at Ames Laboratory (theoretical calculations and temperature dependent Xray powder diffraction measurements) is supported by the Office of Basic Energy Sciences, Materials Sciences Division of the Office of Science, US Department of Energy. NR 46 TC 4 Z9 4 U1 3 U2 44 PU ELSEVIER SCIENCE SA PI LAUSANNE PA PO BOX 564, 1001 LAUSANNE, SWITZERLAND SN 0925-8388 EI 1873-4669 J9 J ALLOY COMPD JI J. Alloy. Compd. PD NOV 15 PY 2014 VL 613 BP 280 EP 287 DI 10.1016/j.jallcom.2014.06.027 PG 8 WC Chemistry, Physical; Materials Science, Multidisciplinary; Metallurgy & Metallurgical Engineering SC Chemistry; Materials Science; Metallurgy & Metallurgical Engineering GA AM7BA UT WOS:000340018500048 ER PT J AU Hanifi, AR Paulson, S Torabi, A Shinbine, A Tucker, MC Birss, V Etsell, TH Sarkar, P AF Hanifi, Amir Reza Paulson, Scott Torabi, Alireza Shinbine, Alyssa Tucker, Michael C. Birss, Viola Etsell, Thomas H. Sarkar, Partha TI Slip-cast and hot-solution infiltrated porous yttria stabilized zirconia (YSZ) supported tubular fuel cells. SO JOURNAL OF POWER SOURCES LA English DT Article DE Hot solution infiltration; NiO-SDC; LSM; GDC-LSCF; Porous YSZ; Tubular SOFC ID NANO-STRUCTURED ELECTRODES; SOFC ANODES; HIGH-PERFORMANCE; DOPED CERIA; THERMAL-STABILITY; CERMET ANODES; IMPREGNATION; CATHODES; REDOX; MICROSTRUCTURE AB Hot solution infiltration was investigated as a flexible and rapid method to incorporate anode and cathode components into fully sintered, porous ceramic tubular templates for use as solid oxide fuel cells (SOFC). Composed of either a porous 8 mol% yttria-stabilized zirconia (YSZ) or 5 wt% NiO-YSZ support structure, a thin Ni-YSZ anode functional layer and an outer ca. 10 gm dense YSZ electrolyte, closed end tubes were first hot solution (ca. 100 degrees C) infiltrated on the inside with NiO-SDC (Sm0.2Ce0.8O1.9) to serve as the anode. Cathodes were either LSM (nominally La0.8Sr0.2MnO3+delta) infiltrated into a thin porous YSZ layer on the outer electrolyte surface, or an LSCF-GDC composite (Gd0.1Ce0.9O1.95-La0.6Sr0.4Co0.2Fe0.8O3-delta) on a thin GDC buffer layer. Although hot solution infiltration of the Ni, Ce and Sm salts into the anode support structure did not result in complete penetration (with the Ni contents in the tube wall ranging between 4 and 10 vol.%), well-sealed full cells produced power densities as high as 275, 196 and 153 mW cm(-2) at 800, 750 and 700 degrees C, respectively. Hot solution infiltration of active SOFC electrode materials is thus shown to be a very flexible approach for the evaluation of their performance. (C) 2014 Elsevier B.V. All rights reserved. C1 [Hanifi, Amir Reza; Torabi, Alireza; Shinbine, Alyssa; Etsell, Thomas H.] Univ Alberta, Dept Chem & Mat Engn, Edmonton, AB T6G 2V4, Canada. [Paulson, Scott; Birss, Viola] Univ Calgary, Dept Chem, Calgary, AB T2N 1N4, Canada. [Tucker, Michael C.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Environm Energy Technol Div, Berkeley, CA 94720 USA. [Sarkar, Partha] Alberta Innovates Technol Futures, Carbon & Energy Management, Edmonton, AB T6N 1E4, Canada. RP Hanifi, AR (reprint author), Univ Alberta, Dept Chem & Mat Engn, Edmonton, AB T6G 2V4, Canada. EM Hanifi@ualberta.ca FU Natural Sciences and Engineering Research Council (NSERC) FX This research was supported through funding to the NSERC Solid Oxide Fuel Cell Canada Strategic Research Network from the Natural Sciences and Engineering Research Council (NSERC) and other sponsors listed at www.sofccanada.com. We would also like to acknowledge Dr. Rob Marr at the University of Calgary Laboratory for Electron Microbeam Analysis (UCLEMA) for assistance with the electron microprobe analyses. NR 46 TC 6 Z9 6 U1 7 U2 88 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0378-7753 EI 1873-2755 J9 J POWER SOURCES JI J. Power Sources PD NOV 15 PY 2014 VL 266 BP 121 EP 131 DI 10.1016/j.jpowsour.2014.05.001 PG 11 WC Chemistry, Physical; Electrochemistry; Energy & Fuels; Materials Science, Multidisciplinary SC Chemistry; Electrochemistry; Energy & Fuels; Materials Science GA AL0GV UT WOS:000338806300015 ER PT J AU Kan, YC Hu, Y Croy, J Ren, Y Sun, CJ Heald, SM Bareno, J Bloom, I Chen, ZH AF Kan, Yongchun Hu, Yuan Croy, Jason Ren, Yang Sun, Cheng-Jun Heald, Steve M. Bareno, Javier Bloom, Ira Chen, Zonghai TI Formation of Li2MnO3 investigated by in situ synchrotron probes SO JOURNAL OF POWER SOURCES LA English DT Article DE In situ probes; XRD; XANES; Factor analysis; Lithium battery ID FE-SUBSTITUTED LI2MNO3; LITHIUM-ION BATTERIES; X-RAY-DIFFRACTION; LAYERED-OXIDE; ELECTROCHEMICAL ACTIVITY; POSITIVE ELECTRODE; PHASE-TRANSITIONS; CATHODE MATERIALS; LOCAL-STRUCTURE; CAPACITY AB Both in situ high-energy X-ray diffraction and in situ X-ray absorption spectroscopy were used to investigate the structural evolution of materials during the solid-state synthesis of Li2MnO3. Combing Xray absorption spectroscopy and factor analysis techniques, we were able to capture the spectrum and evolution of an intermediate phase (MnO2) that could not be detected by the diffraction technique. Meanwhile, the X-ray diffraction data clearly showed the anisotropic crystallization of Li2MnO3 during sintering above 600 degrees C. (C) 2014 Elsevier B.V. All rights reserved. C1 [Kan, Yongchun; Hu, Yuan] Univ Sci & Technol China, State Key Lab Fire Sci, Hefei 230026, Anhui, Peoples R China. [Kan, Yongchun; Croy, Jason; Bareno, Javier; Bloom, Ira; Chen, Zonghai] Argonne Natl Lab, Chem Sci & Engn Div, Argonne, IL 60439 USA. [Ren, Yang; Sun, Cheng-Jun; Heald, Steve M.] Argonne Natl Lab, Xray Sci Div, Argonne, IL 60439 USA. RP Chen, ZH (reprint author), Argonne Natl Lab, Chem Sci & Engn Div, Argonne, IL 60439 USA. EM zonghai.chen@anl.gov RI Chen, Zonghai/F-1067-2015; OI Chen, Zonghai/0000-0001-5371-9463; Bareno, Javier/0000-0003-1230-9278 FU U.S. Department of Energy, Vehicle Technologies Office; U.S. Department of Energy by UChicago Argonne, LLC [DE-AC02-06CH11357]; U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences; US Department of Energy - Basic Energy Sciences, a Major Resources Support grant from NSERC; University of Washington; Canadian Light Source; Advanced Photon Source FX Research at Argonne National Laboratory was funded by U.S. Department of Energy, Vehicle Technologies Office. Argonne National Laboratory is operated for the U.S. Department of Energy by UChicago Argonne, LLC, under contract DE-AC02-06CH11357. The authors also acknowledge the use of the Advanced Photon Source of Argonne National Laboratory supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences. PNC/XSD facilities at the Advanced Photon Source, and research at these facilities, are supported by the US Department of Energy - Basic Energy Sciences, a Major Resources Support grant from NSERC, the University of Washington, the Canadian Light Source, and the Advanced Photon Source. NR 42 TC 8 Z9 8 U1 6 U2 150 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0378-7753 EI 1873-2755 J9 J POWER SOURCES JI J. Power Sources PD NOV 15 PY 2014 VL 266 BP 341 EP 346 DI 10.1016/j.jpowsour.2014.05.032 PG 6 WC Chemistry, Physical; Electrochemistry; Energy & Fuels; Materials Science, Multidisciplinary SC Chemistry; Electrochemistry; Energy & Fuels; Materials Science GA AL0GV UT WOS:000338806300045 ER PT J AU Czakon, M Mitov, A Papucci, M Ruderman, JT Weiler, A AF Czakon, Michal Mitov, Alexander Papucci, Michele Ruderman, Joshua T. Weiler, Andreas TI Removing Gaps in the Exclusion of Top Squark Parameter Space SO PHYSICAL REVIEW LETTERS LA English DT Article ID HADRON COLLIDERS; PAIR PRODUCTION; PP COLLISIONS; FERMILAB TEVATRON; QUARK PRODUCTION; QCD CORRECTIONS; CROSS-SECTION; ROOT-S=8 TEV; SEARCH; LHC AB Light stops are a hallmark of the most natural realizations of weak-scale supersymmetry. While stops have been extensively searched for, there remain open gaps around and below the top mass, due to similarities of stop and top signals with current statistics. We propose a new fast-track avenue to improve light stop searches for R-parity-conserving supersymmetry by comparing top cross section measurements to the theoretical prediction. Stop masses below similar to 180 GeV can now be ruled out for a light neutralino. The possibility of a stop signal contaminating the top mass measurement is also briefly addressed. C1 [Czakon, Michal] Rhein Westfal TH Aachen, Inst Theoret Teilchenphys & Kosmol, D-52056 Aachen, Germany. [Mitov, Alexander] Univ Cambridge, Cavendish Lab, Cambridge CB3 0HE, England. [Papucci, Michele; Ruderman, Joshua T.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Theoret Phys Grp, Berkeley, CA 94720 USA. [Papucci, Michele; Ruderman, Joshua T.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA. [Ruderman, Joshua T.] NYU, Dept Phys, Ctr Cosmol & Particle Phys, New York, NY 10003 USA. [Weiler, Andreas] DESY, D-22607 Hamburg, Germany. [Weiler, Andreas] CERN, Div Theory, CH-1211 Geneva 23, Switzerland. RP Czakon, M (reprint author), Rhein Westfal TH Aachen, Inst Theoret Teilchenphys & Kosmol, D-52056 Aachen, Germany. FU German Research Foundation (DFG) via the Sonderforschungsbereich/Transregio [SFB/TR-9]; Heisenberg programme; UK Science and Technology Facilities Council [ST/L002760/1, ST/K004883/1]; ERC [291377]; Office of Science, Office of High Energy Physics, of the U.S. Department of Energy [DE-AC02-05CH11231]; Miller Institute for Basic Research in Science; German Science Foundation (DFG) under the Collaborative Research Center [(SFB) 676] FX We thank Stefan Berge, Kyle Cranmer, Lance Dixon, Ian Low, Michelangelo Mangano, and Matt Reece for discussions. M. P. and J. T. R. thank the CERN TH group and the Aspen Center for Physics for their hospitality. J. T. R. also thanks CFHEP at IHEP for hospitality. The work of M. C. was supported by the German Research Foundation (DFG) via the Sonderforschungsbereich/Transregio SFB/TR-9 "Computational Particle Physics" and the Heisenberg programme. The work of A. M. is supported by the UK Science and Technology Facilities Council (Grants No. ST/L002760/1 and No. ST/K004883/1) and in part by ERC Grant No. 291377 "LHCtheory: Theoretical predictions and analyses of LHC physics: advancing the precision frontier." M. P. was supported in part by the Director, Office of Science, Office of High Energy Physics, of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. J. T. R. is supported by a fellowship from the Miller Institute for Basic Research in Science. The work of A. W. was supported in part by the German Science Foundation (DFG) under the Collaborative Research Center (SFB) 676. NR 91 TC 31 Z9 31 U1 2 U2 8 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0031-9007 EI 1079-7114 J9 PHYS REV LETT JI Phys. Rev. Lett. PD NOV 14 PY 2014 VL 113 IS 20 AR 201803 DI 10.1103/PhysRevLett.113.201803 PG 6 WC Physics, Multidisciplinary SC Physics GA CB5JT UT WOS:000349664000004 PM 25432037 ER PT J AU Fatemi, V Hunt, B Steinberg, H Eltinge, SL Mahmood, F Butch, NP Watanabe, K Taniguchi, T Gedik, N Ashoori, RC Jarillo-Herrero, P AF Fatemi, Valla Hunt, Benjamin Steinberg, Hadar Eltinge, Stephen L. Mahmood, Fahad Butch, Nicholas P. Watanabe, Kenji Taniguchi, Takashi Gedik, Nuh Ashoori, Raymond C. Jarillo-Herrero, Pablo TI Electrostatic Coupling between Two Surfaces of a Topological Insulator Nanodevice SO PHYSICAL REVIEW LETTERS LA English DT Article ID BORON-NITRIDE; GRAPHENE; BI2SE3; STATE; TRANSPORT; BI2TE3 AB We report on electronic transport measurements of dual-gated nanodevices of the low-carrier density topological insulator (TI) Bi1.5Sb0.5Te1.7Se1.3. In all devices, the upper and lower surface states are independently tunable to the Dirac point by the top and bottom gate electrodes. In thin devices, electric fields are found to penetrate through the bulk, indicating finite capacitive coupling between the surface states. A charging model allows us to use the penetrating electric field as a measurement of the intersurface capacitance CTI and the surface state energy-density relationship mu(n), which is found to be consistent with independent angle-resolved photoemission spectroscopy measurements. At high magnetic fields, increased field penetration through the surface states is observed, strongly suggestive of the opening of a surface state band gap due to broken time-reversal symmetry. C1 [Fatemi, Valla; Hunt, Benjamin; Steinberg, Hadar; Eltinge, Stephen L.; Mahmood, Fahad; Gedik, Nuh; Ashoori, Raymond C.; Jarillo-Herrero, Pablo] MIT, Dept Phys, Cambridge, MA 02139 USA. [Steinberg, Hadar] Hebrew Univ Jerusalem, Racah Inst Phys, IL-91904 Jerusalem, Israel. [Butch, Nicholas P.] NIST, Ctr Neutron Res, Gaithersburg, MD 20899 USA. [Butch, Nicholas P.] Univ Maryland, Dept Phys, Ctr Nanophys & Adv Mat, College Pk, MD 20742 USA. [Butch, Nicholas P.] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA. [Watanabe, Kenji; Taniguchi, Takashi] Natl Inst Mat Sci, Adv Mat Lab, Tsukuba, Ibaraki 3050044, Japan. RP Fatemi, V (reprint author), MIT, Dept Phys, Cambridge, MA 02139 USA. EM vfatemi@mit.edu RI TANIGUCHI, Takashi/H-2718-2011; WATANABE, Kenji/H-2825-2011; Hunt, Benjamin/C-3395-2017 OI WATANABE, Kenji/0000-0003-3701-8119; Hunt, Benjamin/0000-0002-5008-8042 FU DOE, Basic Energy Sciences Office, Division of Materials Sciences and Engineering [DE-SC0006418]; Gordon and Betty Moore Foundation [GBMF2931]; STC Center for Integrated Quantum Materials, NSF [DMR-1231319]; MIT MRSEC Initiative under NSF [DMR-0819762]; NSF [DMR-0819762, ECS-0335765]; U.S. Department of Energy, National Nuclear Security Administration [DE-AC52-07NA27344] FX This work was partly supported by the DOE, Basic Energy Sciences Office, Division of Materials Sciences and Engineering, under Award No. DE-SC0006418 (V. F., S. E., H. S., and P. J. H.), by the Gordon and Betty Moore Foundation Grant No. GBMF2931 and the STC Center for Integrated Quantum Materials, NSF Grant No. DMR-1231319 (B. H. and R. C. A.), and by an MIT MRSEC Initiative under NSF Grant No. DMR-0819762 (F. M. and N. G.). This work made use of the Materials Research Science and Engineering Center Shared Experimental Facilities supported by NSF under Grant No. DMR-0819762. Sample fabrication was performed partly at the Harvard Center for Nanoscale Science supported by the NSF under Grant No. ECS-0335765. Sample synthesis and initial characterization were performed under LDRD (Tracking Code 14-ERD-041) at Lawrence Livermore National Laboratory (LLNL). LLNL is operated by Lawrence Livermore National Security, LLC, for the U.S. Department of Energy, National Nuclear Security Administration, under Contract No. DE-AC52-07NA27344. We thank A. Stern, Y. Baum, K. Burch, D. Drew, B. Skinner, A. Frenzel, and J. D. Sanchez-Yamagishi for discussions and J. R. Jeffries for performing x-ray diffraction measurements. NR 41 TC 11 Z9 11 U1 5 U2 57 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0031-9007 EI 1079-7114 J9 PHYS REV LETT JI Phys. Rev. Lett. PD NOV 14 PY 2014 VL 113 IS 20 AR 206801 DI 10.1103/PhysRevLett.113.206801 PG 5 WC Physics, Multidisciplinary SC Physics GA CB5JT UT WOS:000349664000013 PM 25432050 ER PT J AU Michel, P Divol, L Turnbull, D Moody, JD AF Michel, P. Divol, L. Turnbull, D. Moody, J. D. TI Dynamic Control of the Polarization of Intense Laser Beams via Optical Wave Mixing in Plasmas SO PHYSICAL REVIEW LETTERS LA English DT Article ID INERTIAL CONFINEMENT FUSION; ULTRAHIGH-POWER LASERS; SUPPRESSION; PROBE; PUMP AB When intense laser beams overlap in plasmas, the refractive index modulation created by the beat wave via the ponderomotive force can lead to optical wave mixing phenomena similar to those used in crystals and photorefractive materials. A new comprehensive analytical description of the modification of the polarization state of laser beams crossing at arbitrary angles in a plasma is presented. It is shown that a laser-plasma system can be used to provide full control of the polarization state of a separate "probe" laser beam; simple analytical estimates and practical considerations are provided for the design of novel photonics devices such as laser-plasma polarizers and wave plates. C1 [Michel, P.; Divol, L.; Turnbull, D.; Moody, J. D.] Lawrence Livermore Natl Lab, Livermore, CA 94551 USA. RP Michel, P (reprint author), Lawrence Livermore Natl Lab, Livermore, CA 94551 USA. FU U.S. Department of Energy by Lawrence Livermore National Laboratory [DE-AC52-07NA27344] FX This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract No. DE-AC52-07NA27344. NR 28 TC 13 Z9 13 U1 3 U2 16 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0031-9007 EI 1079-7114 J9 PHYS REV LETT JI Phys. Rev. Lett. PD NOV 14 PY 2014 VL 113 IS 20 AR 205001 DI 10.1103/PhysRevLett.113.205001 PG 5 WC Physics, Multidisciplinary SC Physics GA CB5JT UT WOS:000349664000010 PM 25432044 ER PT J AU Appel, HM Fescemyer, H Ehlting, J Weston, D Rehrig, E Joshi, T Xu, D Bohlmann, J Schultz, J AF Appel, Heidi M. Fescemyer, Howard Ehlting, Juergen Weston, David Rehrig, Erin Joshi, Trupti Xu, Dong Bohlmann, Joerg Schultz, Jack TI Transcriptional responses of Arabidopsis thaliana to chewing and sucking insect herbivores SO FRONTIERS IN PLANT SCIENCE LA English DT Article DE Arabidopsis thaliana; Spodoptera exigua; Pieris brassicae; Myzus persicae; Brevicoryne brassicae; herbivory; hormone signaling; glucosinolates ID GENE-EXPRESSION; PLANT DEFENSE; NICOTIANA-ATTENUATA; SIGNALING PATHWAYS; GLUCOSINOLATE ACCUMULATION; COMBINATORIAL CONTROL; REGULATED GENE; JASMONIC ACID; TRANSFER-RNA; CROSS-TALK AB We tested the hypothesis that Arabidopsis can recognize and respond differentially to insect species at the transcriptional level using a genome wide microarray. Transcriptional reprogramming was characterized using co-expression analysis in damaged and undamaged leaves at two times in response to mechanical wounding and four insect species. In all, 2778 (10.6%) of annotated genes on the array were differentially expressed in at least one treatment. Responses differed mainly between aphid and caterpillar and sampling times. Responses to aphids and caterpillars shared only 10% of up-regulated and 8% of down-regulated genes. Responses to two caterpillars shared 21 and 12% of up- and down-regulated genes, whereas responses to the two aphids shared only 7 and 4% of up-regulated and down-regulated genes. Overlap in genes expressed between 6 and 24h was 3-15%, and depended on the insect species. Responses in attacked and unattacked leaves differed at 6 h but converged by 24 h. Genes responding to the insects are also responsive to many stressors and included primary metabolism. Aphids down-regulated amino acid catabolism; caterpillars stimulated production of amino acids involved in glucosinolate synthesis. Co-expression analysis revealed 17 response networks. Transcription factors were a major portion of differentially expressed genes throughout and responsive genes shared most of the known or postulated binding sites. However, cis-element composition of genes down regulated by the aphid M. persicae was unique, as were those of genes down-regulated by caterpillars. As many as 20 cis-elements were over-represented in one or more treatments, including some from well-characterized classes and others as yet uncharacterized. We suggest that transcriptional changes elicited by wounding and insects are heavily influenced by transcription factors and involve both enrichment of a common set of cis-elements and a unique enrichment of a few cis-elements in responding genes. C1 [Appel, Heidi M.; Schultz, Jack] Univ Missouri, Bond Life Sci Ctr, Columbia, MO 65211 USA. [Appel, Heidi M.; Schultz, Jack] Univ Missouri, Div Plant Sci, Columbia, MO 65211 USA. [Fescemyer, Howard] Penn State Univ, Dept Biol, University Pk, PA 16802 USA. [Ehlting, Juergen; Bohlmann, Joerg] Univ Missouri, Bond Life Sci Ctr, Columbia, MO 65211 USA. [Ehlting, Juergen] Univ Victoria, Dept Biol, Victoria, BC V8W 2Y2, Canada. [Weston, David] Oak Ridge Natl Lab, Biosci Div, Oak Ridge, TN USA. [Rehrig, Erin] Fitchburg State Univ, Dept Biol & Chem, Fitchburg, MA USA. [Joshi, Trupti; Xu, Dong] Univ Missouri, Bond Life Sci Ctr, Inst Informat, Dept Comp Sci, Columbia, MO 65211 USA. RP Appel, HM (reprint author), Univ Missouri, Bond Life Sci Ctr, 1201 Rollins St, Columbia, MO 65211 USA. EM appelh@missouri.edu FU NSF Arabidopsis grant [DEB 0313492] FX We thank two anonymous reviewers for a critical reading of the manuscript, Chris Frost and Clayton Coffman for help with data analysis, and the following individuals for help in conducting experiments: Inga Mewis, Jennifer Heath, JoAnn Snyder, Irmgard Seidl Adams, Nate McCartney, and Roger Snyder. Funding was provided by an NSF Arabidopsis 2010 grant (DEB 0313492) to Jack Schultz. NR 103 TC 10 Z9 10 U1 6 U2 64 PU FRONTIERS RESEARCH FOUNDATION PI LAUSANNE PA PO BOX 110, LAUSANNE, 1015, SWITZERLAND SN 1664-462X J9 FRONT PLANT SCI JI Front. Plant Sci. PD NOV 14 PY 2014 VL 5 AR 565 DI 10.3389/fpls.2014.00565 PG 20 WC Plant Sciences SC Plant Sciences GA AX6ZC UT WOS:000347065500001 PM 25452759 ER PT J AU Kogan, VG Prozorov, R AF Kogan, V. G. Prozorov, R. TI Changing the type of superconductivity by magnetic and potential scattering SO PHYSICAL REVIEW B LA English DT Article ID PARAMAGNETIC IMPURITIES; ALLOYS AB By evaluating the upper and thermodynamic critical fields H-c2 and H-c and their ratio H-c2/H-c at arbitrary temperatures, we argue that situations are possible when a type-II material is transformed into type I by adding magnetic impurities. C1 [Kogan, V. G.] Iowa State Univ, Ames Lab DOE, Ames, IA 50011 USA. Iowa State Univ, Dept Phys, Ames, IA 50011 USA. RP Kogan, VG (reprint author), Iowa State Univ, Ames Lab DOE, Ames, IA 50011 USA. EM kogan@ameslab.gov; prozorov@ameslab.gov FU Department of Energy, Office of Basic Energy Sciences, Division of Materials Sciences and Engineering [DE-AC02-07CH11358] FX The authors are grateful to D. Finnemore, J. Kirtley, J. Thompson, P. Canfield, S. Bud'ko, V. Taufor, and B. Maple for many helpful discussions. The Ames Laboratory is supported by the Department of Energy, Office of Basic Energy Sciences, Division of Materials Sciences and Engineering under Contract No. DE-AC02-07CH11358. NR 8 TC 2 Z9 2 U1 0 U2 4 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1098-0121 EI 1550-235X J9 PHYS REV B JI Phys. Rev. B PD NOV 14 PY 2014 VL 90 IS 18 AR 180502 DI 10.1103/PhysRevB.90.180502 PG 4 WC Physics, Condensed Matter SC Physics GA AU2BY UT WOS:000345422200004 ER PT J AU Gunawardana, KGSH Wilson, SR Mendelev, MI Song, XY AF Gunawardana, K. G. S. H. Wilson, S. R. Mendelev, M. I. Song, Xueyu TI Theoretical calculation of the melting curve of Cu-Zr binary alloys SO PHYSICAL REVIEW E LA English DT Article ID HARD-SPHERE FLUID; FUNDAMENTAL MEASURE-THEORY; FREE-ENERGY MODEL; PERTURBATION-THEORY; METALLIC GLASSES; REPULSIVE FORCES; LIQUID; SIMULATION; STABILITY; SYSTEM AB Helmholtz free energies of the dominant binary crystalline solids found in the Cu-Zr system at high temperatures close to the melting curve are calculated. Our theoretical approach combines fundamental measure density functional theory (applied to the hard-sphere reference system) and a perturbative approach to include the attractive interactions. The studied crystalline solids are Cu(fcc), Cu51Zr14(beta), CuZr(B2), CuZr2(C11b), Zr(hcp), and Zr(bcc). The calculated Helmholtz free energies of crystalline solids are in good agreement with results from molecular-dynamics (MD) simulations. Using the same perturbation approach, the liquid phase free energies are calculated as a function of composition and temperature, from which the melting curve of the entire composition range of this system can be obtained. Phase diagrams are determined in this way for two leading embedded atom method potentials, and the results are compared with experimental data. Theoretical melting temperatures are compared both with experimental values and with values obtained directly from MD simulations at several compositions. C1 [Gunawardana, K. G. S. H.; Wilson, S. R.; Mendelev, M. I.; Song, Xueyu] Iowa State Univ, Ames Lab, Ames, IA 50011 USA. [Song, Xueyu] Iowa State Univ, Dept Chem, Ames, IA 50011 USA. RP Gunawardana, KGSH (reprint author), Iowa State Univ, Ames Lab, Ames, IA 50011 USA. EM xsong@iastate.edu FU Division of Materials Sciences and Engineering, Office of Basic Energy Sciences, U.S. Department of Energy [W-7405-ENG-82]; Iowa State University FX This research was sponsored by the Division of Materials Sciences and Engineering, Office of Basic Energy Sciences, U.S. Department of Energy, under Contract No. W-7405-ENG-82 with Iowa State University. We would like to thank Shihuai Zhou for providing much of the structural information used in this study. NR 41 TC 1 Z9 2 U1 3 U2 31 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 2470-0045 EI 2470-0053 J9 PHYS REV E JI Phys. Rev. E PD NOV 14 PY 2014 VL 90 IS 5 AR 052403 DI 10.1103/PhysRevE.90.052403 PG 8 WC Physics, Fluids & Plasmas; Physics, Mathematical SC Physics GA AU4QB UT WOS:000345595600010 ER PT J AU Bolme, CA Ramos, KJ AF Bolme, C. A. Ramos, K. J. TI The elastic tensor of single crystal RDX determined by Brillouin spectroscopy SO JOURNAL OF APPLIED PHYSICS LA English DT Article ID CYCLOTRIMETHYLENE TRINITRAMINE RDX; CONSTANTS AB The elastic tensor of 1,3,5-trinitroperhydro-1,3,5-triazine (also known as RDX, hexogen, and cyclotrimethylene trinitramine) was determined using Brillouin spectroscopy of as-grown single crystals. This study addresses inconsistencies in the literature between the elastic tensor measurements made using Brillouin spectroscopy in the GHz frequency range and the measurements using various techniques in the kHz-MHz frequency range. These Brillouin results are consistent with previous measurements made in the kHz-MHz frequency range using various techniques and are also consistent with velocity measurements at 15 GHz using picosecond acoustic interferometry. These results are in disagreement with the previously published elastic tensor determined using Brillouin spectroscopy, and there are differences of several percent amongst the consistent set of elastic tensor determinations. The origins of the disagreement and differences are discussed. (C) 2014 AIP Publishing LLC. C1 [Bolme, C. A.; Ramos, K. J.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA. RP Bolme, CA (reprint author), Los Alamos Natl Lab, POB 1663, Los Alamos, NM 87545 USA. OI Bolme, Cynthia/0000-0002-1880-271X FU National Nuclear Security Administration Science Campaign 2; LANL HE Crystal Laboratory FX This work was supported by the National Nuclear Security Administration Science Campaign 2 and performed at Los Alamos National Laboratory under DE-AC52-06NA25396. The authors gratefully acknowledge helpful discussions with Dr. Lewis Stevens, Dr. Dan Hooks, Dr. D. J. Luscher, and Dr. Marc Cawkwell, machining performed by Timothy Pierce, and support in the LANL HE Crystal Laboratory from Tate Hamilton. NR 26 TC 7 Z9 7 U1 1 U2 14 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0021-8979 EI 1089-7550 J9 J APPL PHYS JI J. Appl. Phys. PD NOV 14 PY 2014 VL 116 IS 18 AR 183503 DI 10.1063/1.4901461 PG 7 WC Physics, Applied SC Physics GA AT8ZB UT WOS:000345216300012 ER PT J AU Huang, ZY Fu, H Hadimani, RL Balfour, EA Dembele, SN Teng, BH Jiles, DC AF Huang, Z. Y. Fu, H. Hadimani, R. L. Balfour, E. Agurgo Dembele, S. N. Teng, B. H. Jiles, D. C. TI Enhancement of magnetocaloric effect in the Gd2Al phase by Co alloying SO JOURNAL OF APPLIED PHYSICS LA English DT Article ID MAGNETIC REFRIGERATION; TEMPERATURE; COMPOUND AB To understand the effect of Co doping on the magnetic entropy changes in Gd2Al phase, a series of Gd2AlCox alloys with 0 <= x <= 0.6 were synthesized by arc-melting and the crystal structure was analyzed by XRD. The magnetic properties were investigated, and the entropy changes were calculated for a magnetic field change of 50 kOe. All the as-cast alloys doped with Co exhibited greater magnetic entropy changes than the original binary Gd2Al phase. The main reasons attributed to this are the increase of ferromagnetic interaction indicated by the disappearance of cusp and sharp drop in magnetization and the reduction of the critical field required to trigger the field-induced transition below 50K in Gd2Al phase after Co alloying. (C) 2014 AIP Publishing LLC. C1 [Huang, Z. Y.; Fu, H.; Balfour, E. Agurgo; Dembele, S. N.; Teng, B. H.] Univ Elect Sci & Technol China, Sch Phys Elect, Chengdu 610054, Peoples R China. [Hadimani, R. L.; Jiles, D. C.] Iowa State Univ, Dept Elect & Comp Engn, Ames, IA 50011 USA. [Hadimani, R. L.; Jiles, D. C.] US DOE, Ames Lab, Ames, IA 50011 USA. RP Fu, H (reprint author), Univ Elect Sci & Technol China, Sch Phys Elect, Chengdu 610054, Peoples R China. EM fuhao@uestc.edu.cn OI Hadimani, Ravi/0000-0001-5939-556X FU National Natural Science Foundation of China [51271049]; Barbara and James Palmer endowment at the Department of Electrical and Computer Engineering of Iowa State University FX This work was supported by the National Natural Science Foundation of China (No. 51271049). This work was also funded by Barbara and James Palmer endowment at the Department of Electrical and Computer Engineering of Iowa State University. NR 18 TC 0 Z9 0 U1 2 U2 14 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0021-8979 EI 1089-7550 J9 J APPL PHYS JI J. Appl. Phys. PD NOV 14 PY 2014 VL 116 IS 18 AR 183908 DI 10.1063/1.4900782 PG 4 WC Physics, Applied SC Physics GA AT8ZB UT WOS:000345216300030 ER PT J AU Spirin, RE Salvadori, MC Teixeira, FS Sgubin, LG Cattani, M Brown, IG AF Spirin, R. E. Salvadori, M. C. Teixeira, F. S. Sgubin, L. G. Cattani, M. Brown, I. G. TI Nanocomposite formed by titanium ion implantation into alumina SO JOURNAL OF APPLIED PHYSICS LA English DT Article ID DYNAMIC COMPOSITION CHANGES; GOLD NANOPARTICLES; RESISTIVITY; SIMULATION; CERAMICS; POLYMER; TRIDYN AB Composites of titanium nanoparticles in alumina were formed by ion implantation of titanium into alumina, and the surface electrical conductivity measured in situ as the implantation proceeded, thus generating curves of sheet conductivity as a function of dose. The implanted titanium self-conglomerates into nanoparticles, and the spatial dimensions of the buried nanocomposite layer can thus be estimated from the implantation depth profile. Rutherford backscattering spectrometry was performed to measure the implantation depth profile, and was in good agreement with the calculated profile. Transmission electron microscopy of the titanium-implanted alumina was used for direct visualization of the nanoparticles formed. The measured conductivity of the buried layer is explained by percolation theory. We determine that the saturation dose, phi(0), the maximum implantation dose for which the nanocomposite material still remains a composite, is phi(0) = 2.2 x 10(16) cm(-2), and the corresponding saturation conductivity is sigma(0) = 480 S/m. The percolation dose phi(c), below which the nanocomposite still has basically the conductivity of the alumina matrix, was found to be phi(c) = 0.84 x 10(16) cm(-2). The experimental results are discussed and compared with a percolation theory model. (C) 2014 AIP Publishing LLC. C1 [Spirin, R. E.] Univ Sao Paulo, Polytech Sch, BR-05508970 Sao Paulo, Brazil. [Salvadori, M. C.; Teixeira, F. S.; Sgubin, L. G.; Cattani, M.] Univ Sao Paulo, Inst Phys, BR-05314970 Sao Paulo, Brazil. [Brown, I. G.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. RP Salvadori, MC (reprint author), Univ Sao Paulo, Inst Phys, CP 66318, BR-05314970 Sao Paulo, Brazil. EM mcsalvadori@if.usp.br RI Salvadori, Maria Cecilia/A-9379-2013 FU Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP); Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq), Brazil FX This work was supported by the Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP) and the Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq), Brazil. We are grateful to the Institute of Ion Beam Physics and Materials Research at the Forschungszentrum Dresden-Rossendorf, Germany, for the TRIDYN-FZR computer simulation code. NR 30 TC 0 Z9 0 U1 2 U2 14 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0021-8979 EI 1089-7550 J9 J APPL PHYS JI J. Appl. Phys. PD NOV 14 PY 2014 VL 116 IS 18 AR 184306 DI 10.1063/1.4901643 PG 6 WC Physics, Applied SC Physics GA AT8ZB UT WOS:000345216300041 ER PT J AU Yang, C Zarkadoula, E Dove, MT Todorov, IT Geisler, T Brazhkin, VV Trachenko, K AF Yang, C. Zarkadoula, E. Dove, M. T. Todorov, I. T. Geisler, T. Brazhkin, V. V. Trachenko, K. TI Solid-state diffusion in amorphous zirconolite SO JOURNAL OF APPLIED PHYSICS LA English DT Article ID RADIATION-DAMAGE; MOLECULAR-DYNAMICS; NUCLEAR-WASTE; PLUTONIUM; IMMOBILIZATION; CERAMICS; AMORPHIZATION; DISPOSITION AB We discuss how structural disorder and amorphization affect solid-state diffusion, and consider zirconolite as a currently important case study. By performing extensive molecular dynamics simulations, we disentangle the effects of amorphization and density, and show that a profound increase of solid-state diffusion takes place as a result of amorphization. Importantly, this can take place at the same density as in the crystal, representing an interesting general insight regarding solid-state diffusion. We find that decreasing the density in the amorphous system increases pre-factors of diffusion constants, but does not change the activation energy in the density range considered. We also find that atomic species in zirconolite are affected differently by amorphization and density change. Our microscopic insights are relevant for understanding how solid-state diffusion changes due to disorder and for building predictive models of operation of materials to be used to encapsulate nuclear waste. (C) 2014 AIP Publishing LLC. C1 [Yang, C.; Zarkadoula, E.; Dove, M. T.; Trachenko, K.] Queen Mary Univ London, Sch Phys & Astron, London E1 4NS, England. [Zarkadoula, E.] Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA. [Todorov, I. T.] STFC Daresbury Lab, Warrington WA4 1EP, Cheshire, England. [Geisler, T.] Univ Bonn, Steinmann Inst Geol Mineral & Palaontol, D-53115 Bonn, Germany. [Brazhkin, V. V.] RAS, Inst High Pressure Phys, Moscow 142190, Russia. RP Yang, C (reprint author), Queen Mary Univ London, Sch Phys & Astron, Mile End Rd, London E1 4NS, England. RI Yang, Chenxing/B-4609-2016; OI Zarkadoula, Eva/0000-0002-6886-9664 FU QMUL Research-IT; EPSRC [EP/K000128/1]; CSC FX This research utilised Queen Mary's MidPlus computational facilities, supported by QMUL Research-IT and funded by EPSRC grant EP/K000128/1. We are grateful to E. Maddrell for discussions and to CSC for support. NR 28 TC 1 Z9 1 U1 3 U2 28 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0021-8979 EI 1089-7550 J9 J APPL PHYS JI J. Appl. Phys. PD NOV 14 PY 2014 VL 116 IS 18 AR 184901 DI 10.1063/1.4901326 PG 6 WC Physics, Applied SC Physics GA AT8ZB UT WOS:000345216300054 ER PT J AU Neau, DB Bender, G Boeglin, WE Bartlett, SG Brash, AR Newcomer, ME AF Neau, David B. Bender, Gunes Boeglin, William E. Bartlett, Sue G. Brash, Alan R. Newcomer, Marcia E. TI Crystal Structure of a Lipoxygenase in Complex with Substrate THE ARACHIDONIC ACID-BINDING SITE OF 8R-LIPOXYGENASE SO JOURNAL OF BIOLOGICAL CHEMISTRY LA English DT Article DE Arachidonic Acid (AA) (ARA); Eicosanoid Biosynthesis; Lipid Signaling; Lipoxygenase Pathway; Protein Structure; X-ray Crystallography ID ACTIVE-SITE; SOYBEAN LIPOXYGENASE-1; ARACHIDONIC-ACID; DATA QUALITY; FATTY-ACIDS; INHIBITION; SPECIFICITY; OXYGENATION; CATALYSIS; 15-LIPOXYGENASE AB Background: Lipoxygenases (LOX) catalyze the oxygenation of polyunsaturated fatty acids but generate distinct products from a common substrate. Results: We report the first structure of a LOX-substrate complex. Conclusion: The structure provides a context for understanding product specificity in enzymes that metabolize arachidonic acid. Significance: With roles in the production of potent lipid mediators, LOX are targets for drug design. Lipoxygenases (LOX) play critical roles in mammalian biology in the generation of potent lipid mediators of the inflammatory response; consequently, they are targets for the development of isoform-specific inhibitors. The regio- and stereo-specificity of the oxygenation of polyunsaturated fatty acids by the enzymes is understood in terms of the chemistry, but structural observation of the enzyme-substrate interactions is lacking. Although several LOX crystal structures are available, heretofore the rapid oxygenation of bound substrate has precluded capture of the enzyme-substrate complex, leaving a gap between chemical and structural insights. In this report, we describe the 2.0 angstrom resolution structure of 8R-LOX in complex with arachidonic acid obtained under anaerobic conditions. Subtle rearrangements, primarily in the side chains of three amino acids, allow binding of arachidonic acid in a catalytically competent conformation. Accompanying experimental work supports a model in which both substrate tethering and cavity depth contribute to positioning the appropriate carbon at the catalytic machinery. C1 [Bender, Gunes; Bartlett, Sue G.; Newcomer, Marcia E.] Louisiana State Univ, Dept Biol Sci, Baton Rouge, LA 70803 USA. [Neau, David B.] Cornell Univ, Argonne Natl Lab, Dept Chem & Chem Biol, Northeastern Collaborat Access Team, Argonne, IL 60439 USA. [Boeglin, William E.; Brash, Alan R.] Vanderbilt Univ, Dept Pharmacol, Sch Med, Nashville, TN 37232 USA. RP Newcomer, ME (reprint author), Louisiana State Univ, Dept Biol Sci, Baton Rouge, LA 70803 USA. EM newcomer@lsu.edu FU Nation Institute of General Medical Sciences from the National Institutes of Health [P41 GM103403]; U. S. Department of Energy [DE-AC02-06CH11357] FX This work includes research conducted at the Advanced Photon Source on the Northeastern Collaborative Access Team beamlines, which are supported by a grant from the Nation Institute of General Medical Sciences (P41 GM103403) from the National Institutes of Health. Use of the Advanced Photon Source, an Office of Science User Facility operated for the U. S. Department of Energy Office of Science by Argonne National Laboratory, was supported by the U. S. Department of Energy under Contract DE-AC02-06CH11357. NR 44 TC 14 Z9 15 U1 2 U2 15 PU AMER SOC BIOCHEMISTRY MOLECULAR BIOLOGY INC PI BETHESDA PA 9650 ROCKVILLE PIKE, BETHESDA, MD 20814-3996 USA SN 0021-9258 EI 1083-351X J9 J BIOL CHEM JI J. Biol. Chem. PD NOV 14 PY 2014 VL 289 IS 46 BP 31905 EP 31913 DI 10.1074/jbc.M114.599662 PG 9 WC Biochemistry & Molecular Biology SC Biochemistry & Molecular Biology GA AU0LP UT WOS:000345314700021 PM 25231982 ER PT J AU Howe, JY Allard, LF Bigelow, WC Demers, H Overbury, SH AF Howe, Jane Y. Allard, Lawrence F. Bigelow, Wilbur C. Demers, Hendrix Overbury, Steven H. TI Understanding catalyst behavior during in situ heating through simultaneous secondary and transmitted electron imaging SO NANOSCALE RESEARCH LETTERS LA English DT Article DE Scanning transmission electron microscopy; Scanning electron microscopy; Catalyst; Phase transformation; In situ characterization ID HYDROGENATION REACTIONS; GOLD CATALYSTS; SINGLE ATOMS; MICROSCOPY; RESOLUTION; TEMPERATURES; PERFORMANCE; HEMATITE; SIZE AB By coupling techniques of simultaneous secondary (SE) and transmitted electron (TE) imaging at high resolution in a modern scanning transmission electron microscope (STEM), with the ability to heat specimens using a highly stable MEMS-based heating platform, we obtained synergistic information to clarify the behavior of catalysts during in situ thermal treatments. Au/iron oxide catalyst 'leached' to remove surface Au was heated to temperatures as high as 700 degrees C. The Fe2O3 support particle structure tended to reduce to Fe3O4 and formed surface terraces; the formation, coalescence, and mobility of 1- to 2-nm particles on the terraces were characterized in SE, STEM-ADF, and TEM-BF modes. If combined with simultaneous nanoprobe spectroscopy, this approach will open the door to a new way of studying the kinetics of nano-scaled phenomena. C1 [Howe, Jane Y.; Allard, Lawrence F.; Overbury, Steven H.] Oak Ridge Natl Lab, Phys Sci Directorate, Oak Ridge, TN 37831 USA. [Bigelow, Wilbur C.] Univ Michigan, Dept Mat Sci & Engn, Ann Arbor, MI 48104 USA. [Demers, Hendrix] McGill Univ, Dept Min & Mat Engn, Montreal, PQ H3A 2B2, Canada. [Howe, Jane Y.] Hitachi High Technol Canada Inc, Toronto, ON M9W 6A4, Canada. RP Howe, JY (reprint author), Oak Ridge Natl Lab, Phys Sci Directorate, 1 Bethel Valley Rd, Oak Ridge, TN 37831 USA. EM jane.howe@gmail.com RI Overbury, Steven/C-5108-2016; Howe, Jane/G-2890-2011 OI Overbury, Steven/0000-0002-5137-3961; FU US Department of Energy, Office of Energy Efficiency and Renewable Energy, Vehicle Technologies Office, Propulsion Materials Program FX Microscopy research at the Oak Ridge National Laboratory's High Temperature Materials Laboratory was sponsored by the US Department of Energy, Office of Energy Efficiency and Renewable Energy, Vehicle Technologies Office, Propulsion Materials Program. This is a contributed paper and published as part of the Proceedings of the Microscopy and Microanalysis 2010, Portland, OR, USA, August, 2010. NR 24 TC 2 Z9 2 U1 4 U2 34 PU SPRINGER PI NEW YORK PA 233 SPRING ST, NEW YORK, NY 10013 USA SN 1556-276X J9 NANOSCALE RES LETT JI Nanoscale Res. Lett. PD NOV 14 PY 2014 VL 9 AR 614 DI 10.1186/1556-276X-9-614 PG 6 WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied SC Science & Technology - Other Topics; Materials Science; Physics GA AU2CH UT WOS:000345423100001 PM 25419195 ER PT J AU Muller, A Schippers, S Esteves-Macaluso, D Habibi, M Aguilar, A Kilcoyne, ALD Phaneuf, RA Ballance, CP McLaughlin, BM AF Mueller, A. Schippers, S. Esteves-Macaluso, D. Habibi, M. Aguilar, A. Kilcoyne, A. L. D. Phaneuf, R. A. Ballance, C. P. McLaughlin, B. M. TI Valence-shell photoionization of Ag-like Xe7+ ions: experiment and theory SO JOURNAL OF PHYSICS B-ATOMIC MOLECULAR AND OPTICAL PHYSICS LA English DT Article DE photoionization; xenon ions; cross sections; experiment; theory ID ELECTRON-IMPACT EXCITATION; SINGLY-CHARGED XE; R-MATRIX METHOD; 4D PHOTOIONIZATION; ENERGY REGION; SCATTERING; KRYPTON AB We report on experimental and theoretical results for the photoionization of Ag-like xenon ions, Xe7+, in the photon energy range 95-145 eV. The measurements were carried out at the Advanced Light Source at an energy resolution of Delta E = 65 meV with additional measurements made at Delta E = 28 meV and 39 meV. Small resonance features below the ground-state ionization threshold, at about 106 eV, are due to the presence of metastable Xe7+(4d(10)4f F-2 degrees(5/2, 7/2)) ions in the ion beam. On the basis of the accompanying theoretical calculations using the Dirac atomic R-matrix codes (DARC), an admixture of only a few percent of metastable ions in the parent ion beam is inferred, with almost 100% of the parent ions in the (4d(10)5s S-2(1/2)) ground level. The cross section is dominated by a very strong resonance associated with 4d -> 5f excitation and subsequent autoionization. This prominent feature in the measured spectrum is the 4d(9)5s5f(2)P degrees resonance located at (122.139 +/- 0.01) eV. An absolute peak cross section of 1.2 Gigabarns was measured at 38 meV energy resolution. The experimental natural width Gamma = 76 +/- 3 meV of this resonance compares well with the theoretical estimate of 88 meV obtained from the DARC calculation with 249 target states. Given the complexity of the system, overall satisfactory agreement between theory and experiment is obtained for the photon energy region investigated. C1 [Mueller, A.; Schippers, S.] Univ Giessen, Inst Atom & Mol Phys, D-35392 Giessen, Germany. [Esteves-Macaluso, D.; Aguilar, A.; Kilcoyne, A. L. D.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94720 USA. [Esteves-Macaluso, D.; Habibi, M.; Phaneuf, R. A.] Univ Nevada, Dept Phys, Reno, NV 89557 USA. [Ballance, C. P.] Auburn Univ, Dept Phys, Allison Lab 206, Auburn, AL 36849 USA. [McLaughlin, B. M.] Queens Univ Belfast, Sch Math & Phys, CTAMOP, Belfast BT7 1NN, Antrim, North Ireland. [McLaughlin, B. M.] Harvard Smithsonian Ctr Astrophys, Inst Theoret Atom & Mol Phys, Cambridge, MA 02138 USA. RP Muller, A (reprint author), Univ Giessen, Inst Atom & Mol Phys, D-35392 Giessen, Germany. EM Alfred.Mueller@iamp.physik.uni-giessen.de; b.mclaughlin@qub.ac.uk RI Muller, Alfred/A-3548-2009; Kilcoyne, David/I-1465-2013; Schippers, Stefan/A-7786-2008 OI Muller, Alfred/0000-0002-0030-6929; Schippers, Stefan/0000-0002-6166-7138 FU Deutsche Forschungsgemeinschaft [Mu 1068/10]; US Department of Energy (DOE) [DE-AC03-76SF-00098, DE-FG02-03ER15424]; US Department of Energy (DoE) through Auburn University; US National Science Foundation; Queen's University Belfast; National Science Foundation [OCI-1053575]; Office of Science, Office of Basic Energy Sciences, of the US Department of Energy [DE-AC02-05CH11231] FX We acknowledge support by Deutsche Forschungsgemeinschaft under project number Mu 1068/10 as well as by the US Department of Energy (DOE) under contract DE-AC03-76SF-00098 and grant DE-FG02-03ER15424. C P Ballance was supported by US Department of Energy (DoE) grants through Auburn University. B M McLaughlin acknowledges support by the US National Science Foundation through a grant to ITAMP at the Harvard-Smithsonian Center for Astrophysics, a visiting research fellowship (VRF) from Queen's University Belfast and the hospitality of AM, SS and the University of Giessen. The computational work was carried out at the National Energy Research Scientific Computing Center in Oakland, CA, USA, the Kraken XT5 facility at the National Institute for Computational Science (NICS) in Knoxville, TN, USA and at the High Performance Computing Center Stuttgart (HLRS) of the University of Stuttgart, Stuttgart, Germany. The Kraken XT5 facility is a resource of the Extreme Science and Engineering Discovery Environment (XSEDE), which is supported by National Science Foundation grant number OCI-1053575. The Advanced Light Source is supported by the Director, Office of Science, Office of Basic Energy Sciences, of the US Department of Energy under Contract No. DE-AC02-05CH11231. NR 44 TC 9 Z9 10 U1 0 U2 9 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0953-4075 EI 1361-6455 J9 J PHYS B-AT MOL OPT JI J. Phys. B-At. Mol. Opt. Phys. PD NOV 14 PY 2014 VL 47 IS 21 AR 215202 DI 10.1088/0953-4075/47/21/215202 PG 10 WC Optics; Physics, Atomic, Molecular & Chemical SC Optics; Physics GA AS8KH UT WOS:000344497400009 ER PT J AU Schilter, D Pelmenschikov, V Wang, HX Meier, F Gee, LB Yoda, Y Kaupp, M Rauchfuss, TB Cramer, SP AF Schilter, David Pelmenschikov, Vladimir Wang, Hongxin Meier, Florian Gee, Leland B. Yoda, Yoshitaka Kaupp, Martin Rauchfuss, Thomas B. Cramer, Stephen P. TI Synthesis and vibrational spectroscopy of Fe-57-labeled models of [NiFe] hydrogenase: first direct observation of a nickel-iron interaction SO CHEMICAL COMMUNICATIONS LA English DT Article ID NUCLEAR RESONANT SCATTERING; ACTIVE-SITE; METAL-METAL; ELECTRON LOCALIZABILITY; DENSITY ANALYSIS; LOCALIZATION; PRECURSORS; COMPLEXES; STATE; RAMAN AB A new route to iron carbonyls has enabled synthesis of Fe-57-labeled [NiFe] hydrogenase mimic (OC)(3)Fe-57(pdt)Ni(dppe). Its study by nuclear resonance vibrational spectroscopy revealed Ni-Fe-57 vibrations, as confirmed by calculations. The modes are absent for [(OC)(3)Fe-57(pdt)Ni(dppe)](+), which lacks Ni-Fe-57 bonding, underscoring the utility of the analyses in identifying metal-metal interactions. C1 [Schilter, David; Rauchfuss, Thomas B.] Univ Illinois, Dept Chem, Urbana, IL 61801 USA. [Pelmenschikov, Vladimir; Meier, Florian; Kaupp, Martin] Tech Univ Berlin, Inst Chem, D-10623 Berlin, Germany. [Wang, Hongxin; Gee, Leland B.; Cramer, Stephen P.] Univ Calif Davis, Dept Chem, Davis, CA 95616 USA. [Wang, Hongxin; Cramer, Stephen P.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Phys Biosci Div, Berkeley, CA 94720 USA. [Yoda, Yoshitaka] JASRI, Sayo, Hyogo 6795198, Japan. RP Schilter, D (reprint author), Univ Illinois, Dept Chem, Urbana, IL 61801 USA. EM schilter@illinois.edu; spjcramer@ucdavis.edu RI Gee, Leland/H-1742-2014; Dr. Kaupp, Martin/K-9569-2016; OI Gee, Leland/0000-0002-5817-3997; Schilter, David/0000-0002-5720-6806 FU National Institutes of Health [GM061153-10, GM-65440]; U.S. Department of Energy Office of Biological and Environmental Research (DOE OBER); 'Unifying Concepts in Catalysis' initiative of the German Research Council; JASRI [2013A0032] FX Thanks are given to Drs Mark J. Nilges and Haijun Yao for assistance with EPR and LI-FDI-MS, respectively. Financial support was provided by the National Institutes of Health (GM061153-10 to T.B.R. and GM-65440 to S.P.C.), U.S. Department of Energy Office of Biological and Environmental Research (DOE OBER) (S.P.C.), and the 'Unifying Concepts in Catalysis' initiative of the German Research Council (V.P., F.M., and M.K.). NRVS experiments performed at SPring-8 BL09XU were funded by JASRI (beamtime proposal 2013A0032). NR 34 TC 4 Z9 4 U1 1 U2 48 PU ROYAL SOC CHEMISTRY PI CAMBRIDGE PA THOMAS GRAHAM HOUSE, SCIENCE PARK, MILTON RD, CAMBRIDGE CB4 0WF, CAMBS, ENGLAND SN 1359-7345 EI 1364-548X J9 CHEM COMMUN JI Chem. Commun. PD NOV 14 PY 2014 VL 50 IS 88 BP 13469 EP 13472 DI 10.1039/c4cc04572f PG 4 WC Chemistry, Multidisciplinary SC Chemistry GA AS0KE UT WOS:000343965300010 PM 25237680 ER PT J AU Al-Hamdani, YS Alfe, D von Lilienfeld, OA Michaelides, A AF Al-Hamdani, Yasmine S. Alfe, Dario von Lilienfeld, O. Anatole Michaelides, Angelos TI Water on BN doped benzene: A hard test for exchange-correlation functionals and the impact of exact exchange on weak binding SO JOURNAL OF CHEMICAL PHYSICS LA English DT Article ID BASIS-SET CONVERGENCE; HARTREE-FOCK PSEUDOPOTENTIALS; INITIO MOLECULAR-DYNAMICS; TOTAL-ENERGY CALCULATIONS; DER-WAALS INTERACTIONS; DIFFUSION MONTE-CARLO; AUGMENTED-WAVE METHOD; GAUSSIAN-BASIS SETS; BORON-NITRIDE; NONCOVALENT INTERACTIONS AB Density functional theory (DFT) studies of weakly interacting complexes have recently focused on the importance of van der Waals dispersion forces, whereas the role of exchange has received far less attention. Here, by exploiting the subtle binding between water and a boron and nitrogen doped benzene derivative (1,2-azaborine) we show how exact exchange can alter the binding conformation within a complex. Benchmark values have been calculated for three orientations of the water monomer on 1,2-azaborine from explicitly correlated quantum chemical methods, and we have also used diffusion quantum Monte Carlo. For a host of popular DFT exchange-correlation functionals we show that the lack of exact exchange leads to the wrong lowest energy orientation of water on 1,2-azaborine. As such, we suggest that a high proportion of exact exchange and the associated improvement in the electronic structure could be needed for the accurate prediction of physisorption sites on doped surfaces and in complex organic molecules. Meanwhile to predict correct absolute interaction energies an accurate description of exchange needs to be augmented by dispersion inclusive functionals, and certain non-local van der Waals functionals (optB88- and optB86b-vdW) perform very well for absolute interaction energies. Through a comparison with water on benzene and borazine (B3N3H6) we show that these results could have implications for the interaction of water with doped graphene surfaces, and suggest a possible way of tuning the interaction energy. (C) 2014 Author(s). All article content, except where otherwise noted, is licensed under a Creative Commons Attribution 3.0 Unported License. C1 [Al-Hamdani, Yasmine S.; Alfe, Dario; Michaelides, Angelos] Thomas Young Ctr, London WC1H 0AH, England. [Al-Hamdani, Yasmine S.; Alfe, Dario; Michaelides, Angelos] London Ctr Nanotechnol, London WC1H 0AH, England. [Al-Hamdani, Yasmine S.; Michaelides, Angelos] UCL, Dept Chem, London WC1H 0AJ, England. [Alfe, Dario] UCL, Dept Earth Sci, London WC1E 6BT, England. [von Lilienfeld, O. Anatole] Univ Basel, Inst Phys Chem, Dept Chem, CH-4056 Basel, Switzerland. [von Lilienfeld, O. Anatole] Argonne Natl Labs, Lemont, IL 60439 USA. RP Al-Hamdani, YS (reprint author), Thomas Young Ctr, 17-19 Gordon St, London WC1H 0AH, England. EM angelos.michaelides@ucl.ac.uk RI von Lilienfeld, O. Anatole/D-8529-2011; Alfe`, Dario/C-1521-2008; OI Alfe`, Dario/0000-0002-9741-8678; Michaelides, Angelos/0000-0002-9169-169X FU University College London; Argonne National Laboratory (ANL) through Thomas Young Centre-ANL initiative; European Research Council under European Union [616121]; Royal Society; Swiss National Science foundation [PPOOP2 138932]; Office of Science of the U.S. Department of Energy (DOE) [DEAC05-00OR22725]; Office of Science of the U.S. DOE [DE-AC02-06CH11357] FX We are grateful for support from University College London and Argonne National Laboratory (ANL) through the Thomas Young Centre-ANL initiative. Some of the research leading to these results has received funding from the European Research Council under the European Union's Seventh Framework Programme (FP/2007-2013)/ERC Grant Agreement No. 616121 (HeteroIce project). A. M. is supported by the Royal Society through a Wolfson Research Merit Award. O.A.v.L. acknowledges funding from the Swiss National Science foundation (Grant No. PPOOP2 138932). This research used resources as part of an INCITE project (awarded to D. A.) at the Oak Ridge National Laboratory (Titan) which is supported by the Office of Science of the U. S. Department of Energy (DOE) under Contract No. DEAC05-00OR22725. This research also used resources of the Argonne Leadership Computing Facility at Argonne National Laboratory, which is supported by the Office of Science of the U. S. DOE under Contract No. DE-AC02-06CH11357. In addition, we are grateful for computing resources provided by the London Centre for Nanotechnology and University College London. We would like to thank G. Tocci, C. Gattinoni, and R. Ramakrishnan for useful discussions. NR 110 TC 12 Z9 12 U1 1 U2 32 PU AMER INST PHYSICS PI MELVILLE PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA SN 0021-9606 EI 1089-7690 J9 J CHEM PHYS JI J. Chem. Phys. PD NOV 14 PY 2014 VL 141 IS 18 AR 18C530 DI 10.1063/1.4898356 PG 8 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AT3PZ UT WOS:000344847600074 PM 25399195 ER PT J AU Feng, RR Guo, Y Wang, HF AF Feng, Ran-Ran Guo, Yuan Wang, Hong-Fei TI Reorientation of the "free OH" group in the top-most layer of air/water interface of sodium fluoride aqueous solution probed with sum-frequency generation vibrational spectroscopy SO JOURNAL OF CHEMICAL PHYSICS LA English DT Article ID SURFACE 2ND-HARMONIC GENERATION; LIQUID WATER-SURFACE; MOLECULAR-STRUCTURE; SFG-VS; THEORETICAL-ANALYSIS; SALT-SOLUTIONS; WATER/VAPOR INTERFACE; LANGMUIR MONOLAYER; HALIDE INTERFACES; ORIENTATION AB Many experimental and theoretical studies have established the specific anion, as well as cation, effects on the hydrogen-bond structures at the air/water interface of electrolyte solutions. However, the ion effects on the top-most layer of the air/water interface, which is signified by the non-hydrogenbonded so-called "free OH" group, have not been explicitly discussed or studied. In this report, we present the measurement of changes of the orientational angle of the "free OH" group at the air/water interface of the sodium fluoride (NaF) solutions at different concentrations using the interface selective sum-frequency generation vibrational spectroscopy (SFG-VS) in the ssp and ppp polarizations. The polarization dependent SFG-VS results show that the average tilt angle of the "free OH" changes from about 36.6 degrees +/- 0.5 degrees to 44.1 degrees +/- 0.6 degrees as the NaF concentration increases from 0 to 0.94 M (nearly saturated). Such tilt angle change is around the axis of the other O-H group of the same water molecule at the top-most layer at the air/water interface that is hydrogen-bonded to the water molecules below the top-most layer. These results provide quantitative molecular details of the ion effects of the NaF salt on the structure of the water molecules at the top-most layer of the air/water interface, even though both the Na+ cation and the F- anion are believed to be among the most excluded ions from the air/water interface. (C) 2014 AIP Publishing LLC. C1 [Feng, Ran-Ran] Peking Univ, Int Ctr Quantum Mat, Beijing 100871, Peoples R China. [Guo, Yuan] Chinese Acad Sci, Beijing Natl Lab Mol Sci, Inst Chem, Beijing 100190, Peoples R China. [Wang, Hong-Fei] Pacific NW Natl Lab, William R Wiley Environm Mol Sci Lab, Richland, WA 99352 USA. RP Wang, HF (reprint author), Pacific NW Natl Lab, William R Wiley Environm Mol Sci Lab, 902 Battelle Blvd,POB 999, Richland, WA 99352 USA. EM hongfei.wang@pnnl.gov RI Wang, Hongfei/B-1263-2010 OI Wang, Hongfei/0000-0001-8238-1641 FU Natural Science Foundation of China (NSFC) [20425309, 20533070, 20773143, 20673122]; Ministry of Science and Technology of China (MOST) [2007CB815205]; Pacific Northwest National Laboratory (PNNL) LDRD program; Department of Energy's Office of Biological and Environmental Research (BER) FX SFG-VS data in this report were collected at the Beijing National Laboratory for Molecular Sciences, Institute of Chemistry, the Chinese Academy of Sciences, where R.-R.F. was a graduate student during 2005-2010, and H.-F.W. was a professor during 1999-2009. R.-R.F. thanks the helpful discussion from Wei Gan, Zhen Zhang, and Hong-Tao Bian. H.-F.W. thanks the helpful discussion from Chuanshan Tian. H.-F.W. also thanks the support by the Natural Science Foundation of China (NSFC, Grant Nos. 20425309, 20533070, and 20773143) and the Ministry of Science and Technology of China (MOST No. 2007CB815205). Y.G. thanks the support by the Natural Science Foundation of China (NSFC, Grant No. 20673122). Part of this work was supported by the Pacific Northwest National Laboratory (PNNL) LDRD program, and was conducted at the William R. Wiley Environmental Molecular Sciences Laboratory (EMSL), a national scientific user facility located at the Pacific Northwest National Laboratory and sponsored by the Department of Energy's Office of Biological and Environmental Research (BER). NR 102 TC 6 Z9 6 U1 4 U2 47 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0021-9606 EI 1089-7690 J9 J CHEM PHYS JI J. Chem. Phys. PD NOV 14 PY 2014 VL 141 IS 18 AR 18C507 DI 10.1063/1.4895561 PG 10 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AT3PZ UT WOS:000344847600051 PM 25399172 ER PT J AU Jones, RE Ward, DK Templeton, JA AF Jones, R. E. Ward, D. K. Templeton, J. A. TI Spatial resolution of the electrical conductance of ionic fluids using a Green-Kubo method SO JOURNAL OF CHEMICAL PHYSICS LA English DT Article ID MOLECULAR-DYNAMICS SIMULATIONS; STATISTICAL-MECHANICAL THEORY; TRANSPORT-COEFFICIENTS; IRREVERSIBLE-PROCESSES; THERMAL-CONDUCTIVITY; ATOMISTIC SIMULATION; RECIPROCAL RELATIONS; LIQUID FLOW; FORMULAS; SYSTEMS AB We present a Green-Kubo method to spatially resolve transport coefficients in compositionally heterogeneous mixtures. We develop the underlying theory based on well-known results from mixture theory, Irving-Kirkwood field estimation, and linear response theory. Then, using standard molecular dynamics techniques, we apply the methodology to representative systems. With a homogeneous salt water system, where the expectation of the distribution of conductivity is clear, we demonstrate the sensitivities of the method to system size, and other physical and algorithmic parameters. Then we present a simple model of an electrochemical double layer where we explore the resolution limit of the method. In this system, we observe significant anisotropy in the wall-normal vs. transverse ionic conductances, as well as near wall effects. Finally, we discuss extensions and applications to more realistic systems such as batteries where detailed understanding of the transport properties in the vicinity of the electrodes is of technological importance. (C) 2014 AIP Publishing LLC. C1 [Jones, R. E.] Sandia Natl Labs, Mech Mat Dept, Livermore, CA 94550 USA. [Ward, D. K.] Sandia Natl Labs, Mat Chem Dept, Livermore, CA 94550 USA. [Templeton, J. A.] Sandia Natl Labs, Thermal Fluid Sci & Engn Dept, Livermore, CA 94550 USA. RP Jones, RE (reprint author), Sandia Natl Labs, Mech Mat Dept, Livermore, CA 94550 USA. FU Laboratory Directed Research and Development (LDRD) program at Sandia National Laboratory; Advanced Simulation and Computing (ASC) program at Sandia National Laboratory; U.S. Department of Energy's National Nuclear Security Administration [DE-AC04-94AL85000] FX This work was supported by the Laboratory Directed Research and Development (LDRD) and Advanced Simulation and Computing (ASC) programs at Sandia National Laboratories. Sandia is a multiprogram laboratory managed and operated by Sandia Corporation, a wholly-owned subsidiary of Lockheed Martin Corporation, for the U.S. Department of Energy's National Nuclear Security Administration under Contract No. DE-AC04-94AL85000. The authors are grateful to J. Lechman, K. Mandadapu, and J. Zimmerman for helpful comments on a draft of this paper. NR 78 TC 1 Z9 1 U1 1 U2 9 PU AMER INST PHYSICS PI MELVILLE PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA SN 0021-9606 EI 1089-7690 J9 J CHEM PHYS JI J. Chem. Phys. PD NOV 14 PY 2014 VL 141 IS 18 AR 184110 DI 10.1063/1.4901035 PG 13 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AT3PZ UT WOS:000344847600014 PM 25399135 ER PT J AU Kimmel, GA Zubkov, T Smith, RS Petrik, NG Kay, BD AF Kimmel, Greg A. Zubkov, Tykhon Smith, R. Scott Petrik, Nikolay G. Kay, Bruce D. TI Turning things downside up: Adsorbate induced water flipping on Pt(111) SO JOURNAL OF CHEMICAL PHYSICS LA English DT Article ID AMORPHOUS SOLID WATER; MOLECULAR-DYNAMICS; FUNDAMENTAL-ASPECTS; QUADRUPOLE-MOMENTS; METAL-SURFACES; ICE FILMS; ADSORPTION; INTERFACES; KINETICS; GROWTH AB We have examined the adsorption of the weakly bound species N-2, O-2, CO, and Kr on the (root 37 x root 37)R25.3 degrees water monolayer on Pt(111) using a combination of molecular beam dosing, infrared reflection absorption spectroscopy, and temperature programmed desorption. In contrast to multilayer crystalline ice, the adsorbate-free water monolayer is characterized by a lack of dangling OH bonds protruding into the vacuum (H-up). Instead, the non-hydrogen-bonded OH groups are oriented downward (H-down) to maximize their interaction with the underlying Pt(111) substrate. Adsorption of Kr and O-2 have little effect on the structure and vibrational spectrum of the "root 37" water monolayer while adsorption of both N-2, and CO are effective in "flipping" H-down water molecules into an H-up configuration. This "flipping" occurs readily upon adsorption at temperatures as low as 20 K and the water monolayer transforms back to the H-down, "root 37" structure upon adsorbate desorption above 35 K, indicating small energy differences and barriers between the H-down and H-up configurations. The results suggest that converting water in the first layer from H-down to Hup is mediated by the electrostatic interactions between the water and the adsorbates. (C) 2014 AIP Publishing LLC. C1 [Kimmel, Greg A.; Zubkov, Tykhon; Smith, R. Scott; Petrik, Nikolay G.; Kay, Bruce D.] Pacific NW Natl Lab, Div Phys Sci, Richland, WA 99352 USA. RP Kimmel, GA (reprint author), Pacific NW Natl Lab, Div Phys Sci, MSIN K8-88,POB 999, Richland, WA 99352 USA. EM gregory.kimmel@pnnl.gov; bruce.kay@pnnl.gov RI Smith, Scott/G-2310-2015; Petrik, Nikolay/G-3267-2015; OI Smith, Scott/0000-0002-7145-1963; Petrik, Nikolay/0000-0001-7129-0752; Kimmel, Greg/0000-0003-4447-2440 FU U.S. Department of Energy (DOE), Office of Basic Energy Sciences, Division of Chemical Sciences, Geosciences, and Biosciences; DOE's Office of Biological and Environmental Research; DOE [DE-AC05-76RL01830] FX This work was supported by the U.S. Department of Energy (DOE), Office of Basic Energy Sciences, Division of Chemical Sciences, Geosciences, and Biosciences. The research was performed using EMSL, a national scientific user facility sponsored by DOE's Office of Biological and Environmental Research and located at Pacific Northwest National Laboratory, which is operated by Battelle operated for the DOE under Contract No. DE-AC05-76RL01830. NR 55 TC 4 Z9 4 U1 1 U2 37 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0021-9606 EI 1089-7690 J9 J CHEM PHYS JI J. Chem. Phys. PD NOV 14 PY 2014 VL 141 IS 18 AR 18C515 DI 10.1063/1.4896226 PG 8 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AT3PZ UT WOS:000344847600059 PM 25399180 ER PT J AU Molinero, V Kay, BD AF Molinero, Valeria Kay, Bruce D. TI Preface: Special Topic on Interfacial and Confined Water SO JOURNAL OF CHEMICAL PHYSICS LA English DT Editorial Material AB This special topic on the chemical physics of interfacial and confined water contains a collection of original research papers that showcase recent theoretical and experimental advances in the field. These papers provide a timely discussion of fundamental aspects of interfacial and confined water that are important in both natural environments and engineered applications. (C) 2014 AIP Publishing LLC. C1 [Molinero, Valeria] Univ Utah, Dept Chem, Salt Lake City, UT 84112 USA. [Kay, Bruce D.] Pacific NW Natl Lab, Fundamental & Computat Sci Directorate, Richland, WA 99352 USA. RP Molinero, V (reprint author), Univ Utah, Dept Chem, 315 South 1400 East, Salt Lake City, UT 84112 USA. EM valeria.molinero@utah.edu; bruce.kay@pnnl.gov NR 0 TC 1 Z9 1 U1 1 U2 24 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0021-9606 EI 1089-7690 J9 J CHEM PHYS JI J. Chem. Phys. PD NOV 14 PY 2014 VL 141 IS 18 AR 18C101 DI 10.1063/1.4900822 PG 2 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AT3PZ UT WOS:000344847600044 PM 25399165 ER PT J AU Sellner, B Kathmann, SM AF Sellner, Bernhard Kathmann, Shawn M. TI A matter of quantum voltages SO JOURNAL OF CHEMICAL PHYSICS LA English DT Article ID CORRELATED MOLECULAR CALCULATIONS; ATOMIC SCATTERING FACTORS; GAUSSIAN-BASIS SETS; ELECTRON HOLOGRAPHY; PROGRAM SYSTEM; FREE-ENERGY; DENSITY; POTENTIALS; WATER; APPROXIMATION AB Voltages inside matter are relevant to crystallization, materials science, biology, catalysis, and aqueous chemistry. The variation of voltages in matter can be measured by experiment, however, modern supercomputers allow the calculation of accurate quantum voltages with spatial resolutions of bulk systems well beyond what can currently be measured provided a sufficient level of theory is employed. Of particular interest is the Mean Inner Potential (V-o) - the spatial average of these quantum voltages referenced to the vacuum. Here we establish a protocol to reliably evaluate V-o from quantum calculations. Voltages are very sensitive to the distribution of electrons and provide metrics to understand interactions in condensed phases. In the present study, we find excellent agreement with measurements of V-o for vitrified water and salt crystals and demonstrate the impact of covalent and ionic bonding as well as intermolecular/atomic interactions. Certain aspects in this regard are highlighted making use of simple model systems/approximations. Furthermore, we predict V-o as well as the fluctuations of these voltages in aqueous NaCl electrolytes and characterize the changes in their behavior as the resolution increases below the size of atoms. (C) 2014 AIP Publishing LLC. C1 [Sellner, Bernhard; Kathmann, Shawn M.] Pacific NW Natl Lab, Div Phys Sci, Richland, WA 99352 USA. RP Kathmann, SM (reprint author), Pacific NW Natl Lab, Div Phys Sci, Richland, WA 99352 USA. EM Shawn.Kathmann@pnnl.gov FU Office of Science of the U.S. Department of Energy [DEAC02-05CH11231] FX We would like to gratefully acknowledge helpful discussions with Bernd Kabius, Christopher J. Mundy, and Gregory K. Schenter. This work was supported by the U. S. Department of Energy, Office of Basic Energy Sciences, Division of Chemical Sciences, Geosciences & Biosciences. Pacific Northwest National Laboratory (PNNL) is a multiprogram national laboratory operated for the U.S. Department of Energy (DOE) by Battelle. This research used resources of the National Energy Research Scientific Computing Center, which is supported by the Office of Science of the U.S. Department of Energy under Contract No. DEAC02-05CH11231. NR 60 TC 7 Z9 7 U1 0 U2 18 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0021-9606 EI 1089-7690 J9 J CHEM PHYS JI J. Chem. Phys. PD NOV 14 PY 2014 VL 141 IS 18 AR 18C534 DI 10.1063/1.4898797 PG 13 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AT3PZ UT WOS:000344847600078 PM 25399199 ER PT J AU Thurmer, K Nie, S Feibelman, PJ Bartelt, NC AF Thuermer, Konrad Nie, Shu Feibelman, Peter J. Bartelt, Norman C. TI Clusters, molecular layers, and 3D crystals of water on Ni(111) SO JOURNAL OF CHEMICAL PHYSICS LA English DT Article ID TOTAL-ENERGY CALCULATIONS; AUGMENTED-WAVE METHOD; BASIS-SET; ADSORPTION; H2O; ICE; PT(111); METALS; OXYGEN; NUCLEATION AB We examined the growth and stability of ice layers on Ni(111) up to similar to 7 molecular layers (ML) thick using scanning tunneling microscopy. At low coverage, films were comprised of similar to 1 nm wide two-dimensional (2D) clusters. Only above similar to 0.5 ML did patches of continuous 2D layers emerge, coexisting with the clusters until the first ML was complete. The structure of the continuous layer is clearly different from that of the 2D clusters. Subsequently, a second molecular layer grew on top of the first. 3D crystallites started to form only after this 2nd ML was complete. 2D clusters re-appeared when thicker films were partially evaporated, implying that these clusters represent the equilibrium configuration at low coverage. Binding energies and image simulations computed with density functional theory suggest that the 2D clusters are partially dissociated and surrounded by H adatoms. The complete 2D layer contains only intact water molecules because of the lack of favorable binding sites for H atoms. We propose molecular structures for the 2D layer that are composed of the same pentagon-heptagon binding motif and water density observed on Pt(111). The similarity of the water structures on Pt and Ni suggests a general prescription for generating low-energy configurations on close-packed metal substrates. (C) 2014 AIP Publishing LLC. C1 [Thuermer, Konrad; Nie, Shu; Bartelt, Norman C.] Sandia Natl Labs, Livermore, CA 94550 USA. [Feibelman, Peter J.] Sandia Natl Labs, Albuquerque, NM 87185 USA. RP Thurmer, K (reprint author), Sandia Natl Labs, Livermore, CA 94550 USA. RI Thurmer, Konrad/L-4699-2013 OI Thurmer, Konrad/0000-0002-3078-7372 FU DOE Office of Basic Energy Sciences, Division of Materials Science and Engineering; U.S. Department of Energy's National Nuclear Security Administration [DE-AC04-94AL85000] FX This work was supported by the DOE Office of Basic Energy Sciences, Division of Materials Science and Engineering. Sandia is operated by the Lockheed Martin Co. for the U.S. Department of Energy's National Nuclear Security Administration under Contract No. DE-AC04-94AL85000. VASP was developed at T. U. Wien's Institut fur Theoretische Physik. We thank an anonymous reviewer for making the interesting suggestion that configurational entropy might favor low coverage clusters. NR 48 TC 3 Z9 4 U1 9 U2 52 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0021-9606 EI 1089-7690 J9 J CHEM PHYS JI J. Chem. Phys. PD NOV 14 PY 2014 VL 141 IS 18 AR 18C520 DI 10.1063/1.4896300 PG 10 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AT3PZ UT WOS:000344847600064 PM 25399185 ER PT J AU White, AJ Gorshkov, VN Wang, RX Tretiak, S Mozyrsky, D AF White, Alexander J. Gorshkov, Vyacheslav N. Wang, Ruixi Tretiak, Sergei Mozyrsky, Dmitry TI Semiclassical Monte Carlo: A first principles approach to non-adiabatic molecular dynamics SO JOURNAL OF CHEMICAL PHYSICS LA English DT Article ID QUANTUM-CLASSICAL DYNAMICS; EXCITED-STATE DYNAMICS; BORN-OPPENHEIMER TRAJECTORIES; DENSITY-FUNCTIONAL THEORY; CHARGE-TRANSFER; ELECTRONIC DEGREES; SCATTERING THEORY; TIME; SYSTEMS; DECOHERENCE AB Modeling the dynamics of photophysical and (photo)chemical reactions in extended molecular systems is a new frontier for quantum chemistry. Many dynamical phenomena, such as intersystem crossing, non-radiative relaxation, and charge and energy transfer, require a non-adiabatic description which incorporate transitions between electronic states. Additionally, these dynamics are often highly sensitive to quantum coherences and interference effects. Several methods exist to simulate non-adiabatic dynamics; however, they are typically either too expensive to be applied to large molecular systems (10's-100's of atoms), or they are based on ad hoc schemes which may include severe approximations due to inconsistencies in classical and quantum mechanics. We present, in detail, an algorithm based on Monte Carlo sampling of the semiclassical time-dependent wavefunction that involves running simple surface hopping dynamics, followed by a post-processing step which adds little cost. The method requires only a few quantities from quantum chemistry calculations, can systematically be improved, and provides excellent agreement with exact quantum mechanical results. Here we show excellent agreement with exact solutions for scattering results of standard test problems. Additionally, we find that convergence of the wavefunction is controlled by complex valued phase factors, the size of the non-adiabatic coupling region, and the choice of sampling function. These results help in determining the range of applicability of the method, and provide a starting point for further improvement. (C) 2014 AIP Publishing LLC. C1 [White, Alexander J.; Gorshkov, Vyacheslav N.; Wang, Ruixi; Tretiak, Sergei; Mozyrsky, Dmitry] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA. [White, Alexander J.; Tretiak, Sergei] Los Alamos Natl Lab, Ctr Nonlinear Studies CNLS, Los Alamos, NM 87545 USA. [Gorshkov, Vyacheslav N.] Natl Tech Univ Ukraine, UA-03056 Kiev, Ukraine. [Wang, Ruixi] Wayne State Univ, Dept Chem, Detroit, MI 48202 USA. [Tretiak, Sergei] Los Alamos Natl Lab, Ctr Integrated Nanotechnol CINT, Los Alamos, NM 87545 USA. RP White, AJ (reprint author), Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA. EM serg@lanl.gov; mozyrsky@lanl.gov RI Tretiak, Sergei/B-5556-2009; Gorshkov, Vyacheslav/J-3329-2015; White, Alexander/D-8754-2014; OI Tretiak, Sergei/0000-0001-5547-3647; Gorshkov, Vyacheslav/0000-0002-7700-5649; White, Alexander/0000-0002-7771-3899; Mozyrsky, Dima/0000-0001-5305-4617 FU U.S. Department of Energy through the Los Alamos National Laboratory (LANL) LDRD Program; U.S. Department of Energy [DE-AC52-06NA25396]; Center for Nonlinear Studies (CNLS); Center for Integrated Nanotechnology (CINT) at LANL FX We acknowledge the support of the U.S. Department of Energy through the Los Alamos National Laboratory (LANL) LDRD Program. LANL is operated by Los Alamos National Security, LLC, for the National Nuclear Security Administration of the U.S. Department of Energy under Contract No. DE-AC52-06NA25396. We acknowledge the support of the Center for Nonlinear Studies (CNLS) and the Center for Integrated Nanotechnology (CINT) at LANL. We also thank J.E. Subotnik for sharing his numerical results reported in Ref. 48. NR 83 TC 6 Z9 6 U1 1 U2 34 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0021-9606 EI 1089-7690 J9 J CHEM PHYS JI J. Chem. Phys. PD NOV 14 PY 2014 VL 141 IS 18 AR 184101 DI 10.1063/1.4900988 PG 12 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AT3PZ UT WOS:000344847600005 PM 25399126 ER PT J AU Campbell, PG Merrill, MD Wood, BC Montalvo, E Worsley, MA Baumann, TF Biener, J AF Campbell, P. G. Merrill, M. D. Wood, B. C. Montalvo, E. Worsley, M. A. Baumann, T. F. Biener, J. TI Battery/supercapacitor hybrid via non-covalent functionalization of graphene macro-assemblies SO JOURNAL OF MATERIALS CHEMISTRY A LA English DT Article ID ELECTROCHEMICAL ENERGY-STORAGE; HIGH-SURFACE-AREA; CARBON NANOTUBES; SUPERCAPACITOR ELECTRODES; NEUTRON-SCATTERING; ANTHRAQUINONE; PERFORMANCE; CAPACITORS; PHENANTHRENEQUINONE; DEPOSITION AB Binder-free, monolithic, high surface area graphene macro-assemblies (GMAs) are promising materials for supercapacitor electrodes, but, like all graphitic carbon based supercapacitor electrodes, still tack sufficient energy density for demanding practical applications. Here, we demonstrate that the energy storage capacity of GMAs can be increased nearly 3-fold (up to 23 W h kg(-1)) by facile, non-covalent surface modification with anthraquinone (AQ). AQ provides battery-like redox charge storage (927 C g(-1)) without affecting the conductivity and capacitance of the GMA support. The resulting AQ-GMA battery/supercapacitor hybrid electrodes demonstrate excellent power performance, show remarkable long-term cycling stability and, by virtue of their excellent mechanical properties, allow for further increases in volumetric energy density by mechanical compression of the treated electrode. Our measured capacity is very close to the theoretical maximum obtained using detailed density functional theory calculations, suggesting nearly all incorporated AQ is made available for charge storage. C1 [Campbell, P. G.; Merrill, M. D.; Wood, B. C.; Montalvo, E.; Worsley, M. A.; Baumann, T. F.; Biener, J.] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA. RP Campbell, PG (reprint author), Lawrence Livermore Natl Lab, 7000 East Ave L-367, Livermore, CA 94550 USA. EM campbell82@llnl.gov OI Campbell, Patrick/0000-0003-0167-4624; Worsley, Marcus/0000-0002-8012-7727 FU U.S. Department of Energy by Lawrence Livermore National Laboratory [DE-AC52-07NA27344]; DOE Office of Energy Efficiency and Renewable Energy; Lawrence Livermore National Laboratory Directed Research and Development (LDRD) [12-ERD-035] FX This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344. Funding was provided by the DOE Office of Energy Efficiency and Renewable Energy, and the Lawrence Livermore National Laboratory Directed Research and Development (LDRD) Grant 12-ERD-035. NR 36 TC 12 Z9 12 U1 9 U2 71 PU ROYAL SOC CHEMISTRY PI CAMBRIDGE PA THOMAS GRAHAM HOUSE, SCIENCE PARK, MILTON RD, CAMBRIDGE CB4 0WF, CAMBS, ENGLAND SN 2050-7488 EI 2050-7496 J9 J MATER CHEM A JI J. Mater. Chem. A PD NOV 14 PY 2014 VL 2 IS 42 BP 17764 EP 17770 DI 10.1039/c4ta03605k PG 7 WC Chemistry, Physical; Energy & Fuels; Materials Science, Multidisciplinary SC Chemistry; Energy & Fuels; Materials Science GA AS0IO UT WOS:000343961300009 ER PT J AU Mancini, A Barbieri, VR Neuefeind, JC Page, K Malavasi, L AF Mancini, Alessandro Barbieri, Victoria Raissa Neuefeind, Joerg C. Page, Katharine Malavasi, Lorenzo TI Correlation between the local scale structure and the electrochemical properties in lithium orthosilicate cathode materials SO JOURNAL OF MATERIALS CHEMISTRY A LA English DT Article ID ELECTRICAL ENERGY-STORAGE; CRYSTAL-STRUCTURE; LI2MNSIO4; LI2FESIO4; BATTERY; POLYMORPH; CHEMISTRY AB Lithium metal orthosilicates with general formula Li2MSiO4 (M = Mn, Fe and Co) are among the most attractive new materials as potential high-specific-energy cathodes for lithium batteries. All the members of this family present a rich polymorphism with at least three clearly identified crystal structures of each Li2MSiO4 compound. Several theoretical investigations have highlighted that the energy stability of the different polymorphs is very close to each other irrespective of their average crystal structures. At the same time, the calculated and experimental electrochemical performances are again very similar among different polymorphs. By means of neutron total scattering investigation of different polymorphs (monoclinic and orthorhombic) of Li2FeSiO4 and Li2MnSiO4 orthosilicates coupled to Pair Distribution Function (PDF) analysis we showed that, at the local scale, all the polymorphs have the same structure (in particular the structure of the monoclinic polymorph) irrespective of the average structure they possess. This experimental evidence of a strong similarity at the local scale can be correlated with the observed electrochemical similarity (such as the lithium extraction voltages) among the different orthosilicate polymorphs, thus providing an approach to elucidate the relevance of local versus long-range structure. C1 [Mancini, Alessandro; Barbieri, Victoria Raissa; Malavasi, Lorenzo] Univ Pavia, Dept Chem, I-27100 Pavia, Italy. [Mancini, Alessandro; Barbieri, Victoria Raissa; Malavasi, Lorenzo] Univ Pavia, INSTM, I-27100 Pavia, Italy. [Neuefeind, Joerg C.; Page, Katharine] Oak Ridge Natl Lab, Chem & Engn Mat Div, Spallat Neutron Source, Oak Ridge, TN 37831 USA. [Page, Katharine] Los Alamos Natl Lab, Lujan Neutron Scattering Ctr, Los Alamos, NM 87545 USA. RP Malavasi, L (reprint author), Univ Pavia, Dept Chem, I-27100 Pavia, Italy. EM lorenzo.malavasi@unipv.it RI Page, Katharine/C-9726-2009; Neuefeind, Joerg/D-9990-2015; Malavasi, Lorenzo/P-1966-2016; OI Page, Katharine/0000-0002-9071-3383; Neuefeind, Joerg/0000-0002-0563-1544; Malavasi, Lorenzo/0000-0003-4724-2376 FU INTSM-RL research project "ATLANTE"; Scientific User Facilities Division, Office of Basic Energy Sciences; US Department of Energy; Department of Energy Office of Basic Energy Sciences FX Funding from the INTSM-RL research project "ATLANTE" is acknowledged. Research conducted at the ORNL's Spallation Neutron Source was sponsored by the Scientific User Facilities Division, Office of Basic Energy Sciences, and US Department of Energy. This work has benefited from the use of the Lujan Center at the Los Alamos Neutron Science Center, funded by the Department of Energy Office of Basic Energy Sciences. NR 23 TC 3 Z9 3 U1 9 U2 41 PU ROYAL SOC CHEMISTRY PI CAMBRIDGE PA THOMAS GRAHAM HOUSE, SCIENCE PARK, MILTON RD, CAMBRIDGE CB4 0WF, CAMBS, ENGLAND SN 2050-7488 EI 2050-7496 J9 J MATER CHEM A JI J. Mater. Chem. A PD NOV 14 PY 2014 VL 2 IS 42 BP 17867 EP 17874 DI 10.1039/c4ta04063e PG 8 WC Chemistry, Physical; Energy & Fuels; Materials Science, Multidisciplinary SC Chemistry; Energy & Fuels; Materials Science GA AS0IO UT WOS:000343961300021 ER PT J AU Chen, L Liu, YZ Ashuri, M Liu, CH Shaw, LL AF Chen, Lin Liu, Yuzi Ashuri, Maziar Liu, Caihong Shaw, Leon L. TI Li2S encapsulated by nitrogen-doped carbon for lithium sulfur batteries SO JOURNAL OF MATERIALS CHEMISTRY A LA English DT Article ID CATHODE MATERIAL; ION BATTERIES; HIGH-CAPACITY; S BATTERIES; CYCLE LIFE; PERFORMANCE; PARTICLES; COMPOSITE; SILICON; CELLS AB Using high-energy ball milling of the Li2S plus carbon black mixture followed by carbonization of pyrrole, we have established a facile approach to synthesize Li2S-plus-C composite particles of average size similar to 400 nm, encapsulated by a nitrogen-doped carbon shell. Such an engineered core-shell structure exhibits an ultrahigh initial discharge specific capacity (1029 mA h g(-1)), reaching 88% of the theoretical capacity (1165 mA h g(-1) of Li2S) and thus offering the highest utilization of Li2S in the cathode among all of the reported works for the encapsulated Li2S cathodes. This Li2S/C composite core with a nitrogen-doped carbon shell can still retain 652 mA h g(-1) after prolonged 100 cycles. These superior properties are attributed to the nitrogen-doped carbon shell that can improve the conductivity to enhance the utilization of Li2S in the cathode. Fine particle sizes and the presence of carbon black within the Li2S core may also play a role in high utilization of Li2S in the cathode. C1 [Chen, Lin; Ashuri, Maziar; Liu, Caihong; Shaw, Leon L.] Wanger Inst Sustainable Energy Res, Chicago, IL 60616 USA. [Chen, Lin; Ashuri, Maziar; Liu, Caihong; Shaw, Leon L.] IIT, Dept Mech Mat & Aerosp Engn, Chicago, IL 60616 USA. [Liu, Yuzi] Argonne Natl Lab, Ctr Nanoscale Mat, Argonne, IL 60439 USA. RP Chen, L (reprint author), Wanger Inst Sustainable Energy Res, Chicago, IL 60616 USA. EM lshaw2@iit.edu RI Ashuri, Maziar/K-3413-2015; Liu, Caihong/I-3222-2014; Liu, Yuzi/C-6849-2011 OI Ashuri, Maziar/0000-0001-8610-1643; Liu, Caihong/0000-0002-8582-912X; FU U. S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-AC02-06CH11357] FX The use of the Center for Nanoscale Materials was supported by the U. S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract no. DE-AC02-06CH11357. The authors also would like to thank Jose Orozco for training of multiply instruments at IIT, Dr Nancy L. Dietz Rago for FESEM training at ANL, and Dr Xiao-min Lin at ANL for offering us the Gatan vacuum transfer holder for EFTEM measurement. NR 39 TC 33 Z9 33 U1 8 U2 135 PU ROYAL SOC CHEMISTRY PI CAMBRIDGE PA THOMAS GRAHAM HOUSE, SCIENCE PARK, MILTON RD, CAMBRIDGE CB4 0WF, CAMBS, ENGLAND SN 2050-7488 EI 2050-7496 J9 J MATER CHEM A JI J. Mater. Chem. A PD NOV 14 PY 2014 VL 2 IS 42 BP 18026 EP 18032 DI 10.1039/c4ta04103h PG 7 WC Chemistry, Physical; Energy & Fuels; Materials Science, Multidisciplinary SC Chemistry; Energy & Fuels; Materials Science GA AS0IO UT WOS:000343961300041 ER PT J AU Velasco-Velez, JJ Wu, CH Pascal, TA Wan, LWF Guo, JH Prendergast, D Salmeron, M AF Velasco-Velez, Juan-Jesus Wu, Cheng Hao Pascal, Tod A. Wan, Liwen F. Guo, Jinghua Prendergast, David Salmeron, Miquel TI The structure of interfacial water on gold electrodes studied by x-ray absorption spectroscopy SO SCIENCE LA English DT Article ID FREQUENCY VIBRATIONAL SPECTROSCOPY; AU(111) SURFACE; MOLECULES; ADSORPTION; RU(0001); FORCE; LAYER AB The molecular structure of the electrical double layer determines the chemistry in all electrochemical processes. Using x-ray absorption spectroscopy (XAS), we probed the structure of water near gold electrodes and its bias dependence. Electron yield XAS detected at the gold electrode revealed that the interfacial water molecules have a different structure from those in the bulk. First principles calculations revealed that similar to 50% of the molecules lie flat on the surface with saturated hydrogen bonds and another substantial fraction with broken hydrogen bonds that do not contribute to the XAS spectrum because their core-excited states are delocalized by coupling with the gold substrate. At negative bias, the population of flat-lying molecules with broken hydrogen bonds increases, producing a spectrum similar to that of bulk water. C1 [Velasco-Velez, Juan-Jesus; Wu, Cheng Hao; Salmeron, Miquel] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA. [Wu, Cheng Hao] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA. [Pascal, Tod A.; Wan, Liwen F.; Prendergast, David] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Mol Foundry, Joint Ctr Energy Storage Res, Berkeley, CA 94720 USA. [Guo, Jinghua] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94720 USA. [Guo, Jinghua] Univ Calif Santa Cruz, Dept Chem & Biochem, Santa Cruz, CA 95064 USA. [Salmeron, Miquel] Univ Calif Berkeley, Dept Mat Sci & Engn, Berkeley, CA 94720 USA. RP Salmeron, M (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA. EM mbsalmeron@lbl.gov RI Wu, Cheng Hao/C-9565-2014; Foundry, Molecular/G-9968-2014 FU Office of Basic Energy Sciences (BES), Division of Materials Sciences and Engineering, of the U.S. Department of Energy (DOE) [DE-AC02-05CH11231]; Alexander von Humboldt Foundation, Germany; Joint Center for Energy Storage Research, an Energy Innovation Hub - U.S. DOE; DOE-BES; DOE-Advanced Scientific Computing Research; DOE Office of Science [DE-AC02-05CH11231] FX This work was supported by the Office of Basic Energy Sciences (BES), Division of Materials Sciences and Engineering, of the U.S. Department of Energy (DOE) under contract no. DE-AC02-05CH11231 (through the Chemical and Mechanical Properties of Surfaces, Interfaces and Nanostructures program). J.-J.V.-V. acknowledges financial support from the Alexander von Humboldt Foundation, Germany. C.H.W. acknowledges the Advanced Light Source (ALS) Doctoral Fellowship in Residence. Theory and simulations by T.A.P., L.F.W., and D.P. were supported by the Joint Center for Energy Storage Research, an Energy Innovation Hub funded by the U.S. DOE and facilitated by a user project at the Molecular Foundry. Computations were performed with the computing resources of the National Energy Research Scientific Computing Center (NERSC). The ALS and Molecular Foundry (supported by DOE-BES) and NERSC (supported by DOE-Advanced Scientific Computing Research) are DOE Office of Science User Facilities, supported by the DOE Office of Science under contract no. DE-AC02-05CH11231. We thank C.-H. Chuang, B.-Y. Wang, D. Zhang, X. Feng, and M. W. West for support at the beamline. We also thank J. Zhang for help with AFM imaging and C. Das Pemmaraju, C. Schwartz, P. Ross, J. Colchero, G. Thornton, H. Fang, and S. Harris for useful discussions. NR 34 TC 55 Z9 56 U1 24 U2 193 PU AMER ASSOC ADVANCEMENT SCIENCE PI WASHINGTON PA 1200 NEW YORK AVE, NW, WASHINGTON, DC 20005 USA SN 0036-8075 EI 1095-9203 J9 SCIENCE JI Science PD NOV 14 PY 2014 VL 346 IS 6211 BP 831 EP 834 DI 10.1126/science.1259437 PG 4 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AT0YL UT WOS:000344659900039 PM 25342657 ER PT J AU Romps, DM Seeley, JT Vollaro, D Molinari, J AF Romps, David M. Seeley, Jacob T. Vollaro, David Molinari, John TI Projected increase in lightning strikes in the United States due to global warming SO SCIENCE LA English DT Article ID CLIMATE-CHANGE; CONVECTIVE RAINFALL; PRECIPITATION; DISTRIBUTIONS; FREQUENCY; PARAMETERIZATION; RADAR; FIRE; NOX AB Lightning plays an important role in atmospheric chemistry and in the initiation of wildfires, but the impact of global warming on lightning rates is poorly constrained. Here we propose that the lightning flash rate is proportional to the convective available potential energy (CAPE) times the precipitation rate. Using observations, the product of CAPE and precipitation explains 77% of the variance in the time series of total cloud-toground lightning flashes over the contiguous United States (CONUS). Storms convert CAPE times precipitated water mass to discharged lightning energy with an efficiency of 1%. When this proxy is applied to 11 climate models, CONUS lightning strikes are predicted to increase 12 +/- 5% per degree Celsius of global warming and about 50% over this century. C1 [Romps, David M.; Seeley, Jacob T.] Univ Calif Berkeley, Dept Earth & Planetary Sci, Berkeley, CA 94720 USA. [Romps, David M.; Seeley, Jacob T.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Earth Sci, Berkeley, CA 94720 USA. [Vollaro, David; Molinari, John] SUNY Albany, Dept Atmospher & Environm Sci, Albany, NY 12222 USA. RP Romps, DM (reprint author), Univ Calif Berkeley, Dept Earth & Planetary Sci, Berkeley, CA 94720 USA. EM romps@berkeley.edu RI Romps, David/F-8285-2011; OI Seeley, Jacob/0000-0003-0769-292X FU Scientific Discovery through Advanced Computing (SciDAC) program - U.S. Department of Energy Office of Advanced Scientific Computing Research and Office of Biological and Environmental Research; U.S. Department of Energy's Earth System Modeling, an Office of Science, Office of Biological and Environmental Research program [DE-AC02-05CH11231]; National Science Foundation (NSF) Graduate Research Fellowship [DGE1106400]; NSF [AGS1132576] FX D.M.R. acknowledges support from the Scientific Discovery through Advanced Computing (SciDAC) program funded by the U.S. Department of Energy Office of Advanced Scientific Computing Research and Office of Biological and Environmental Research, and by the U.S. Department of Energy's Earth System Modeling, an Office of Science, Office of Biological and Environmental Research program under contract no. DE-AC02-05CH11231. J.T.S. acknowledges support from the National Science Foundation (NSF) Graduate Research Fellowship under grant no. DGE1106400. D.V. and J.M. acknowledge support from NSF under grant no. AGS1132576. Thanks are due to the SPARC data center for archiving the high-resolution radiosonde data and making them publicly available. The authors are also grateful to J. Paul, B. Lawrence, K. Sugioka, and N. Jeevanjee for their help with the precipitation data. Thanks also to three anonymous reviewers. Data sources are described in the online supplementary materials. NR 38 TC 51 Z9 51 U1 7 U2 89 PU AMER ASSOC ADVANCEMENT SCIENCE PI WASHINGTON PA 1200 NEW YORK AVE, NW, WASHINGTON, DC 20005 USA SN 0036-8075 EI 1095-9203 J9 SCIENCE JI Science PD NOV 14 PY 2014 VL 346 IS 6211 BP 851 EP 854 DI 10.1126/science.1259100 PG 4 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AT0YL UT WOS:000344659900045 PM 25395536 ER PT J AU Agakishiev, G Arnold, O Belver, D Belyaev, A Berger-Chen, JC Blanco, A Bohmer, M Boyard, JL Cabanelas, P Chernenko, S Dybczak, A Epple, E Fabbietti, L Fateev, O Finocchiaro, P Fonte, P Friese, J Frohlich, I Galatyuk, T Garzon, JA Gernhauser, R Gobel, K Golubeva, M Gonzalez-Diaz, D Guber, F Gumbcridzc, M Hcinz, T Hcnnino, T Holzmann, R Icrusalimov, A Iori, I Ivashkin, A Jurkovic, M Kampfer, B Karavicheva, T Koenig, I Koenig, W Kolb, BW Korcyl, G Kornakov, G Kotte, R Krasa, A Krizek, F Krucken, R Kuc, H Kuhn, W Kugler, A Kunz, T Kurepin, A Ladygin, V Lalik, R Lapidus, K Lebedev, A Lopes, L Lorenz, M Maier, L Mangiarotti, A Markert, J Metag, V Michel, J Muntz, C Munzer, R Naumann, L Pachmayer, YC Palka, M Parpottas, Y Pechenov, V Pechenova, O Pietraszko, J Przygoda, W Ramstein, B Reshetin, A Rustamov, A Sadovsky, A Salabura, P Schmah, A Schwab, E Siebenson, J Sobolev, YG Spruck, B Strobele, II Stroth, J Sturm, C Tarantola, A Teilab, K Tlusty, P Traxler, M Tsertos, H Vasiliev, T Wagner, V Weber, M Wendisch, C Wustenfeld, J Yurevich, S Zanevsky, Y Gaitanos, T Weil, J AF Agakishiev, G. Arnold, O. Belver, D. Belyaev, A. Berger-Chen, J. C. Blanco, A. Boehmer, M. Boyard, J. L. Cabanelas, P. Chernenko, S. Dybczak, A. Epple, E. Fabbietti, L. Fateev, O. Finocchiaro, P. Fonte, P. Friese, J. Froehlich, I. Galatyuk, T. Garzon, J. A. Gernhaeuser, R. Goebel, K. Golubeva, M. Gonzalez-Diaz, D. Guber, F. Gumbcridzc, M. Hcinz, T. Hcnnino, T. Holzmann, R. Icrusalimov, A. Iori, I. Ivashkin, A. Jurkovic, M. Kaempfer, B. Karavicheva, T. Koenig, I. Koenig, W. Kolb, B. W. Korcyl, G. Kornakov, G. Kotte, R. Krasa, A. Krizek, F. Kruecken, R. Kuc, H. Kuehn, W. Kugler, A. Kunz, T. Kurepin, A. Ladygin, V. Lalik, R. Lapidus, K. Lebedev, A. Lopes, L. Lorenz, M. Maier, L. Mangiarotti, A. Markert, J. Metag, V. Michel, J. Muentz, C. Muenzer, R. Naumann, L. Pachmayer, Y. C. Palka, M. Parpottas, Y. Pechenov, V. Pechenova, O. Pietraszko, J. Przygoda, W. Ramstein, B. Reshetin, A. Rustamov, A. Sadovsky, A. Salabura, P. Schmah, A. Schwab, E. Siebenson, J. Sobolev, Yu. G. Spruck, B. Stroebele, I. I. Stroth, J. Sturm, C. Tarantola, A. Teilab, K. Tlusty, P. Traxler, M. Tsertos, H. Vasiliev, T. Wagner, V. Weber, M. Wendisch, C. Wuestenfeld, J. Yurevich, S. Zanevsky, Y. Gaitanos, T. Weil, J. CA HADES Collaboration TI Medium effects in proton-induced K-0 production at 3.5 GeV SO PHYSICAL REVIEW C LA English DT Article ID HEAVY-ION COLLISIONS; STRANGE-PARTICLE PRODUCTION; K+-NUCLEUS SCATTERING; KAON PRODUCTION; P COLLISIONS; BEAM ENERGY; MATTER; CONDENSATION; MESONS; FLOW AB We present the analysis of the inclusive K-0 production in p + p and p + Nb collisions measured with the HADES detector (GSI Helmholtzzentrum for Heavy-Ion Research, Darmstadt) at a beam kinetic energy of 3.5 GeV. Data are compared to the Giessen Boltzmann-Uehling-Uhlenbeck (GiBUU) transport model. The data suggest the presence of a repulsive momentum-dependent kaon potential as predicted by the chiral perturbation theory (ChPT). For the kaon at rest and at normal nuclear density, the ChPT potential amounts to approximate to 35 MeV. A detailed tuning of the kaon production cross sections implemented in the model has been carried out to reproduce the experimental data measured in p + p collisions. The uncertainties in the parameters of the model were examined with respect to the sensitivity of the experimental results from p + Nb collisions to the in-medium kaon potential. C1 [Agakishiev, G.; Belyaev, A.; Chernenko, S.; Fateev, O.; Icrusalimov, A.; Ladygin, V.; Vasiliev, T.; Zanevsky, Y.] Joint Inst Nucl Res, Dubna 141980, Russia. [Arnold, O.; Berger-Chen, J. C.; Boehmer, M.; Epple, E.; Fabbietti, L.; Friese, J.; Gernhaeuser, R.; Jurkovic, M.; Kruecken, R.; Kunz, T.; Lalik, R.; Lapidus, K.; Maier, L.; Muenzer, R.; Siebenson, J.; Weber, M.] Tech Univ Munich, Dept Phys E12, D-85748 Garching, Germany. [Arnold, O.; Berger-Chen, J. C.; Epple, E.; Fabbietti, L.; Lalik, R.; Lapidus, K.; Muenzer, R.; Siebenson, J.] Origin & Struct Univ, Excellence Cluster, D-85748 Garching, Germany. [Belver, D.; Cabanelas, P.; Garzon, J. A.] Univ Santiago, Fac Fis, LabCAF, Santiago De Compostela 15706, Spain. [Blanco, A.; Fonte, P.; Lopes, L.; Mangiarotti, A.] LIP, Lab Instrumentacao & Fis Expt Particulas, P-3004516 Coimbra, Portugal. [Boyard, J. L.; Hcnnino, T.; Kuc, H.; Ramstein, B.] Univ Paris 11, CNRS IN2P3, UMR 8608, Inst Phys Nucl, F-91406 Orsay, France. [Dybczak, A.; Korcyl, G.; Kuc, H.; Palka, M.; Przygoda, W.; Salabura, P.] Jagiellonian Univ, Smoluchowski Inst Phys, PL-30059 Krakow, Poland. [Finocchiaro, P.] Ist Nazl Fis Nucl, Lab Nazl Sud, I-95125 Catania, Italy. [Froehlich, I.; Goebel, K.; Lorenz, M.; Markert, J.; Michel, J.; Muentz, C.; Pachmayer, Y. C.; Pechenova, O.; Rustamov, A.; Stroebele, I. I.; Tarantola, A.; Teilab, K.] Goethe Univ, Inst Kernphys, D-60438 Frankfurt, Germany. [Galatyuk, T.; Gonzalez-Diaz, D.; Gumbcridzc, M.; Kornakov, G.] Tech Univ Darmstadt, D-64289 Darmstadt, Germany. [Golubeva, M.; Guber, F.; Ivashkin, A.; Karavicheva, T.; Kurepin, A.; Reshetin, A.; Sadovsky, A.] Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia. [Hcinz, T.; Holzmann, R.; Koenig, I.; Koenig, W.; Kolb, B. W.; Pechenov, V.; Pietraszko, J.; Schwab, E.; Stroth, J.; Sturm, C.; Traxler, M.; Yurevich, S.] GSI Helmholtzzentrum Schwerionenforsch, GmbH, D-64291 Darmstadt, Germany. [Iori, I.] Ist Nazl Fis Nucl, Sez Milano, I-20133 Milan, Italy. [Kaempfer, B.; Kotte, R.; Wendisch, C.; Wuestenfeld, J.] Helmholtz Zentrum Dresden Rossendorf, Inst Strahlenphys, D-01314 Dresden, Germany. [Krasa, A.; Krizek, F.; Kugler, A.; Sobolev, Yu. G.; Tlusty, P.; Wagner, V.] Acad Sci Czech Republic, Inst Nucl Phys, CZ-25068 Rez, Czech Republic. [Kuehn, W.; Metag, V.; Spruck, B.] Univ Giessen, Inst Phys 2, D-35392 Giessen, Germany. [Lebedev, A.] Inst Theoret & Expt Phys, Moscow 117218, Russia. [Parpottas, Y.; Tsertos, H.] Univ Cyprus, Dept Phys, CY-1678 Nicosia, Cyprus. [Schmah, A.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Gaitanos, T.] Inst Theoret Phys I, D-35392 Giessen, Germany. [Weil, J.] Frankfurt Inst Adv Studies, D-60438 Frankfurt, Germany. [Fonte, P.] ISEC Coimbra, Coimbra, Portugal. [Galatyuk, T.; Gumbcridzc, M.] EMMI, ExtreMe Matter Inst, D-64291 Darmstadt, Germany. [Galatyuk, T.; Gumbcridzc, M.] Univ Milan, Dipartimento Fis, I-20133 Milan, Italy. [Kaempfer, B.; Wendisch, C.] Tech Univ Dresden, D-01062 Dresden, Germany. [Parpottas, Y.] Frederick Univ, CY-1036 Nicosia, Cyprus. RP Lapidus, K (reprint author), Tech Univ Munich, Dept Phys E12, D-85748 Garching, Germany. EM kirill.lapidus@ph.tum.de RI Mangiarotti, Alessio/I-1072-2012; Kruecken, Reiner/A-1640-2013; Blanco, Alberto/L-2520-2014; Guber, Fedor/I-4271-2013; Fonte, Paulo/B-1842-2008; Gonzalez Diaz, Diego/K-7265-2014; Cabanelas, Pablo/B-2034-2016; Gobel, Kathrin/B-8531-2016; Kurepin, Alexey/H-4852-2013 OI Tsertos, Charalambos/0000-0001-5966-343X; Finocchiaro, Paolo/0000-0001-7502-2229; Mangiarotti, Alessio/0000-0001-7837-6057; Kruecken, Reiner/0000-0002-2755-8042; Guber, Fedor/0000-0001-8790-3218; Fonte, Paulo/0000-0002-2275-9099; Weil, Janus/0000-0003-1218-0574; Blanco, Alberto/0000-0001-9827-8294; Gonzalez Diaz, Diego/0000-0002-6809-5996; Cabanelas, Pablo/0000-0002-5416-4647; Gobel, Kathrin/0000-0003-2832-8465; Kurepin, Alexey/0000-0002-1851-4136 FU LIP Coimbra, Coimbra (Portugal) [PTDC/FIS/113339/2009]; SIP JUC Cracow, Cracow (Poland) [NN202286038, NN202198639]; HZ Dresden-Rossendorf (HZDR), Dresden (Germany) [BMBF 06DR9059D]; TU Munchen, Garching (Germany) FX The HADES Collaboration gratefully acknowledges support by the grants LIP Coimbra, Coimbra (Portugal): PTDC/FIS/113339/2009; SIP JUC Cracow, Cracow (Poland): NN202286038 28-JAN-2010 and NN202198639 01-OCT-2010; HZ Dresden-Rossendorf (HZDR), Dresden (Germany): BMBF 06DR9059D; TU Munchen, Garching (Germany): MLL Munchen, DFG EClust 153, VH-NG-330, BMBF 06MT9156 TP5, GSI TMKrue 1012; NPI AS CR, Rez, Rez (Czech Republic): MSMT LC07050, GAASCR IAA100480803; USC S. de Compostela, Santiago de Compostela (Spain): CPAN:CSD2007-00042; Goethe University, Frankfurt (Germany): HA216/EMMI HIC for FAIR (LOEWE), BMBF:06FY9100I, GSI F&E EU Contract No. HP3-283286. NR 61 TC 7 Z9 7 U1 0 U2 8 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0556-2813 EI 1089-490X J9 PHYS REV C JI Phys. Rev. C PD NOV 13 PY 2014 VL 90 IS 5 AR UNSP 054906 DI 10.1103/PhysRevC.90.054906 PG 12 WC Physics, Nuclear SC Physics GA CA2WR UT WOS:000348766900004 ER PT J AU Tkachenko, S Dutta, D Ent, R Ispiryan, M AF Tkachenko, S. Dutta, D. Ent, R. Ispiryan, M. CA CLAS Collaboration TI Measurement of the structure function of the nearly free neutron using spectator tagging in inelastic H-2(e, e' p(s)) X scattering with CLAS (vol 89, 045206, 2014) SO PHYSICAL REVIEW C LA English DT Correction C1 [Dutta, D.] Mississippi State Univ, Mississippi State, MS 39762 USA. [Ent, R.] Thomas Jefferson Natl Accelerator Facil, Newport News, VA 23606 USA. [Ispiryan, M.] Univ Houston, Houston, TX 77004 USA. NR 1 TC 0 Z9 0 U1 0 U2 0 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0556-2813 EI 1089-490X J9 PHYS REV C JI Phys. Rev. C PD NOV 13 PY 2014 VL 90 IS 5 AR 059901 DI 10.1103/PhysRevC.90.059901 PG 1 WC Physics, Nuclear SC Physics GA CA2WR UT WOS:000348766900007 ER PT J AU Wu, JJ Lee, TSH Thomas, AW Young, RD AF Wu, Jia-Jun Lee, T. -S. H. Thomas, A. W. Young, R. D. TI Finite-volume Hamiltonian method for coupled-channels interactions in lattice QCD SO PHYSICAL REVIEW C LA English DT Article ID NUCLEON RESONANCE REGION; MESON PRODUCTION; BAG MODEL; STATES AB Within a multichannel formulation of pp scattering, we investigate the use of the finite-volume Hamiltonian approach to resolve scattering observables from lattice QCD spectra. The asymptotic matching of the well-known Luscher formalism encodes a unique finite-volume spectrum. Nevertheless, in many practical situations, such as coupled-channels systems, it is advantageous to interpolate isolated lattice spectra in order to extract physical scattering parameters. Here we study the use of the Hamiltonian framework as a parametrization that can be fit directly to lattice spectra. We find that, with a modest amount of lattice data, the scattering parameters can be reproduced rather well, with only a minor degree of model dependence. C1 [Wu, Jia-Jun; Lee, T. -S. H.] Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA. [Thomas, A. W.; Young, R. D.] Univ Adelaide, Spec Res Ctr Subatom Struct Matter CSSM, Sch Chem & Phys, Adelaide, SA 5005, Australia. [Thomas, A. W.; Young, R. D.] Univ Adelaide, ARC, Ctr Excellence Particle Phys Terascale, Sch Chem & Phys, Adelaide, SA 5005, Australia. RP Wu, JJ (reprint author), Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA. RI Thomas, Anthony/G-4194-2012 OI Thomas, Anthony/0000-0003-0026-499X FU U.S. Department of Energy, Office of Nuclear Physics Division [DE-AC02-06CH11357]; Office of Science of the U.S. Department of Energy [DE-AC02-05CH11231]; University of Adelaide; Australian Research Council through the ARC Centre of Excellence for Particle Physics at the Terascale [FL0992247, DP140103067, FT120100821] FX We wish to thank Raul Briceno for helpful correspondence. This work is supported by the U.S. Department of Energy, Office of Nuclear Physics Division, under Contract No. DE-AC02-06CH11357. This research used resources of the National Energy Research Scientific Computing Center, which is supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231, and resources provided on the Fusion, 320-node computing cluster operated by the Laboratory Computing Resource Center at Argonne National Laboratory. This work was also supported by the University of Adelaide and the Australian Research Council through the ARC Centre of Excellence for Particle Physics at the Terascale and Grants No. FL0992247 (AWT), No. DP140103067, and No. FT120100821 (RDY). NR 44 TC 11 Z9 11 U1 0 U2 2 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0556-2813 EI 1089-490X J9 PHYS REV C JI Phys. Rev. C PD NOV 13 PY 2014 VL 90 IS 5 AR 055206 DI 10.1103/PhysRevC.90.055206 PG 14 WC Physics, Nuclear SC Physics GA CA2WR UT WOS:000348766900006 ER PT J AU Sun, YP Emma, P Raubenheimer, T Wu, JH AF Sun, Yipeng Emma, Paul Raubenheimer, Tor Wu, Juhao TI X-band rf driven free electron laser driver with optics linearization SO PHYSICAL REVIEW SPECIAL TOPICS-ACCELERATORS AND BEAMS LA English DT Article ID OPERATION AB In this paper, a compact hard X-ray free electron lasers (FEL) design is proposed with all X-band rf acceleration and two stage bunch compression. It eliminates the need of a harmonic rf linearization section by employing optics linearization in its first stage bunch compression. Quadrupoles and sextupoles are employed in a bunch compressor one (BC1) design, in such a way that second order longitudinal dispersion of BC1 cancels the second order energy correlation in the electron beam. Start-to-end 6-D simulations are performed with all the collective effects included. Emittance growth in the horizontal plane due to coherent synchrotron radiation is investigated and minimized, to be on a similar level with the successfully operating Linac coherent light source (LCLS). At a FEL radiation wavelength of 0.15 nm, a saturation length of 40 meters can be achieved by employing an undulator with a period of 1.5 cm. Without tapering, a FEL radiation power above 10 GW is achieved with a photon pulse length of 50 fs, which is LCLS-like performance. The overall length of the accelerator plus undulator is around 250 meters which is much shorter than the LCLS length of 1230 meters. That makes it possible to build hard X-ray FEL in a laboratory with limited size. C1 [Emma, Paul; Raubenheimer, Tor; Wu, Juhao] SLAC Natl Accelerator Lab, Menlo Pk, CA 94025 USA. [Sun, Yipeng] Argonne Natl Lab, Argonne, IL 60439 USA. RP Sun, YP (reprint author), Argonne Natl Lab, 9700 S Cass Ave, Argonne, IL 60439 USA. EM yisun@aps.anl.gov FU U.S. Department of Energy, Office of Science [DE-AC02-06CH11357]; U.S. Department of Energy [DE-AC02-76SF00515] FX Most of the work was done at SLAC National Accelerator Laboratory. The paper was finished at Argonne National Laboratory. Work supported by the U.S. Department of Energy, Office of Science, under Contract No. DE-AC02-06CH11357. Work also supported by the U.S. Department of Energy under Contract DE-AC02-76SF00515. The authors would like to thank M. Woodley, A. Chao, Z. Huang, C. Adolphsen, Y. Ding, C. Limborg-Deprey for helpful discussions, C. Adolphsen for the proofreading. NR 31 TC 0 Z9 0 U1 3 U2 6 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1098-4402 J9 PHYS REV SPEC TOP-AC JI Phys. Rev. Spec. Top.-Accel. Beams PD NOV 13 PY 2014 VL 17 IS 11 AR 110703 DI 10.1103/PhysRevSTAB.17.110703 PG 12 WC Physics, Nuclear; Physics, Particles & Fields SC Physics GA CA2XS UT WOS:000348770000001 ER PT J AU Croken, MM Ma, YF Markillie, LM Taylor, RC Orr, G Weiss, LM Kim, K AF Croken, Matthew McKnight Ma, Yanfen Markillie, Lye Meng Taylor, Ronald C. Orr, Galya Weiss, Louis M. Kim, Kami TI Distinct Strains of Toxoplasma gondii Feature Divergent Transcriptomes Regardless of Developmental Stage SO PLOS ONE LA English DT Article ID GENE-EXPRESSION; RNA-SEQ; PSEUDOKINASES; VIRULENCE; PARASITES; DATABASE; FAMILY; CYST AB Using high through-put RNA sequencing, we assayed the transcriptomes of three different strains of Toxoplasma gondii representing three common genotypes under both in vitro tachyzoite and in vitro bradyzoite-inducing alkaline stress culture conditions. Strikingly, the differences in transcriptional profiles between the strains, RH, PLK, and CTG, is much greater than differences between tachyzoites and alkaline stressed in vitro bradyzoites. With an FDR of 10%, we identified 241 genes differentially expressed between CTG tachyzoites and in vitro bradyzoites, including 5 putative AP2 transcription factors. We also observed a close association between cell cycle regulated genes and differentiation. By Gene Set Enrichment Analysis (GSEA), there are a number of KEGG pathways associated with the in vitro bradyzoite transcriptomes of PLK and CTG, including pyrimidine metabolism and DNA replication. These functions are likely associated with cell-cycle arrest. When comparing mRNA levels between strains, we identified 1,526 genes that were differentially expressed regardless of culture-condition as well as 846 differentially expressed only in bradyzoites and 542 differentially expressed only in tachyzoites between at least two strains. Using GSEA, we identified that ribosomal proteins were expressed at significantly higher levels in the CTG strain than in either the RH or PLK strains. This association holds true regardless of life cycle stage. C1 [Croken, Matthew McKnight; Kim, Kami] Albert Einstein Coll Med, Dept Microbiol & Immunol, Bronx, NY 10467 USA. [Ma, Yanfen; Weiss, Louis M.; Kim, Kami] Albert Einstein Coll Med, Dept Pathol, Bronx, NY 10467 USA. [Markillie, Lye Meng; Orr, Galya] Pacific NW Natl Lab, Environm Mol Sci Lab, Richland, WA 99352 USA. [Taylor, Ronald C.] Pacific NW Natl Lab, Div Biol Sci, Computat Biol & Bioinformat Grp, Richland, WA 99352 USA. [Weiss, Louis M.; Kim, Kami] Albert Einstein Coll Med, Dept Med, Bronx, NY 10467 USA. RP Weiss, LM (reprint author), Albert Einstein Coll Med, Dept Pathol, Bronx, NY 10467 USA. EM louis.weiss@einstein.yu.edu; kami.kim@einstein.yu.edu OI Taylor, Ronald/0000-0001-9777-9767; Kim, Kami/0000-0003-3384-152X FU National Institutes of Health (NIH) [AI095094] FX Research was supported by National Institutes of Health (NIH) grants AI095094 (LMW), AI087625 (KK), and by grant 40070 (LMW) from Environmental Molecular Sciences Laboratory (EMSL) Pacific Northwest National Laboratory. MMC was supported by the Training Program in Cellular and Molecular Biology and Genetics, funded by NIH T32 GM007491 awarded to the Albert Einstein College of Medicine. A portion of the research was performed using EMSL, a national scientific user facility sponsored by the Department of Energy's Office of Biological and Environmental Research and located at Pacific Northwest National Lab. This work was also supported in part by the Center for AIDS Research at the Albert Einstein College of Medicine and Montefiore Medical Center funded by the National Institutes of Health (NIH AI-051519). The funders had no role in study design, data collection and analysis, decision to publish, or preparation of the manuscript. NR 34 TC 5 Z9 5 U1 1 U2 9 PU PUBLIC LIBRARY SCIENCE PI SAN FRANCISCO PA 1160 BATTERY STREET, STE 100, SAN FRANCISCO, CA 94111 USA SN 1932-6203 J9 PLOS ONE JI PLoS One PD NOV 13 PY 2014 VL 9 IS 11 AR e111297 DI 10.1371/journal.pone.0111297 PG 10 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AY6YT UT WOS:000347709300014 PM 25393307 ER PT J AU Soler, MA Nelson, T Roitberg, AE Tretiak, S Femandez-Alberti, S AF Soler, Miguel A. Nelson, Tarnmie Roitberg, Adrian E. Tretiak, Sergei Femandez-Alberti, Sebastian TI Signature of Nonadiabatic Coupling in Excited-State Vibrational Modes SO JOURNAL OF PHYSICAL CHEMISTRY A LA English DT Article ID UNIDIRECTIONAL ENERGY-TRANSFER; CONICAL INTERSECTIONS; CONJUGATED MOLECULES; ELECTRONIC COHERENCE; EXCITONIC COUPLINGS; QUANTUM-CHEMISTRY; EMISSION-SPECTRA; DYNAMICS; ABSORPTION; SIMULATION AB Using analytical excited-state gradients, vibrational normal modes have been calculated at the minimum of the electronic excited-state potential energy surfaces for a set of extended conjugated molecules with different coupling between them. Molecular model systems composed of units of polyphenylene ethynylene (PPE), polyphenylenevinylene (PPV), and naphthacene/pentacene (NP) have been considered. In all cases except the NP model, the influence of the nonadiabatic coupling on the excited-state equilibrium normal modes is revealed as a unique highest frequency adiabatic vibrational mode that overlaps with the coupling vector. This feature is removed by using a locally diabatic representation in which the effect of NA interaction is removed. Comparison of the original adiabatic modes with a set of vibrational modes computed in the locally diabatic representation demonstrates that the effect of nonadiabaticity is confined to only a few modes. This suggests that the nonadiabatic character of a molecular system may be detected spectroscopically by identifying these unique state-specific high frequency vibrational modes. C1 [Soler, Miguel A.; Femandez-Alberti, Sebastian] Univ Nacl Quilmes, Bernal, Argentina. [Nelson, Tarnmie; Tretiak, Sergei] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA. [Roitberg, Adrian E.] Univ Florida, Dept Chem, Quantum Theory Project, Gainesville, FL 32611 USA. RP Tretiak, S (reprint author), Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA. EM serg@lanl.gov; sfalberti@gmail.com RI Tretiak, Sergei/B-5556-2009; OI Tretiak, Sergei/0000-0001-5547-3647; SOLER, MIGUEL/0000-0002-5780-9949 FU CONICET; UNQ; ANPCyT [PICT-2010-2375]; National Science Foundation [CHE-0239129, CHE-0808910]; U.S. Department of Energy; Los Alamos LDRD; National Nuclear Security Administration of the U.S. Department of Energy [DE-AC5206NA25396]; Center for Integrated Nanotechnologies (CINT); Center for Nonlinear Studies (CNLS) at LANL FX This work was partially supported by CONICET, UNQ, ANPCyT (PICT-2010-2375), National Science Foundation Grant No. CHE-0239129 and CHE-0808910, and U.S. Department of Energy and Los Alamos LDRD funds. Los Alamos National Laboratory is operated by Los Alamos National Security, LLC, for the National Nuclear Security Administration of the U.S. Department of Energy under contract DE-AC5206NA25396. The authors acknowledge support from the Center for Integrated Nanotechnologies (CINT) and the Center for Nonlinear Studies (CNLS) at LANL. NR 59 TC 5 Z9 5 U1 0 U2 15 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1089-5639 J9 J PHYS CHEM A JI J. Phys. Chem. A PD NOV 13 PY 2014 VL 118 IS 45 BP 10372 EP 10379 DI 10.1021/jp503350k PG 8 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AT5IK UT WOS:000344976900011 PM 24844735 ER PT J AU Hong, J Jeon, S Kim, JJ Devi, D Chacon-Madrid, K Lee, W Koo, SM Wideman, J Sfeir, MY Peteanu, LA AF Hong, Jiyun Jeon, Sukyung Kim, Janice J. Devi, Diane Chacon-Madrid, Kelly Lee, Wynee Koo, Seung Moh Wideman, Jurjen Sfeir, Matthew Y. Peteanu, Linda A. TI The Effects of Side-Chain-Induced Disorder on the Emission Spectra and Quantum Yields of Oligothiophene Nanoaggregates: A Combined Experimental and MD-TDDFT Study SO JOURNAL OF PHYSICAL CHEMISTRY A LA English DT Article ID MOLECULAR-DYNAMICS SIMULATIONS; INTERCHAIN INTERACTIONS; ENERGY-TRANSFER; ALPHA-OLIGOTHIOPHENES; CHEMICAL CALCULATIONS; ELECTRONIC-STRUCTURES; COMPUTER EXPERIMENTS; CONJUGATED POLYMERS; PACKING STRUCTURES; OPTICAL-PROPERTIES AB Oligomeric thiophenes are commonly used components in organic electronics and solar cells. These molecules stack and/or aggregate readily under the processing conditions used to form thin films for these applications, significantly altering their optical and charge-transport properties. To determine how these effects depend on the substitution pattern of the thiophene main chains, nanoaggregates of three sexithiophene oligomers having different alkyl substitution patterns were formed using solvent-poisoning techniques and studied using steady-state and time-resolved emission spectroscopy. The results indicate the substantial role played by the side-chain substituents in determining the emissive properties of these species. Both the measured spectral changes and their dependence on substitution are well-modeled by combined quantum chemistry and molecular dynamics simulations. The simulations connect the side-chain-induced disorder, which determines the favorable chain-packing configurations within the aggregates, with their measured electronic spectra. C1 [Hong, Jiyun; Jeon, Sukyung; Kim, Janice J.; Devi, Diane; Chacon-Madrid, Kelly; Lee, Wynee; Koo, Seung Moh; Peteanu, Linda A.] Carnegie Mellon Univ, Dept Chem, Pittsburgh, PA 15213 USA. [Wideman, Jurjen] Zernike Inst Adv Mat Nijenborgh, NL-49747 AG Groningen, Netherlands. [Sfeir, Matthew Y.] Brookhaven Natl Lab, CFN, Upton, NY 11973 USA. RP Peteanu, LA (reprint author), Carnegie Mellon Univ, Dept Chem, 4400 Fifth Ave, Pittsburgh, PA 15213 USA. EM peteanu@cmu.edu RI Wen, Jin/G-6039-2014; OI Wen, Jin/0000-0001-6136-8771; Koo, Seung Moh/0000-0001-9331-4786; Sfeir, Matthew/0000-0001-5619-5722 FU NSF [CHE-1012529]; U.S. Department of Energy, Office of Basic Energy Sciences [DE-AC02-98CH10886]; National Natural Science Foundation of China [21290192, 21273102] FX L.A.P. acknowledges NSF (Grant CHE-1012529) for financial support. This work was performed in part at the Center for Functional Nanomaterials at Brookhaven National Laboratory, which is supported by the U.S. Department of Energy, Office of Basic Energy Sciences, under Contract DE-AC02-98CH10886. J.M. thanks the National Natural Science Foundation of China (Grants 21290192 and 21273102) for support and the High Performance Computing Center of Nanjing University for providing the IBM Blade cluster system. NR 55 TC 4 Z9 4 U1 2 U2 27 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1089-5639 J9 J PHYS CHEM A JI J. Phys. Chem. A PD NOV 13 PY 2014 VL 118 IS 45 BP 10464 EP 10473 DI 10.1021/jp504254a PG 10 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AT5IK UT WOS:000344976900021 PM 24992478 ER PT J AU Fransted, KA Jackson, NE Zong, R Mara, MW Huang, J Harpham, MR Shelby, ML Thununel, RP Chen, LX AF Fransted, Kelly A. Jackson, Nicholas E. Zong, Ruifa Mara, Michael W. Huang, Jier Harpham, Michael R. Shelby, Megan L. Thummel, Randolph P. Chen, Lin X. TI Ultrafast Structural Dynamics of Cu(I)-Bicinchoninic Acid and Their Implications for Solar Energy Applications SO JOURNAL OF PHYSICAL CHEMISTRY A LA English DT Article ID ABSORPTION FINE-STRUCTURE; COPPER(I) DIIMINE COMPLEXES; TRANSFER EXCITED-STATES; X-RAY; CU(NN)2+ SYSTEMS; CU(I) COMPLEXES; SPECTROSCOPY; CELLS; ELECTRON; HAMILTONIANS AB In this study, ultrafast optical transient absorption and X-ray transient absorption (XTA) spectroscopy are used to probe the excited-state dynamics and structural evolution of copper(I) bicinchoninic acid ([Cu(I)(BCA)(2)](+)), which has similar but less frequently studied biquinoline-based ligands compared to phenanthroline-based complexes. The optical transient absorption measurements performed on the complex in a series of polar protic solvents demonstrate a strong solvent dependency for the excited lifetime, which ranges from approximately 40 ps in water to over 300 ps in 2-methoxyethanol. The XTA experiments showed a reduction of the prominent 1s -> 4pz edge peak in the excited-state X-ray absorption near-edge structure (XANES) spectrum, which is indicative of an interaction with a fifth ligand, most likely the solvent. Analysis of the extended X-ray absorption fine structure (EXAFS) spectrum shows a shortening of the metal-ligand bond in the excited state and an increase in the coordination number for the Cu(II) metal center. A flattened structure is supported by DFT calculations that show that the system relaxes into a flattened geometry with a lowest-energy triplet state that has a dipole-forbidden transition to the ground state. While the short excited-state lifetime relative to previously studied Cu(I) diimine complexes could be attributed to this dark triplet state, the strong solvent dependency and the reduction of the 1s -> 4pz peak in the XTA data suggest that solvent interaction could also play a role. This detailed study of the dynamics in different solvents provides guidance for modulating excited-state pathways and lifetimes through structural factors such as solvent accessibility to fulfill the excited-state property requirements for efficient light harvesting and electron injection. C1 [Fransted, Kelly A.; Mara, Michael W.; Huang, Jier; Harpham, Michael R.; Shelby, Megan L.; Chen, Lin X.] Argonne Natl Lab, Chem Sci & Engn Div, Argonne, IL 60439 USA. [Jackson, Nicholas E.; Mara, Michael W.; Shelby, Megan L.; Chen, Lin X.] Northwestern Univ, Dept Chem, Evanston, IL 60439 USA. [Zong, Ruifa; Thummel, Randolph P.] Univ Houston, Dept Chem, Houston, TX 77204 USA. RP Thununel, RP (reprint author), Univ Houston, Dept Chem, 4800 Calhoun Rd, Houston, TX 77204 USA. EM thummel@uh.edu; Ichen@anl.gov FU Division of Chemical Sciences, Biosciences, Office of Basic Energy Sciences of the U.S. Department of Energy [DE-AC02-06CH11357, DE-FG02-07ER15888]; Robert A. Welch Foundation [E-621]; U.S. DOE [DE-AC02-06CH11357] FX We would like to acknowledge support from the Division of Chemical Sciences, Biosciences, Office of Basic Energy Sciences of the U.S. Department of Energy through Grant DE-AC02-06CH11357 (K.A.F. and L.X.C.), as well as DE-AC02-06CH11357 and DE-FG02-07ER15888 (R.Z. and R.P.T.) for support of this work. R.Z. and R.P.T. also thank the Robert A. Welch Foundation (Grant E-621). The authors would like to thank Dr. Xiaoyi Zhang of 11-ID-D at the Advanced Photon Source for her help with the XTA measurements. Use of beamline 11-ID-D at the Advanced Photon Source was supported by the U.S. DOE under Contract No. DE-AC02-06CH11357. The authors would also like to thank Dr. Dugan Hayes for his advice on experimental design. NR 60 TC 7 Z9 7 U1 4 U2 18 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1089-5639 J9 J PHYS CHEM A JI J. Phys. Chem. A PD NOV 13 PY 2014 VL 118 IS 45 BP 10497 EP 10506 DI 10.1021/jp504294j PG 10 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AT5IK UT WOS:000344976900024 PM 25015003 ER PT J AU Llansola-Portoles, MJ Bergkamp, JJ Finkelstein-Shapiro, D Sherman, BD Kodis, G Dimitrijevic, NM Gust, D Moore, TA Moore, AL AF Llansola-Portoles, Manuel J. Bergkamp, Jesse J. Finkelstein-Shapiro, Daniel Sherman, Benjamin D. Kodis, Gerdenis Dimitrijevic, Nada M. Gust, Devens Moore, Thomas A. Moore, Ana L. TI Controlling Surface Defects and Photophysics in TiO2 Nanoparticles SO JOURNAL OF PHYSICAL CHEMISTRY A LA English DT Article ID TITANIUM-DIOXIDE; SEMICONDUCTOR NANOCLUSTERS; PHOTOCATALYTIC REDUCTION; PARTICLES; SCIENCE; OXYGEN; EFFICIENCY; NANOTUBES; MOLECULES; STATES AB Titanium dioxide (TiO2) is widely used for photocatalysis and solar cell applications, and the electronic structure of bulk TiO2 is well understood. However, the surface structure of nanoparticulate TiO2, which has a key role in properties such as solubility and catalytic activity, still remains controversial. Detailed understanding of surface defect structures may help explain reactivity and overall materials performance in a wide range of applications. In this work we address the solubility problem and surface defects control on TiO2 nanoparticles. We report the synthesis and characterization of similar to 4 nm TiO2 anatase spherical nanoparticles that are soluble and stable in a wide range of organic solvents and water. By controlling the temperature during the synthesis, we are able to tailor the density of defect states on the surface of the TiO2 nanoparticles without affecting parameters such as size, shape, core crystallinity, and solubility. The morphology of both kinds of nanoparticles was determined by TEM. EPR experiments were used to characterize the surface defects, and transient absorption measurements demonstrate the influence of the TiO2 defect states on photoinduced electron transfer dynamics. C1 [Llansola-Portoles, Manuel J.; Bergkamp, Jesse J.; Finkelstein-Shapiro, Daniel; Sherman, Benjamin D.; Kodis, Gerdenis; Gust, Devens; Moore, Thomas A.; Moore, Ana L.] Arizona State Univ, Dept Chem & Biochem, Ctr Bioenergy & Photosynth, Tempe, AZ 85287 USA. [Dimitrijevic, Nada M.] Argonne Natl Lab, Chem Sci & Engn Div, Argonne, IL 60439 USA. [Dimitrijevic, Nada M.] Argonne Natl Lab, Ctr Nanoscale Mat, Argonne, IL 60439 USA. RP Llansola-Portoles, MJ (reprint author), Arizona State Univ, Dept Chem & Biochem, Ctr Bioenergy & Photosynth, Tempe, AZ 85287 USA. EM mjllansola@gmail.com OI Llansola-Portoles, Manuel Jose/0000-0002-8065-9459; Finkelstein Shapiro, Daniel/0000-0001-8015-5376 FU Center for Bio-Inspired Solar Fuel Production, an Energy Frontier Research Center - U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-SC0001016]; National Science Foundation [CHB-1124895]; Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-AC02-06CH11357] FX The work at ASU was supported by the Center for Bio-Inspired Solar Fuel Production, an Energy Frontier Research Center funded by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences under Award Number DE-SC0001016, National Science Foundation CHB-1124895, and the research at ANL was supported by the Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract No DE-AC02-06CH11357. NR 50 TC 7 Z9 7 U1 3 U2 51 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1089-5639 J9 J PHYS CHEM A JI J. Phys. Chem. A PD NOV 13 PY 2014 VL 118 IS 45 BP 10631 EP 10638 DI 10.1021/jp506284q PG 8 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AT5IK UT WOS:000344976900037 PM 25109403 ER PT J AU Pistner, AJ Pupillo, RC Yap, GPA Lutterman, DA Ma, YZ Rosenthal, J AF Pistner, Allen J. Pupillo, Rachel C. Yap, Glenn P. A. Lutterman, Daniel A. Ma, Ying-Zhong Rosenthal, Joel TI Electrochemical, Spectroscopic, and O-1(2) Sensitization Characteristics of 10,10-Dimethylbiladiene Complexes of Zinc and Copper SO JOURNAL OF PHYSICAL CHEMISTRY A LA English DT Article ID PHOTODYNAMIC THERAPY; LINEAR TETRAPYRROLES; COBALT COMPLEXES; ELECTRON-TRANSFER; PHOTOSENSITIZERS; PORPHYRIN; CHEMISTRY; OCTAETHYLBILINDIONE; LIGANDS; DENSITY AB The synthesis, electrochemistry, and photophysical characterization of a 10,10-dimethylbiladiene tetrapyrrole bearing ancillary pentafluorophenyl groups at the 5- and 15-meso positions (DMBil1) is presented. This nonmacrocyclic tetrapyrrole platform is robust and can serve as an excellent ligand scaffold for Zn2+ and Cu2+ centers. X-ray diffraction studies conducted for DMBil1 along with the corresponding Zn[DMBil1] and Cu[DMBil1] complexes show that this ligand scaffold binds a single metal ion within the tetrapyrrole core. Additionally, electrochemical experiments revealed that all three of the aforementioned compounds display an interesting redox chemistry as the DMBil1 framework can be both oxidized and reduced by two electrons. Spectroscopic and photophysical experiments carried out for DMBil1, Zn[DMBil1], and Cu[DMBil1] provide a basic picture of the electronic properties of these platforms. All three biladiene derivatives strongly absorb light in the visible region and are weakly emissive. The ability of these compounds to sensitize the formation of O-1(2) at wavelengths longer than 500 nm was probed. Both the free base and Zn2+ 10,10-dimethylbiladiene architectures show modest efficiencies for O-1(2) sensitization. The combination of structural, electrochemical, and photophysical data detailed herein provides a basis for the design of additional biladiene constructs for the activation of O-2 and other small molecules. C1 [Pistner, Allen J.; Pupillo, Rachel C.; Yap, Glenn P. A.; Rosenthal, Joel] Univ Delaware, Dept Chem & Biochem, Newark, DE 19716 USA. [Lutterman, Daniel A.; Ma, Ying-Zhong] Oak Ridge Natl Lab, Div Chem Sci, Oak Ridge, TN 37831 USA. RP Rosenthal, J (reprint author), Univ Delaware, Dept Chem & Biochem, Newark, DE 19716 USA. EM joelr@udel.edu RI Lutterman, Daniel/C-9704-2016; Ma, Yingzhong/L-6261-2016 OI Lutterman, Daniel/0000-0002-4875-6056; Ma, Yingzhong/0000-0002-8154-1006 FU American Chemical Society Petroleum Research Fund; NSF CAREER Award [CHE1352120]; U.S. Department of Energy, Office of Science, Basic Energy Sciences, Chemical Sciences, Geo-sciences, and Biosciences Division FX J.R. thanks Oak Ridge Associated Universities for a Ralph E. Powe Junior Faculty Enhancement Award. Additional financial support for this work was provided in part by the American Chemical Society Petroleum Research Fund and NSF CAREER Award CHE1352120. Work by D.A.L. and Y.-Z.M. was supported by the U.S. Department of Energy, Office of Science, Basic Energy Sciences, Chemical Sciences, Geo-sciences, and Biosciences Division. NMR and other data were acquired at UD using instrumentation obtained with assistance from the NSF and NIH (NSF MIR 0421224, NSF CRIF MU CHE0840401 and CHE0541775, NIH P20 RR017716). NR 63 TC 1 Z9 1 U1 3 U2 20 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1089-5639 J9 J PHYS CHEM A JI J. Phys. Chem. A PD NOV 13 PY 2014 VL 118 IS 45 BP 10639 EP 10648 DI 10.1021/jp506412r PG 10 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AT5IK UT WOS:000344976900038 PM 25187099 ER PT J AU Popolan-Vaida, DM Wilson, KR Leone, SR AF Popolan-Vaida, Denisia M. Wilson, Kevin R. Leone, Stephen R. TI Reaction of Iodine Atoms with Submicrometer Squalane and Squalene Droplets: Mechanistic Insights into Heterogeneous Reactions SO JOURNAL OF PHYSICAL CHEMISTRY A LA English DT Article ID GENERATING PARTICLE BEAMS; CATALYZED ISOMERIZATION; CONTROLLED DIMENSIONS; AERODYNAMIC LENSES; NOZZLE EXPANSIONS; N-BUTENES; KINETICS; RADICALS; AEROSOLS; HEAT AB The gas-phase reaction of iodine atoms with hydrocarbon molecules is energetically unfavorable, and there is no direct evidence for iodinated product formation by either H abstraction or I addiction reactions at ambient termperature. Here we consider the possible heterogeneous reaction of I atoms with submicrometer droplets composed of a saturated alkane, squalane (Sq), and an unsaturated alkene, squalene (Sqe). The investigations are performed in an atmospheric pressure photochemical flow tube reactor in conjunction with a vacuum ultraviolet photoionization aerosol mass spectrometer and a scanning mobility particle sizer. Squalane, a branched alkane, is unreactive toward I atoms within the signal-to-noise, and an upper limit of the effective reactive uptake coefficient is estimated to be g(I)(Sq) = 8.58 x 10(-7). In contrast, the reaction of I atoms with unsaturated submicrometer squalene droplets results in observable iodinated squalene products. The effective reactive uptake coefficient of I atom with squalene particles is determined to be g(I)(Sqe) = (1.20 +/- 0.52) x 10(-4) at an average I concentration of 1.5 x 10(14) molecules cm(-3). C1 [Popolan-Vaida, Denisia M.; Wilson, Kevin R.; Leone, Stephen R.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA. [Popolan-Vaida, Denisia M.; Leone, Stephen R.] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA. [Leone, Stephen R.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA. RP Leone, SR (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA. EM srl@berkeley.edu FU Office of Energy Research, Office of Basic Energy Sciences, Chemical Sciences Division of the U.S. Department of Energy [DE-AC02-05CH11231]; Alexander von Humboldt Foundation FX This work was supported by the Director, Office of Energy Research, Office of Basic Energy Sciences, Chemical Sciences Division of the U.S. Department of Energy under Contract DE-AC02-05CH11231. The authors acknowledge constructive discussions with Dr. M. D. Ward and the technical assistance from Dr. D. J. Taube. In particular, D.M.P.-V. is grateful to the Alexander von Humboldt Foundation for a Feodor Lynen fellowship. NR 39 TC 2 Z9 2 U1 4 U2 18 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1089-5639 J9 J PHYS CHEM A JI J. Phys. Chem. A PD NOV 13 PY 2014 VL 118 IS 45 BP 10688 EP 10698 DI 10.1021/jp5085247 PG 11 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AT5IK UT WOS:000344976900043 PM 25327465 ER PT J AU Ondarse-Alvarez, D Oldani, N Tretiak, S Fernandez-Alberti, S AF Ondarse-Alvarez, D. Oldani, N. Tretiak, S. Fernandez-Alberti, S. TI Computational Study of Photoexcited Dynamics in Bichromophoric Cross-Shaped Oligofluorene SO JOURNAL OF PHYSICAL CHEMISTRY A LA English DT Article ID LIGHT-EMITTING-DIODES; UNIDIRECTIONAL ENERGY-TRANSFER; STATE MOLECULAR-DYNAMICS; CONJUGATED POLYMERS; OPTOELECTRONIC DEVICES; NONLINEAR POLARIZABILITIES; SUBSTITUTED POLYTHIOPHENES; POLYFLUORENE DERIVATIVES; NONADIABATIC COUPLINGS; ELECTRONIC COHERENCE AB The non-adiabatic excited state molecular dynamics (NA-ESMD) approach is applied to investigate photoexcited dynamics and relaxation pathways in a spiro-linked conjugated polyfluorene at room (T = 300 K) and low (T = 10 K) temperatures. This dimeric aggregate consists of two perpendicularly oriented weakly interacting a-polyfluorene oligomers. The negligible coupling between the monomer chains results in an initial absorption band composed of equal contributions of the two lowest excited electronic states, each localized on one of the two chains. After photoexcitation, an efficient ultrafast localization of the entire electronic population to the lowest excited state is observed on the time scale of about 100 fs. Both internal conversion between excited electronic states and vibronic energy relaxation on a single electronic state contribute to this process. Thus, photoexcited dynamics of the polyfluorene dimer follows two distinct pathways with substantial temperature dependence on their efficiency. One relaxation channel involves resonance electronic energy transfer between the monomer chains, whereas the second pathway concerns the relaxation of the electronic energy on the same chain that has been initially excited due to electron-phonon coupling. Despite the slower vibrational relaxation, a more efficient ultrafast electronic relaxation is observed at low temperature. Our numerical simulations analyze the effects of molecular geometry distortion during the electronic energy redistribution and suggest spectroscopic signatures reflecting complex electron-vibrational dynamics. C1 [Ondarse-Alvarez, D.; Oldani, N.; Fernandez-Alberti, S.] Univ Nacl Quilmes, Bernal, Argentina. [Tretiak, S.] Los Alamos Natl Lab, Div Theoret, Ctr Nonlinear Studies CNLS, Los Alamos, NM 87545 USA. [Tretiak, S.] Los Alamos Natl Lab, Ctr Integrated Nanotechnol CINT, Los Alamos, NM 87545 USA. RP Fernandez-Alberti, S (reprint author), Univ Nacl Quilmes, Roque Saenz Pena 352,B1876BXD, Bernal, Argentina. EM sfalberti@gmail.com RI Tretiak, Sergei/B-5556-2009 OI Tretiak, Sergei/0000-0001-5547-3647 FU CONICET; UNQ; ANPCyT [PICT-2010-2375]; U.S. Department of Energy; Los Alamos LDRD funds; National Nuclear Security Administration of the U.S. Department of Energy [DE-AC52-06NA25396]; Center for Integrated Nanotechnology (CINT) at LANL; Center for Nonlinear Studies (CNLS) at LANL FX This work was partially supported by CONICET, UNQ, ANPCyT (PICT-2010-2375) and the U.S. Department of Energy and Los Alamos LDRD funds. Los Alamos National Laboratory is operated by Los Alamos National Security, LLC, for the National Nuclear Security Administration of the U.S. Department of Energy under contract DE-AC52-06NA25396. We acknowledge support of Center for Integrated Nanotechnology (CINT) and Center for Nonlinear Studies (CNLS) at LANL. NR 96 TC 4 Z9 4 U1 2 U2 16 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1089-5639 J9 J PHYS CHEM A JI J. Phys. Chem. A PD NOV 13 PY 2014 VL 118 IS 45 BP 10742 EP 10753 DI 10.1021/jp504720n PG 12 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AT5IK UT WOS:000344976900050 PM 25341055 ER PT J AU Ryberg, E Forssen, C Hammer, HW Platter, L AF Ryberg, Emil Forssen, Christian Hammer, H. -W. Platter, Lucas TI Constraining low-energy proton capture on beryllium-7 through charge radius measurements SO EUROPEAN PHYSICAL JOURNAL A LA English DT Article ID EFFECTIVE-FIELD THEORY; CROSS-SECTION; HALO NUCLEI; SCATTERING; BE-7(P; EFT AB In this paper, we point out that a measurement of the charge radius of boron-8 provides indirect access to the S-factor for radiative proton capture on beryllium-7 at low energies. We use leading-order halo effective field theory to explore this correlation and we give a relation between the charge radius and the S-factor. Furthermore, we present important technical aspects relevant to the renormalization of point-like P -wave interactions in the presence of a repulsive Coulomb interaction. C1 [Ryberg, Emil; Forssen, Christian; Platter, Lucas] Chalmers, Dept Fundamental Phys, S-41296 Gothenburg, Sweden. [Hammer, H. -W.] Tech Univ Darmstadt, Inst Kernphys, D-64289 Darmstadt, Germany. [Hammer, H. -W.] GSI Helmholtzzentrum Schwerionenforsch GmbH, ExtreMe Matter Inst EMMI, D-64291 Darmstadt, Germany. [Platter, Lucas] Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA. RP Ryberg, E (reprint author), Chalmers, Dept Fundamental Phys, S-41296 Gothenburg, Sweden. EM emilr@chalmers.se RI Forssen, Christian/C-6093-2008; Platter, Lucas/N-3887-2013 OI Forssen, Christian/0000-0003-3458-0480; Platter, Lucas/0000-0001-6632-8250 FU Swedish Research Council [dnr. 2010-4078]; European Research Council under the European Community's Seventh Framework Programme [240603]; BMBF [05P12PDFTE]; DFG [SFB 634]; Office of Nuclear Physics, U.S. Department of Energy [DE-AC02-06CH11357]; Helmholtz Association [HA216/EMMI] FX We thank D.R. Phillips and H. Esbensen for useful discussions. This research was supported in part by the Swedish Research Council (dnr. 2010-4078), the European Research Council under the European Community's Seventh Framework Programme (FP7/2007-2013) / ERC grant agreement no. 240603, the BMBF under grant 05P12PDFTE, the DFG through SFB 634, the Office of Nuclear Physics, U.S. Department of Energy under contract no. DE-AC02-06CH11357 and by the Helmholtz Association under contract HA216/EMMI. We express our appreciation to the Extreme Matter Institute at GSI and the Institute for Nuclear Theory in Seattle, where part of this work was carried out. NR 44 TC 7 Z9 7 U1 0 U2 2 PU SPRINGER PI NEW YORK PA 233 SPRING ST, NEW YORK, NY 10013 USA SN 1434-6001 EI 1434-601X J9 EUR PHYS J A JI Eur. Phys. J. A PD NOV 13 PY 2014 VL 50 IS 11 AR 170 DI 10.1140/epja/i2014-14170-2 PG 13 WC Physics, Nuclear; Physics, Particles & Fields SC Physics GA AT7XO UT WOS:000345148000001 ER PT J AU Krogstad, DV Choi, SH Lynd, NA Audus, DJ Perry, SL Gopez, JD Hawker, CJ Kramer, EJ Tirrell, MV AF Krogstad, Daniel V. Choi, Soo-Hyung Lynd, Nathaniel A. Audus, Debra J. Perry, Sarah L. Gopez, Jeffrey D. Hawker, Craig J. Kramer, Edward J. Tirrell, Matthew V. TI Small Angle Neutron Scattering Study of Complex Coacervate Micelles and Hydrogels Formed from Ionic Diblock and Triblock Copolymers SO JOURNAL OF PHYSICAL CHEMISTRY B LA English DT Article ID CHARGED BLOCK-COPOLYMERS; CORE; PROTEINS; BEHAVIOR; LENGTH; WATER AB A complex coacervate is a fluid phase that results from the electrostatic interactions between two oppositely charged macromolecules. The nature of the coacervate core structure of hydrogels and micelles formed from complexation between pairs of diblock or triblock copolymers containing oppositely charged end-blocks as a function of polymer and salt concentration was investigated. Both ABA triblock copolymers of poly[(allyl glycidyl ether)-b-(ethylene oxide)-b-(allyl glycidyl ether)] and analogous poly[(allyl glycidyl ether)-b-(ethylene oxide)] diblock copolymers, which were synthesized to be nearly one-half of the symmetrical triblock copolymers, were studied. The poly(allyl glycidyl ether) blocks were functionalized with either guanidinium or sulfonate groups via postpolymerization modification. Mixing of oppositely charged block copolymers resulted in the formation of nanometer-scale coacervate domains. Small angle neutron scattering (SANS) experiments were used to investigate the size and spacing of the coacervate domains. The SANS patterns were fit using a previously vetted, detailed model consisting of polydisperse coreshell micelles with a randomly distributed sphere or body-centered cubic (BCC) structure factor. For increasing polymer concentration, the size of the coacervate domains remained constant while the spatial extent of the poly(ethylene oxide) (PEO) corona decreased. However, increasing salt concentration resulted in a decrease in both the coacervate domain size and the corona size due to a combination of the electrostatic interactions being screened and the shrinkage of the neutral PEO blocks. Additionally, for the triblock copolymers that formed BCC ordered domains, the water content in the coacervate domains was calculated to increase from approximately 16.8% to 27.5% as the polymer concentration decreased from 20 to 15 wt %. C1 [Krogstad, Daniel V.; Hawker, Craig J.; Kramer, Edward J.] Univ Calif Santa Barbara, Dept Mat, Santa Barbara, CA 93106 USA. [Krogstad, Daniel V.; Choi, Soo-Hyung; Lynd, Nathaniel A.; Audus, Debra J.; Gopez, Jeffrey D.; Hawker, Craig J.; Kramer, Edward J.] Univ Calif Santa Barbara, Mat Res Lab, Santa Barbara, CA 93106 USA. [Audus, Debra J.; Gopez, Jeffrey D.; Kramer, Edward J.] Univ Calif Santa Barbara, Dept Chem Engn, Santa Barbara, CA 93106 USA. [Hawker, Craig J.] Univ Calif Santa Barbara, Dept Chem & Biochem, Santa Barbara, CA 93106 USA. [Choi, Soo-Hyung] Hongik Univ, Dept Chem Engn, Seoul 121791, South Korea. [Perry, Sarah L.; Tirrell, Matthew V.] Univ Chicago, Inst Mol Engn, Chicago, IL 60637 USA. [Tirrell, Matthew V.] Argonne Natl Lab, Lemont, IL 60439 USA. RP Tirrell, MV (reprint author), Jones Lab 222, 5747 South Ellis Ave, Chicago, IL 60637 USA. EM mtirrell@uchicago.edu RI Choi, Soo-hyung/H-9734-2012; OI Choi, Soo-hyung/0000-0002-4078-6285; Perry, Sarah/0000-0003-2301-6710 FU National Science Foundation [DMR 1121053]; Argonne National Laboratory under U.S. Department of Energy [DE-ACO2-06CH11357]; Scientific User Facilities Division, Office of Basic Energy Sciences, US Department of Energy FX The synthesis, SANS and microscopy work reported here was partially supported by the IVIRSEC Program of the National Science Foundation under Award No. DMR 1121053 (D.V.K, NA.L, S.-H.C., DJ.A., J.G., CJ.H., and EJ.K.). SANS, interpretation, and writing were supported by the University of Chicago (D.V.K, S.L.P., M.V.T.), and by the Laboratory Directed Research and Development Program of the Argonne National Laboratory under U.S. Department of Energy Contract No. DE-ACO2-06CH11357 (M.V.T.). The research conducted at the ORNL's High Flux Isotope Reactor was sponsored by the Scientific User Facilities Division, Office of Basic Energy Sciences, US Department of Energy. The authors would like to thank Dr. Urban Volker and Dr. Sai Venkatesh Pingali for their help and support with the SANS experiment. NR 36 TC 19 Z9 19 U1 6 U2 67 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1520-6106 J9 J PHYS CHEM B JI J. Phys. Chem. B PD NOV 13 PY 2014 VL 118 IS 45 BP 13011 EP 13018 DI 10.1021/jp509175a PG 8 WC Chemistry, Physical SC Chemistry GA AT5IH UT WOS:000344976600022 PM 25338302 ER PT J AU Jiang, QL Sheng, X Shi, B Feng, XJ Xu, T AF Jiang, Qinglong Sheng, Xia Shi, Bing Feng, Xinjian Xu, Tao TI Nickel-Cathoded Perovskite Solar Cells SO JOURNAL OF PHYSICAL CHEMISTRY C LA English DT Article ID INORGANIC HOLE CONDUCTOR; CHARGE-TRANSPORT; SENSITIZED TIO2; DEPOSITION; EFFICIENCY; IODIDE AB Current lead halide perovskite solar cells use high work function (phi) precious metals, such as gold (phi = 5.1 eV), as the back cathode to maximize the attainable photovoltage. We report herein a set of perovskite-type solar cells that use nickel (phi = 5.04 eV), an earth-abundant element and non-precious metal, as back cathode and achieve the same open-circuit voltage as gold and an efficiency of 10.4%. This work opens a nickel-and-dimed (low-cost) way toward high-efficient perovskite solar cells. C1 [Jiang, Qinglong; Feng, Xinjian; Xu, Tao] No Illinois Univ, Dept Chem & Biochem, De Kalb, IL 60115 USA. [Sheng, Xia; Feng, Xinjian] Chinese Acad Sci, Suzhou Inst Nanotech & Nanobion, Suzhou 215123, Jiangsu, Peoples R China. [Shi, Bing] Argonne Natl Lab, Adv Photon Source, Argonne, IL 60439 USA. RP Xu, T (reprint author), No Illinois Univ, Dept Chem & Biochem, De Kalb, IL 60115 USA. EM txu@niu.edu FU U.S. National Science Foundation [CBET-1150617]; US DOE office of Science, Office of Basic energy Sciences [DE-AC02-06CH11357, DE-AC-02-98CH10886]; [NSFC-21371178] FX We acknowledge the support from the U.S. National Science Foundation (CBET-1150617). Ski is supported by the US DOE office of Science, Office of Basic energy Sciences, under Contract No. DE-AC02-06CH11357 and DE-AC-02-98CH10886. X.F. acknowledges the support from NSFC-21371178. NR 20 TC 19 Z9 20 U1 10 U2 87 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1932-7447 J9 J PHYS CHEM C JI J. Phys. Chem. C PD NOV 13 PY 2014 VL 118 IS 45 BP 25878 EP 25883 DI 10.1021/jp506991x PG 6 WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Chemistry; Science & Technology - Other Topics; Materials Science GA AT5IW UT WOS:000344978000007 ER PT J AU Seo, DM Afroz, T Allen, JL Boyle, PD Trulove, PC De Long, HC Henderson, WA AF Seo, Daniel M. Afroz, Taliman Allen, Joshua L. Boyle, Paul D. Trulove, Paul C. De Long, Hugh C. Henderson, Wesley A. TI Structural Interactions within Lithium Salt Solvates: Cyclic Carbonates and Esters SO JOURNAL OF PHYSICAL CHEMISTRY C LA English DT Article ID AMORPHOUS CONCENTRATED LIQUID; PROPYLENE CARBONATE; ETHYLENE CARBONATE; GAMMA-BUTYROLACTONE; CRYSTAL-STRUCTURE; AB-INITIO; IONIC ASSOCIATION; LOW-TEMPERATURE; NONAQUEOUS ELECTROLYTES; VIBRATIONAL FREQUENCIES AB Only limited information is available regarding the manner in which cyclic carbonate and ester solvents coordinate Li+ cations in electrolyte solutions for lithium batteries. One approach to gleaning significant insight into these interactions is to examine crystalline solvate structures. To this end, eight new solvate structures are reported with ethylene carbonate, gamma-butyrolactone, and gamma-valerolactone: (EC)(3):LiClO4, (EC)(2):LiClO4, (EC)(2):LiBF4, (GBL)(4):LiPF6, (GBL)(1):LiClO4, (GVL)(1):LiClO4, (GBL)(1):LiBF4, and (GBL)(1):LiCF3SO3. The crystal structure of (EC)(1):LiCF3SO3 is also re-reported for comparison. These structures enable the factors that govern the manner in which the ions are coordinated and the ion/solvent packing-in the solid-state-to be scrutinized in detail. C1 [Seo, Daniel M.; Afroz, Taliman; Allen, Joshua L.; Henderson, Wesley A.] N Carolina State Univ, Dept Chem & Biomol Engn, Ion Liquids & Electrolytes Energy Technol ILEET L, Raleigh, NC 27695 USA. [Boyle, Paul D.] N Carolina State Univ, Dept Chem, Xray Struct Facil, Raleigh, NC 27695 USA. [Trulove, Paul C.] US Naval Acad, Dept Chem, Annapolis, MD 21402 USA. [De Long, Hugh C.] Air Force Off Sci Res, Arlington, VA 22203 USA. [Henderson, Wesley A.] Pacific NW Natl Lab, Electrochem Mat & Syst Grp, Energy & Environm Directorate, Richland, WA 99352 USA. RP Henderson, WA (reprint author), N Carolina State Univ, Dept Chem & Biomol Engn, Ion Liquids & Electrolytes Energy Technol ILEET L, Raleigh, NC 27695 USA. EM Wesley.Henderson@pnnl.gov FU U.S. Department of Energy, Office of Basic Energy Sciences, Division of Materials Sciences and Engineering [DE-SC0002169] FX The authors wish to express their gratitude to the U.S. Department of Energy, Office of Basic Energy Sciences, Division of Materials Sciences and Engineering, which supported this research under Award DE-SC0002169. NR 60 TC 7 Z9 7 U1 6 U2 34 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1932-7447 J9 J PHYS CHEM C JI J. Phys. Chem. C PD NOV 13 PY 2014 VL 118 IS 45 BP 25884 EP 25889 DI 10.1021/jp5079168 PG 6 WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Chemistry; Science & Technology - Other Topics; Materials Science GA AT5IW UT WOS:000344978000008 ER PT J AU Deshlahra, P Igesia, E AF Deshlahra, Prashant Igesia, Enrique TI Methanol Oxidative Dehydrogenation on Oxide Catalysts: Molecular and Dissociative Routes and Hydrogen Addition Energies as Descriptors of Reactivity SO JOURNAL OF PHYSICAL CHEMISTRY C LA English DT Article ID DENSITY-FUNCTIONAL THEORY; SELECTIVE OXIDATION; HETEROPOLY COMPOUNDS; SURFACE-CHEMISTRY; MOLYBDENUM OXIDE; REDOX PROPERTIES; DIMETHYL ETHER; ACID CATALYSIS; METAL-OXIDES; SILICA AB The oxidative dehydrogenation (ODH) of alkanols on oxide catalysts is generally described as involving H-abstraction from alkoxy species formed via OH dissociation. Kinetic and isotopic data cannot discern between such routes and those involving kinetically-relevant H-abstraction from undissociated alkanols. Here, we combine such experiments with theoretical estimates of activation energies and entropies to show that the latter molecular routes prevail over dissociative routes for methanol reactions on polyoxometalate (POM) clusters at all practical reaction temperatures. The stability of the late transition states that mediate H-abstraction depend predominantly on the stability of the OH bond formed, making H-addition energies (HAE) accurate and single-valued descriptors of reactivity. Density functional theory-derived activation energies depend linearly on HAE values at each O-atom location on clusters with a range of composition (H3PMo12, H4SiMo12, H3PW12, H4PV1Mo11, and H4PV1W11); both barriers and HAE values reflect the lowest unoccupied molecular orbital energy of metal centers that accept the electron and the protonation energy of O-atoms that accept the proton involved in the H-atom transfer. Bridging O-atoms form OH bonds that are stronger than those of terminal atoms and therefore exhibit more negative HAE values and higher ODH reactivity on all POM clusters. For each cluster composition, ODH turnover rates reflect the reactivity-averaged HAE of all accessible O-atoms, which can be evaluated for each cluster composition to provide a rigorous and accurate predictor of ODH reactivity for catalysts with known structure. These relations together with oxidation reactivity measurements can then be used to estimate HAE values and to infer plausible structures for catalysts with uncertain active site structures. C1 [Deshlahra, Prashant; Igesia, Enrique] Univ Calif Berkeley, Dept Chem Engn, Berkeley, CA 94720 USA. [Igesia, Enrique] EO Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA. RP Igesia, E (reprint author), Univ Calif Berkeley, Dept Chem Engn, Berkeley, CA 94720 USA. EM iglesia@berkeley.edu FU U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-AC05-76RL0-1830]; DOE [47582]; National Science Foundation [ACI-1053575, CHE-0840505] FX This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under contract DE-AC05-76RL0-1830. Computational facilities were provided by the Environmental Molecular Science Laboratory (EMSL) at Pacific Northwest National Laboratory (PNNL), a DOE Office of Science User Facility, under proposal 47582. The use of molecular DFT calculations using Gaussian program was made possible by the Extreme Science and Engineering Discovery Environment (XSEDE) and a UC Berkeley College of Chemistry facility, which are supported by National Science Foundation grants (ACI-1053575 and CHE-0840505, respectively). We thank Dr. David Hibbitts (UC-Berkeley) for assistance with the statistical mechanics treatments and Dr. Robert Carr, Mr. William Knaeble, and Mr. Nee lay Phadke (UC-Berkeley) for technical discussions and a critical review of the concepts developed in this manuscript. NR 52 TC 8 Z9 8 U1 3 U2 24 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1932-7447 J9 J PHYS CHEM C JI J. Phys. Chem. C PD NOV 13 PY 2014 VL 118 IS 45 BP 26115 EP 26129 DI 10.1021/jp507922u PG 15 WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Chemistry; Science & Technology - Other Topics; Materials Science GA AT5IW UT WOS:000344978000034 ER PT J AU Yang, CT Wood, BC Bhethanabotla, VR Joseph, B AF Yang, Chi-Ta Wood, Brandon C. Bhethanabotla, Venkat R. Joseph, Babu TI CO2 Adsorption on Anatase TiO2 (101) Surfaces in the Presence of Subnanometer Ag/Pt Clusters: Implications for CO2 Photoreduction SO JOURNAL OF PHYSICAL CHEMISTRY C LA English DT Article ID TOTAL-ENERGY CALCULATIONS; ELASTIC BAND METHOD; WAVE BASIS-SET; CARBON-DIOXIDE; PHOTOCATALYTIC CONVERSION; TIO2(101) SURFACE; HYDROCARBON FUELS; OXYGEN VACANCIES; SADDLE-POINTS; REDUCTION AB Using density functional theory calculations, we show how CO2 adsorption on perfect and reduced anatase TiO2 (101) surfaces can be substantially modified by the presence of surface Ag and Pt octamer clusters. We find that adsorption is affected even at sites where the adsorbate is not in direct contact with the octamer, which we attribute to charge donation to CO2 from the Ag/Pt-modified surface, as well as an electrostatic competition between attractive (Ti-O) and repulsive (Ti-C) interactions. In addition, TiO2-supported Pt octamers offer key advantages that could be leveraged for CO2 photoreduction, including providing additional stable adsorption sites for bent CO2 species and facilitating charge transfer to aid in CO2- anion formation. Electronic structure analysis suggests these factors arise primarily from the hybridization of the bonding molecular orbitals of CO2 with d orbitals of the Pt atoms. Our results show that, for adsorption on TiO(2-)supported Pt octamers, the O-C-O bending and C-O asymmetric stretching frequencies can be used as reliable indicators of the presence of the CO2- anion intermediate as well as to distinguish unique adsorption geometries or sites. Finally, we suggest a possible pathway for subsequent CO2 dissociation to CO at the surface of a reduced anatase TiO2 (101)-supported Pt octamer, which has a computed energy barrier of 1.01 eV. C1 [Yang, Chi-Ta; Bhethanabotla, Venkat R.; Joseph, Babu] Univ S Florida, Dept Chem & Biomed Engn, Tampa, FL 33620 USA. [Wood, Brandon C.] Lawrence Livermore Natl Lab, Quantum Simulat Grp, Livermore, CA 94550 USA. RP Joseph, B (reprint author), Univ S Florida, Dept Chem & Biomed Engn, Tampa, FL 33620 USA. EM bjoseph@usf.edu FU U.S. Department of Energy by Lawrence Livermore National Laboratory [DE-AC52-07NA27344] FX The authors thank the USE supercomputing center for computing time and support along with XSEDE and NERSC supercomputing resources. A portion of this work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344. NR 63 TC 10 Z9 10 U1 9 U2 98 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1932-7447 J9 J PHYS CHEM C JI J. Phys. Chem. C PD NOV 13 PY 2014 VL 118 IS 45 BP 26236 EP 26248 DI 10.1021/jp509219n PG 13 WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Chemistry; Science & Technology - Other Topics; Materials Science GA AT5IW UT WOS:000344978000046 ER PT J AU Espinosa-Faller, FJ Conradson, DR Riha, SC Martucci, MB Fredrick, SJ Vogel, S Prieto, AL Conradson, SD AF Espinosa-Faller, Francisco J. Conradson, Dylan R. Riha, Shannon C. Martucci, Mary B. Fredrick, Sarah J. Vogel, Sven Prieto, Amy L. Conradson, Steven D. TI Neutron Diffraction and X-ray Absorption Fine Structure Evidence for Local Lattice Distortions and Aperiodic Antisite Substitution in Cu2ZnSnS4 Nanoparticles SO JOURNAL OF PHYSICAL CHEMISTRY C LA English DT Article ID SOLAR-CELLS; SEMICONDUCTOR NANOCRYSTALS; HETEROGENEOUS CATALYSIS; ABSORBER; PHOTOVOLTAICS; KESTERITE; INK AB A thorough structure determination has been performed on Cu2ZnSnS4 nanoparticles, a popular photovoltaic material, using neutron diffractionto characterize the long-range average crystal structureand X-ray absorption fine structure (XAFS) spectroscopy at the Cu, Zn, and Sn K-edges to elucidate the element-specific local structure. This is the first combined multiscale approach on nanoparticles of this material. The results indicate the presence of aperiodic disorder on the cation sites that is diminished by annealing. This disorder involves local lattice distortions around the crystallographic sites rather than the presence of interstitial atoms. It is most consistent with the known antisite substitutions that are integral to CZTS (referring to the ordering of the Cu, Zn, and Sn between planes). However, instead of being confined within single unit cells so as to maintain the crystallographic symmetry, periodicity, and homogeneity, the substitutional disorder appears to extend over larger regions consisting of multiple unit cells but still smaller than the physical dimensions of the nanoparticles. These results therefore imply the presence of nanoscale domains characterized by local fluctuations in composition that cause the individual domains to be enriched in certain metal ions and depleted in others. These will be mirrored by domains with the opposite fluctuations at other locations in the crystal so that the overall composition remains close to the stoichiometric Cu2ZnSnS4. This disorder is likely pronounced in these samples due to the relatively low temperature reaction (300 degrees C) and annealing (350 degrees C) conditions and can be expected to have a significant effect on the resulting physical properties of the material and its photovoltaic performance. C1 [Conradson, Dylan R.; Martucci, Mary B.; Vogel, Sven; Conradson, Steven D.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA. [Riha, Shannon C.; Martucci, Mary B.; Fredrick, Sarah J.; Prieto, Amy L.] Colorado State Univ, Dept Chem, Ft Collins, CO 80523 USA. [Espinosa-Faller, Francisco J.] Univ Marista Merida, Merida 97300, Yucatan, Mexico. RP Prieto, AL (reprint author), Colorado State Univ, Dept Chem, Ft Collins, CO 80523 USA. EM amy.prieto@colostate.edu; steven.conradson@synchrotron-soleil.fr FU DOE-Basic Energy Sciences under FWP [2012LANLE389]; Conacyt-Mexico [169108]; Heavy Element Chemistry Program of the Division of Chemical Sciences, Biosdences, and Geosciences, Office of Basic Energy Sciences at Los Alamos National Laboratory that is operated by Los Alamos National Security, LLC; National Nuclear Security Administration of U.S. Department of Energy [DE-AC52-06NA2S396]; Colorado State University; Center for Revolutionary Solar Photoconversion (CRSP); NSF Graduate Fellowship program FX Part of this research was performed on the HIPPO instrument at the Lujan Center at Los Alamos National Laboratory supported by DOE-Basic Energy Sciences under FWP #2012LANLE389. Portions of this research were carried out at the Stanford Synchrotron Radiation Lightsource, a Directorate of SLAC National Accelerator Laboratory and an Office of Science User Facility operated for the U.S. Department of Energy Office of Science by Stanford University. FJEF would like to thank Conacyt-Mexico for financial support (Grant No. 169108). SDC and MBM were supported by the Heavy Element Chemistry Program of the Division of Chemical Sciences, Biosdences, and Geosciences, Office of Basic Energy Sciences at Los Alamos National Laboratory that is operated by Los Alamos National Security, LLC, for the National Nuclear Security Administration of U.S. Department of Energy under Contract DE-AC52-06NA2S396. TEM imaging was supported in part by the Microscopy Imaging Network core infrastructure grant from Colorado State University. ALP and SCR thank the Center for Revolutionary Solar Photoconversion (CRSP) for funding. SJF thanks the NSF Graduate Fellowship program for funding. NR 42 TC 7 Z9 7 U1 3 U2 31 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1932-7447 J9 J PHYS CHEM C JI J. Phys. Chem. C PD NOV 13 PY 2014 VL 118 IS 45 BP 26292 EP 26303 DI 10.1021/jp502150s PG 12 WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Chemistry; Science & Technology - Other Topics; Materials Science GA AT5IW UT WOS:000344978000052 ER PT J AU Cherakara, MJ Germann, TC Kober, EM Strachan, A AF Cherakara, Mathew J. Germann, Timothy C. Kober, Edward M. Strachan, Alejandro TI Shock Loading of Granular Ni/Al Composites. Part 1: Mechanics of Loading SO JOURNAL OF PHYSICAL CHEMISTRY C LA English DT Article ID SOLID-STATE REACTIONS; NI-AL SYSTEM; MOLECULAR-DYNAMICS; SIMULATIONS; EXPLOSIVES; MODEL AB We present molecular dynamics simulations of the thermomechanical response under shock loading of a granular material consisting of laminated Ni/Al grains. We observe two regimes: At low piston velocities (mu(p) less than or similar to 1km/s), the shock wave is diffuse, and the width of the shock front decreases with increasing piston velocity. Beyond a critical shock strength, however, the width remains relatively constant at approximately the mean grain radius. This change in behavior follows from an evolution of the mechanism of compaction with increasing insult strength. The mechanism evolves from plastic deformation-mediated pore collapse for relatively weak shocks, to solid extrusion and fluid ejecta filling pores ahead of the shock front at intermediate strengths, and finally to atomic jetting into the pore for very strong shocks (mu(p) less than or similar to 2 km/s). High-energy fluid ejecta into pores leads to the formation of flow vorticity and can result in a large fraction of the input energy localizing into translational kinetic energy components in addition to the formation of hot spots. This has implications for the mechanical mixing of Ni and Al in these reactive composites. C1 [Cherakara, Mathew J.; Strachan, Alejandro] Purdue Univ, Sch Mat Engn, W Lafayette, IN 47907 USA. [Cherakara, Mathew J.; Strachan, Alejandro] Purdue Univ, Birck Nanotechnol Ctr, W Lafayette, IN 47907 USA. [Cherakara, Mathew J.; Germann, Timothy C.; Kober, Edward M.] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA. RP Strachan, A (reprint author), Purdue Univ, Sch Mat Engn, W Lafayette, IN 47907 USA. EM strachan@purdue.edu OI Germann, Timothy/0000-0002-6813-238X FU U.S. Defense Threat Reduction Agency [HDTRA1-10-1-0119]; U.S. Department of Energy National Nuclear Security Administration [t DE-AC52-06NA25396]; Institute for Materials Science (LANL); ExMatEx project FX We thank John Barber for discussions and suggestions regarding the polygon packing problem. This work was supported by the U.S. Defense Threat Reduction Agency, HDTRA1-10-1-0119 (Program Manager Suhithi Peiris) and used resources provided by the Los Alamos National Laboratory Institutional Computing Program, which is supported by the U.S. Department of Energy National Nuclear Security Administration under Contract DE-AC52-06NA25396. E.M.K. acknowledges support from the Institute for Materials Science (LANL), and T.C.G. acknowledges support from the ExMatEx project. NR 45 TC 4 Z9 4 U1 5 U2 26 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1932-7447 J9 J PHYS CHEM C JI J. Phys. Chem. C PD NOV 13 PY 2014 VL 118 IS 45 BP 26377 EP 26386 DI 10.1021/jp507795w PG 10 WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Chemistry; Science & Technology - Other Topics; Materials Science GA AT5IW UT WOS:000344978000061 ER PT J AU Lee, JJ Schmitt, FT Moore, RG Johnston, S Cui, YT Li, W Yi, M Liu, ZK Hashimoto, M Zhang, Y Lu, DH Devereaux, TP Lee, DH Shen, ZX AF Lee, J. J. Schmitt, F. T. Moore, R. G. Johnston, S. Cui, Y. -T. Li, W. Yi, M. Liu, Z. K. Hashimoto, M. Zhang, Y. Lu, D. H. Devereaux, T. P. Lee, D. -H. Shen, Z. -X. TI Interfacial mode coupling as the origin of the enhancement of T-c in FeSe films on SrTiO3 SO NATURE LA English DT Article ID HIGH-TEMPERATURE SUPERCONDUCTIVITY; PHOTOEMISSION AB Films of iron selenide (FeSe) one unit cell thick grown on strontium titanate (SrTiO3 or STO) substrates have recently shown(1-4) superconducting energy gaps opening at temperatures close to the boiling point of liquid nitrogen (77 kelvin), which is a record for the iron-based superconductors. The gap opening temperature usually sets the superconducting transition temperature T-c, as the gap signals the formation of Cooper pairs, the bound electron states responsible for superconductivity. To understand why Cooper pairs form at such high temperatures, we examine the role of the SrTiO3 substrate. Here we report high-resolution angle-resolved photoemission spectroscopy results that reveal an unexpected characteristic of the single-unit-cell FeSe/SrTiO3 system: shake-off bands suggesting the presence of bosonic modes, most probably oxygen optical phonons in SrTiO3 (refs 5-7), which couple to the FeSe electrons with only a small momentum transfer. Such interfacial coupling assists superconductivity in most channels, including those mediated by spin fluctuations(8-14). Our calculations suggest that this coupling is responsible for raising the superconducting gap opening temperature in single-unit-cell FeSe/SrTiO3. C1 [Lee, J. J.; Schmitt, F. T.; Moore, R. G.; Cui, Y. -T.; Li, W.; Yi, M.; Liu, Z. K.; Zhang, Y.; Devereaux, T. P.; Shen, Z. -X.] SLAC Natl Accelerator Lab, Stanford Inst Mat & Energy Sci, Menlo Pk, CA 94025 USA. [Lee, J. J.; Yi, M.; Liu, Z. K.; Shen, Z. -X.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA. [Lee, J. J.; Yi, M.; Liu, Z. K.; Shen, Z. -X.] Stanford Univ, Dept Appl Phys, Stanford, CA 94305 USA. [Lee, J. J.; Yi, M.; Liu, Z. K.; Shen, Z. -X.] Stanford Univ, Geballe Lab Adv Mat, Stanford, CA 94305 USA. [Johnston, S.] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada. [Johnston, S.] Univ British Columbia, Quantum Matter Inst, Vancouver, BC V6T 1Z4, Canada. [Johnston, S.] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA. [Hashimoto, M.; Lu, D. H.] SLAC Natl Accelerator Lab, Stanford Synchrotron Radiat Lightsource, Menlo Pk, CA 94025 USA. [Zhang, Y.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94720 USA. [Lee, D. -H.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA. [Lee, D. -H.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA. RP Shen, ZX (reprint author), SLAC Natl Accelerator Lab, Stanford Inst Mat & Energy Sci, Menlo Pk, CA 94025 USA. EM zxshen@stanford.edu RI Cui, Yong-Tao/G-8505-2015; Johnston, Steven/J-7777-2016 OI Cui, Yong-Tao/0000-0002-8015-1049; FU US Department of Energy, Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division; Department of Energy, Office of Basic Energy Sciences, Division of Materials Science, under the Quantum Material programme [DE-AC02-05CH11231] FX This work was supported by the US Department of Energy, Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division. D.-H.L. is supported by the Department of Energy, Office of Basic Energy Sciences, Division of Materials Science, under the Quantum Material programme DE-AC02-05CH11231. Measurements were performed at the Stanford Synchrotron Radiation Lightsource, a national user facility operated by Stanford University on behalf of the US Department of Energy, Office of Basic Energy Sciences. NR 27 TC 131 Z9 133 U1 22 U2 207 PU NATURE PUBLISHING GROUP PI LONDON PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND SN 0028-0836 EI 1476-4687 J9 NATURE JI Nature PD NOV 13 PY 2014 VL 515 IS 7526 BP 245 EP U207 DI 10.1038/nature13894 PG 12 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AT0MZ UT WOS:000344631400045 PM 25391962 ER PT J AU Xie, JJ Wu, JJ Zou, BS AF Xie, Ju-Jun Wu, Jia-Jun Zou, Bing-Song TI Role of the possible Sigma*(1/2(-)) state in the Lambda p -> Lambda p pi(0) reaction SO PHYSICAL REVIEW C LA English DT Article AB The Lambda p -> Lambda p pi(0) reaction near threshold is studied within an effective Lagrangian method. The production process is described by single-pion and single-kaon exchange. In addition to the role played by the Sigma*(1385) resonance of spin-parity J(P) = 3/2(+), the effects of a newly proposed Sigma* (J(P) = 1/2(-)) state with mass and width around 1380 MeV and 120 MeV are investigated. We show that our model leads to a good description of the experimental data on the total cross section of the Lambda p -> Lambda p pi(0) reaction by including the contributions from the possible Sigma* (1/2(-)) state. However, the theoretical calculations by considering only the Sigma*(1385) resonance fail to reproduce the experimental data, especially for the enhancement close to the reaction threshold. On the other hand, it is found that the single-pion exchange is dominant. Furthermore, we also demonstrate that the angular distributions provide direct information of this reaction, hence could be useful for the investigation of the existence of the Sigma*(1/2(-)) state and may be tested by future experiments. C1 [Xie, Ju-Jun] Chinese Acad Sci, Inst Modern Phys, Lanzhou 730000, Peoples R China. [Xie, Ju-Jun] Chinese Acad Sci, Inst Modern Phys, Res Ctr Hadron, Lanzhou 730000, Peoples R China. [Xie, Ju-Jun] Chinese Acad Sci, Inst Modern Phys, CSR Phys, Lanzhou 730000, Peoples R China. [Xie, Ju-Jun] Lanzhou Univ, Lanzhou 730000, Peoples R China. [Xie, Ju-Jun; Zou, Bing-Song] Chinese Acad Sci, Inst Theoret Phys, State Key Lab Theoret Phys, Beijing 100190, Peoples R China. [Wu, Jia-Jun] Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA. RP Xie, JJ (reprint author), Chinese Acad Sci, Inst Modern Phys, Lanzhou 730000, Peoples R China. EM xiejujun@impcas.ac.cn; zoubs@itp.ac.cn FU National Natural Science Foundation of China [11105126, 11035006, 11121092, 11261130311]; Chinese Academy of Sciences [KJCX2-EW-N01]; Ministry of Science and Technology of China [2009CB825200]; U.S. Department of Energy, Office of Science, Office of Nuclear Physics [DE-AC02-06CH11357] FX We would like to thank Prof. T.-S. H. Lee and Xu Cao for useful discussions. This work is partly supported by the National Natural Science Foundation of China under Grants No. 11105126, No. 11035006, No. 11121092, No. 11261130311 (RC110 by DFG and NSFC), the Chinese Academy of Sciences under Project No. KJCX2-EW-N01, and the Ministry of Science and Technology of China (2009CB825200). This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Contract No. DE-AC02-06CH11357. NR 33 TC 0 Z9 0 U1 1 U2 1 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0556-2813 EI 1089-490X J9 PHYS REV C JI Phys. Rev. C PD NOV 12 PY 2014 VL 90 IS 5 AR 055204 DI 10.1103/PhysRevC.90.055204 PG 6 WC Physics, Nuclear SC Physics GA CJ0UP UT WOS:000355194400003 ER PT J AU Yu, T Tyson, TA Gao, P Wu, T Hong, X Ghose, S Chen, YS AF Yu, T. Tyson, T. A. Gao, P. Wu, T. Hong, X. Ghose, S. Chen, Y. -S. TI Structural changes related to the magnetic transitions in hexagonal InMnO3 SO PHYSICAL REVIEW B LA English DT Article ID PAIR DISTRIBUTION FUNCTION; LUMNO3; PHASE AB Two magnetic ordering transitions are found in InMnO3, the paramagnetic to antiferromagnetic transition at similar to 118 K and a lower possible spin rotation transition near 42 K. Multiple length scale structural measurements reveal enhanced local distortion found to be connected with tilting of the MnO5 polyhedra as temperature is reduced. Coupling is observed between the lattice and the spin manifested as changes in the structure near both of the magnetic ordering temperatures (at similar to 42 and similar to 118 K). External parameters, such as pressure, are expected to modify the coupling. C1 [Yu, T.; Tyson, T. A.; Gao, P.; Wu, T.] New Jersey Inst Technol, Dept Phys, Newark, NJ 07102 USA. [Hong, X.] SUNY Stony Brook, Inst Mineral Phys, Stony Brook, NY 11794 USA. [Ghose, S.] Brookhaven Natl Lab, Photon Sci Directorate, Upton, NY 11973 USA. [Chen, Y. -S.] Univ Chicago, ChemMatCARS, Argonne, IL 60439 USA. [Chen, Y. -S.] Argonne Natl Lab, Adv Photon Source, Argonne, IL 60439 USA. RP Tyson, TA (reprint author), New Jersey Inst Technol, Dept Phys, Newark, NJ 07102 USA. EM tyson@njit.edu FU DOE Grant [DE-FG02-07ER46402]; US Department of Energy; National Science Foundation; Department of Energy [NSF/CHE-1346572]; U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-AC02-06CH11357]; NSF MRI Grant [DMR-0923032] FX This work was supported by DOE Grant No. DE-FG02-07ER46402. Synchrotron powder x-ray diffraction and x-ray absorption data acquisition were performed at Brookhaven National Laboratory's NSLS, which is funded by the US Department of Energy. Single-crystal x-ray diffraction measurements were performed at the beamline 15-ID-B, Advanced Photon Source, Argonne National Laboratory. ChemMat-CARS Sector 15 is principally supported by the National Science Foundation and Department of Energy under Grant No. NSF/CHE-1346572. Use of the Advanced Photon Source was supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract No. DE-AC02-06CH11357. The physical properties measurement system was acquired under NSF MRI Grant No. DMR-0923032 (ARRA award). NR 25 TC 1 Z9 1 U1 0 U2 48 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 2469-9950 EI 2469-9969 J9 PHYS REV B JI Phys. Rev. B PD NOV 12 PY 2014 VL 90 IS 17 AR 174106 DI 10.1103/PhysRevB.90.174106 PG 9 WC Physics, Condensed Matter SC Physics GA CA2YT UT WOS:000348773000002 ER PT J AU Aad, G Abbott, B Abdallah, J Khalek, SA Abdinov, O Aben, R Abi, B Abolins, M AbouZeid, OS Abramowicz, H Abreu, H Abreu, R Abulaiti, Y Acharya, BS Adamczyk, L Adams, DL Adelman, J Adomeit, S Adye, T Agatonovic-Jovin, T Aguilar-Saavedra, JA Agustoni, M Ahlen, SP Ahmadov, F Aielli, G Akerstedt, H Akesson, TPA Akimoto, G Akimov, AV Alberghi, GL Albert, J Albrand, S Verzini, MJA Aleksa, M Aleksandrov, IN Alexa, C Alexander, G Alexandre, G Alexopoulos, T Alhroob, M Alimonti, G Alio, L Alison, J Allbrooke, BMM Allison, LJ Allport, PP Aloisio, A Alonso, A Alonso, F Alpigiani, C Altheimer, A Gonzalez, BA Alviggi, MG Amako, K Coutinho, YA Amelung, C Amidei, D Dos Santos, SPA Amorim, A Amoroso, S Amram, N Amundsen, G Anastopoulos, C Ancu, LS Andari, N Andeen, T Anders, CF Anders, G Anderson, KJ Andreazza, A Andrei, V Anduaga, XS Angelidakis, S Angelozzi, I Anger, P Angerami, A Anghinolfi, F Anisenkov, AV Anjos, N Annovi, A Antonaki, A Antonelli, M Antonov, A Antos, J Anulli, F Aoki, M Bella, LA Apolle, R Arabidze, G Aracena, I Arai, Y Araque, JP Arce, ATH Arduh, FA Arguin, JF Argyropoulos, S Arik, M Armbruster, AJ Arnaez, O Arnal, V Arnold, H Arratia, M Arslan, O Artamonov, A Artoni, G Asai, S Asbah, N Ashkenazi, A Asman, B Asquith, L Assamagan, K Astalos, R Atkinson, M Atlay, NB Auerbach, B Augsten, K Aurousseau, M Avolio, G Axen, B Azuelos, G Azuma, Y Baak, MA Baas, AE Bacci, C Bachacou, H Bachas, K Backes, M Backhaus, M Mayes, JB Badescu, E Bagiacchi, P Bagnaia, P Bai, Y Bain, T Baines, JT Baker, OK Balek, P Balli, F Banas, E Banerjee, S Bannoura, AAE Bansal, V Bansil, HS Barak, L Baranov, SP Barberio, EL Barberis, D Barbero, M Barillari, T Barisonzi, M Barklow, T Barlow, N Barnes, SL Barnett, BM Barnett, RM Barnovska, Z Baroncelli, A Barone, G Barr, AJ Barreiro, F da Costa, JBG Bartoldus, R Barton, AE Bartos, P Bartsch, V Bassalat, A Basye, A Bates, RL Batista, SJ Batley, JR Battaglia, M Battistin, M Bauer, F Bawa, HS Beattie, MD Beau, T Beauchemin, PH Beccherle, R Bechtle, P Beck, HP Becker, K Becker, S Beckingham, M Becot, C Beddall, AJ Beddall, A Bedikian, S Bednyakov, VA Bee, CP Beemster, LJ Beermann, TA Begel, M Behr, K Belanger-Champagne, C Bell, PJ Bell, WH Bella, G Bellagamba, L Bellerive, A Bellomo, M Belotskiy, K Beltramello, O Benary, O Benchekroun, D Bendtz, K Benekos, N Benhammou, Y Noccioli, EB Garcia, JAB Benjamin, DP Bensinger, JR Bentvelsen, S Berge, D Kuutmann, EB Berger, N Berghaus, F Beringer, J Bernard, C Bernat, P Bernius, C Bernlochner, FU Berry, T Berta, P Bertella, C Bertoli, G Bertolucci, F Bertsche, C Bertsche, D Besana, MI Besjes, GJ Bessidskaia, O Bessner, M Besson, N Betancourt, C Bethke, S Bhimji, W Bianchi, RM Bianchini, L Bianco, M Biebel, O Bieniek, SP Bierwagen, K Biesiada, J Biglietti, M De Mendizabal, JB Bilokon, H Bindi, M Binet, S Bingul, A 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CA ATLAS Collaboration TI Search for neutral Higgs bosons of the minimal supersymmetric standard model in pp collisions at root s=8 TeV with the ATLAS detector SO JOURNAL OF HIGH ENERGY PHYSICS LA English DT Article DE Hadron-Hadron Scattering ID BENCHMARK SCENARIOS; MASSLESS PARTICLES; BROKEN SYMMETRIES; MONTE-CARLO; MSSM; LHC; MASSES; PROGRAM; DISCOVERY; COUPLINGS AB A search for the neutral Higgs bosons predicted by the Minimal Supersymmetric Standard Model (MSSM) is reported. The analysis is performed on data from proton-proton collisions at a centre-of-mass energy of 8 TeV collected with the ATLAS detector at the Large Hadron Collider. The samples used for this search were collected in 2012 and correspond to integrated luminosities in the range 19.5-20.3 fb(-1). The MSSM Higgs bosons are searched for in the tau tau final state. 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M.; Kaneda, M.; Klioutchnikova, T.; Krasznahorkay, A.; Lantzsch, K.; Lassnig, M.; Miotto, G. Lehmann; Lenzi, B.; Lichard, P.; Macina, D.; Malyukov, S.; Mandelli, B.; Mapelli, L.; Martin, B.; Marzin, A.; Messina, A.; Meyer, J.; Milic, A.; Mornacchi, G.; Nairz, A. M.; Nakahama, Y.; Negri, G.; Nessi, M.; Nicquevert, B.; Nordberg, M.; Oide, H.; Palestini, S.; Pauly, T.; Pernegger, H.; Peters, K.; Petersen, B. A.; Pommes, K.; Poppleton, A.; Poulard, G.; Prasad, S.; Rammensee, M.; Raymond, M.; Rembser, C.; Rodrigues, L.; Roe, S.; Ruiz-Martinez, A.; Salzburger, A.; Savu, D. O.; Schaefer, D.; Schlenker, S.; Schmieden, K.; Serfon, C.; Sfyrla, A.; Solans, C. A.; Spigo, G.; Stelzer, H. J.; Teischinger, F. A.; Ten Kate, H.; Tremblet, L.; Tricoli, A.; Tsarouchas, C.; Unal, G.; van der Ster, D.; van Eldik, N.; van Woerden, M. C.; Vandelli, W.; Vigne, R.; Voss, R.; Vuillermet, R.; Wells, P. S.; Wengler, T.; Wenig, S.; Werner, P.; Wilkens, H. G.; Wotschack, J.; Young, C. J. 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Y.; Xu, L.; Zhu, Y.] Univ Sci & Technol China, Dept Modern Phys, Hefei, Anhui, Peoples R China. [Chen, S.; Li, Y.] Nanjing Univ, Dept Phys, Nanjing, Jiangsu, Peoples R China. [Chen, L.; Feng, C.; Ge, P.; Ma, L. L.; Zhang, X.; Zhao, Y.; Zhao, Z.; Zhu, C. G.] Shandong Univ, Sch Phys, Jinan, Shandong, Peoples R China. [Li, L.; Yang, H.] Shanghai Jiao Tong Univ, Dept Phys, Shanghai 200030, Peoples R China. [Chen, X.] Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China. [Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Donini, J.; Dubreuil, E.; Ghodbane, N.; Gilles, G.; Gris, Ph.; Guicheney, C.; Liao, H.; Pallin, D.; Podlyski, F.; Santoni, C.; Theveneaux-Pelzer, T.; Valery, L.; Vazeille, F.] Clermont Univ, Lab Phys Corpusculaire, Clermont Ferrand, France. [Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Donini, J.; Dubreuil, E.; Ghodbane, N.; Gilles, G.; Gris, Ph.; Guicheney, C.; Liao, H.; Pallin, D.; Podlyski, F.; Santoni, C.; Theveneaux-Pelzer, T.; Valery, L.; Vazeille, F.] Univ Clermont Ferrand, Clermont Ferrand, France. [Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Donini, J.; Dubreuil, E.; Ghodbane, N.; Gilles, G.; Gris, Ph.; Guicheney, C.; Liao, H.; Pallin, D.; Podlyski, F.; Santoni, C.; Theveneaux-Pelzer, T.; Valery, L.; Vazeille, F.] CNRS, IN2P3, Clermont Ferrand, France. [Altheimer, A.; Andeen, T.; Angerami, A.; Bain, T.; Brooijmans, G.; Chen, Y.; Cole, B.; Guo, J.; Hu, D.; Hughes, E. W.; Huseynov, N.; Mohapatra, S.; Nikiforou, N.; Parsons, J. A.; Scherzer, M. I.; Thompson, E. N.; Tian, F.; Tuts, P. M.; Urbaniec, D.; Wulf, E.; Zhou, L.] Columbia Univ, Nevis Lab, Irvington, NY USA. [Aloisio, A.; Alonso, A.; Dam, M.; Galster, G.; Hansen, J. B.; Hansen, J. D.; Hansen, P. H.; Joergensen, M. D.; Loevschall-Jensen, A. E.; Monk, J.; Pedersen, L. E.; Petersen, T. C.; Pingel, A.; Thomsen, L. A.; Wiglesworth, C.; Xella, S.] Univ Copenhagen, Niels Bohr Inst, Copenhagen, Denmark. [Capua, M.; La Rotonda, L.; Mastroberardino, A.; Policicchio, A.; Salvatore, D.; Scarfone, V.; Schioppa, M.; Susinno, G.; Tassi, E.] INFN Grp Collegato Cosenza, Lab Nazl Frascati, Arcavacata Di Rende, Italy. [Capua, M.; Crosetti, G.; La Rotonda, L.; Mastroberardino, A.; Policicchio, A.; Salvatore, D.; Scarfone, V.; Schioppa, M.; Susinno, G.; Tassi, E.] Univ Calabria, Dipartimento Fis, I-87036 Arcavacata Di Rende, Italy. [Adamczyk, L.; Bold, T.; Dabrowski, W.; Dwuznik, M.; Dyndal, M.; Grabowska-Bold, I.; Kisielewska, D.; Knue, A.; Koperny, S.; Kowalski, T. Z.; Mindur, B.; Przybycien, M.; Zemla, A.] AGH Univ Sci & Technol, Fac Phys & Appl Comp Sci, Krakow, Poland. [Palka, M.] Jagiellonian Univ, Marian Smoluchowski Inst Phys, Krakow, Poland. [Banas, E.; de Renstrom, P. A. Bruckman; Chwastowski, J. J.; Derendarz, D.; Gornicki, E.; Hajduk, Z.; Iwanski, W.; Kaczmarska, A.; Korcyl, K.; Malecki, Pa.; Olszewski, A.; Olszowska, J.; Stanecka, E.; Staszewski, R.; Trzebinski, M.; Trzupek, A.; Wolter, M. W.; Wosiek, B. K.; Wozniak, K. W.; Zabinski, B.] Polish Acad Sci, Henryk Niewodniczanski Inst Nucl Phys, Krakow, Poland. [Cao, T.; Firan, A.; Hoffman, J.; Kama, S.; Kehoe, R.; Randle-Conde, A. S.; Sekula, S. J.; Stroynowski, R.; Turvey, A. J.; Wang, H.; Ye, J.] So Methodist Univ, Dept Phys, Dallas, TX 75275 USA. [Izen, J. M.; Leyton, M.; Lou, X.; Namasivayam, H.; Reeves, K.] Univ Texas Dallas, Dept Phys, Dallas, TX 75230 USA. [Argyropoulos, S.; Asbah, N.; Bessner, M.; Bloch, I.; Borroni, S.; Camarda, S.; Dassoulas, J.; Deterre, C.; Dietrich, J.; Filipuzzi, M.; Friedrich, C.; Glazov, A.; Fajardo, L. S. Gomez; Grahn, K-J.; Gregor, I. M.; Grohsjean, A.; Haleem, M.; Hamnett, P. G.; Hengler, C.; Hiller, K. H.; Howarth, J.; Huang, Y.; Belenguer, M. Jimenez; Katzy, J.; Keller, J. S.; Kondrashova, N.; Kuhl, T.; Lisovyi, M.; Lobodzinska, E.; Lohwasser, K.; Medinnis, M.; Monig, K.; Garcia, R. F. Naranjo; Naumann, T.; Peschke, R.; Petit, E.; Radescu, V.; Rubinskiy, I.; Schaefer, R.; Sedov, G.; Shushkevich, S.; South, D.; Stanescu-Bellu, M.; Stanitzki, M. M.; Starovoitov, P.; Styles, N. A.; Tackmann, K.; Vankov, P.; Wang, J.; Wasicki, C.; Wildt, M. A.; Yatsenko, E.; Yildirim, E.] DESY, Hamburg, Germany. [Argyropoulos, S.; Asbah, N.; Bessner, M.; Bloch, I.; Borroni, S.; Camarda, S.; Dassoulas, J.; Deterre, C.; Dietrich, J.; Filipuzzi, M.; Friedrich, C.; Glazov, A.; Fajardo, L. S. Gomez; Grahn, K-J.; Gregor, I. M.; Grohsjean, A.; Haleem, M.; Hamnett, P. G.; Hengler, C.; Hiller, K. H.; Howarth, J.; Huang, Y.; Belenguer, M. Jimenez; Katzy, J.; Keller, J. S.; Kondrashova, N.; Kuhl, T.; Lisovyi, M.; Lobodzinska, E.; Lohwasser, K.; Medinnis, M.; Monig, K.; Garcia, R. F. Naranjo; Naumann, T.; Peschke, R.; Petit, E.; Radescu, V.; Rubinskiy, I.; Schaefer, R.; Sedov, G.; Shushkevich, S.; South, D.; Stanescu-Bellu, M.; Stanitzki, M. M.; Starovoitov, P.; Styles, N. A.; Tackmann, K.; Vankov, P.; Wang, J.; Wasicki, C.; Wildt, M. A.; Yatsenko, E.; Yildirim, E.] DESY, Zeuthen, Germany. [Burmeister, I.; Esch, H.; Gossling, C.; Jentzsch, J.; Jung, C. A.; Klingenberg, R.; Wittig, T.] Tech Univ Dortmund, Inst Expt Phys 4, Dortmund, Germany. [Anger, P.; Friedrich, F.; Grohs, J. P.; Gumpert, C.; Hauswald, L.; Kobel, M.; Mader, W. F.; Morgenstern, M.; Novgorodova, O.; Pohl, M.; Rudolph, C.; Schnoor, U.; Siegert, F.; Socher, F.; Staerz, S.; Straessner, A.; Vest, A.; Wahrmund, S.] Tech Univ Dresden, Inst Kern & Teilchenphys, D-01062 Dresden, Germany. [Arce, A. T. H.; Benjamin, D. P.; Bocci, A.; Cerio, B. C.; Kajomovitz, E.; Kotwal, A.; Kruse, M. C.; Li, L.; Li, S.; Liu, M.; Oh, S. H.; Pollard, C. S.; Wang, C.] Duke Univ, Dept Phys, Durham, NC 27706 USA. [Bhimji, W.; Bristow, T. M.; Clark, P. J.; Dias, F. A.; Edwards, N. C.; Walls, F. M. Garay; Glaysher, P. C. F.; Harrington, R. D.; Leonidopoulos, C.; Martin, V. J.; Mills, C.; O'Brien, B. J.; Okamura, W.; Pino, S. A. Olivares; Proissl, M.; Selbach, K. E.; Smart, B. H.; Washbrook, A.; Wynne, B. M.] Univ Edinburgh, Sch Phys & Astron, SUPA, Edinburgh, Midlothian, Scotland. [Annovi, A.; Antonelli, M.; Bilokon, H.; Curatolo, M.; Di Nardo, R.; Esposito, B.; Gatti, C.; Laurelli, P.; Maccarrone, G.; Prokofiev, K.; Sansoni, A.; Testa, M.; Vilucchi, E.] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy. [Amoroso, S.; Arnold, H.; Betancourt, C.; Boehler, M.; Bruneliere, R.; Buehrer, F.; Buscher, D.; Coniavitis, E.; Consorti, V.; Dao, V.; Di Simone, A.; Fehling-Kaschek, M.; Flechl, M.; Giuliani, C.; Herten, G.; Jakobs, K.; Javurek, T.; Jenni, P.; Kiss, F.; Koneke, K.; Kopp, A. K.; Kuehn, S.; Lai, S.; Landgraf, U.; Madar, R.; Mahboubi, K.; Mohr, W.; Pagacova, M.; Parzefall, U.; Rave, T. C.; Ronzani, M.; Ruhr, F.; Rurikova, Z.; Ruthmann, N.; Schillo, C.; Schmidt, E.; Schumacher, M.; Sommer, P.; Sundermann, J. E.; Temming, K. K.; Tsiskaridze, V.; Ungaro, F. C.; von Radziewski, H.; Anh, T. Vu; Warsinsky, M.; Weiser, C.; Werner, M.; Zimmermann, S.] Univ Freiburg, Fak Math & Phys, D-79106 Freiburg, Germany. [Alexandre, G.; Ancu, L. S.; Barone, G.; Bell, P. J.; Bell, W. H.; Noccioli, E. Benhar; De Mendizabal, J. Bilbao; Bucci, F.; Toro, R. Camacho; Clark, A.; Delitzsch, C. M.; della Volpe, D.; Doglioni, C.; Ferrere, D.; Gadomski, S.; Gonzalez-Sevilla, S.; Goulette, M. P.; Gramling, J.; Guescini, F.; Iacobucci, G.; Katre, A.; La Rosa, A.; Merola, L.; Muenstermann, D.; Nektarijevic, S.; Nikolics, K.; Picazio, A.; Rosbach, K.; Tykhonov, A.; Vallecorsa, S.; Wu, X.] Univ Geneva, Sect Phys, Geneva, Switzerland. [Barberis, D.; Darbo, G.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Gemme, C.; Guido, E.; Morettini, P.; Osculati, B.; Parodi, F.; Passaggio, S.; Rossi, L. P.; Schiavi, C.] Ist Nazl Fis Nucl, Sez Genova, I-16146 Genoa, Italy. [Barberis, D.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Guido, E.; Osculati, B.; Parodi, F.; Schiavi, C.] Univ Genoa, Dipartimento Fis, Genoa, Italy. [Jejelava, J.; Tskhadadze, E. G.] Iv Javakhishvili Tbilisi State Univ, E Andronikashvili Inst Phys, Tbilisi, Rep of Georgia. [Djobava, T.; Durglishvili, A.; Khubuab, J.; Mosidze, M.] Tbilisi State Univ, Inst High Energy Phys, GE-380086 Tbilisi, Rep of Georgia. [Duren, M.; Kreutzfeldt, K.; Stenzel, H.] Univ Giessen, Inst Phys 2, D-35390 Giessen, Germany. [Bates, R. L.; Britton, D.; Buckley, A. G.; Bussey, P.; Buttar, C. M.; Buzatu, A.; Cinca, D.; D'Auria, S.; Doherty, T.; Doyle, A. T.; Ferrag, S.; Ferrando, J.; de Lima, D. E. Ferreira; Gemmell, A.; Gul, U.; Ortiz, N. G. Gutierrez; Kar, D.; Knue, A.; O'Shea, V.; Barrera, C. Oropeza; Qin, G.; Quilty, D.; Ravenscroft, T.; Robson, A.; Saxon, D. H.; Smith, K. M.; Denis, R. D. St.; Stewart, G. A.; Thompson, A. S.; Wright, M.] Univ Glasgow, Sch Phys & Astron, SUPA, Glasgow, Lanark, Scotland. [Bierwagen, K.; Bindi, M.; Blumenschein, U.; George, M.; Graber, L.; Grosse-Knetter, J.; Hamer, M.; Kareem, M. J.; Kawamura, G.; Keil, M.; Kroeninger, K.; Lemmer, B.; Magradze, E.; Mchedlidze, G.; Llacer, M. Moreno; Musheghyan, H.; Nackenhorst, O.; Nadal, J.; Quadt, A.; Rieger, J.; Schorlemmer, A. L. S.; Serkin, L.; Shabalina, E.; Stolte, P.; Schroeder, T. Vazquez; Weingarten, J.; Zinonos, Z.] Univ Gottingen, Inst Phys 2, D-37073 Gottingen, Germany. [Albrand, S.; Brown, J.; Collot, J.; Crepe-Renaudin, S.; Dechenaux, B.; Delsart, P. A.; Gabaldon, C.; Genest, M. H.; Hostachy, J-Y.; Ledroit-Guillon, F.; Lleres, A.; Lucotte, A.; Malek, F.; Monini, C.; Stark, J.; Trocme, B.; Wu, M.] Univ Grenoble Alpes, CNRS, IN2P3, Lab Phys Subatom & Cosmol, Grenoble, France. [McFarlane, K. W.] Hampton Univ, Dept Phys, Hampton, VA 23668 USA. [da Costa, J. Barreiro Guimaraes; Butler, B.; Catastini, P.; Conventi, F.; Franklin, M.; Huth, J.; Ippolito, V.; Mateos, D. Lopez; Mergelmeyer, S.; Morii, M.; Skottowe, H. P.; Spearman, W. R.; Sun, S.; Tolley, E.; Yen, A. L.; della Porta, G. Zevi] Harvard Univ, Lab Particle Phys & Cosmol, Cambridge, MA 02138 USA. [Andrei, V.; Baas, A. E.; Brandt, O.; Davygora, Y.; Dietzsch, T. A.; Djuvsland, J. I.; Dunford, M.; Hanke, P.; Jongmanns, J.; Khomich, A.; Kluge, E. -E.; Laier, H.; Lang, V. S.; Meier, K.; Mueller, F.; Poddar, S.; Scharf, V.; Schultz-Coulon, H. -C.; Stamen, R.; Wessels, M.] Heidelberg Univ, Kirchhoff Inst Phys, Heidelberg, Germany. [Anders, C. F.; Giulini, M.; Kasieczka, G.; Narayan, R.; Schaetzel, S.; Schmitt, S.; Schoening, A.] Heidelberg Univ, Inst Phys, Heidelberg, Germany. [Colombo, T.; Kretz, M.; Kugel, A.] Heidelberg Univ, ZITI Inst Tech Informat, Mannheim, Germany. [Nagasaka, Y.] Hiroshima Inst Technol, Fac Appl Informat Sci, Hiroshima, Japan. [Bortolotto, V.; Castillo, L. R. Flores] Chinese Univ Hong Kong, Dept Phys, Shatin, Hong Kong, Peoples R China. Univ Hong Kong, Dept Phys, Hong Kong, Hong Kong, Peoples R China. Hong Kong Univ Sci & Technol, Dept Phys, Kowloon, Hong Kong, Peoples R China. [Brunet, S.; Dattagupta, A.; Evans, H.; Gagnon, P.; Lammers, S.; Martinez, N. Lorenzo; Luehring, F.; Ogren, H.; Penwell, J.; Poveda, J.; Weinert, B.; Zieminska, D.] Indiana Univ, Dept Phys, Bloomington, IN 47405 USA. [Franz, S.; Jussel, P.; Kneringer, E.; Lukas, W.; Ritsch, E.; Usanova, A.] Leopold Franzens Univ, Inst Astro & Teilchenphys, Innsbruck, Austria. [Mallik, U.; Mandrysch, R.; Morange, N.; Zaidan, R.] Univ Iowa, Iowa City, IA USA. [Chen, C.; Cochran, J.; De Lorenzi, F.; Dudziak, F.; Krumnack, N.; Pluth, D.; Prell, S.; Shrestha, S.; Yamamoto, K.] Iowa State Univ, Dept Phys & Astron, Ames, IA USA. [Ahmadov, F.; Aleksandrov, I. N.; Bednyakov, V. A.; Boyko, I. R.; Budagov, I. A.; Chelkov, G. A.; Cheplakov, A.; Chizhov, M. V.; Dedovich, D. V.; Demichev, M.; Glonti, G. L.; Gostkin, M. I.; Huston, J.; Javadov, N.; Karpov, S. N.; Karpova, Z. M.; Kazarinov, M. Y.; Khramov, E.; Kruchonak, U.; Krumshteyn, Z. V.; Kukhtin, V.; Ladygin, E.; Minashvili, I. A.; Mineev, M.; Olchevski, A. G.; Peshekhonov, V. D.; Plotnikova, E.; Potrap, I. N.; Pozdnyakov, V.; Rusakovich, N. A.; Sadykov, R.; Sapronov, A.; Shiyakova, M.; Sisakyan, A. N.; Soloshenko, A.; Topilin, N. D.; Vinogradov, V. B.; Yeletskikh, I.; Zhemchugov, A.; Zimine, N. I.] JINR Dubna, Joint Inst Nucl Res, Dubna, Russia. [Amako, K.; Aoki, M.; Arai, Y.; Ikegami, Y.; Ikeno, M.; Iwasaki, H.; Kanzaki, J.; Kohriki, T.; Kondo, T.; Kono, T.; Makida, Y.; Nagano, K.; Nakamura, K.; Nozaki, M.; Odaka, S.; Sasaki, O.; Suzuki, Y.; Takubo, Y.; Tanaka, S.; Terada, S.; Tokushuku, K.; Tsuno, S.; Unno, Y.; Yamada, M.; Yamamoto, A.; Yasu, Y.] High Energy Accelerator Res Org, KEK, Tsukuba, Ibaraki, Japan. [Aloisio, A.; Chen, Y.; Hasegawa, M.; Inamaru, Y.; Kishimoto, T.; Kurashige, H.; Kurumida, R.; Ochi, A.; Shimizu, S.; Takeda, H.; Yakabe, R.; Yamazaki, Y.; Yuan, L.] Kobe Univ, Grad Sch Sci, Kobe, Hyogo, Japan. [Ishino, M.; Sumida, T.; Tashiro, T.] Kyoto Univ, Fac Sci, Kyoto, Japan. [Takashima, R.] Kyoto Univ, Kyoto 612, Japan. [Kawagoe, K.; Oda, S.; Otono, H.; Tojo, J.] Kyushu Univ, Dept Phys, Fukuoka 812, Japan. [Verzini, M. J. Alconada; Alonso, F.; Anduaga, X. S.; Arduh, F. A.; Dova, M. T.; Monticelli, F.; Wahlberg, H.] Univ Nacl La Plata, Inst Fis La Plata, La Plata, Argentina. [Verzini, M. J. Alconada; Alonso, F.; Anduaga, X. S.; Arduh, F. A.; Dova, M. T.; Monticelli, F.; Wahlberg, H.] Consejo Nacl Invest Cient & Tecn, La Plata, Argentina. [Allison, L. J.; Barton, A. E.; Beattie, M. D.; Borissov, G.; Bouhova-Thacker, E. V.; Chilingarov, A.; Dearnaley, W. J.; Fox, H.; Grimm, K.; Henderson, R. C. W.; Hughes, G.; Jones, R. W. L.; Kartvelishvili, V.; Long, R. E.; Love, P. A.; Maddocks, H. J.; Smizanska, M.; Walder, J.] Univ Lancaster, Dept Phys, Lancaster, England. [Chiodini, G.; Gorini, E.; Orlando, N.; Perrino, R.; Primavera, M.; Spagnolo, S.; Ventura, A.] Ist Nazl Fis Nucl, Sez Lecce, I-73100 Lecce, Italy. [Chiodini, G.; Gorini, E.; Orlando, N.; Perrino, R.; Primavera, M.; Spagnolo, S.; Ventura, A.] Univ Salento, Dipartimento Matemat Fis, Lecce, Italy. [Allport, P. P.; Bundock, A. C.; Burdin, S.; D'Onofrio, M.; Dervan, P.; Gwilliam, C. B.; Hayward, H. S.; Jackson, M.; Jones, T. J.; King, B. T.; Klein, M.; Klein, U.; Kretzschmar, J.; Laycock, P.; Lehan, A.; Mahmoud, S.; Maxfield, S. J.; Mehta, A.; Migas, S.; Price, J.; Readioff, N. P.; Schnellbach, Y. J.; Sellers, G.; Vossebeld, J. H.; Waller, P.] Univ Liverpool, Oliver Lodge Lab, Liverpool L69 3BX, Merseyside, England. [Cindro, V.; Deliyergiyev, M.; Filipcic, A.; Gorisek, A.; Kersevan, B. P.; Kramberger, G.; Mandic, I.; Mikuz, M.; Sfiligoj, T.] Jozef Stefan Inst, Dept Phys, Ljubljana, Slovenia. [Alpigiani, C.; Bona, M.; Bret, M. Cano; Cerrito, L.; Fletcher, G.; Goddard, J. R.; Hickling, R.; Landon, M. P. J.; Lloyd, S. L.; Morris, J. D.; Piccaro, E.; Rizvi, E.; Sandbach, R. L.; Snidero, G.; Castanheira, M. Teixeira Dias] Queen Mary Univ London, Sch Phys & Astron, London, England. [Berry, T.; Boisvert, V.; Brooks, T.; Connelly, I. A.; Copic, K.; Cowan, G.; Duguid, L.; George, S.; Gibson, S. M.; Kempster, J. J.; Vazquez, J. G. 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W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Vannucci, F.; Varouchas, D.] UPMC, Lab Phys Nucl & Hautes Energies, Paris, France. [Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; Davignon, O.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Vannucci, F.; Varouchas, D.] Univ Paris Diderot, Paris, France. [Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; Davignon, O.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Vannucci, F.; Varouchas, D.] CNRS, IN2P3, Paris, France. [Akesson, T. P. A.; Bocchetta, S. S.; Bryngemark, L.; Floderus, A.; Hawkins, A. D.; Hedberg, V.; Ivarsson, J.; Jarlskog, G.; Lytken, E.; Meirose, B.; Mjornmark, J. U.; Smirnova, O.; Viazlo, O.] Lund Univ, Fysiska Inst, Lund, Sweden. [Arnal, V.; Barreiro, F.; Cantero, J.; De la Torre, H.; Del Peso, J.; Glasman, C.; Merino, J. Llorente; Terron, J.] Univ Autonoma Madrid, Dept Fis Teor C 15, Madrid, Spain. [Blum, W.; Buscher, V.; Caputo, R.; Caudron, J.; Ellinghaus, F.; Endner, O. C.; Ertel, E.; Fiedler, F.; Torregrosa, E. Fullana; Goeringer, C.; Heck, T.; Hohlfeld, M.; Hsu, P. J.; Hulsing, T. A.; Karnevskiy, M.; Kleinknecht, K.; Konig, S.; Kopke, L.; Lin, T. H.; Lungwitz, M.; Masetti, L.; Mattmann, J.; Meyer, C.; Moreno, D.; Moritz, S.; Mueller, T.; Poettgen, R.; Sander, H. G.; Schafer, U.; Schmitt, C.; Schott, M.; Schroeder, C.; Schuh, N.; Simioni, E.; Tapprogge, S.; Wollstadt, S. J.; Zimmermann, C.] Johannes Gutenberg Univ Mainz, Inst Phys, Mainz, Germany. [Barnes, S. L.; Borri, M.; Cox, B. E.; Da Via, C.; Forti, A.; Ponce, J. M. Iturbe; Joshi, K. D.; Klinger, J. A.; Loebinger, F. K.; Marsden, S. P.; Masik, J.; Neep, T. J.; Oh, A.; Owen, M.; Pater, J. R.; Peters, R. F. Y.; Price, D.; Qin, Y.; Queitsch-Maitland, M.; Robinson, J. E. M.; Schwanenberger, C.; Thompson, R. J.; Tomlinson, L.; Watts, S.; Webb, S.; Woudstra, M. J.; Wyatt, T. R.; Yang, U. K.] Univ Manchester, Sch Phys & Astron, Manchester, Lancs, England. [Aad, G.; Alio, L.; Barbero, M.; Bertella, C.; Clemens, J. C.; Coadou, Y.; Diglio, S.; Djama, F.; Feligioni, L.; Hoffmann, D.; Hubaut, F.; Knoops, E. B. F. G.; Le Guirriec, E.; Li, B.; Madaffari, D.; Mochizuki, K.; Monnier, E.; Muanza, S.; Nagai, Y.; Pralavorio, P.; Rozanov, A.; Serre, T.; Talby, M.; Tiouchichine, E.; Tisserant, S.; Toth, J.; Touchard, F.; Ughetto, M.; Vacavant, L.] Aix Marseille Univ, CPPM, Marseille, France. [Aad, G.; Alio, L.; Barbero, M.; Bertella, C.; Clemens, J. C.; Coadou, Y.; Diglio, S.; Djama, F.; Feligioni, L.; Hoffmann, D.; Hubaut, F.; Knoops, E. B. F. G.; Le Guirriec, E.; Li, B.; Madaffari, D.; Mochizuki, K.; Monnier, E.; Muanza, S.; Nagai, Y.; Pralavorio, P.; Rozanov, A.; Serre, T.; Talby, M.; Tiouchichine, E.; Tisserant, S.; Toth, J.; Touchard, F.; Ughetto, M.; Vacavant, L.] CNRS, IN2P3, Marseille, France. [Bellomo, M.; Brau, B.; Dallapiccola, C.; Daya-Ishmukhametova, R. K.; Koffas, T.; Moyse, E. J. W.; Pais, P.; Pueschel, E.; Varol, T.; Ventura, D.; Willocq, S.] Univ Massachusetts, Dept Phys, Amherst, MA 01003 USA. [Belanger-Champagne, C.; Chapleau, B.; Cheatham, S.; Corso-Radu, A.; Mantifel, R.; Robertson, S. H.; Robichaud-Veronneau, A.; Stockton, M. C.; Stoebe, M.; Vachon, B.; Wang, K.; Warburton, A.] McGill Univ, Dept Phys, Montreal, PQ, Canada. [Barberio, E. L.; Brennan, A. J.; Jennens, D.; Kubota, T.; Hanninger, G. Nunes; Nuti, F.; Rados, P.; Spiller, L. A.; Tan, K. G.; Taylor, G. N.; Thong, W. M.; Urquijo, P.; Volpi, M.; Zanzi, D.] Univ Melbourne, Sch Phys, Melbourne, Vic 3010, Australia. [Amidei, D.; Chelstowska, M. A.; Cheng, H. C.; Dai, T.; Diehl, E. B.; Dubbert, J.; Feng, H.; Ferretti, C.; Goldfarb, S.; Harper, D.; Hu, X.; Levin, D.; Liu, L.; Long, J. D.; Lu, N.; Mc Kee, S. P.; McCarn, A.; Neal, H. A.; Panikashvili, N.; Qian, J.; Searcy, J.; Thun, R. P.; Wilson, A.; Wu, Y.; Yu, J. M.; Zhang, D.; Zhou, B.; Zhu, J.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA. [Abolins, M.; Gonzalez, B. Alvarez; Arabidze, G.; Brock, R.; Bromberg, C.; Chegwidden, A.; Fisher, W. C.; Halladjian, G.; Hauser, R.; Hayden, D.; Huston, J.; Koll, J.; Linnemann, J. T.; Martin, B.; Pope, B. G.; Schoenrock, B. D.; Schwienhorst, R.; Ta, D.; Tollefson, K.; True, P.; Willis, C.; Zhang, H.] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA. [Alimonti, G.; Andreazza, A.; Besana, M. I.; Carminati, L.; Cavalli, D.; Citterio, M.; Consonni, S. M.; Costa, G.; Fanti, M.; Giugni, D.; Lari, T.; Mandelli, L.; Merritt, F. S.; Perini, L.; Pizio, C.; Ragusa, F.; Resconi, S.; Simoniello, R.; Tartarelli, G. F.; Troncon, C.; Turra, R.; Perez, M. Villaplana] Ist Nazl Fis Nucl, Sez Milano, I-20133 Milan, Italy. [Andreazza, A.; Carminati, L.; Consonni, S. M.; Fanti, M.; Perini, L.; Pizio, C.; Ragusa, F.; Simoniello, R.; Turra, R.; Perez, M. Villaplana] Univ Milan, Dipartimento Fis, Milan, Italy. [Bogouch, A.; Harkusha, S.; Kulchitsky, Y.; Kurochkin, Y. A.; Tsiareshka, P. V.] Natl Acad Sci Belarus, BI Stepanov Inst Phys, Minsk, Byelarus. 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V.; Kramarenko, V. A.; Maevskiy, A.; Rud, V. I.; Sivoklokov, S. Yu.; Smirnova, L. N.; Turchikhin, S.] Moscow MV Lomonosov State Univ, DV Skobeltsyn Inst Nucl Phys, Moscow, Russia. [Adomeit, S.; Becker, S.; Biebel, O.; Bock, C.; Bortfeldt, J.; Calfayan, P.; Chow, B. K. B.; Duckeck, G.; Ebke, J.; Elmsheuser, J.; Heller, C.; Hertenberger, R.; Hoenig, F.; Legger, F.; Lorenz, J.; Mann, A.; Mehlhase, S.; Meineck, C.; Mitrevski, J.; Nunnemann, T.; Rauscher, F.; Ruschke, A.; Sanders, M. P.; Schaile, D.; Schieck, J.; Unverdorben, C.; Vladoiu, D.; Walker, R.; Wittkowski, J.] Univ Munich, Fak Phys, Munich, Germany. [Barillari, T.; Bethke, S.; Bronner, J.; Compostella, G.; Cortiana, G.; Flowerdew, M. J.; Goblirsch-Kolb, M.; Ince, T.; Kiryunin, A. E.; Kluth, S.; Kneringer, E.; Kortner, O.; Kortner, S.; Kroha, H.; Macchiolo, A.; Maier, A. A.; Manfredini, A.; Meoni, E.; Moser, H. G.; Nagel, M.; Nisius, R.; Nowak, S.; Oberlack, H.; Pahl, C.; Richter, R.; Salihagic, D.; Sandstroem, R.; Schacht, P.; Schwegler, Ph.; Sforza, F.; Spettel, F.; Stern, S.; Stonjek, S.; Terzo, S.; von der Schmitt, H.; Wildauer, A.] Max Planck Inst Phys & Astrophys, Werner Heisenberg Inst, D-80805 Munich, Germany. [Shimojima, M.] Nagasaki Inst Appl Sci, Nagasaki, Japan. [Hasegawa, S.; Horii, Y.; Morvaj, L.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Grad Sch Sci, Nagoya, Aichi 4648601, Japan. [Hasegawa, S.; Horii, Y.; Morvaj, L.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Kobayashi Maskawa Inst, Nagoya, Aichi 4648601, Japan. [Aloisio, A.; Alviggi, M. G.; Canale, V.; Carlino, G.; Chiefari, G.; Cooke, M.; de Asmundis, R.; Di Donato, C.; Doria, A.; Giordano, R.; Iengo, P.; Izzo, V.; Meroni, C.; Patricelli, S.; Perrella, S.; Rossi, E.; Sanchez, A.; Sekhniaidze, G.; Zurzolo, G.] Ist Nazl Fis Nucl, Sez Napoli, I-80125 Naples, Italy. [Aloisio, A.; Alviggi, M. G.; Canale, V.; Chiefari, G.; Di Donato, C.; Giordano, R.; Meroni, C.; Patricelli, S.; Perrella, S.; Rossi, E.; Sanchez, A.; Zurzolo, G.] Univ Naples Federico II, Dipartimento Fis, Naples, Italy. [Gorelov, I.; Hoeferkamp, M. R.; Seidel, S. C.; Toms, K.; Wang, R.] Univ New Mexico, Dept Phys & Astron, Albuquerque, NM 87131 USA. [Besjes, G. J.; Caron, S.; Chekulaev, S. V.; Croft, V.; De Groot, N.; Filthaut, F.; Fortin, D.; Galea, C.; Klok, P. F.; Kneringer, E.; Konig, A. C.; Ramos, J. A. Manjarres; Palacino, G.; Codina, E. Perez; Salvucci, A.; Seuster, R.; Strubig, A.] Radboud Univ Nijmegen, Nikhef, Inst Math Astrophys & Particle Phys, Nijmegen, Netherlands. [Aben, R.; Angelozzi, I.; Beemster, L. J.; Bentvelsen, S.; Berge, D.; Bobbink, G. J.; Bos, K.; Boterenbrood, H.; Butti, P.; Castelli, A.; Colijn, A. P.; de Jong, P.; De Nooij, L.; Deigaard, I.; Deluca, C.; Deviveiros, P. O.; Dhaliwal, S.; Ferrari, P.; Gadatsch, S.; Geerts, D. A. A.; Hartjes, F.; Hessey, N. P.; Hod, N.; Igonkina, O.; Kluit, P.; Koffeman, E.; Lee, H.; Linde, F.; Mahlstedt, J.; Mechnich, J.; Oussoren, K. P.; Pani, P.; Sabato, G.; Salek, D.; Slawinska, M.; Valencic, N.; Van Den Wollenberg, W.; Van Der Deijl, P. C.; van der Geer, R.; van der Graaf, H.; Van der Leeuw, R.; Verkerke, W.; Vermeulen, J. C.; Vreeswijk, M.; Weits, H.] Nikhef, Natl Inst Subat Phys, Amsterdam, Netherlands. [Aben, R.; Angelozzi, I.; Beemster, L. J.; Bentvelsen, S.; Berge, D.; Bobbink, G. J.; Bos, K.; Boterenbrood, H.; Butti, P.; Castelli, A.; Colijn, A. P.; de Jong, P.; De Nooij, L.; Deigaard, I.; Deluca, C.; Deviveiros, P. O.; Dhaliwal, S.; Ferrari, P.; Gadatsch, S.; Geerts, D. A. A.; Hartjes, F.; Hessey, N. P.; Hod, N.; Igonkina, O.; Kluit, P.; Koffeman, E.; Lee, H.; Linde, F.; Mahlstedt, J.; Mechnich, J.; Oussoren, K. P.; Pani, P.; Sabato, G.; Salek, D.; Slawinska, M.; Valencic, N.; Van Den Wollenberg, W.; Van Der Deijl, P. C.; van der Geer, R.; van der Graaf, H.; Van der Leeuw, R.; Verkerke, W.; Vermeulen, J. C.; Vreeswijk, M.; Weits, H.] Univ Amsterdam, Amsterdam, Netherlands. [Burghgrave, B.; Calkins, R.; Chakraborty, D.; Cole, S.; Suhr, C.; Yurkewicz, A.; Zutshi, V.] No Illinois Univ, Dept Phys, De Kalb, IL USA. [Anisenkov, A. V.; Bobrovnikov, V. S.; Bogdanchikov, A. G.; Kazanin, V. F.; Korol, A. A.; Malyshev, V. M.; Maslennikov, A. L.; Maximov, D. A.; Peleganchuk, S. V.; Rezanova, O. L.; Skovpen, K. Yu.; Soukharev, A. M.; Talyshev, A. A.; Tikhonov, Yu. A.] SB RAS, Budker Inst Nucl Phys, Novosibirsk, Russia. [Cranmer, K.; Haas, A.; Heinrich, L.; van Huysduynen, L. Hooft; Kaplan, B.; Karthik, K.; Konoplich, R.; Kreiss, S.; Lewis, G. H.; Meroni, C.; Mincer, A. I.; Nemethy, P.; Neves, R. M.] NYU, Dept Phys, New York, NY USA. [Gan, K. K.; Ishmukhametov, R.; Kagan, H.; Kass, R. D.; Merritt, H.; Moss, J.; Nagarkar, A.; Pignotti, D. T.; Tannenwald, B. B.; Yang, Y.] Ohio State Univ, Columbus, OH 43210 USA. [Nakano, I.] Okayama Univ, Fac Sci, Okayama 700, Japan. [Abbott, B.; Alhroob, M.; Bertsche, C.; Bertsche, D.; Gutierrez, P.; Hasib, A.; Norberg, S.; Saleem, M.; Severini, H.; Skubic, P.; Strauss, M.] Univ Oklahoma, Homer L Dodge Dept Phys & Astron, Norman, OK 73019 USA. [Abi, B.; Bousson, N.; Donszelmann, T. Cuhadar; Khanov, A.; Rizatdinova, F.; Sidorov, D.; Yu, J.] Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USA. [Chytka, L.; Hamal, P.; Hrabovsky, M.; Kvita, J.; Nozka, L.] Palacky Univ, RCPTM, CR-77147 Olomouc, Czech Republic. [Brau, J. E.; Brost, E.; Hopkins, W. H.; Majewski, S.; Potter, C. T.; Ptacek, E.; Radloff, P.; Shamim, M.; Sinev, N. B.; Strom, D. M.; Torrence, E.; Wanotayaroj, C.; Winklmeier, F.] Univ Oregon, Ctr High Energy Phys, Eugene, OR 97403 USA. [Khalek, S. Abdel; Adelman, J.; Becot, C.; Binet, S.; Bourdarios, C.; Charfeddine, D.; De Vivie De Regie, J. B.; Duflot, L.; Escalier, M.; Fayard, L.; Fournier, D.; Gkougkousis, E. L.; Grivaz, J. -F.; Guillemin, T.; Hariri, F.; Henrot-Versille, S.; Hrivnac, J.; Iconomidou-Fayard, L.; Kado, M.; Lounis, A.; Makovec, N.; Nellist, C.; Poggioli, L.; Puzo, P.; Renaud, A.; Rousseau, D.; Rybkin, G.; Schaffer, A. C.; Scifo, E.; Serin, L.; Simion, S.; Tanaka, R.; Tran, H. L.; Zerwas, D.; Zhang, Z.] Univ Paris 11, LAL, Orsay, France. [Khalek, S. Abdel; Adelman, J.; Aloisio, A.; Alonso, A.; Altheimer, A.; Amorim, A.; Andreazza, A.; Becot, C.; Binet, S.; Bourdarios, C.; Charfeddine, D.; De Vivie De Regie, J. B.; Duflot, L.; Escalier, M.; Fayard, L.; Fournier, D.; Gkougkousis, E. L.; Grivaz, J. -F.; Guillemin, T.; Hariri, F.; Henrot-Versille, S.; Hrivnac, J.; Iconomidou-Fayard, L.; Kado, M.; Lounis, A.; Makovec, N.; Nellist, C.; Poggioli, L.; Puzo, P.; Renaud, A.; Rousseau, D.; Rybkin, G.; Schaffer, A. C.; Scifo, E.; Serin, L.; Simion, S.; Tanaka, R.; Tran, H. L.; Zerwas, D.; Zhang, Z.] CNRS, IN2P3, F-91405 Orsay, France. [Endo, M.; Hanagaki, K.; Lee, J. S. H.; Nomachi, M.; Sugaya, Y.; Teoh, J. J.; Yamaguchi, Y.] Osaka Univ, Grad Sch Sci, Osaka, Japan. [Bugge, L.; Bugge, M. K.; Cameron, D.; Catmore, J. R.; Franconi, L.; Gjelsten, B. K.; Gramstad, E.; Morisbak, V.; Ould-Saada, F.; Pajchel, K.; Pedersen, M.; Read, A. L.; Rohne, O.; Stapnes, S.; Strandlie, A.] Univ Oslo, Dept Phys, Oslo, Norway. [Apolle, R.; Barr, A. J.; Behr, K.; Boddy, C. R.; Bruni, A.; Buckingham, R. M.; Cooper-Smith, N. J.; Ortuzar, M. Crispin; Dafinca, A.; Davies, E.; Gallas, E. J.; Gupta, S.; Gwenlan, C.; Hall, D.; Hays, C. P.; Henderson, J.; Howard, J.; Huffman, T. B.; Issever, C.; Kalderon, C. W.; King, R. S. B.; Kogan, L. A.; Lewis, A.; Nagai, K.; Nickerson, R. B.; Pachal, K.; Pinder, A.; Ryder, N. C.; Sawyer, C.; Short, D.; Tseng, J. C-L.; Viehhauser, G. H. A.; Weidberg, A. R.; Zhong, J.] Univ Oxford, Dept Phys, Oxford, England. [Conta, C.; Dondero, P.; Ferrari, R.; Fraternali, M.; Gaudio, G.; Geich-Gimbel, Ch.; Livan, M.; Negri, A.; Polesello, G.; Rebuzzi, D. M.; Rimoldi, A.; Vercesi, V.] Univ Pavia, INFN Sez Pavia, I-27100 Pavia, Italy. [Conta, C.; Dondero, P.; Ferrari, R.; Fraternali, M.; Gaudio, G.; Geich-Gimbel, Ch.; Livan, M.; Negri, A.; Polesello, G.; Rebuzzi, D. M.; Rimoldi, A.; Vercesi, V.] Univ Pavia, Dipartimento Fis, I-27100 Pavia, Italy. [Brendlinger, K.; Heim, S.; Hines, E.; Hong, T. M.; Jackson, B.; Kroll, J.; Kunkle, J.; Lester, C. M.; Lipeles, E.; Meyer, C.; Ospanov, R.; Saxon, J.; Stahlman, J.; Thomson, E.; Tuna, A. N.; Vanguri, R.; Williams, H. H.] Univ Penn, Dept Phys, Philadelphia, PA 19104 USA. [Ezhilov, A.; Fedin, O. L.; Gratchev, V.; Grebenyuk, O. G.; Levchenko, M.; Maleev, V. P.; Ryabov, Y. F.; Schegelsky, V. A.; Sedykh, E.; Seliverstov, D. M.; Solovyev, V.] Petersburg Nucl Phys Inst, Gatchina, Russia. [Beccherle, R.; Bertolucci, F.; Cavasinni, V.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Leone, S.; Roda, C.; Scuri, F.; Volpi, G.; White, S.] Univ Pisa, INFN Sez Pisa, Pisa, Italy. [Beccherle, R.; Bertolucci, F.; Cavasinni, V.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Leone, S.; Roda, C.; Scuri, F.; Volpi, G.; White, S.] Univ Pisa, Dipartimento Fis E Fermi, Pisa, Italy. [Bianchi, R. M.; Boudreau, J.; Cleland, W.; Escobar, C.; Mueller, J.; Prieur, D.; Sapp, K.; Su, J.; Yoosoofmiya, R.] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA. [Aguilar-Saavedra, J. A.; Dos Santos, S. P. Amor; Amorim, A.; Araque, J. P.; Cantrill, R.; Carvalho, J.; Castro, N. F.; Muino, P. Conde; Da Cunha Sargedas De Sousa, M. J.; Do Valle Wemans, A.; Fiolhais, M. C. N.; Galhardo, B.; Gomes, A.; Goncalo, R.; Jorge, P. M.; Lopes, L.; Miguens, J. Machado; Maio, A.; Maneira, J.; Marques, C. N.; Onofre, A.; Palma, A.; Pedro, R.; Pina, J.; Pinto, B.; Santos, H.; Saraiva, J. G.; Silva, J.; Delgado, A. Tavares; Veloso, F.; Wolters, H.] Lab Instrumentacao & Fis Expt Particulas LIP, Lisbon, Portugal. [Amorim, A.; Muino, P. Conde; Da Cunha Sargedas De Sousa, M. J.; Fiolhais, M. C. N.; Gomes, A.; Jorge, P. M.; Miguens, J. Machado; Maio, A.; Maneira, J.; Palma, A.; Pedro, R.; Pina, J.; Delgado, A. Tavares] Univ Lisbon, Fac Ciencias, P-1699 Lisbon, Portugal. [Dos Santos, S. P. Amor; Carvalho, J.; Galhardo, B.; Veloso, F.; Wolters, H.] Univ Coimbra, Dept Phys, Coimbra, Portugal. [Gomes, A.; Maio, A.; Pina, J.; Saraiva, J. G.; Silva, J.] Univ Lisbon, Ctr Fis Nucl, P-1699 Lisbon, Portugal. [Onofre, A.] Univ Minho, Dept Fis, Braga, Portugal. [Aguilar-Saavedra, J. A.] Univ Granada, Dept Fis Teor & Cosmos, Granada, Spain. [Aguilar-Saavedra, J. A.] Univ Granada, CAFPE, Granada, Spain. [Do Valle Wemans, A.] Univ Nova Lisboa, Dept Fis, Caparica, Portugal. [Do Valle Wemans, A.] Univ Nova Lisboa, Fac Ciencias & Tecnol, CEFITEC, Caparica, Portugal. [Bohm, J.; Chudoba, J.; Havranek, M.; Hejbal, J.; Jakoubek, T.; Kepka, O.; Kupco, A.; Kus, V.; Lokajicek, M.; Lysak, R.; Marcisovsky, M.; Mikestikova, M.; Nemecek, S.; Sicho, P.; Staroba, P.; Svatos, M.; Tasevsky, M.; Vrba, V.] Acad Sci Czech Republic, Inst Phys, Prague, Czech Republic. [Augsten, K.; Gallus, P.; Guenther, J.; Jakubek, J.; Kohout, Z.; Myska, M.; Pospisil, S.; Seifert, F.; Simak, V.; Slavicek, T.; Smolek, K.; Solar, M.; Solc, J.; Sopczak, A.; Sopko, B.; Sopko, V.; Suk, M.; Turecek, D.; Vacek, V.; Vlasak, M.; Vokac, P.; Vykydal, Z.; Zeman, M.] Czech Tech Univ, Prague, Czech Republic. [Balek, P.; Berta, P.; Cerny, K.; Chalupkova, I.; Davidek, T.; Dolejsi, J.; Dolezal, Z.; Faltova, J.; Kodys, P.; Leitner, R.; Pleskot, V.; Reznicek, P.; Rybar, M.; Scheirich, D.; Spousta, M.; Sykora, T.; Tas, P.; Todorova-Nova, S.; Valkar, S.; vorobel, V.] Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic. [Borisov, A.; Denisov, S. P.; Fakhrutdinov, R. M.; Fenyuk, A. B.; Golubkov, D.; Kamenshchikov, A.; Karyukhin, A. N.; Korotkov, V. A.; Kozhin, A. S.; Minaenko, A. A.; Myagkov, A. G.; Nikolaenko, V.; Solodkov, A. A.; Solovyanov, O. V.; Starchenko, E. A.; Zaitsev, A. M.; Zenin, O.] Inst High Energy Phys, State Res Ctr, Protvino, Russia. [Adye, T.; Aloisio, A.; Baines, J. T.; Barnett, B. M.; Burke, S.; Dewhurst, A.; Dopke, J.; Emeliyanov, D.; Gallop, B. J.; Gee, C. N. P.; Haywood, S. J.; Kirk, J.; Martin-Haugh, S.; McCubbin, N. A.; McMahon, S. J.; Middleton, R. P.; Murray, W. J.; Phillips, P. W.; Sankey, D. P. C.; Scott, W. G.; Tyndel, M.; Wickens, F. J.; Wielers, M.] Rutherford Appleton Lab, Particle Phys Dept, Didcot OX11 0QX, Oxon, England. [Tanaka, S.] Ritsumeikan Univ, Shiga, Japan. [Aloisio, A.; Anulli, F.; Bagiacchi, P.; Bagnaia, P.; Bini, C.; Ciapetti, G.; De Pedis, D.; De Salvo, A.; Di Domenico, A.; Falciano, S.; Gabrielli, A.; Gauzzi, P.; Gentile, S.; Giagu, S.; Kuna, M.; Lacava, F.; Luci, C.; Luminari, L.; Marzano, F.; Mirabelli, G.; Monzani, S.; Nisati, A.; Pasqualucci, E.; Petrolo, E.; Pontecorvo, L.; Rescigno, M.; Rosati, S.; Tehrani, F. Safai; Sidoti, A.; Vanadia, M.; Vari, R.; Veneziano, S.; Verducci, M.; Zanello, L.] Univ Roma La Sapienza, INFN Sez Roma, I-00185 Rome, Italy. [Bagiacchi, P.; Bagnaia, P.; Bini, C.; Ciapetti, G.; Di Domenico, A.; Gabrielli, A.; Gauzzi, P.; Gentile, S.; Giagu, S.; Kuna, M.; Lacava, F.; Luci, C.; Monzani, S.; Vanadia, M.; Verducci, M.; Zanello, L.] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy. [Aielli, G.; Cardarelli, R.; Cattani, G.; Di Ciaccio, A.; Grossi, G. C.; Iuppa, R.; Liberti, B.; Mazzaferro, L.; Paolozzi, L.; Salamon, A.; Santonico, R.] Univ Roma Tor Vergata, INFN Sez Roma Tor Vergata, Rome, Italy. [Aielli, G.; Cattani, G.; Di Ciaccio, A.; Grossi, G. C.; Iuppa, R.; Mazzaferro, L.; Paolozzi, L.; Santonico, R.] Univ Roma Tor Vergata, Dipartimento Fis, I-00173 Rome, Italy. [Bacci, C.; Baroncelli, A.; Biglietti, M.; Ceradini, F.; Di Micco, B.; Farilla, A.; Graziani, E.; Iodice, M.; Orestano, D.; Passeri, A.; Pastore, F.; Petrucci, F.; Puddu, D.; Salamanna, G.; Stanescu, C.; Taccini, C.; Trovatelli, M.] Univ Rome Tre, INFN Sez Roma Tre, I-00146 Rome, Italy. [Bacci, C.; Baroncelli, A.; Ceradini, F.; Di Micco, B.; Orestano, D.; Pastore, F.; Petrucci, F.; Puddu, D.; Salamanna, G.; Taccini, C.; Trovatelli, M.] Univ Rome Tre, Dipartimento Matemat & Fis, I-00146 Rome, Italy. [Benchekroun, D.; Boutouil, S.; Chafaq, A.; El Moursli, R. Cherkaoui; Derkaoui, J. E.; El Kacimi, M.; Fassi, F.; Ghazlane, H.; Gouighri, M.; Goujdami, D.; Haddad, N.; Hoummada, A.; Idrissi, Z.; Ouchrif, M.; Tayalati, Y.] Univ Hassan 2, Reseau Univ Phys Hautes Energies, Fac Sci Ain Chock, Casablanca, Morocco. [Ghazlane, H.] Ctr Natl Energie Sci Tech Nucl, Rabat, Morocco. [El Moursli, R. Cherkaoui; Fassi, F.; Haddad, N.; Idrissi, Z.] Univ Cadi Ayyad, LPHEA, Fac Sci Semlalia, Marrakech, Morocco. [Boutouil, S.; Derkaoui, J. E.; Ouchrif, M.; Tayalati, Y.] Univ Mohamed Premier, Fac Sci, Oujda, Morocco. [Boutouil, S.; Derkaoui, J. E.; Ouchrif, M.; Tayalati, Y.] LPTPM, Oujda, Morocco. [El Moursli, R. Cherkaoui; Fassi, F.; Haddad, N.; Idrissi, Z.] Univ Mohammed V Agdal, Fac Sci, Rabat, Morocco. [Bachacou, H.; Balli, F.; Bauer, F.; Besson, N.; Blanchard, J. -B.; Boonekamp, M.; Calandri, A.; Chevalier, L.; Hoffmann, M. Dano; Deliot, F.; Ernwein, J.; Etienvre, A. I.; Formica, A.; Giraud, P. F.; Goncalves Pinto Firmino Da Costa, J.; Guyot, C.; Hanna, R.; Hassani, S.; Kozanecki, W.; Lancon, E.; Laporte, J. F.; Maiani, C.; Mal, P.; Mansoulie, B.; Martinez, H.; Mermod, P.; Meyer, J-P.; Nicolaidou, R.; Ouraou, A.; Protopapadaki, E.; Royon, C. R.; Schoeffel, L.; Schune, Ph.; Schwemling, Ph.; Schwindling, J.; Tsionou, D.; Vranjes, N.; Xiao, M.] CEA Saclay, IRFU, DSM, Commissariat Energie Atom & Energies Alternat, F-91191 Gif Sur Yvette, France. [Battaglia, M.; Debenedetti, C.; Grabas, H. M. X.; Grillo, A. A.; Kuhl, A.; Law, A. T.; Liang, Z.; Litke, A. M.; Lockman, W. S.; Manning, P. M.; Nielsen, J.; Reece, R.; Sadrozinski, H. F-W.; Seiden, A.] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA. [Aloisio, A.; Alonso, A.; Blackburn, D.; Coccaro, A.; Goussiou, A. G.; Harris, O. M.; Hsu, S. -C.; Lubatti, H. J.; Marx, M.; Rompotis, N.; Rosten, R.; Rothberg, J.; De Bruin, P. H. Sales; Watts, G.] Univ Washington, Dept Phys, Seattle, WA 98195 USA. [Anastopoulos, C.; Costanzo, D.; Donszelmann, T. Cuhadar; Dawson, I.; Fletcher, G. T.; Hodgkinson, M. C.; Hodgson, P.; Johansson, P.; Korolkova, E. V.; Paredes, B. Lopez; Miyagawa, P. S.; Paganis, E.; Suruliz, K.; Tovey, D. R.] Univ Sheffield, Dept Phys & Astron, Sheffield, S Yorkshire, England. [Hasegawa, Y.; Takeshita, T.] Shinshu Univ, Dept Phys, Nagano, Japan. [Atlay, N. B.; Buchholz, P.; Czirr, H.; Fleck, I.; Gaur, B.; Ibragimov, I.; Ikematsu, K.; Rosenthal, O.; Walkowiak, W.; Ziolkowski, M.] Univ Siegen, Fachbereich Phys, D-57068 Siegen, Germany. [Buat, Q.; Dawe, E.; O'Neil, D. C.; Stelzer, B.; Tanasijczuk, A. J.; Torres, H.; Van Nieuwkoop, J.; Vetterli, M. C.] Simon Fraser Univ, Dept Phys, Burnaby, BC V5A 1S6, Canada. [Aracena, I.; Mayes, J. Backus; Barklow, T.; Bartoldus, R.; Bawa, H. S.; Black, J. E.; Cogan, J. G.; Eifert, T.; Fulsom, B. G.; Gao, Y. S.; Garelli, N.; Grenier, P.; Kagan, M.; Kocian, M.; Koi, T.; Lowe, A. J.; Malone, C.; Mount, R.; Nef, P. D.; Nelson, T. K.; Piacquadio, G.; Salnikov, A.; Schwartzman, A.; Silverstein, D.; Strauss, E.; Su, D.; Swiatlowski, M.; Wittgen, M.; Young, C.] SLAC Natl Accelerator Lab, Stanford, CA USA. [Astalos, R.; Bartos, P.; Blazek, T.; Federic, P.; Plazak, L.; Stavina, P.; Sykora, I.; Tokar, S.; Zenis, T.] Comenius Univ, Fac Math Phys & Informat, Bratislava, Slovakia. [Antos, J.; Bruncko, D.; Kladiva, E.; Strizenec, P.] Slovak Acad Sci, Inst Expt Phys, Dept Subnucl Phys, Kosice 04353, Slovakia. [Hamilton, A.] Univ Cape Town, Dept Phys, ZA-7925 Cape Town, South Africa. [Aurousseau, M.; Castaneda-Miranda, E.; Lee, C. A.; Yacoob, S.] Univ Johannesburg, Dept Phys, Johannesburg, South Africa. [Bristow, K.; Carrillo-Montoya, G. D.; Hamity, G. N.; Hsu, C.; March, L.; Garcia, B. R. Mellado; Ruan, X.; Boeriu, O. E. Vickey] Univ Witwatersrand, Sch Phys, Johannesburg, South Africa. [Abulaiti, Y.; Akerstedt, H.; Asman, B.; Bassalat, A.; Bendtz, K.; Bertoli, G.; Bessidskaia, O.; Bohm, C.; Clement, C.; Cribbs, W. A.; Eriksson, D.; Gellerstedt, K.; Hellman, S.; Johansson, K. E.; Jon-And, K.; Khandanyan, H.; Kim, H.; Klimek, P.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Petridis, A.; Plucinski, P.; Rossetti, V.; Silverstein, S. B.; Sjolin, J.; Strandberg, S.; Tylmad, M.] Stockholm Univ, Dept Phys, S-10691 Stockholm, Sweden. [Abulaiti, Y.; Akerstedt, H.; Asman, B.; Bendtz, K.; Bertoli, G.; Bessidskaia, O.; Clement, C.; Cribbs, W. A.; Gellerstedt, K.; Hellman, S.; Johansson, K. E.; Jon-And, K.; Khandanyan, H.; Kim, H.; Klimek, P.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Petridis, A.; Plucinski, P.; Rossetti, V.; Sjolin, J.; Strandberg, S.; Tylmad, M.] Oskar Klein Ctr, Stockholm, Sweden. [Jovicevic, J.; Kuwertz, E. S.; Lund-Jensen, B.; Morley, A. K.; Strandberg, J.] Royal Inst Technol, Dept Phys, S-10044 Stockholm, Sweden. [Bee, C. P.; Campoverde, A.; Chen, K.; Engelmann, R.; Grassi, V.; Hobbs, J.; Jia, J.; Li, H.; Lindquist, B. E.; Mastrandrea, P.; McCarthy, R. L.; Miucci, A.; Puldon, D.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.] SUNY Stony Brook, Dept Phys & Astron & Chem, Stony Brook, NY 11794 USA. [Bartsch, V.; Cerri, A.; Barajas, C. A. Chavez; De Sanctis, U.; De Santo, A.; Grout, Z. J.; Potter, C. J.; Salvatore, F.; Castillo, I. Santoyo; Shehu, C. Y.; Sutton, M. R.; Vivarelli, I.] Univ Sussex, Dept Phys & Astron, Brighton, E Sussex, England. [Black, C. W.; Cuthbert, C.; Finelli, K. D.; Jeng, G. -Y.; Limosani, A.; Patel, N. D.; Saavedra, A. F.; Scarcella, M.; Varvell, K. E.; Watson, I. J.; Yabsley, B.] Univ Sydney, Sch Phys, Sydney, NSW 2006, Australia. [Abdallah, J.; Chu, M. L.; Hou, S.; Jamin, D. O.; Lee, S. C.; Lin, S. C.; Liu, B.; Liu, D.; Lo Sterzo, F.; Mazini, R.; Ren, Z. L.; Shi, L.; Soh, D. A.; Teng, P. K.; Wang, C.; Wang, S. M.; Weng, Z.; Zhang, L.] Acad Sinica, Inst Phys, Taipei, Taiwan. [Abreu, H.; Di Mattia, A.; Kopeliansky, R.; Musto, E.; Rozen, Y.; Tarem, S.] Technion Israel Inst Technol, Dept Phys, IL-32000 Haifa, Israel. [Abramowicz, H.; Alexander, G.; Amram, N.; Ashkenazi, A.; Bella, G.; Benary, O.; Benhammou, Y.; Davies, M.; Etzion, E.; Gershon, A.; Gueta, O.; Guttman, N.; Munwes, Y.; Oren, Y.; Sadeh, I.; Silver, Y.; Soffer, A.; Taiblum, N.] Tel Aviv Univ, Raymond & Beverly Sackler Sch Phys & Astron, IL-69978 Tel Aviv, Israel. [Bachas, K.; Gkaitatzis, S.; Gkialas, I.; Iliadis, D.; Kordas, K.; Kouskoura, V.; Leisos, A.; Papageorgiou, K.; Hernandez, D. Paredes; Petridou, C.; Sampsonidis, D.; Sidiropoulou, O.] Aristotle Univ Thessaloniki, Dept Phys, GR-54006 Thessaloniki, Greece. [Akimoto, G.; Asai, S.; Azuma, Y.; Dohmae, T.; Enari, Y.; Hanawa, K.; Kanaya, N.; Kataoka, Y.; Kawamoto, T.; Kazama, S.; Kessoku, K.; Kobayashi, T.; Komori, Y.; Mashimo, T.; Masubuchi, T.; Minami, Y.; Nakamura, T.; Ninomiya, Y.; Okuyama, T.; Sakamoto, H.; Sasaki, Y.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamaguchi, H.; Yamamoto, S.; Yamamura, T.; Yamanaka, T.; Yoshihara, K.] Univ Tokyo, Int Ctr Elementary Particle Phys, Tokyo, Japan. [Akimoto, G.; Asai, S.; Azuma, Y.; Dohmae, T.; Enari, Y.; Hanawa, K.; Kanaya, N.; Kataoka, Y.; Kawamoto, T.; Kazama, S.; Kessoku, K.; Kobayashi, T.; Komori, Y.; Mashimo, T.; Masubuchi, T.; Minami, Y.; Nakamura, T.; Ninomiya, Y.; Okuyama, T.; Sakamoto, H.; Sasaki, Y.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamaguchi, H.; Yamamoto, S.; Yamamura, T.; Yamanaka, T.; Yoshihara, K.] Univ Tokyo, Dept Phys, Tokyo 113, Japan. [Bratzler, U.; Fukunaga, C.] Tokyo Metropolitan Univ, Grad Sch Sci & Technol, Tokyo 158, Japan. [Hirose, M.; Ishitsuka, M.; Jinnouchi, O.; Kobayashi, D.; Kuze, M.; Motohashi, K.; Nagai, R.; Nobe, T.; Pettersson, N. E.] Tokyo Inst Technol, Dept Phys, Tokyo 152, Japan. [AbouZeid, O. S.; Batista, S. J.; Brelier, B.; Chau, C. C.; DeMarco, D. A.; Ilic, N.; Keung, J.; Krieger, P.; Mc Goldrick, G.; Orr, R. S.; Polifka, R.; Rudolph, M. S.; Savard, P.; Schramm, S.; Sinervo, P.; Spreitzer, T.; Taenzer, J.; Teuscher, R. J.; Thompson, P. D.; Trischuk, W.; Venturi, N.] Univ Toronto, Dept Phys, Toronto, ON, Canada. [Canepa, A.; Koutsman, A.; Oram, C. J.; Schouten, D.; Stelzer-Chilton, O.; Tafirout, R.; Trigger, I. M.] TRIUMF, Vancouver, BC V6T 2A3, Canada. [Garcia, J. A. Benitez; Bustos, A. C. Florez; Qureshi, A.; Taylor, W.] York Univ, Dept Phys & Astron, Toronto, ON M3J 2R7, Canada. [Hara, K.; Hayashi, T.; Kim, S. H.; Kiuchi, K.; Nagata, K.; Ukegawa, F.] Univ Tsukuba, Fac Pure & Appl Sci, Tsukuba, Ibaraki, Japan. [Beauchemin, P. H.; Hamilton, S.; Mercurio, K. M.; Rolli, S.; Sliwa, K.; Wetter, J.] Tufts Univ, Dept Phys & Astron, Medford, MA 02155 USA. [Navarro, G.; Sandoval, C.] Univ Antonio Narino, Ctr Invest, Bogota, Colombia. [Gerbaudo, D.; Lankford, A. J.; Mete, A. S.; Nelson, A.; Rao, K.; Relich, M.; Scannicchio, D. A.; Schernau, M.; Shimmin, C. O.; Taffard, A.; Unel, G.; Whiteson, D.; Zhou, N.] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA USA. [Acharya, B. S.; Brazzale, S. F.; Cobal, M.; Giordani, M. P.; Kotov, V. M.; Pinamonti, M.; Quayle, W. B.; Shaw, K.; Soualah, R.] Ist Nazl Fis Nucl, Grp Collegato Udine, Sez Trieste, Udine, Italy. [Acharya, B. S.; Quayle, W. B.; Shaw, K.] Abdus Salaam Int Ctr Theoret Phys, Trieste, Italy. [Brazzale, S. F.; Cobal, M.; Giordani, M. P.; Pinamonti, M.; Soualah, R.] Univ Udine, Dipartimento Chim Fis & Ambiente, I-33100 Udine, Italy. [Atkinson, M.; Basye, A.; Benekos, N.; Cavaliere, V.; Chang, P.; Errede, D.; Errede, S.; Giordani, M. P.; Lie, K.; Liss, T. M.; Neubauer, M. S.; Shang, R.; Vichou, I.] Univ Illinois, Dept Phys, Urbana, IL 61801 USA. [Kuutmann, E. Bergeaas; Brenner, R.; Buszello, C. P.; Ekelof, T.; Ellert, M.; Ferrari, A.; Isaksson, C.; Madsen, A.; Ohman, H.; Pelikan, D.; Rangel-Smith, C.] Uppsala Univ, Dept Phys & Astron, Uppsala, Sweden. [Urban, S. Cabrera; Gimenez, V. Castillo; Costa, M. J.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Quiles, A. Irles; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; Marti-Garcia, S.; Mitsou, V. A.; Moles-Valls, R.; Garcia, E. Oliver; Lopez, S. Pedraza; Garcia-Estan, M. T. Perez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Pastor, E. Torro; Valero, A.; Gallego, E. Valladolid; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Inst Fis Corpuscular IFIC, Valencia, Spain. [Urban, S. Cabrera; Gimenez, V. Castillo; Costa, M. J.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Quiles, A. Irles; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; Marti-Garcia, S.; Mitsou, V. A.; Moles-Valls, R.; Garcia, E. Oliver; Lopez, S. Pedraza; Garcia-Estan, M. T. Perez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Pastor, E. Torro; Valero, A.; Gallego, E. Valladolid; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Dept Fis Atom Mol & Nucl, Valencia, Spain. [Urban, S. Cabrera; Gimenez, V. Castillo; Costa, M. J.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Quiles, A. Irles; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; Marti-Garcia, S.; Mitsou, V. A.; Moles-Valls, R.; Garcia, E. Oliver; Lopez, S. Pedraza; Garcia-Estan, M. T. Perez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Pastor, E. Torro; Valero, A.; Gallego, E. Valladolid; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Dept Ingn Elect, Valencia, Spain. [Urban, S. Cabrera; Gimenez, V. Castillo; Costa, M. J.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Quiles, A. Irles; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; Marti-Garcia, S.; Mitsou, V. A.; Moles-Valls, R.; Garcia, E. Oliver; Lopez, S. Pedraza; Garcia-Estan, M. T. Perez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Pastor, E. Torro; Valero, A.; Gallego, E. Valladolid; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, IMB CNM, Valencia, Spain. [Urban, S. Cabrera; Gimenez, V. Castillo; Costa, M. J.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Quiles, A. Irles; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; Marti-Garcia, S.; Mitsou, V. A.; Moles-Valls, R.; Garcia, E. Oliver; Lopez, S. Pedraza; Garcia-Estan, M. T. Perez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Pastor, E. Torro; Valero, A.; Gallego, E. Valladolid; Ferrer, J. A. Valls; Vos, M.] CSIC, Valencia, Spain. [Fedorko, W.; Gay, C.; Gecse, Z.; King, S. B.; Lister, A.; Swedish, S.; Viel, S.] Univ British Columbia, Dept Phys, Vancouver, BC V5Z 1M9, Canada. [Albert, J.; Bansal, V.; Berghaus, F.; Bernlochner, F. U.; David, C.; Fincke-Keeler, M.; Hamano, K.; Hill, E.; Keeler, R.; Kowalewski, R.; Lefebvre, M.; Marino, C. P.; McPherson, R. A.; Ouellette, E. A.; Pearce, J.; Sobie, R.; Venturi, M.] Univ Victoria, Dept Phys & Astron, Victoria, BC, Canada. [Beckingham, M.; Farrington, S. M.; Harrison, P. F.; Janus, M.; Jeske, C.; Jones, G.; Martin, T. A.; Murray, W. 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RI Li, Liang/O-1107-2015; Monzani, Simone/D-6328-2017; Maneira, Jose/D-8486-2011; Prokoshin, Fedor/E-2795-2012; KHODINOV, ALEKSANDR/D-6269-2015; Staroba, Pavel/G-8850-2014; Goncalo, Ricardo/M-3153-2016; Gauzzi, Paolo/D-2615-2009; Mindur, Bartosz/A-2253-2017; Fabbri, Laura/H-3442-2012; Solodkov, Alexander/B-8623-2017; Zaitsev, Alexandre/B-8989-2017; Peleganchuk, Sergey/J-6722-2014; Yang, Haijun/O-1055-2015; Aguilar Saavedra, Juan Antonio/F-1256-2016; Wemans, Andre/A-6738-2012; Leyton, Michael/G-2214-2016; Jones, Roger/H-5578-2011; Perrino, Roberto/B-4633-2010; SULIN, VLADIMIR/N-2793-2015; Nechaeva, Polina/N-1148-2015; Vykydal, Zdenek/H-6426-2016; Olshevskiy, Alexander/I-1580-2016; Snesarev, Andrey/H-5090-2013; Kantserov, Vadim/M-9761-2015; Vanadia, Marco/K-5870-2016; Ippolito, Valerio/L-1435-2016; Tikhomirov, Vladimir/M-6194-2015; Chekulaev, Sergey/O-1145-2015; Warburton, Andreas/N-8028-2013; Gorelov, Igor/J-9010-2015; Gladilin, Leonid/B-5226-2011; De, Kaushik/N-1953-2013; Carvalho, Joao/M-4060-2013; Mashinistov, Ruslan/M-8356-2015; Buttar, Craig/D-3706-2011; Gonzalez de la Hoz, Santiago/E-2494-2016; Guo, Jun/O-5202-2015; Marti-Garcia, Salvador/F-3085-2011; Della Pietra, Massimo/J-5008-2012; Cavalli-Sforza, Matteo/H-7102-2015; Petrucci, Fabrizio/G-8348-2012; Negrini, Matteo/C-8906-2014; Ferrer, Antonio/H-2942-2015; Grancagnolo, Sergio/J-3957-2015; Doyle, Anthony/C-5889-2009; spagnolo, stefania/A-6359-2012; Ciubancan, Liviu Mihai/L-2412-2015; Zhukov, Konstantin/M-6027-2015; Shmeleva, Alevtina/M-6199-2015; Gavrilenko, Igor/M-8260-2015; Connell, Simon/F-2962-2015; Livan, Michele/D-7531-2012; Smirnova, Oxana/A-4401-2013; Bosman, Martine/J-9917-2014; Joergensen, Morten/E-6847-2015; Mitsou, Vasiliki/D-1967-2009; Villa, Mauro/C-9883-2009; Riu, Imma/L-7385-2014; Mir, Lluisa-Maria/G-7212-2015; White, Ryan/E-2979-2015; Brooks, William/C-8636-2013; Di Domenico, Antonio/G-6301-2011 OI Li, Liang/0000-0001-6411-6107; Monzani, Simone/0000-0002-0479-2207; Maneira, Jose/0000-0002-3222-2738; Prokoshin, Fedor/0000-0001-6389-5399; KHODINOV, ALEKSANDR/0000-0003-3551-5808; Goncalo, Ricardo/0000-0002-3826-3442; Gauzzi, Paolo/0000-0003-4841-5822; Mindur, Bartosz/0000-0002-5511-2611; Fabbri, Laura/0000-0002-4002-8353; Solodkov, Alexander/0000-0002-2737-8674; Zaitsev, Alexandre/0000-0002-4961-8368; Peleganchuk, Sergey/0000-0003-0907-7592; Aguilar Saavedra, Juan Antonio/0000-0002-5475-8920; Wemans, Andre/0000-0002-9669-9500; Leyton, Michael/0000-0002-0727-8107; Jones, Roger/0000-0002-6427-3513; Perrino, Roberto/0000-0002-5764-7337; SULIN, VLADIMIR/0000-0003-3943-2495; Vykydal, Zdenek/0000-0003-2329-0672; Olshevskiy, Alexander/0000-0002-8902-1793; Kantserov, Vadim/0000-0001-8255-416X; Vanadia, Marco/0000-0003-2684-276X; Ippolito, Valerio/0000-0001-5126-1620; Tikhomirov, Vladimir/0000-0002-9634-0581; Warburton, Andreas/0000-0002-2298-7315; Gorelov, Igor/0000-0001-5570-0133; Gladilin, Leonid/0000-0001-9422-8636; De, Kaushik/0000-0002-5647-4489; Carvalho, Joao/0000-0002-3015-7821; Mashinistov, Ruslan/0000-0001-7925-4676; Gonzalez de la Hoz, Santiago/0000-0001-5304-5390; Guo, Jun/0000-0001-8125-9433; Della Pietra, Massimo/0000-0003-4446-3368; Petrucci, Fabrizio/0000-0002-5278-2206; Negrini, Matteo/0000-0003-0101-6963; Ferrer, Antonio/0000-0003-0532-711X; Grancagnolo, Sergio/0000-0001-8490-8304; Doyle, Anthony/0000-0001-6322-6195; spagnolo, stefania/0000-0001-7482-6348; Ciubancan, Liviu Mihai/0000-0003-1837-2841; Connell, Simon/0000-0001-6000-7245; Livan, Michele/0000-0002-5877-0062; Smirnova, Oxana/0000-0003-2517-531X; Bosman, Martine/0000-0002-7290-643X; Joergensen, Morten/0000-0002-6790-9361; Mitsou, Vasiliki/0000-0002-1533-8886; Villa, Mauro/0000-0002-9181-8048; Riu, Imma/0000-0002-3742-4582; Mir, Lluisa-Maria/0000-0002-4276-715X; White, Ryan/0000-0003-3589-5900; Brooks, William/0000-0001-6161-3570; Di Domenico, Antonio/0000-0001-8078-2759 FU ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWF and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile; CAS, MOST and NSFC, China; COLCIENCIAS, Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF, DNSRC and Lundbeck Foundation, Denmark; EPLANET, ERC and NSRF, European Union; IN2P3-CNRS, CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, DFG, HGF, MPG and AvH Foundation, Germany; GSRT and NSRF, Greece; ISF, MIN-ERVA, GIF, I-CORE and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; FOM and NWO, Netherlands; BRF and RCN, Norway; MNiSW and NCN, Poland; GRICES and FCT, Portugal; MNE/IFA, Romania; MES of Russia and ROSATOM, Russian Federation; JINR; MSTD, Serbia; MSSR, Slovakia; ARRS and MIZS, Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC and Wallenberg Foundation, Sweden; SER, SNSF and Cantons of Bern and Geneva, Switzerland; NSC, Taiwan; TAEK, Turkey; STFC, the Royal Society and Leverhulme Trust, United Kingdom; DOE and NSF, United States of America FX We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWF and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile; CAS, MOST and NSFC, China; COLCIENCIAS, Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF, DNSRC and Lundbeck Foundation, Denmark; EPLANET, ERC and NSRF, European Union; IN2P3-CNRS, CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, DFG, HGF, MPG and AvH Foundation, Germany; GSRT and NSRF, Greece; ISF, MIN-ERVA, GIF, I-CORE and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; FOM and NWO, Netherlands; BRF and RCN, Norway; MNiSW and NCN, Poland; GRICES and FCT, Portugal; MNE/IFA, Romania; MES of Russia and ROSATOM, Russian Federation; JINR; MSTD, Serbia; MSSR, Slovakia; ARRS and MIZS, Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC and Wallenberg Foundation, Sweden; SER, SNSF and Cantons of Bern and Geneva, Switzerland; NSC, Taiwan; TAEK, Turkey; STFC, the Royal Society and Leverhulme Trust, United Kingdom; DOE and NSF, United States of America. NR 91 TC 56 Z9 56 U1 6 U2 64 PU SPRINGER PI NEW YORK PA 233 SPRING ST, NEW YORK, NY 10013 USA SN 1029-8479 J9 J HIGH ENERGY PHYS JI J. High Energy Phys. PD NOV 12 PY 2014 IS 11 AR 056 DI 10.1007/JHEP11(2014)056 PG 47 WC Physics, Particles & Fields SC Physics GA AZ0AC UT WOS:000347908000003 ER PT J AU Liang, SH Mukherjee, A Patel, ND Bishop, CB Dagotto, E Moreo, A AF Liang, Shuhua Mukherjee, Anamitra Patel, Niravkumar D. Bishop, Christopher B. Dagotto, Elbio Moreo, Adriana TI Diverging nematic susceptibility, physical meaning of T* scale, and pseudogap in the spin fermion model for the pnictides SO PHYSICAL REVIEW B LA English DT Article ID IRON ARSENIDE SUPERCONDUCTOR; TRANSITION; MAGNETISM; ORDER AB Using Monte Carlo simulations with a tunable uniaxial strain, the nematic susceptibility of the spin fermion model for the pnictides is calculated. The results are in excellent agreement with the experiments by Chu et al. [Science 337, 710 (2012)]. Via a Ginzburg-Landau analysis, our study suggests a nematicity in the spin fermion model primarily originating in magnetism, but with the lattice/orbital also playing a key role by boosting up critical temperatures and separating the structural T-S and Neel T-N transitions. At T > T-S, Curie-Weiss behavior is observed with a characteristic temperature T* being the T-N of the purely electronic system. In this temperature regime, short-range magnetic order with wave vectors (pi, 0)-(0, pi) induce local nematic fluctuations and a density-of-states pseudogap, compatible with several experiments. The present analysis relies on the study of a particular model for the iron superconductors; thus further studies are needed to conclusively establish the driver of nematicity in real materials. C1 [Liang, Shuhua; Dagotto, Elbio; Moreo, Adriana] Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA. [Liang, Shuhua; Mukherjee, Anamitra; Patel, Niravkumar D.; Bishop, Christopher B.; Dagotto, Elbio; Moreo, Adriana] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA. RP Liang, SH (reprint author), Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA. NR 41 TC 8 Z9 8 U1 4 U2 9 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1098-0121 EI 1550-235X J9 PHYS REV B JI Phys. Rev. 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L Gay, APR Leonard, A Marage, PE Mohammadi, A Pernie, L Reis, T Seva, T Thomas, L Vander Velde, C Vanlaer, P Wang, J Adler, V Beernaert, K Benucci, L Cimmino, A Costantini, S Crucy, S Dildick, S Garcia, G Klein, B Lellouch, J Mccartin, J Rios, AAO Ryckbosch, D Diblen, SS Sigamani, M Strobbe, N Thyssen, F Tytgat, M Walsh, S Yazgan, E Zaganidis, N Basegmez, S Beluffi, C Bruno, G Castello, R Caudron, A Ceard, L Da Silveira, GG Delaere, C du Pree, T Favart, D Forthomme, L Giammanco, A Hollar, J Jez, P Komm, M Lemaitre, V Liao, J Militaru, O Nuttens, C Pagano, D Pin, A Piotrzkowski, K Popov, A Quertenmont, L Selvaggi, M Marono, MV Garcia, JMV Beliy, N Caebergs, T Daubie, E Hammad, GH Alves, GA Martins, MC Martins, TD Pol, ME Souza, MHG Alda, WL Carvalho, W Chinellato, J Custodio, A Da Costa, EM Damiao, DD Martins, CD De Souza, SF Malbouisson, H Malek, M Figueiredo, DM Mundim, L Nogima, H Da Silva, WLP Santaolalla, J Santoro, A Sznajder, A Manganote, EJT Pereira, AV Bernardes, CA Dias, FA Tomei, TRFP Gregores, EM Mercadante, PG Novaes, SF Padula, SS Genchev, V Iaydjiev, P Marinov, A Piperov, S Rodozov, M Sultanov, G Vutova, M Dimitrov, A Glushkov, I Hadjiiska, R Kozhuharov, V Litov, L Pavlov, B Petkov, P Bian, JG Chen, GM Chen, HS Chen, M Du, R Jiang, CH Liang, D Liang, S Meng, X Plestina, R Tao, J Wang, X Wang, Z Asawatangtrakuldee, C Ban, Y Guo, Y Li, Q Li, W Liu, S Mao, Y Qian, SJ Wang, D Zhang, L Zou, W Avila, C Sierra, LFC Florez, C Gomez, JP Moreno, BG Sanabria, JC Godinovic, N Lelas, D Polic, D Puljak, I Antunovic, Z Kovac, M Brigljevic, V Kadija, K Luetic, J Mekterovic, D Morovic, S Sudic, L Attikis, A Mavromanolakis, G Mousa, J Nicolaou, C Ptochos, F Razis, PA Finger, M Finger, M Assran, Y Elgammal, S Kamel, AE Mahmoud, MA Mahrous, A Radi, A Kadastik, M Muntel, M Murumaa, M Raidal, M Tiko, A Eerola, P Fedi, G Voutilainen, M Harkonen, J Karimaki, V Kinnunen, R Kortelainen, MJ Lampen, T Lassila-Perini, K Lehti, S Linden, T Luukka, P Maenpaa, T Peltola, T 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Rekovic, V. Robles, J. Salur, S. Schnetzer, S. Seitz, C. Somalwar, S. Stone, R. Thomas, S. Thomassen, P. Walker, M. Rose, K. Spanier, S. Yang, Z. C. York, A. Bouhali, O. Eusebi, R. Flanagan, W. Gilmore, J. Kamon, T. Khotilovich, V. Krutelyov, V. Montalvo, R. Osipenkov, I. Pakhotin, Y. Perloff, A. Roe, J. Safonov, A. Sakuma, T. Suarez, I. Tatarinov, A. Toback, D. Akchurin, N. Cowden, C. Damgov, J. Dragoiu, C. Dudero, P. R. Faulkner, J. Kovitanggoon, K. Kunori, S. Lee, S. W. Libeiro, T. Volobouev, I. Appelt, E. Delannoy, A. G. Greene, S. Gurrola, A. Johns, W. Maguire, C. Mao, Y. Melo, A. Sharma, M. Sheldon, P. Snook, B. Tuo, S. Velkovska, J. Arenton, M. W. Boutle, S. Cox, B. Francis, B. Goodell, J. Hirosky, R. Ledovskoy, A. Li, H. Lin, C. Neu, C. Wood, J. Gollapinni, S. Harr, R. Karchin, P. E. Don, C. Kottachchi Kankanamge Lamichhane, P. Belknap, D. A. Borrello, L. Carlsmith, D. Cepeda, M. Dasu, S. Duric, S. Friis, E. Grothe, M. Hall-Wilton, R. Herndon, M. Herve, A. Klabbers, P. Klukas, J. Lanaro, A. Lazaridis, C. Levine, A. Loveless, R. Mohapatra, A. Ojalvo, I. Perry, T. Pierro, G. A. Polese, G. Ross, I. Sarangi, T. Savin, A. Smith, W. H. Woods, N. CA CMS Collaboration TI Measurement of differential cross sections for the production of a pair of isolated photons in pp collisions at root s=7TeV SO EUROPEAN PHYSICAL JOURNAL C LA English DT Article ID LHC; HIERARCHY; BOSON; MASS AB A measurement of differential cross sections for the production of a pair of isolated photons in proton-proton collisions at root s = 7 TeV is presented. The data sample corresponds to an integrated luminosity of 5.0 fb(-1) collected with the CMS detector. A data-driven isolation template method is used to extract the prompt diphoton yield. The measured cross section for two isolated photons, with transverse energy above 40 and 25 GeV respectively, in the pseudorapidity range vertical bar eta vertical bar < 2.5, vertical bar eta vertical bar (sic) [1.44, 1.57] and with an angular separation Delta R > 0.45, is 17.2 +/-0.2 (stat) +/-1.9 (syst) +/- 0.4 (lumi) pb. Differential cross sections are measured as a function of the diphoton invariant mass, the diphoton transverse momentum, the azimuthal angle difference between the two photons, and the cosine of the polar angle in the Collins-Soper reference frame of the diphoton system. The results are compared to theoretical predictions at leading, next-to-leading, and next-to-next-to-leading order in quantum chromodynamics. C1 [Chatrchyan, S.; Khachatryan, V.; Sirunyan, A. M.; Tumasyan, A.] Yerevan Phys Inst, Yerevan 375036, Armenia. [Adam, W.; Bergauer, T.; Dragicevic, M.; Eroe, J.; Fabjan, C.; Friedl, M.; Fruehwirth, R.; Ghete, V. 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[Barone, L.; Cavallari, F.; Del Re, D.; Diemoz, M.; Grassi, M.; Jorda, C.; Longo, E.; Margaroli, F.; Meridiani, P.; Micheli, F.; Nourbakhsh, S.; Organtini, G.; Paramatti, R.; Rahatlou, S.; Rovelli, C.; Soffi, L.; Traczyk, P.] Ist Nazl Fis Nucl, Sez Roma, Rome, Italy. [Barone, L.; Del Re, D.; Grassi, M.; Longo, E.; Margaroli, F.; Micheli, F.; Nourbakhsh, S.; Organtini, G.; Rahatlou, S.; Soffi, L.; Traczyk, P.] Univ Rome, Rome, Italy. [Costa, S.; Amapane, N.; Arcidiacono, R.; Argiro, S.; Arneodo, M.; Bellan, R.; Biino, C.; Cartiglia, N.; Casasso, S.; Degano, A.; Demaria, N.; Mariotti, C.; Maselli, S.; Migliore, E.; Monaco, V.; Musich, M.; Obertino, M. M.; Ortona, G.; Pacher, L.; Pastrone, N.; Pelliccioni, M.; Potenza, A.; Romero, A.; Ruspa, M.; Sacchi, R.; Solano, A.; Staiano, A.; Tamponi, U.] Ist Nazl Fis Nucl, Sez Torino, I-10125 Turin, Italy. [Amapane, N.; Argiro, S.; Bellan, R.; Casasso, S.; Costa, M.; Degano, A.; Migliore, E.; Monaco, V.; Ortona, G.; Pacher, L.; Potenza, A.; Romero, A.; Sacchi, R.; Solano, A.] Univ Turin, Turin, Italy. [Arcidiacono, R.; Arneodo, M.; Obertino, M. M.; Ruspa, M.] Univ Piemonte Orientale, Novara, Italy. [Belforte, S.; Candelise, V.; Casarsa, M.; Cossutti, F.; Della Ricca, G.; Gobbo, B.; La Licata, C.; Marone, M.; Montanino, D.; Penzo, A.; Schizzi, A.; Umer, T.; Zanetti, A.] Ist Nazl Fis Nucl, Sez Trieste, Trieste, Italy. [Candelise, V.; Della Ricca, G.; La Licata, C.; Marone, M.; Montanino, D.; Schizzi, A.; Umer, T.] Univ Trieste, Trieste, Italy. [Chang, S.; Kim, T. Y.; Nam, S. K.] Kangwon Natl Univ, Chunchon, South Korea. [Kim, D. H.; Kim, G. N.; Kim, J. E.; Kim, M. S.; Kong, D. J.; Lee, S.; Oh, Y. D.; Park, H.; Sakharov, A.; Son, D. C.] Kyungpook Natl Univ, Taegu 702701, South Korea. [Kim, J. Y.; Kim, Zero J.; Song, S.] Chonnam Natl Univ, Inst Universe & Elementary Particles, Kwangju, South Korea. [Choi, S.; Gyun, D.; Hong, B.; Jo, M.; Kim, H.; Kim, Y.; Lee, B.; Lee, K. S.; Park, S. K.; Roh, Y.] Korea Univ, Seoul, South Korea. [Choi, M.; Kim, J. H.; Park, C.; Park, I. C.; Park, S.; Ryu, G.] Univ Seoul, Seoul, South Korea. [Choi, Y.; Choi, Y. K.; Goh, J.; Kwon, E.; Lee, J.; Seo, H.; Yu, I.] Sungkyunkwan Univ, Suwon, South Korea. [Juodagalvis, A.] Vilnius Univ, Vilnius, Lithuania. [Komaragiri, J. R.] Univ Malaya, Natl Ctr Particle Phys, Kuala Lumpur, Malaysia. [Castilla-Valdez, H.; De la Cruz-Burelo, E.; Heredia-de la Cruz, I.; Lopez-Fernandez, R.; Martinez-Ortega, J.; Sanchez-Hernandez, A.; Villasenor-Cendejas, L. M.] IPN, Ctr Invest & Estudios Avanzados, Mexico City 07738, DF, Mexico. [Moreno, S. Carrillo; Valencia, F. Vazquez] Univ Iberoamer, Mexico City, DF, Mexico. [Ibarguen, H. A. Salazar] Benemerita Univ Autonoma Puebla, Puebla, Mexico. [Linares, E. Casimiro; Pineda, A. Morelos] Univ Autonoma San Luis Potosi, San Luis Potosi, Mexico. [Krofcheck, D.] Univ Auckland, Auckland 1, New Zealand. [Butler, P. H.; Doesburg, R.; Reucroft, S.] Univ Canterbury, Christchurch 1, New Zealand. [Ahmad, A.; Ahmad, M.; Asghar, M. I.; Butt, J.; Hassan, Q.; Hoorani, H. R.; Khan, W. A.; Khurshid, T.; Qazi, S.; Shah, M. A.; Shoaib, M.] Quaid I Azam Univ, Natl Ctr Phys, Islamabad, Pakistan. [Bialkowska, H.; Bluj, M.; Boimska, B.; Frueboes, T.; Gorski, M.; Kazana, M.; Nawrocki, K.; Romanowska-Rybinska, K.; Szleper, M.; Wrochna, G.; Zalewski, P.] Natl Ctr Nucl Res, Otwock, Poland. [Brona, G.; Bunkowski, K.; Cwiok, M.; Dominik, W.; Doroba, K.; Kalinowski, A.; Konecki, M.; Krolikowski, J.; Misiura, M.; Wolszczak, W.] Univ Warsaw, Inst Expt Phys, Fac Phys, Warsaw, Poland. [Bargassa, P.; Silva, C. Beirao Da Cruz E.; Faccioli, P.; Parracho, P. G. Ferreira; Gallinaro, M.; Nguyen, F.; Antunes, J. Rodrigues; Seixas, J.; Varela, J.; Vischia, P.] Lab Instrumentacao Fis Expt Particulas, Lisbon, Portugal. [Golutvin, I.; Karjavin, V.; Konoplyanikov, V.; Korenkov, V.; Kozlov, G.; Lanev, A.; Malakhov, A.; Matveev, V.; Mitsyn, V. V.; Moisenz, P.; Palichik, V.; Perelygin, V.; Shmatov, S.; Shulha, S.; Skatchkov, N.; Smirnov, V.; Tikhonenko, E.; Zarubin, A.] Joint Inst Nucl Res, Dubna, Russia. [Golovtsov, V.; Ivanov, Y.; Kim, V.; Levchenko, P.; Murzin, V.; Oreshkin, V.; Smirnov, I.; Sulimov, V.; Uvarov, L.; Vavilov, S.; Vorobyev, A.; Vorobyev, An.] Petersburg Nucl Phys Inst, Gatchina, St Petersburg, Russia. [Andreev, Yu.; Dermenev, A.; Gninenko, S.; Golubev, N.; Kirsanov, M.; Krasnikov, N.; Pashenkov, A.; Tlisov, D.; Toropin, A.] Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia. [Epshteyn, V.; Gavrilov, V.; Lychkovskaya, N.; Popov, V.; Safronov, G.; Semenov, S.; Spiridonov, A.; Stolin, V.; Vlasov, E.; Zhokin, A.] Inst Theoret & Expt Phys, Moscow 117259, Russia. [Andreev, V.; Azarkin, M.; Dremin, I.; Kirakosyan, M.; Leonidov, A.; Mesyats, G.; Rusakov, S. V.; Vinogradov, A.] PN Lebedev Phys Inst, Moscow 117924, Russia. [Belyaev, A.; Boos, E.; Dubinin, M.; Dudko, L.; Ershov, A.; Gribushin, A.; Klyukhin, V.; Kodolova, O.; Lokhtin, I.; Obraztsov, S.; Petrushanko, S.; Savrin, V.; Snigirev, A.] Moscow MV Lomonosov State Univ, Skobeltsyn Inst Nucl Phys, Moscow, Russia. [Azhgirey, I.; Bayshev, I.; Bitioukov, S.; Kachanov, V.; Kalinin, A.; Konstantinov, D.; Krychkine, V.; Petrov, V.; Ryutin, R.; Sobol, A.; Tourtchanovitch, L.; Troshin, S.; Tyurin, N.; Uzunian, A.; Volkov, A.] Inst High Energy Phys, State Res Ctr Russian Federat, Protvino, Russia. [Adzic, P.; Dordevic, M.; Ekmedzic, M.; Milosevic, J.] Univ Belgrade, Fac Phys, Belgrade 11001, Serbia. [Adzic, P.; Dordevic, M.; Ekmedzic, M.; Milosevic, J.] Univ Belgrade, Vinca Inst Nucl Sci, Belgrade, Serbia. [Aguilar-Benitez, M.; Maestre, J. Alcaraz; Battilana, C.; Calvo, E.; Cerrada, M.; Llatas, M. Chamizo; Colino, N.; De la Cruz, B.; Peris, A. Delgado; Vazquez, D. Dominguez; Bedoya, C. Fernandez; Ramos, J. P. Fernandez; Ferrando, A.; Flix, J.; Fouz, M. C.; Lopez, O. Gonzalez; Lopez, S. Goy; Hernandez, J. M.; Josa, M. I.; Merino, G.; De Martino, E. Navarro; Yzquierdo, A. Perez-Calero; Pelayo, J. Puerta; Olmeda, A. Quintario; Redondo, I.; Romero, L.; Soares, M. S.; Willmott, C.; Garcia-Bellido, A.] CIEMAT, E-28040 Madrid, Spain. [Albajar, C.; de Troconiz, J. F.; Missiroli, M.] Univ Autonoma Madrid, Madrid, Spain. [Brun, H.; Cuevas, J.; Menendez, J. Fernandez; Folgueras, S.; Caballero, I. Gonzalez; Iglesias, L. Lloret] Univ Oviedo, Oviedo, Spain. [Cifuentes, J. A. Brochero; Cabrillo, I. J.; Calderon, A.; Campderros, J. Duarte; Fernandez, M.; Gomez, G.; Sanchez, J. Gonzalez; Graziano, A.; Virto, A. Lopez; Marco, J.; Marco, R.; Rivero, C. Martinez; Matorras, F.; Sanchez, F. J. Munoz; Gomez, J. Piedra; Rodrigo, T.; Rodrguez-Marrero, A. Y.; Ruiz-Jimeno, A.; Scodellaro, L.; Vila, I.; Cortabitarte, R. Vilar] CSIC Univ Cantabria, IFCA, Santander, Spain. [Moreno, B. Gomez; Bloch, D.; Sharma, A.; Abbaneo, D.; Auffray, E.; Auzinger, G.; Bachtis, M.; Baillon, P.; Ball, A. H.; Barney, D.; Benaglia, A.; Bendavid, J.; Benhabib, L.; Benitez, J. F.; Bernet, C.; Bianchi, G.; Bocci, A.; Bonato, A.; Bondu, O.; Botta, C.; Breuker, H.; Camporesi, T.; Cerminara, G.; Christiansen, T.; Perez, J. A. Coarasa; Colafranceschi, S.; D'Alfonso, M.; d'Enterria, D.; Dabrowski, A.; David, A.; De Guio, F.; De Roeck, A.; De Visscher, S.; Dobson, M.; Dupont-Sagorin, N.; Elliott-Peisert, A.; Eugster, J.; Franzoni, G.; Funk, W.; Giffels, M.; Gigi, D.; Gill, K.; Giordano, D.; Girone, M.; Giunta, M.; Glege, F.; Gowdy, S.; Guida, R.; Hammer, J.; Hansen, M.; Harris, P.; Hegeman, J.; Innocente, V.; Janot, P.; Karavakis, E.; Kousouris, K.; Krajczar, K.; Lecoq, P.; Lourenco, C.; Magini, N.; Malgeri, L.; Mannelli, M.; Masetti, L.; Meijers, F.; Mersi, S.; Meschi, E.; Moortgat, F.; Mulders, M.; Musella, P.; Orsini, L.; Cortezon, E. Palencia; Pape, L.; Perez, E.; Perrozzi, L.; Petrilli, A.; Petrucciani, G.; Pfeiffer, A.; Pierini, M.; Pimia, M.; Piparo, D.; Plagge, M.; Racz, A.; Reece, W.; Rolandi, G.; Rovere, M.; Sakulin, H.; Santanastasio, F.; Sch, C. Fer; Schwick, C.; Sekmen, S.; Siegrist, P.; Silva, P.; Simon, M.; Sphicas, P.; Spiga, D.; Steggemann, J.; Stieger, B.; Stoye, M.; Treille, D.; Tsirou, A.; Veres, G. I.; Vlimant, J. R.; Wohri, H. K.; Zeuner, W. D.] CERN, European Org Nucl Res, CH-1211 Geneva, Switzerland. [Bertl, W.; Deiters, K.; Erdmann, W.; Horisberger, R.; Ingram, Q.; Kaestli, H. C.; Konig, S.; Kotlinski, D.; Langenegger, U.; Renker, D.; Rohe, T.] Paul Scherrer Inst, Villigen, Switzerland. [Bachmair, F.; Bani, L.; Bianchini, L.; Bortignon, P.; Buchmann, M. A.; Casal, B.; Chanon, N.; Deisher, A.; Dissertori, G.; Dittmar, M.; Donega, M.; Dunser, M.; Eller, P.; Grab, C.; Hits, D.; Lustermann, W.; Mangano, B.; Marini, A. C.; Del Arbol, P. Martinez Ruiz; Meister, D.; Mohr, N.; Nageli, C.; Nef, P.; Nessi-Tedaldi, F.; Pandolfi, F.; Peruzzi, M.; Quittnat, M.; Rebane, L.; Ronga, F. J.; Rossini, M.; Starodumov, A.; Takahashi, M.; Theofilatos, K.; Wallny, R.; Weber, H. A.; Paus, C.] Swiss Fed Inst Technol, Inst Particle Phys, Zurich, Switzerland. [Amsler, C.; Canelli, M. F.; Chiochia, V.; De Cosa, A.; Favaro, C.; Hinzmann, A.; Hreus, T.; Rikova, M. Ivova; Kilminster, B.; Mejias, B. Millan; Ngadiuba, J.; Robmann, P.; Snoek, H.; Taroni, S.; Verzetti, M.; Yang, Y.] Univ Zurich, Zurich, Switzerland. [Cardaci, M.; Chen, K. H.; Ferro, C.; Kuo, C. M.; Li, S. W.; Lin, W.; Volpe, R.; Yu, S. S.; Lu, Y.] Natl Cent Univ, Chungli 32054, Taiwan. [Bartalini, P.; Chang, P.; Chang, Y. H.; Chang, Y. W.; Chao, Y.; Chen, K. F.; Chen, P. H.; Dietz, C.; Grundler, U.; Hou, W. -S.; Hsiung, Y.; Lei, Y. J.; Liu, Y. F.; Lu, R. -S.; Majumder, D.; Petrakou, E.; Shi, X.; Shiu, J. G.; Tzeng, Y. M.; Wang, M.; Wilken, R.; Kao, S. C.] Natl Taiwan Univ, Taipei 10764, Taiwan. [Asavapibhop, B.; Suwonjandee, N.] Chulalongkorn Univ, Bangkok, Thailand. [Adiguzel, A.; Bakirci, M. N.; Cerci, S.; Dozen, C.; Dumanoglu, I.; Eskut, E.; Girgis, S.; Gokbulut, G.; Gurpinar, E.; Hos, I.; Kangal, E. E.; Topaksu, A. Kayis; Onengut, G.; Ozdemir, K.; Ozturk, S.; Polatoz, A.; Sogut, K.; Cerci, D. Sunar; Tali, B.; Topakli, H.; Vergili, M.] Cukurova Univ, Adana, Turkey. [Akin, I. V.; Aliev, T.; Bilin, B.; Bilmis, S.; Deniz, M.; Gamsizkan, H.; Guler, A. M.; Karapinar, G.; Ocalan, K.; Ozpineci, A.; Serin, M.; Sever, R.; Surat, U. E.; Yalvac, M.; Zeyrek, M.] Middle E Tech Univ, Dept Phys, TR-06531 Ankara, Turkey. [Gulmez, E.; Isildak, B.; Kaya, M.; Kaya, O.; Ozkorucuklu, S.] Bogazici Univ, Istanbul, Turkey. [Bahtiyar, H.; Barlas, E.; Cankocak, K.; Gunaydin, Y. O.; Vardarli, F. I.; Yucel, M.] Istanbul Tech Univ, TR-80626 Istanbul, Turkey. [Levchuk, L.; Sorokin, P.] Kharkov Inst Phys & Technol, Natl Sci Ctr, Kharkov, Ukraine. [Brooke, J. J.; Clement, E.; Cussans, D.; Flacher, H.; Frazier, R.; Goldstein, J.; Grimes, M.; Heath, G. P.; Heath, H. F.; Jacob, J.; Kreczko, L.; Lucas, C.; Meng, Z.; Newbold, D. M.; Paramesvaran, S.; Poll, A.; Senkin, S.; Smith, V. J.; Williams, T.] Univ Bristol, Bristol, Avon, England. [Bell, K. W.; Belyaev, A.; Brew, C.; Brown, R. M.; Cockerill, D. J. A.; Coughlan, J. A.; Harder, K.; Harper, S.; Ilic, J.; Olaiya, E.; Petyt, D.; Shepherd-Themistocleous, C. H.; Thea, A.; Tomalin, I. R.; Womersley, W. J.; Worm, S. D.] Rutherford Appleton Lab, Didcot OX11 0QX, Oxon, England. [Della Ricca, G.; Baber, M.; Bainbridge, R.; Buchmuller, O.; Burton, D.; Colling, D.; Cripps, N.; Cutajar, M.; Dauncey, P.; Davies, G.; Ferguson, W.; Fulcher, J.; Futyan, D.; Gilbert, A.; Bryer, A. Guneratne; Hall, G.; Hatherell, Z.; Hays, J.; Iles, G.; Jarvis, M.; Karapostoli, G.; Kenzie, M.; Lane, R.; Lucas, R.; Lyons, L.; Magnan, A. -M.; Marrouche, J.; Mathias, B.; Nandi, R.; Nash, J.; Nikitenko, A.; Pela, J.; Pesaresi, M.; Petridis, K.; Pioppi, M.; Raymond, D. M.; Rogerson, S.; Rose, A.; Seez, C.; Sharp, P.; Sparrow, A.; Tapper, A.; Acosta, M. Vazquez; Virdee, T.; Wakefield, S.; Wardle, N.] Univ London Imperial Coll Sci Technol & Med, London, England. [Cole, J. E.; Hobson, P. R.; Khan, A.; Kyberd, P.; Leggat, D.; Leslie, D.; Martin, W.; Reid, I. D.; Symonds, P.; Teodorescu, L.; Turner, M.] Brunel Univ, Uxbridge UB8 3PH, Middx, England. [Dittmann, J.; Hatakeyama, K.; Kasmi, A.; Liu, H.; Scarborough, T.] Baylor Univ, Waco, TX 76798 USA. [Charaf, O.; Cooper, S. I.; Henderson, C.; Rumerio, P.] Univ Alabama, Tuscaloosa, AL USA. [Avetisyan, A.; Bose, T.; Fantasia, C.; Heister, A.; Lawson, P.; Lazic, D.; Richardson, C.; Rohlf, J.; Sperka, D.; St John, J.; Sulak, L.] Boston Univ, Boston, MA 02215 USA. [Bhattacharya, S.; Alimena, J.; Christopher, G.; Cutts, D.; Demiragli, Z.; Ferapontov, A.; Garabedian, A.; Heintz, U.; Jabeen, S.; Kukartsev, G.; Laird, E.; Landsberg, G.; Luk, M.; Narain, M.; Segala, M.; Sinthuprasith, T.; Speer, T.; Swanson, J.] Brown Univ, Providence, RI 02912 USA. [Breedon, R.; Breto, G.; Sanchez, M. Calderon De la Barca; Chauhan, S.; Chertok, M.; Conway, J.; Conway, R.; Cox, P. T.; Erbacher, R.; Gardner, M.; Ko, W.; Kopecky, A.; Lander, R.; Miceli, T.; Mulhearn, M.; Pellett, D.; Pilot, J.; Ricci-Tam, F.; Rutherford, B.; Searle, M.; Shalhout, S.; Smith, J.; Squires, M.; Tripathi, M.; Wilbur, S.; Yohay, R.] Univ Calif Davis, Davis, CA 95616 USA. [Weber, H.; Andreev, V.; Cline, D.; Cousins, R.; Erhan, S.; Everaerts, P.; Farrell, C.; Felcini, M.; Hauser, J.; Ignatenko, M.; Jarvis, C.; Rakness, G.; Schlein, P.; Takasugi, E.; Valuev, V.] Univ Calif Los Angeles, Los Angeles, CA USA. [Liu, H.; Babb, J.; Clare, R.; Ellison, J.; Gary, J. W.; Hanson, G.; Heilman, J.; Jandir, P.; Lacroix, F.; Long, O. R.; Luthra, A.; Malberti, M.; Nguyen, H.; Shrinivas, A.; Sturdy, J.; Sumowidagdo, S.; Wimpenny, S.] Univ Calif Riverside, Riverside, CA 92521 USA. [Sharma, V.; Simon, M.; Andrews, W.; Branson, J. G.; Cerati, G. B.; Cittolin, S.; D'Agnolo, R. T.; Evans, D.; Holzner, A.; Kelley, R.; Kovalskyi, D.; Lebourgeois, M.; Letts, J.; Macneill, I.; Padhi, S.; Palmer, C.; Pieri, M.; Sani, M.; Simon, S.; Sudano, E.; Tadel, M.; Tu, Y.; Vartak, A.; Wasserbaech, S.; Wurthwein, F.; Yagil, A.; Yoo, J.] Univ Calif San Diego, La Jolla, CA 92093 USA. [Barge, D.; Bradmiller-Feld, J.; Campagnari, C.; Danielson, T.; Dishaw, A.; Flowers, K.; Sevilla, M. Franco; Geffert, P.; George, C.; Golf, F.; Incandela, J.; Justus, C.; Villalba, R. Magana; Mccoll, N.; Pavlunin, V.; Richman, J.; Rossin, R.; Stuart, D.; To, W.; West, C.] Univ Calif Santa Barbara, Santa Barbara, CA 93106 USA. [Apresyan, A.; Bornheim, A.; Bunn, J.; Chen, Y.; Di Marco, E.; Duarte, J.; Kcira, D.; Mott, A.; Newman, H. B.; Pena, C.; Rogan, C.; Spiropulu, M.; Timciuc, V.; Wilkinson, R.; Xie, S.; Zhu, R. Y.] CALTECH, Pasadena, CA 91125 USA. [Azzolini, V.; Calamba, A.; Carroll, R.; Ferguson, T.; Iiyama, Y.; Jang, D. W.; Paulini, M.; Russ, J.; Vogel, H.; Vorobiev, I.] Carnegie Mellon Univ, Pittsburgh, PA 15213 USA. [Cumalat, J. P.; Drell, B. R.; Ford, W. T.; Gaz, A.; Lopez, E. Luiggi; Nauenberg, U.; Smith, J. G.; Stenson, K.; Ulmer, K. A.; Wagner, S. R.] Univ Colorado, Boulder, CO 80309 USA. [Alexander, J.; Chatterjee, A.; Chu, J.; Eggert, N.; Gibbons, L. K.; Hopkins, W.; Khukhunaishvili, A.; Kreis, B.; Mirman, N.; Kaufman, G. Nicolas; Patterson, J. R.; Ryd, A.; Salvati, E.; Sun, W.; Teo, W. D.; Thom, J.; Thompson, J.; Tucker, J.; Weng, Y.; Winstrom, L.; Wittich, P.] Cornell Univ, Ithaca, NY USA. [Winn, D.] Fairfield Univ, Fairfield, CT 06430 USA. [Yang, Y.; Abdullin, S.; Albrow, M.; Anderson, J.; Apollinari, G.; Bauerdick, L. A. T.; Beretvas, A.; Berryhill, J.; Bhat, P. C.; Burkett, K.; Butler, J. N.; Chetluru, V.; Cheung, H. W. K.; Chlebana, F.; Cihangir, S.; Elvira, V. D.; Fisk, I.; Freeman, J.; Gao, Y.; Gottschalk, E.; Gray, L.; Green, D.; Grunendahl, S.; Gutsche, O.; Hare, D.; Harris, R. M.; Hirschauer, J.; Hooberman, B.; Jindariani, S.; Joshi, U.; Kaadze, K.; Klima, B.; Kwan, S.; Linacre, J.; Lincoln, D.; Lipton, R.; Lykken, J.; Maeshima, K.; Marraffino, J. M.; Outschoorn, V. I. Martinez; Maruyama, S.; Mason, D.; McBride, P.; Mishra, K.; Mrenna, S.; Musienko, Y.; Nahn, S.; Newman-Holmes, C.; O'Dell, V.; Prokofyev, O.; Ratnikova, N.; Sexton-Kennedy, E.; Sharma, S.; Spalding, W. J.; Spiegel, L.; Taylor, L.; Tkaczyk, S.; Tran, N. V.; Uplegger, L.; Vaandering, E. W.; Vidal, R.; Whitbeck, A.; Whitmore, J.; Wu, W.; Yun, J. C.; Johnson, K. F.] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA. [Acosta, D.; Avery, P.; Bourilkov, D.; Cheng, T.; Das, S.; De Gruttola, M.; Di Giovanni, G. P.; Dobur, D.; Field, R. D.; Fisher, M.; Fu, Y.; Furic, I. K.; Hugon, J.; Kim, B.; Konigsberg, J.; Korytov, A.; Kropivnitskaya, A.; Kypreos, T.; Low, J. F.; Matchev, K.; Milenovic, P.; Mitselmakher, G.; Muniz, L.; Rinkevicius, A.; Shchutska, L.; Skhirtladze, N.; Snowball, M.; Yelton, J.; Zakaria, M.] Univ Florida, Gainesville, FL USA. [Gaultney, V.; Hewamanage, S.; Linn, S.; Markowitz, P.; Martinez, G.; Rodriguez, J. L.] Florida Int Univ, Miami, FL 33199 USA. [Adams, T.; Askew, A.; Bochenek, J.; Chen, J.; Diamond, B.; Haas, J.; Hagopian, S.; Hagopian, V.; Johnson, K. F.; Prosper, H.; Veeraraghavan, V.; Weinberg, M.] Florida State Univ, Tallahassee, FL 32306 USA. [Baarmand, M. M.; Dorney, B.; Hohlmann, M.; Kalakhety, H.; Yumiceva, F.] Florida Inst Technol, Melbourne, FL 32901 USA. [Adams, M. R.; Apanasevich, L.; Bazterra, V. E.; Betts, R. R.; Bucinskaite, I.; Cavanaugh, R.; Evdokimov, O.; Gauthier, L.; Gerber, C. E.; Hofman, D. J.; Khalatyan, S.; Kurt, P.; Moon, D. H.; O'Brien, C.; Silkworth, C.; Turner, P.; Varelas, N.] Univ Illinois, Chicago, IL USA. [Akgun, U.; Albayrak, E. 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Hoorani, Hafeez/D-1791-2013; Leonidov, Andrey/M-4440-2013; Andreev, Vladimir/M-8665-2015; Cakir, Altan/P-1024-2015; Matorras, Francisco/I-4983-2015; TUVE', Cristina/P-3933-2015; Dudko, Lev/D-7127-2012; KIM, Tae Jeong/P-7848-2015; Paganoni, Marco/A-4235-2016; Azarkin, Maxim/N-2578-2015; de Jesus Damiao, Dilson/G-6218-2012; Lazzizzera, Ignazio/E-9678-2015; Sen, Sercan/C-6473-2014; D'Alessandro, Raffaello/F-5897-2015; Wulz, Claudia-Elisabeth/H-5657-2011; Belyaev, Alexander/F-6637-2015; Trocsanyi, Zoltan/A-5598-2009; Montanari, Alessandro/J-2420-2012; Hernandez Calama, Jose Maria/H-9127-2015; ciocci, maria agnese /I-2153-2015; My, Salvatore/I-5160-2015; Lo Vetere, Maurizio/J-5049-2012; Ragazzi, Stefano/D-2463-2009; Manganote, Edmilson/K-8251-2013; Lokhtin, Igor/D-7004-2012; da Cruz e Silva, Cristovao/K-7229-2013; Grandi, Claudio/B-5654-2015; Chinellato, Jose Augusto/I-7972-2012; Leonidov, Andrey/P-3197-2014; Benussi, Luigi/O-9684-2014; Petrushanko, Sergey/D-6880-2012; Bernardes, Cesar Augusto/D-2408-2015; Raidal, Martti/F-4436-2012; Calderon, Alicia/K-3658-2014; VARDARLI, Fuat Ilkehan/B-6360-2013 OI da Cruz e silva, Cristovao/0000-0002-1231-3819; Casarsa, Massimo/0000-0002-1353-8964; Ligabue, Franco/0000-0002-1549-7107; Diemoz, Marcella/0000-0002-3810-8530; Tricomi, Alessia Rita/0000-0002-5071-5501; bianco, stefano/0000-0002-8300-4124; Demaria, Natale/0000-0003-0743-9465; Benaglia, Andrea Davide/0000-0003-1124-8450; Ciulli, Vitaliano/0000-0003-1947-3396; Androsov, Konstantin/0000-0003-2694-6542; Fiorendi, Sara/0000-0003-3273-9419; Gonzi, Sandro/0000-0003-4754-645X; Levchenko, Petr/0000-0003-4913-0538; Yazgan, Efe/0000-0001-5732-7950; Paulini, Manfred/0000-0002-6714-5787; Di Matteo, Leonardo/0000-0001-6698-1735; Baarmand, Marc/0000-0002-9792-8619; Boccali, Tommaso/0000-0002-9930-9299; Menasce, Dario Livio/0000-0002-9918-1686; Gerosa, Raffaele/0000-0001-8359-3734; Attia Mahmoud, Mohammed/0000-0001-8692-5458; Bilki, Burak/0000-0001-9515-3306; Rolandi, Luigi (Gigi)/0000-0002-0635-274X; Sguazzoni, Giacomo/0000-0002-0791-3350; Vilela Pereira, Antonio/0000-0003-3177-4626; Sznajder, Andre/0000-0001-6998-1108; Da Silveira, Gustavo Gil/0000-0003-3514-7056; Mundim, Luiz/0000-0001-9964-7805; Haj Ahmad, Wael/0000-0003-1491-0446; Konecki, Marcin/0000-0001-9482-4841; Xie, Si/0000-0003-2509-5731; Leonardo, Nuno/0000-0002-9746-4594; Goh, Junghwan/0000-0002-1129-2083; Ruiz, Alberto/0000-0002-3639-0368; Govoni, Pietro/0000-0002-0227-1301; Tuominen, Eija/0000-0002-7073-7767; Calvo Alamillo, Enrique/0000-0002-1100-2963; Flix, Josep/0000-0003-2688-8047; Cerrada, Marcos/0000-0003-0112-1691; Perez-Calero Yzquierdo, Antonio/0000-0003-3036-7965; Novaes, Sergio/0000-0003-0471-8549; Della Ricca, Giuseppe/0000-0003-2831-6982; Tomei, Thiago/0000-0002-1809-5226; Dubinin, Mikhail/0000-0002-7766-7175; Stahl, Achim/0000-0002-8369-7506; Gulmez, Erhan/0000-0002-6353-518X; Tinoco Mendes, Andre David/0000-0001-5854-7699; Rovelli, Tiziano/0000-0002-9746-4842; Matorras, Francisco/0000-0003-4295-5668; TUVE', Cristina/0000-0003-0739-3153; Dudko, Lev/0000-0002-4462-3192; KIM, Tae Jeong/0000-0001-8336-2434; Paganoni, Marco/0000-0003-2461-275X; de Jesus Damiao, Dilson/0000-0002-3769-1680; Lazzizzera, Ignazio/0000-0001-5092-7531; Sen, Sercan/0000-0001-7325-1087; D'Alessandro, Raffaello/0000-0001-7997-0306; Wulz, Claudia-Elisabeth/0000-0001-9226-5812; Belyaev, Alexander/0000-0002-1733-4408; Trocsanyi, Zoltan/0000-0002-2129-1279; Montanari, Alessandro/0000-0003-2748-6373; Hernandez Calama, Jose Maria/0000-0001-6436-7547; ciocci, maria agnese /0000-0003-0002-5462; My, Salvatore/0000-0002-9938-2680; Lo Vetere, Maurizio/0000-0002-6520-4480; Ragazzi, Stefano/0000-0001-8219-2074; Korenkov, Vladimir/0000-0002-2342-7862; Giubilato, Piero/0000-0003-4358-5355; Gallinaro, Michele/0000-0003-1261-2277; Sogut, Kenan/0000-0002-9682-2855; Grandi, Claudio/0000-0001-5998-3070; Chinellato, Jose Augusto/0000-0002-3240-6270; Benussi, Luigi/0000-0002-2363-8889; FU SCOAP3 FX Funded by SCOAP3 / License Version CC BY 4.0. NR 36 TC 6 Z9 6 U1 11 U2 65 PU SPRINGER PI NEW YORK PA 233 SPRING ST, NEW YORK, NY 10013 USA SN 1434-6044 EI 1434-6052 J9 EUR PHYS J C JI Eur. Phys. J. C PD NOV 12 PY 2014 VL 74 IS 11 AR 3129 DI 10.1140/epjc/s10052-014-3129-3 PG 30 WC Physics, Particles & Fields SC Physics GA AX8PK UT WOS:000347170900001 ER PT J AU Browning, JF Baggetto, L Jungjohann, KL Wang, Y Tenhaeff, WE Keum, JK Wood, DL Veith, GM AF Browning, James F. Baggetto, Loic Jungjohann, Katherine L. Wang, Yongqiang Tenhaeff, Wyatt E. Keum, Jong K. Wood, David L., III Veith, Gabriel M. TI In Situ Determination of the Liquid/Solid Interface Thickness and Composition for the Li Ion Cathode LiMn1.5Ni0.5O4 SO ACS APPLIED MATERIALS & INTERFACES LA English DT Article DE liquid-solid interface; Li ion batteries; SEI layer; in situ battery; neutron reflectometry ID X-RAY REFLECTOMETRY; ELECTRODE/ELECTROLYTE INTERFACE; SEI FORMATION; LITHIUM; BATTERIES; ELECTRODES; SURFACE; MODEL; ELECTROLYTES; LITHIATION AB Using neutron reflectometry, we have determined the thickness and scattering length density profile of the electrode electrolyte interface for the high-voltage cathode LiMn1.5Ni0.5O4 in situ at open circuit voltage and fully delithiated. Upon exposure to a liquid electrolyte, a thin 3.3 nm Li-rich interface forms due to the ordering of the electrolyte on the cathode surface. This interface changes in composition, as evident by an increase in the scattering length density of the new layer, with charging as the condensed layer evolves from being lithium rich to one containing a much higher concentration of F from the LiPF6 salt. These results show the surface chemistry evolves as a function of the potential. C1 [Browning, James F.; Keum, Jong K.] Oak Ridge Natl Lab, Chem & Engn Mat Div, Oak Ridge, TN 37831 USA. [Baggetto, Loic; Tenhaeff, Wyatt E.; Wood, David L., III; Veith, Gabriel M.] Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37831 USA. [Jungjohann, Katherine L.] Sandia Natl Labs, Ctr Integrated Nanotechnol, Albuquerque, NM 87185 USA. [Wang, Yongqiang] Los Alamos Natl Lab, Mat Sci & Technol Div, Los Alamos, NM 87545 USA. RP Veith, GM (reprint author), Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37831 USA. EM veithgm@ornl.gov RI Browning, James/C-9841-2016; Keum, Jong/N-4412-2015; Baggetto, Loic/D-5542-2017 OI Browning, James/0000-0001-8379-259X; Keum, Jong/0000-0002-5529-1373; Baggetto, Loic/0000-0002-9029-2363 FU Materials Sciences and Engineering Division, Office of Basic Energy Sciences, U.S. Department of Energy (DOE) under UT-Battelle, LLC; Laboratory Directed Research and Development Program of Oak Ridge National Laboratory; Scientific User Facilities Division, Office of Basic Energy Sciences, U.S. DOE; U.S. DOE's National Nuclear Security Administration [DE-AC04-94AL85000]; National Nuclear Security Administration of the U.S. DOE [DE-AC52-06NA25396] FX This research was supported by the Materials Sciences and Engineering Division, Office of Basic Energy Sciences, U.S. Department of Energy (DOE), under contract with UT-Battelle, LLC (G.M.V.). A portion of this work was sponsored by the Laboratory Directed Research and Development Program of Oak Ridge National Laboratory, managed by UT-Battelle, LLC, for the U.S. DOE (L.B., W.E.T., D.L.W.). Neutron reflectometry measurements were carried out on the liquids reflectometer at the Spallation Neutron Source, which is sponsored by the Scientific User Facilities Division, Office of Basic Energy Sciences, U.S. DOE (J.F.B., J.K.K.). STEM imaging and RBS experiments were performed at the Center for Integrated Nanotechnologies, an Office of Science User Facility operated for the U.S. DOE Office of Science. Sandia National Laboratories is a multiprogram laboratory operated by Sandia Corp., a wholly owned subsidiary of Lockheed Martin Co., for the U.S. DOE's National Nuclear Security Administration under Contract DE-AC04-94AL85000 (K.L.J.). RBS experiments were performed at the Center for Integrated Nanotechnologies, an Office of Science User Facility operated for the U.S. DOE Office of Science. Los Alamos National Laboratory, an affirmative action equal opportunity employer, is operated by Los Alamos National Security, LLC, for the National Nuclear Security Administration of the U.S. DOE under Contract DE-AC52-06NA25396 (Y.W.). NR 33 TC 12 Z9 12 U1 13 U2 95 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1944-8244 J9 ACS APPL MATER INTER JI ACS Appl. Mater. Interfaces PD NOV 12 PY 2014 VL 6 IS 21 BP 18569 EP 18576 DI 10.1021/am5032055 PG 8 WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Science & Technology - Other Topics; Materials Science GA AT5IY UT WOS:000344978200029 PM 25285852 ER PT J AU Verde, MG Liu, HD Carroll, KJ Baggetto, L Veith, GM Meng, YS AF Verde, Michael G. Liu, Haodong Carroll, Kyler J. Baggetto, Loic Veith, Gabriel M. Meng, Y. Shirley TI Effect of Morphology and Manganese Valence on the Voltage Fade and Capacity Retention of Li[Li2/12Ni3/12Mn7/12]O-2 SO ACS APPLIED MATERIALS & INTERFACES LA English DT Article DE Li-rich; Li-excess; Li-ion battery; cathode; high energy density; surface; XPS ID LITHIUM-ION BATTERIES; X-RAY-DIFFRACTION; CATHODE MATERIALS; PHOTOELECTRON-SPECTROSCOPY; LAYERED OXIDES; SOLID-SOLUTION; LI2MNO3; LI1.20MN0.54CO0.13NI0.13O2; ELECTRODES; MECHANISM AB We have determined the electrochemical characteristics of the high voltage, high capacity Li-ion battery cathode material Li[Li2/12Ni3/12Mn7/12]O-2 prepared using three different synthesis routes: sol-gel, hydroxide coprecipitation, and carbonate coprecipitation. Each route leads to distinct morphologies and surface areas while maintaining the same crystal structures. X-ray photoelectron spectroscopy (XPS) measurements reveal differences in their surface chemistries upon cycling, which correlate with voltage fading. Indeed, we observe the valence state of Mn on the surface to decrease upon lithiation, and this reduction is specifically correlated to discharging below 3.6 V. Furthermore, the data shows a correlation of the formation of Li2CO3 with the Mn oxidation state from the decomposition of electrolyte. These phenomena are related to each material's electrochemistry in order to expand upon the reaction mechanisms taking place-specifically in terms of the particle morphology produced by each synthetic approach. C1 [Verde, Michael G.; Liu, Haodong; Carroll, Kyler J.; Meng, Y. Shirley] Univ Calif San Diego, Dept NanoEngn, La Jolla, CA 92093 USA. [Baggetto, Loic; Veith, Gabriel M.] Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA. RP Verde, MG (reprint author), Univ Calif San Diego, Dept NanoEngn, La Jolla, CA 92093 USA. EM mverdejr@gmail.com; shmeng@ucsd.edu RI Baggetto, Loic/D-5542-2017 OI Baggetto, Loic/0000-0002-9029-2363 FU Assistant Secretary for Energy Efficiency and Renewable Energy, Office of Vehicle Technologies of the U.S. Department of Energy [AC02-05CH11231, 7056412]; U.S. Department of Energy (DOE), Basic Energy Sciences (BES), Materials Sciences and Engineering Division FX The authors are grateful for the financial support from the Assistant Secretary for Energy Efficiency and Renewable Energy, Office of Vehicle Technologies of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231, Subcontract No. 7056412 under the Batteries for Advanced Transportation Technologies (BATT) Program. The U.S. Department of Energy (DOE), Basic Energy Sciences (BES), Materials Sciences and Engineering Division supported a portion of this work (BET, XPS LB, GMV). We are also grateful for the contributions from undergraduate research assistants at the University of California San Diego (UCSD), Han Nguyen and Michael Tang. NR 56 TC 22 Z9 22 U1 8 U2 108 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1944-8244 J9 ACS APPL MATER INTER JI ACS Appl. Mater. Interfaces PD NOV 12 PY 2014 VL 6 IS 21 BP 18868 EP 18877 DI 10.1021/am504701s PG 10 WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Science & Technology - Other Topics; Materials Science GA AT5IY UT WOS:000344978200064 PM 25275709 ER PT J AU Yildirim, H Greeley, JP Sankaranarayanan, SKRS AF Yildirim, Handan Greeley, Jeffrey P. Sankaranarayanan, Subramanian K. R. S. TI Localized Order-Disorder Transitions Induced by Li Segregation in Amorphous TiO2 Nanoparticles SO ACS APPLIED MATERIALS & INTERFACES LA English DT Article DE amorphous titania; nanoparticle; lithiation; segregation; diffusion; Li-ion batteries ID TITANIUM-DIOXIDE NANOPARTICLES; MOLECULAR-DYNAMICS SIMULATION; LITHIUM-ION BATTERIES; RATE PERFORMANCE; ENERGY-STORAGE; ANATASE TIO2; ADSORPTION; INSERTION; SURFACE; NANOSTRUCTURES AB Li segregation and transport characteristics in amorphous TiO2 nanopartides (NPs) are studied using molecular dynamics (MD) simulations. A strong intrapartide segregation of Li is observed, and the degree of segregation is found to correlate with Li concentration. With increasing Li concentration, Li diffusivity and segregation are enhanced, and this behavior is tied to the structural response of the NPs with increasing lithiation. The atoms in the amorphous NPs undergo rearrangement in the regions of high Li concentration, introducing new pathways for Li transport and segregation. These localized atomic rearrangements, in turn, induce preferential crystallization near the surfaces of the NPs. Such rich, dynamical responses are not expected for crystalline NPs, where the presence of well-defined lattice sites leads to limited segregation and transport at high Li concentrations. The preferential crystallization in the near-surface region in amorphous NPs may offer enhanced stability and fast Li transport for Li-ion battery applications, in addition to having potentially useful properties for other materials science applications. C1 [Yildirim, Handan; Greeley, Jeffrey P.] Purdue Univ, Sch Chem Engn, W Lafayette, IN 47907 USA. [Sankaranarayanan, Subramanian K. R. S.] Argonne Natl Lab, Ctr Nanoscale Mat, Argonne, IL 60439 USA. RP Greeley, JP (reprint author), Purdue Univ, Sch Chem Engn, W Lafayette, IN 47907 USA. EM jgreeley@purdue.edu; skrssank@anl.gov FU DOE Early Career Award through the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences/Chemical Sciences; U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-AC02-06CH11357]; Office of Science of the U.S. Department of Energy [DE-AC02-05CH11231] FX A DOE Early Career Award for J.G. through the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences/Chemical Sciences, is acknowledged. Use of the Center for Nanoscale Materials was supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract No: DE-AC02-06CH11357. The authors also acknowledge the use of computational resources through the National Energy Research Scientific Computing Center (NERSC). This research used resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. NR 66 TC 3 Z9 3 U1 4 U2 30 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1944-8244 J9 ACS APPL MATER INTER JI ACS Appl. Mater. Interfaces PD NOV 12 PY 2014 VL 6 IS 21 BP 18962 EP 18970 DI 10.1021/am5048398 PG 9 WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Science & Technology - Other Topics; Materials Science GA AT5IY UT WOS:000344978200074 PM 25303039 ER PT J AU Chaukulkar, RP de Peuter, K Stradins, P Pylypenko, S Bell, JP Yang, YA Agarwal, S AF Chaukulkar, Rohan P. de Peuter, Koen Stradins, Paul Pylypenko, Svitlana Bell, Jacob P. Yang, Yongan Agarwal, Sumit TI Single-Step Plasma Synthesis of Carbon-Coated Silicon Nanoparticles SO ACS APPLIED MATERIALS & INTERFACES LA English DT Article DE Si nanoparticles; radio frequency plasmas; nanoparticle synthesis ID LITHIUM-ION BATTERIES; GAS-PHASE HYDROSILYLATION; AMORPHOUS-CARBON; CARBIDE FILMS; METAL NANOPARTICLES; ANODE MATERIAL; CRITICAL SIZE; QUANTUM DOTS; SIC MATRIX; CORE-LEVEL AB We have developed a novel single-step technique based on nonthermal, radio frequency (rf) plasmas to synthesize sub-10 nm, core-shell, carbon-coated crystalline Si (c-Si) nanoparticles (NPs) for potential application in Li+ batteries and as fluorescent markers. Hydrogen-terminated c-Si NPs nucleate and grow in a SiH4-containing, low-temperature plasma in the upstream section of a tubular quartz reactor. The c-Si NPs are then transported downstream by gas flow, and are coated with amorphous carbon (a-C) in a second C2H2-containing plasma. X-ray diffraction (XRD), X-ray photoelectron spectroscopy, and in situ attenuated total reflection Fourier transform infrared spectroscopy show that a thin, < 1 rim, 3C-SiC layer forms at the c-Si/a-C interface. By varying the downstream C2H2 plasma rf power, we can alter the nature of the a-C coating as well as the thickness of the interfacial 3C-SiC layer. The transmission electron microscopy (TEM) analysis is in agreement with the Si NP core size determined by Raman spectroscopy, photoluminescence spectroscopy, and XRD analysis. The size of the c-Si NP core, and the corresponding light emission from these NPs, was directly controlled by varying the thickness of the interfacial 3C-SiC layer. This size tunable emission thus also demonstrates the versatility of this technique for synthesizing c-Si NPs for potential applications in light emitting diodes, biological markers, and nanocrystal inks. C1 [Chaukulkar, Rohan P.; Agarwal, Sumit] Colorado Sch Mines, Dept Chem & Biol Engn, Golden, CO 80401 USA. [de Peuter, Koen] Eindhoven Univ Technol, Dept Appl Phys, NL-5600 MB Eindhoven, Netherlands. [Stradins, Paul] Natl Renewable Energy Lab, Natl Ctr Photovolta, Golden, CO 80401 USA. [Pylypenko, Svitlana] Colorado Sch Mines, Dept Met & Mat Engn, Golden, CO 80401 USA. [Bell, Jacob P.; Yang, Yongan] Colorado Sch Mines, Dept Chem & Geochem, Golden, CO 80401 USA. RP Agarwal, S (reprint author), Colorado Sch Mines, Dept Chem & Biol Engn, Golden, CO 80401 USA. EM sagarwal@mines.edu RI Yang, Yongan/C-2688-2011; Agarwal, Sumit/D-8950-2011 OI Yang, Yongan/0000-0003-1451-2923; FU NSF CAREER program [CBET-0846923]; U.S. Department of Energy [DE-AC36-08-GO28308]; National Renewable Energy Laboratory; Eindhoven University of Technology FX We gratefully acknowledge support from the NSF CAREER program (Grant No. CBET-0846923). P.S. acknowledges support from U.S. Department of Energy under Contract No. DE-AC36-08-GO28308 with the National Renewable Energy Laboratory. K.d.P. acknowledges support from the Eindhoven University of Technology. The authors would like to thank H. A. MacPherson and Dr. C. R. Stoldt at the University of Colorado for the Raman measurements, and the surface analysis group at the National Renewable Energy Laboratory for support and access to the XPS. NR 70 TC 7 Z9 7 U1 15 U2 133 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1944-8244 J9 ACS APPL MATER INTER JI ACS Appl. Mater. Interfaces PD NOV 12 PY 2014 VL 6 IS 21 BP 19026 EP 19034 DI 10.1021/am504913n PG 9 WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Science & Technology - Other Topics; Materials Science GA AT5IY UT WOS:000344978200081 PM 25275941 ER PT J AU Tan, HQ Zhao, Z Zhu, WB Coker, EN Li, BS Zheng, M Yu, WX Fan, HY Sun, ZC AF Tan, Huaqiao Zhao, Zhao Zhu, Wan-bin Coker, Eric N. Li, Binsong Zheng, Min Yu, Weixing Fan, Hongyou Sun, Zaicheng TI Oxygen Vacancy Enhanced Photocatalytic Activity of Pervoskite SrTiO3 SO ACS APPLIED MATERIALS & INTERFACES LA English DT Article DE SrTiO3; NaBH4; oxygen vacancy; core/shell nanostructure; photocatlytic H-2 generation ID VISIBLE-LIGHT; HYDROGEN-PRODUCTION; WATER OXIDATION; H-2 EVOLUTION; DOPED ZNO; TIO2; NANOPARTICLES; PERFORMANCE; COCATALYSTS; ABSORPTION C1 [Tan, Huaqiao; Zhao, Zhao; Zheng, Min; Sun, Zaicheng] Chinese Acad Sci, Changchun Inst Opt Fine Mech & Phys, State Key Lab Luminescence & Applicat, Changchun 130033, Peoples R China. [Zhao, Zhao] Univ Chinese Acad Sci, Beijing 100000, Peoples R China. [Zhu, Wan-bin; Yu, Weixing] Chinese Acad Sci, Changchun Inst Opt Fine Mech & Phys, State Key Lab Appl Opt, Changchun 130033, Peoples R China. [Coker, Eric N.; Li, Binsong; Fan, Hongyou] Sandia Natl Labs, Adv Mat Lab, Albuquerque, NM 87185 USA. [Fan, Hongyou] Univ New Mexico, Dept Chem & Nucl Engn, Ctr Microengn & Mat, Albuquerque, NM 87106 USA. RP Sun, ZC (reprint author), Chinese Acad Sci, Changchun Inst Opt Fine Mech & Phys, State Key Lab Luminescence & Applicat, 3888 East Nanhu Rd, Changchun 130033, Peoples R China. EM sunzc@ciomp.ac.cn RI Zheng, Min/B-6267-2013; Sun, Zaicheng/B-5397-2012; Yu, Weixing/G-3658-2012 OI Sun, Zaicheng/0000-0001-5277-5308; Yu, Weixing/0000-0002-3216-526X FU "Hundred Talent Program" of CAS; open research fund program of State Key Laboratory of Luminescence and Applications (Changchun Institute of Optics, Fine Mechanics and Physics, CAS); Key Laboratory of Functional Inorganic Material Chemistry (Heilongjiang University), Ministry of Education, P. R. China; U.S. Department of Energy, Office of Basic Energy Sciences, Division of Materials Sciences and Engineering; U.S. Department of Energy's National Nuclear Security Administration [DE-AC04-94AL85000] FX The authors thank the National Natural Science Foundation of China (No. 21301166, 21201159, 61361166004, and 61176016); Science and Technology Department of Jilin Province (No. 20130522127JH and 20121801) are gratefully acknowledged. Z.S. thanks the support of the "Hundred Talent Program" of CAS. Supported by open research fund program of State Key Laboratory of Luminescence and Applications (Changchun Institute of Optics, Fine Mechanics and Physics, CAS) and Key Laboratory of Functional Inorganic Material Chemistry (Heilongjiang University), Ministry of Education, P. R. China. HF acknowledges the support from the U.S. Department of Energy, Office of Basic Energy Sciences, Division of Materials Sciences and Engineering. Sandia is a multiprogram laboratory operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the U.S. Department of Energy's National Nuclear Security Administration under Contract DE-AC04-94AL85000. NR 41 TC 50 Z9 50 U1 35 U2 205 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1944-8244 J9 ACS APPL MATER INTER JI ACS Appl. Mater. Interfaces PD NOV 12 PY 2014 VL 6 IS 21 BP 19184 EP 19190 DI 10.1021/am5051907 PG 7 WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Science & Technology - Other Topics; Materials Science GA AT5IY UT WOS:000344978200100 PM 25311356 ER PT J AU Braid, JL Koldemir, U Sellinger, A Collins, RT Furtak, TE Olson, DC AF Braid, Jennifer L. Koldemir, Unsal Sellinger, Alan Collins, Reuben T. Furtak, Thomas E. Olson, Dana C. TI Conjugated Phosphonic Acid Modified Zinc Oxide Electron Transport Layers for Improved Performance in Organic Solar Cells SO ACS APPLIED MATERIALS & INTERFACES LA English DT Article DE organic photovoltaics; inverted devices; work function tuning; phosphonic acid; conjugated linkage ID SELF-ASSEMBLED MONOLAYERS; INDIUM-TIN OXIDE; WORK FUNCTION; BENZYLPHOSPHONIC ACIDS; SURFACE-PROPERTIES; BINDING AB Phosphonic acid modification of zinc oxide (ZnO) electron transport layers in inverted P3HT:ICBA solar cells was studied to determine the effect of conjugated linkages between the aromatic and phosphonic add attachment groups. For example, zinc oxide treated with 2,6-difluorophenylvinylphosphonic acid, having a conjugated vinyl group connecting the aromatic moiety to the phosphonic add group, showed a 0.78 eV decrease in the effective work function versus unmodified ZnO, whereas nonconjugated 2,6-difluorophenyle-thylphosphonic acid resulted in a 0.57 eV decrease, as measured by Kelvin probe. This resulted in an average power conversion efficiency of 5.89% for conjugated 2,6-difluorophenyvinylphosphonic add modified solar cells, an improvement over unmodified (5.24%) and nonconjugated phosphonic add modified devices (5.64%), indicating the importance of the conjugated linkage. C1 [Braid, Jennifer L.; Collins, Reuben T.; Furtak, Thomas E.] Colorado Sch Mines, Dept Phys, Golden, CO 80401 USA. [Koldemir, Unsal; Sellinger, Alan] Colorado Sch Mines, Dept Chem & Geochem, Golden, CO 80401 USA. [Braid, Jennifer L.; Sellinger, Alan; Olson, Dana C.] Natl Renewable Energy Lab, Golden, CO 80401 USA. RP Olson, DC (reprint author), Natl Renewable Energy Lab, Golden, CO 80401 USA. EM aselli@mines.edu; rtcollin@mines.edu; dana.olson@nrel.gov RI Sellinger, Alan/C-6250-2015; Collins, Reuben/O-2545-2014; Braid, Jennifer/A-7705-2017 OI Sellinger, Alan/0000-0001-6705-1548; Collins, Reuben/0000-0001-7910-3819; Braid, Jennifer/0000-0002-0677-7756 FU U.S. Department of Energy [DE-AC36-08-GO28308]; National Renewable Energy Laboratory through the DOE SETP program; National Science Foundation [DMR-0907409]; Renewable Energy Materials Research Science and Engineering Center FX This work was supported by the U.S. Department of Energy under Contract DE-AC36-08-GO28308 with the National Renewable Energy Laboratory through the DOE SETP program. Partial support from the National Science Foundation through Grant DMR-0907409 and the Renewable Energy Materials Research Science and Engineering Center is also acknowledged for RTC and TEF. NR 34 TC 11 Z9 11 U1 1 U2 46 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1944-8244 J9 ACS APPL MATER INTER JI ACS Appl. Mater. Interfaces PD NOV 12 PY 2014 VL 6 IS 21 BP 19229 EP 19234 DI 10.1021/am505182c PG 6 WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Science & Technology - Other Topics; Materials Science GA AT5IY UT WOS:000344978200105 PM 25329245 ER PT J AU Bhaway, SM Kisslinger, K Zhang, LH Yager, KG Schmitt, AL Mahanthappa, MK Karim, A Vogt, BD AF Bhaway, Sarang M. Kisslinger, Kim Zhang, Lihua Yager, Kevin G. Schmitt, Andrew L. Mahanthappa, Mahesh K. Karim, Alamgir Vogt, Bryan D. TI Mesoporous Carbon-Vanadium Oxide Films by Resol-Assisted, Triblock Copolymer-Templated Cooperative Self-Assembly SO ACS APPLIED MATERIALS & INTERFACES LA English DT Article DE block copolymer; self-assembly; vanadia; templated synthesis; nanopores; FDU-16 ID ENVIRONMENTAL ELLIPSOMETRIC POROSIMETRY; TRANSITION-METAL OXIDES; LITHIUM-ION BATTERIES; HYBRID THIN-FILMS; MOLECULAR-SIEVES; SOLAR-CELLS; TIO2; PERFORMANCE; ELECTRODE; REDUCTION AB Unlike other crystalline metal oxides amenable to templating by the combined assemblies of soft and hard chemistries (CASH) method, vanadium oxide nanostructures templated by poly(ethylene oxide-b-1,4-butadiene-b-ethylene oxide) (OBO) triblock copolymers are not preserved upon high temperature calcination in argon. Triconstituent cooperative assembly of a phenolic resin oligomer (resol) and an OBO triblock in a VOCl3 precursor solution enhances the carbon yield and can prevent breakout crystallization of the vanadia during calcination. However, the calcination environment significantly influences the observed mesoporous morphology in these composite thin films. Use of an argon atmosphere in this processing protocol leads to nearly complete loss of carbon vanadium oxide thin film mesostructure, due to carbothermal reduction of vanadium oxide. This reduction mechanism also explains why the CASH method is not more generally successful for the fabrication of ordered mesoporous vanadia. Carbonization under a nitrogen atmosphere at temperatures up to 800 degrees C instead enables formation of a block copolymer-templated mesoporous structure, which apparently stems from the formation of a minor fraction of a stabilizing vanadium oxynitride. Thus, judicious selection of the inert gas for template removal is critical for the synthesis of well-defined, mesoporous vanadia carbon composite films. This resol-assisted assembly method may generally apply to the fabrication of other mesoporous materials, wherein inorganic framework crystallization is problematic due to kinetically competitive carbothermal reduction processes. C1 [Bhaway, Sarang M.; Karim, Alamgir; Vogt, Bryan D.] Univ Akron, Dept Polymer Engn, Akron, OH 44325 USA. [Kisslinger, Kim; Zhang, Lihua; Yager, Kevin G.] Brookhaven Natl Lab, Ctr Funct Nanomat, Upton, NY 11973 USA. [Schmitt, Andrew L.; Mahanthappa, Mahesh K.] Univ Wisconsin, Dept Chem, Madison, WI 53706 USA. RP Vogt, BD (reprint author), Univ Akron, Dept Polymer Engn, Akron, OH 44325 USA. EM vogt@uakron.edu RI Vogt, Bryan/H-1986-2012; Zhang, Lihua/F-4502-2014; Yager, Kevin/F-9804-2011; Kisslinger, Kim/F-4485-2014; OI Vogt, Bryan/0000-0003-1916-7145; Yager, Kevin/0000-0001-7745-2513; Mahanthappa, Mahesh/0000-0002-9871-804X FU National Science Foundation [CBET-1336057]; NSF American Competitiveness in Chemistry Postdoctoral Fellowship [CHE-1041975]; U.S. Department of Energy, Office of Basic EnergySciences [DE-AC02-98CH10886]; U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-AC02-06CH11357]; Ohio Research Scholars Program Research Cluster on Surfaces in Advanced Materials FX This work has been partial supported by the National Science Foundation under grant CBET-1336057. A.L.S. gratefully acknowledges financial support from a NSF American Competitiveness in Chemistry Postdoctoral Fellowship (CHE-1041975). Research carried out at the Center for Functional Nanomaterials, Brookhaven National Laboratory, was supported by the U.S. Department of Energy, Office of Basic EnergySciences, under Contract No. DE-AC02-98CH10886. Use of the Sector 8-ID-E beamline of the Advanced Photon Source at Argonne National Laboratory for GISAXS measurements was supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract No. DE-AC02-06CH11357. The authors also thank Dr. Zhorro Nikolov for his assistance with XPS data analysis. Changhuai Ye and Zhe Qiang are acknowledged for help with GISAXS measurements. Some TEM data were obtained at the (cryo) TEM facility at the Liquid Crystal Institute, Kent State University, supported by the Ohio Research Scholars Program Research Cluster on Surfaces in Advanced Materials. S.M.B. thanks Dr. Min Gao for assistance with the TEM. NR 62 TC 4 Z9 4 U1 5 U2 72 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1944-8244 J9 ACS APPL MATER INTER JI ACS Appl. Mater. Interfaces PD NOV 12 PY 2014 VL 6 IS 21 BP 19288 EP 19298 DI 10.1021/am505307t PG 11 WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Science & Technology - Other Topics; Materials Science GA AT5IY UT WOS:000344978200113 PM 25317954 ER PT J AU Ren, XD Lau, KC Yu, MZ Bi, XX Kreidler, E Curtiss, LA Wu, YY AF Ren, Xiaodi Lau, Kah Chun Yu, Mingzhe Bi, Xuanxuan Kreidler, Eric Curtiss, Larry A. Wu, Yiying TI Understanding Side Reactions in K-O-2 Batteries for Improved Cycle Life SO ACS APPLIED MATERIALS & INTERFACES LA English DT Article DE metal-air batteries; potassium-oxygen battery; side reactions; O-2 crossover; ion selective separator ID SUPEROXIDE NAO2 BATTERY; NONAQUEOUS LI-O-2; POTASSIUM SUPEROXIDE; LITHIUM BATTERIES; ORGANIC-SOLVENTS; CARBON ELECTRODE; AIR BATTERIES; CHALLENGES; STABILITY; CATIONS AB Superoxide based metal-air (or metal-oxygen) batteries, including potassium and sodium-oxygen batteries, have emerged as promising alternative chemistries in the metal-air battery family because of much improved round-trip efficiencies (>90%). In order to improve the cycle life of these batteries, it is crucial to understand and control the side reactions between the electrodes and the electrolyte. For potassium-oxygen batteries using ether-based electrolytes, the side reactions on the potassium anode have been identified as the main cause of battery failure. The composition of the side products formed on the anode, including some reaction intermediates, have been identified and quantified. Combined experimental studies and density functional theory (DFT) calculations show the side reactions are likely driven by the interaction of potassium with ether molecules and the crossover of oxygen from the cathode. To inhibit these side reactions, the incorporation of a polymeric potassium ion selective membrane (Nafion-K+) as a battery separator is demonstrated that significantly improves the battery cycle life. The K-O-2 battery with the Nafion-K+ separator can be discharged and charged for more than 40 cycles without increases in charging overpotential. C1 [Ren, Xiaodi; Yu, Mingzhe; Bi, Xuanxuan; Wu, Yiying] Ohio State Univ, Dept Chem & Biochem, Columbus, OH 43210 USA. [Lau, Kah Chun; Curtiss, Larry A.] Argonne Natl Lab, Div Mat Sci, Argonne, IL 60439 USA. [Lau, Kah Chun; Curtiss, Larry A.] Argonne Natl Lab, Joint Ctr Energy Storage Res, Argonne, IL 60439 USA. [Kreidler, Eric] Honda Res Inst USA Inc, Columbus, OH 43212 USA. RP Wu, YY (reprint author), Ohio State Univ, Dept Chem & Biochem, 100 West 18th Ave, Columbus, OH 43210 USA. EM wu@chemistry.ohio-state.edu RI Lau, Kah Chun/A-9348-2013; Ren, Xiaodi/M-5843-2014; Yu, Mingzhe/N-5907-2016 OI Lau, Kah Chun/0000-0002-4925-3397; Ren, Xiaodi/0000-0002-2025-7554; FU Honda Research Institute USA; CNM Carbon Cluster at Argonne National Laboratory; ALCF Fusion Cluster at Argonne National Laboratory; Joint Center for Energy Storage Research (JCESR), an Energy Innovation Hub - U.S. Department of Energy, Office of Science, Basic Energy Sciences FX We are thankful for the financial support from Honda Research Institute USA. We acknowledge grants of computer time through the CNM Carbon Cluster at Argonne National Laboratory, the ALCF Fusion Cluster at Argonne National Laboratory. K.C.L. and L.A.C. were supported as part of the Joint Center for Energy Storage Research (JCESR), an Energy Innovation Hub funded by the U.S. Department of Energy, Office of Science, Basic Energy Sciences. NR 30 TC 17 Z9 17 U1 18 U2 88 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1944-8244 J9 ACS APPL MATER INTER JI ACS Appl. Mater. Interfaces PD NOV 12 PY 2014 VL 6 IS 21 BP 19299 EP 19307 DI 10.1021/am505351s PG 9 WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Science & Technology - Other Topics; Materials Science GA AT5IY UT WOS:000344978200114 PM 25295518 ER PT J AU Song, CK Eckstein, BJ Tam, TLD Trahey, L Marks, TJ AF Song, Charles Kiseok Eckstein, Brian J. Tam, Teck Lip Dexter Trahey, Lynn Marks, Tobin J. TI Conjugated Polymer Energy Level Shifts in Lithium-Ion Battery Electrolytes SO ACS APPLIED MATERIALS & INTERFACES LA English DT Article DE lithium-ion battery; conjugated polymer; electron affinity; cyclic voltammetry; electrolyte; organic photovoltaics ID HETEROJUNCTION SOLAR-CELLS; LIGHT-EMITTING-DIODES; CONDUCTING POLYMER; SIDE-CHAINS; ELECTRODES; POTENTIALS; LI; REDUCTION; ANODE; POLYTHIOPHENES AB The ionization potentials (IPs) and electron affinities (EAs) of widely used conjugated polymers are evaluated by cyclic voltammetry (CV) in conventional electrochemical and lithium-ion battery media, and also by ultraviolet photoelectron spectroscopy (UPS) in vacuo. By comparing the data obtained in the different systems, it is found that the IPs of the conjugated polymer films determined by conventional CV (IPC) can be correlated with UPS-measured HOMO energy levels (E-H,E-UPS) by the relationship E-H,E-UPS = (1.14 +/- 0.23) X qIP(C) + (4.62 +/- 0.10) eV, where q is the electron charge. It is also found that the EAs of the conjugated polymer films measured via CV in conventional (EA(C)) and Li+ battery (EA(B)) media can be linearly correlated by the relationship EA(B) = (1.07 +/- 0.13) x EA(C) + (2.84 +/- 0.22) V. The slopes and intercepts of these equations can be correlated with the dielectric constants of the polymer film environments and the redox potentials of the reference electrodes, as modified by the surrounding electrolyte, respectively. C1 [Song, Charles Kiseok; Eckstein, Brian J.; Tam, Teck Lip Dexter; Marks, Tobin J.] Northwestern Univ, Dept Chem, Evanston, IL 60208 USA. [Trahey, Lynn] Argonne Natl Lab, Chem Sci & Engn Div, Argonne, IL 60439 USA. [Marks, Tobin J.] Northwestern Univ, Dept Mat Sci & Engn, Evanston, IL 60208 USA. RP Trahey, L (reprint author), Argonne Natl Lab, Chem Sci & Engn Div, 9700 S Cass Ave, Argonne, IL 60439 USA. EM trahey@anl.gov; t-marks@northwestern.edu FU Institute for Sustainability and Energy at Northwestern (ISEN); Argonne-Northwestern Solar Energy Research (ANSER) Center, an Energy Frontier Research Center - U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-SC0001059]; Agency of Science, Technology and Research (A*STAR); Northwestern U., the NSF [CHE-0923236, CHE-9871268]; Pfizer; State of Illinois; Northwestern U., the State of Illinois; Keck foundation; NSF-MRSEC; NSF-NSEC FX This research was supported in part by the Institute for Sustainability and Energy at Northwestern (ISEN) (C.K.S.) and by the Argonne-Northwestern Solar Energy Research (ANSER) Center, an Energy Frontier Research Center funded by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Award Number DE-SC0001059 (B.J.E.). This research was also supported by the Agency of Science, Technology and Research (A*STAR; T.L.D.T.). We acknowledge the Integrated Molecular Structure Education and Research Center (IMSERC) for molecular characterization facilities for NMR spectroscopy supported by Northwestern U., the NSF under grants CHE-0923236 and CHE-9871268, Pfizer, and the State of Illinois. We also thank the Nanoscale Integrated Fabrication, Testing, and Instrument (NIFTI) and Keck Interdisciplinary Surface Science (KECK-II) facilities of Northwestern University's Atomic and Nanoscale Characterization Experimental (NUANCE) Center for UPS experiments, supported by Northwestern U., the State of Illinois, the Keck foundation, NSF-MRSEC, and NSF-NSEC. Finally, we thank Dr. Antonio Facchetti, J. T. Shin, and J. L. Song for helpful discussions. NR 57 TC 7 Z9 7 U1 6 U2 42 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1944-8244 J9 ACS APPL MATER INTER JI ACS Appl. Mater. Interfaces PD NOV 12 PY 2014 VL 6 IS 21 BP 19347 EP 19354 DI 10.1021/am505416m PG 8 WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Science & Technology - Other Topics; Materials Science GA AT5IY UT WOS:000344978200119 PM 25329000 ER PT J AU Li, YZ Rios, O Kessler, MR AF Li, Yuzhan Rios, Orlando Kessler, Michael R. TI Thermomagnetic Processing of Liquid-Crystalline Epoxy Resins and Their Mechanical Characterization Using Nanoindentation SO ACS APPLIED MATERIALS & INTERFACES LA English DT Article DE liquid-crystalline epoxy resins; thermomagnetic processing; molecular orientation; mechanical properties ID HIGH MAGNETIC-FIELD; RIGID-ROD; SENSING INDENTATION; BIPHENYL MESOGEN; SINGLE-CRYSTALS; THERMOSETS; ANISOTROPY; ORIENTATION; POLYMERS; KINETICS AB A thermomagnetic processing method was used to produce a biphenyl-based liquid-crystalline epoxy resin (LCER) with oriented liquid-crystalline (LC) domains. The orientation of the LCER was confirmed and quantified using two-dimensional X-ray diffraction. The effect of molecular alignment on the mechanical and thermomechanical properties of the LCER was investigated using nanoindentation and thermomechanical analysis, respectively. The effect of the orientation on the fracture behavior was also examined. The results showed that macroscopic orientation of the LC domains was achieved, resulting in an epoxy network with an anisotropic modulus, hardness, creep behavior, and thermal expansion. C1 [Li, Yuzhan; Kessler, Michael R.] Washington State Univ, Sch Mech & Mat Engn, Pullman, WA 99164 USA. [Rios, Orlando] Oak Ridge Natl Lab, Mat Proc & Mfg Grp, Oak Ridge, TN 37831 USA. RP Kessler, MR (reprint author), Washington State Univ, Sch Mech & Mat Engn, POB 642920, Pullman, WA 99164 USA. EM MichaelR.Kessler@wsu.edu RI Kessler, Michael/C-3153-2008; Rios, Orlando/E-6856-2017 OI Kessler, Michael/0000-0001-8436-3447; Rios, Orlando/0000-0002-1814-7815 FU Critical Materials Institute, an Energy Innovation Hub - U.S. Department of Energy, Office of Energy Efficiency and Renewable Energy , and Advanced Manufacturing Office [DE-AC05-00OR22725]; UT-Battelle, LLC; Air Force Office of Scientific Research [FA9550-12-1-0108] FX The authors thank Dr. Scott Schlorholtz at the Materials Analysis Research Laboratory at Iowa State University for his help with the XRD experiments and Dr. Amy Wo for the helpful discussion regarding the nanoindentation experiments. The authors also thank Dr. Valerie Lynch-Holm at the Franceschi Microscopy & Imaging Center at Washington State University. Research sponsored in part by the Critical Materials Institute, an Energy Innovation Hub funded by U.S. Department of Energy, Office of Energy Efficiency and Renewable Energy, and Advanced Manufacturing Office, under contract DE-AC05-00OR22725 with UT-Battelle, LLC. Support through the Air Force Office of Scientific Research (Award FA9550-12-1-0108) is gratefully acknowledged. NR 37 TC 5 Z9 5 U1 2 U2 41 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1944-8244 J9 ACS APPL MATER INTER JI ACS Appl. Mater. Interfaces PD NOV 12 PY 2014 VL 6 IS 21 BP 19456 EP 19464 DI 10.1021/am505874t PG 9 WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Science & Technology - Other Topics; Materials Science GA AT5IY UT WOS:000344978200131 PM 25318760 ER PT J AU Berman, D Deshmukh, SA Sankaranarayanan, SKRS Erdemir, A Sumant, AV AF Berman, Diana Deshmukh, Sanket A. Sankaranarayanan, Subramanian K. R. S. Erdemir, Ali Sumant, Anirudha V. TI Extraordinary Macroscale Wear Resistance of One Atom Thick Graphene Layer SO ADVANCED FUNCTIONAL MATERIALS LA English DT Article DE single layer graphene; wear; friction; tribology; MD Simulations ID DIAMOND-LIKE CARBON; SLIDING STEEL SURFACES; RAMAN-SPECTROSCOPY; FRICTION; GRAPHITE; DYNAMICS; HYDROGEN; NITROGEN; DEFECTS; FUTURE AB During the last few years, graphene's unusual friction and wear properties have been demonstrated at nano to micro scales but its industrial tribological potential has not been fully realized. The macroscopic wear resistance of one atom thick graphene coating is reported by subjecting it to pin-on-disc type wear testing against most commonly used steel against steel tribo-pair. It is shown that when tested in hydrogen, a single layer of graphene on steel can last for 6400 sliding cycles, while few-layer graphene (3-4 layers) lasts for 47 000 cycles. Furthermore, these graphene layers are shown to completely cease wear despite the severe sliding conditions including high contact pressures (approximate to 0.5 GPa) observed typically in macroscale wear tests. The computational simulations show that the extraordinary wear performance originates from hydrogen passivation of the dangling bonds in a ruptured graphene, leading to significant stability and longer lifetime of the graphene protection layer. Also, the electronic properties of these graphene sheets are theoretically evaluated and the improved wear resistance is demonstrated to preserve the electronic properties of graphene and to have significant potential for flexible electronics. The findings demonstrate that tuning the atomistic scale chemical interactions holds the promise of realizing extraordinary tribological properties of monolayer graphene coatings. C1 [Berman, Diana; Deshmukh, Sanket A.; Sankaranarayanan, Subramanian K. R. S.; Sumant, Anirudha V.] Argonne Natl Lab, Ctr Nanoscale Mat, Argonne, IL 60439 USA. [Erdemir, Ali] Argonne Natl Lab, Div Energy Syst, Argonne, IL 60439 USA. RP Berman, D (reprint author), Argonne Natl Lab, Ctr Nanoscale Mat, 9700 S Cass Ave, Argonne, IL 60439 USA. EM sumant@anl.gov FU U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-AC02-06CH11357]; Office of Science of the U.S. Department of Energy [DE-AC02-05CH11231] FX Use of the Center for Nanoscale Materials was supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract No. DE-AC02-06CH11357. This research used resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. NR 41 TC 23 Z9 23 U1 10 U2 99 PU WILEY-V C H VERLAG GMBH PI WEINHEIM PA BOSCHSTRASSE 12, D-69469 WEINHEIM, GERMANY SN 1616-301X EI 1616-3028 J9 ADV FUNCT MATER JI Adv. Funct. Mater. PD NOV 12 PY 2014 VL 24 IS 42 BP 6640 EP 6646 DI 10.1002/adfm.201401755 PG 7 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied; Physics, Condensed Matter SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AT2QC UT WOS:000344778200008 ER PT J AU Shao, M Keum, JK Kumar, R Chen, JH Browning, JF Das, S Chen, W Hou, JH Do, C Littrell, KC Rondinone, A Geohegan, DB Sumpter, BG Xiao, K AF Shao, Ming Keum, Jong Kahk Kumar, Rajeev Chen, Jihua Browning, James F. Das, Sanjib Chen, Wei Hou, Jianhui Do, Changwoo Littrell, Kenneth C. Rondinone, Adam Geohegan, David B. Sumpter, Bobby G. Xiao, Kai TI Understanding How Processing Additives Tune the Nanoscale Morphology of High Efficiency Organic Photovoltaic Blends: From Casting Solution to Spun-Cast Thin Film SO ADVANCED FUNCTIONAL MATERIALS LA English DT Article DE polymer photovoltaics; morphology; neutron scattering; reflectometry; Flory-Huggins theory ID POLYMER SOLAR-CELLS; PERFORMANCE; DEVICES AB Adding a small amount of a processing additive to the casting solution of photoactive organic blends has been demonstrated to be an effective method for achieving improved power conversion efficiency (PCE) in organic photovoltaics (OPVs). However, an understanding of the nano-structural evolution occurring in the transformation from casting solution to thin photoactive films is still lacking. In this report, the effects of the processing additive diiodooctane (DIO) on the morphology of the established blend of PBDTTT-C-T polymer and the fullerene derivative PC71BM used for OPVs are investigated, starting in the casting solution and tracing the effects in spun-cast thin films by using neutron/X-ray scattering, neutron reflectometry, and other characterization techniques. The results reveal that DIO has no observable effect on the structures of PBDTTT-C-T and PC71BM in solution; however, in the spun-cast films, it significantly promotes their molecular ordering and phase segregation, resulting in improved PCE. Thermodynamic analysis based on Flory-Huggins theory provides a rationale for the effects of DIO on different characteristics of phase segregation due to changes in concentration resulting from evaporation of the solvent and additive during film formation. Such information may help improve the rational design of ternary blends to more consistently achieve improved PCE for OPVs. C1 [Shao, Ming; Keum, Jong Kahk; Kumar, Rajeev; Chen, Jihua; Rondinone, Adam; Geohegan, David B.; Sumpter, Bobby G.; Xiao, Kai] Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA. [Keum, Jong Kahk; Browning, James F.; Do, Changwoo; Littrell, Kenneth C.] Oak Ridge Natl Lab, Neutron Scattering Sci Div, Oak Ridge, TN 37831 USA. [Kumar, Rajeev; Sumpter, Bobby G.] Oak Ridge Natl Lab, Comp Sci & Math Div, Oak Ridge, TN 37831 USA. [Das, Sanjib] Univ Tennessee, Dept Elect Engn & Comp Sci, Knoxville, TN 37996 USA. [Chen, Wei] Argonne Natl Lab, Div Mat Sci, Argonne, IL 60439 USA. [Hou, Jianhui] Chinese Acad Sci, Inst Chem, Beijing 10080, Peoples R China. RP Shao, M (reprint author), Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA. EM xiaok@ornl.gov RI Littrell, Kenneth/D-2106-2013; Geohegan, David/D-3599-2013; KUMAR, RAJEEV/D-2562-2010; Do, Changwoo/A-9670-2011; Das, Sanjib/A-9255-2017; Chen, Jihua/F-1417-2011; Hou, Jianhui /E-5824-2011; Chen, Wei/G-6055-2011; Sumpter, Bobby/C-9459-2013; Kumar, Rajeev/Q-2255-2015; Rondinone, Adam/F-6489-2013; Browning, James/C-9841-2016; Keum, Jong/N-4412-2015 OI Littrell, Kenneth/0000-0003-2308-8618; Geohegan, David/0000-0003-0273-3139; Do, Changwoo/0000-0001-8358-8417; Das, Sanjib/0000-0002-5281-4458; Chen, Jihua/0000-0001-6879-5936; Hou, Jianhui /0000-0002-2105-6922; Chen, Wei/0000-0001-8906-4278; Sumpter, Bobby/0000-0001-6341-0355; Kumar, Rajeev/0000-0001-9494-3488; Rondinone, Adam/0000-0003-0020-4612; Browning, James/0000-0001-8379-259X; Keum, Jong/0000-0002-5529-1373 FU Oak Ridge National Laboratory by the Office of Basic Energy Sciences, U.S. Department of Energy; Laboratory Directed Research and Development award, Oak Ridge National Laboratory (ORNL) FX M.S. and J.K. contributed equally for this work. This research was conducted at the Center for Nanophase Materials Sciences (CNMS), High Flux Isotope Reactor (HFIR) and Spallation Neutron Source (SNS) which are sponsored at Oak Ridge National Laboratory by the Office of Basic Energy Sciences, U.S. Department of Energy. KX and DBG acknowledge the support provided by a Laboratory Directed Research and Development award from the Oak Ridge National Laboratory (ORNL) for the neutron experiments. NR 37 TC 16 Z9 16 U1 2 U2 77 PU WILEY-V C H VERLAG GMBH PI WEINHEIM PA BOSCHSTRASSE 12, D-69469 WEINHEIM, GERMANY SN 1616-301X EI 1616-3028 J9 ADV FUNCT MATER JI Adv. Funct. Mater. PD NOV 12 PY 2014 VL 24 IS 42 BP 6647 EP 6657 DI 10.1002/adfm.201401547 PG 11 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied; Physics, Condensed Matter SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AT2QC UT WOS:000344778200009 ER PT J AU Rappe, KG AF Rappe, Kenneth G. TI Integrated Selective Catalytic Reduction-Diesel Particulate Filter Aftertreatment: Insights into Pressure Drop, NOx Conversion, and Passive Soot Oxidation Behavior SO INDUSTRIAL & ENGINEERING CHEMISTRY RESEARCH LA English DT Article ID ZEOLITE CATALYSTS; CU-SSZ-13; AMMONIA; SITES; FLOW; NH3 AB Integrating urea-selective catalytic reduction (SCR) and diesel particulate filter (DPF) technologies into a single device has the potential to reduce the complexity of current diesel aftertreatment strategies. Fundamental studies were performed to shed light on the pressure drop and reaction behavior of integrated SCR and DPF systems. Details of SCR washcoat amount and location were investigated for effect on pressure drop during soot filtration. The SCR catalyst primarily impacted depth filtration of soot, promoted by increased catalyst located within the upstream portion of the porous filter wall. This effect is believed to be related to the nature of the porous filter substrate and pore network and changing of the rate at which pores plug in the presence of catalyst. SCR catalyst on the wall of the inlet filter channel also had an effect on the pressure rise during cake filtration of soot. NOx reduction efficiency measurements were performed to determine the nature and magnitude of the effect of soot on SCR performance. The effect of soot on the SCR performance is primarily attributed to the contribution of passive soot oxidation, and the propensity for soot oxidation to shift the NO2/NOx fraction relative to 0.5. SCR performance at NO2/NOx < 0.5 is adversely affected by the presence of soot oxidation by increasing the SCR dependency on standard (NO only) SCR reactions; conversely, at NO2/NOx > 0.5, the SCR performance is positively impacted by a decreased dependency on NO2-only SCR reactions. Temperature-programmed oxidation studies were performed to evaluate the impact of SCR on passive soot oxidation. SCR adversely impacts soot oxidation performance via NO2 diffusive effects, decreasing NO2 concentration in the inlet channel. This impact can be minimized or recovered at higher NO2 concentration and NO2/NOx fractions >0.5. C1 Pacific NW Natl Lab, Richland, WA 99354 USA. RP Rappe, KG (reprint author), Pacific NW Natl Lab, POB 999, Richland, WA 99354 USA. EM ken.rappe@pnnl.gov FU U.S. Department of Energy (DOE), Office of Energy Efficiency and Renewable Energy, Vehicle Technologies Program; U.S. Department of Energy by Battelle Memorial Institute [DE-AC06-76RLO 1830] FX This work was performed at the Applied Process Engineering Laboratory at Pacific Northwest National Laboratory (PNNL). The author wishes to thank Gary Maupin for assistance in operating the soot loading apparatus and Jarrod Crum and Brian Riley for assistance in acquiring SEM images of the SCR/DPF samples. The author gratefully acknowledges funding provided for the research from the U.S. Department of Energy (DOE), Office of Energy Efficiency and Renewable Energy, Vehicle Technologies Program. PNNL is a multiprogram national laboratory operated for the U.S. Department of Energy by Battelle Memorial Institute under Contract DE-AC06-76RLO 1830. Figure 1 is reused with permission from SAGE Publications under license number 3466720963654. NR 30 TC 2 Z9 2 U1 2 U2 48 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0888-5885 J9 IND ENG CHEM RES JI Ind. Eng. Chem. Res. PD NOV 12 PY 2014 VL 53 IS 45 BP 17547 EP 17557 DI 10.1021/ie502832f PG 11 WC Engineering, Chemical SC Engineering GA AT4JT UT WOS:000344906400003 ER PT J AU Fu, Y Li, BS Jiang, YB Dunphy, DR Tsai, A Tam, SY Fan, HY Zhang, HX Rogers, D Rempe, S Atanassov, P Cecchi, JL Brinker, CJ AF Fu, Yaqin Li, Binsong Jiang, Ying-Bing Dunphy, Darren R. Tsai, Andy Tam, Siu-Yue Fan, Hongyou Zhang, Hongxia Rogers, David Rempe, Susan Atanassov, Plamen Cecchi, Joseph L. Brinker, C. Jeffrey TI Atomic Layer Deposition of L-Alanine Polypeptide SO JOURNAL OF THE AMERICAN CHEMICAL SOCIETY LA English DT Article ID SPECTROSCOPY; AGENT AB L-Alanine polypeptide thin films were synthesized via atomic layer deposition (ALD). Instead of using an amino acid monomer as the precursor, an L-alanine amino acid derivatized with a protecting group was used to prevent self-polymerization, increase the vapor pressure, and allow linear cycle-by-cycle growth emblematic of ALD. The successful deposition of a conformal polypeptide film has been confirmed by FTIR, TEM, and Mass Spectrometry, and the ALD process has been extended to polyvaline. C1 [Fu, Yaqin; Jiang, Ying-Bing; Dunphy, Darren R.; Atanassov, Plamen; Cecchi, Joseph L.; Brinker, C. Jeffrey] Univ New Mexico, Dept Chem & Biol Engn, Albuquerque, NM 87131 USA. [Fu, Yaqin; Jiang, Ying-Bing; Dunphy, Darren R.; Atanassov, Plamen; Cecchi, Joseph L.; Brinker, C. Jeffrey] Univ New Mexico, Ctr Microengineered Mat, Albuquerque, NM 87131 USA. [Jiang, Ying-Bing] Univ New Mexico, Dept Earth & Planetary Sci, Albuquerque, NM 87131 USA. [Tsai, Andy; Tam, Siu-Yue] T3 Sci LLC, Blaine, MN 55449 USA. [Li, Binsong; Fan, Hongyou; Rogers, David; Rempe, Susan; Brinker, C. Jeffrey] Sandia Natl Labs, Albuquerque, NM 87185 USA. [Zhang, Hongxia] Angstrom Thin Film Technol LLC, Albuquerque, NM 87113 USA. RP Jiang, YB (reprint author), Univ New Mexico, Dept Chem & Biol Engn, Albuquerque, NM 87131 USA. EM ybjiang@unm.edu; cjbrink@sandia.gov FU U.S. Department of Energy (DOE), Office of Basic Energy Sciences (BES) Catalysis Sciences Program [DE-FG02-02-ER15368]; DOE BES Division of Materials Sciences and Engineering; Air Force Office of Scientific Research [FA 9550-10-1-0054]; Sandia National Laboratories (SNL) Laboratory Directed Research and Development (LDRD) program; U.S. Department of Energy's NNSA [DE-AC04-94AL85000] FX Y.F. and D.D. were supported by the U.S. Department of Energy (DOE), Office of Basic Energy Sciences (BES) Catalysis Sciences Program Grant DE-FG02-02-ER15368; H.F. and C.J.B. were supported by the DOE BES Division of Materials Sciences and Engineering; B.L. and Y.-B.J.. were supported by the Air Force Office of Scientific Research Grant FA 9550-10-1-0054; and D.R. and S.R. were supported by the Sandia National Laboratories (SNL) Laboratory Directed Research and Development (LDRD) program. SNL is a multiprogram laboratory operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Company, for the U.S. Department of Energy's NNSA under Contract DE-AC04-94AL85000. The authors also want to thank Dr. Ken Sherrell at UNM Dept. of Chemistry for his help in mass spectrometry measurements. NR 19 TC 3 Z9 3 U1 4 U2 29 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0002-7863 J9 J AM CHEM SOC JI J. Am. Chem. Soc. PD NOV 12 PY 2014 VL 136 IS 45 BP 15821 EP 15824 DI 10.1021/ja5043403 PG 4 WC Chemistry, Multidisciplinary SC Chemistry GA AT4JQ UT WOS:000344906100004 PM 25355683 ER PT J AU Zadrozny, JM Niklas, J Poluektov, OG Freedman, DE AF Zadrozny, Joseph M. Niklas, Jens Poluektov, Oleg G. Freedman, Danna E. TI Multiple Quantum Coherences from Hyperfine Transitions in a Vanadium(IV) Complex SO JOURNAL OF THE AMERICAN CHEMICAL SOCIETY LA English DT Article ID SPIN; CRYSTAL; LIGANDS; QUBITS; DECOHERENCE; COMPUTERS; LATTICE; DESIGN; MAGNET AB We report a vanadium complex in a nuclear-spin free ligand field that displays two key properties for an ideal candidate qubit system: long coherence times that persist at high temperature, T-2 = 1.2 mu s at 80 K, and the observation of quantum coherences from multiple transitions. The electron paramagnetic resonance (EPR) spectrum of the complex [V(C8S8)(3)](2) displays multiple transitions arising from a manifold of states produced by the hyperfine coupling of the S = 1/2 electron spin and I = 7/2 nuclear spin. Transient nutation experiments reveal Rabi oscillations for multiple transitions. These observations suggest that each pair of hyperfine levels hosted within [V(C8S8)(3)](2) are candidate qubits. The realization of multiple quantum coherences within a transition metal complex illustrates an emerging method of developing scalability and addressability in electron spin qubits. This study presents a rare molecular demonstration of multiple Rabi oscillations originating from separate transitions. These results extend observations of multiple quantum coherences from prior reports in solid-state compounds to the new realm of highly modifiable coordination compounds. C1 [Zadrozny, Joseph M.; Freedman, Danna E.] Northwestern Univ, Dept Chem, Evanston, IL 60208 USA. [Niklas, Jens; Poluektov, Oleg G.] Argonne Natl Lab, Chem Sci & Engn Div, Argonne, IL 60439 USA. RP Freedman, DE (reprint author), Northwestern Univ, Dept Chem, 2145 Sheridan Rd, Evanston, IL 60208 USA. EM danna.freedman@northwestern.edu RI Zadrozny, Joseph/D-8206-2015; Niklas, Jens/I-8598-2016; Zadrozny, Joseph/A-1429-2017; OI Zadrozny, Joseph/0000-0002-1309-6545; Niklas, Jens/0000-0002-6462-2680; Zadrozny, Joseph/0000-0002-1309-6545; Freedman, Danna/0000-0002-2579-8835 FU Northwestern University; state of Illinois; U.S. Department of Energy Office of Science, Office of Basic Energy Sciences, Division of Chemical Sciences, Geosciences, and Biosciences [DE-AC02-06CH11357] FX We thank Prof. Brian Hoffman and Dr. Veronika Hooke for preliminary continuous wave X-band EPR spectra and M. S. Fataftah, M. J. Graham for helpful discussions. We acknowledge support from Northwestern University and the state of Illinois. This material is based upon work supported by the U.S. Department of Energy Office of Science, Office of Basic Energy Sciences, Division of Chemical Sciences, Geosciences, and Biosciences, under Contract DE-AC02-06CH11357 (J.N. and O.G.P.). NR 42 TC 20 Z9 20 U1 4 U2 40 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0002-7863 J9 J AM CHEM SOC JI J. Am. Chem. Soc. PD NOV 12 PY 2014 VL 136 IS 45 BP 15841 EP 15844 DI 10.1021/ja507846k PG 4 WC Chemistry, Multidisciplinary SC Chemistry GA AT4JQ UT WOS:000344906100009 PM 25340518 ER PT J AU Zhang, S Hao, YZ Su, D Doan-Nguyen, VVT Wu, YT Li, J Sun, SH Murray, CB AF Zhang, Sen Hao, Yizhou Su, Dong Doan-Nguyen, Vicky V. T. Wu, Yaoting Li, Jing Sun, Shouheng Murray, Christopher B. TI Monodisperse Core/Shell Ni/FePt Nanoparticles and Their Conversion to Ni/Pt to Catalyze Oxygen Reduction SO JOURNAL OF THE AMERICAN CHEMICAL SOCIETY LA English DT Article ID ALLOY NANOPARTICLES; STRAIN CONTROL; ELECTROCATALYSTS; SHELL; CORE; MONOLAYER; NANOWIRES; EFFICIENT; PD; ELECTROOXIDATION AB We report a size-controllable synthesis of monodisperse core/shell Ni/FePt nanoparticles (NPs) via a seed-mediated growth and their subsequent conversion to Ni/Pt NPs. Preventing surface oxidation of the Ni seeds is essential for the growth of uniform FePt shells. These Ni/FePt NPs have a thin (approximate to 1 nm) FePt shell and can be converted to Ni/Pt by acetic acid wash to yield active catalysts for oxygen reduction reaction (ORR). Tuning the core size allows the optimization of their electrocatalytic activity. The specific activity and mass activity of 4.2/0.8 nm core/shell Ni/FePt after acetic acid wash reach 1.95 mA/cm(2) and 490 mA/mg(pt) at 0.9 V (vs reversible hydrogen electrode), which are much higher than those of benchmark commercial Pt catalyst (0.34 mA/cm(2) and 92 mA/mg(pt) at 0.9 V). Our studies provide a robust approach to monodisperse core/shell NPs with nonprecious metal core, making it possible to develop advanced NP catalysts with ultralow Pt content for ORR and many other heterogeneous reactions. C1 [Zhang, Sen; Wu, Yaoting; Murray, Christopher B.] Univ Penn, Dept Chem, Philadelphia, PA 19104 USA. [Hao, Yizhou; Doan-Nguyen, Vicky V. T.; Murray, Christopher B.] Univ Penn, Dept Mat Sci & Engn, Philadelphia, PA 19104 USA. [Su, Dong; Li, Jing] Brookhaven Natl Lab, Ctr Funct Nanomat, Upton, NY 11973 USA. [Sun, Shouheng] Brown Univ, Dept Chem, Providence, RI 02912 USA. RP Murray, CB (reprint author), Univ Penn, Dept Chem, Philadelphia, PA 19104 USA. EM cbmurray@sas.upenn.edu RI Zhang, Sen/E-4226-2015 FU Nature Conservancy; U.S. Department of Energy, Office of Basic Energy Sciences [DE-AC02-98CH10886]; Catalysis Center for Energy Innovation, an Energy Frontier Research Center; U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-SC0001004]; U.S. Department of Energy, Office of Energy Efficiency and Renewable Energy, Fuel Cell Technologies Program; U.S. Army Research Laboratory; U.S. Army Research Office under the Multi University Research Initiative (MURI) [W911NF-11-1-0353] FX This work was supported by NatureNet Science Fellowship from The Nature Conservancy. Partial work on electron microscopy carried out at the Center for Functional Nanomaterials, Brookhaven National Laboratory, was supported by the U.S. Department of Energy, Office of Basic Energy Sciences, under contract no. DE-AC02-98CH10886. Partial work on Ni nanoparticle chemistry was supported by the Catalysis Center for Energy Innovation, an Energy Frontier Research Center funded by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences under award no. DE-SC0001004. Partial work on electrochemistry was supported by the U.S. Department of Energy, Office of Energy Efficiency and Renewable Energy, Fuel Cell Technologies Program and by the U.S. Army Research Laboratory and the U.S. Army Research Office under the Multi University Research Initiative (MURI, grant no. W911NF-11-1-0353) on "Stress-Controlled Catalysis via Engineered Nanostructures". NR 47 TC 47 Z9 48 U1 36 U2 294 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0002-7863 J9 J AM CHEM SOC JI J. Am. Chem. Soc. PD NOV 12 PY 2014 VL 136 IS 45 BP 15921 EP 15924 DI 10.1021/ja5099066 PG 4 WC Chemistry, Multidisciplinary SC Chemistry GA AT4JQ UT WOS:000344906100029 PM 25350678 ER PT J AU Scott, AD Pelmenschikov, V Guo, YS Yan, LF Wang, HX George, SJ Dapper, CH Newton, WE Yoda, Y Tanaka, Y Cramer, SP AF Scott, Aubrey D. Pelmenschikov, Vladimir Guo, Yisong Yan, Lifen Wang, Hongxin George, Simon J. Dapper, Christie H. Newton, William E. Yoda, Yoshitaka Tanaka, Yoshihito Cramer, Stephen P. TI Structural Characterization of CO-Inhibited Mo-Nitrogenase by Combined Application of Nuclear Resonance Vibrational Spectroscopy, Extended X-ray Absorption Fine Structure, and Density Functional Theory: New Insights into the Effects of CO Binding and the Role of the Interstitial Atom SO JOURNAL OF THE AMERICAN CHEMICAL SOCIETY LA English DT Article ID AZOTOBACTER-VINELANDII NITROGENASE; IRON-MOLYBDENUM COFACTOR; ELECTRON-PARAMAGNETIC-RESONANCE; FEMO-COFACTOR; ACTIVE-SITE; VANADIUM NITROGENASE; CARBON-MONOXIDE; KLEBSIELLA-PNEUMONIAE; INFRARED-SPECTROSCOPY; CRYSTAL-STRUCTURE AB The properties of CO-inhibited Azotobacter vinelandii (Av) Mo-nitrogenase (N(2)ase) have been examined by the combined application of nuclear resonance vibrational spectroscopy (NRVS), extended X-ray absorption fine structure (EXAFS), and density functional theory (DFT). Dramatic changes in the NRVS are seen under high-CO conditions, especially in a 188 cm(1) mode associated with symmetric breathing of the central cage of the FeMo-cofactor. Similar changes are reproduced with the alpha-H195Q N(2)ase variant. In the frequency region above 450 cm(1), additional features are seen that are assigned to Fe-CO bending and stretching modes (confirmed by (CO)-C-13 isotope shifts). The EXAFS for wild-type N(2)ase shows evidence for a significant cluster distortion under high-CO conditions, most dramatically in the splitting of the interaction between Mo and the shell of Fe atoms originally at 5.08 angstrom in the resting enzyme. A DFT model with both a terminal -CO and a partially reduced -CHO ligand bound to adjacent Fe sites is consistent with both earlier FT-IR experiments, and the present EXAFS and NRVS observations for the wild-type enzyme. Another DFT model with two terminal CO ligands on the adjacent Fe atoms yields Fe-CO bands consistent with the alpha-H195Q variant NRVS. The calculations also shed light on the vibrational shake modes of the interstitial atom inside the central cage, and their interaction with the Fe-CO modes. Implications for the CO and N-2 reactivity of N(2)ase are discussed. C1 [Pelmenschikov, Vladimir] Tech Univ Berlin, Inst Chem, D-10623 Berlin, Germany. [Scott, Aubrey D.; Yan, Lifen; Wang, Hongxin; George, Simon J.; Cramer, Stephen P.] Univ Calif Davis, Dept Chem, Davis, CA 95616 USA. [Guo, Yisong] Carnegie Mellon Univ, Dept Chem, Pittsburgh, PA 15213 USA. [Wang, Hongxin; Cramer, Stephen P.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Phys Biosci Div, Berkeley, CA 94720 USA. [Dapper, Christie H.; Newton, William E.] Virginia Polytech Inst & State Univ, Dept Biochem, Blacksburg, VA 24061 USA. [Yoda, Yoshitaka] SPring8 JASRI, Res & Utilizat Div, Sayo, Hyogo 6795198, Japan. [Tanaka, Yoshihito] RIKEN SPring 8 Ctr, SR Mat Sci Instrumentat Unit, Sayo, Hyogo 6795148, Japan. RP Cramer, SP (reprint author), Univ Calif Davis, Dept Chem, Davis, CA 95616 USA. EM spjcramer@ucdavis.edu RI Guo, Yisong/C-7785-2009 OI Guo, Yisong/0000-0002-4132-3565 FU NIH [GM-65440]; NSF [CHE 1308384]; DOE Office of Biological and Environmental Research; Deutsche Forschungsgemeinschaft (DFG) via the "Unifying Concepts in Catalysis" (UniCat) Excellence Cluster FX We thank Saeed Kamali for assistance early on with NRVS data collection at SPring-8. The experiments at SPring-8 were performed at BL09XU with the approval of JASRI (Proposal No. 2009A0015-2013B0103), and at BL19LXU with the approval of RIKEN (Proposal No. 20120107 and 20130022). V.P. thanks Sven de Marothy for the XYZviewer program. This work was funded by NIH grant GM-65440 (S.P.C.), NSF grant CHE 1308384 (S.P.C.), the DOE Office of Biological and Environmental Research (S.P.C.), and the Deutsche Forschungsgemeinschaft (DFG) via the "Unifying Concepts in Catalysis" (UniCat) Excellence Cluster (V.P.). NR 100 TC 8 Z9 8 U1 10 U2 64 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0002-7863 J9 J AM CHEM SOC JI J. Am. Chem. Soc. PD NOV 12 PY 2014 VL 136 IS 45 BP 15942 EP 15954 DI 10.1021/ja505720m PG 13 WC Chemistry, Multidisciplinary SC Chemistry GA AT4JQ UT WOS:000344906100033 PM 25275608 ER PT J AU Senesi, AJ Eichelsdoerfer, DJ Brown, KA Lee, B Auyeung, E Choi, CHJ Macfarlane, RJ Young, KL Mirkin, CA AF Senesi, Andrew J. Eichelsdoerfer, Daniel J. Brown, Keith A. Lee, Byeongdu Auyeung, Evelyn Choi, Chung Hang J. Macfarlane, Robert J. Young, Kaylie L. Mirkin, Chad A. TI Oligonucleotide Flexibility Dictates Crystal Quality in DNA-Programmable Nanoparticle Superlattices SO ADVANCED MATERIALS LA English DT Article DE DNA; superlattices; metamaterials; X-ray scattering; ligand flexibility ID SINGLE-STRANDED-DNA; GRAIN-GROWTH; REFRACTIVE-INDEX; ATOM EQUIVALENTS; METAMATERIALS; PARTICLES; CRYSTALLIZATION; MOLECULES; RANGE; NANOSTRUCTURES C1 [Senesi, Andrew J.; Eichelsdoerfer, Daniel J.; Brown, Keith A.; Choi, Chung Hang J.; Macfarlane, Robert J.; Young, Kaylie L.; Mirkin, Chad A.] Northwestern Univ, Dept Chem, Evanston, IL 60208 USA. [Senesi, Andrew J.; Lee, Byeongdu] Argonne Natl Lab, Xray Sci Div, Argonne, IL 60439 USA. [Auyeung, Evelyn; Mirkin, Chad A.] Northwestern Univ, Dept Mat Sci & Engn, Evanston, IL 60208 USA. RP Mirkin, CA (reprint author), Northwestern Univ, Dept Chem, 2145 Sheridan Rd, Evanston, IL 60208 USA. EM chadnano@northwestern.edu RI Mirkin, Chad/E-3911-2010; OI Lee, Byeongdu/0000-0003-2514-8805 FU AFOSR Awards [FA9550-11-1-0275, FA9550-12-1-0141]; Department of Defense [32 CFR 168a]; AFOSR [32 CFR 168a]; Northwestern University's International Institute for Nanotechnology; Croucher Foundation; U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-AC02-06CH11357] FX This material is based upon work supported by the AFOSR Awards FA9550-11-1-0275 and FA9550-12-1-0141. D.J.E., E.A. and K.L.Y. acknowledge the Department of Defense and AFOSR for a National Defense Science and Engineering Graduate (NDSEG) Fellowship, 32 CFR 168a. K.A.B. gratefully acknowledges support from Northwestern University's International Institute for Nanotechnology. C.H.J.C. acknowledges a postdoctoral research fellowship from The Croucher Foundation. The SAXS experiments were carried out at Sector 5-ID of the DuPont-Northwestern-Dow Collaborative Access Team and Sector 12-ID-B at the Advanced Photon Source. Use of the Advanced Photon Source at Argonne National Laboratory was supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract No. DE-AC02-06CH11357. The TEM work was performed at the EPIC facility of the NU Atomic and Nanoscale Characterization Experimental Center (NUANCE) at Northwestern University. NR 56 TC 15 Z9 15 U1 1 U2 43 PU WILEY-V C H VERLAG GMBH PI WEINHEIM PA BOSCHSTRASSE 12, D-69469 WEINHEIM, GERMANY SN 0935-9648 EI 1521-4095 J9 ADV MATER JI Adv. Mater. PD NOV 12 PY 2014 VL 26 IS 42 BP 7235 EP 7240 DI 10.1002/adma.201402548 PG 6 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied; Physics, Condensed Matter SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AT2RS UT WOS:000344783300013 PM 25244608 ER PT J AU Sales, BC Saparov, B McGuire, MA Singh, DJ Parker, DS AF Sales, Brian C. Saparov, Bayrammurad McGuire, Michael A. Singh, David J. Parker, David S. TI Ferromagnetism of Fe3Sn and Alloys SO SCIENTIFIC REPORTS LA English DT Article ID HARD MAGNETIC-MATERIALS; INTERMETALLIC COMPOUNDS; SINGLE-CRYSTALS; DIFFRACTION AB Hexagonal Fe3Sn has many of the desirable properties for a new permanent magnet phase with a Curie temperature of 725 K, a saturation moment of 1.18 MA/m. and anisotropy energy, K-1 of 1.8 MJ/m(3). However, contrary to earlier experimental reports, we found both experimentally and theoretically that the easy magnetic axis lies in the hexagonal plane, which is undesirable for a permanent magnet material. One possibility for changing the easy axis direction is through alloying. We used first principles calculations to investigate the effect of elemental substitutions. The calculations showed that substitution on the Sn site has the potential to switch the easy axis direction. However, transition metal substitutions with Co or Mn do not have this effect. We attempted synthesis of a number of these alloys and found results in accord with the theoretical predictions for those that were formed. However, the alloys that could be readily made all showed an in-plane easy axis. The electronic structure of Fe3Sn is reported, as are some are magnetic and structural properties for the Fe3Sn2, and Fe5Sn3 compounds, which could be prepared as mm-sized single crystals. C1 [Sales, Brian C.; Saparov, Bayrammurad; McGuire, Michael A.; Singh, David J.; Parker, David S.] Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37831 USA. RP Sales, BC (reprint author), Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37831 USA. EM salesbc@ornl.gov RI McGuire, Michael/B-5453-2009 OI McGuire, Michael/0000-0003-1762-9406 FU Critical Materials Institute, an Energy Innovation Hub - U.S. Department of Energy, Office of Energy Efficiency and Renewable Energy, Advanced Manufacturing Office; U.S. Department of Energy, Office of Energy Efficiency and Renewable Energy, Vehicle Technologies, Propulsion Materials Program FX This research was supported by the Critical Materials Institute, an Energy Innovation Hub funded by the U.S. Department of Energy, Office of Energy Efficiency and Renewable Energy, Advanced Manufacturing Office. MAM. acknowledges support of the U.S. Department of Energy, Office of Energy Efficiency and Renewable Energy, Vehicle Technologies, Propulsion Materials Program. NR 15 TC 6 Z9 6 U1 13 U2 63 PU NATURE PUBLISHING GROUP PI LONDON PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND SN 2045-2322 J9 SCI REP-UK JI Sci Rep PD NOV 12 PY 2014 VL 4 AR 7024 DI 10.1038/srep07024 PG 6 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AT2JL UT WOS:000344760700014 PM 25387850 ER PT J AU Laverock, J Chen, B Preston, ARH Newby, D Piper, LFJ Tung, LD Balakrishnan, G Glans, PA Guo, JH Smith, KE AF Laverock, J. Chen, B. Preston, A. R. H. Newby, D. Piper, L. F. J. Tung, L. D. Balakrishnan, G. Glans, P-A Guo, J-H Smith, K. E. TI Low-energy V t(2g) orbital excitations in NdVO3 SO JOURNAL OF PHYSICS-CONDENSED MATTER LA English DT Article DE resonant inelastic x-ray scattering; orbital excitations; crystal field excitations ID ELEMENTARY EXCITATIONS; ORDER AB The electronic structure of NdVO3 and YVO3 has been investigated as a function of sample temperature using resonant inelastic soft x-ray scattering at the V L-3-edge. Most of the observed spectral features are in good agreement with an atomic crystal-field multiplet model. However, a low energy feature is observed at similar to 0.4 eV that cannot be explained by crystal-field arguments. The resonant behaviour of this feature establishes it as due to excitations of the V t(2g) states. Moreover, this feature exhibits a strong sample temperature dependence, reaching maximum intensity in the orbitally-ordered phase of NdVO3, before becoming suppressed at low temperatures. This behaviour indicates that the origin of this feature is a collective orbital excitation, i.e. the bi-orbiton. C1 [Laverock, J.; Chen, B.; Preston, A. R. H.; Newby, D.; Piper, L. F. J.; Smith, K. E.] Boston Univ, Dept Phys, Boston, MA 02215 USA. [Piper, L. F. J.] Binghamton Univ, Dept Phys Appl Phys & Astron, Binghamton, NY 13902 USA. [Tung, L. D.; Balakrishnan, G.] Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England. [Glans, P-A; Guo, J-H] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Dept Phys, Berkeley, CA 94720 USA. [Smith, K. E.] Univ Auckland, Sch Chem Sci, Auckland 1142, New Zealand. [Smith, K. E.] Univ Auckland, MacDiarmid Inst Adv Mat & Nanotechnol, Auckland 1142, New Zealand. RP Laverock, J (reprint author), Boston Univ, Dept Phys, 590 Commonwealth Ave, Boston, MA 02215 USA. EM laverock@bu.edu RI Laverock, Jude/G-4537-2010; Glans, Per-Anders/G-8674-2016; Piper, Louis/C-2960-2011; Balakrishnan, Geetha/P-5977-2016; Chen, Bo/C-5428-2017 OI Laverock, Jude/0000-0003-3653-8171; Piper, Louis/0000-0002-3421-3210; Balakrishnan, Geetha/0000-0002-5890-1149; Chen, Bo/0000-0002-9263-5171 FU Department of Energy [DE-FG02-98ER45680]; US Department of Energy [DE-AC02-05CH11231, DE-AC02-98CH10886]; EPSRC [EP/I007210/1] FX The Boston University program is supported in part by the Department of Energy under Grant No. DE-FG02-98ER45680. The ALS, Berkeley, is supported by the US Department of Energy under Contract No. DE-AC02-05CH11231. The NSLS, Brookhaven, is supported by the US Department of Energy under Contract No. DE-AC02-98CH10886. GB gratefully acknowledges financial support from EPSRC Grant EP/I007210/1. NR 38 TC 1 Z9 1 U1 4 U2 21 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0953-8984 EI 1361-648X J9 J PHYS-CONDENS MAT JI J. Phys.-Condes. Matter PD NOV 12 PY 2014 VL 26 IS 45 AR 455603 DI 10.1088/0953-8984/26/45/455603 PG 9 WC Physics, Condensed Matter SC Physics GA AR7ZT UT WOS:000343796200011 PM 25336521 ER PT J AU Zhao, X Nguyen, MC Wang, CZ Ho, KM AF Zhao, Xin Manh Cuong Nguyen Wang, Cai-Zhuang Ho, Kai-Ming TI New stable Re-B phases for ultra-hard materials SO JOURNAL OF PHYSICS-CONDENSED MATTER LA English DT Article DE ultra-hard materials; rhenium boride; genetic algorithm; first-principles calculations ID SUPERHARD RHENIUM DIBORIDE; AUGMENTED-WAVE METHOD; AMBIENT-PRESSURE; BORIDES; SUPERCONDUCTIVITY; STABILITY AB As a distinct class of ultra-hard materials, transition metal borides are found to have superior mechanical properties that challenge the traditional materials. In this work, we explored new stable structures for rhenium borides with different stoichiometries using genetic algorithm in combination with first-principles calculations. Based on theoretical calculations, ReB in a P-3m1 structure is found to be stable against decomposition reactions below 10 GPa and ReB3 in a P-6m2 structure is stable above 22 GPa. Two new phases of Re2B are predicted to be thermodynamically stable at pressures higher than 55 GPa and 80 GPa respectively. We also show that a C2/m structure discovered for ReB4 has energy lower than that of the R-3m structure reported earlier (Wang et al 2013 J. Alloys Compd. 573 20). Elastic and vibrational properties from first-principles calculations indicate that the low-energy structures obtained in our search are mechanically and dynamically stable and are promising targets as new ultra-hard materials. C1 [Zhao, Xin] US DOE, Ames Lab, Ames, IA 50011 USA. Iowa State Univ, Dept Phys & Astron, Ames, IA 50011 USA. RP Zhao, X (reprint author), US DOE, Ames Lab, Ames, IA 50011 USA. EM wangcz@ameslab.gov RI Nguyen, Manh Cuong/G-2783-2015; OI Nguyen, Manh Cuong/0000-0001-8027-9029; Zhao, Xin/0000-0002-3580-512X FU US Department of Energy, Basic Energy Sciences, Division of Materials Science and Engineering [DE-AC02-07CH11358] FX Work at Ames Laboratory was supported by the US Department of Energy, Basic Energy Sciences, Division of Materials Science and Engineering, under Contract No. DE-AC02-07CH11358, including a grant of computer time at the National Energy Research Supercomputing Centre (NERSC) in Berkeley, CA. NR 28 TC 2 Z9 2 U1 1 U2 23 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0953-8984 EI 1361-648X J9 J PHYS-CONDENS MAT JI J. Phys.-Condes. Matter PD NOV 12 PY 2014 VL 26 IS 45 AR 455401 DI 10.1088/0953-8984/26/45/455401 PG 7 WC Physics, Condensed Matter SC Physics GA AR7ZT UT WOS:000343796200007 PM 25318642 ER PT J AU Reddi, K Elgowainy, A Sutherland, E AF Reddi, Krishna Elgowainy, Amgad Sutherland, Erika TI Hydrogen refueling station compression and storage optimization with tube-trailer deliveries SO INTERNATIONAL JOURNAL OF HYDROGEN ENERGY LA English DT Article DE Hydrogen refueling station; Tube-trailer; Simulation model; Compression; Storage; Fuel cell electric vehicles ID CYLINDER AB Hydrogen refueling stations require high capital investment, with compression and storage comprising more than half of the installed cost of refueling equipment. Refueling station configurations and operation strategies can reduce capital investment while improving equipment utilization. Argonne National Laboratory developed a refueling model to evaluate the impact of various refueling compression and storage configurations and tube trailer operating strategies on the cost of hydrogen refueling. The modeling results revealed that a number of strategies can be employed to reduce fueling costs. Proper sizing of the high-pressure buffer storage reduces the compression requirement considerably, thus reducing refueling costs. Employing a tube trailer to initially fill the vehicle's tank also reduces the compression and storage requirements, further reducing refueling costs. Reducing the cut-off pressure of the tube trailer for initial vehicle fills can also significantly reduce the refueling costs. Finally, increasing the trailer's return pressure can cut refueling costs, especially for delivery distances less than 100 km, and in early markets, when refueling stations will be grossly underutilized. Copyright (C) 2014, Hydrogen Energy Publications, LLC. Published by Elsevier Ltd. All rights reserved. C1 [Reddi, Krishna; Elgowainy, Amgad] Argonne Natl Lab, Argonne, IL 60439 USA. [Sutherland, Erika] US DOE, Fuel Cell Technol Off, Washington, DC 20585 USA. RP Reddi, K (reprint author), Argonne Natl Lab, 9700 S Cass Ave, Argonne, IL 60439 USA. EM kreddi@anl.gov FU Fuel Cell Technologies Office of the U.S. Department of Energy's Office of Energy Efficiency and Renewable Energy [DE-ACO2-06CH11357] FX This research effort was supported by the Fuel Cell Technologies Office of the U.S. Department of Energy's Office of Energy Efficiency and Renewable Energy under Contract Number DE-ACO2-06CH11357. NR 35 TC 5 Z9 5 U1 1 U2 16 PU PERGAMON-ELSEVIER SCIENCE LTD PI OXFORD PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, ENGLAND SN 0360-3199 EI 1879-3487 J9 INT J HYDROGEN ENERG JI Int. J. Hydrog. Energy PD NOV 11 PY 2014 VL 39 IS 33 BP 19169 EP 19181 DI 10.1016/j.ijhydene.2014.09.099 PG 13 WC Chemistry, Physical; Electrochemistry; Energy & Fuels SC Chemistry; Electrochemistry; Energy & Fuels GA AU7TO UT WOS:000345803900046 ER PT J AU Kogan, VG Mints, RG AF Kogan, V. G. Mints, R. G. TI Effect of current injection into thin-film Josephson junctions SO PHYSICAL REVIEW B LA English DT Article ID FLUX AB New thin-film Josephson junctions have recently been tested in which the current injected into one of the junction banks governs Josephson phenomena. One thus can continuously manage the phase distribution at the junction by changing the injected current. A method of calculating the distribution of injected currents is proposed for a half-infinite thin-film strip with source-sink points at arbitrary positions at the film edges. The strip width W is assumed small relative to Lambda = 2 lambda(2)/d; lambda is the bulk London penetration depth of the film material and d is the film thickness. C1 [Kogan, V. G.] US DOE, Ames Lab, Ames, IA 50011 USA. [Mints, R. G.] Tel Aviv Univ, Raymond & Beverly Sackler Sch Phys & Astron, IL-69978 Tel Aviv, Israel. RP Kogan, VG (reprint author), US DOE, Ames Lab, Ames, IA 50011 USA. EM kogan@ameslab.gov; mints@post.tau.ac.il FU Department of Energy, Office of Basic Energy Sciences, Division of Materials Sciences and Engineering [DE-AC02-07CH11358] FX The authors are grateful to A. Ustinov for the interest and comments and to E. Goldobin for sharing experimental information and many helpful discussions. The Ames Laboratory is supported by the Department of Energy, Office of Basic Energy Sciences, Division of Materials Sciences and Engineering under Contract No. DE-AC02-07CH11358. NR 13 TC 0 Z9 0 U1 2 U2 6 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1098-0121 EI 1550-235X J9 PHYS REV B JI Phys. Rev. B PD NOV 11 PY 2014 VL 90 IS 18 AR 184504 DI 10.1103/PhysRevB.90.184504 PG 5 WC Physics, Condensed Matter SC Physics GA AU2RL UT WOS:000345465300004 ER PT J AU Lucy, JM Ball, MR Restrepo, OD Hauser, AJ Soliz, JR Freeland, JW Woodward, PM Windl, W Yang, FY AF Lucy, J. M. Ball, M. R. Restrepo, O. D. Hauser, A. J. Soliz, J. R. Freeland, J. W. Woodward, P. M. Windl, W. Yang, F. Y. TI Strain-tunable extraordinary magnetocrystalline anisotropy in Sr2CrReO6 epitaxial films SO PHYSICAL REVIEW B LA English DT Article ID INITIO MOLECULAR-DYNAMICS; MAGNETIC-ANISOTROPY; TRANSITION; MOMENT; NI AB We report the discovery of extraordinarily large anisotropy fields and strain-tunable magnetocrystalline anisotropy in Sr2CrReO6 epitaxial films. We determine the strain-induced tetragonal distortions and octahedral rotations in Sr2CrReO6 epitaxial films grown on (LaAlO3)(0.3)(Sr2AlTaO6)(0.7) (LSAT), SrTiO3 (STO), and SrCr0.5Nb0.5O3/LSAT substrates using x-ray diffraction and density functional theory. The structural distortions drive dramatic changes in magnetocrystalline anisotropy. We use magnetometry measurements and first principles calculations to determine the atomic origins of the large anisotropy observed. These techniques elucidate the interplay between structural deformations and magnetic behavior and lay the groundwork for the study of other strongly correlated systems in this class of ferromagnetic oxides. C1 [Lucy, J. M.; Yang, F. Y.] Ohio State Univ, Dept Phys, Columbus, OH 43210 USA. [Ball, M. R.; Restrepo, O. D.; Windl, W.] Ohio State Univ, Dept Mat Sci & Engn, Columbus, OH 43210 USA. [Hauser, A. J.] Univ Calif Santa Barbara, California Nanosyst Inst, Santa Barbara, CA 93106 USA. [Soliz, J. R.; Woodward, P. M.] Ohio State Univ, Dept Chem, Columbus, OH 43210 USA. [Freeland, J. W.] Argonne Natl Lab, Adv Photon Source, Argonne, IL 60439 USA. RP Lucy, JM (reprint author), Ohio State Univ, Dept Phys, 191 West Woodruff Ave, Columbus, OH 43210 USA. EM fyyang@physics.osu.edu FU Center for Emergent Materials at the Ohio State University; NanoSystems Laboratory; Center for Electron Microscopy and Analysis at The Ohio State University; U.S. Department of Energy, Office of Science [DEAC02-06CH11357]; NSF Materials Research Science and Engineering Center [DMR-1420451] FX This work is supported by the Center for Emergent Materials at the Ohio State University, a NSF Materials Research Science and Engineering Center (DMR-1420451). Partial support is provided by the NanoSystems Laboratory and the Center for Electron Microscopy and Analysis at The Ohio State University. Work at Argonne National Laboratory, including the Advanced Photon Source, is supported by the U.S. Department of Energy, Office of Science under Grant No. DEAC02-06CH11357. NR 38 TC 5 Z9 5 U1 2 U2 27 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1098-0121 EI 1550-235X J9 PHYS REV B JI Phys. Rev. B PD NOV 11 PY 2014 VL 90 IS 18 AR 180401 DI 10.1103/PhysRevB.90.180401 PG 6 WC Physics, Condensed Matter SC Physics GA AU2RL UT WOS:000345465300001 ER PT J AU Mattsson, TR Root, S Mattsson, AE Shulenburger, L Magyar, RJ Flicker, DG AF Mattsson, Thomas R. Root, Seth Mattsson, Ann E. Shulenburger, Luke Magyar, Rudolph J. Flicker, Dawn G. TI Validating density-functional theory simulations at high energy-density conditions with liquid krypton shock experiments to 850 GPa on Sandia's Z machine SO PHYSICAL REVIEW B LA English DT Article ID INITIO MOLECULAR-DYNAMICS; AUGMENTED-WAVE METHOD; SOLID KRYPTON; PHASE-TRANSITIONS; ELECTRON-GAS; STATE; EQUATION; XENON AB We use Sandia's Z machine and magnetically accelerated flyer plates to shock compress liquid krypton to 850 GPa and compare with results from density-functional theory (DFT) based simulations using the AM05 functional. We also employ quantum Monte Carlo calculations to motivate the choice of AM05. We conclude that the DFT results are sensitive to the quality of the pseudopotential in terms of scattering properties at high energy/temperature. A new Kr projector augmented wave potential was constructed with improved scattering properties which resulted in excellent agreement with the experimental results to 850 GPa and temperatures above 10 eV (110 kK). Finally, we present comparisons of our data from the Z experiments and DFT calculations to current equation of state models of krypton to determine the best model for high energy-density applications. C1 [Mattsson, Thomas R.; Root, Seth; Mattsson, Ann E.; Shulenburger, Luke; Magyar, Rudolph J.; Flicker, Dawn G.] Sandia Natl Labs, Albuquerque, NM 87185 USA. RP Mattsson, TR (reprint author), Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA. EM trmatts@sandia.gov; sroot@sandia.gov; aematts@sandia.gov; lshulen@sandia.gov; rjmagya@sandia.gov; dgflick@sandia.gov FU NNSA Science Campaigns; Predictive Theory and Modeling for Materials and Chemical Science program; Office of Basic Energy Sciences (BES); Department of Energy (DOE); U.S. Department of Energy's National Nuclear Security Administration [DE-AC04-94AL85000] FX The authors thank all members of the Sandia Z facility that contributed to the design, fabrication, and fielding of the Z experiments. The authors especially appreciate the dedicated efforts of the cryo-team: A. Lopez, J. Lynch, J. Villalva, and K. Shelton as well as the engineering designs by D. Dalton and the diagnostics by C. Meyer. The work was supported by the NNSA Science Campaigns. L.S. was supported through the Predictive Theory and Modeling for Materials and Chemical Science program by the Office of Basic Energy Sciences (BES), Department of Energy (DOE). Sandia National Laboratories is a multiprogram laboratory operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Company, for the U.S. Department of Energy's National Nuclear Security Administration under Contract No. DE-AC04-94AL85000. NR 53 TC 3 Z9 3 U1 3 U2 18 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1098-0121 EI 1550-235X J9 PHYS REV B JI Phys. Rev. B PD NOV 11 PY 2014 VL 90 IS 18 AR 184105 DI 10.1103/PhysRevB.90.184105 PG 10 WC Physics, Condensed Matter SC Physics GA AU2RL UT WOS:000345465300003 ER PT J AU Shi, HL Saparov, B Singh, DJ Sefat, AS Du, MH AF Shi, Hongliang Saparov, Bayrammurad Singh, David J. Sefat, Athena S. Du, Mao-Hua TI Ternary chalcogenides Cs2Zn3Se4 and Cs2Zn3Te4: Potential p-type transparent conducting materials SO PHYSICAL REVIEW B LA English DT Article ID MOLECULAR-BEAM EPITAXY; WIDE-BAND-GAP; SEMICONDUCTOR NANOCRYSTALS; ELECTRICAL-CONDUCTION; DIMENSIONAL REDUCTION; DELAFOSSITE STRUCTURE; CUPROUS DELAFOSSITES; DEFECT MECHANISMS; THIN-FILMS; OXIDE AB We report the prediction of two ternary chalcogenides that can potentially be used as p-type transparent conductors along with experimental synthesis and initial characterization of these compounds, Cs(2)Zn(3)Ch(4) (Ch = Se, Te). In particular, the structures are predicted based on density functional calculations and confirmed by experiments. Phase diagrams, electronic structure, optical properties, and defect properties of Cs2Zn3Se4 and Cs2Zn3Te4 are calculated to assess the viability of these materials as p-type transparent conducting materials (TCMs). Cs2Zn3Se4 and Cs2Zn3Te4, which are stable under ambient air, display large optical band gaps (calculated to be 3.61 and 2.83 eV, respectively) and have small hole effective masses (0.5-0.77m(e)) that compare favorably with other proposed p-type TCMs. Defect calculations show that undoped Cs2Zn3Se4 and Cs2Zn3Te4 are p-type materials. However, the free hole concentration may be limited by low-energy native donor defects, e.g., Zn interstitials. Nonequilibrium growth techniques should be useful for suppressing the formation of native donor defects, thereby increasing the hole concentration. C1 [Shi, Hongliang; Saparov, Bayrammurad; Singh, David J.; Sefat, Athena S.; Du, Mao-Hua] Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA. RP Shi, HL (reprint author), Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA. EM mhdu@ornl.gov RI Shi, Hongliang/A-7568-2010; Du, Mao-Hua/B-2108-2010; Sefat, Athena/R-5457-2016 OI Shi, Hongliang/0000-0003-0713-4688; Du, Mao-Hua/0000-0001-8796-167X; Sefat, Athena/0000-0002-5596-3504 FU Department of Energy, Basic Energy Sciences, Materials Sciences and Engineering Division FX This paper was supported by the Department of Energy, Basic Energy Sciences, Materials Sciences and Engineering Division. NR 68 TC 3 Z9 3 U1 1 U2 19 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 2469-9950 EI 2469-9969 J9 PHYS REV B JI Phys. Rev. B PD NOV 11 PY 2014 VL 90 IS 18 AR 184104 DI 10.1103/PhysRevB.90.184104 PG 9 WC Physics, Condensed Matter SC Physics GA AU2RL UT WOS:000345465300002 ER PT J AU Coloma, P Minakata, H Parke, SJ AF Coloma, Pilar Minakata, Hisakazu Parke, Stephen J. TI Interplay between appearance and disappearance channels for precision measurements of theta(23) and delta SO PHYSICAL REVIEW D LA English DT Article ID NEUTRINO OSCILLATION EXPERIMENTS; LINE-EXPERIMENT-SIMULATOR; LEPTONIC CP VIOLATION; NO-NU-A; SOLAR; BEAM; T2K AB We discuss how the CP- violating phase delta and the mixing angle theta(23) can be measured precisely in an environment where there are strong correlations between them. This is achieved by paying special attention to the mutual roles and the interplay between the appearance and the disappearance channels in longbaseline neutrino oscillation experiments. We analyze and clarify the general structure of the theta(23) - theta(13) - delta degeneracy for both the appearance and disappearance channels in a more complete fashion than what has previously been discussed in the literature. A full understanding of this degeneracy is of vital importance if theta(23) is close to maximal mixing. The relative importance between the appearance and disappearance channels depends upon the particular setup and how close to maximal mixing nature has chosen the value for theta(23). For facilities that operate with a narrow band beam or a wideband beam centered on the first oscillation extremum, the contribution of the disappearance channel depends critically on the systematic uncertainties assumed for this channel, whereas for facilities that operate at energies above the first oscillation extremum or at the second oscillation extremum, the appearance channels dominate. On the other hand, for d we find that the disappearance channel usually improves the sensitivity, modestly for facilities around the first oscillation extremum and more significantly for facilities operating at an energy above the first oscillation extremum, especially near delta similar to +/-pi 2 C1 [Coloma, Pilar] Virginia Tech, Ctr Neutrino Phys, Blacksburg, VA 24061 USA. [Minakata, Hisakazu] Univ Sao Paulo, Inst Fis, BR-05315970 Sao Paulo, Brazil. [Parke, Stephen J.] Fermilab Natl Accelerator Lab, Dept Theoret Phys, Batavia, IL 60510 USA. RP Coloma, P (reprint author), Virginia Tech, Ctr Neutrino Phys, Blacksburg, VA 24061 USA. EM pcoloma@vt.edu; hisakazu.minakata@gmail.com; parke@fnal.gov OI Coloma, Pilar/0000-0002-1164-9900; Parke, Stephen/0000-0003-2028-6782 FU NORDITA; organizers of the workshop "NuNews: News in Neutrino Physics,"; KAKENHI through Tokyo Metropolitan University; Japan Society' for the Promotion of Science [23540315]; European Union FP7 ITN INVISIBLES (Marie Curie Actions [PITN-GA-2011-289442]; Fermi Research Alliance [DEACO2-07CH11359]; U.S. Department of Energy [DE-SC0003915] FX All the authors thank NORDITA and the organizers of the workshop "NuNews: News in Neutrino Physics," where part of this work was completed, for financial support and hospitality. P. C. thanks Enrique Fernandez-Martinez for providing the files needed to simulate the ESSvSB setup. P. C. and H. M. thank the Fermilab Theory Group for hospitality during their visits. H. M. thanks Universidade de Sao Paulo for the great opportunity of a stay as Pesquisador Visitante Internacional. He is also partially supported by KAKENHI received through Tokyo Metropolitan University, Grant-inAid for Scientific Research No. 23540315, Japan Society' for the Promotion of Science. S. P. acknowledges partial support from the European Union FP7 ITN INVISIBLES (Marie Curie Actions, PITN-GA-2011-289442). Fermilab is operated by the Fermi Research Alliance under Contract No. DEACO2-07CH11359 with the U.S. Department of Energy'. Also, this work has been partially supported by the U.S. Department of Energy under Grant No. DE-SC0003915. NR 75 TC 16 Z9 16 U1 0 U2 3 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1550-7998 EI 1550-2368 J9 PHYS REV D JI Phys. Rev. D PD NOV 11 PY 2014 VL 90 IS 9 AR 093003 DI 10.1103/PhysRevD.90.093003 PG 17 WC Astronomy & Astrophysics; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AU3SQ UT WOS:000345534300002 ER PT J AU TerAvest, MA Zajdel, TJ Ajo-Franklin, CM AF TerAvest, Michaela A. Zajdel, Tom J. Ajo-Franklin, Caroline M. TI The Mtr Pathway of Shewanella oneidensis MR-1 Couples Substrate Utilization to Current Production in Escherichia coli SO CHEMELECTROCHEM LA English DT Article DE bioelectrochemistry; Escherichia coli; metabolic engineering; Shewanella oneidensis; synthetic biology ID STRAIN MR-1; CELLS AB Introducing an electronic interface into Escherichia coli will allow its enormous synthetic biology toolkit to be leveraged in bioelectrochemical applications. While E.coli expressing the Mtr pathway of Shewanella oneidensis MR-1 transfer electrons to an anode, it has remained unclear if this current production alters the intracellular state of E.coli, which is a critical requirement for bioelectronic technologies. Here we address this by characterizing current production in Mtr-expressing E.coli and its effects on cellular viability, substrate consumption, and product generation. We found that cymA-mtr E.coli sustained approximate to 8-fold higher current levels than a control strain. This increased current production did not change E.coli viability or substrate consumption, but it did alter metabolic fluxes. A shift to more oxidized products strongly suggests that the Mtr pathway improves redox balance in E.coli. By demonstrating the Mtr module couples current production to intracellular state, this work establishes Mtr-expressing E.coli as a platform for accelerated development of bioelectronic technologies. C1 [Ajo-Franklin, Caroline M.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Phys Biosci Div, Div Mat Sci, Berkeley, CA 94720 USA. [Ajo-Franklin, Caroline M.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Synthet Biol Inst, Berkeley, CA 94720 USA. [Zajdel, Tom J.] Univ Calif Berkeley, Dept Elect Engn & Comp Sci, Berkeley, CA 94720 USA. [TerAvest, Michaela A.] Univ Calif Berkeley, Calif Inst Quantitat Biosci, Berkeley, CA 94720 USA. RP TerAvest, MA (reprint author), Univ Calif Berkeley, Calif Inst Quantitat Biosci, Berkeley, CA 94720 USA. EM cajo-franklin@lbl.gov RI Foundry, Molecular/G-9968-2014 FU Office of Naval Research [N000141310551]; Office of Science, Office of Basic Energy Sciences, of the U.S. Department of Energy [DE-AC02-05CH11231] FX This work was supported by the Office of Naval Research (award number N000141310551) and performed at the Molecular Foundry. Work at the Molecular Foundry was supported by the Office of Science, Office of Basic Energy Sciences, of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. We also thank Dr. Behzad Rad and Dr. Heather Jensen for helpful discussions related to this work. NR 15 TC 7 Z9 8 U1 1 U2 29 PU WILEY-V C H VERLAG GMBH PI WEINHEIM PA BOSCHSTRASSE 12, D-69469 WEINHEIM, GERMANY SN 2196-0216 J9 CHEMELECTROCHEM JI ChemElectroChem PD NOV 11 PY 2014 VL 1 IS 11 SI SI BP 1874 EP 1879 DI 10.1002/celc.201402194 PG 6 WC Electrochemistry SC Electrochemistry GA AT9GW UT WOS:000345237000017 ER PT J AU Byun, HS Pirbadian, S Nakano, A Shi, L El-Naggar, MY AF Byun, Hye Suk Pirbadian, Sahand Nakano, Aiichiro Shi, Liang El-Naggar, Mohamed Y. TI Kinetic Monte Carlo Simulations and Molecular Conductance Measurements of the Bacterial Decaheme Cytochrome MtrF SO CHEMELECTROCHEM LA English DT Article DE bacteria; cytochromes; electron transfer; Monte Carlo simulations; respiration ID SHEWANELLA-ONEIDENSIS MR-1; OUTER-MEMBRANE-CYTOCHROMES; EXTRACELLULAR ELECTRON-TRANSPORT; C-TYPE CYTOCHROMES; PUTREFACIENS MR-1; METAL REDUCTION; CHARGE-TRANSFER; FREE-ENERGY; NANOWIRES; OMCA AB Microorganisms overcome the considerable hurdle of respiring extracellular solid substrates by deploying large multiheme cytochrome complexes that form 20 nanometer conduits to traffic electrons through the periplasm and across the cellular outer membrane. Here we report the first kinetic Monte Carlo simulations and single-molecule scanning tunneling microscopy (STM) measurements of the Shewanella oneidensis MR-1 outer membrane decaheme cytochrome MtrF, which can perform the final electron transfer step from cells to minerals and microbial fuel cell anodes. We find that the calculated electron transport rate through MtrF is consistent with previously reported in vitro measurements of the Shewanella Mtr complex, as well as in vivo respiration rates on electrode surfaces assuming a reasonable (experimentally verified) coverage of cytochromes on the cell surface. The simulations also reveal a rich phase diagram in the overall electron occupation density of the hemes as a function of electron injection and ejection rates. Single-molecule tunneling spectroscopy confirms MtrF's ability to mediate electron transport between an STM tip and an underlying Au(111) surface, but at rates higher than expected from previously calculated heme-to-heme electron transfer rates for solvated molecules. C1 [Byun, Hye Suk; Pirbadian, Sahand; Nakano, Aiichiro; El-Naggar, Mohamed Y.] Univ So Calif, Dept Phys & Astron, Los Angeles, CA 90089 USA. [Nakano, Aiichiro] Univ So Calif, Los Angeles, CA 90089 USA. [Shi, Liang] Pacific NW Natl Lab, Richland, WA 99354 USA. RP Byun, HS (reprint author), Univ So Calif, Dept Phys & Astron, Los Angeles, CA 90089 USA. EM mnaggar@usc.edu FU Division of Chemical Sciences, Geosciences, and Biosciences, Office of Basic Energy Sciences of the US Department of Energy [DE-FG02-13ER16415] FX This work was funded by the Division of Chemical Sciences, Geosciences, and Biosciences, Office of Basic Energy Sciences of the US Department of Energy through grant DE-FG02-13ER16415 to ME-N. We gratefully acknowledge valuable conversations with J. Blumberger, K. Rosso, and M. Breuer, who provided the QM/MM calculation results to us ahead of publication (reference 17c). NR 56 TC 7 Z9 7 U1 6 U2 37 PU WILEY-V C H VERLAG GMBH PI WEINHEIM PA BOSCHSTRASSE 12, D-69469 WEINHEIM, GERMANY SN 2196-0216 J9 CHEMELECTROCHEM JI ChemElectroChem PD NOV 11 PY 2014 VL 1 IS 11 SI SI BP 1932 EP 1939 DI 10.1002/celc.201402211 PG 8 WC Electrochemistry SC Electrochemistry GA AT9GW UT WOS:000345237000025 ER PT J AU Ichihashi, O Vishnivetskaya, TA Borole, AP AF Ichihashi, Osamu Vishnivetskaya, Tatiana A. Borole, Abhijeet P. TI High-Performance Bioanode Development for Fermentable Substrates via Controlled Electroactive Biofilm Growth SO CHEMELECTROCHEM LA English DT Article DE biofilms; continuous flow; direct electron transfer; exoelectrogenic catalysts; microbial fuel cells ID MICROBIAL FUEL-CELLS; ELECTRICITY-GENERATION; AEROMONAS-HYDROPHILA; GLUCOSE; METABOLISM; CONVERSION; ANODES AB A bioanode was optimized to generate current densities reaching 38.4 +/- 4.9Am(-2), which brings bioelectrochemical systems closer to commercial consideration. Glucose and lactate were fed together in a continuous or fed-batch mode. The current density increased from 2.3Am(-2) to 38.4Am(-2) over a 33day period and remained stable thereafter. The Coulombic efficiency ranged from 50% to 80%. A change in substrate concentration from 200mgL(-1) to 5mgL(-1) decreased maximum current density from 38.4Am(-2) to 12.3Am(-2). The anode consortia included Firmicutes (55.0%), Proteobacteria (41.8%) and Bacteroidetes (2.1%) constituting two potentially electrogenic genera: Geobacter (6.8%) and Aeromonas (31.9%). The current production was found to be limited by kinetics during the growth period (33days), and mass transfer, thereafter. The results indicate the necessity of removing spent biomass for efficient long-term operation and treatment of wastewater streams. C1 [Ichihashi, Osamu; Borole, Abhijeet P.] Oak Ridge Natl Lab, Biosci Div, Oak Ridge, TN 37831 USA. [Vishnivetskaya, Tatiana A.; Borole, Abhijeet P.] Univ Tennessee, Ctr Interdisciplinary Res & Educ, Energy Sci & Engn Program, Dept Chem & Biomol Engn, Knoxville, TN 37996 USA. [Ichihashi, Osamu] Tohoku Univ Oosaki Miyagi, Grad Sch Agr Sci, Sendai, Miyagi 9896711, Japan. RP Ichihashi, O (reprint author), Gifu Univ, River Basin Res Ctr, Gifu 5011193, Japan. EM borolea@ornl.gov OI Vishnivetskaya, Tatiana/0000-0002-0660-023X; Borole, Abhijeet/0000-0001-8423-811X FU overseas study program of "International training for construction of sustainable agriculture" - "Institutional Program for Young Researcher Overseas Visits" of the Japan Society for the Promotion of Science; U.S. Department of Energy [DE-AC05-00OR22725]; U.S. Government [DE-AC05-00OR22725] FX Financial support for O.I. was obtained from an overseas study program of "International training for construction of sustainable agriculture," funded by the "Institutional Program for Young Researcher Overseas Visits" of the Japan Society for the Promotion of Science. ORNL is managed by UT-Battelle, Inc. via a contract #DE-AC05-00OR22725 for the U.S. Department of Energy. The authors would like to thank Tse-Luan Lu for help with genomic DNA isolation. The submitted manuscript has been authored by a contractor of the U.S. Government under contract No. DE-AC05-00OR22725. Accordingly, the U.S. Government retains a nonexclusive, royalty-free license to publish or reproduce the published form of this contribution, or allow others to do so, for U.S. Government purposes. NR 34 TC 2 Z9 2 U1 1 U2 18 PU WILEY-V C H VERLAG GMBH PI WEINHEIM PA POSTFACH 101161, 69451 WEINHEIM, GERMANY SN 2196-0216 J9 CHEMELECTROCHEM JI ChemElectroChem PD NOV 11 PY 2014 VL 1 IS 11 SI SI BP 1940 EP 1947 DI 10.1002/celc.201402206 PG 8 WC Electrochemistry SC Electrochemistry GA AT9GW UT WOS:000345237000026 ER PT J AU Babanova, S Matanovic, I Atanassov, P AF Babanova, Sofia Matanovic, Ivana Atanassov, Plamen TI Quinone-Modified Surfaces for Enhanced Enzyme-Electrode Interactions in Pyrroloquinoline-Quinone-Dependent Glucose Dehydrogenase Anodes SO CHEMELECTROCHEM LA English DT Article DE bioanodes; electron transfer; glucose dehydrogenase; glucose oxidation; surface modification ID BRILLOUIN-ZONE INTEGRATIONS; INITIO MOLECULAR-DYNAMICS; MODIFIED CARBON NANOTUBES; TOTAL-ENERGY CALCULATIONS; AUGMENTED-WAVE METHOD; BIOFUEL CELL; DIRECT BIOELECTROCATALYSIS; BILIRUBIN OXIDASE; OXYGEN REDUCTION; BASIS-SET AB An approach for enhancing the enzyme-electrode interface reactions with pyrroloquinoline quinone (PQQ)-dependent glucose dehydrogenase (GDH) is described in this study. Modification of carbonaceous electrodes with ubiquinone or its functional analogues (1,2- and 1,4-benzoquinones) that have the appropriate redox potential to provide a driving force for an electron transfer to occur, along with fast electron-transfer rate through these molecules, creates an electron sink on the electrode surface that can pull electrons from the cofactor, increasing the electron-transfer rate and generating higher current densities. Several important parameters are experimentally evaluated and/or calculated using density functional theory. Among the quinones investigated, 1,4-benzoquinone has the greatest influence on the PQQ-dependent GDH anodes, yielding 5.1-fold higher current densities on single-walled, and 3.3-fold on multi-walled carbon nanotube papers in comparison to unmodified PQQ-dependent GDH anodes. C1 [Babanova, Sofia; Matanovic, Ivana; Atanassov, Plamen] Univ New Mexico, Ctr Emerging Energy Technol, Dept Chem & Nucl Engn, Albuquerque, NM 87131 USA. [Matanovic, Ivana] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA. RP Babanova, S (reprint author), Univ New Mexico, Ctr Emerging Energy Technol, Dept Chem & Nucl Engn, 1 Univ New Mexico, Albuquerque, NM 87131 USA. EM plamen@unm.edu FU NSF-CBET grant [1158936]; LDRD-DR grant [20120003DR]; Office of Science of the U.S. Department of Energy [DE-AC52-06NA25396]; Department of Energy's Office of Biological and Environmental Research FX This work was supported by NSF-CBET grant number 1158936 and LDRD-DR grant number 20120003DR. Computational work was performed using the computational resources of LANL, supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC52-06NA25396 and EMSL, a national scientific user facility sponsored by the Department of Energy's Office of Biological and Environmental Research and located at Pacific Northwest National Laboratory. NR 65 TC 4 Z9 4 U1 2 U2 23 PU WILEY-V C H VERLAG GMBH PI WEINHEIM PA BOSCHSTRASSE 12, D-69469 WEINHEIM, GERMANY SN 2196-0216 J9 CHEMELECTROCHEM JI ChemElectroChem PD NOV 11 PY 2014 VL 1 IS 11 SI SI BP 2017 EP 2028 DI 10.1002/celc.201402104 PG 12 WC Electrochemistry SC Electrochemistry GA AT9GW UT WOS:000345237000035 ER PT J AU Biswas, M Libera, JA Darling, SB Elam, JW AF Biswas, Mahua Libera, Joseph A. Darling, Seth B. Elam, Jeffrey W. TI New Insight into the Mechanism of Sequential Infiltration Synthesis from Infrared Spectroscopy SO CHEMISTRY OF MATERIALS LA English DT Article ID ATOMIC LAYER DEPOSITION; COPOLYMER TEMPLATES; FILMS; TRIMETHYLALUMINUM; NANOSTRUCTURES; POLYMERS; FTIR; PMMA AB Sequential infiltration synthesis (SIS) has been recently demonstrated to increase the etch resistance of optical, e-beam, and block copolymer lithography resists for sub-50 nm pattern transfer. Although SIS can dramatically enhance pattern transfer relevant to device applications, the complex processes involved in SIS are not clearly understood. Fundamental knowledge of the chemistry underlying SIS is necessary to ensure a high degree of perfection in large-scale lithography. To this end, we performed in situ Fourier transform infrared (FTIR) spectroscopic measurements during the SIS of Al2O3 using trimethylaluminum (TMA) and H2O into poly(methyl methacrylate) (PMMA). The FTIR results revealed that TMA reacts quickly with PMMA to form an unstable complex. The subsequent conversion of this intermediate complex into stable AlO linkages is slow and must compete with rapid TMA desorption. We support this interpretation of the FTIR data using density functional theory to calculate plausible structures for the unstable TMAPMMA complex and the covalently linked species. As a consequence of this two-step reaction between TMA and PMMA, the detailed history of the TMA exposure becomes critical to achieving reliable patterns in SIS lithography. We demonstrate this using scanning electron microscopy to image the patterns resulting from SIS treatment of block copolymer films under different TMA exposure conditions. This better understanding of the SIS reaction dynamics should improve reliability in SIS lithography as well as other SIS applications. C1 [Biswas, Mahua; Libera, Joseph A.; Elam, Jeffrey W.] Argonne Natl Lab, Div Energy Syst, Argonne, IL 60439 USA. [Darling, Seth B.] Univ Chicago, Inst Mol Engn, Chicago, IL 60637 USA. RP Darling, SB (reprint author), Univ Chicago, Inst Mol Engn, Chicago, IL 60637 USA. EM darling@anl.gov; jelam@anl.gov FU U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-AC02-06CH11357]; Technology Maturation Grant through the Technology Development and Commercialization Division at Argonne FX Use of the Center for Nanoscale Materials was supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract No. DE-AC02-06CH11357. The authors want to thank Dr. Wei Chen from Materials Science Division, Argonne National Laboratory, for providing PS-r-PMMA polymer. The authors gratefully acknowledge support from a Technology Maturation Grant through the Technology Development and Commercialization Division at Argonne. NR 29 TC 16 Z9 16 U1 6 U2 33 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0897-4756 EI 1520-5002 J9 CHEM MATER JI Chem. Mat. PD NOV 11 PY 2014 VL 26 IS 21 BP 6135 EP 6141 DI 10.1021/cm502427q PG 7 WC Chemistry, Physical; Materials Science, Multidisciplinary SC Chemistry; Materials Science GA AT4JL UT WOS:000344905600008 ER PT J AU Oh, SM Myung, ST Hwang, JY Scrosati, B Amine, K Sun, YK AF Oh, Seung-Min Myung, Seung-Taek Hwang, Jang-Yeon Scrosati, Bruno Amine, Khalil Sun, Yang-Kook TI High Capacity O3-Type Na[Li-0.05(Ni0.25Fe0.25Mn0.5)(0.95)]O-2 Cathode for Sodium Ion Batteries SO CHEMISTRY OF MATERIALS LA English DT Article ID ELECTROCHEMICAL PROPERTIES; ENERGY-STORAGE; DRYING METHOD; INTERCALATION; ELECTRODE; NAXCOO2; OXIDE; LI AB In this work we report Na[Li-0.05(Ni0.25Fe(0.25)Mn(0.5))(0.95)]O2 layered cathode materials that were synthesized via a coprecipitation method. The Na[Li-0.05(Ni(0.25)Fe0.25Mn(0.5))(0.95)]O-2 electrode exhibited an exceptionally high capacity (180.1 mA h g1 at 0.1 C-rate) as well as excellent capacity retentions (0.2 C-rate: 89.6%, 0.5 C-rate: 92.1%) and rate capabilities at various C-rates (0.1 C-rate: 180.1 mA h g1, 1 C-rate: 130.9 mA h g1, 5 C-rate: 96.2 mA h g1), which were achieved due to the Li supporting structural stabilization by introduction into the transition metal layer. By contrast, the electrode performance of the lithium-free Na[Ni0.25Fe0.25Mn0.5]O-2 cathode was inferior because of structural disintegration presumably resulting from Fe3+ migration from the transition metal layer to the Na layer during cycling. The long-term cycling using a full cell consisting of a Na[Li-0.05(Ni0(.25)Fe(0.25)Mn(0.5))(0.95)]O-2 cathode was coupled with a hard carbon anode which exhibited promising cycling data including a 76% capacity retention over 200 cycles. C1 [Oh, Seung-Min; Hwang, Jang-Yeon; Sun, Yang-Kook] Hanyang Univ, Dept Energy Engn, Seoul 133791, South Korea. [Myung, Seung-Taek] Sejong Univ, Dept Nano Engn, Seoul 143747, South Korea. [Scrosati, Bruno] Italian Inst Technol, I-16163 Genoa, Italy. [Amine, Khalil] Argonne Natl Lab, Chem Sci & Engn Div, Argonne, IL 60439 USA. RP Sun, YK (reprint author), Hanyang Univ, Dept Energy Engn, Seoul 133791, South Korea. EM yksun@hanyang.ac.kr FU Global Frontier R&D Program on Center for Hybrid Interface Materials (HIM) - Ministry of Science, ICT & Future Planning [2013M3A6B1078875]; Human Resources Development program of the Korea Institute of Energy Technology Evaluation and Planning (KETEP) - Korea government Ministry of Trade, Industry and Energy [20124010203310] FX This work was supported by the Global Frontier R&D Program (2013M3A6B1078875) on Center for Hybrid Interface Materials (HIM) funded by the Ministry of Science, ICT & Future Planning and supported by the Human Resources Development program (No. 20124010203310) of the Korea Institute of Energy Technology Evaluation and Planning (KETEP) grant funded by the Korea government Ministry of Trade, Industry and Energy. NR 28 TC 29 Z9 30 U1 18 U2 144 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0897-4756 EI 1520-5002 J9 CHEM MATER JI Chem. Mat. PD NOV 11 PY 2014 VL 26 IS 21 BP 6165 EP 6171 DI 10.1021/cm502481b PG 7 WC Chemistry, Physical; Materials Science, Multidisciplinary SC Chemistry; Materials Science GA AT4JL UT WOS:000344905600012 ER PT J AU Chung, YG Camp, J Haranczyk, M Sikora, BJ Bury, W Krungleviciute, V Yildirim, T Farha, OK Sholl, DS Snurr, RQ AF Chung, Yongchul G. Camp, Jeffrey Haranczyk, Maciej Sikora, Benjamin J. Bury, Wojciech Krungleviciute, Vaiva Yildirim, Taner Farha, Omar K. Sholl, David S. Snurr, Randall Q. TI Computation-Ready, Experimental Metal-Organic Frameworks: A Tool To Enable High-Throughput Screening of Nanoporous Crystals SO CHEMISTRY OF MATERIALS LA English DT Article ID HYDROGEN STORAGE; POROUS MATERIALS; SURFACE-AREAS; ADSORPTION; SEPARATION; ZEOLITES; GEOMETRY; SERIES; LIMITS; MOFS AB Experimentally refined crystal structures for metalorganic frameworks (MOFs) often include solvent molecules and partially occupied or disordered atoms. This creates a major impediment to applying high-throughput computational screening to MOFs. To address this problem, we have constructed a database of MOF structures that are derived from experimental data but are immediately suitable for molecular simulations. The computation-ready, experimental (CoRE) MOF database contains over 4700 porous structures with publically available atomic coordinates. Important physical and chemical properties including the surface area and pore dimensions are reported for these structures. To demonstrate the utility of the database, we performed grand canonical Monte Carlo simulations of methane adsorption on all structures in the CoRE MOF database. We investigated the structural properties of the CoRE MOFs that govern methane storage capacity and found that these relationships agree well with those derived recently from a large database of hypothetical MOFs. C1 [Chung, Yongchul G.; Sikora, Benjamin J.; Snurr, Randall Q.] Northwestern Univ, Dept Chem & Biol Engn, Evanston, IL 60208 USA. [Bury, Wojciech; Farha, Omar K.] Northwestern Univ, Dept Chem, Evanston, IL 60208 USA. [Camp, Jeffrey; Sholl, David S.] Georgia Inst Technol, Sch Chem & Biomol Engn, Atlanta, GA 30332 USA. [Haranczyk, Maciej] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Comp Res Div, Berkeley, CA 94720 USA. [Bury, Wojciech] Warsaw Univ Technol, Dept Chem, PL-00664 Warsaw, Poland. [Krungleviciute, Vaiva; Yildirim, Taner] NIST, NIST Ctr Neutron Res, Gaithersburg, MD 20899 USA. [Krungleviciute, Vaiva; Yildirim, Taner] Univ Penn, Dept Mat Sci & Engn, Philadelphia, PA 19104 USA. [Farha, Omar K.] King Abdulaziz Univ, Fac Sci, Dept Chem, Jeddah 21589, Saudi Arabia. RP Sholl, DS (reprint author), Georgia Inst Technol, Sch Chem & Biomol Engn, 311 Ferst Dr, Atlanta, GA 30332 USA. RI Snurr, Randall/B-6699-2009; Chung, Yongchul/G-7017-2015; Haranczyk, Maciej/A-6380-2014; Faculty of, Sciences, KAU/E-7305-2017 OI Chung, Yongchul/0000-0002-7756-0589; Haranczyk, Maciej/0000-0001-7146-9568; FU U.S. Department of Energy, Office of Basic Energy Sciences, Division of Chemical Sciences, Geosciences and Biosciences [DE-FG02-12ER16362]; office of the Provost; Office for Research; Northwestern University Information Technology FX This research was supported by the U.S. Department of Energy, Office of Basic Energy Sciences, Division of Chemical Sciences, Geosciences and Biosciences, under Award DE-FG02-12ER16362. This research was supported in part through the computational resources and staff contributions provided for the Quest high-performance computing facility at Northwestern University, which is jointly supported by the office of the Provost, the Office for Research, and Northwestern University Information Technology. We thank Dr. Diego A. Gomez-Gualdron and Dr. Christopher E. Wilmer for providing methane GCMC data for the hypothetical MOFs. NR 36 TC 53 Z9 54 U1 18 U2 100 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0897-4756 EI 1520-5002 J9 CHEM MATER JI Chem. Mat. PD NOV 11 PY 2014 VL 26 IS 21 BP 6185 EP 6192 DI 10.1021/cm502594j PG 8 WC Chemistry, Physical; Materials Science, Multidisciplinary SC Chemistry; Materials Science GA AT4JL UT WOS:000344905600015 ER PT J AU Strobridge, FC Clement, RJ Leskes, M Middlemiss, DS Borkiewicz, OJ Wiaderek, KM Chapman, KW Chupas, PJ Grey, CP AF Strobridge, Fiona C. Clement, Raphaele J. Leskes, Michal Middlemiss, Derek S. Borkiewicz, Olaf J. Wiaderek, Kamila M. Chapman, Karena W. Chupas, Peter J. Grey, Clare P. TI Identifying the Structure of the Intermediate, Li2/3CoPO4, Formed during Electrochemical Cycling of LiCoPO4 SO CHEMISTRY OF MATERIALS LA English DT Article ID X-RAY-DIFFRACTION; DENSITY-FUNCTIONAL THEORY; TRANSITION-METAL PHOSPHATES; INITIO MOLECULAR-DYNAMICS; TOTAL-ENERGY CALCULATIONS; SOLID-SOLUTION PHASES; AUGMENTED-WAVE METHOD; LI-ION BATTERY; LITHIUM BATTERIES; LIFEPO4 NANOPARTICLES AB In situ synchrotron diffraction measurements and subsequent Rietveld refinements are used to show that the high energy density cathode material LiCoPO4 (space group Pnma) undergoes two distinct two-phase reactions upon charge and discharge, both occurring via an intermediate Li-2/3(Co2+)(2/3)(Co3+)(1/3)PO4 phase. Two resonances are observed for Li2/3CoPO4 with intensity ratios of 2:1 and 1:1 in the P-31 and 7Li NMR spectra, respectively. An ordering of Co2+/Co3+ oxidation states is proposed within a (a X 3b X c) supercell, and Li+/vacancy ordering is investigated using experimental NMR data in combination with first-principles solid-state DFT calculations. In the lowest energy configuration, both the Co3+ ions and Li vacancies are found to order along the b-axis. Two other low energy Li+/vacancy ordering schemes are found only 5 meV per formula unit higher in energy. All three configurations lie below the LiCoPO4CoPO4 convex hull and they may be readily interconverted by Li+ hops along the b-direction. C1 [Strobridge, Fiona C.; Clement, Raphaele J.; Leskes, Michal; Middlemiss, Derek S.; Grey, Clare P.] Univ Cambridge, Dept Chem, Cambridge CB2 1EW, Cambs, England. [Borkiewicz, Olaf J.; Wiaderek, Kamila M.; Chapman, Karena W.; Chupas, Peter J.] Argonne Natl Lab, Adv Photon Source, Xray Sci Div, Argonne, IL 60439 USA. [Grey, Clare P.] SUNY Stony Brook, Dept Chem, Stony Brook, NY 11794 USA. RP Grey, CP (reprint author), Univ Cambridge, Dept Chem, Lensfield Rd, Cambridge CB2 1EW, Cambs, England. EM cpg27@cam.ac.uk RI Leskes, Michal/J-4674-2015 OI Leskes, Michal/0000-0002-7172-9689 FU EPSRC for a Doctoral Training Partnership Award; Department of Energy (DOE); U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-SC0001294]; EU; Marie Curie intra-European fellowship; U.S. Department of Energy [DE-AC02-06CH11357]; U.S. DOE, Office of Basic Energy Sciences [DE-AC02-98CH10886] FX We thank the EPSRC for a Doctoral Training Partnership Award (support to FCS) and the Department of Energy (DOE) for support via the Northeastern Center for Chemical Energy Storage, an Energy Frontier Research Center funded by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences under Award Number DE-SC0001294 (FCS, CPG, OJB, KMW, KWC, PJC). We thank the EU for financial support via an EU-ERC Advanced Fellowship (RJC) and a Marie Curie intra-European fellowship (ML). Work done at Argonne and use of the Advanced Photon Source (APS), an Office of Science User Facility operated for the U.S. Department of Energy Office of Science by Argonne National Laboratory, were supported by the U.S. Department of Energy under Contract No. DE-AC02-06CH11357. An allocation of time upon the NANO computer cluster at the Center for Functional Nanomaterials, Brookhaven National Laboratory, U.S.A., which is supported by the U.S. DOE, Office of Basic Energy Sciences, under Contract DE-AC02-98CH10886, is acknowledged. This work used the ARCHER UK National Supercomputing Service (http://www.archer.ac.uk). We thank Hao Liu, Xiao Hua, Ieuan Seymour, Dr. Phoebe Allan and Dr. Sylvia Britto for their help and discussions, Dr. Matthew Suchomel for instrument support, and Dr. Jan Ilavsky for help with the Irena software. NR 79 TC 11 Z9 12 U1 10 U2 121 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0897-4756 EI 1520-5002 J9 CHEM MATER JI Chem. Mat. PD NOV 11 PY 2014 VL 26 IS 21 BP 6193 EP 6205 DI 10.1021/cm502680w PG 13 WC Chemistry, Physical; Materials Science, Multidisciplinary SC Chemistry; Materials Science GA AT4JL UT WOS:000344905600016 ER PT J AU Omenya, F Miller, JK Fang, J Wen, BH Zhang, RB Wang, Q Chernova, NA Whittingham, MS AF Omenya, Fredrick Miller, Joel K. Fang, Jin Wen, Bohua Zhang, Ruibo Wang, Qi Chernova, Natasha A. Whittingham, M. Stanley TI Single-Phase Lithiation and Delithiation of Simferite Compounds Li(Mg,Mn,Fe)PO4 SO CHEMISTRY OF MATERIALS LA English DT Article ID ROOM-TEMPERATURE; SOLID-SOLUTION; LIFEPO4; LIXFEPO4; CATHODE; LI-X(MNYFE1-Y)PO4; DEINTERCALATION; SUBSTITUTION; DIFFRACTION; BATTERIES AB Understanding the phase transformation behavior of electrode materials for lithium ion batteries is critical in determining the electrode kinetics and battery performance. Here, we demonstrate the lithiation/delithiation mechanism and electrochemical behavior of the simferite compound, LiMg0.5Fe0.3Mn0.2PO4. In contrast to the equilibrium two-phase nature of LiFePO4, LiMg(0.5)Fe(0.3)Mn(0.)2PO(4) undergoes a one-phase reaction mechanism as confirmed by ex situ X-ray diffraction at different states of delithiation and electrochemical measurements. The equilibrium voltage measurement by galvanostatic intermittent titration technique shows a continuous change in voltage at Mn3+/Mn2+ redox couple with addition of Mg2+ in LiMn0.4Fe0.6PO4 olivine structure. There is, however, no significant change in the Fe3+/Fe2+ redox potential. C1 [Omenya, Fredrick; Miller, Joel K.; Fang, Jin; Wen, Bohua; Zhang, Ruibo; Wang, Qi; Chernova, Natasha A.; Whittingham, M. Stanley] SUNY Binghamton, Binghamton, NY 13902 USA. [Wang, Qi] Brookhaven Natl Lab, Upton, NY 11973 USA. [Whittingham, M. Stanley] SUNY Stony Brook, Dept Chem, Northeastern Ctr Chem Energy Storage, Stony Brook, NY 11794 USA. RP Whittingham, MS (reprint author), SUNY Binghamton, Binghamton, NY 13902 USA. EM stanwhit@gmail.com RI Zhang, Ruibo/B-4659-2015 FU Northeastern Center for Chemical Energy Storage, an Energy Frontier Research Center - U.S. Department of Energy, Office of Science, Basic Energy Sciences [DE-SC0001294]; U.S. Department of Energy, Office of Science, Basic Energy Sciences [DE-AC02-06CH11357, DE-AC02-98CH10886] FX This research is supported as part of the Northeastern Center for Chemical Energy Storage, an Energy Frontier Research Center funded by the U.S. Department of Energy, Office of Science, Basic Energy Sciences, under Award Number DE-SC0001294. Use of the Advanced Photon Source at Argonne National Laboratory and the National Synchrotron Light Source at Brookhaven National Laboratory is supported by the U.S. Department of Energy, Office of Science, Basic Energy Sciences, under Contract Nos. DE-AC02-06CH11357 and DE-AC02-98CH10886, respectively. We also acknowledge the support of the National Institute of Standards and Technology U.S. Department of Commerce, in providing the neutron research facilities used in this work. We thank Dr. Hui Wu of NIST for her help with neutron data collection and analysis. NR 27 TC 3 Z9 3 U1 2 U2 49 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0897-4756 EI 1520-5002 J9 CHEM MATER JI Chem. Mat. PD NOV 11 PY 2014 VL 26 IS 21 BP 6206 EP 6212 DI 10.1021/cm502832b PG 7 WC Chemistry, Physical; Materials Science, Multidisciplinary SC Chemistry; Materials Science GA AT4JL UT WOS:000344905600017 ER PT J AU Mohanty, D Li, JL Abraham, DP Huq, A Payzant, EA Wood, DL Daniel, C AF Mohanty, Debasish Li, Jianlin Abraham, Daniel P. Huq, Ashfia Payzant, E. Andrew Wood, David L., III Daniel, Claus TI Unraveling the Voltage-Fade Mechanism in High-Energy-Density Lithium-Ion Batteries: Origin of the Tetrahedral Cations for Spinel Conversion SO CHEMISTRY OF MATERIALS LA English DT Article ID LAYERED COMPOSITE CATHODE; DIFFRACTION; ELECTRODES; OXIDES; TRANSFORMATION; HYSTERESIS; NEUTRON AB High-voltage layered lithium- and manganese-rich (LMR) oxides have the potential to dramatically enhance the energy density of current Li-ion energy storage systems. However, these materials are currently not used commonly; one reason is their inability to maintain a consistent voltage profile (voltage fade) during electrochemical cycling. This report rationalizes the cause of this voltage fade by providing evidence of layered to spinel (LS) structural evolution pathways in the host Li1.2Mn0.55Ni0.15Co0.1O2 oxide. By employing neutron powder diffraction, we show that LS structural rearrangement in the LMR oxide occurs through a tetrahedral cation intermediate via the following: (i) diffusion of lithium atoms from octahedral to tetrahedral sites of the lithium layer [(LiLioct -> LiLitet] which is followed by the dispersal of the lithium ions from the adjacent octahedral site of the metal layer to the tetrahedral sites of lithium layer [LiTMoct -> LiLitet]; (ii) migration of Mn from the octahedral sites of the transition-metal layer to the permanent octahedral site of lithium layer via tetrahedral site of lithium layer [MnTMoct -> MnLitet -> MnLioct)]. These findings open the door to potential routes to mitigate this atomic restructuring in the high-voltage LMR composite oxide by manipulating their composition/structure for practical use in high-energy-density lithium-ion batteries. C1 [Mohanty, Debasish; Li, Jianlin; Wood, David L., III; Daniel, Claus] Oak Ridge Natl Lab, Energy & Transportat Sci Div, Oak Ridge, TN 37831 USA. [Huq, Ashfia; Payzant, E. Andrew] Oak Ridge Natl Lab, Chem & Engn Mat Div, Oak Ridge, TN 37831 USA. [Abraham, Daniel P.] Argonne Natl Lab, Chem Sci & Engn Div, Argonne, IL 60439 USA. [Wood, David L., III; Daniel, Claus] Univ Tennessee, Bredesen Ctr Interdisciplinary Res & Grad Educ, Knoxville, TN 37996 USA. RP Mohanty, D (reprint author), Oak Ridge Natl Lab, Energy & Transportat Sci Div, Oak Ridge, TN 37831 USA. EM mohantyd@ornl.gov; wooddl@ornl.gov; danielc@ornl.gov RI Payzant, Edward/B-5449-2009; Huq, Ashfia/J-8772-2013; Daniel, Claus/A-2060-2008; Mohanty, Debasish/B-6207-2012; Li, Jianlin/D-3476-2011; OI Payzant, Edward/0000-0002-3447-2060; Huq, Ashfia/0000-0002-8445-9649; Daniel, Claus/0000-0002-0571-6054; Mohanty, Debasish/0000-0003-1141-0657; Li, Jianlin/0000-0002-8710-9847; Wood, David/0000-0002-2471-4214 FU U.S. Department of Energy (DOE) [DE-AC05-000R22725]; Office of Energy Efficiency and Renewable Energy for the Vehicle Technologies Office's Applied Battery Research Program (Program Managers: Peter Faguy and David Howell); Scientific User Facilities Division, Office of Basic Energy Sciences; VTO's ABR Program FX This research at Oak Ridge National Laboratory, managed by UT Battelle, LLC, for the U.S. Department of Energy (DOE), under contract DE-AC05-000R22725, was sponsored by the Office of Energy Efficiency and Renewable Energy for the Vehicle Technologies Office's Applied Battery Research Program (Program Managers: Peter Faguy and David Howell). Part of this research was supported by the ORNL's User Facility at the Spa Ration Neutron Source, which is sponsored by the Scientific User Facilities Division, Office of Basic Energy Sciences. The HES050 material was obtained from Argonne National Laboratory, in collaboration with Andrew Jansen and Bryant Polzin. The electrodes and cell fabrication, and pouch cell testing, were carried out at the DOE's Battery Manufacturing R&D Facility at Oak Ridge National Laboratory, which is supported by VTO's ABR Program. We thank Roberta A. Meisner at ORNL for her help in XRD data collection. NR 31 TC 45 Z9 45 U1 11 U2 93 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0897-4756 EI 1520-5002 J9 CHEM MATER JI Chem. Mat. PD NOV 11 PY 2014 VL 26 IS 21 BP 6272 EP 6280 DI 10.1021/cm5031415 PG 9 WC Chemistry, Physical; Materials Science, Multidisciplinary SC Chemistry; Materials Science GA AT4JL UT WOS:000344905600026 ER PT J AU Zhou, Y Dyck, J Graham, TW Luo, HM Leonard, DN Qu, J AF Zhou, Yan Dyck, Jeffrey Graham, Todd W. Luo, Huimin Leonard, Donovan N. Qu, Jun TI Ionic Liquids Composed of Phosphonium Cations and Organophosphate, Carboxylate, and Sulfonate Anions as Lubricant Antiwear Additives SO LANGMUIR LA English DT Article ID SOLUBILITY PARAMETERS; TRIBOLOGICAL PERFORMANCE; NEAT LUBRICANTS; FATTY-ACIDS; OFHC COPPER; PART 2; OIL; DECOMPOSITION; HYDROCARBON; MECHANISMS AB Oil-soluble phosphonium-based ionic liquids (ILs) have recently been reported as potential ashless lubricant additives. This study is to expand the IL chemistry envelope and to achieve fundamental correlations between the ion structures and ILs physiochemical and tribological properties. Here we present eight ILs containing two different phosphonium cations and seven different anions from three groups: organophosphate, carboxylate, and sulfonate. The oil solubility of ILs seems largely governed by the IL molecule size and structure complexity. When used as oil additives, the ranking of effectiveness in wear protection for the anions are organophosphate > carboxylate > sulfonate. All selected ILs outperformed a commercial ashless antiwear additive. Surface characterization from the top and the cross-section revealed the nanostructures and compositions of the tribo-films formed by the ILs. Some fundamental insights were achieved: branched and long alkyls improve the ILs oil solubility, anions of a phosphonium-phosphate IL contribute most phosphorus in the tribo-film, and carboxylate anions, though free of P, S, N, or halogen, can promote the formation of an antiwear tribo-film. C1 [Zhou, Yan; Leonard, Donovan N.; Qu, Jun] Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37830 USA. [Zhou, Yan] Texas A&M Univ, College Stn, TX 77843 USA. [Dyck, Jeffrey; Graham, Todd W.] Cytec Canada, Applicat Technol Grp, Niagara Falls, ON L2H 6S5, Canada. [Luo, Huimin] Oak Ridge Natl Lab, Energy & Transportat Sci Div, Oak Ridge, TN 37831 USA. RP Qu, J (reprint author), Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37830 USA. EM qujn@ornl.gov OI Qu, Jun/0000-0001-9466-3179 FU Vehicle Technologies Program, Office of Energy Efficiency and Renewable Energy, U.S. Department of Energy (DOE); U.S. Department of Energy [DE-AC05-00OR22725] FX The authors thank Dr. H. M. Meyer of Oak Ridge National Laboratory (ORNL) for his advice on XPS analysis and W. C. Barnhill of ORNL for exposure corrosion testing. Research sponsored by the Vehicle Technologies Program, Office of Energy Efficiency and Renewable Energy, U.S. Department of Energy (DOE). Y.Z. was appointed to ORNL through the Oak Ridge Associated Universities/Oak Ridge Institute for Science and Engineering's Advanced Short-Term Research Opportunity program. The authors also thank the Laboratory for Molecular Simulation at Texas A&M University for providing the access to Materials Studio. This manuscript has been authored by UT-Battelle, LLC, under Contract No. DE-AC05-00OR22725 with the U.S. Department of Energy. The United States Government retains and the publisher, by accepting the article for publication, acknowledges that the U.S. Government retains a nonexclusive, paid-up, irrevocable, worldwide license to publish or reproduce the published form of this manuscript, or allow others to do so, for U.S. Government purposes. NR 53 TC 20 Z9 20 U1 5 U2 43 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0743-7463 J9 LANGMUIR JI Langmuir PD NOV 11 PY 2014 VL 30 IS 44 BP 13301 EP 13311 DI 10.1021/la5032366 PG 11 WC Chemistry, Multidisciplinary; Chemistry, Physical; Materials Science, Multidisciplinary SC Chemistry; Materials Science GA AT4JG UT WOS:000344905100021 PM 25330413 ER PT J AU Oliver, RC Lipfert, J Fox, DA Lo, RH Kim, JJ Doniach, S Columbus, L AF Oliver, Ryan C. Lipfert, Jan Fox, Daniel A. Lo, Ryan H. Kim, Justin J. Doniach, Sebastian Columbus, Linda TI Tuning Micelle Dimensions and Properties with Binary Surfactant Mixtures SO LANGMUIR LA English DT Article ID SMALL-ANGLE SCATTERING; ADVANCED PHOTON SOURCE; X-RAY-SCATTERING; MEMBRANE-PROTEINS; DETERGENTS; MODEL; MICELLIZATION; REMEDIATION; SYSTEMS; DRUGS AB Detergent micelles are used in many areas of research and technology, in particular, as mimics of the cellular membranes in the purification and biochemical and structural characterization of membrane proteins. Applications of detergent micelles are often hindered by the limited set of properties of commercially available detergents. Mixtures of micelle-forming detergents provide a means to systematically obtain additional micellar properties and expand the repertoire of micelle features available; however, our understanding of the properties of detergent mixtures is still limited. In this study, the shape and size of binary mixtures of seven different detergents commonly used in molecular host-guest systems and membrane protein research were investigated. The data suggests that the detergents form ideally mixed micelles with sizes and shapes different from those of pure individual micelles. For most measurements of size, the mixtures varied linearly with detergent mole fraction and therefore can be calculated from the values of the pure detergents. We propose that properties such as the geometry, size, and surface charge can be systematically and predictably tuned for specific applications. C1 [Oliver, Ryan C.; Fox, Daniel A.; Lo, Ryan H.; Kim, Justin J.; Columbus, Linda] Univ Virginia, Dept Chem, Charlottesville, VA 22904 USA. [Lipfert, Jan] Univ Munich, Dept Phys, Munich, Germany. [Lipfert, Jan] Univ Munich, Ctr Nanosci CeNS, Munich, Germany. [Doniach, Sebastian] Stanford Univ, Dept Phys, Biophys Program, Stanford, CA 94305 USA. [Doniach, Sebastian] Stanford Univ, Dept Appl Phys, Biophys Program, Stanford, CA 94305 USA. [Doniach, Sebastian] Stanford Univ, Stanford Synchrotron Radiat Lab, Stanford, CA 94305 USA. RP Columbus, L (reprint author), Univ Virginia, Dept Chem, Charlottesville, VA 22904 USA. EM columbus@virginia.edu OI Columbus, Linda/0000-0002-2574-0561 FU National Science Foundation [MCB 0845668]; Netherlands Organisation for Scientific Research (NWO) FX This research was funded by a National Science Foundation CAREER award (MCB 0845668) and is supported by The Netherlands Organisation for Scientific Research (NWO). NR 31 TC 5 Z9 5 U1 2 U2 21 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0743-7463 J9 LANGMUIR JI Langmuir PD NOV 11 PY 2014 VL 30 IS 44 BP 13353 EP 13361 DI 10.1021/la503458n PG 9 WC Chemistry, Multidisciplinary; Chemistry, Physical; Materials Science, Multidisciplinary SC Chemistry; Materials Science GA AT4JG UT WOS:000344905100027 PM 25312254 ER PT J AU Wang, WW Wang, WY Lu, XY Bobade, S Chen, JH Kang, NG Zhang, QY Mays, J AF Wang, Wenwen Wang, Weiyu Lu, Xinyi Bobade, Sachin Chen, Jihua Kang, Nam-Goo Zhang, Qiuyu Mays, Jimmy TI Synthesis and Characterization of Comb and Centipede Multigraft Copolymers PnBA-g-PS with High Molecular Weight Using Miniemulsion Polymerization SO MACROMOLECULES LA English DT Article ID FREE-RADICAL POLYMERIZATION; THERMOPLASTIC ELASTOMERS; ANIONIC-POLYMERIZATION; GRAFT-COPOLYMERS; EMULSION POLYMERIZATION; BLOCK-COPOLYMERS; MECHANICAL-PROPERTIES; TENSILE PROPERTIES; CLICK CHEMISTRY; LATEX-PARTICLES AB Comb and centipede multigraft copolymers, poly(n-butyl acrylate)-g-polystyrene (PnBA-g-PS) with PnBA backbones and PS side chains, were synthesized via high-vacuum anionic polymerization and miniemulsion polymerization. Single-tailed and double-tailed PS macromonomers were synthesized by anionic polymerization and Steglich esterification. Subsequently, the copolymerization of each macromonomer and nBA was carried out in miniemulsion, and multigraft copolymers were obtained. The latex particles of multigraft copolymers were characterized using dynamic light scattering. The molecular weights of macromonomers and multigraft copolymers were analyzed by size exclusion chromatography. Moreover, the molecular weights and structures of macromonomers were investigated by matrix-assisted laser desorption/ionization time-of-flight mass spectrometry and H-1 nuclear magnetic resonance spectroscopy. The weight contents of PS in comb and centipede multigraft copolymers were calculated by H-1 nuclear magnetic resonance spectroscopy. The thermal properties of multigraft copolymers were characterized by thermogravimetric analysis and differential scanning calorimetry. The microphase separation of multigraft copolymers was observed by atomic force microscopy and transmission electronic microscopy. Rheological measurements showed that comb and centipede multigraft copolymers have elastic properties when the weight content of PS side chains is 2632 wt %. Centipede multigraft copolymers possess better elastic properties than comb multigraft copolymers with the similar weight content of PS. These findings are similar to previous results on poly(isoprene-g-polystyrene) comb and centipede copolymers made by anionic polymerization. C1 [Wang, Wenwen; Zhang, Qiuyu] Northwestern Polytech Univ, Sch Sci, Minist Educ, Key Lab Appl Phys & Chem Space, Xian 710072, Peoples R China. [Wang, Weiyu; Lu, Xinyi; Bobade, Sachin; Kang, Nam-Goo; Mays, Jimmy] Univ Tennessee, Dept Chem, Knoxville, TN 37996 USA. [Chen, Jihua] Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA. RP Zhang, QY (reprint author), Northwestern Polytech Univ, Sch Sci, Minist Educ, Key Lab Appl Phys & Chem Space, Xian 710072, Peoples R China. EM qyzhang1803@gmail.com; jimmy@utk.edu RI Chen, Jihua/F-1417-2011; Wang, Weiyu/A-6317-2016 OI Chen, Jihua/0000-0001-6879-5936; Wang, Weiyu/0000-0002-2914-1638 NR 45 TC 9 Z9 9 U1 4 U2 48 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0024-9297 EI 1520-5835 J9 MACROMOLECULES JI Macromolecules PD NOV 11 PY 2014 VL 47 IS 21 BP 7284 EP 7295 DI 10.1021/ma501866t PG 12 WC Polymer Science SC Polymer Science GA AT4JN UT WOS:000344905800003 ER PT J AU Cotanda, P Sudre, G Modestino, MA Chen, XC Balsara, NP AF Cotanda, Pepa Sudre, Guillaume Modestino, Miguel A. Chen, X. Chelsea Balsara, Nitash P. TI High Anion Conductivity and Low Water Uptake of Phosphonium Containing Diblock Copolymer Membranes SO MACROMOLECULES LA English DT Article ID POLYMER-ELECTROLYTE MEMBRANES; LIQUID BLOCK-COPOLYMERS; ALKALINE FUEL-CELLS; IONIC-LIQUID; EXCHANGE MEMBRANES; RADICAL POLYMERIZATION; MOLECULAR-WEIGHT; RAFT PROCESS; MORPHOLOGY; TRANSPORT AB Poly[(styrene)-block-((2-acryloxy)ethyltributylphosphonium bromide)] diblock copolymers (STBP) were synthesized in two steps. First, reversible additionfragmentation chain transfer polymerization was used to synthesize the diblock copolymer precursors poly[(styrene)-block-(bromoethyl acrylate)] (SBEA), followed by functionalization with tributylphosphine. Copolymers with overall molecular weights ranging from 31 to 87 kg/mol were synthesized. The volume fraction of the ion-containing monomers in the copolymers was fixed at about 0.57. Self-assembly of these copolymers into ordered morphologies with tunable domain sizes was demonstrated by small-angle X-ray scattering. The effect of morphology on water uptake and bromide ion conductivity was explored in samples equilibrated in liquid water. The use of the pendant tributylphosphonium cations, which have some hydrophobic character, results in low water uptake and high anionic conductivity. The conductivity increases with increasing domain size while water uptake is unaffected by domain size. C1 [Cotanda, Pepa; Sudre, Guillaume; Modestino, Miguel A.; Balsara, Nitash P.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Joint Ctr Artificial Photosynth, Berkeley, CA 94720 USA. [Cotanda, Pepa; Sudre, Guillaume; Modestino, Miguel A.; Chen, X. Chelsea; Balsara, Nitash P.] Univ Calif Berkeley, Dept Chem & Biomol Engn, Berkeley, CA 94720 USA. [Chen, X. Chelsea; Balsara, Nitash P.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA. [Balsara, Nitash P.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Environm Energy Technol Div, Berkeley, CA 94720 USA. RP Balsara, NP (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Joint Ctr Artificial Photosynth, Berkeley, CA 94720 USA. EM nbalsara@berkeley.edu RI Sudre, Guillaume/A-3061-2013 OI Sudre, Guillaume/0000-0003-3545-7046 FU Office of Science of the U.S. Department of Energy [DE-SC0004993]; Office of Science, Office of Basic Energy Sciences, of the U.S. Department of Energy [DE-AC02-05CH11231] FX This material is based upon work performed by the Joint Center for Artificial Photosynthesis, a DOE Energy Innovation Hub, supported through the Office of Science of the U.S. Department of Energy under Award DE-SC0004993. SAXS experiments were performed at Lawrence Berkeley National Laboratory's Advance Light Source, Beamline 7.3.3. Beamline 7.3.3 of the Advanced Light Source is supported by the Director of the Office of Science, Office of Basic Energy Sciences, of the U.S. Department of Energy under Contract DE-AC02-05CH11231. NR 58 TC 22 Z9 23 U1 16 U2 106 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0024-9297 EI 1520-5835 J9 MACROMOLECULES JI Macromolecules PD NOV 11 PY 2014 VL 47 IS 21 BP 7540 EP 7547 DI 10.1021/ma501744w PG 8 WC Polymer Science SC Polymer Science GA AT4JN UT WOS:000344905800031 ER PT J AU Iyer-Biswas, S Wright, CS Henry, JT Lo, K Burov, S Lin, YH Crooks, GE Crosson, S Dinner, AR Scherer, NF AF Iyer-Biswas, Srividya Wright, Charles S. Henry, Jonathan T. Lo, Klevin Burov, Stanislav Lin, Yihan Crooks, Gavin E. Crosson, Sean Dinner, Aaron R. Scherer, Norbert F. TI Scaling laws governing stochastic growth and division of single bacterial cells SO PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA LA English DT Article DE single-cell dynamics; cell-to-cell variability; exponential growth; Hinshelwood cycle; Arrhenius law ID ESCHERICHIA-COLI; GENE-EXPRESSION; CYCLE; TEMPERATURE; SIZE; SYNCHRONIZATION; VARIABILITY; KINETICS; CULTURES; NOISE AB Uncovering the quantitative laws that govern the growth and division of single cells remains a major challenge. Using a unique combination of technologies that yields unprecedented statistical precision, we find that the sizes of individual Caulobacter crescentus cells increase exponentially in time. We also establish that they divide upon reaching a critical multiple (approximate to 1.8) of their initial sizes, rather than an absolute size. We show that when the temperature is varied, the growth and division timescales scale proportionally with each other over the physiological temperature range. Strikingly, the cell-size and division-time distributions can both be rescaled by their mean values such that the condition-specific distributions collapse to universal curves. We account for these observations with a minimal stochastic model that is based on an autocatalytic cycle. It predicts the scalings, as well as specific functional forms for the universal curves. Our experimental and theoretical analysis reveals a simple physical principle governing these complex biological processes: a single temperature-dependent scale of cellular time governs the stochastic dynamics of growth and division in balanced growth conditions. C1 [Iyer-Biswas, Srividya; Wright, Charles S.; Lo, Klevin; Burov, Stanislav; Dinner, Aaron R.; Scherer, Norbert F.] Univ Chicago, James Franck Inst, Chicago, IL 60637 USA. [Iyer-Biswas, Srividya; Wright, Charles S.; Lo, Klevin; Burov, Stanislav; Dinner, Aaron R.; Scherer, Norbert F.] Univ Chicago, Inst Biophys Dynam, Chicago, IL 60637 USA. [Henry, Jonathan T.; Crosson, Sean] Univ Chicago, Dept Biochem & Mol Biol, Chicago, IL 60637 USA. [Dinner, Aaron R.; Scherer, Norbert F.] Univ Chicago, Dept Chem, Chicago, IL 60637 USA. [Lin, Yihan] CALTECH, Dept Biol, Pasadena, CA 91125 USA. [Crooks, Gavin E.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Phys Biosci Div, Berkeley, CA 94720 USA. RP Dinner, AR (reprint author), Univ Chicago, James Franck Inst, 5640 S Ellis Ave, Chicago, IL 60637 USA. EM dinner@uchicago.edu; nfschere@uchicago.edu OI Wright, Charles/0000-0003-4268-3965 FU National Science Foundation (NSF) [NSF PHY-1305542, NSF DMR-MRSEC 0820054]; W. M. Keck Foundation; University of Chicago Materials Research Science and Engineering Center FX We thank Aretha Fiebig, Ariel Amir, Rutger Hermsen, Gurol Suel, Kingshuk Ghosh, Matt Scott, Terry Hwa, William Loomis, and Leo Kadanoff for insightful discussions. We thank the National Science Foundation (NSF) (NSF PHY-1305542) and the W. M. Keck Foundation for financial support. We also acknowledge partial financial and central facilities assistance of the University of Chicago Materials Research Science and Engineering Center, supported by the NSF (NSF DMR-MRSEC 0820054). NR 53 TC 32 Z9 32 U1 3 U2 33 PU NATL ACAD SCIENCES PI WASHINGTON PA 2101 CONSTITUTION AVE NW, WASHINGTON, DC 20418 USA SN 0027-8424 J9 P NATL ACAD SCI USA JI Proc. Natl. Acad. Sci. U. S. A. PD NOV 11 PY 2014 VL 111 IS 45 BP 15912 EP 15917 DI 10.1073/pnas.1403232111 PG 6 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AS8WW UT WOS:000344526800029 PM 25349411 ER PT J AU Bogorad, IW Chen, CT Theisen, MK Wu, TY Schlenz, AR Lam, AT Liao, JC AF Bogorad, Igor W. Chen, Chang-Ting Theisen, Matthew K. Wu, Tung-Yun Schlenz, Alicia R. Lam, Albert T. Liao, James C. TI Building carbon-carbon bonds using a biocatalytic methanol condensation cycle SO PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA LA English DT Article DE methanol metabolism; metabolic engineering; cell-free synthesis; bio-ethanol; bio-butanol ID PYRUVATE FORMATE-LYASE; ESCHERICHIA-COLI; BACILLUS-METHANOLICUS; LIQUID FUELS; DEHYDROGENASE; FRUCTOSE-6-PHOSPHATE; CHROMATOGRAPHY; HYDROCARBONS; PERFORMANCE; METABOLISM AB Methanol is an important intermediate in the utilization of natural gas for synthesizing other feedstock chemicals. Typically, chemical approaches for building C-C bonds from methanol require high temperature and pressure. Biological conversion of methanol to longer carbon chain compounds is feasible; however, the natural biological pathways for methanol utilization involve carbon dioxide loss or ATP expenditure. Here we demonstrated a biocatalytic pathway, termed the methanol condensation cycle (MCC), by combining the nonoxidative glycolysis with the ribulose monophosphate pathway to convert methanol to higher-chain alcohols or other acetyl-CoA derivatives using enzymatic reactions in a carbon-conserved and ATP-independent system. We investigated the robustness of MCC and identified operational regions. We confirmed that the pathway forms a catalytic cycle through C-13-carbon labeling. With a cell-free system, we demonstrated the conversion of methanol to ethanol or n-butanol. The high carbon efficiency and low operating temperature are attractive for transforming natural gas-derived methanol to longer-chain liquid fuels and other chemical derivatives. C1 [Bogorad, Igor W.; Chen, Chang-Ting; Theisen, Matthew K.; Wu, Tung-Yun; Schlenz, Alicia R.; Lam, Albert T.; Liao, James C.] Univ Calif Los Angeles, Dept Chem & Biomol Engn, Los Angeles, CA 90095 USA. [Bogorad, Igor W.; Theisen, Matthew K.; Liao, James C.] Univ Calif Los Angeles, Dept Bioengn, Los Angeles, CA 90095 USA. [Liao, James C.] Univ Calif Los Angeles, DOE Inst Genom & Prote, Los Angeles, CA 90095 USA. RP Liao, JC (reprint author), Univ Calif Los Angeles, Dept Chem & Biomol Engn, Los Angeles, CA 90095 USA. EM liaoj@ucla.edu FU Reducing Emissions using Methanotrophic Organisms for Transportation Energy (REMOTE) program of the Advanced Research Projects Agency-Energy [DE-AR0000430]; National Science Foundation [0963183] FX This work is supported by the Reducing Emissions using Methanotrophic Organisms for Transportation Energy (REMOTE) program of the Advanced Research Projects Agency-Energy (Award DE-AR0000430). This material is based on research performed in a renovated collaboratory by National Science Foundation Grant 0963183, which is an award funded under the American Recovery and Reinvestment Act of 2009. NR 35 TC 18 Z9 18 U1 3 U2 42 PU NATL ACAD SCIENCES PI WASHINGTON PA 2101 CONSTITUTION AVE NW, WASHINGTON, DC 20418 USA SN 0027-8424 J9 P NATL ACAD SCI USA JI Proc. Natl. Acad. Sci. U. S. A. PD NOV 11 PY 2014 VL 111 IS 45 BP 15928 EP 15933 DI 10.1073/pnas.1413470111 PG 6 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AS8WW UT WOS:000344526800032 PM 25355907 ER PT J AU Heber, EM Hawthorne, MF Kueffer, PJ Garabalino, MA Thorp, SI Pozzi, ECC Hughes, AM Maitz, CA Jalisatgi, SS Nigg, DW Curotto, P Trivillin, VA Schwint, AE AF Heber, Elisa M. Hawthorne, M. Frederick Kueffer, Peter J. Garabalino, Marcela A. Thorp, Silvia I. Pozzi, Emiliano C. C. Hughes, Andrea Monti Maitz, Charles A. Jalisatgi, Satish S. Nigg, David W. Curotto, Paula Trivillin, Veronica A. Schwint, Amanda E. TI Therapeutic efficacy of boron neutron capture therapy mediated by boron-rich liposomes for oral cancer in the hamster cheek pouch model SO PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA LA English DT Article DE oncology; cancer; boronated liposomes; BNCT; neutron radiation ID MURINE TUMORS; UNILAMELLAR LIPOSOMES; SELECTIVE DELIVERY; RECURRENT HEAD; NECK-CANCER; BNCT; FACILITY; BORONOPHENYLALANINE; CARCINOGENESIS; NORMALIZATION AB The application of boron neutron capture therapy (BNCT) mediated by liposomes containing B-10-enriched polyhedral borane and carborane derivatives for the treatment of head and neck cancer in the hamster cheek pouch oral cancer model is presented. These liposomes are composed of an equimolar ratio of cholesterol and 1,2-distearoyl-sn-glycero-3-phosphocholine, incorporating K[nido-7-CH3(CH2)(15)-7,8-C2B9H11] (MAC) in the bilayer membrane while encapsulating the hydrophilic species Na-3[ae-B20H17NH3] (TAC) in the aqueous core. Unilamellar liposomes with a mean diameter of 83 nm were administered i.v. in hamsters. After 48 h, the boron concentration in tumors was 67 +/- 16 ppm whereas the precancerous tissue contained 11 +/- 6 ppm, and the tumor/normal pouch tissue boron concentration ratio was 10:1. Neutron irradiation giving a 5-Gy dose to precancerous tissue (corresponding to 21 Gy in tumor) resulted in an overall tumor response (OR) of 70% after a 4-wk posttreatment period. In contrast, the beam-only protocol gave an OR rate of only 28%. Once-repeated BNCT treatment with readministration of liposomes at an interval of 4, 6, or 8 wk resulted in OR rates of 70-88%, of which the complete response ranged from 37% to 52%. Because of the good therapeutic outcome, it was possible to extend the follow-up of BNCT treatment groups to 16 wk after the first treatment. No radiotoxicity to normal tissue was observed. A salient advantage of these liposomes was that only mild mucositis was observed in dose-limiting precancerous tissue with a sustained tumor response of 70-88%. C1 [Heber, Elisa M.; Garabalino, Marcela A.; Thorp, Silvia I.; Pozzi, Emiliano C. C.; Hughes, Andrea Monti; Curotto, Paula; Trivillin, Veronica A.; Schwint, Amanda E.] Comis Nacl Energia Atom, San Martin B1650KNA, Buenos Aires, DF, Argentina. [Hawthorne, M. Frederick; Kueffer, Peter J.; Maitz, Charles A.; Jalisatgi, Satish S.] Univ Missouri, Int Inst Nano & Mol Med, Columbia, MO 65211 USA. [Nigg, David W.] Idaho Natl Lab, Idaho Falls, ID 83415 USA. [Trivillin, Veronica A.; Schwint, Amanda E.] Consejo Nacl Invest Cient & Tecn, RA-1033 Buenos Aires, DF, Argentina. RP Hawthorne, MF (reprint author), Univ Missouri, Int Inst Nano & Mol Med, Columbia, MO 65211 USA. EM hawthornem@missouri.edu; schwint@cnea.gov.ar FU University of Missouri through the International Institute for Nano and Molecular Medicine; US Department of Energy through Idaho National Laboratory; Agencia Nacional de Promocion Cientifica y Tecnologica; Consejo Nacional de Investigaciones Cientificas y Tecnicas of Argentina FX The authors acknowledge the expert staff of Reactor Argentino 3 nuclear reactor. This study was supported in part by the University of Missouri through the International Institute for Nano and Molecular Medicine, by the US Department of Energy through Idaho National Laboratory, and by grants from Agencia Nacional de Promocion Cientifica y Tecnologica and Consejo Nacional de Investigaciones Cientificas y Tecnicas of Argentina. NR 51 TC 9 Z9 9 U1 3 U2 27 PU NATL ACAD SCIENCES PI WASHINGTON PA 2101 CONSTITUTION AVE NW, WASHINGTON, DC 20418 USA SN 0027-8424 J9 P NATL ACAD SCI USA JI Proc. Natl. Acad. Sci. U. S. A. PD NOV 11 PY 2014 VL 111 IS 45 BP 16077 EP 16081 DI 10.1073/pnas.1410865111 PG 5 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AS8WW UT WOS:000344526800057 PM 25349432 ER PT J AU Lorbeer, C Mudring, AV AF Lorbeer, C. Mudring, A. -V. TI Quantum cutting in nanoparticles producing two green photons SO CHEMICAL COMMUNICATIONS LA English DT Article ID DOWNCONVERSION; LIGDF4-EU3+ AB A synthetic route to nanoscale NaGdF4:Ln is presented which allows for quantum cutting based on the Gd-Er-Tb system. This shows, that cross-relaxation and other energy transfer processes necessary for multiphoton emission can be achieved in nanoparticles even if the large surface and the potentially huge amount of killer traps would suggest a lack of subsequent emission. C1 [Lorbeer, C.; Mudring, A. -V.] Ruhr Univ Bochum, D-44801 Bochum, Germany. [Mudring, A. -V.] Iowa State Univ, Dept Mat Sci & Engn, Ames, IA 50010 USA. [Mudring, A. -V.] Ames Lab DOE, Crit Mat Inst, Ames, IA 50010 USA. RP Mudring, AV (reprint author), Ruhr Univ Bochum, Univ Str 150, D-44801 Bochum, Germany. EM mudring@iastate.edu FU Critical Materials Institute, an Energy Innovation Hub - U.S. Department of Energy, Office of Energy Efficiency and Renewable Energy, Advanced Manufacturing Office; European Research Council with an ERC starting grant ("EMIL") [200475]; Fonds der Chemischen Industrie for a Dozentenstipendium; Fonds der Chemischen Industrie FX This work was supported in part by the Critical Materials Institute, an Energy Innovation Hub funded by the U.S. Department of Energy, Office of Energy Efficiency and Renewable Energy, Advanced Manufacturing Office and the European Research Council with an ERC starting grant ("EMIL", contract no. 200475). A.-V. M. thanks the Fonds der Chemischen Industrie for a Dozentenstipendium, C. L. thanks the Fonds der Chemischen Industrie for a doctoral scholarship. DESY (proposal no. II-20090181) is acknowledged for access to synchrotron facilities. NR 13 TC 5 Z9 5 U1 0 U2 29 PU ROYAL SOC CHEMISTRY PI CAMBRIDGE PA THOMAS GRAHAM HOUSE, SCIENCE PARK, MILTON RD, CAMBRIDGE CB4 0WF, CAMBS, ENGLAND SN 1359-7345 EI 1364-548X J9 CHEM COMMUN JI Chem. Commun. PD NOV 11 PY 2014 VL 50 IS 87 BP 13282 EP 13284 DI 10.1039/c4cc04400b PG 3 WC Chemistry, Multidisciplinary SC Chemistry GA AS0KI UT WOS:000343965700021 PM 25229069 ER PT J AU Maguire, K Sullivan, M Pan, YC Gal-Yam, A Hook, IM Howell, DA Nugent, PE Mazzali, P Chotard, N Clubb, KI Filippenko, AV Kasliwal, MM Kandrashoff, MT Poznanski, D Saunders, CM Silverman, JM Walker, E Xu, D AF Maguire, K. Sullivan, M. Pan, Y. -C. Gal-Yam, A. Hook, I. M. Howell, D. A. Nugent, P. E. Mazzali, P. Chotard, N. Clubb, K. I. Filippenko, A. V. Kasliwal, M. M. Kandrashoff, M. T. Poznanski, D. Saunders, C. M. Silverman, J. M. Walker, E. Xu, D. TI Exploring the spectral diversity of low-redshift Type Ia supernovae using the Palomar Transient Factory SO MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY LA English DT Article DE supernovae: general; galaxies: general; distance scale ID HUBBLE-SPACE-TELESCOPE; HIGH-VELOCITY FEATURES; DELAYED-DETONATION MODELS; TIME OPTICAL-SPECTRA; DIGITAL SKY SURVEY; WHITE-DWARF STAR; LEGACY SURVEY; DARK-ENERGY; SN 2011FE; CIRCUMSTELLAR MATERIAL AB We present an investigation of the optical spectra of 264 low-redshift (z < 0.2) Type Ia supernovae (SNe Ia) discovered by the Palomar Transient Factory, an untargeted transient survey. We focus on velocity and pseudo-equivalent width measurements of the Si II 4130, 5972, and 6355 angstrom lines, as well those of the Ca II near-infrared (NIR) triplet, up to +5 days relative to the SN B-band maximum light. We find that a high-velocity component of the Ca II NIR triplet is needed to explain the spectrum in similar to 95 per cent of SNe Ia observed before-5 days, decreasing to similar to 80 per cent at maximum. The average velocity of the Ca II high-velocity component is similar to 8500 km s(-1) higher than the photospheric component. We confirm previous results that SNe Ia around maximum light with a larger contribution from the high-velocity component relative to the photospheric component in their Ca II NIR feature have, on average, broader light curves and lower Ca II NIR photospheric velocities. We find that these relations are driven by both a stronger high-velocity component and a weaker contribution from the photospheric Ca II NIR component in broader light curve SNe Ia. We identify the presence of C II in very-early-time SN Ia spectra (before - 10 days), finding that >40 per cent of SNe Ia observed at these phases show signs of unburnt material in their spectra, and that C II features are more likely to be found in SNe Ia having narrower light curves. C1 [Maguire, K.] European Southern Observ Astron Res Southern Hemi, D-85748 Garching, Germany. [Sullivan, M.] Univ Southampton, Southampton SO17 1BJ, Hants, England. [Pan, Y. -C.; Hook, I. M.] Univ Oxford, DWB, Dept Phys Astrophys, Oxford OX1 3RH, England. [Gal-Yam, A.] Weizmann Inst Sci, Benoziyo Ctr Astrophys, IL-76100 Rehovot, Israel. [Hook, I. M.] INAF Osservatorio Astron Roma, I-00040 Rome, Italy. [Howell, D. A.] Las Cumbres Observ Global Telescope Network, Goleta, CA 93117 USA. [Howell, D. A.] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA. [Nugent, P. E.; Clubb, K. I.; Filippenko, A. V.; Kandrashoff, M. T.] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA. [Nugent, P. E.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 94720 USA. [Mazzali, P.] Liverpool John Moores Univ, Astrophys Res Inst, IC2, Liverpool L3 5RF, Merseyside, England. [Mazzali, P.] INAF Osservatorio Astron, I-35122 Padua, Italy. [Mazzali, P.] Max Planck Inst Astrophys, D-85748 Garching, Germany. [Chotard, N.] Univ Lyon 1, CNRS, Inst Phys Nucl Lyon, IN2P3, F-69622 Villeurbanne, France. [Kasliwal, M. M.] Carnegie Inst Sci, Pasadena, CA 91101 USA. [Poznanski, D.] Tel Aviv Univ, Sch Phys & Astron, IL-69978 Tel Aviv, Israel. [Saunders, C. M.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Phys, Berkeley, CA 94720 USA. [Saunders, C. M.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA. [Silverman, J. M.] Univ Texas Austin, Dept Astron, Austin, TX 78712 USA. [Walker, E.] Yale Univ, Dept Phys, New Haven, CT 06520 USA. [Xu, D.] Univ Copenhagen, Niels Bohr Inst, Dark Cosmol Ctr, DK-2100 Copenhagen O, Denmark. RP Maguire, K (reprint author), European Southern Observ Astron Res Southern Hemi, Karl Schwarzschild Str 2, D-85748 Garching, Germany. EM kate.maguire@eso.org OI Sullivan, Mark/0000-0001-9053-4820; Hook, Isobel/0000-0002-2960-978X FU European Community; Royal Society; EU/FP7-ERC [307260]; Quantum Universe I-Core program by the Israeli Committee for planning and funding; ISF; GIF; Minerva; Kimmel award; ARCHES award; Lyon Institute of Origins [ANR-10-LABX-66]; Hubble Fellowship; Carnegie-Princeton Fellowship; NSF [AST-1302771, AST-1211916]; Christopher R. Redlich Fund; Richard and Rhoda Goldman Fund; TABASGO Foundation; UK Science and Technology Facilities Council; W.M. Keck Foundation; European Organization for Astronomical Research in the Southern hemisphere, Chile [084.A-0149(A), 085.A-0777(A)]; NASA FX KM is supported by a Marie Curie Intra-European Fellowship, within the 7th European Community Framework Programme (FP7). MS acknowledges support from the Royal Society. AGY is supported by the EU/FP7-ERC grant no [307260], the Quantum Universe I-Core program by the Israeli Committee for planning and funding, the ISF, GIF, Minerva, and ISF grants, and Kimmel and ARCHES awards. NC acknowledges support from the Lyon Institute of Origins under grant ANR-10-LABX-66. MMK acknowledges generous support from the Hubble Fellowship and Carnegie-Princeton Fellowship. JMS is supported by an NSF Astronomy and Astrophysics Postdoctoral Fellowship under award AST-1302771. AVF's supernova group at UC Berkeley has received generous financial assistance from Gary and Cynthia Bengier, the Christopher R. Redlich Fund, the Richard and Rhoda Goldman Fund, the TABASGO Foundation, and NSF grant AST-1211916.; The LT is operated on the island of La Palma by Liverpool John Moores University in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias with financial support from the UK Science and Technology Facilities Council. This work also makes use of observations from the LCOGT network. Some of the data presented herein were obtained at the W.M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration (NASA). The Observatory was made possible by the generous financial support of the W.M. Keck Foundation. We thank the dedicated staffs at all the observatories we used for their excellent assistance with the observations. Based on data taken at the European Organization for Astronomical Research in the Southern hemisphere, Chile, under program IDs 084.A-0149(A) and 085.A-0777(A). Observations obtained with the SuperNova Integral Field Spectrograph on the University of Hawaii 2.2-m telescope as part of the Nearby Supernova Factory II project, a scientific collaboration between the Centre de Recherche Astronomique de Lyon, Institut de Physique Nucleaire de Lyon, Laboratoire de Physique Nucleaire et des Hautes Energies, Lawrence Berkeley National Laboratory, Yale University, University of Bonn, Max Planck Institute for Astrophysics, Tsinghua Center for Astrophysics, and Centre de Physique des Particules de Marseille. This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with NASA. NR 106 TC 24 Z9 24 U1 1 U2 5 PU OXFORD UNIV PRESS PI OXFORD PA GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND SN 0035-8711 EI 1365-2966 J9 MON NOT R ASTRON SOC JI Mon. Not. Roy. Astron. Soc. PD NOV 11 PY 2014 VL 444 IS 4 BP 3258 EP 3274 DI 10.1093/mnras/stu1607 PG 17 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AR2FW UT WOS:000343400100019 ER PT J AU Beutler, F Saito, S Brownstein, JR Chuang, CH Cuesta, AJ Percival, WJ Ross, AJ Ross, NP Schneider, DP Samushia, L Sanchez, AG Seo, HJ Tinker, JL Wagner, C Weaver, BA AF Beutler, Florian Saito, Shun Brownstein, Joel R. Chuang, Chia-Hsun Cuesta, Antonio J. Percival, Will J. Ross, Ashley J. Ross, Nicholas P. Schneider, Donald P. Samushia, Lado Sanchez, Ariel G. Seo, Hee-Jong Tinker, Jeremy L. Wagner, Christian Weaver, Benjamin A. TI The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: signs of neutrino mass in current cosmological data sets SO MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY LA English DT Article DE surveys; cosmological parameters; cosmology: observations; large-scale structure of Universe ID DIGITAL SKY SURVEY; TELESCOPE LENSING SURVEY; BACKGROUND POWER SPECTRUM; TRITIUM BETA-SPECTRUM; SOUTH-POLE TELESCOPE; DATA RELEASE; GROWTH-RATE; HUBBLE CONSTANT; ACOUSTIC-OSCILLATIONS; CFHTLENS AB We investigate the cosmological implications of the latest growth of structure measurement from the Baryon Oscillation Spectroscopic Survey (BOSS) CMASS Data Release 11 with particular focus on the sum of the neutrino masses, Sigma m(nu). We examine the robustness of the cosmological constraints from the baryon acoustic oscillation (BAO) scale, the Alcock-Paczynski effect and redshift-space distortions (DV/r(s), F-AP, f sigma(8)) of Beutler et al., when introducing a neutrino mass in the power spectrum template. We then discuss how the neutrino mass relaxes discrepancies between the cosmic microwave background (CMB) and other low-redshift measurements within Lambda cold dark matter. Combining our cosmological constraints with 9-year Wilkinson Microwave Anisotropy Probe (WMAP9) yields Sigma m(nu) = 0.36 +/- 0.14 eV (68 per cent c. l.), which represents a 2.6 sigma preference for non-zero neutrino mass. The significance can be increased to 3.3 sigma when including weak lensing results and other BAO constraints, yielding Sigma m(nu) = 0.35 +/- 0.10 eV (68 per cent c. l.). However, combining CMASS with Planck data reduces the preference for neutrino mass to similar to 2 sigma. When removing the CMB lensing effect in the Planck temperature power spectrum (by marginalizing over A(L)), we see shifts of similar to 1 sigma in sigma(8) and Omega(m), which have a significant effect on the neutrino mass constraints. In the case of CMASS plus Planck without the A(L) lensing signal, we find a preference for a neutrino mass of Sigma m(nu) = 0.34 +/- 0.14 eV (68 per cent c.l.), in excellent agreement with the WMAP9+CMASS value. The constraint can be tightened to 3.4 sigma yielding Sigma m(nu) = 0.36 +/- 0.10 eV (68 per cent c.l.) when weak lensing data and other BAO constraints are included. C1 [Beutler, Florian] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Saito, Shun] Univ Tokyo, Todai Inst Adv Study, Kavli Inst Phys & Math Univers WPI, Chiba 2778582, Japan. [Brownstein, Joel R.] Univ Utah, Dept Phys & Astron, Salt Lake City, UT 84112 USA. [Chuang, Chia-Hsun] Univ Autonoma Madrid, Inst Fis Teor UAM CSIC, E-28049 Madrid, Spain. [Cuesta, Antonio J.] Univ Barcelona, Inst Ciencies Cosmos, IEEC UB, E-08028 Barcelona, Spain. [Percival, Will J.; Ross, Ashley J.; Samushia, Lado] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England. [Ross, Nicholas P.] Drexel Univ, Dept Phys, Philadelphia, PA 19104 USA. [Schneider, Donald P.] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA. [Schneider, Donald P.] Penn State Univ, Inst Gravitat & Cosmos, University Pk, PA 16802 USA. [Sanchez, Ariel G.] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany. [Seo, Hee-Jong] Ohio State Univ, Dept Phys, Ctr Cosmol & Astroparticle Phys, Columbus, OH 43210 USA. [Tinker, Jeremy L.; Weaver, Benjamin A.] NYU, Ctr Cosmol & Particle Phys, New York, NY 10003 USA. [Wagner, Christian] Max Planck Inst Astrophys, D-85748 Garching, Germany. RP Beutler, F (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA. EM fbeutler@lbl.gov OI Beutler, Florian/0000-0003-0467-5438; Cuesta Vazquez, Antonio Jose/0000-0002-4153-9470 FU Japan Society for the Promotion of Science (JSPS) [25887012]; Alfred P. Sloan Foundation; National Science Foundation; US Department of Energy Office of Science; University of Arizona; Brazilian Participation Group; Brookhaven National Laboratory; Carnegie Mellon University; University of Florida; French Participation Group; German Participation Group; Harvard University; Instituto de Astrofisica de Canarias; Michigan State/Notre Dame/JINA Participation Group; Johns Hopkins University; Lawrence Berkeley National Laboratory; Max Planck Institute for Astrophysics; Max Planck Institute for Extraterrestrial Physics; New Mexico State University; New York University; Ohio State University; Pennsylvania State University; University of Portsmouth; Princeton University; Spanish Participation Group; University of Tokyo; University of Utah; Vanderbilt University; University of Virginia; University of Washington; Yale University; Office of Science of the US Department of Energy [DE-AC02-05CH11231] FX We would like to thank Renee Hlozek for providing the MCMC chains for the Planck re-analysis. FB would like to thank Martin Kilbinger and Catherine Heymans for help with the CFHTLenS data set and COSMOPMC. FB would also like to thank Martin White, Uros Seljak, Eric Linder, Daniel Dwyer, Morag Scrimgeour, Michael Mortonson, Marcel Schmittful and Blake Sherwin for helpful discussion. SS would like to thank Kiyotomo Ichiki and Masahiro Takada for providing their MCMC code for weak lensing analysis and for useful discussions. SS is supported by a Grant-in-Aid for Young Scientists (Start-up) from the Japan Society for the Promotion of Science (JSPS) (No. 25887012).; Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation and the US Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/.; SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington and Yale University.; This research used resources of the National Energy Research Scientific Computing Center, which is supported by the Office of Science of the US Department of Energy under Contract No. DE-AC02-05CH11231. NR 109 TC 48 Z9 48 U1 1 U2 19 PU OXFORD UNIV PRESS PI OXFORD PA GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND SN 0035-8711 EI 1365-2966 J9 MON NOT R ASTRON SOC JI Mon. Not. Roy. Astron. Soc. PD NOV 11 PY 2014 VL 444 IS 4 BP 3501 EP + DI 10.1093/mnras/stu1702 PG 16 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AR2FW UT WOS:000343400100035 ER PT J AU Arnold, CW Tovesson, F Meierbachtol, K Bredeweg, T Jandel, M Jorgenson, HJ Laptev, A Rusev, G Shields, DW White, M Blakeley, RE Mader, DM Hecht, AA AF Arnold, C. W. Tovesson, F. Meierbachtol, K. Bredeweg, T. Jandel, M. Jorgenson, H. J. Laptev, A. Rusev, G. Shields, D. W. White, M. Blakeley, R. E. Mader, D. M. Hecht, A. A. TI Development of position-sensitive time-of-flight spectrometer for fission fragment research SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT LA English DT Article DE Spectrometers; Fission; Fission product yields; TOF; 2E-2v ID MASS-SPECTROMETER; PRODUCTS; ENERGY AB A position sensitive, high resolution time detector for fission fragments has been developed. The SPectrometer for Ion DEtermination in fission Research (SPIDER) is a 2E-2v spectrometer designed to measure the mass of light fission fragments to a single mass unit. The time pick off detector pairs to be used in SPIDER have been tested with alpha-particles from Th-229 and its decay chain and alpha-particles and spontaneous fission fragments from Cf-252. Each detector module is comprised of thin electron conversion foil, electrostatic mirror, microchannel plates, and delay line anodes. Particle trajectories on the order of 700 mm are determined accurately to within 0.7 mm. Flight Limes were measured with 250 ps resolution FWHM. Computed particle velocities are accurate to within 0.06 mm/ns corresponding to a precision of 0.5%. An ionization chamber capable of 400 keV energy resolution coupled with the velocity measurements described here will pave the way for modestly efficient measurements of light fission fragments with unit mass resolution. (C) 2014 Elsevier B.V. All rights reserved, C1 [Arnold, C. W.; Tovesson, F.; Meierbachtol, K.; Bredeweg, T.; Jandel, M.; Jorgenson, H. J.; Laptev, A.; Rusev, G.; Shields, D. W.; White, M.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA. [Shields, D. W.] Colorado Sch Mines, Golden, CO 80401 USA. [Blakeley, R. E.; Mader, D. M.; Hecht, A. A.] Univ New Mexico, Albuquerque, NM 87131 USA. RP Arnold, CW (reprint author), Los Alamos Natl Lab, POB 1663, Los Alamos, NM 87545 USA. EM arnold@lanl.gov RI Laptev, Alexander/D-4686-2009; OI Laptev, Alexander/0000-0002-9759-9907; Rusev, Gencho/0000-0001-7563-1518; White, Morgan/0000-0003-3876-421X; Tovesson, Fredrik/0000-0002-3509-978X FU U.S. Department of Energy at Los Alamos National Laboratory; Los Alamos National Security, LLC [DE-AC52-06NA25396] FX This work was performed under the auspices of the U.S. Department of Energy at Los Alamos National Laboratory operated by the Los Alamos National Security, LLC under Contract No, DE-AC52-06NA25396. NR 13 TC 1 Z9 1 U1 3 U2 15 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0168-9002 EI 1872-9576 J9 NUCL INSTRUM METH A JI Nucl. Instrum. Methods Phys. Res. Sect. A-Accel. Spectrom. Dect. Assoc. Equip. PD NOV 11 PY 2014 VL 764 BP 53 EP 58 DI 10.1016/j.nima.2014.07.001 PG 6 WC Instruments & Instrumentation; Nuclear Science & Technology; Physics, Nuclear; Physics, Particles & Fields SC Instruments & Instrumentation; Nuclear Science & Technology; Physics GA AP3OT UT WOS:000341987000009 ER PT J AU Mashnik, SG Kerby, LM AF Mashnik, Stepan G. Kerby, Leslie M. TI MCNP6 fragmentation of light nuclei at intermediate energies SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT LA English DT Article DE Monte Carlo; Transport codes; MCNP6; Cascade-exciton model (CEM); Los Alamos version of the quark-gluon string model (LAQGSM) ID REACTION CROSS-SECTIONS; PROTON-INDUCED REACTIONS; CASCADE-EXCITON MODEL; QUARK-GLUON STRINGS; SHIELD-HIT; COLLISIONS; CARBON; PARTICLE; TARGETS; HYDROGEN AB Fragmentation reactions induced on light target nuclei by protons and light nuclei of energies around 1 GeV/nucleon and below are studied with the latest Los Alamos Monte Carlo transport code MCNP6 and with its cascade-exciton model (CEM) and Los Alamos version of the quark-gluon string model (LAQGSM) event generators, version 03.03, used as stand-alone codes. Such reactions are involved in different applications, like cosmic-ray-induced single event upsets (SEU's), radiation protection, and cancer therapy with proton and ion beams, among others; therefore, it is important that MCNP6 simulates them as well as possible. CEM and LAQGSM assume that intermediate-energy fragmentation reactions on light nuclei occur generally in two stages. The first stage is the intranuclear cascade (INC), Followed by the second, Fermi breakup disintegration of light excited residual nuclei produced after the INC. Both CEM and LAQGSM account also for coalescence of light fragments (complex particles) up to He-4 from energetic nucleons emitted during INC. We investigate the validity and performance of MCNP6, CEM, and LAQGSM in simulating fragmentation reactions at intermediate energies and discuss possible ways of further improving these codes. (C) 2014 Elsevier B.V. All rights reserved. C1 [Mashnik, Stepan G.; Kerby, Leslie M.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA. [Kerby, Leslie M.] Univ Idaho, Moscow, ID 83844 USA. RP Mashnik, SG (reprint author), Los Alamos Natl Lab, POB 1663, Los Alamos, NM 87545 USA. EM mashnik@lanl.gov OI Kerby, Leslie/0000-0002-4496-6427 FU National Nuclear Security Administration of the U.S. Department of Energy at Los Alamos National Laboratory [DE-AC52-06NA253996]; M. Hildred Blewett Fellowship of the American Physical Society FX this study was carried out under the auspices of the National Nuclear Security Administration of the U.S. Department of Energy at Los Alamos National Laboratory under Contract No. DE-AC52-06NA253996.; This work is supported in part (for L.M.K.) by the M. Hildred Blewett Fellowship of the American Physical Society, www.aps.org NR 70 TC 7 Z9 7 U1 0 U2 5 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0168-9002 EI 1872-9576 J9 NUCL INSTRUM METH A JI Nucl. Instrum. Methods Phys. Res. Sect. A-Accel. Spectrom. Dect. Assoc. Equip. PD NOV 11 PY 2014 VL 764 BP 59 EP 81 DI 10.1016/j.nima.2014.07.016 PG 23 WC Instruments & Instrumentation; Nuclear Science & Technology; Physics, Nuclear; Physics, Particles & Fields SC Instruments & Instrumentation; Nuclear Science & Technology; Physics GA AP3OT UT WOS:000341987000010 ER PT J AU Haines, JR McManamy, TJ Gabriel, TA Battle, RE Chipley, KK Crabtree, JA Jacobs, LL Lousteau, DC Rennich, MJ Riemer, BW AF Haines, J. R. McManamy, T. J. Gabriel, T. A. Battle, R. E. Chipley, K. K. Crabtree, J. A. Jacobs, L. L. Lousteau, D. C. Rennich, M. J. Riemer, B. W. TI Spallation neutron source target station design, development, and commissioning SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT LA English DT Article DE Targets; High power; Spallation; Mercury; Particle accelerator ID MERCURY TARGET; VESSELS AB The spallation neutron source target station is designed to safely, reliably, and efficiently convert a 1 GeV beam of protons to a high flux of about 1 meV neutrons that are available at 24 neutron scattering instrument beam lines. Research and development findings, design requirements, design description, initial checkout testing, and results from early operation with beam are discussed for each of the primary target subsystems, including the mercury target, neutron moderators and reflector, surrounding vessels and shielding, utilities, remote handling equipment, and instrumentation and controls. Future plans for the mercury target development program are also briefly discussed. (C) 2014 Elsevier B.V. All rights reserved. C1 [Haines, J. R.; McManamy, T. J.; Gabriel, T. A.; Battle, R. E.; Chipley, K. K.; Crabtree, J. A.; Jacobs, L. L.; Lousteau, D. C.; Rennich, M. J.; Riemer, B. W.] Oak Ridge Natl Lab, Oak Ridge, TN 37831 USA. RP Haines, JR (reprint author), Oak Ridge Natl Lab, POB 2008, Oak Ridge, TN 37831 USA. EM hainesjr@ornl.gov OI Rennich, Mark/0000-0001-6945-0075; Riemer, Bernard/0000-0002-6922-3056 NR 27 TC 2 Z9 2 U1 1 U2 13 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0168-9002 EI 1872-9576 J9 NUCL INSTRUM METH A JI Nucl. Instrum. Methods Phys. Res. Sect. A-Accel. Spectrom. Dect. Assoc. Equip. PD NOV 11 PY 2014 VL 764 BP 94 EP 115 DI 10.1016/j.nima.2014.03.068 PG 22 WC Instruments & Instrumentation; Nuclear Science & Technology; Physics, Nuclear; Physics, Particles & Fields SC Instruments & Instrumentation; Nuclear Science & Technology; Physics GA AP3OT UT WOS:000341987000012 ER PT J AU Hoppe, EW Aalseth, CE Farmer, OT Hossbach, TW Liezers, M Miley, HS Overman, NR Reeves, JH AF Hoppe, E. W. Aalseth, C. E. Farmer, O. T. Hossbach, T. W. Liezers, M. Miley, H. S. Overman, N. R. Reeves, J. H. TI Reduction of radioactive backgrounds in electroformed copper for ultra-sensitive radiation detectors SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT LA English DT Article DE Low background; Copper; Electroforming; Thorium; Uranium; ICP-MS ID DOUBLE-BETA DECAY; INTERNATIONAL GERMANIUM EXPERIMENT; UNDERGROUND MEASUREMENTS; SPECTROMETERS; SAMPLES AB Ultra-pure construction materials are required for the next generation of neutrino physics, dark matter and environmental science applications. These materials are also important for use in high-purity germanium spectrometers used in screening materials for radiopurity. The next-generation science applications require materials with radiopurity levels at or below 1 mu Bq/kg Th-232 and U-238. Yet radiometric analysis lacks sensitivity below similar to 10 mu Bq/kg for the U and Th decay chains. This limits both the selection of clean materials and the validation of purification processes. Copper is an important high-purity material for low-background experiments due to the ease with which it can be purified by electrochemical methods. Electroplating for purification into near-final shapes, known as electroforming, is one such method. Continued refinement of the copper electroforming process is underway, for the First time guided by an ICP-MS based assay method that can measure Th-232 and U-238 near the desired purity levels. An assay of electroformed copper at a mu Bq/kg level has been achieved and is described. The implications of electroformed copper at or better than this purity on next-generation low-background experiments are discussed. (C) 2014 Elsevier B.V. All rights reserved. C1 [Reeves, J. H.] Reeves & Son LW, Richland, WA 99352 USA. [Hoppe, E. W.; Aalseth, C. E.; Farmer, O. T.; Hossbach, T. W.; Liezers, M.; Miley, H. S.; Overman, N. R.] Pacific NW Natl Lab, Richland, WA 99352 USA. RP Hoppe, EW (reprint author), Pacific NW Natl Lab, Richland, WA 99352 USA. EM cric.hoppe@pnnl.gov FU United States Department of Energy, NNSA Office of Research and Engineering [NA-22]; Office of Nuclear Physics in the DOE Office of Science; Battelle Memorial Institute [DE-AC05-76RLO1830] FX The authors would like to acknowledge the United States Department of Energy, NNSA Office of Research and Engineering (NA-22), and the Office of Nuclear Physics in the DOE Office of Science for their support of this work, Pacific Northwest National Laboratory is managed by Battelle Memorial Institute under Contract DE-AC05-76RLO1830. Further, the authors wish to gratefully acknowledge the scientific leadership of our deceased colleague, Ronald L. Brodzinski, who with humor and resolution inspired us to confidently approach the unknown again and again. NR 27 TC 10 Z9 10 U1 1 U2 14 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0168-9002 EI 1872-9576 J9 NUCL INSTRUM METH A JI Nucl. Instrum. Methods Phys. Res. Sect. A-Accel. Spectrom. Dect. Assoc. Equip. PD NOV 11 PY 2014 VL 764 BP 116 EP 121 DI 10.1016/j.nima.2014.06.082 PG 6 WC Instruments & Instrumentation; Nuclear Science & Technology; Physics, Nuclear; Physics, Particles & Fields SC Instruments & Instrumentation; Nuclear Science & Technology; Physics GA AP3OT UT WOS:000341987000013 ER PT J AU Ball, R Beene, JR Ben-Moshe, M Benhammou, Y Bensimon, B Chapman, JW Etzion, E Ferretti, C Friedman, PS Levin, DS Silver, Y Varner, RL Weaverdyck, C Wetzel, R Zhou, B Anderson, T McKinny, K Bentefour, EH AF Ball, R. Beene, J. R. Ben-Moshe, M. Benhammou, Y. Bensimon, B. Chapman, J. W. Etzion, E. Ferretti, C. Friedman, P. S. Levin, D. S. Silver, Y. Varner, R. L. Weaverdyck, C. Wetzel, R. Zhou, B. Anderson, T. McKinny, K. Bentefour, E. H. TI Development of a plasma panel radiation detector SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT LA English DT Article DE Radiation detector; Gaseous ionization detector; Micropattern gaseous detectors; Neutron detectors; Plasma panels; Pixel radiation detector AB This article reports on the development and experimental results of commercial plasma display panels adapted for their potential use as micropattern gas radiation detectors. The plasma panel sensor (PPS) design and materials include glass substrates, metal electrodes and inert gas mixtures which provide a physically robust, hermetically sealed device. Plasma display panels used as detectors were tested with cosmic ray muons, beta rays and gamma rays, protons, and thermal neutrons. The results demonstrated rise times and time resolution of a few nanoseconds, as well as sub-millimeter spatial resolution compatible with the pixel pitch. (C) 2014 Elsevier B.V. All rights reserved. C1 [Ball, R.; Chapman, J. W.; Ferretti, C.; Levin, D. S.; Weaverdyck, C.; Wetzel, R.; Zhou, B.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA. [Beene, J. R.; Varner, R. L.] Oak Ridge Natl Lab, Div Phys, Oak Ridge, TN 37831 USA. [Ben-Moshe, M.; Benhammou, Y.; Bensimon, B.; Etzion, E.; Silver, Y.] Tel Aviv Univ, Beverly & Raymond Suckler Sch Phys & Astron, IL-69978 Tel Aviv, Israel. [Friedman, P. S.] Integrated Sensors LLC, Ottawa Hills, OH 43606 USA. [Anderson, T.; McKinny, K.] GE Measurement & Control, Twinsburg, OH 44087 USA. [Bentefour, E. H.] Ion Beam Applicat SA, B-1348 Louvain La Neuve, Belgium. RP Levin, DS (reprint author), Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA. FU U.S. Department of Energy (DOE) - Office of Nuclear Physics Small Business Innovation Research grant [DE-SC0006204, DE-FG02-07ER84749]; U.S. DOE, Office of Nuclear Physics, Applications of Nuclear Science and Technology grant [DE-FG02-12ER41788]; I-CORE Program of the Planning and Budgeting Committee; Israel Science Foundation [1937/12]; Israel-American Binational Science Foundation [1008123]; agency of the United States Government FX Development of the PPS project was funded by the U.S. Department of Energy (DOE) - Office of Nuclear Physics Small Business Innovation Research grant award numbers DE-SC0006204 and DE-FG02-07ER84749 to Integrated Sensors, U.S. DOE, Office of Nuclear Physics, Applications of Nuclear Science and Technology grant to Oak Ridge National Laboratory, operated by UT-Battelle, LLC for the U.S. DOE, and DOE - Office of High Energy Physics grant number DE-FG02-12ER41788 to the University of Michigan. The research at Tel Aviv University was supported by the I-CORE Program of the Planning and Budgeting Committee and the Israel Science Foundation (Grant number 1937/12). Funding for scientific exchange and collaboration between Tel Aviv University and the University of Michigan was provided by the Israel-American Binational Science Foundation, Grant number 1008123.; Disclaimer: This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof The views and opinions of authors expressed herein do not necessarily state or reflect those of the United States Government or any agency thereof. NR 33 TC 2 Z9 2 U1 1 U2 17 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0168-9002 EI 1872-9576 J9 NUCL INSTRUM METH A JI Nucl. Instrum. Methods Phys. Res. Sect. A-Accel. Spectrom. Dect. Assoc. Equip. PD NOV 11 PY 2014 VL 764 BP 122 EP 132 DI 10.1016/j.nima.2014.07.028 PG 11 WC Instruments & Instrumentation; Nuclear Science & Technology; Physics, Nuclear; Physics, Particles & Fields SC Instruments & Instrumentation; Nuclear Science & Technology; Physics GA AP3OT UT WOS:000341987000014 ER PT J AU Arnold, O Bilheux, JC Borreguero, JM Buts, A Campbell, SI Chapon, L Doucet, M Draper, N Leal, RF Gigg, MA Lynch, VE Markvardsen, A Mikkelson, DJ Mikkelson, RL Miller, R Palmen, K Parker, P Passos, G Perring, TG Peterson, PF Ren, S Reuter, MA Savici, AT Taylor, JW Taylor, RJ Tolchenoy, R Zhou, W Zikoysky, J AF Arnold, O. Bilheux, J. C. Borreguero, J. M. Buts, A. Campbell, S. I. Chapon, L. Doucet, M. Draper, N. Leal, R. Ferraz Gigg, M. A. Lynch, V. E. Markvardsen, A. Mikkelson, D. J. Mikkelson, R. L. Miller, R. Palmen, K. Parker, P. Passos, G. Perring, T. G. Peterson, P. F. Ren, S. Reuter, M. A. Savici, A. T. Taylor, J. W. Taylor, R. J. Tolchenoy, R. Zhou, W. Zikoysky, J. TI Mantid-Data analysis and visualization package for neutron scattering and mu SR experiments SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT LA English DT Article DE Data analysis; Data visualization; Computer interfaces AB The Mantid framework is a software solution developed for the analysis and visualization of neutron scattering and muon spin measurements. The framework is jointly developed by software engineers and scientists at the ISIS Neutron and Muon Facility and the Oak Ridge National Laboratory. The objectives, functionality and novel design aspects of Mantid are described. Published by Elsevier B.V. C1 [Arnold, O.; Buts, A.; Chapon, L.; Draper, N.; Gigg, M. A.; Markvardsen, A.; Palmen, K.; Parker, P.; Passos, G.; Perring, T. G.; Savici, A. T.; Taylor, J. W.; Taylor, R. J.] Rutherford Appleton Lab, ISIS Facil, Didcot OX11 0QX, Oxon, England. [Arnold, O.; Draper, N.; Gigg, M. A.; Tolchenoy, R.] Tessella Ltd, Abingdon, Oxon, England. [Bilheux, J. C.; Borreguero, J. M.; Campbell, S. I.; Doucet, M.; Lynch, V. E.; Mikkelson, D. J.; Mikkelson, R. L.; Peterson, P. F.; Ren, S.; Reuter, M. A.; Savici, A. T.; Zikoysky, J.] Oak Ridge Natl Lab, Oak Ridge, TN 37831 USA. [Chapon, L.; Leal, R. Ferraz] Inst Laue Langevin, Grenoble, France. [Mikkelson, D. J.; Mikkelson, R. L.] Univ Wisconsin Stout, Menomonie, WI USA. [Miller, R.] Oak Ridge Natl Lab, Comp & Computat Sci Directorate, Oak Ridge, TN USA. [Taylor, J. W.] Tessellu Inc, Newton, MA USA. RP Savici, AT (reprint author), Oak Ridge Natl Lab, Oak Ridge, TN 37831 USA. EM saviciat@ornl.gov RI Lynch, Vickie/J-4647-2012; Borreguero, Jose/B-2446-2009; Doucet, Mathieu/A-5333-2010; Savici, Andrei/F-2790-2013; Campbell, Stuart/A-8485-2010; Bilheux, Jean/A-2823-2016 OI Lynch, Vickie/0000-0002-5836-7636; Borreguero, Jose/0000-0002-0866-8158; Doucet, Mathieu/0000-0002-5560-6478; Savici, Andrei/0000-0001-5127-8967; Campbell, Stuart/0000-0001-7079-0878; Bilheux, Jean/0000-0003-2172-6487 FU Scientific User Facilities Division, Office of Basic Energy Sciences, US Department of Energy; Science and Technology Facilities Council (STFC) UK; NMI3 [WP6] FX The development team would like to thank all instrument scientists and students at ISIS and SNS for their feedback and contributions, R Radaelli, and R. McGreevy for championing the project at ISIS in the initial stages, and R. McGreevy, I. Anderson, and M. Hagen for forging the collaboration between ORNL and STFC. We acknowledge A. Hillier for contributions to this paper. Work at ORNL was sponsored by the Scientific User Facilities Division, Office of Basic Energy Sciences, US Department of Energy. Work at the ISIS facility was funded by the Science and Technology Facilities Council (STFC) UK. Development for ILL instruments was funded by NMI3 (WP6). NR 13 TC 100 Z9 100 U1 6 U2 52 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0168-9002 EI 1872-9576 J9 NUCL INSTRUM METH A JI Nucl. Instrum. Methods Phys. Res. Sect. A-Accel. Spectrom. Dect. Assoc. Equip. PD NOV 11 PY 2014 VL 764 BP 156 EP 166 DI 10.1016/j.nima.2014.07.029 PG 11 WC Instruments & Instrumentation; Nuclear Science & Technology; Physics, Nuclear; Physics, Particles & Fields SC Instruments & Instrumentation; Nuclear Science & Technology; Physics GA AP3OT UT WOS:000341987000018 ER PT J AU Pelliccia, D Sen, T AF Pelliccia, Daniele Sen, Tanaji TI A two-step method for retrieving the longitudinal profile of an electron bunch from its coherent radiation SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT LA English DT Article DE Phase retrieval; Electron bunch longitudinal profile; Kramers-Kronig; Iterative method; Coherent transition radiation; Photoinjector ID CHARGED-PARTICLE-BUNCH; PHASE RETRIEVAL; X-RAY; TRANSITION RADIATION; SHAPE; SPECTRUM; RECONSTRUCTION; DIFFRACTION; SYNCHROTRON; OBJECT AB The coherent radiation emitted by an electron bunch provides a diagnostic signal that can be used to estimate its longitudinal distribution. Commonly only the amplitude of the intensity spectrum can be measured and the associated phase must be calculated to obtain the bunch profile. Very recently an iterative method was proposed to retrieve this phase. However ambiguities associated with non-uniqueness of the solution are always present in the phase retrieval procedure. Here we present a method to overcome the ambiguity problem by first performing multiple independent runs of the phase retrieval procedure and then second, sorting the good solutions by means of cross-correlation analysis. Results obtained with simulated bunches of various shapes and experimental measured spectra are presented, discussed and compared with the established Kramers-Kronig method It is shown that even when the effect of the ambiguities is strong, as is the case for a double peak in the profile, the cross-correlation post-processing is able to filter out unwanted solutions. We show that, unlike the Kramers-Kronig method, the combined approach presented is able to faithfully reconstruct complicated bunch profiles. (C) 2014 Elsevier B.V. All rights reserved. C1 [Pelliccia, Daniele] Monash Univ, Sch Phys, Clayton, Vic 3800, Australia. [Sen, Tanaji] Fermilab Natl Accelerator Lab, Accelerator Phys Ctr, Batavia, IL 60510 USA. RP Sen, T (reprint author), Fermilab Natl Accelerator Lab, Accelerator Phys Ctr, POB 500, Batavia, IL 60510 USA. RI Pelliccia, Daniele/A-3140-2012 OI Pelliccia, Daniele/0000-0001-8751-2620 FU Australian Research Council [DE120101504]; Fermi Research Alliance, LLC [DE-AC02-07CH11359]; United States Department of Energy FX D.P. acknowledges the support of the Australian Research Council (Grant no. DE120101504). T.S. thanks Charles Thangaraj and Randy Thurman-Keup for generously sharing their data and useful discussions. Fermilab is operated by Fermi Research Alliance, LLC under Contract no. DE-AC02-07CH11359 with the United States Department of Energy. NR 33 TC 2 Z9 2 U1 1 U2 2 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0168-9002 EI 1872-9576 J9 NUCL INSTRUM METH A JI Nucl. Instrum. Methods Phys. Res. Sect. A-Accel. Spectrom. Dect. Assoc. Equip. PD NOV 11 PY 2014 VL 764 BP 206 EP 214 DI 10.1016/j.nima.2014.07.024 PG 9 WC Instruments & Instrumentation; Nuclear Science & Technology; Physics, Nuclear; Physics, Particles & Fields SC Instruments & Instrumentation; Nuclear Science & Technology; Physics GA AP3OT UT WOS:000341987000024 ER PT J AU Wang, ZH Morris, CL Bacon, JD Brockwell, MI Ramsey, JC AF Wang, Zhehui Morris, C. L. Bacon, J. D. Brockwell, M. I. Ramsey, J. C. TI A double-helix neutron detector using micron-size B-10 powder SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT LA English DT Article DE Double-helix electrode configuration; B-10 powder; Neutron detection efficiency; Detector lifetime ID PROPORTIONAL COUNTER AB A double-helix electrode configuration is combined with a B-10 powder coating technique to build large-area (9 in. x 36 in., or about 23 cm by 91 cm) neutron detectors. The neutron detection efficiency for each of the four prototypes is comparable to 3.7 x 10(3) cm(3) of He-3 inside a cylindrical tube 91 cm long. One unit has been operational continuously for 18 months and the change of efficiency is less than 1%. An analytic model for pulse height spectra is described and the predicted mean film thicknesses agree with the experiment to within 30%. Further detector optimization is possible through film texture, powder size, moderator box and gas. The estimated production cost per unit is less than 3k US$ and the technology is thus suitable for deployment in large numbers. (C) 2014 Elsevier B.V. All rights reserved, C1 [Wang, Zhehui; Morris, C. L.; Bacon, J. D.; Brockwell, M. I.; Ramsey, J. C.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA. RP Wang, ZH (reprint author), Los Alamos Natl Lab, POB 1663, Los Alamos, NM 87545 USA. EM zwang@lanl.gov FU CRADA agreement with TSA systems, Longmont, CO, USA FX We thank Mr, Michael Everhart-Erickson, Ms. Laura Barber and Ms, Erica Sullivan for their efforts in commercialization of the 10B-based neutron detector technology. This work was supported in part by a CRADA agreement with TSA systems, Longmont, CO, USA. NR 13 TC 1 Z9 1 U1 1 U2 6 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0168-9002 EI 1872-9576 J9 NUCL INSTRUM METH A JI Nucl. Instrum. Methods Phys. Res. Sect. A-Accel. Spectrom. Dect. Assoc. Equip. PD NOV 11 PY 2014 VL 764 BP 261 EP 267 DI 10.1016/j.nima.2014.07.056 PG 7 WC Instruments & Instrumentation; Nuclear Science & Technology; Physics, Nuclear; Physics, Particles & Fields SC Instruments & Instrumentation; Nuclear Science & Technology; Physics GA AP3OT UT WOS:000341987000033 ER PT J AU Abe, Y dos Anjos, JC Barriere, JC Baussan, E Bekman, I Bergevin, M Bezerra, TJC Bezrukov, L Blucher, E Buck, C Busenitz, J Cabrera, A Caden, E Camilleri, L Carr, R Cerrada, M Chang, PJ Chauveau, E Chimenti, P Collin, AP Conover, E Conrad, JM Crespo-Anadon, JI Crum, K Cucoanes, A Damon, E Dawson, JV Dhooghe, J Dietrich, D Djurcic, Z Dracos, M Elnimr, M Etenko, A Fallot, M von Feilitzsch, F Felde, J Fernandes, SM Fischer, V Franco, D Franke, M Furuta, H Gil-Botella, I Giot, L Goger-Neff, M Gonzalez, LFG Goodenough, L Goodman, MC Grant, C Haag, N Hara, T Haser, J Hofmann, M Horton-Smith, GA Hourlier, A Ishitsuka, M Jochum, J Jollet, C Kaether, F Kalousis, LN Kamyshkov, Y Kaplan, DM Kawasaki, T Kemp, E de Kerret, H Kryn, D Kuze, M Lachenmaier, T Lane, CE Lasserre, T Letourneau, A Lhuillier, D Lima, HP Lindner, M Lopez-Castano, JM LoSecco, JM Lubsandorzhiev, B Lucht, S Maeda, J Mariani, C Maricic, J Martino, J Matsubara, T Mention, G Meregaglia, A Miletic, T Milincic, R Minotti, A Nagasaka, Y Nikitenko, Y Novella, P Oberauer, L Obolensky, M Onillon, A Osborn, A Palomares, C Pepe, IM Perasso, S Pfahler, P Porta, A Pronost, G Reichenbacher, J Reinhold, B Rohling, M Roncin, R Roth, S Rybolt, B Sakamoto, Y Santorelli, R Schilithz, AC Schonert, S Schoppmann, S Shaevitz, MH Sharankova, R Shimojima, S Shrestha, D Sibille, V Sinev, V Skorokhvatov, M Smith, E Spitz, J Stahl, A Stancu, I Stokes, LFF Strait, M Stuken, A Suekane, F Sukhotin, S Sumiyoshi, T Sun, Y Svoboda, R Terao, K Tonazzo, A Thi, HHT Valdiviesso, G Vassilopoulos, N Veyssiere, C Vivier, M Wagner, S Walsh, N Watanabe, H Wiebusch, C Winslow, L Wurm, M Yang, G Yermia, F Zimmer, V AF Abe, Y. dos Anjos, J. C. Barriere, J. C. Baussan, E. Bekman, I. Bergevin, M. Bezerra, T. J. C. Bezrukov, L. Blucher, E. Buck, C. Busenitz, J. Cabrera, A. Caden, E. Camilleri, L. Carr, R. Cerrada, M. Chang, P. -J. Chauveau, E. Chimenti, P. Collin, A. P. Conover, E. Conrad, J. M. Crespo-Anadon, J. I. Crum, K. Cucoanes, A. Damon, E. Dawson, J. V. Dhooghe, J. Dietrich, D. Djurcic, Z. Dracos, M. Elnimr, M. Etenko, A. Fallot, M. von Feilitzsch, F. Felde, J. Fernandes, S. M. Fischer, V. Franco, D. Franke, M. Furuta, H. Gil-Botella, I. Giot, L. Goeger-Neff, M. Gonzalez, L. F. G. Goodenough, L. Goodman, M. C. Grant, C. Haag, N. Hara, T. Haser, J. Hofmann, M. Horton-Smith, G. A. Hourlier, A. Ishitsuka, M. Jochum, J. Jollet, C. Kaether, F. Kalousis, L. N. Kamyshkov, Y. Kaplan, D. M. Kawasaki, T. Kemp, E. de Kerret, H. Kryn, D. Kuze, M. Lachenmaier, T. Lane, C. E. Lasserre, T. Letourneau, A. Lhuillier, D. Lima, H. P., Jr. Lindner, M. Lopez-Castano, J. M. LoSecco, J. M. Lubsandorzhiev, B. Lucht, S. Maeda, J. Mariani, C. Maricic, J. Martino, J. Matsubara, T. Mention, G. Meregaglia, A. Miletic, T. Milincic, R. Minotti, A. Nagasaka, Y. Nikitenko, Y. Novella, P. Oberauer, L. Obolensky, M. Onillon, A. Osborn, A. Palomares, C. Pepe, I. M. Perasso, S. Pfahler, P. Porta, A. Pronost, G. Reichenbacher, J. Reinhold, B. Roehling, M. Roncin, R. Roth, S. Rybolt, B. Sakamoto, Y. Santorelli, R. Schilithz, A. C. Schoenert, S. Schoppmann, S. Shaevitz, M. H. Sharankova, R. Shimojima, S. Shrestha, D. Sibille, V. Sinev, V. Skorokhvatov, M. Smith, E. Spitz, J. Stahl, A. Stancu, I. Stokes, L. F. F. Strait, M. Stueken, A. Suekane, F. Sukhotin, S. Sumiyoshi, T. Sun, Y. Svoboda, R. Terao, K. Tonazzo, A. Thi, H. H. Trinh Valdiviesso, G. Vassilopoulos, N. Veyssiere, C. Vivier, M. Wagner, S. Walsh, N. Watanabe, H. Wiebusch, C. Winslow, L. Wurm, M. Yang, G. Yermia, F. Zimmer, V. TI Precision muon reconstruction in Double Chooz SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT LA English DT Article DE Double Chooz; Munn reconstruction; Neutrino detector AB We describe a muon track reconstruction algorithm for the reactor anti-neutrino experiment Double Chooz, The Double Chooz detector consists of two optically isolated volumes of the liquid scintillator viewed by PMTs, and an Outer Veto above these made of crossed scintillator strips. Muons are reconstructed by their Outer Veto hit positions along with timing information from the other two detector volumes. All muons are fit under the hypothesis that they are through-going and ultrarelativistic, If the energy depositions suggest that the muon may have stopped, the reconstruction fits also for this hypothesis and chooses between the two via the relative goodness-of-fit. In the ideal case of a through-going muon intersecting the center of the detector, the resolution is similar to 40 mm in each transverse dimension. High quality muon reconstruction is an important tool for reducing the impact of the cosmogenic isotope background in Double Chooz. (C) 2014 Elsevier B.V. All rights reserved. C1 [Bekman, I.; Lucht, S.; Roth, S.; Schoppmann, S.; Stahl, A.; Stueken, A.; Wiebusch, C.] Rhein Westfal TH Aachen, Inst Phys 3, D-52056 Aachen, Germany. [Busenitz, J.; Elnimr, M.; Fernandes, S. M.; Reichenbacher, J.; Stancu, I.; Sun, Y.] Univ Alabama, Dept Phys & Astron, Tuscaloosa, AL 35487 USA. [Djurcic, Z.; Goodenough, L.; Goodman, M. C.; Yang, G.] Argonne Natl Lab, Argonne, IL 60439 USA. [Cabrera, A.; Dawson, J. V.; Franco, D.; Hourlier, A.; de Kerret, H.; Kryn, D.; Lasserre, T.; Novella, P.; Obolensky, M.; Perasso, S.; Roncin, R.; Tonazzo, A.] Univ Paris Diderot, Sorbonne Paris Cite, Observ Paris, CEA IRFU,CNRS IN2P3,AstroParticule & Cosmol, F-75205 Paris 13, France. [dos Anjos, J. C.; Lima, H. P., Jr.; Pepe, I. M.; Schilithz, A. C.; Valdiviesso, G.] Ctr Brasileiro Pesquisas Fis, BR-22290180 Rio De Janeiro, Brazil. [Blucher, E.; Conover, E.; Crum, K.; Strait, M.] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA. [Cerrada, M.; Crespo-Anadon, J. I.; Gil-Botella, I.; Lopez-Castano, J. M.; Palomares, C.; Santorelli, R.] CIEMAT, E-28040 Madrid, Spain. [Camilleri, L.; Carr, R.; Shaevitz, M. H.] Columbia Univ, New York, NY 10027 USA. [Bergevin, M.; Dhooghe, J.; Felde, J.; Grant, C.; Svoboda, R.; Walsh, N.] Univ Calif Davis, Davis, CA 95616 USA. [Caden, E.; Damon, E.; Lane, C. E.; Maricic, J.; Miletic, T.; Milincic, R.; Smith, E.] Drexel Univ, Dept Phys, Philadelphia, PA 19104 USA. [Nagasaka, Y.] Hiroshima Inst Technol, Hiroshima 7315193, Japan. [Kaplan, D. M.; Yang, G.] IIT, Dept Phys, Chicago, IL 60616 USA. [Bezrukov, L.; Lubsandorzhiev, B.; Nikitenko, Y.; Sinev, V.] Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia. [Barriere, J. C.; Fischer, V.; Lasserre, T.; Lhuillier, D.; Mention, G.; Sibille, V.; Veyssiere, C.; Vivier, M.] IRFU, Ctr Saclay, Commissariat Energies Atom & Energies Alternat, F-91191 Gif Sur Yvette, France. [Chang, P. -J.; Horton-Smith, G. A.; Shrestha, D.] Kansas State Univ, Dept Phys, Manhattan, KS 66506 USA. [Hara, T.] Kobe Univ, Dept Phys, Kobe, Hyogo 6578501, Japan. [Cabrera, A.; Etenko, A.; Skorokhvatov, M.; Sukhotin, S.] NRC Kurchatov Inst, Moscow 123182, Russia. [Conrad, J. M.; Spitz, J.; Terao, K.; Winslow, L.] MIT, Cambridge, MA 02139 USA. [Buck, C.; Collin, A. P.; Haser, J.; Kaether, F.; Lindner, M.; Reinhold, B.; Wagner, S.; Watanabe, H.] Max Planck Inst Kernphys, D-69117 Heidelberg, Germany. [Kawasaki, T.] Niigata Univ, Dept Phys, Niigata 9502181, Japan. [LoSecco, J. M.] Univ Notre Dame, Notre Dame, IN 46556 USA. [Baussan, E.; Dracos, M.; Jollet, C.; Meregaglia, A.; Minotti, A.; Vassilopoulos, N.] Univ Strasbourg, CNRS IN2P3, IPHC, F-67037 Strasbourg, France. [Cucoanes, A.; Fallot, M.; Giot, L.; Martino, J.; Onillon, A.; Porta, A.; Pronost, G.; Yermia, F.] Univ Nantes, Ecole Mines Nantes, CNRS IN2P3, SUBATECH, F-44307 Nantes, France. [Kamyshkov, Y.; Osborn, A.; Rybolt, B.] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA. [Bezerra, T. J. C.; Chauveau, E.; Furuta, H.; Suekane, F.] Tohoku Univ, Res Ctr Neutrino Sci, Sendai, Miyagi 9808578, Japan. [Sakamoto, Y.] Tohoku Gakuin Univ, Sendai, Miyagi 9813193, Japan. [Abe, Y.; Ishitsuka, M.; Kuze, M.; Sharankova, R.] Tokyo Inst Technol, Dept Phys, Tokyo 1528551, Japan. [Maeda, J.; Matsubara, T.; Shimojima, S.; Sumiyoshi, T.] Tokyo Metropolitan Univ, Dept Phys, Tokyo 1920397, Japan. [von Feilitzsch, F.; Franke, M.; Goeger-Neff, M.; Haag, N.; Hofmann, M.; Oberauer, L.; Pfahler, P.; Schoenert, S.; Thi, H. H. Trinh; Zimmer, V.] Tech Univ Munich, Dept Phys, D-85748 Garching, Germany. [Dietrich, D.; Jochum, J.; Lachenmaier, T.; Roehling, M.; Stokes, L. F. F.; Wurm, M.] Univ Tubingen, Kepler Ctr Astro & Particle Phys, D-72076 Tubingen, Germany. [Chimenti, P.] Univ Fed Abc, BR-09210580 Santo Andre, SP, Brazil. [Gonzalez, L. F. G.; Kemp, E.] Univ Estadual Campinas, BR-13083970 Campinas, SP, Brazil. [Kalousis, L. N.; Mariani, C.] Virginia Tech, Ctr Neutrino Phys, Blacksburg, VA 24061 USA. RP Strait, M (reprint author), Univ Chicago, Enrico Fermi Inst, 5640 S Ellis Ave, Chicago, IL 60637 USA. EM strait@hep.uchiago.edu RI Skorokhvatov, Mikhail/R-9735-2016; Wiebusch, Christopher/G-6490-2012; Inst. of Physics, Gleb Wataghin/A-9780-2017; Santorelli, Roberto/L-6017-2015; Horton-Smith, Glenn/A-4409-2011; Chimenti, Pietro/F-9898-2012; Mariani, Camillo/J-6070-2015; Cerrada, Marcos/J-6934-2014; Valdiviesso, Gustavo/G-3404-2011; Junqueira de Castro Bezerra, Thiago/F-1610-2013; Stahl, Achim/E-8846-2011; Gil Botella, Ines/H-8991-2015; Bezrukov, Leonid/M-5654-2013; Schoppmann, Stefan/M-3057-2015; Palomares, Carmen/H-7783-2015; Roth, Stefan/J-2757-2016; Kamyshkov, Yuri/J-7999-2016 OI Wiebusch, Christopher/0000-0002-6418-3008; Santorelli, Roberto/0000-0002-0012-2644; Horton-Smith, Glenn/0000-0001-9677-9167; Spitz, Joshua/0000-0002-6288-7028; Franco, Davide/0000-0001-5604-2531; Lindner, Manfred/0000-0002-3704-6016; Chimenti, Pietro/0000-0002-9755-5066; Mariani, Camillo/0000-0003-3284-4681; Cerrada, Marcos/0000-0003-0112-1691; Valdiviesso, Gustavo/0000-0002-0381-3619; Junqueira de Castro Bezerra, Thiago/0000-0002-0424-7903; Stahl, Achim/0000-0002-8369-7506; Schoppmann, Stefan/0000-0002-7208-0578; Palomares, Carmen/0000-0003-4374-9065; Roth, Stefan/0000-0003-3616-2223; Kamyshkov, Yuri/0000-0002-3789-7152 FU CEA; CNRS/IN2P3; LabEx UnivEarthS in France [ANR-11-1DEX-0005-02]; Ministry of Education, Culture, Sports, Science and Technology of Japan (MEXT); Japan Society for the Promotion of Science (JSPS); Department of Energy; National Science Foundation of the United States; Ministerio de Ciencia e Innovacion (MICINN) of Spain; Max Planck Gesellschaft; Deutsche Forschungsgemeinschaft DEG [SBH WI 2152]; Transregional Collaborative Research Center TR27; excellence cluster "Origin and Structure of the Universe"; Maier-Leibnitz-Laboratorium Garching in Germany; Russian Academy of Science; Kurchatov Institute and RFBR (the Russian Foundation for Basic Research); Brazilian Ministry of Science, Technology and Innovation (MCTI); Financiadora de Estudos c Projetos (FINEP); Conselho Nacional de Desenvolvimento Cientifico e Tecnoleigico (CNPq); Sao Paulo Research Foundation (FAPESP); Brazilian Network for High Energy Physics (RENAFAE) in Brazil; the computer center CCIN2P3 FX We thank the French electricity company EDF; the European fund FEDER; the Region de Champagne Ardenne; the Departement des Ardennes; and the Communaute des Communes Ardennes Rives acknowledge the support from the CEA, CNRS/IN2P3, the computer center CCIN2P3, and LabEx UnivEarthS in France (ANR-11-1DEX-0005-02); the Ministry of Education, Culture, Sports, Science and Technology of Japan (MEXT) and the Japan Society for the Promotion of Science (JSPS); the Department of Energy and the National Science Foundation of the United States; the Ministerio de Ciencia e Innovacion (MICINN) of Spain; the Max Planck Gesellschaft, and the Deutsche Forschungsgemeinschaft DEG (SBH WI 2152), the Transregional Collaborative Research Center TR27, the excellence cluster "Origin and Structure of the Universe", and the Maier-Leibnitz-Laboratorium Garching in Germany; the Russian Academy of Science, the Kurchatov Institute and RFBR (the Russian Foundation for Basic Research); the Brazilian Ministry of Science, Technology and Innovation (MCTI), the Financiadora de Estudos c Projetos (FINEP), the Conselho Nacional de Desenvolvimento Cientifico e Tecnoleigico (CNPq), the Sao Paulo Research Foundation (FAPESP), and the Brazilian Network for High Energy Physics (RENAFAE) in Brazil. NR 15 TC 4 Z9 4 U1 1 U2 20 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0168-9002 EI 1872-9576 J9 NUCL INSTRUM METH A JI Nucl. Instrum. Methods Phys. Res. Sect. A-Accel. Spectrom. Dect. Assoc. Equip. PD NOV 11 PY 2014 VL 764 BP 330 EP 339 DI 10.1016/j.nima.2014.07.058 PG 10 WC Instruments & Instrumentation; Nuclear Science & Technology; Physics, Nuclear; Physics, Particles & Fields SC Instruments & Instrumentation; Nuclear Science & Technology; Physics GA AP3OT UT WOS:000341987000044 ER PT J AU Kaplan, AC Henzl, V Menloye, HO Swinhoe, MT Behan, AP Flaska, M Pozzi, SA AF Kaplan, Alexis C. Henzl, Vladimir Menlove, Howard O. Swinhoe, Martyn T. Belian, Anthony P. Flaska, Marek Pozzi, Sara A. TI Determination of total plutonium content in spent nuclear fuel assemblies with the differential die-away self-interrogation instrument SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT LA English DT Article DE Nondestructive assay; Plutonium measurement; DDSI; Spent fuel AB As a part of the Next Generation Safeguards Initiative Spent Fuel project, we simulate the response of the Differential Die-away Self-Interrogation (DDSI) instrument to determine total elemental plutonium content in an assayed spent nuclear fuel assembly (SFA). We apply recently developed concepts that relate total plutonium mass with SFA multiplication and passive neutron count rate. In this work, the multiplication of the SFA is determined from the die-away time in the early time domain of the Rossi-Alpha distributions measured directly by the DDSI instrument. We utilize MCNP to test the method against 44 pressurized water reactor SFAs from a simulated spent fuel library with a wide dynamic range of characteristic parameters such as initial enrichment, burnup, and cooling time. Under ideal conditions, discounting possible errors of a real world measurement, a root mean square agreement between true and determined total Pu mass of 2.1% is achieved. Published by Elsevier B.V. C1 [Kaplan, Alexis C.; Henzl, Vladimir; Menlove, Howard O.; Swinhoe, Martyn T.; Belian, Anthony P.] Los Alamos Natl Lab, Los Alamos, NM 87544 USA. [Kaplan, Alexis C.; Flaska, Marek; Pozzi, Sara A.] Univ Michigan, Dept Nucl Engn & Radiol Sci, Ann Arbor, MI 48109 USA. RP Kaplan, AC (reprint author), Los Alamos Natl Lab, POB 1663, Los Alamos, NM 87544 USA. FU U.S. Department of Homeland Security [2012-DN-130-NF0001-02]; Next Generation Safeguards Initiative (NGSI); Office of Nonproliferation and International Security (NIS); National Nuclear Security Administration (NNSA); U.S. Department of Homeland Security or the National Nuclear Security Administration [LA-UR-13-29465] FX This material is partially based upon work supported by the U.S. Department of Homeland Security under Grant award no, 2012-DN-130-NF0001-02. The authors also would like to acknowledge the support of the Next Generation Safeguards Initiative (NGSI), Office of Nonproliferation and International Security (NIS), the National Nuclear Security Administration (NNSA). The views and conclusions contained in this document are those of the authors and should not be interpreted as necessarily representing the official policies, either expressed or implied, of the U.S. Department of Homeland Security or the National Nuclear Security Administration, LA-UR-13-29465. NR 10 TC 0 Z9 0 U1 0 U2 10 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0168-9002 EI 1872-9576 J9 NUCL INSTRUM METH A JI Nucl. Instrum. Methods Phys. Res. Sect. A-Accel. Spectrom. Dect. Assoc. Equip. PD NOV 11 PY 2014 VL 764 BP 347 EP 351 DI 10.1016/j.nima.2014.08.003 PG 5 WC Instruments & Instrumentation; Nuclear Science & Technology; Physics, Nuclear; Physics, Particles & Fields SC Instruments & Instrumentation; Nuclear Science & Technology; Physics GA AP3OT UT WOS:000341987000046 ER PT J AU Barletta, W Battaglia, M Klute, M Mangano, M Prestemon, S Rossi, L Skands, P AF Barletta, William Battaglia, Marco Klute, Markus Mangano, Michelangelo Prestemon, Soren Rossi, Lucio Skands, Peter TI Future hadron colliders: From physics perspectives to technology R&D SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT LA English DT Article DE Future hadron colliders; Superconducting magnet technology; High energy proton beams ID CROSS-SECTIONS; LHC; NB3SN; COLLISIONS; PARTICLE; MAGNETS; BOSON AB High energy hadron colliders have been instrumental to discoveries in particle physics at the energy frontier and their role as discovery machines will remain unchallenged for the foreseeable future. The full exploitation of the WC is now the highest priority of the energy frontier collider program. This includes the high luminosity LHC project which is made possible by a successful technology readiness program for Nb3Sn superconductor and magnet engineering based on long-term high field magnet R&D programs. These programs open the path towards collisions with luminosity of 5 x 10(34) cm(-2) S-1 and represents the foundation to consider future proton colliders of higher energies. This paper discusses physics requirements, experimental conditions, technological aspects and design challenges for the development towards proton colliders of increasing energy and luminosity. (C) 2014 Elsevier B.V. All rights reserved. C1 [Barletta, William] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA. [Barletta, William; Klute, Markus] MIT, Dept Phys, Cambridge, MA 02139 USA. [Battaglia, Marco] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA. [Battaglia, Marco; Prestemon, Soren] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Battaglia, Marco; Mangano, Michelangelo; Rossi, Lucio; Skands, Peter] CERN, CH-1211 Geneva, Switzerland. RP Battaglia, M (reprint author), Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA. EM MBattaglia@lbl.gov NR 52 TC 12 Z9 12 U1 1 U2 11 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0168-9002 EI 1872-9576 J9 NUCL INSTRUM METH A JI Nucl. Instrum. Methods Phys. Res. Sect. A-Accel. Spectrom. Dect. Assoc. Equip. PD NOV 11 PY 2014 VL 764 BP 352 EP 368 DI 10.1016/j.nima.2014.07.010 PG 17 WC Instruments & Instrumentation; Nuclear Science & Technology; Physics, Nuclear; Physics, Particles & Fields SC Instruments & Instrumentation; Nuclear Science & Technology; Physics GA AP3OT UT WOS:000341987000047 ER PT J AU Vojta, D Matanovic, I Kovacevic, G Baranovic, G AF Vojta, Danijela Matanovic, Ivana Kovacevic, Goran Baranovic, Goran TI The study of secondary effects in vibrational and hydrogen bonding properties of 2-and 3-ethynylpyridine and ethynylbenzene by IR spectroscopy SO SPECTROCHIMICA ACTA PART A-MOLECULAR AND BIOMOLECULAR SPECTROSCOPY LA English DT Article DE Ethynylpyridine; Ethynylbenzene; Hydrogen bonding; IR wavenumber shifts; Anharmonic wavenumbers ID CENTER-DOT-N; AB-INITIO; PHENOL; PHENYLACETYLENE; COMPLEXES; PYRIDINE; METHANOL; SCALE; WATER; TETRACHLOROMETHANE AB Weak hydrogen bonds formed by 2- and 3-ethynylpyridine and ethynylbenzene with trimethylphosphate and phenol were characterized by IR spectroscopy and DFT calculations (B3LYP/6-311++G(d, p)). The structure and stability of ethynylpyridines and ethynylbenzene in the gas phase and in the complexes with trimethylphosphate and phenol are discussed in terms of geometry and electronic charge redistribution. Anharmonic effects are taken into account when calculating vibrational wavenumbers of these systems what lead to partial improvement of agreement with experiment. The changes in the electronic charge distribution are behind the frequency shifts of the C C stretching in opposite direction depending on the role the ethyne molecule has in a hydrogen bonded complex (Delta(nu) over tilde = +9 cm(-1) in trimethylphosphate complexes, Delta(nu) over tilde = -3 cm(-1) in phenol complexes). The association constants were determined by keeping the concentrations of proton donors approximately constant and low enough to avoid self-association and the proton acceptors were present in excess. The values obtained for the association constants and enthalpy changes in C2Cl4 (for trimethylphosphate complexes K approximate to 0.5-1.0 mol(-1) dm(3) and -Delta H-r(circle minus) approximate to 6-8 kJ mol(-1), for phenol complexes K approximate to 20-40 mol(-1) dm(3) -Delta H-r(circle minus) approximate to 17-22 kJ mol(-1)) are in good agreement with literature data. (C) 2014 Elsevier B.V. All rights reserved. C1 [Vojta, Danijela; Baranovic, Goran] Rudjer Boskovic Inst, Div Organ Chem & Biochem, Zagreb 10001, Croatia. [Matanovic, Ivana] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA. [Kovacevic, Goran] Rudjer Boskovic Inst, Div Mat Phys, Zagreb 10001, Croatia. RP Baranovic, G (reprint author), Rudjer Boskovic Inst, Div Organ Chem & Biochem, Bijenicka C 54, Zagreb 10001, Croatia. EM goran.baranovic@irb.hr FU Ministry of Science, Education and Sport of the Croatian Government [0982904-2927]; LANL LDRD program, U.S. Department of Energy, Energy Efficiency and Renewable Energy; U.S. Department of Energy [DE-AC52-06NA25396] FX This work was supported by a Grant No. 0982904-2927 from the Ministry of Science, Education and Sport of the Croatian Government. D. Vojta and G. Baranovic thank to J. Aleric and T. Parlic-Risovic from Croatian Metrology Institute for the measurements of densities of liquids. I. Matanovic thanks the LANL LDRD program for a postdoctoral fellowship, U.S. Department of Energy, Energy Efficiency and Renewable Energy for financial support. Los Alamos National Laboratory is operated by Los Alamos National Security, LLC for the National Nuclear Security Administration of the U.S. Department of Energy under contract DE-AC52-06NA25396. This paper has been designated LA-UR-12-26989. NR 36 TC 3 Z9 3 U1 0 U2 11 PU PERGAMON-ELSEVIER SCIENCE LTD PI OXFORD PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, ENGLAND SN 1386-1425 J9 SPECTROCHIM ACTA A JI Spectroc. Acta Pt. A-Molec. Biomolec. Spectr. PD NOV 11 PY 2014 VL 132 BP 215 EP 224 DI 10.1016/j.saa.2014.04.166 PG 10 WC Spectroscopy SC Spectroscopy GA AN1GN UT WOS:000340330800026 PM 24866088 ER PT J AU Fu, W Li, H Lubow, S Li, ST Liang, E AF Fu, Wen Li, Hui Lubow, Stephen Li, Shengtai Liang, Edison TI EFFECTS OF DUST FEEDBACK ON VORTICES IN PROTOPLANETARY DISKS SO ASTROPHYSICAL JOURNAL LETTERS LA English DT Article DE accretion, accretion disks; hydrodynamics; instabilities; protoplanetary disks ID ROSSBY-WAVE INSTABILITY; TRANSITIONAL DISKS; ACCRETION DISKS; GAP EDGES; PLANET; DISCS; DISTRIBUTIONS; SIMULATIONS; FILTRATION; PARTICLES AB We carried out two-dimensional, high-resolution simulations to study the effect of dust feedback on the evolution of vortices induced by massive planets in protoplanetary disks. Various initial dust to gas disk surface density ratios (0.001-0.01) and dust particle sizes (Stokes number 4 x 10(-4)-0.16) are considered. We found that while dust particles migrate inward, vortices are very effective at collecting them. When dust density becomes comparable to gas density within the vortex, a dynamical instability is excited and it alters the coherent vorticity pattern and destroys the vortex. This dust feedback effect is stronger with a higher initial dust/gas density ratio and larger dust grain. Consequently, we found that the disk vortex lifetime can be reduced up to a factor of 10. We discuss the implications of our findings on the survivability of vortices in protoplanetary disks and planet formation. C1 [Fu, Wen; Liang, Edison] Rice Univ, Dept Phys & Astron, Houston, TX 77005 USA. [Fu, Wen; Li, Hui; Li, Shengtai] Los Alamos Natl Lab, Los Alamos, NM 87545 USA. [Lubow, Stephen] Space Telescope Sci Inst, Baltimore, MD 21218 USA. RP Fu, W (reprint author), Rice Univ, Dept Phys & Astron, Houston, TX 77005 USA. EM wf5@rice.edu OI Li, Shengtai/0000-0002-4142-3080 FU LDRD program; UC laboratory fees research program; DOE/Office of Fusion Energy Science through CMSO at LANL; NASA [NNX11AK61G]; IGPP program FX Simulations in this work were performed using the Institutional Computing Facilities at LANL. We thank Geoffroy Lesur and Andrea Isella for helpful discussions. W.F., H.L., and S.L. gratefully acknowledge support by the LDRD and IGPP programs, the UC laboratory fees research program, and the DOE/Office of Fusion Energy Science through CMSO at LANL. W.F. and S.L. also acknowledge support from NASA grant NNX11AK61G. NR 31 TC 12 Z9 12 U1 1 U2 3 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 2041-8205 EI 2041-8213 J9 ASTROPHYS J LETT JI Astrophys. J. Lett. PD NOV 10 PY 2014 VL 795 IS 2 AR L39 DI 10.1088/2041-8205/795/2/L39 PG 7 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AU3FY UT WOS:000345499000015 ER PT J AU Lee, J Prasankumar, RP AF Lee, Jinho Prasankumar, Rohit P. TI Correlation between quantum charge fluctuations and magnetic ordering in multiferroic LuFe2O4 SO EUROPEAN PHYSICAL JOURNAL B LA English DT Article AB We examine the interplay between quantum charge fluctuations and magnetic ordering in multiferroic LuFe2O4 and show that this can couple spin and charge degrees of freedom in a LuFe2O4 bilayer below the Neel temperature T-N. Our analysis supports the idea that the double exchange mechanism normally used in metallic systems can be applied to charge-ordered insulators. This causes ferrimagnetic spin order to reduce the transfer integrals between Fe2+ and Fe3+ in LuFe2O4, decreasing charge fluctuations and increasing the polarization in this system below T-N. This work thus provides a more detailed understanding of the mechanism for spin-charge coupling in LuFe2O4. C1 [Lee, Jinho; Prasankumar, Rohit P.] Los Alamos Natl Lab, Ctr Integrated Nanotechnol, Los Alamos, NM 87545 USA. RP Lee, J (reprint author), Los Alamos Natl Lab, Ctr Integrated Nanotechnol, POB 1663, Los Alamos, NM 87545 USA. EM rpprasan@lanl.gov FU LANL Laboratory Directed Research and Development Program; National Nuclear Security administration of the U.S. Department of Energy [DE-AC52-06NA25396] FX The authors would like to acknowledge Dr. S. A. Trugman, Dr. C. D. Batista, Dr. D. A. Yarotski, and Dr. A.J. Taylor of Los Alamos National Laboratory, Prof. D. Talbayev at Tulane University, Dr. C. L. Zhang and Prof. S.-W. Cheong at Rutgers University, and Prof. X. S. Xu at the University of Nebraska for their contributions to this work. This work was performed at the Center for Integrated Nanotechnologies, a US Department of Energy, Office of Basic Energy Sciences (BES) user facility and was also supported by the LANL Laboratory Directed Research and Development Program. Los Alamos National Laboratory, an affirmative action equal opportunity employer, is operated by Los Alamos National Security, LLC, for the National Nuclear Security administration of the U.S. Department of Energy under Contract No. DE-AC52-06NA25396. NR 17 TC 2 Z9 2 U1 2 U2 31 PU SPRINGER PI NEW YORK PA 233 SPRING ST, NEW YORK, NY 10013 USA SN 1434-6028 EI 1434-6036 J9 EUR PHYS J B JI Eur. Phys. J. B PD NOV 10 PY 2014 VL 87 IS 11 AR 267 DI 10.1140/epjb/e2014-50177-2 PG 5 WC Physics, Condensed Matter SC Physics GA AT5WK UT WOS:000345010400004 ER PT J AU Adamczyk, L Guryn, W Turnau, J AF Adamczyk, Leszek Guryn, Wlodek Turnau, Jacek TI Central exclusive production at RHIC SO INTERNATIONAL JOURNAL OF MODERN PHYSICS A LA English DT Article DE Diffraction; QCD; exotics ID REACTION POMERON-POMERON; 450 GEV/C; GLUEBALLS AB The present status and future plans of the physics program of Central Exclusive Production (CEP) at RHIC are described. The measurements are based on the detection of the forward protons from the Double Pomeron Exchange (DPE) process in the Roman Pot system and of the recoil system of charged particles from the DPE process measured in the STAR experiment's Time Projection Chamber (TPC). The data described here were taken using polarized proton-proton collisions at root s = 200 GeV. The preliminary spectra of two-pion mass reconstructed by STAR TPC in central region of pseudorapidity vertical bar eta vertical bar < 1, are presented. Near future plans to take data with the current system at center-of-mass energy root s = 200 GeV and plans to upgrade the forward proton tagging system are presented. Also a possible addition of the RPs to the sPHENIX detector is discussed. C1 [Adamczyk, Leszek] AGH Univ Sci & Technol, Fac Phys & Appl Comp Sci, PL-30059 Krakow, Poland. [Guryn, Wlodek] Brookhaven Natl Lab, Upton, NY 11973 USA. [Turnau, Jacek] Inst Nucl Phys, PL-31342 Krakow, Poland. RP Adamczyk, L (reprint author), AGH Univ Sci & Technol, Fac Phys & Appl Comp Sci, PL-30059 Krakow, Poland. EM Leszek.Adamczyk@agh.edu.pl; guryn@bnl.gov; Jacek.Turnau@ifj.edu.pl FU Office of NP within the U.S. DOE Office of Science; Polish National Science Centre [UMO-2011/01/M/ST2/04126] FX This work was supported in part by the Office of NP within the U.S. DOE Office of Science and by the Polish National Science Centre under contract UMO-2011/01/M/ST2/04126. We also thank our colleagues from the Ultraperipheral Collisions Physics Working Group at STAR for many helpful discussions. NR 26 TC 10 Z9 10 U1 0 U2 2 PU WORLD SCIENTIFIC PUBL CO PTE LTD PI SINGAPORE PA 5 TOH TUCK LINK, SINGAPORE 596224, SINGAPORE SN 0217-751X EI 1793-656X J9 INT J MOD PHYS A JI Int. J. Mod. Phys. A PD NOV 10 PY 2014 VL 29 IS 28 SI SI AR 1446010 DI 10.1142/S0217751X14460105 PG 8 WC Physics, Nuclear; Physics, Particles & Fields SC Physics GA AU3LU UT WOS:000345515500011 ER PT J AU Albrow, M AF Albrow, Michael CA CDF Collaboration TI Central exclusive production at the Tevatron SO INTERNATIONAL JOURNAL OF MODERN PHYSICS A LA English DT Article DE QCD; diffraction; charmonia ID MESON PAIR PRODUCTION; HADRON COLLIDERS AB The Collider Detector at Fermilab, CDF, observed for the first time in hadron-hadron collisions photon-photon (gamma + gamma -> e(+)e(-), mu(+)mu(-)) and photon-pomeron (gamma + P -> J/psi, psi(2S)) interactions, as well as p + (p) over bar -> p + chi(c) + (p) over bar by double pomeron exchange, P + P or DPE. Exclusive pi(+)pi(-) production was also measured at root s = 900 GeV and 1960 GeV; resonance structures are discussed. C1 [Albrow, Michael; CDF Collaboration] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA. RP Albrow, M (reprint author), Fermilab Natl Accelerator Lab, POB 500,Wilson Rd, Batavia, IL 60510 USA. EM albrow@fnal.gov NR 36 TC 4 Z9 4 U1 0 U2 1 PU WORLD SCIENTIFIC PUBL CO PTE LTD PI SINGAPORE PA 5 TOH TUCK LINK, SINGAPORE 596224, SINGAPORE SN 0217-751X EI 1793-656X J9 INT J MOD PHYS A JI Int. J. Mod. Phys. A PD NOV 10 PY 2014 VL 29 IS 28 SI SI AR 1446009 DI 10.1142/S0217751X14460099 PG 14 WC Physics, Nuclear; Physics, Particles & Fields SC Physics GA AU3LU UT WOS:000345515500010 ER PT J AU Albrow, M AF Albrow, Michael TI Central exclusive production issue: Introduction SO INTERNATIONAL JOURNAL OF MODERN PHYSICS A LA English DT Article DE QCD; diffraction; pomeron; glueball AB I give a brief introduction to central exclusive production in hadron-hadron collisions, the subject of this special issue of the International Journal of Modern Physics A. C1 Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA. RP Albrow, M (reprint author), Fermilab Natl Accelerator Lab, POB 500,Wilson Rd, Batavia, IL 60510 USA. EM albrow@fnal.gov FU US Department of Energy through Fermilab FX I acknowledge with thanks Valery Khoze and Christophe Royon, co-editors of this special edition, and all the authors of the contributed papers. I also acknowledge support from the US Department of Energy through Fermilab. NR 20 TC 3 Z9 3 U1 0 U2 1 PU WORLD SCIENTIFIC PUBL CO PTE LTD PI SINGAPORE PA 5 TOH TUCK LINK, SINGAPORE 596224, SINGAPORE SN 0217-751X EI 1793-656X J9 INT J MOD PHYS A JI Int. J. Mod. Phys. A PD NOV 10 PY 2014 VL 29 IS 28 SI SI AR 1402006 DI 10.1142/S0217751X14020060 PG 4 WC Physics, Nuclear; Physics, Particles & Fields SC Physics GA AU3LU UT WOS:000345515500001 ER PT J AU Albrow, M AF Albrow, Michael TI Double pomeron exchange at the CERN Intersecting Storage Rings and Sp(p)over-barS Collider SO INTERNATIONAL JOURNAL OF MODERN PHYSICS A LA English DT Article DE QCD; diffraction; pomeron; glueball ID PP COLLISIONS; GEV-C; ISR; SCATTERING; ENERGIES; SEARCH; MODEL AB The CERN Intersecting Storage Rings, with root s(pp) from 22 GeV to 63 GeV and root s(alpha alpha) = 126 GeV, allowed the first observations of p + p -> p + X + p with two leading protons (x(F) > 0.95) or two rapidity gaps Delta y > 3. Studies of the central hadronic system (X) were made to search for glueballs, finding f(0) and f(2) resonances, and to advance our understanding of hadronic diffraction. I review the experiments, not including those at the Split Field Magnet (SFM) facility covered elsewhere in this volume. Some double pomeron exchange studies at the CERN Sp (p) over barS Collider are also covered. C1 Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA. RP Albrow, M (reprint author), Fermilab Natl Accelerator Lab, POB 500,Wilson Rd, Batavia, IL 60510 USA. EM albrow@fnal.gov NR 34 TC 3 Z9 3 U1 0 U2 0 PU WORLD SCIENTIFIC PUBL CO PTE LTD PI SINGAPORE PA 5 TOH TUCK LINK, SINGAPORE 596224, SINGAPORE SN 0217-751X EI 1793-656X J9 INT J MOD PHYS A JI Int. J. Mod. Phys. A PD NOV 10 PY 2014 VL 29 IS 28 SI SI AR 1446014 DI 10.1142/S0217751X14460142 PG 11 WC Physics, Nuclear; Physics, Particles & Fields SC Physics GA AU3LU UT WOS:000345515500015 ER PT J AU Albrow, M Collins, P Penzo, A AF Albrow, Michael Collins, Paula Penzo, Aldo CA FSC Team CMS Collaboration HERSCHEL Team LHCb Collaboration TI Forward shower counters for diffractive physics at the LHC SO INTERNATIONAL JOURNAL OF MODERN PHYSICS A LA English DT Article DE QCD; diffraction; pomeron AB The LHC detectors have incomplete angular coverage in the forward direction, for example in the region 6 less than or similar to vertical bar eta vertical bar less than or similar to 8, which can be improved with the addition of simple scintillation counters around the beam pipes about 50 m to 120 m from the intersection point. These counters detect showers created by particles hitting the beam pipes and nearby material. The absence of signals in these counters in low pileup conditions is an indication of a forward rapidity gap as a signature of diffraction. In addition, they can be used to detect hadrons from low mass diffractive excitations of the proton, not accompanied by a leading proton but adjacent to a rapidity gap over (e. g.) 3 less than or similar to vertical bar eta vertical bar less than or similar to 6. Such a set of forward shower counters, originally used at CDF, was used in CMS (FSC) for high-beta* running with TOTEM during LHC Run-1. During LS1 the CMS FSC system is being upgraded for future low pileup runs. A similar system, called HERSCHEL is being installed in LHCb. ALICE is implementing scintillation counters, ADA and ADC, with 4.5 less than or similar to vertical bar eta vertical bar less than or similar to 6.4. C1 [Albrow, Michael] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA. [Collins, Paula] CERN, PH Div, CH-1211 Geneva 23, Switzerland. [Penzo, Aldo] Ist Nazl Fis Nucl, Area Ric, I-34149 Trieste, Italy. [Penzo, Aldo] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA. RP Albrow, M (reprint author), Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA. EM albrow@fnal.gov; Paula.Collins@cern.ch; Aldo.Penzo@ts.infn.it NR 17 TC 5 Z9 5 U1 1 U2 2 PU WORLD SCIENTIFIC PUBL CO PTE LTD PI SINGAPORE PA 5 TOH TUCK LINK, SINGAPORE 596224, SINGAPORE SN 0217-751X EI 1793-656X J9 INT J MOD PHYS A JI Int. J. Mod. Phys. A PD NOV 10 PY 2014 VL 29 IS 28 SI SI AR 1446018 DI 10.1142/S0217751X1446018X PG 11 WC Physics, Nuclear; Physics, Particles & Fields SC Physics GA AU3LU UT WOS:000345515500019 ER PT J AU Bjorken, JD AF Bjorken, J. D. TI Double diffraction at zero impact parameter SO INTERNATIONAL JOURNAL OF MODERN PHYSICS A LA English DT Article DE QCD; diffraction AB Protons may sometimes have the configuration of a compact diquark, separated transversely from the quark by a string. If both protons in a collision have this form, the strings may be parallel, giving final states with high multiplicity, ellipticity and a ridge structure, or transverse, with leading protons and (sometimes) rapidity gaps. Simple considerations lead one to expect, at root s(pp) approximate to 100 GeV, central masses in the few GeV/c(2) range, appropriate for glueball states. C1 Stanford Linear Accelerator Ctr, Stanford, CA 94309 USA. RP Bjorken, JD (reprint author), Stanford Linear Accelerator Ctr, Stanford, CA 94309 USA. EM bjorken@slac.stanford.edu NR 2 TC 2 Z9 2 U1 3 U2 3 PU WORLD SCIENTIFIC PUBL CO PTE LTD PI SINGAPORE PA 5 TOH TUCK LINK, SINGAPORE 596224, SINGAPORE SN 0217-751X EI 1793-656X J9 INT J MOD PHYS A JI Int. J. Mod. Phys. A PD NOV 10 PY 2014 VL 29 IS 28 SI SI AR 1446006 DI 10.1142/S0217751X14460063 PG 4 WC Physics, Nuclear; Physics, Particles & Fields SC Physics GA AU3LU UT WOS:000345515500007 ER PT J AU Gutierrez, G Reyes, MA AF Gutierrez, Gaston Reyes, Marco A. TI Fixed target experiments at the Fermilab Tevatron SO INTERNATIONAL JOURNAL OF MODERN PHYSICS A LA English DT Article DE Glueballs; exotics; double pomeron exchange ID SPIN-PARITY ANALYSIS; PHI-MESON PRODUCTION; K-P INTERACTIONS; 300 GEV/C; SYSTEM; STATISTICS; STATES; MODEL AB This paper presents a review of the study of Exclusive Central Production at a center-of- mass energy of root s = 40 GeV at the Fermilab Fixed Target program. In all reactions reviewed in this paper, protons with an energy of 800 GeV were extracted from the Tevatron accelerator at Fermilab and directed to a Liquid Hydrogen target. The states reviewed include pi(+) pi(-), K-s(0) K-s(0), K-s(0) K-+/- pi(inverted perpendicular), phi phi and D*(+/-). Partial Wave Analysis results will be presented on the light states but only the cross-section will be reviewed in the diffractive production of D*(+/-). C1 [Gutierrez, Gaston] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA. [Reyes, Marco A.] Univ Guanajuato, Dept Phys, Guanajuato 37150, Mexico. RP Gutierrez, G (reprint author), Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA. EM gaston@fnal.gov; marco@fisica.ugto.mx FU US Department of Energy; CONACYT Mexico FX We would like to thank many people who provided information about the Fermilab FT program. This work was funded by the US Department of Energy and CONACYT Mexico. M. A. Reyes would like to thank CONACYT for supporting a sabbatical stay at Fermilab while this paper was being written. NR 44 TC 4 Z9 4 U1 1 U2 2 PU WORLD SCIENTIFIC PUBL CO PTE LTD PI SINGAPORE PA 5 TOH TUCK LINK, SINGAPORE 596224, SINGAPORE SN 0217-751X EI 1793-656X J9 INT J MOD PHYS A JI Int. J. Mod. Phys. A PD NOV 10 PY 2014 VL 29 IS 28 SI SI AR 1446008 DI 10.1142/S0217751X14460087 PG 12 WC Physics, Nuclear; Physics, Particles & Fields SC Physics GA AU3LU UT WOS:000345515500009 ER PT J AU Aad, G Abbott, B Abdallah, J Khalek, SA Abdinov, O Aben, R Abi, B Abolins, M AbouZeid, OS Abramowicz, H Abreu, H Abreu, R Abulaiti, Y Acharya, BS Adamczyk, L Adams, DL Adelman, J Adomeit, S Adye, T Agatonovic-Jovin, T Aguilar-Saavedra, JA Agustoni, M Ahlen, SP Ahmadov, F Aielli, G Akerstedt, H Akesson, TPA Akimoto, G Akimov, AV Alberghi, GL Albert, J Albrand, S AlconadaVerzini, MJ Aleksa, M Aleksandrov, IN Alexa, C Alexander, G Alexandre, G Alexopoulos, T Alhroob, M Alimonti, G Alio, L Alison, J Allbrooke, BMM Allison, LJ Allport, PP Almond, J Aloisio, A Alonso, A Alonso, F Alpigiani, C Altheimer, A Gonzalez, BA Alviggi, MG Amako, K Coutinho, YA Amelung, C Amidei, D Dos Santos, SPA Amorim, A Amoroso, S Amram, N Amundsen, G Anastopoulos, C Ancu, LS Andari, N Andeen, T Anders, CF Anders, G Anderson, KJ Andreazza, A Andrei, V Anduaga, XS Angelidakis, S Angelozzi, I Anger, P Angerami, A Anghinolfi, F Anisenkov, AV Anjos, N Annovi, A Antonaki, A Antonelli, M Antonov, A Antos, J Anulli, F Aoki, M Bella, LA Apolle, R Arabidze, G Aracena, I Arai, Y Araque, JP Arce, ATH Arguin, JF Argyropoulos, S Arik, M Armbruster, AJ Arnaez, O Arnal, V Arnold, H Arratia, M Arslan, O Artamonov, A Artoni, G Asai, S Asbah, N Ashkenazi, A Asman, B Asquith, L Assamagan, K Astalos, R Atkinson, M Atlay, NB Auerbach, B Augsten, K Aurousseau, M Avolio, G Azuelos, G Azuma, Y Baak, MA Bacci, C Bachacou, H Bachas, K Backes, M Backhaus, M Mayes, JB Badescu, E Bagiacchi, P Bagnaia, P Bai, Y Bain, T Baines, JT Baker, OK Baker, S Balek, P Balli, F Banas, E Banerjee, S Bannoura, AAE Bansal, V Bansil, HS Barak, L Baranov, SP Barberio, EL Barberis, D Barbero, M Barillari, T Barisonzi, M Barklow, T Barlow, N Barnett, BM Barnett, RM Barnovska, Z Baroncelli, A Barone, G Barr, AJ Barreiro, F da Costa, JBG Bartoldus, R Barton, AE Bartos, P Bartsch, V Bassalat, A Basye, A Bates, RL Batkova, L Batley, JR Battaglia, M Battistin, M Bauer, F Bawa, HS Beau, T Beauchemin, PH Beccherle, R Bechtle, P Beck, HP Becker, K Becker, S Beckingham, M Becot, C Beddall, AJ Beddall, A Bedikian, S Bednyakov, VA Bee, CP Beemster, LJ Beermann, TA Begel, M Behr, K Belanger-Champagne, C Bell, PJ Bell, WH Bella, G Bellagamba, L Bellerive, A Bellomo, M Belotskiy, K Beltramello, O Benary, O Benchekroun, D Bendtz, K Benekos, N Benhammou, Y Noccioli, EB Garcia, JAB Benjamin, DP Bensinger, JR Benslama, K Bentvelsen, S Berge, D Kuutmann, EB Berger, N Berghaus, F Berglund, E Beringer, J Bernard, C Bernat, P Bernius, C Bernlochner, FU Berry, T Berta, P Bertella, C Bertolia, G Bertolucci, F Bertsche, D Besana, MI Besjes, GJ Bessidskaia, O Bessner, MF Besson, N Betancourt, C Bethke, S Bhimji, W Bianchi, RM Bianchini, L Bianco, M Biebel, O Bieniek, SP Bierwagen, K Biesiada, J Biglietti, M De Mendizabal, JB Bilokon, H Bindi, M Binet, S Bingul, A 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CA Atlas Collaboration TI Measurement of the cross section of high transverse momentum Z -> b(b)over-bar production in proton-proton collisions at root s=8 TeV with the ATLAS detector SO PHYSICS LETTERS B LA English DT Article DE LHC; Boosted b(b)over-bar topologies ID TEVATRON; PAIR AB This Letter reports the observation of a high transverse momentum Z -> b (b) over bar signal in proton-proton collisions at root s = 8TeVand the measurement of its production cross section. The data analysed were collected in 2012 with the ATLAS detector at the LHC and correspond to an integrated luminosity of 19.5 fb(-1). The Z -> b (b) over bar decay is reconstructed from a pair of b-tagged jets, clustered with the anti- k(t) jet algorithm with R = 0.4, that have low angular separation and form a dijet with p(T) > 200 GeV. The signal yield is extracted from a fit to the dijet invariant mass distribution, with the dominant, multi-jet background mass shape estimated by employing a fully data-driven technique that reduces the dependence of the analysis on simulation. The fiducial cross section is determined to be sigma(fid)(Z -> b (b) over bar) = 2.02 +/- 0.20 (stat.) +/- 0.25 (syst.) +/- 0.06 (lumi.) pb = 2.02 +/- 0.33 pb, in good agreement with next-to-leading-order theoretical predictions. Published by Elsevier B.V. C1 [Jackson, P.; Soni, N.; White, M. J.] Univ Adelaide, Dept Phys, Adelaide, SA, Australia. [Bouffard, J.; Edson, W.; Ernst, J.; Guindon, S.; Jain, V.] SUNY Albany, Dept Phys, Albany, NY 12222 USA. [Butt, A. I.; Chan, K.; Czodrowski, P.; Gingrich, D. M.; Moore, R. W.; Pinfold, J. L.; Saddique, A.; Sbrizzi, A.; Subramania, H. S.; Vaque, F. Vives] Univ Alberta, Dept Phys, Edmonton, AB, Canada. [Cakir, O.; Ciftci, A. K.; Ciftci, R.; Yildiz, H. 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[Alexa, C.; Badescu, E.; Boldea, V.; Buda, S. I.; Caprini, I.; Caprini, M.; Chitan, A.; Ciubancan, M.; Constantinescu, S.; Cuciuc, C. -M.; Dita, P.; Dita, S.; Ducu, O. A.; Jinaru, A.; Maurer, J.; Olariu, A.; Pantea, D.; Popeneciu, G. A.; Rotaru, M.; Stoicea, G.; Tudorache, A.; Tudorache, V.] Natl Inst Phys & Nucl Engn, Bucharest, Romania. [Popeneciu, G. A.] Natl Inst Res & Dev Isotop & Mol Technol, Dept Phys, Cluj Napoca, Romania. Univ Politehn Bucuresti, Bucharest, Romania. West Univ Timisoara, Timisoara, Romania. [Gonzalez Silva, M. L.; Otero y Garzon, G.; Piegaia, R.; Reisin, H.; Romeo, G.; Sacerdoti, S.] Univ Buenos Aires, Dept Fis, Buenos Aires, DF, Argentina. [Arratia, M.; Barlow, N.; Batley, J. R.; Brochu, F. M.; Buttinger, W.; Carter, J. R.; Chapman, J. D.; Cottin, G.; French, S. T.; Frost, J. A.; Gillam, T. P. S.; Hill, J. C.; Kaneti, S.; Khoo, T. J.; Lester, C. G.; Moeller, V.; Mueller, T.; Parker, M. A.; Robinson, D.; Sandoval, T.; Thomson, M.; Ward, C. 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Fernandez; Franchino, S.; Francis, D.; Froidevaux, D.; Garonne, V.; Gianotti, F.; Gillberg, D.; Glatzer, J.; Godlewski, J.; Goossens, L.; Gorini, B.; Gray, H. M.; Hauschild, M.; Hawkings, R. J.; Heller, M.; Helsens, C.; Correia, A. M. Henriques; Hervas, L.; Hoecker, A.; Hubacek, Z.; Huhtinen, M.; Jaekel, M. R.; Jakobsen, S.; Jansen, H.; Jenni, P.; Jungst, R. M.; Kaneda, M.; Klioutchnikova, T.; Krasznahorkay, A.; Lantzsch, K.; Lassnig, M.; Miotto, G. Lehmann; Lenzi, B.; Lichard, P.; Macina, D.; Malyukov, S.; Mandelli, B.; Mapelli, L.; Martin, B.; Marzin, A.; Messina, A.; Meyer, J.; Mornacchi, G.; Nairz, A. M.; Nakahama, Y.; Negri, G.; Nessi, M.; Nicquevert, B.; Nordberg, M.; Ohm, C. C.; Palestini, S.; Pauly, T.; Pernegger, H.; Peters, K.; Pommes, K.; Poppleton, A.; Poulard, G.; Prasad, S.; Rammensee, M.; Raymond, M.; Rembser, C.; Rodrigues, L.; Roe, S.; Ruiz-Martinez, A.; Salzburger, A.; Savu, D. O.; Schlenker, S.; Schmieden, K.; Serfon, C.; Sfyrla, A.; Solans, C. A.; Spigo, G.; Stelzer, H. J.; Teischinger, F. A.; Ten Kate, H.; Tremblet, L.; Tricoli, A.; Tsarouchas, C.; Unal, G.; van der Ster, D.; van Eldik, N.; van Woerden, M. C.; Vandelli, W.; Vigne, R.; Voss, R.; Vuillermet, R.; Wells, P. S.; Wengler, T.; Wenig, S.; Werner, P.; Wilkens, H. G.; Wotschack, J.; Young, C. J. S.; Zwalinski, L.] CERN, Geneva, Switzerland. [Alison, J.; Anderson, K. J.; Boveia, A.; Cheng, Y.; Facini, G.; Fiascaris, M.; Gardner, R. W.; Ilchenko, Y.; Kapliy, A.; Li, H. L.; Meehan, S.; Melachrinos, C.; Merritt, F. S.; Meyer, C.; Miller, D. W.; Okumura, Y.; Onyisi, P. U. E.; Oreglia, M. J.; Penning, B.; Pilcher, J. E.; Shochet, M. J.; Tompkins, L.; Vukotic, I.; Webster, J. S.] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA. [Carquin, E.; Diaz, M. A.; Vogel, M.] Pontificia Univ Catolica Chile, Dept Fis, Santiago, Chile. [Brooks, W. K.; Kuleshov, S.; Pezoa, R.; Prokoshin, F.; White, R.] Univ Tecn Federico Santa Maria, Dept Fis, Valparaiso, Chile. [Bai, Y.; Fang, Y.; Jin, S.; Lu, F.; Ouyang, Q.; Ren, H.; Shan, L. Y.; Sun, X.; Wanga, J.; Xu, D.; Yao, L.; Zhu, H.; Zhuang, X.] Chinese Acad Sci, Inst High Energy Phys, Beijing, Peoples R China. [Gao, J.; Guan, L.; Han, L.; Jiang, Y.; Li, B.; Liu, J. B.; Liu, K.; Liu, M.; Liu, Y.; Peng, H.; Song, H. Y.; Xu, L.; Zhao, Z.; Zhu, Y.] Univ Sci & Technol China, Dept Modern Phys, Hefei, Anhui, Peoples R China. [Chen, S.; Li, Y.; Wang, C.] Nanjing Univ, Dept Phys, Nanjing, Jiangsu, Peoples R China. Shandong Univ, Sch Phys, Jinan, Shandong, Peoples R China. [Li, L.; Yang, H.] Shanghai Jiao Tong Univ, Dept Phys, Shanghai 200030, Peoples R China. [Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Donini, J.; Dubreuil, E.; Ghodbane, N.; Gilles, G.; Gris, Ph.; Guicheney, C.; Liao, H.; Pallin, D.; Hernandez, D. Paredes; Podlyski, F.; Santoni, C.; Theveneaux-Pelzer, T.; Valery, L.; Vazeille, F.] Clermont Univ, Phys Corpusculaire Lab, Clermont Ferrand, France. [Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Donini, J.; Dubreuil, E.; Ghodbane, N.; Gilles, G.; Gris, Ph.; Guicheney, C.; Liao, H.; Pallin, D.; Hernandez, D. Paredes; Podlyski, F.; Santoni, C.; Theveneaux-Pelzer, T.; Valery, L.; Vazeille, F.] Univ Clermont Ferrand, Clermont Ferrand, France. [Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Donini, J.; Dubreuil, E.; Ghodbane, N.; Gilles, G.; Gris, Ph.; Guicheney, C.; Liao, H.; Pallin, D.; Hernandez, D. Paredes; Podlyski, F.; Santoni, C.; Theveneaux-Pelzer, T.; Valery, L.; Vazeille, F.] CNRS, IN2P3, Clermont Ferrand, France. [Altheimer, A.; Andeen, T.; Angerami, A.; Bain, T.; Brooijmans, G.; Chen, Y.; Cole, B.; Guo, J.; Hu, D.; Hughes, E. W.; Mohapatra, S.; Nikiforou, N.; Parsons, J. A.; Reale, V. Perez; Scherzer, M. I.; Thompson, E. N.; Tian, F.; Tuts, P. M.; Urbaniec, D.; Wulf, E.; Zhou, L.] Columbia Univ, Nevis Lab, Irvington, NY USA. [Alonso, A.; Dam, M.; Galster, G.; Hansen, J. B.; Hansen, J. D.; Hansen, P. H.; Heisterkamp, S.; Joergensen, M. D.; Loevschall-Jensen, A. E.; Mehlhase, S.; Monk, J.; Petersen, T. C.; Pingel, A.; Simonyan, M.; Thomsen, L. A.; Wiglesworth, C.; Xella, S.] Univ Copenhagen, Niels Bohr Inst, DK-2100 Copenhagen, Denmark. [Capua, M.; Crosetti, G.; La Rotonda, L.; Mastroberardino, A.; Policicchio, A.; Salvatore, D.; Schioppa, M.; Susinno, G.; Tassi, E.] Univ Calabria, Ist Nazl Fis Nucl, Lab Nazl Frascati, Grp Collegato Cosenza, I-87036 Arcavacata Di Rende, Italy. [Capua, M.; Crosetti, G.; La Rotonda, L.; Mastroberardino, A.; Policicchio, A.; Salvatore, D.; Schioppa, M.; Susinno, G.; Tassi, E.] Univ Calabria, Dipartimento Fis, I-87036 Arcavacata Di Rende, Italy. [Adamczyk, L.; Bold, T.; Dabrowski, W.; Dwuznik, M.; Dyndal, M.; Goulette, M. P.; Grabowska-Bold, I.; Kisielewska, D.; Koperny, S.; Kowalski, T. Z.; Mindur, B.; Palka, M.; Przybycien, M.; Zemla, A.] AGH Univ Sci & Technol, Fac Phys & Appl Comp Sci, Krakow, Poland. [Palka, M.] Jagiellonian Univ, Marian Smoluchowski Inst Phys, Krakow, Poland. [Banas, E.; de Renstrom, P. A. Bruckman; Chwastowski, J. J.; Derendarz, D.; Gornicki, E.; Hajduk, Z.; Iwanski, W.; Kaczmarska, A.; Korcyl, K.; Malecki, Pa.; Olszewski, A.; Olszowska, J.; Stanecka, E.; Staszewski, R.; Trzebinski, M.; Trzupek, A.; Wolter, M. W.; Wosiek, B. K.; Wozniak, K. W.; Zabinski, B.] Polish Acad Sci, Henryk Niewodniczanski Inst Nucl Phys, Krakow, Poland. [Cao, T.; Firan, A.; Hoffman, J.; Kama, S.; Kehoe, R.; Randle-Conde, A. S.; Sekula, S. J.; Stroynowski, R.; Wang, H.; Ye, J.] So Methodist Univ, Dept Phys, Dallas, TX 75275 USA. [Izen, J. M.; Leyton, M.; Lou, X.; Namasivayam, H.; Reeves, K.] Univ Texas Dallas, Dept Phys, Richardson, TX 75083 USA. [Argyropoulos, S.; Asbah, N.; Bessner, M. F.; Bloch, I.; Borroni, S.; Camarda, S.; Dassoulas, J. A.; Deterre, C.; Dietrich, J.; Filipuzzi, M.; Friedrich, C.; Glazov, A.; Fajardo, L. S. Gomez; Grahn, K. -J.; Gregor, I. M.; Grohsjean, A.; Haleem, M.; Hamnett, P. G.; Hengler, C.; Hiller, K. H.; Howarth, J.; Huang, Y.; Belenguer, M. Jimenez; Katzy, J.; Keller, J. S.; Kondrashova, N.; Kuhl, T.; Lange, C.; Lisovyi, M.; Lobodzinska, E.; Lohwasser, K.; Medinnis, M.; Moenig, K.; Naumann, T.; Peschke, R.; Petit, E.; Radescu, V.; Rubinskiy, I.; Schaefer, R.; Sedov, G.; Shushkevich, S.; South, D.; Stanescu-Bellu, M.; Stanitzki, M. M.; Starovoitov, P.; Styles, N. A.; Tackmann, K.; Vankov, P.; Wang, J.; Wasicki, C.; Wildt, M. A.; Yatsenko, E.; Yildirim, E.] DESY, Hamburg, Germany. [Argyropoulos, S.; Asbah, N.; Bessner, M. F.; Bloch, I.; Borroni, S.; Camarda, S.; Dassoulas, J. A.; Deterre, C.; Dietrich, J.; Filipuzzi, M.; Friedrich, C.; Glazov, A.; Fajardo, L. S. Gomez; Grahn, K. -J.; Gregor, I. M.; Grohsjean, A.; Haleem, M.; Hamnett, P. G.; Hengler, C.; Hiller, K. H.; Howarth, J.; Huang, Y.; Belenguer, M. Jimenez; Katzy, J.; Keller, J. S.; Kondrashova, N.; Kuhl, T.; Lange, C.; Lisovyi, M.; Lobodzinska, E.; Lohwasser, K.; Medinnis, M.; Moenig, K.; Naumann, T.; Peschke, R.; Petit, E.; Radescu, V.; Rubinskiy, I.; Schaefer, R.; Sedov, G.; Shushkevich, S.; South, D.; Stanescu-Bellu, M.; Stanitzki, M. M.; Starovoitov, P.; Styles, N. A.; Tackmann, K.; Vankov, P.; Wang, J.; Wasicki, C.; Wildt, M. A.; Yatsenko, E.; Yildirim, E.] DESY, Zeuthen, Germany. [Burmeister, I.; Esch, H.; Goessling, C.; Jentzsch, J.; Jung, C. A.; Klingenberg, R.; Wittig, T.] Tech Univ Dortmund, Inst Expt Phys 4, Dortmund, Germany. [Anger, P.; Friedrich, F.; Grohs, J. P.; Gumpert, C.; Kobel, M.; Leonhardt, K.; Mader, W. F.; Morgenstern, M.; Rudolph, C.; Schnoor, U.; Siegert, F.; Socher, F.; Staerz, S.; Straessner, A.; Vest, A.; Wahrmund, S.] Tech Univ Dresden, Inst Kern & Teilchenphys, D-01062 Dresden, Germany. [Arce, A. T. H.; Benjamin, D. P.; Bocci, A.; Cerio, B.; Kajomovitz, E.; Kotwal, A.; Kruse, M. C.; Li, L.; Li, S.; Liu, M.; Oh, S. H.; Pollard, C. S.; Wang, C.] Duke Univ, Dept Phys, Durham, NC 27706 USA. [Bhimji, W.; Bristow, T. M.; Clark, P. J.; Debenedetti, C.; Edwards, N. C.; Walls, F. M. Garay; Glaysher, P. C. F.; Harrington, R. D.; Martin, V. J.; Mills, C.; O'Brien, B. J.; Pino, S. A. Olivares; Proissl, M.; Selbach, K. E.; Smart, B. H.; Washbrook, A.; Wynne, B. M.] Univ Edinburgh, Sch Phys & Astron, SUPA, Edinburgh, Midlothian, Scotland. [Annovi, A.; Antonelli, M.; Bilokon, H.; Chiarella, V.; Curatolo, M.; Di Nardo, R.; Esposito, B.; Gatti, C.; Laurelli, P.; Maccarrone, G.; Prokofiev, K.; Sansoni, A.; Testa, M.; Vilucchi, E.] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy. [Amoroso, S.; Arnold, H.; Betancourt, C.; Boehler, M.; Bruneliere, R.; Buehrer, F.; Buescher, D.; Consorti, V.; Di Simone, A.; Fehling-Kaschek, M.; Flechl, M.; Giuliani, C.; Herten, G.; Jakobs, K.; Javurek, T.; Jenni, P.; Kiss, F.; Koeneke, K.; Kopp, A. K.; Kuehn, S.; Lai, S.; Landgraf, U.; Madar, R.; Mahboubi, K.; Mohr, W.; Pagacova, M.; Parzefall, U.; Rave, T. C.; Ruehr, F.; Rurikova, Z.; Ruthmann, N.; Schillo, C.; Schmidt, E.; Schumacher, M.; Sommer, P.; Sundermann, J. E.; Temming, K. K.; Tsiskaridze, V.; Ungaro, F. C.; von Radziewski, H.; Anh, T. Vu; Warsinsky, M.; Weiser, C.; Werner, M.; Zimmermann, S.] Univ Freiburg, Fak Mathemat & Phys, D-79106 Freiburg, Germany. [Alexandre, G.; Ancu, L. S.; Barone, G.; Bell, P. J.; Bell, W. H.; Noccioli, E. Benhar; De Mendizabal, J. Bilbao; Bucci, F.; Toro, R. Camacho; Clark, A.; Delitzsch, C. M.; della Volpe, D.; Doglioni, C.; Ferrere, D.; Gadomski, S.; Gonzalez-Sevilla, S.; Gramling, J.; Guescini, F.; Iacobucci, G.; Katre, A.; La Rosa, A.; Mermod, P.; Miucci, A.; Muenstermann, D.; Nektarijevic, S.; Nessi, M.; Nikolics, K.; Picazio, A.; Pohl, M.; Rosbach, K.; Vallecorsa, S.; Wu, X.] Univ Geneva, Sect Phys, Geneva, Switzerland. [Barberis, D.; Darbo, G.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Gemme, C.; Guido, E.; Morettini, P.; Osculati, B.; Parodi, F.; Passaggio, S.; Rossi, L. P.; Schiavi, C.] Univ Genoa, Ist Nazl Fis Nucl, Sez Genova, Genoa, Italy. [Barberis, D.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Guido, E.; Osculati, B.; Parodi, F.; Schiavi, C.] Univ Genoa, Dipartimento Fis, Genoa, Italy. [Jejelava, J.; Tskhadadze, E. G.] Iv Javakhishvili Tbilisi State Univ, E Andronikashvili Inst Phys, Tbilisi, Rep of Georgia. [Djobava, T.; Durglishvili, A.; Khubua, J.; Mosidze, M.] Tbilisi State Univ, Inst High Energy Phys, Tbilisi, Rep of Georgia. [Dueren, M.; Kreutzfeldt, K.; Stenzel, H.] Univ Giessen, Inst Phys 2, Giessen, Germany. [Bates, R. L.; Britton, D.; Buckley, A. G.; Bussey, P.; Buttar, C. M.; Buzatu, A.; D'Auria, S.; Doherty, T.; Doyle, A. T.; Ferrag, S.; Ferrando, J.; de Lima, D. E. Ferreira; Gemmell, A.; Gul, U.; Ortiz, N. G. Gutierrez; Kar, D.; Knue, A.; Moraes, A.; O'Shea, V.; Barrera, C. Oropeza; Qin, G.; Quilty, D.; Ravenscroft, T.; Robson, A.; Saxon, D. H.; Smith, K. M.; Denis, R. D. St.; Stewart, G. A.; Thompson, A. S.; Wright, M.] Univ Glasgow, Sch Phys & Astron, SUPA, Glasgow, Lanark, Scotland. [Bierwagen, K.; Bindi, M.; Blumenschein, U.; George, M.; Goujdami, D.; Graber, L.; Grosse-Knetter, J.; Hamer, M.; Hensel, C.; Kawamura, G.; Keil, M.; Kroeninger, K.; Lemmer, B.; Magradze, E.; Mchedlidze, G.; Llacer, M. Moreno; Musheghyan, H.; Nackenhorst, O.; Nadal, J.; Quadt, A.; Rieger, J.; Schorlemmer, A. L. S.; Serkin, L.; Shabalina, E.; Stolte, P.; Schroeder, T. Vazquez; Weingarten, J.; Zinonos, Z.] Univ Gottingen, Inst Phys 2, Gottingen, Germany. [Albrand, S.; Brown, J.; Collot, J.; Crepe-Renaudin, S.; Dechenaux, B.; Delsart, P. A.; Gabaldon, C.; Genest, M. H.; Hostachy, J. -Y.; Le, B. T.; Ledroit-Guillon, F.; Lleres, A.; Lucotte, A.; Malek, F.; Monini, C.; Stark, J.; Trocme, B.; Wu, M.] Univ Grenoble Alpes, CNRS, IN2P3, Lab Phys Subatom & Cosmol, Grenoble, France. [McFarlane, K. W.] Hampton Univ, Dept Phys, Hampton, VA 23668 USA. [da Costa, J. Barreiro Guimaraes; Butler, B.; Catastini, P.; Conti, G.; Franklin, M.; Huth, J.; Ippolito, V.; Mateos, D. Lopez; Mercurio, K. M.; Morii, M.; Skottowe, H. P.; Spearman, W. R.; Yen, A. L.; della Porta, G. Zevi] Harvard Univ, Lab Particle Phys & Cosmol, Cambridge, MA 02138 USA. [Andrei, V.; Brandt, O.; Davygora, Y.; Dietzsch, T. A.; Dunford, M.; Hanke, P.; Hofmann, J. I.; Jongmanns, J.; Khomich, A.; Kluge, E. -E.; Laier, H.; Lang, V. S.; Meier, K.; Mueller, F.; Poddar, S.; Scharf, V.; Schultz-Coulon, H. -C.; Stamen, R.; Wessels, M.] Heidelberg Univ, Kirchhoff Inst Phys, Heidelberg, Germany. [Anders, C. F.; Giulini, M.; Kasieczka, G.; Narayan, R.; Schaetzel, S.; Schmitt, S.; Schoening, A.] Heidelberg Univ, Inst Phys, Heidelberg, Germany. [Colombo, T.; Kretz, M.; Kugel, A.] Heidelberg Univ, ZITI Inst Tech Informat, Mannheim, Germany. [Nagasaka, Y.] Hiroshima Inst Technol, Fac Appl Informat Sci, Hiroshima, Japan. [Brunet, S.; Dattagupta, A.; Evans, H.; Gagnon, P.; Lammers, S.; Martinez, N. Lorenzo; Luehring, F.; Ogren, H.; Penwell, J.; Poveda, J.; Weinert, B.; Zieminska, D.] Indiana Univ, Dept Phys, Bloomington, IN 47405 USA. [Franz, S.; Jussel, P.; Kneringer, E.; Lukas, W.; Nagai, K.; Ritsch, E.; Usanova, A.] Leopold Franzens Univ, Inst Astro & Teilchenphys, Innsbruck, Austria. [Cinca, D.; Gandrajula, R. P.; Mallik, U.; Mandrysch, R.; Morange, N.; Zaidan, R.] Univ Iowa, Iowa City, IA USA. [Chen, C.; Cochran, J.; De Lorenzi, F.; Dudziak, F.; Krumnack, N.; Prell, S.; Shrestha, S.; Yamamoto, K.] Iowa State Univ, Dept Phys & Astron, Ames, IA USA. [Ahmadov, F.; Aleksandrov, I. N.; Bednyakov, V. A.; Boyko, I. R.; Budagov, I. A.; Chelkov, G. A.; Cheplakov, A.; Chizhov, M. V.; Dedovich, D. V.; Demichev, M.; Glonti, G. L.; Gostkin, M. I.; Huseynov, N.; Javadov, N.; Karpov, S. N.; Kazarinov, M. Y.; Khramov, E.; Kotov, V. M.; Kruchonak, U.; Krumshteyn, Z. V.; Kukhtin, V.; Ladygin, E.; Minashvili, I. A.; Mineev, M.; Olchevski, A. G.; Peshekhonov, V. D.; Plotnikova, E.; Potrap, I. N.; Pozdnyakov, V.; Rusakovich, N. A.; Sadykov, R.; Sapronov, A.; Shiyakova, M.; Sisakyan, A. N.; Soloshenko, A.; Topilin, N. D.; Vinogradov, V. B.; Zhemchugov, A.; Zimine, N. I.] Joint Inst Nucl Res Dubna, Dubna, Russia. [Amako, K.; Aoki, M.; Arai, Y.; Ikegami, Y.; Ikeno, M.; Iwasaki, H.; Kanzaki, J.; Kohriki, T.; Kondo, T.; Kono, T.; Makida, Y.; Mitsui, S.; Nagano, K.; Nakamura, K.; Nozaki, M.; Odaka, S.; Sasaki, O.; Suzuki, Y.; Takubo, Y.; Tanaka, S.; Terada, S.; Tokushuku, K.; Tsuno, S.; Unno, Y.; Yamada, M.; Yamamoto, A.; Yasu, Y.] High Energy Accelerator Res Org, KEK, Tsukuba, Ibaraki, Japan. [Inamaru, Y.; Kishimoto, T.; Kitamura, T.; Kurashige, H.; Kurumida, R.; Matsushita, T.; Ochi, A.; Shimizu, S.; Takeda, H.; Tani, K.; Watanabe, I.; Yamazaki, Y.; Yuan, L.] Kobe Univ, Grad Sch Sci, Kobe, Hyogo 657, Japan. [Ishino, M.; Sumida, T.; Tashiro, T.] Kyoto Univ, Fac Sci, Kyoto, Japan. [Takashima, R.] Kyoto Univ, Kyoto 612, Japan. [Kawagoe, K.; Oda, S.; Otono, H.; Tojo, J.] Kyushu Univ, Dept Phys, Fukuoka 812, Japan. [AlconadaVerzini, M. J.; Alonso, F.; Anduaga, X. S.; Dova, M. T.; Monticelli, F.; Tripiana, M. F.; Wahlberg, H.] Univ Nacl La Plata, Inst Fis La Plata, La Plata, Buenos Aires, Argentina. [AlconadaVerzini, M. J.; Alonso, F.; Anduaga, X. S.; Dova, M. T.; Monticelli, F.; Tripiana, M. F.; Wahlberg, H.] Consejo Nacl Invest Cient & Tecn, La Plata, Buenos Aires, Argentina. [Allison, L. J.; Barton, A. E.; Borissov, G.; Bouhova-Thacker, E. V.; Chilingarov, A.; Dearnaley, W. J.; Fox, H.; Grimm, K.; Henderson, R. C. W.; Hughes, G.; Jones, R. W. L.; Kartvelishvili, V.; Long, R. E.; Love, P. A.; Maddocks, H. J.; Smizanska, M.; Walder, J.] Univ Lancaster, Dept Phys, Lancaster, England. [Chiodini, G.; Gorini, E.; Orlando, N.; Perrino, R.; Primavera, M.; Spagnolo, S.; Ventura, A.] Univ Salento, Ist Nazl Fis Nucl, Sez Lecce, Lecce, Italy. [Gorini, E.; Orlando, N.; Spagnolo, S.; Ventura, A.] Univ Salento, Dipartimento Matemat & Fis, Lecce, Italy. [Allport, P. P.; Bundock, A. C.; Burdin, S.; D'Onofrio, M.; Dervan, P.; Gwilliam, C. B.; Hayward, H. S.; Jackson, M.; Jones, T. J.; King, B. T.; Klein, M.; Klein, U.; Kretzschmar, J.; Laycock, P.; Lehan, A.; Mahmoud, S.; Maxfield, S. J.; Mehta, A.; Migas, S.; Price, J.; Readioff, N. P.; Schnellbach, Y. J.; Sellers, G.; Vossebeld, H.; Waller, P.] Univ Liverpool, Oliver Lodge Lab, Liverpool L69 3BX, Merseyside, England. [Cindro, V.; Deliyergiyev, M.; Filipcic, A.; Gorisek, A.; Kersevan, B. P.; Kramberger, G.; Mandic, I.; Mikuz, M.; Tykhonov, A.] Jozef Stefan Inst, Dept Phys, Ljubljana, Slovenia. [Cindro, V.; Deliyergiyev, M.; Filipcic, A.; Gorisek, A.; Kersevan, B. P.; Kramberger, G.; Mandic, I.; Mikuz, M.; Tykhonov, A.] Univ Ljubljana, Ljubljana, Slovenia. [Alpigiani, C.; Bona, M.; Bret, M. Cano; Cerrito, L.; Fletcher, G.; Goddard, J. R.; Hickling, R.; Landon, M. P. J.; Lloyd, S. L.; Morris, J. D.; Piccaro, E.; Rizvi, E.; Salamanna, G.; Sandbach, R. L.; Snidero, G.; Castanheira, M. Teixeira Dias] Queen Mary Univ, Sch Phys & Astron, London, England. [Berry, T.; Boisvert, V.; Brooks, T.; Cantrill, R.; Connelly, I. A.; Cooper-Smith, N. J.; Cowan, G.; Duguid, L.; George, S.; Gibson, S. M.; Kempster, J. J.; Vazquez, J. G. Panduro; Pastore, Fr.; Rose, M.; Spano, F.; Teixeira-Dias, P.; Thomas-Wilsker, J.] Royal Holloway Univ London, Dept Phys, Surrey, England. [Baker, S.; Bernat, P.; Bieniek, S. P.; Butterworth, J. M.; Campanelli, M.; Casadei, D.; Chislett, R. T.; Cooper, B. D.; Davison, A. R.; Davison, P.; Falla, R. J.; Gregersen, K.; Gutschow, C.; Hesketh, G. G.; Jansen, E.; Konstantinidis, N.; Korn, A.; Lambourne, L.; Leney, K. J. C.; Martyniuk, A. C.; Mcfayden, J. A.; Nurse, E.; Ochoa, M. I.; Pilkington, A. D.; Scanlon, T.; Sherwood, P.; Simmons, B.; Wardrope, D. R.; Waugh, B. M.; Wijeratne, P. A.] UCL, Dept Phys & Astron, London, England. [Bernius, C.; Greenwood, Z. D.; Jana, D. K.; Sawyer, L.; Sircar, A.; Subramaniam, R.] Louisiana Tech Univ, Ruston, LA 71270 USA. [Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; Davignon, O.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Liu, K.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Vannucci, F.; Varouchas, D.] UPMC, Lab Phys Nucl & Hautes Energies, Paris, France. [Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; Davignon, O.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Liu, K.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Vannucci, F.; Varouchas, D.] Univ Paris Diderot, Paris, France. [Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; Davignon, O.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Liu, K.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Vannucci, F.; Varouchas, D.] CNRS, IN2P3, Paris, France. [Akesson, T. P. A.; Bocchetta, S. S.; Bryngemark, L.; Floderus, A.; Hawkins, A. D.; Hedberg, V.; Ivarsson, J.; Jarlskog, G.; Lytken, E.; Meirose, B.; Mjornmark, J. U.; Smirnova, O.; Viazlo, O.] Lund Univ, Inst Fys, Lund, Sweden. [Arnal, V.; Barreiro, F.; Cantero, J.; De la Torre, H.; Del Peso, J.; Glasman, C.; Llorente Merino, J.; Terron, J.] Univ Autonoma Madrid, Dept Fis Teor C 15, Madrid, Spain. [Blum, W.; Buescher, V.; Caputo, R.; Ellinghaus, F.; Endner, O. C.; Ertel, E.; Fiedler, F.; Torregrosa, E. Fullana; Goeringer, C.; Heck, T.; Hohlfeld, M.; Hsu, P. J.; Huelsing, T. A.; Ji, W.; Karnevskiy, M.; Kleinknecht, K.; Koenig, S.; Koepke, L.; Lungwitz, M.; Masetti, L.; Mattmann, J.; Meyer, C.; Moreno, D.; Moritz, S.; Mueller, T.; Poettgen, R.; Sander, H. G.; Schaefer, U.; Schmitt, C.; Schott, M.; Schroeder, C.; Schuh, N.; Simioni, E.; Tapprogge, S.; Wollstadt, S. J.; Zimmermann, C.] Johannes Gutenberg Univ Mainz, Inst Phys, Mainz, Germany. [Almond, J.; Borri, M.; Brown, G.; Cox, B. E.; Da Via, C.; Forti, A.; Ponce, J. M. Iturbe; Joshi, K. D.; Klinger, A.; Loebinger, F. K.; Masik, J.; Oh, A.; Owen, M.; Pater, J. R.; Peters, R. F. Y.; Price, D.; Queitsch-Maitland, M.; Robinson, J. E. M.; Schwanenberger, C.; Tomlinson, L.; Woudstra, M. J.] Univ Manchester, Sch Phys & Astron, Manchester, Lancs, England. [Aad, G.; Alio, L.; Barbero, M.; Bertella, C.; Chen, L.; Clemens, J. C.; Coadou, Y.; Diglio, S.; Djama, F.; Feligioni, L.; Gao, J.; Hoffmann, D.; Hubaut, F.; Knoops, E. B. F. G.; Le Guirriec, E.; Li, B.; Madaffari, D.; Mochizuki, K.; Monnier, E.; Muanza, S.; Nagai, Y.; Pralavorio, P.; Rozanov, A.; Serre, T.; Talby, M.; Tiouchichine, E.; Tisserant, S.; Toth, J.; Touchard, F.; Ughetto, M.; Vacavant, L.] Aix Marseille Univ, CPPM, Marseille, France. [Bellomo, M.; Brau, B.; Colon, G.; Dallapiccola, C.; Daya-Ishmukhametova, R. K.; Meade, A.; Moyse, E. J. W.; Pais, P.; Pueschel, E.; Varol, T.; Ventura, D.; Willocq, S.] Univ Massachusetts, Dept Phys, Amherst, MA 01003 USA. [Belanger-Champagne, C.; Chapleau, B.; Cheatham, S.; Corriveau, F.; Mantifel, R.; Robertson, S. H.; Robichaud-Veronneau, A.; Stockton, M. C.; Stoebe, M.; Vachon, B.; Wang, K.; Warburton, A.] McGill Univ, Dept Phys, Montreal, PQ, Canada. [Barberio, E. L.; Brennan, A. J.; Jennens, D.; Kubota, T.; Limosani, A.; Hanninger, G. Nunes; Nuti, F.; Petersen, B. A.; Rados, P.; Shao, Q. T.; Tan, K. G.; Taylor, G. N.; Thong, W. M.; Volpi, M.] Univ Melbourne, Sch Phys, Melbourne, Vic 3010, Australia. [Amidei, D.; Chelstowska, M. A.; Cheng, H. C.; Dai, T.; Diehl, E. B.; Dubbert, J.; Feng, H.; Ferretti, C.; Fleischmann, P.; Goldfarb, S.; Harper, D.; Levin, D.; Liu, L.; Long, J. D.; Mc kee, S. P.; McCarn, A.; Neal, H. A.; Panikashvili, N.; Qian, J.; Searcy, J.; Thun, R. P.; Wilson, A.; Wu, Y.; Xu, L.; Yu, J. M.; Zhang, D.; Zhou, B.; Zhu, J.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA. [Abolins, M.; Gonzalez, B. Alvarez; Arabidze, G.; Brock, R.; Bromberg, C.; Caughron, S.; Chegwidden, A.; Fisher, W. C.; Halladjian, G.; Hauser, R.; Hayden, D.; Huston, J.; Koll, J.; Linnemann, J. T.; Martin, B.; Pope, B. G.; Schoenrock, B. D.; Schwienhorst, R.; Ta, D.; Tollefson, K.; True, P.; Willis, C.; Zhang, H.] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA. [Alimonti, G.; Andreazza, A.; Besana, M. I.; Carminati, L.; Cavalli, D.; Citterio, M.; Consonni, S. M.; Costa, G.; Fanti, M.; Giugni, D.; Lari, T.; Mandelli, L.; Meloni, F.; Meroni, C.; Perini, L.; Pizio, C.; Ragusa, F.; Resconi, S.; Simoniello, R.; Tartarelli, G. F.; Troncon, C.; Turra, R.; Perez, M. Villaplana] Univ Milan, Ist Nazl Fis Nucl, Sez Milano, Milan, Italy. [Andreazza, A.; Carminati, L.; Consonni, S. M.; Fanti, M.; Meloni, F.; Perini, L.; Pizio, C.; Ragusa, F.; Simoniello, R.; Turra, R.; Perez, M. Villaplana] Univ Milan, Dipartimento Fis, Milan, Italy. [Bogouch, A.; Harkusha, S.; Kulchitsky, Y.; Kurochkin, Y. A.; Tsiareshka, P. V.] Natl Acad Sci Belarus, BI Stepanov Inst Phys, Minsk, Byelarus. [Yanush, S.] Natl Sci & Educ Ctr Particle & High Energy Phys, Minsk, Byelarus. [Taylor, F. E.] MIT, Dept Phys, Cambridge, MA 02139 USA. [Arguin, J. -F.; Azuelos, G.; Dallaire, F.; Gauthier, L.; Leroy, C.; Rezvani, R.; Soueid, P.] Univ Montreal, Grp Particle Phys, Montreal, PQ, Canada. [Akimov, A. V.; Baranov, S. P.; Gavrilenko, I. L.; Komar, A. A.; Mashinistov, R.; Mouraviev, S. V.; Nechaeva, P. Yu.; Shmeleva, A.; Snesarev, A. A.; Sulin, V. V.; Tikhomirov, V. O.; Zhukov, K.] Acad Sci, PN Lebedev Phys Inst, Moscow, Russia. [Artamonov, A.; Gorbounov, P. A.; Khovanskiy, V.; Shatalov, P. B.; Tsukerman, I. I.] Inst Theoret & Expt Phys, Moscow 117259, Russia. [Antonov, A.; Belotskiy, K.; Bulekov, O.; Dolgoshein, B. A.; Kantserov, V. A.; Khodinov, A.; Krasnopevtsev, D.; Romaniouk, A.; Shulga, E.; Smirnov, S. Yu.; Smirnov, Y.; Soldatov, E. Yu.; Tikhomirov, V. O.; Timoshenko, S.; Vorobev, K.] Moscow Phys Engn Inst MEPhI, Moscow, Russia. [Boldyrev, A. S.; Gladilin, L. K.; Grishkevich, Y. V.; Kramarenko, V. A.; Rud, V. I.; Sivoklokov, S. Yu.; Smirnova, L. N.; Turchikhin, S.] Moscow MV Lomonosov State Univ, DV Skobeltsyn Inst Nucl Phys, Moscow, Russia. [Adomeit, S.; Becker, S.; Biebel, O.; Bock, C.; Bortfeldt, J.; Calfayan, P.; Chow, B. K. B.; Duckeck, G.; Ebke, J.; Elmsheuser, J.; Heller, C.; Hertenberger, R.; Legger, F.; Lorenz, J.; Mann, A.; Meineck, C.; Mitrevski, J.; Nunnemann, T.; Rauscher, F.; Ruschke, A.; Sanders, M. P.; Schaile, D.; Schieck, J.; Schmitt, C.; Vladoiu, D.; Walker, R.; Will, J. Z.; Wittkowski, J.] Univ Munich, Fak Phys, Munich, Germany. [Barillari, T.; Bethke, S.; Bronner, J.; Compostella, G.; Cortiana, G.; Flowerdew, M. J.; Goblirsch-Kolb, M.; Ince, T.; Kiryunin, A. E.; Kluth, S.; Kortner, O.; Kortner, S.; Kroha, H.; Macchiolo, A.; Manfredini, A.; Menke, S.; Moser, H. G.; Nagel, M.; Nisius, R.; Nowak, S.; Oberlack, H.; Pahl, C.; Pospelov, G. E.; Richter, R.; Salihagic, D.; Sandstroem, R.; Schacht, P.; Schwegler, Ph.; Sforza, F.; Stern, S.; Stonjek, S.; Terzo, S.; von der schmitt, H.; Weigell, P.; Wildauer, A.; Zanzi, D.] Max Planck Inst Phys & Astrophys, Werner Heisenberg Inst, D-80805 Munich, Germany. [Shimojima, M.] Nagasaki Inst Appl Sci, Nagasaki, Japan. [Hasegawa, S.; Morvaj, L.; Ohshima, T.; Takahashi, Y.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Grad Sch Sci, Nagoya, Aichi 4648601, Japan. [Hasegawa, S.; Morvaj, L.; Ohshima, T.; Takahashi, Y.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Kobayashi Maskawa Inst, Nagoya, Aichi 4648601, Japan. [Aloisio, A.; Alviggi, M. G.; Canale, V.; Carlino, G.; Chiefari, G.; Conventi, F.; de Asmundis, R.; Della Pietra, M.; Di Donato, C.; Doria, A.; Giordano, R.; Iengo, P.; Izzo, V.; Merola, L.; Patricelli, S.; Rossi, E.; Sanchez, A.; Sekhniaidzea, G.; Zurzolo, G.] Univ Naples Federico II, Ist Nazl Fis Nucl, Sez Napoli, Naples, Italy. [Aloisio, A.; Alviggi, M. G.; Canale, V.; Chiefari, G.; Di Donato, C.; Giordano, R.; Merola, L.; Patricelli, S.; Rossi, E.; Sanchez, A.; Zurzolo, G.] Univ Naples Federico II, Dipartimento Fis, Naples, Italy. [Gorelov, I.; Hoeferkamp, M. R.; Seidel, S. C.; Toms, K.; Wang, R.] Univ New Mexico, Dept Phys & Astron, Albuquerque, NM 87131 USA. [Besjes, G. J.; Caron, S.; Croft, V.; Dao, V.; De Groot, N.; Filthaut, F.; Galea, C.; Klok, P. F.; Konig, A. C.; Salvucci, A.] Radboud Univ Nijmegen Nikhef, Inst Math Astrophys & Particle Phys, Nijmegen, Netherlands. [Aben, R.; Angelozzi, I.; Beemster, L. J.; Bentvelsen, S.; Berge, D.; Berglund, E.; Bobbink, G. J.; Bos, K.; Boterenbrood, H.; Butti, P.; Castelli, A.; Colijn, A. P.; de Jong, P.; De Nooij, L.; Deigaard, I.; Deluca, C.; Deviveiros, P. O.; Dhaliwal, S.; Ferrari, P.; Gadatsch, S.; Geerts, D. A. A.; Hartjes, F.; Hessey, N. P.; Hod, N.; Igonkina, O.; Kluit, P.; Koffeman, E.; Lee, H.; Lenz, T.; Linde, F.; Mahlstedt, J.; Mechnich, J.; Oussoren, K. P.; Pani, P.; Salek, D.; Valencic, N.; Van Der Deijl, P. C.; van der Geer, R.; van der Graaf, H.; Van Der Leeuw, R.; van Vulpen, I.; Verkerke, W.; Vermeulen, J. C.; Milosavljevic, M. Vranjes; Vreeswijk, M.; Weits, H.] Nikhef Natl Inst Subatom Phys, Amsterdam, Netherlands. [Aben, R.; Angelozzi, I.; Beemster, L. J.; Bentvelsen, S.; Berge, D.; Berglund, E.; Bobbink, G. J.; Bos, K.; Boterenbrood, H.; Butti, P.; Castelli, A.; Colijn, A. P.; de Jong, P.; De Nooij, L.; Deigaard, I.; Deluca, C.; Deviveiros, P. O.; Dhaliwal, S.; Ferrari, P.; Gadatsch, S.; Geerts, D. A. A.; Hartjes, F.; Hessey, N. P.; Hod, N.; Igonkina, O.; Kluit, P.; Koffeman, E.; Lee, H.; Lenz, T.; Linde, F.; Mahlstedt, J.; Mechnich, J.; Oussoren, K. P.; Pani, P.; Salek, D.; Valencic, N.; Van Der Deijl, P. C.; van der Geer, R.; van der Graaf, H.; Van Der Leeuw, R.; van Vulpen, I.; Verkerke, W.; Vermeulen, J. C.; Milosavljevic, M. Vranjes; Vreeswijk, M.; Weits, H.] Univ Amsterdam, Amsterdam, Netherlands. [Burghgrave, B.; Calkins, R.; Chakraborty, D.; Cole, S.; Suhr, C.; Yurkewicz, A.; Zutshi, V.] No Illinois Univ, Dept Phys, De Kalb, IL USA. [Anisenkov, A. V.; Bobrovnikov, V. S.; Bogdanchikov, A. G.; Kazanin, V. F.; Korol, A. A.; Malyshev, V. M.; Maslennikov, A. L.; Maximov, D. A.; Peleganchuk, S. V.; Rezanova, O. L.; Skovpen, K. Yu.; Soukharev, A. M.; Talyshev, A. A.; Tikhonov, Yu. A.] RAS, Budker Inst Nucl Phys, SB, Novosibirsk, Russia. [Cranmer, K.; Haas, A.; Heinrich, L.; van Huysduynen, L. Hooft; Kaplan, B.; Karthik, K.; Konoplich, R.; Kreiss, S.; Lewis, G. H.; Mincer, A. I.; Nemethy, P.; Neves, R. M.] NYU, Dept Phys, New York, NY 10003 USA. [Gan, K. K.; Ishmukhametov, R.; Kagan, H.; Kass, R. D.; Merritt, H.; Moss, J.; Nagarkar, A.; Pignotti, D. T.; Yang, Y.] Ohio State Univ, Columbus, OH 43210 USA. [Nakano, I.] Okayama Univ, Fac Sci, Okayama 700, Japan. [Abbott, B.; Bertsche, D.; Gutierrez, P.; Hasib, A.; Norberg, S.; Saleem, M.; Severini, H.; Skubic, P.; Strauss, M.] Univ Oklahoma, Homer L Dodge Dept Phys & Astron, Norman, OK 73019 USA. [Abi, B.; Bousson, N.; Khanov, A.; Rizatdinova, F.; Sidorov, D.; Yu, J.] Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USA. [Chytka, L.; Hamal, P.; Hrabovsky, M.; Kvita, J.; Nozka, L.] Palacky Univ, RCPTM, CR-77147 Olomouc, Czech Republic. [Brau, J. E.; Brost, E.; Majewski, S.; Potter, C. T.; Ptacek, E.; Radloff, P.; Shamim, M.; Sinev, N. B.; Strom, D. M.; Torrence, E.; Wanotayaroj, C.; Winklmeier, F.] Univ Oregon, Ctr High Energy Phys, Eugene, OR 97403 USA. [Khalek, S. Abdel; Bassalat, A.; Becot, C.; Binet, S.; Bourdarios, C.; Charfeddine, D.; De Regie, J. B. De Vivie; Duflot, L.; Escalier, M.; Fayard, L.; Fournier, D.; Grivaz, J. -F.; Guillemin, T.; Henrot-Versille, S.; Hrivnac, J.; Iconomidou-Fayard, L.; Kado, M.; Li, Y.; Lounis, A.; Makovec, N.; Poggioli, L.; Puzo, P.; Renaud, A.; Rousseau, D.; Rybkin, G.; Schaffer, A. C.; Scifo, E.; Serin, L.; Simion, S.; Tanaka, R.; Tran, H. L.; Zerwas, D.; Zhang, Z.] Univ Paris 11, LAL, Orsay, France. [Khalek, S. Abdel; Bassalat, A.; Becot, C.; Binet, S.; Bourdarios, C.; Charfeddine, D.; De Regie, J. B. De Vivie; Duflot, L.; Escalier, M.; Fayard, L.; Fournier, D.; Grivaz, J. -F.; Guillemin, T.; Henrot-Versille, S.; Hrivnac, J.; Iconomidou-Fayard, L.; Kado, M.; Li, Y.; Lounis, A.; Makovec, N.; Poggioli, L.; Puzo, P.; Renaud, A.; Rousseau, D.; Rybkin, G.; Schaffer, A. C.; Scifo, E.; Serin, L.; Simion, S.; Tanaka, R.; Tran, H. L.; Zerwas, D.; Zhang, Z.] CNRS, IN2P3, F-91405 Orsay, France. [Endo, M.; Hanagaki, K.; Lee, J. S. H.; Nomachi, M.; Okamura, W.; Sugaya, Y.; Teoh, J. J.] Osaka Univ, Grad Sch Sci, Osaka, Japan. [Bugge, L.; Bugge, M. K.; Cameron, D.; Catmore, J. R.; Gjelsten, B. K.; Gramstad, E.; Ould-Saada, F.; Pajchel, K.; Pedersen, M.; Read, A. L.; Rohne, O.; Stapnes, S.; Strandlie, A.] Univ Oslo, Dept Phys, Oslo, Norway. [Apolle, R.; Barr, A. J.; Behr, K.; Boddy, C. R.; Buckingham, R. M.; Cooper-Sarkar, A. M.; Ortuzar, M. Crispin; Dafinca, A.; Davies, E.; Gallas, E. J.; Gupta, S.; Gwenlan, C.; Hall, D.; Hays, C. P.; Henderson, J.; Howard, J.; Huffman, T. B.; Issever, C.; Kalderon, C. W.; King, R. S. B.; Kogan, L. A.; Lewis, A.; Livermore, S. S. A.; Nickerson, R. B.; Pachal, K.; Pinder, A.; Ryder, N. C.; Sawyer, C.; Short, D.; Tseng, J. C-L.; Vickey, T.; Viehhauser, G. H. A.; Weidberg, A. R.; Zhong, J.] Univ Oxford, Dept Phys, Oxford, England. [Conta, C.; Dondero, P.; Ferrari, R.; Fraternali, M.; Gaudioa, G.; Livan, M.; Negri, A.; Polesello, G.; Rebuzzi, D. M.; Rimoldi, A.; Vercesi, V.] Univ Pavia, Ist Nazl Fis Nucl, Sez Pavia, I-27100 Pavia, Italy. [Conta, C.; Dondero, P.; Fraternali, M.; Livan, M.; Negri, A.; Rebuzzi, D. M.; Rimoldi, A.] Univ Pavia, Dipartimento Fis, I-27100 Pavia, Italy. [Brendlinger, K.; Heim, S.; Hines, E.; Hong, T. M.; Jackson, B.; Kroll, J.; Kunkle, J.; Lester, C. M.; Lipeles, E.; Ospanov, R.; Saxon, J.; Schaefer, D.; Stahlman, J.; Thomson, E.; Tuna, A. N.; Vanguri, R.; Williams, H. H.] Univ Penn, Dept Phys, Philadelphia, PA 19104 USA. [Ezhilov, A.; Fedin, O. L.; Gratchev, V.; Grebenyuk, O. G.; Levchenko, M.; Maleev, V. P.; Ryabov, Y. F.; Schegelsky, V. A.; Sedykh, E.; Seliverstov, D. M.; Solovyev, V.] Petersburg Nucl Phys Inst, Gatchina, Russia. [Beccherle, R.; Bertolucci, F.; Cavasinni, V.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Roda, C.; Scuri, F.; Volpi, G.; White, S.] Univ Pisa, Ist Nazl Fis Nucl, Sez Pisa, I-56100 Pisa, Italy. [Beccherle, R.; Bertolucci, F.; Cavasinni, V.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Roda, C.; Scuri, F.; Volpi, G.; White, S.] Univ Pisa, Dipartimento Fis E Fermi, Pisa, Italy. [Bianchi, R. M.; Boudreau, J.; Cleland, W.; Escobar, C.; Kittelmann, T.; Mueller, J.; Prieur, D.; Sapp, K.; Su, J.; Yoosoofmiya, R.] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA. [Aguilar-Saavedra, J. A.; Amor Dos Santos, S. P.; Amorim, A.; Anjos, N.; Araque, J. P.; Carvalho, J.; Castro, N. F.; Muino, P. Conde; Da Cunha Sargedas De Sousa, M. J.; Wemans, A. Do Valle; Fiolhais, M. C. N.; Galhardo, B.; Gomes, A.; Goncalo, R.; Jorge, P. M.; Lopes, L.; Miguens, J. Machado; Maio, A.; Maneira, J.; Marques, C. N.; Onofre, A.; Palma, A.; Pedro, R.; Pina, J.; Pinto, B.; Santos, H.; Saraiva, J. G.; Silva, J.; Delgado, A. Tavares; Veloso, F.; Wolters, H.] Lab Instrumentacao & Fis Expt Particulas LIP, Lisbon, Portugal. [Amorim, A.; Muino, P. Conde; Da Cunha Sargedas De Sousa, M. J.; Gomes, A.; Jorge, P. M.; Miguens, J. Machado; Maio, A.; Maneira, J.; Palma, A.; Pedro, R.; Pina, J.; Delgado, A. Tavares] Univ Lisbon, Fac Ciencias, Lisbon, Portugal. [Amor Dos Santos, S. P.; Carvalho, J.; Fiolhais, M. C. N.; Galhardo, B.; Veloso, F.; Wolters, H.] Univ Coimbra, Dept Phys, Coimbra, Portugal. [Gomes, A.; Maio, A.; Pina, J.; Saraiva, J. G.; Silva, J.] Univ Lisbon, Ctr Fis Nucl, Lisbon, Portugal. [Onofre, A.] Univ Minho, Dept Fis, Braga, Portugal. [Aguilar-Saavedra, J. A.] Univ Granada, Dept Fis Teor & Cosmos, Granada, Spain. [Aguilar-Saavedra, J. A.] Univ Granada, CAFPE, Granada, Spain. [Wemans, A. Do Valle] Univ Nova Lisboa, Fac Ciencias & Tecnol, Dept Fis, Caparica, Portugal. [Wemans, A. Do Valle] Univ Nova Lisboa, Fac Ciencias & Tecnol, CEFITEC, Caparica, Portugal. [Bohm, J.; Chudoba, J.; Havranek, M.; Hejbal, J.; Jakoubek, T.; Kepka, O.; Kupco, A.; Kus, V.; Lokajicek, M.; Lysak, R.; Marcisovsky, M.; Mikestikova, M.; Nemecek, S.; Sicho, P.; Staroba, P.; Svatos, M.; Tasevsky, M.; Vrba, V.] Acad Sci Czech Republic, Inst Phys, Prague, Czech Republic. [Augsten, K.; Gallus, P.; Gunther, J.; Jakubek, J.; Kohout, Z.; Kral, V.; Myska, M.; Pospisil, S.; Seifert, F.; Simak, V.; Slavicek, T.; Smolek, K.; Solar, M.; Solc, J.; Sopczak, A.; Sopko, V.; Sopko, B.; Suk, M.; Turecek, D.; Vacek, V.; Vlasak, M.; Vokac, P.; Vykydal, Z.; Zeman, M.] Czech Tech Univ, CR-16635 Prague, Czech Republic. [Balek, P.; Berta, P.; Cerny, K.; Chalupkova, I.; Davidek, T.; Dolejsi, J.; Dolezal, Z.; Faltova, J.; Kodys, P.; Leitner, R.; Pleskot, V.; Reznicek, P.; Rybar, M.; Scheirich, D.; Spousta, M.; Sykora, T.; Tas, P.; Todorova-Nova, S.; Valkar, S.; Vorobel, V.] Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic. [Borisov, A.; Denisov, S. P.; Fakhrutdinov, R. M.; Fenyuk, A. B.; Golubkov, D.; Karyukhin, A. N.; Korotkov, V. A.; Kozhin, A. S.; Minaenko, A. A.; Myagkov, A. G.; Nikolaenko, V.; Solodkov, A. A.; Solovyanov, O. V.; Starchenko, E. A.; Zaitsev, A. M.; Zenin, O.] Inst High Energy Phys, State Res Ctr, Protvino, Russia. [Adye, T.; Apolle, R.; Baines, J. T.; Barnett, B. M.; Burke, S.; Davies, E.; Dewhurst, A.; Emeliyanov, D.; Gallop, B. J.; Gee, C. N. P.; Haywood, S. J.; Kirk, J.; Martin-Haugh, S.; McCubbin, N. A.; McMahon, S. J.; Middleton, R. P.; Murray, W. J.; Phillips, P. W.; Sankey, D. P. C.; Scott, W. G.; Tyndel, M.; Wickens, F. J.; Wielers, M.] Rutherford Appleton Lab, Particle Phys Dept, Didcot OX11 0QX, Oxon, England. [Benslama, K.] Univ Regina, Dept Phys, Regina, SK S4S 0A2, Canada. [Tanaka, S.] Ritsumeikan Univ, Kusatsu, Shiga, Japan. [Anulli, F.; Bagiacchi, P.; Bagnaia, P.; Bini, C.; Ciapetti, G.; De Pedis, D.; De Salvo, A.; Di Domenico, A.; Dionisi, C.; Falciano, S.; Gabrielli, A.; Gauzzi, P.; Gentile, S.; Giagu, S.; Kuna, M.; Lacava, F.; Luci, C.; Luminari, L.; Marzano, F.; Mirabelli, G.; Monzani, S.; Nisati, A.; Pasqualucci, E.; Petrolo, E.; Pontecorvo, L.; Rescigno, M.; Rosati, S.; Tehrani, F. Safai; Sidoti, A.; Camillocci, E. Solfaroli; Vanadia, M.; Vari, R.; Veneziano, S.; Zanello, L.] Univ Roma La Sapienza, Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy. [Bagiacchi, P.; Bagnaia, P.; Bini, C.; Ciapetti, G.; Di Domenico, A.; Dionisi, C.; Gabrielli, A.; Gauzzi, P.; Gentile, S.; Giagu, S.; Kuna, M.; Lacava, F.; Luci, C.; Messina, A.; Monzani, S.; Camillocci, E. Solfaroli; Vanadia, M.; Zanello, L.] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy. [Aielli, G.; Cardarelli, R.; Cattani, G.; Grossi, G. C.; Iuppa, R.; Liberti, B.; Mazzaferro, L.; Paolozzi, L.; Salamon, A.; Santonico, R.] Univ Roma Tor Vergata, Ist Nazl Fis Nucl, Sez Roma Tor Vergata, Rome, Italy. [Aielli, G.; Cattani, G.; Di Ciaccio, A.; Grossi, G. C.; Iuppa, R.; Mazzaferro, L.; Paolozzi, L.; Santonico, R.] Univ Roma Tor Vergata, Dipartimento Fis, I-00173 Rome, Italy. [Bacci, C.; Baroncelli, A.; Biglietti, M.; Bortolotto, V.; Ceradini, F.; Di Micco, B.; Farilla, A.; Graziani, E.; Iodice, M.; Orestano, D.; Passeri, A.; Pastore, F.; Petrucci, F.; Stanescu, C.; Trovatelli, M.] Univ Roma Tre, Ist Nazl Fis Nucl, Sez Roma Tre, Rome, Italy. [Bacci, C.; Bortolotto, V.; Ceradini, F.; Di Micco, B.; Orestano, D.; Pastore, F.; Petrucci, F.; Trovatelli, M.] Univ Roma Tre, Dipartimento Matemat & Fis, Rome, Italy. [Benchekroun, D.; Chafaq, A.; Gouighri, M.; Hoummada, A.] Univ Hassan 2, Reseau Univ Phys Hautes Energies, Fac Sci Ain Chock, Casablanca, Morocco. [Ghazlane, H.] Ctr Natl Energie Sci Tech Nucl, Rabat, Morocco. 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R.; Schoeffel, L.; Schune, Ph.; Schwemling, Ph.; Schwindling, J.; Tsionou, D.; Vranjes, N.; Xiao, M.] CEA Saclay, DSM IRFU, Inst Rech Lois Fondamentales Univers, Commissariat Energie Atom & Energies Alternat, F-91191 Gif Sur Yvette, France. [Battaglia, M.; Grillo, A. A.; Kuhl, A.; Law, A. T.; Liang, Z.; Litke, A. M.; Lockman, W. S.; Manning, P. M.; Nielsen, J.; Reece, R.; Sadrozinski, H. F-W.; Schumm, B. A.; Seiden, A.] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA. [Beckingham, M.; Blackburn, D.; Coccaro, A.; Harris, O. M.; Hsu, S. -C.; Lubatti, H. J.; Marx, M.; Rompotis, N.; Rosten, R.; Rothberg, J.; De Bruin, P. H. Sales; Verducci, M.; Watts, G.] Univ Washington, Dept Phys, Seattle, WA 98195 USA. [Anastopoulos, C.; Costanzo, D.; Donszelmann, T. Cuhadar; Dawson, I.; Fletcher, G. T.; Hodgkinson, M. C.; Hodgson, P.; Johansson, P.; Korolkova, E. V.; Paredes, B. Lopez; Miyagawa, P. S.; Paganis, E.; Suruliz, K.; Tovey, D. R.] Univ Sheffield, Dept Phys & Astron, Sheffield, S Yorkshire, England. [Hasegawa, Y.; Takeshita, T.] Shinshu Univ, Dept Phys, Nagano, Japan. [Atlay, N. B.; Buchholz, P.; Czirr, H.; Fleck, I.; Gaur, B.; Ibragimov, I.; Ikematsu, K.; Rosenthal, O.; Sipica, V.; Walkowiak, W.; Ziolkowski, M.] Univ Siegen, Fachbereich Phys, D-57068 Siegen, Germany. [Buat, Q.; Dawe, E.; Godfrey, J.; O'Neil, D. C.; Petteni, M.; Stelzer, B.; Tanasijczuk, A. J.; Torres, H.; Trottier-McDonald, M.; van Nieuwkoop, J.; Vetterli, M. C.] Simon Fraser Univ, Dept Phys, Burnaby, BC V5A 1S6, Canada. [Aracena, I.; Mayes, J. Backus; Barklow, T.; Bartoldus, R.; Bawa, H. S.; Black, J. E.; Campoverde, A.; Cogan, J. G.; Eifert, T.; Fulsom, B. G.; Gao, Y. S.; Garelli, N.; Grenier, P.; Kagan, M.; Kocian, M.; Koi, T.; Lowe, A. J.; Malone, C.; Mount, R.; Nelson, T. K.; Piacquadio, G.; Salnikov, A.; Schwartzman, A.; Silverstein, D.; Strauss, E.; Su, D.; Swiatlowski, M.; Wittgen, M.; Young, C.] SLAC Natl Accelerator Lab, Stanford, CA USA. [Astalos, R.; Bartos, P.; Batkova, L.; Blazek, T.; Federic, P.; Plazak, L.; Stavina, P.; Sykora, I.; Tokar, S.; Zenis, T.] Comenius Univ, Fac Math Phys & Informat, Bratislava, Slovakia. [Antos, J.; Bruncko, D.; Kladiva, E.; Strizenec, P.] Slovak Acad Sci, Inst Expt Phys, Dept Subnucl Phys, Kosice 04353, Slovakia. [Hamilton, A.] Univ Cape Town, Dept Phys, ZA-7925 Cape Town, South Africa. [Aurousseau, M.; Castaneda-Miranda, E.; Connell, S. H.; Yacoob, S.] Univ Johannesburg, Dept Phys, Johannesburg, South Africa. [Bristow, K.; Carrillo-Montoya, G. D.; Chen, X.; Garcia, B. R. Mellado; Ruan, X.; Vickey, T.; Boeriu, O. E. Vickey] Univ Witwatersrand, Sch Phys, Johannesburg, South Africa. [Abulaiti, Y.; Akerstedt, H.; Asman, B.; Bendtz, K.; Bertolia, G.; Bessidskaia, O.; Bohm, C.; Clement, C.; Cribbs, W. A.; Eriksson, D.; Gellerstedt, K.; Hellman, S.; Johanssona, K. E.; Jon-And, K.; Khandanyan, H.; Kim, H.; Klimek, P.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Petridis, A.; Plucinski, P.; Rossetti, V.; Silverstein, S. B.; Sjolin, J.; Strandberg, S.; Tylmad, M.] Stockholm Univ, Dept Phys, S-10691 Stockholm, Sweden. [Abulaiti, Y.; Akerstedt, H.; Asman, B.; Bendtz, K.; Bertolia, G.; Bessidskaia, O.; Clement, C.; Cribbs, W. A.; Gellerstedt, K.; Hellman, S.; Jon-And, K.; Khandanyan, H.; Kim, H.; Klimek, P.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Petridis, A.; Plucinski, P.; Rossetti, V.; Sjolin, J.; Strandberg, S.; Tylmad, M.] Oskar Klein Ctr, Stockholm, Sweden. [Jovicevic, J.; Kuwertz, E. S.; Lund-Jensen, B.; Morley, A. K.; Strandberg, J.] Royal Inst Technol, Dept Phys, S-10044 Stockholm, Sweden. [Bee, C. P.; Campoverde, A.; Chen, K.; Engelmann, R.; Grassi, V.; Hobbs, J.; Jia, J.; Li, H.; Lindquist, B. E.; Mastrandrea, P.; McCarthy, R. L.; Puldon, D.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA. [Bee, C. P.; Campoverde, A.; Chen, K.; Engelmann, R.; Grassi, V.; Hobbs, J.; Jia, J.; Li, H.; Lindquist, B. E.; Mastrandrea, P.; McCarthy, R. L.; Puldon, D.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.] SUNY Stony Brook, Dept Chem, Stony Brook, NY 11794 USA. [Bartsch, V.; Cerri, A.; Barajas, C. A. Chavez; De Santo, A.; Grout, Z. J.; Potter, C. J.; Salvatore, F.; Castillo, I. Santoyo; Shehu, C. Y.; Sutton, M. R.; Vivarelli, I.] Univ Sussex, Dept Phys & Astron, Brighton, E Sussex, England. [Black, C. W.; Cuthbert, C.; Finelli, K. D.; Jeng, G. -Y.; Patel, N. D.; Saavedra, A. F.; Scarcella, M.; Varvell, K. E.; Watson, I. J.; Yabsley, B.] Univ Sydney, Sch Phys, Sydney, NSW 2006, Australia. [Abdallah, J.; Chu, M. L.; Hou, S.; Jamin, D. O.; Lee, C. A.; Lee, S. C.; Li, B.; Lin, S. C.; Liu, B.; Liu, D.; Lo Sterzo, F.; Mazini, R.; Ren, Z. L.; Shi, L.; Soh, D. A.; Teng, P. K.; Wang, C.; Wang, S. M.; Weng, Z.; Zhang, L.] Acad Sinica, Inst Phys, Taipei, Taiwan. [Abreu, H.; Di Mattia, A.; Kopeliansky, R.; Musto, E.; Rozen, Y.; Tarem, S.] Technion Israel Inst Technol, Dept Phys, IL-32000 Haifa, Israel. [Abramowicz, H.; Alexander, G.; Amram, N.; Ashkenazi, A.; Bella, G.; Benary, O.; Benhammou, Y.; Davies, M.; Etzion, E.; Gershon, A.; Gueta, O.; Guttman, N.; Munwes, Y.; Oren, Y.; Sadeh, I.; Silver, Y.; Soffer, A.; Taiblum, N.] Tel Aviv Univ, Raymond & Beverly Sackler Sch Phys & Astron, IL-69978 Tel Aviv, Israel. [Bachas, K.; Gkaitatzis, S.; Gkialas, I.; Iliadis, D.; Kordas, K.; Kouskoura, V.; Leisos, A.; Nomidis, I.; Papageorgiou, K.; Petridou, C.; Sampsonidis, D.; Sidiropoulou, O.] Aristotle Univ Thessaloniki, Dept Phys, GR-54006 Thessaloniki, Greece. [Akimoto, G.; Asai, S.; Azuma, Y.; Dohmae, T.; Enari, Y.; Hanawa, K.; Kanaya, N.; Kataoka, Y.; Kawamoto, T.; Kazama, S.; Kessoku, K.; Kobayashi, T.; Komori, Y.; Mashimo, T.; Masubuchi, T.; Nakamura, T.; Ninomiya, Y.; Okuyama, T.; Sakamoto, H.; Sasaki, Y.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamaguchi, H.; Yamaguchi, Y.; Yamamoto, S.; Yamamura, T.; Yamanaka, T.; Yoshihara, K.] Univ Tokyo, Int Ctr Elementary Particle Phys, Tokyo, Japan. [Akimoto, G.; Asai, S.; Azuma, Y.; Dohmae, T.; Enari, Y.; Hanawa, K.; Kanaya, N.; Kataoka, Y.; Kawamoto, T.; Kazama, S.; Kessoku, K.; Kobayashi, T.; Komori, Y.; Mashimo, T.; Masubuchi, T.; Nakamura, T.; Ninomiya, Y.; Okuyama, T.; Sakamoto, H.; Sasaki, Y.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamaguchi, H.; Yamaguchi, Y.; Yamamoto, S.; Yamamura, T.; Yamanaka, T.; Yoshihara, K.] Univ Tokyo, Dept Phys, Tokyo 113, Japan. [Bratzler, U.; Fukunaga, C.] Tokyo Metropolitan Univ, Grad Sch Sci & Technol, Tokyo 158, Japan. [Hirose, M.; Ishitsuka, M.; Jinnouchi, O.; Kanno, T.; Kuze, M.; Nagai, R.; Nobe, T.; Pettersson, N. E.] Tokyo Inst Technol, Dept Phys, Tokyo 152, Japan. [AbouZeid, O. S.; Brelier, B.; Chau, C. C.; Ilic, N.; Keung, J.; Krieger, P.; Mc Goldrick, G.; Orr, R. S.; Polifka, R.; Rudolph, M. S.; Savard, P.; Schramm, S.; Sinervo, P.; Spreitzer, T.; Taenzer, J.; Teuscher, R. J.; Thompson, P. D.; Trischuk, W.; Venturi, N.] Univ Toronto, Dept Phys, Toronto, ON, Canada. [Azuelos, G.; Canepa, A.; Chekulaev, S. V.; Fortin, D.; Gingrich, D. M.; Koutsman, A.; Oakham, F. G.; Oram, C. J.; Codina, E. Perez; Savard, P.; Schouten, D.; Seuster, R.; Stelzer-Chilton, O.; Tafirout, R.; Trigger, I. M.; Vetterli, M. C.] TRIUMF, Vancouver, BC V6T 2A3, Canada. [Garcia, J. A. Benitez; Bustos, A. C. Florez; Ramos, J. A. Manjarres; Palacino, G.; Qureshi, A.; Taylor, W.] York Univ, Dept Phys & Astron, Toronto, ON M3J 2R7, Canada. [Hara, K.; Hayashi, T.; Kim, S. H.; Kiuchi, K.; Ukegawa, F.] Univ Tsukuba, Fac Pure & Appl Sci, Tsukuba, Ibaraki, Japan. [Beauchemin, P. H.; Hamilton, S.; Meoni, E.; Rolli, S.; Sliwa, K.; Wetter, J.] Tufts Univ, Dept Phys & Astron, Medford, MA 02155 USA. [Losada, M.; Navarro, G.; Sandoval, C.] Univ Antonio Narino, Ctr Invest, Bogota, Colombia. [Corso-Radu, A.; Farrell, S.; Gerbaudo, D.; Lankford, A. J.; Mete, A. S.; Nelson, A.; Rao, K.; Relich, M.; Scannicchio, D. A.; Schernau, M.; Shimmin, C. O.; Taffard, A.; Unel, G.; Whiteson, D.; Zhou, N.] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA USA. [Acharya, B. S.; Alhroob, M.; Brazzale, S. F.; Cobal, M.; De Sanctis, U.; Giordani, M. P.; Pinamonti, M.; Quayle, W. B.; Shaw, K.; Soualah, R.] Ist Nazl Fis Nucl, Grp Collegato Udine, Sez Trieste, Udine, Italy. [Acharya, B. S.; De Sanctis, U.; Quayle, W. B.; Shaw, K.] Abdus Salaam Int Ctr Theoret Phys, Trieste, Italy. [Alhroob, M.; Brazzale, S. F.; Cobal, M.; Giordani, M. P.; Pinamonti, M.; Soualah, R.] Univ Udine, Dipartimento Chim Fis & Ambiente, I-33100 Udine, Italy. [Atkinson, M.; Basye, A.; Benekos, N.; Cavaliere, V.; Chang, P.; Coggeshall, J.; Errede, D.; Errede, S.; Lie, K.; Liss, T. M.; Neubauer, M. S.; Shang, R.; Vichou, I.] Univ Illinois, Dept Phys, Urbana, IL 61801 USA. [Brenner, R.; Buszello, C. P.; Coniavitis, E.; Ekelof, T.; Ellert, M.; Ferrari, A.; Isaksson, C.; Madsen, A.; Ohman, H.; Pelikan, D.; Rangel-Smith, C.] Uppsala Univ, Dept Phys & Astron, Uppsala, Sweden. [Cabrera Urban, S.; Castillo Gimenez, V.; Costa, M. J.; Fassi, F.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Garcia Navarro, J. E.; Gonzalez de la Hoz, S.; Hernndez Jimenez, Y.; Higon-Rodriguez, E.; Irles Quiles, A.; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; March, L.; Marti-Garcia, S.; Mitsou, V. A.; Moles-Valls, R.; Oliver Garcia, E.; Pedraza Lopez, S.; Perez Garcia-Estan, M. T.; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, J.; Sanchez Martinez, V.; Soldevila, U.; Torro Pastor, E.; Valero, A.; Valladolid Gallego, E.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Inst Fis Corpuscular, IFIC, Valencia, Spain. [Cabrera Urban, S.; Castillo Gimenez, V.; Costa, M. J.; Fassi, F.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Garcia Navarro, J. E.; Gonzalez de la Hoz, S.; Hernndez Jimenez, Y.; Higon-Rodriguez, E.; Irles Quiles, A.; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; March, L.; Marti-Garcia, S.; Mitsou, V. A.; Moles-Valls, R.; Oliver Garcia, E.; Pedraza Lopez, S.; Perez Garcia-Estan, M. T.; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, J.; Sanchez Martinez, V.; Soldevila, U.; Torro Pastor, E.; Valero, A.; Valladolid Gallego, E.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Dept Fis Atom Mol & Nucl, Valencia, Spain. [Cabrera Urban, S.; Castillo Gimenez, V.; Costa, M. J.; Fassi, F.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Garcia Navarro, J. E.; Gonzalez de la Hoz, S.; Hernndez Jimenez, Y.; Higon-Rodriguez, E.; Irles Quiles, A.; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; March, L.; Marti-Garcia, S.; Mitsou, V. A.; Moles-Valls, R.; Oliver Garcia, E.; Pedraza Lopez, S.; Perez Garcia-Estan, M. T.; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, J.; Sanchez Martinez, V.; Soldevila, U.; Torro Pastor, E.; Valero, A.; Valladolid Gallego, E.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Dept Ingn Elect, Valencia, Spain. [Cabrera Urban, S.; Castillo Gimenez, V.; Costa, M. J.; Fassi, F.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Garcia Navarro, J. E.; Gonzalez de la Hoz, S.; Hernndez Jimenez, Y.; Higon-Rodriguez, E.; Irles Quiles, A.; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; March, L.; Marti-Garcia, S.; Mitsou, V. A.; Moles-Valls, R.; Oliver Garcia, E.; Pedraza Lopez, S.; Perez Garcia-Estan, M. T.; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, J.; Sanchez Martinez, V.; Soldevila, U.; Torro Pastor, E.; Valero, A.; Valladolid Gallego, E.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, IMB CNM, Valencia, Spain. [Fedorko, W.; Gay, C.; Gecse, Z.; King, S. B.; Lister, A.; Loh, C. W.; Swedish, S.; Viel, S.] Univ British Columbia, Dept Phys, Vancouver, BC, Canada. [Albert, J.; Bansal, V.; Berghaus, F.; Bernlochner, F. U.; David, C.; Fincke-Keeler, M.; Hamano, K.; Hill, E.; Keeler, R.; Kowalewski, R.; Lefebvre, M.; Marino, C. P.; McPherson, R. A.; Ouellette, E. A.; Pearce, J.; Sobie, R.; Venturi, M.] Univ Victoria, Dept Phys & Astron, Victoria, BC, Canada. [Farrington, S. M.; Harrison, P. F.; Janus, M.; Jeske, C.; Jones, G.; Martin, T. A.; Murray, W. J.; Pianori, E.] Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England. [Iizawa, T.; Kimura, N.; Mitani, T.; Sakurai, Y.; Yorita, K.] Waseda Univ, Tokyo, Japan. [Barak, L.; Bressler, S.; Citron, Z. H.; Duchovni, E.; Gabizon, O.; Gross, E.; Groth-Jensen, J.; Lellouch, D.; Levinson, L. J.; Mikenberg, G.; Milov, A.; Milstein, D.; Pitt, M.; Roth, I.; Schaarschmidt, J.; Smakhtin, V.] Weizmann Inst Sci, Dept Particle Phys, IL-76100 Rehovot, Israel. [Banerjee, Sw.; Castillo, L. R. Flores; Hard, A. S.; Ji, H.; Ju, X.; Kashif, L.; Kruse, A.; Ming, Y.; Pan, Y. B.; Wang, F.; Wiedenmann, W.; Wu, S. L.; Yang, H.; Zhang, F.; Zobernig, G.] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA. [Redelbach, A.; Schreyer, M.; Siragusa, G.; Stroehmer, R.; Tam, J. Y. C.; Trefzger, T.; Weber, S. W.; Zibell, A.] Univ Wurzburg, Fak Phys & Astron, D-97070 Wurzburg, Germany. [Bannoura, A. A. E.; Barisonzi, M.; Becker, K.; Beermann, T. A.; Boek, J.; Boek, T. T.; Braun, H. M.; Cornelissen, T.; Duda, D.; Ernis, G.; Fischer, J.; Fleischmann, S.; Flick, T.; Hamacher, K.; Harenberg, T.; Heim, T.; Hirschbuehl, D.; Kersten, S.; Khoroshilov, A.; Kohlmann, S.; Lenzen, G.; Maettig, P.; Neumann, M.; Pataraia, S.; Sandhoff, M.; Sartisohn, G.; Wagner, W.; Wicke, D.; Zeitnitz, C.] Berg Univ Wuppertal, Fachbereich Phys C, Wuppertal, Germany. [Adelman, J.; Baker, O. K.; Bedikian, S.; Cummings, J.; Czyczula, Z.; Demers, S.; Erdmann, J.; Garberson, F.; Golling, T.; Guest, D.; Henrichs, A.; Ideal, E.; Lagouri, T.; Lee, L.; Leister, A. G.; Loginov, A.; Tipton, P.; Wall, R.; Walsh, B.; Wang, X.] Yale Univ, Dept Phys, New Haven, CT USA. [Hakobyan, H.; Vardanyan, G.] Yerevan Phys Inst, Yerevan 375036, Armenia. [Rahal, G.] IN2P3, Ctr Calcul, Villeurbanne, France. [Acharya, B. S.] Kings Coll London, Dept Phys, London, England. [Bawa, H. S.; Gao, Y. S.; Lowe, A. J.] Calif State Univ Fresno, Dept Phys, Fresno, CA 93740 USA. [Chen, L.; Gao, J.] CNRS, IN2P3, Marseille, France. [Conventi, F.; Della Pietra, M.] Univ Napoli Parthenope, Naples, Italy. [Corriveau, F.; McPherson, R. A.; Robertson, S. H.; Sobie, R.; Teuscher, R. J.] Inst Particle Phys, Vancouver, BC, Canada. [Fedin, O. L.] St Petersburg State Polytech Univ, Dept Phys, St Petersburg, Russia. [Gkialas, I.; Papageorgiou, K.] Univ Aegean, Dept Financial & Management Engn, Chios, Greece. [Grinstein, S.; Juste Rozas, A.; Martinez, M.] ICREA, Barcelona, Spain. [Ilchenko, Y.; Onyisi, P. U. E.] Univ Texas Austin, Dept Phys, Austin, TX 78712 USA. [Jejelava, J.] Ilia State Univ, Inst Theoret Phys, Tbilisi, Rep of Georgia. [Kono, T.] Ochanomizu Univ, Ochadai Acad Prod, Tokyo 112, Japan. [Konoplich, R.] Manhattan Coll, New York, NY USA. [Korol, A. A.; Maximov, D. A.; Rezanova, O. L.; Talyshev, A. A.; Tikhonov, Yu. A.] Novosibirsk State Univ, Novosibirsk 630090, Russia. [Lin, S. C.] Acad Sinica, Inst Phys, Acad Sinica Grid Comp, Taipei, Taiwan. [Mal, P.] Natl Inst Sci Educ & Res, Sch Phys Sci, Bhubaneswar, Orissa, India. [Myagkov, A. G.; Nikolaenko, V.; Zaitsev, A. M.] State Univ, Moscow Inst Phys & Technol, Dolgoprudnyi, Russia. [Pinamonti, M.] Scuola Int Super Studi Avanzati, SISSA, Trieste, Italy. [Purohit, M.] Univ S Carolina, Dept Phys & Astron, Columbia, SC 29208 USA. [Shi, L.; Soh, D. A.; Weng, Z.] Sun Yat Sen Univ, Sch Phys & Engn, Guangzhou 510275, Guangdong, Peoples R China. [Smirnova, L. N.; Turchikhin, S.] Moscow MV Lomonosov State Univ, Fac Phys, Moscow, Russia. [Toth, J.] Inst Particle & Nucl Phys, Wigner Res Ctr Phys, Budapest, Hungary. [Wildt, M. A.] Univ Hamburg, Inst Expt Phys, Hamburg, Germany. [Yacoob, S.] Univ KwaZulu Natal, Discipline Phys, Durban, South Africa. RP Aad, G (reprint author), Aix Marseille Univ, CPPM, Marseille, France. RI Brooks, William/C-8636-2013; Connell, Simon/F-2962-2015; Bosman, Martine/J-9917-2014; Joergensen, Morten/E-6847-2015; Mitsou, Vasiliki/D-1967-2009; Riu, Imma/L-7385-2014; Cabrera Urban, Susana/H-1376-2015; Mir, Lluisa-Maria/G-7212-2015; Garcia, Jose /H-6339-2015; Marti-Garcia, Salvador/F-3085-2011; Della Pietra, Massimo/J-5008-2012; Cavalli-Sforza, Matteo/H-7102-2015; Castro, Nuno/D-5260-2011; Boyko, Igor/J-3659-2013; Nemecek, Stanislav/G-5931-2014; Gutierrez, Phillip/C-1161-2011; Di Domenico, Antonio/G-6301-2011; Ventura, Andrea/A-9544-2015; Livan, Michele/D-7531-2012; De, Kaushik/N-1953-2013; Moraes, Arthur/F-6478-2010; Smirnova, Oxana/A-4401-2013; Villa, Mauro/C-9883-2009; Wemans, Andre/A-6738-2012; White, Ryan/E-2979-2015; Li, Liang/O-1107-2015; Pacheco Pages, Andres/C-5353-2011; Vranjes Milosavljevic, Marija/F-9847-2016; Perrino, Roberto/B-4633-2010; SULIN, VLADIMIR/N-2793-2015; Nechaeva, Polina/N-1148-2015; Vykydal, Zdenek/H-6426-2016; Olshevskiy, Alexander/I-1580-2016; Snesarev, Andrey/H-5090-2013; Kantserov, Vadim/M-9761-2015; Solfaroli Camillocci, Elena/J-1596-2012; BESSON, NATHALIE/L-6250-2015; Vanadia, Marco/K-5870-2016; Ippolito, Valerio/L-1435-2016; Maneira, Jose/D-8486-2011; Prokoshin, Fedor/E-2795-2012; KHODINOV, ALEKSANDR/D-6269-2015; Staroba, Pavel/G-8850-2014; Goncalo, Ricardo/M-3153-2016; Gauzzi, Paolo/D-2615-2009; Mindur, Bartosz/A-2253-2017; Fabbri, Laura/H-3442-2012; Solodkov, Alexander/B-8623-2017; Zaitsev, Alexandre/B-8989-2017; Peleganchuk, Sergey/J-6722-2014; Monzani, Simone/D-6328-2017; Warburton, Andreas/N-8028-2013; Gorelov, Igor/J-9010-2015; Gladilin, Leonid/B-5226-2011; Carvalho, Joao/M-4060-2013; Mashinistov, Ruslan/M-8356-2015; Buttar, Craig/D-3706-2011; Gonzalez de la Hoz, Santiago/E-2494-2016; Guo, Jun/O-5202-2015; Aguilar Saavedra, Juan Antonio/F-1256-2016; Leyton, Michael/G-2214-2016; Jones, Roger/H-5578-2011; Petrucci, Fabrizio/G-8348-2012; Negrini, Matteo/C-8906-2014; Ferrer, Antonio/H-2942-2015; Grancagnolo, Sergio/J-3957-2015; Doyle, Anthony/C-5889-2009; spagnolo, stefania/A-6359-2012; Ciubancan, Liviu Mihai/L-2412-2015; Zhukov, Konstantin/M-6027-2015; Shmeleva, Alevtina/M-6199-2015; Gavrilenko, Igor/M-8260-2015; Tikhomirov, Vladimir/M-6194-2015; Yang, Haijun/O-1055-2015; Chekulaev, Sergey/O-1145-2015 OI Brooks, William/0000-0001-6161-3570; Connell, Simon/0000-0001-6000-7245; Bosman, Martine/0000-0002-7290-643X; Joergensen, Morten/0000-0002-6790-9361; Mitsou, Vasiliki/0000-0002-1533-8886; Riu, Imma/0000-0002-3742-4582; Mir, Lluisa-Maria/0000-0002-4276-715X; Della Pietra, Massimo/0000-0003-4446-3368; Castro, Nuno/0000-0001-8491-4376; Boyko, Igor/0000-0002-3355-4662; Di Domenico, Antonio/0000-0001-8078-2759; Ventura, Andrea/0000-0002-3368-3413; Livan, Michele/0000-0002-5877-0062; De, Kaushik/0000-0002-5647-4489; Moraes, Arthur/0000-0002-5157-5686; Smirnova, Oxana/0000-0003-2517-531X; Villa, Mauro/0000-0002-9181-8048; Wemans, Andre/0000-0002-9669-9500; White, Ryan/0000-0003-3589-5900; Li, Liang/0000-0001-6411-6107; Pacheco Pages, Andres/0000-0001-8210-1734; Vranjes Milosavljevic, Marija/0000-0003-4477-9733; Perrino, Roberto/0000-0002-5764-7337; SULIN, VLADIMIR/0000-0003-3943-2495; Vykydal, Zdenek/0000-0003-2329-0672; Olshevskiy, Alexander/0000-0002-8902-1793; Kantserov, Vadim/0000-0001-8255-416X; Solfaroli Camillocci, Elena/0000-0002-5347-7764; Vanadia, Marco/0000-0003-2684-276X; Ippolito, Valerio/0000-0001-5126-1620; Maneira, Jose/0000-0002-3222-2738; Prokoshin, Fedor/0000-0001-6389-5399; KHODINOV, ALEKSANDR/0000-0003-3551-5808; Goncalo, Ricardo/0000-0002-3826-3442; Gauzzi, Paolo/0000-0003-4841-5822; Mindur, Bartosz/0000-0002-5511-2611; Fabbri, Laura/0000-0002-4002-8353; Solodkov, Alexander/0000-0002-2737-8674; Zaitsev, Alexandre/0000-0002-4961-8368; Peleganchuk, Sergey/0000-0003-0907-7592; Monzani, Simone/0000-0002-0479-2207; Warburton, Andreas/0000-0002-2298-7315; Gorelov, Igor/0000-0001-5570-0133; Gladilin, Leonid/0000-0001-9422-8636; Carvalho, Joao/0000-0002-3015-7821; Mashinistov, Ruslan/0000-0001-7925-4676; Gonzalez de la Hoz, Santiago/0000-0001-5304-5390; Guo, Jun/0000-0001-8125-9433; Aguilar Saavedra, Juan Antonio/0000-0002-5475-8920; Leyton, Michael/0000-0002-0727-8107; Jones, Roger/0000-0002-6427-3513; Petrucci, Fabrizio/0000-0002-5278-2206; Negrini, Matteo/0000-0003-0101-6963; Ferrer, Antonio/0000-0003-0532-711X; Grancagnolo, Sergio/0000-0001-8490-8304; Doyle, Anthony/0000-0001-6322-6195; spagnolo, stefania/0000-0001-7482-6348; Ciubancan, Liviu Mihai/0000-0003-1837-2841; Tikhomirov, Vladimir/0000-0002-9634-0581; FU ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWF, Austria; FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq, Brazil; FAPESP, Brazil; NSERC, Canada; NRC, Canada; CFI, Canada; CERN; CONICYT, Chile; CAS, China; MOST, China; NSFC, China; COL-CIENCIAS, Colombia; MSMT CR, Czech Republic; MPO CR, Czech Republic; VSC CR, Czech Republic; DNRF, Denmark; DNSRC, Denmark; Lundbeck Foundation, Denmark; EPLANET; ERC; NSRF; European Union; IN2P3-CNRS, France; CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, Germany; DFG, Germany; HGF, Germany; MPG, Germany; AvH Foundation, Germany; GSRT, Greece; NSRF, Greece; ISF, Israel; MINERVA, Israel; GIF, Israel; I-CORE, Israel; Benoziyo Center, Israel; INFN, Italy; MEXT, Japan; JSPS, Japan; CNRST, Morocco; FOM, Netherlands; NWO, Netherlands; BRF, Norway; RCN, Norway; MNiSW, Poland; NCN, Poland; GRICES, Portugal; FCT, Portugal; MNE/IFA, Romania; MES of Russia; ROSATOM, Russian Federation; JINR; MSTD, Serbia; MSSR, Slovakia; ARRS, Slovenia; MIZS, Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC, Sweden; Wallenberg Foundation, Sweden; SER, Switzerland; SNSF, Switzerland; Cantons of Bern and Geneva, Switzerland; NSC, Taiwan; TAEK, Turkey; STFC, United Kingdom; Royal Society, United Kingdom; Leverhulme Trust, United Kingdom; DOE, United States; NSF, United States FX We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWF and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile; CAS, MOST and NSFC, China; COL-CIENCIAS, Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF, DNSRC and Lundbeck Foundation, Denmark; EPLANET, ERC and NSRF, European Union; IN2P3-CNRS, CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, DFG, HGF, MPG and AvH Foundation, Germany; GSRT and NSRF, Greece; ISF, MINERVA, GIF, I-CORE and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; FOM and NWO, Netherlands; BRF and RCN, Norway; MNiSW and NCN, Poland; GRICES and FCT, Portugal; MNE/IFA, Romania; MES of Russia and ROSATOM, Russian Federation; JINR; MSTD, Serbia; MSSR, Slovakia; ARRS and MIZS, Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC and Wallenberg Foundation, Sweden; SER, SNSF and Cantons of Bern and Geneva, Switzerland; NSC, Taiwan; TAEK, Turkey; STFC, the Royal Society and Leverhulme Trust, United Kingdom; DOE and NSF, United States. NR 40 TC 5 Z9 5 U1 8 U2 87 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0370-2693 EI 1873-2445 J9 PHYS LETT B JI Phys. Lett. B PD NOV 10 PY 2014 VL 738 BP 25 EP 43 DI 10.1016/j.physletb.2014.09.020 PG 19 WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AT0KK UT WOS:000344624900005 ER PT J AU Aad, G Abbott, B Abdallah, J Khalek, SA Abdinov, O Aben, R Abi, B Abolins, M AbouZeid, OS Abramowicz, H Abreu, H Abreu, R Abulaiti, Y Acharya, BS Adamczyk, L Adams, DL Adelman, J Adomeit, S Adye, T Adye, T Aguilar-Saavedra, JA Agustoni, M Ahlen, SP Ahmadov, F Aielli, G Akerstedt, H Akesson, TP Akimoto, G Akimov, AV Alberghi, GL Albert, J Albrand, S Verzini, MJA Aleksa, M Aleksandrov, IN Alexa, C Alexander, G Alexandre, G Alexopoulos, T Alhroob, M Alimonti, G Alio, L Alison, J Allbrooke, BMM Allison, LJ Allport, PP Almond, J Aloisio, A Alonso, A Alonso, F Alpigiani, C Altheimer, A Gonzalez, BA Alviggi, MG Amako, K Coutinho, YA Amelung, C Amidei, D Dos Santos, SPA Amorim, A Amoroso, S Amram, N Amundsen, G Anastopoulos, C Ancu, LS Andari, N Andeen, T Anders, CF Anders, G Anderson, KJ Andreazza, A Andrei, V Anduaga, XS Angelidakis, S Angelozzi, I Anger, P Angerami, A Anghinolfi, F Anisenkov, AV Anjos, N Annovi, A Antonaki, A Antonelli, M Antonov, A Antos, J Anulli, F Aoki, M Bella, LA Apolle, R Arabidze, G Aracena, I Arai, Y Araque, JP Arce, ATH Arguin, JF Argyropoulos, S Arik, M Armbruster, AJ Arnaez, O Arnal, V Arnold, H Arratia, M Arslan, O Artamonov, A Artoni, G Asai, S Asbah, N Ashkenazi, A Asman, B Asquith, L Assamagan, K Astalos, R Atkinson, M Atlay, NB Auerbach, B Augsten, K Aurousseau, M Avolio, G Azuelos, G Azuma, Y Baak, MA Baas, A Bacci, C Bachacou, H Bachas, K Backes, M Backhaus, M Mayes, JB Badescu, E Bagiacchi, P Bagnaia, P Bai, Y Bain, T Baines, JT Baker, OK Balek, P Balli, F Banas, E Banerjee, S Bannoura, AAE Bansal, V Bansil, HS Barak, L Baranov, SP Barberio, EL Barberis, D Barbero, M Barillari, T Barisonzi, M Barklow, T Barlow, N Barnett, BM Barnett, RM Barnovska, Z Baroncelli, A Barone, G Barr, AJ Barreiro, F da Costa, JBG Bartoldus, R Barton, AE Bartos, P Bartsch, V Bassalat, A Basye, A Bates, RL Batley, JR Battaglia, M Battistin, M Bauer, F Bawa, HS Beattie, MD Beau, T Beauchemin, PH Beccherle, R Bechtle, P Beck, HP Becker, K Becker, S Beckingham, M Becot, C Beddall, AJ Beddall, A Bedikian, S Bednyakov, VA Bee, CP Beemster, LJ Beermann, TA Begel, M Behr, K Belanger-Champagne, C Bell, PJ Bell, WH Bella, G Bellagamba, L Bellerive, A Bellomo, M Belotskiy, K Beltramello, O Benary, O Benchekroun, D Bendtz, K Benekos, N Benhammou, Y Noccioli, EB Garcia, JAB Benjamin, DP Bensinger, JR Benslama, K Bentvelsen, S Berge, D Kuutmann, EB Berger, N Berghaus, F Beringer, J Bernard, C Bernat, P Bernius, C Bernlochner, FU Berry, T Berta, P Bertella, C Bertoli, G Bertolucci, F Bertsche, C Bertsche, D Besana, MI Besjes, GJ Bessidskaia, O Bessner, MF Besson, N Betancourt, C Bethke, S Bhimji, W Bianchi, RM Bianchini, L Bianco, M Biebel, O Bieniek, SP Bierwagen, K Biesiada, J Biglietti, M De Mendizabal, JB Bilokon, H Bindi, M Binet, S Bingul, A Bini, C Black, CW Black, JE Black, KM Blackburn, D Blair, RE Blanchard, JB Blazek, T Bloch, I Blocker, C Blum, W Blumenschein, U Bobbink, GJ Bobrovnikov, VS Bocchetta, SS Bocci, A Bock, C Boddy, CR Boehler, M Boek, TT Bogaerts, JA Bogdanchikov, AG Bogouch, A Bohm, C Bohm, J Boisvert, V Bold, T Boldea, V Boldyrev, AS Bomben, M Bona, M Boonekamp, M Borisov, A Borissov, G Borri, M Borroni, S Bortfeldt, J Bortolotto, V Bos, K Boscherini, D Bosman, M Boterenbrood, H Boudreau, J Bouffard, J Bouhova-Thacker, EV Boumediene, D Bourdarios, C Bousson, N Boutouil, S Boveia, A Boyd, J Boyko, IR Bracinik, J Brandt, A Brandt, G Brandt, O Bratzler, U Brau, B Brau, JE Braun, HM Brazzale, SF Brelier, B Brendlinger, K Brennan, AJ Brenner, R Bressler, S Bristow, K Bristow, TM Britton, D Brochu, FM Brock, I Brock, R Bromberg, C Bronner, J Brooijmans, G Brooks, T Brooks, WK Brosamer, J Brost, E Brown, J de Renstrom, PAB Bruncko, D Bruneliere, R Brunet, S Bruni, A Bruni, G 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Colombo, T Colon, G Compostella, G Muino, PC Coniavitis, E Conidi, MC Connell, SH Connelly, IA Consonni, SM Consorti, V Constantinescu, S Conta, C Conti, G Conventi, F Cooke, M Cooper, BD Cooper-Sarkar, AM Cooper-Smith, NJ Copic, K Cornelissen, T Corradi, M Corriveau, F Corso-Radu, A Cortes-Gonzalez, A Cortiana, G Costa, G Costa, MJ Costanzo, D Cote, D Cottin, G Cowan, G Cox, BE Cranmer, K Cree, G Crepe-Renaudin, S Crescioli, F Cribbs, WA Ortuzar, MC Cristinziani, M Croft, V Crosetti, G Cuciuc, CM Donszelmann, TC Cummings, J Curatolo, M Cuthbert, C Czirr, H Czodrowski, P Czyczula, Z D'Auria, S D'Onofrio, M De Sousa, MJDS Da Via, C Dabrowski, W Dafinca, A Dai, T Dai, T Dallaire, F Dallapiccola, C Dam, M Daniells, AC DanoHoffmann, M Dao, V Darbo, G Darmora, S Dassoulas, JA Dattagupta, A Davey, W David, C Davidek, T Davies, E Davies, M Davignon, O Davison, AR Davison, P Davygora, Y Dawe, E Dawson, I Daya-Ishmukhametova, RK De, K de Asmundis, R De Castro, S De Cecco, S De Groot, N de Jong, 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CA ATLAS Collaboration TI Search for the Standard Model Higgs boson decay to mu(+)mu(-) with the ATLAS detector SO PHYSICS LETTERS B LA English DT Article ID HADRON COLLIDERS; QCD CORRECTIONS; NNLO QCD; LHC; SYMMETRIES; MASS AB A search is reported for Higgs boson decay to mu(+)mu(-) using data with an integrated luminosity of 24.8 fb(-1) collected with the ATLAS detector in pp collisions at root s = 7 and 8 TeV at the CERN Large Hadron Collider. The observed dimuon invariant mass distribution is consistent with the Standard Model background-only hypothesis in the 120-150 GeV search range. For a Higgs boson with a mass of 125.5 GeV, the observed (expected) upper limit at the 95% confidence level is 7.0 (7.2) times the Standard Model expectation. This corresponds to an upper limit on the branching ratio BR(H -> mu(+)mu(-)) of 1.5 x10(-3). Published by Elsevier B.V. C1 [Bouffard, J.; Edson, W.; Ernst, J.; Fischer, A.; Guindon, S.; Jain, V.] SUNY Albany, Dept Phys, Albany, NY 12222 USA. 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S.; Kondrashova, N.; Kuhl, T.; Lisovyi, M.; Lobodzinska, E.; Lohwasser, K.; Medinnis, M.; Moenig, K.; Naumann, T.; Peschke, R.; Petit, E.; Radescu, V.; Rubinskiy, I.; Schaefer, R.; Sedov, G.; Shushkevich, S.; South, D.; Stanescu-Bellu, M.; Stanitzki, M. M.; Starovoitov, P.; Styles, N. A.; Tackmann, K.; Vankov, P.; Wang, J.; Wasicki, C.; Wildt, M. A.; Yildirim, E.] DESY, Zeuthen, Germany. [Burmeister, I.; Esch, H.; Goessling, C.; Jentzsch, J.; Jung, C. A.; Klingenberg, R.; Wittig, T.] Tech Univ Dortmund, Inst Expt Phys 4, Dortmund, Germany. [Anger, P.; Friedrich, F.; Grohs, J. P.; Gumpert, C.; Kobel, M.; Leonhardt, K.; Mader, W. F.; Morgenstern, M.; Novgorodova, O.; Rudolph, C.; Schnoor, U.; Siegert, F.; Socher, F.; Staerz, S.; Straessner, A.; Vest, A.; Wahrmund, S.] Tech Univ Dresden, Inst Kern & Teilchenphys, D-01062 Dresden, Germany. [Arce, A. T. H.; Benjamin, D. P.; Bocci, A.; Cerio, B.; Kajomovitz, E.; Kotwal, A.; Kruse, M. C.; Li, L.; Li, S.; Liu, M.; Oh, S. H.; Pollard, C. S.; Wang, C.] Duke Univ, Dept Phys, Durham, NC 27706 USA. [Bhimji, W.; Bristow, T. M.; Clark, P. J.; Dias, F. A.; Edwards, N. C.; Walls, F. M. Garay; Glaysher, P. C. F.; Harrington, R. D.; Leonidopoulos, C.; Martin, V. J.; Mills, C.; O'Brien, B. J.; Pino, S. A. Olivares; Proissl, M.; Selbach, K. E.; Smart, B. H.; Washbrook, A.; Wynne, B. M.] Univ Edinburgh, Sch Phys & Astron, SUPA, Edinburgh, Midlothian, Scotland. [Annovi, A.; Antonelli, M.; Bilokon, H.; Chiarella, V.; Curatolo, M.; Di Nardo, R.; Esposito, B.; Gatti, C.; Laurelli, P.; Maccarrone, G.; Prokofiev, K.; Sansoni, A.; Testa, M.; Vilucchi, E.] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy. [Amoroso, S.; Arnold, H.; Betancourt, C.; Boehler, M.; Bruneliere, R.; Buehrer, F.; Buescher, D.; Coniavitis, E.; Consorti, V.; Di Simone, A.; Fehling-Kaschek, M.; Flechl, M.; Giuliani, C.; Herten, G.; Jakobs, K.; Javurek, T.; Jenni, P.; Kiss, F.; Koeneke, K.; Kopp, A. K.; Kuehn, S.; Lai, S.; Landgraf, U.; Madar, R.; Mahboubi, K.; Mohr, W.; Pagacova, M.; Parzefall, U.; Rave, T. C.; Ronzani, M.; Ruehr, F.; Rurikova, Z.; Ruthmann, N.; Schillo, C.; Schmidt, E.; Schumacher, M.; Sommer, P.; Sundermann, J. E.; Temming, K. K.; Tsiskaridze, V.; Ungaro, F. C.; von Radziewski, H.; Anh, T. Vu; Warsinsky, M.; Weiser, C.; Werner, M.; Zimmermann, S.] Univ Freiburg, Fak Math & Phys, D-79106 Freiburg, Germany. [Alexandre, G.; Ancu, L. S.; Barone, G.; Bell, P. J.; Bell, W. H.; Noccioli, E. Benhar; De Mendizabal, J. Bilbao; Bucci, F.; Toro, R. Camacho; Clark, A.; Delitzsch, C. M.; della Volpe, D.; Doglioni, C.; Ferrere, D.; Gadomski, S.; Gonzalez-Sevilla, S.; Goulette, M. P.; Gramling, J.; Guescini, F.; Iacobucci, G.; Katre, A.; La Rosa, A.; Mermod, P.; Miucci, A.; Muenstermann, D.; Nektarijevic, S.; Nessi, M.; Nikolics, K.; Picazio, A.; Pohl, M.; Rosbach, K.; Tykhonov, A.; Vallecorsa, S.; Wu, X.] Univ Geneva, Sect Phys, Geneva, Switzerland. [Barberis, D.; Darbo, G.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Gemme, C.; Guido, E.; Morettini, P.; Osculatia, B.; Parodi, F.; Passaggio, S.; Rossi, L. P.; Schiavi, C.] Univ Genoa, Ist Nazl Fis Nucl, Sez Genova, Genoa, Italy. [Barberis, D.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Guido, E.; Osculatia, B.; Parodi, F.; Schiavi, C.] Univ Genoa, Dipartimento Fis, Genoa, Italy. [Jejelava, J.; Tskhadadze, E. G.] Iv Javakhishvili Tbilisi State Univ, E Andronikashvili Inst Phys, Tbilisi, Rep of Georgia. [Djobava, T.; Durglishvili, A.; Khubuab, J.; Mosidze, M.] Tbilisi State Univ, Inst High Energy Phys, Tbilisi, Rep of Georgia. [Dueren, M.; Kreutzfeldt, K.; Stenzel, H.] Univ Giessen, Inst Phys 2, Giessen, Germany. [Bates, R. L.; Britton, D.; Buckley, A. G.; Bussey, P.; Buttar, C. M.; Buzatu, A.; Cinca, D.; D'Auria, S.; Doherty, T.; Doyle, A. T.; Ferrag, S.; Ferrando, J.; de Lima, D. E. Ferreira; Gemmell, A.; Gul, U.; Ortiz, N. G. Gutierrez; Kar, D.; Knue, A.; O'Shea, V.; Barrera, C. Oropeza; Qin, G.; Quilty, D.; Ravenscroft, T.; Robson, A.; Saxon, D. H.; Smith, K. M.; Denis, R. D. St.; Stewart, G. A.; Thompson, A. S.; Wright, M.] Univ Glasgow, Sch Phys & Astron, SUPA, Glasgow, Lanark, Scotland. [Bierwagen, K.; Bindi, M.; Blumenschein, U.; George, M.; Graber, L.; Grosse-Knetter, J.; Hamer, M.; Hensel, C.; Kawamura, G.; Keil, M.; Kroeninger, K.; Lemmer, B.; Magradze, E.; Mchedlidze, G.; Llacer, M. Moreno; Nackenhorst, O.; Nadal, J.; Quadt, A.; Rieger, J.; Schorlemmer, A. L. S.; Serkin, L.; Shabalina, E.; Stolte, P.; Schroeder, T. Vazquez; Weingarten, J.; Zinonos, Z.] Univ Gottingen, Inst Phys 2, Gottingen, Germany. [Albrand, S.; Brown, J.; Collot, J.; Crepe-Renaudin, S.; Dechenaux, B.; Delsart, P. A.; Gabaldon, C.; Genest, M. H.; Hostachy, J-Y.; Ledroit-Guillon, F.; Lleres, A.; Lucotte, A.; Malek, F.; Monini, C.; Stark, J.; Trocme, B.; Wu, M.] Univ Grenoble Alpes, CNRS, IN2P3, Lab Phys Subatom & Cosmol, Grenoble, France. [McFarlane, K. W.] Hampton Univ, Dept Phys, Hampton, VA 23668 USA. [da Costa, J. Barreiro Guimaraes; Butler, B.; Catastini, P.; Conti, G.; Franklin, M.; Huth, J.; Ippolito, V.; Mateos, D. Lopez; Mercurio, K. M.; Morii, M.; Skottowe, H. P.; Spearman, W. R.; Sun, S.; Yen, A. L.; della Porta, G. Zevi] Harvard Univ, Lab Particle Phys & Cosmol, Cambridge, MA 02138 USA. [Andrei, V.; Baas, A.; Brandt, O.; Davygora, Y.; Dietzsch, T. A.; Dunford, M.; Hanke, P.; Hofmann, J. I.; Jongmanns, J.; Khomich, A.; Kluge, E. -E.; Laier, H.; Lang, V. S.; Meier, K.; Mueller, F.; Poddar, S.; Scharf, V.; Schultz-Coulon, H. -C.; Stamen, R.; Wessels, M.] Heidelberg Univ, Kirchhoff Inst Phys, Heidelberg, Germany. [Anders, C. F.; Giulini, M.; Kasieczka, G.; Narayan, R.; Schaetzel, S.; Schmitt, S.; Schoening, A.] Heidelberg Univ, Inst Phys, Heidelberg, Germany. [Colombo, T.; Kretz, M.; Kugel, A.] Heidelberg Univ, ZITI Inst Tech Informat, Mannheim, Germany. [Nagasaka, Y.] Hiroshima Inst Technol, Fac Appl Informat Sci, Hiroshima, Japan. [Brunet, S.; Dattagupta, A.; Evans, H.; Gagnon, P.; Lammers, S.; Martinez, N. Lorenzo; Luehring, F.; Ogren, H.; Penwell, J.; Poveda, J.; Weinert, B.; Zieminska, D.] Indiana Univ, Dept Phys, Bloomington, IN USA. [Franz, S.; Jussel, P.; Kneringer, E.; Lukas, W.; Nagai, K.; Ritsch, E.; Usanova, A.] Leopold Franzens Univ, Inst Astro & Teilchenphys, Innsbruck, Austria. [Mallik, U.; Mandrysch, R.; Morange, N.; Zaidan, R.] Univ Iowa, Iowa City, IA USA. [Chen, C.; Cochran, J.; De Lorenzi, F.; Dudziak, F.; Krumnack, N.; Prell, S.; Shrestha, S.; Yamamoto, K.] Iowa State Univ, Dept Phys & Astron, Ames, IA USA. [Ahmadov, F.; Aleksandrov, I. N.; Bednyakov, V. A.; Boyko, I. R.; Budagov, I. A.; Chelkov, G. A.; Cheplakov, A.; Chizhov, M. V.; Dedovich, D. V.; Demichev, M.; Glonti, G. L.; Gostkin, M. I.; Huseynov, N.; Javadov, N.; Karpov, S. N.; Karpova, Z. M.; Kazarinov, M. Y.; Khramov, E.; Kotov, V. M.; Kruchonak, U.; Krumshteyn, Z. V.; Kukhtin, V.; Ladygin, E.; Minashvili, I. A.; Mineev, M.; Olchevski, A. G.; Peshekhonov, V. D.; Plotnikova, E.; Potrap, I. N.; Pozdnyakov, V.; Rusakovich, N. A.; Sadykov, R.; Sapronov, A.; Shiyakova, M.; Sisakyan, A. N.; Soloshenko, A.; Topilin, N. D.; Vinogradov, V. B.; Zhemchugov, A.; Zimine, N. I.] Joint Inst Nucl Res Dubna, Dubna, Russia. [Amako, K.; Aoki, M.; Arai, Y.; Ikegami, Y.; Ikeno, M.; Iwasaki, H.; Kanzaki, J.; Kohriki, T.; Kondo, T.; Kono, T.; Makida, Y.; Mitsui, S.; Nagano, K.; Nakamura, K.; Nozaki, M.; Odaka, S.; Sasaki, O.; Suzuki, Y.; Takubo, Y.; Tanaka, S.; Terada, S.; Tokushuku, K.; Tsuno, S.; Unno, Y.; Yamada, M.; Yamamoto, A.; Yasu, Y.] High Energy Accelerator Res Org, KEK, Tsukuba, Ibaraki, Japan. [Chen, Y.; Hasegawa, M.; Inamaru, Y.; Kishimoto, T.; Kurashige, H.; Kurumida, R.; Ochi, A.; Shimizu, S.; Takeda, H.; Yakabe, R.; Yamazaki, Y.; Yuan, L.] Kobe Univ, Grad Sch Sci, Kobe, Hyogo 657, Japan. [Ishino, M.; Sumida, T.; Tashiro, T.] Kyoto Univ, Fac Sci, Kyoto, Japan. [Takashima, R.] Kyoto Univ, Kyoto 612, Japan. [Kawagoe, K.; Oda, S.; Otono, H.; Tojo, J.] Kyushu Univ, Dept Phys, Fukuoka 812, Japan. [Alconada Verzini, M. J.; Alonso, F.; Anduaga, X. S.; Dova, M. T.; Monticelli, F.; Wahlberg, H.] Univ Nacl La Plata, Inst Fis La Plata, La Plata, Buenos Aires, Argentina. [Alconada Verzini, M. J.; Alonso, F.; Anduaga, X. S.; Dova, M. T.; Monticelli, F.; Wahlberg, H.] Consejo Nacl Invest Cient & Tecn, La Plata, Buenos Aires, Argentina. [Allison, L. J.; Barton, A. E.; Beattie, M. D.; Borissov, G.; Bouhova-Thacker, E. V.; Chilingarov, A.; Dearnaley, W. J.; Fox, H.; Grimm, K.; Henderson, R. C. W.; Hughes, G.; Jones, R. W. L.; Kartvelishvili, V.; Long, R. E.; Love, P. A.; Maddocks, H. J.; Smizanska, M.; Walder, J.] Univ Lancaster, Dept Phys, Lancaster, England. [Gorini, E.; Orlando, N.; Perrino, R.; Primavera, M.; Spagnolo, S.; Ventura, A.] Univ Salento, Ist Nazl Fis Nucl, Sez Lecce, Lecce, Italy. [Gorini, E.; Orlando, N.; Spagnolo, S.; Ventura, A.] Univ Salento, Dipartimento Matemat & Fis, Lecce, Italy. [Allport, P. P.; Bundock, A. C.; Burdin, S.; D'Onofrio, M.; Dervan, P.; Gwilliam, C. B.; Hayward, H. S.; Jackson, M.; Jones, T. J.; King, B. T.; Klein, M.; Klein, U.; Kretzschmar, J.; Laycock, P.; Lehan, A.; Mahmoud, S.; Maxfield, S. J.; Mehta, A.; Migas, S.; Price, J.; Readioff, N. P.; Schnellbach, Y. J.; Sellers, G.; Vossebeld, J. H.; Waller, P.] Univ Liverpool, Oliver Lodge Lab, Liverpool L69 3BX, Merseyside, England. [Cindro, V.; Deliyergiyev, M.; Filipcic, A.; Gorisek, A.; Kersevan, B. P.; Kramberger, G.; Mandic, I.; Mikuz, M.; Sfiligoj, T.] Jozef Stefan Inst, Dept Phys, Ljubljana, Slovenia. [Cindro, V.; Deliyergiyev, M.; Filipcic, A.; Gorisek, A.; Kersevan, B. P.; Kramberger, G.; Mandic, I.; Mikuz, M.; Sfiligoj, T.] Univ Ljubljana, Ljubljana, Slovenia. [Alpigiani, C.; Bona, M.; Bret, M. Cano; Cerrito, L.; Fletcher, G.; Goddard, J. R.; Hickling, R.; Landon, M. P. J.; Lloyd, S. L.; Morris, J. D.; Piccaro, E.; Rizvi, E.; Sandbach, R. L.; Snidero, G.; Castanheira, M. Teixeira Dias] Queen Mary Univ London, Sch Phys & Astron, London, England. [Berry, T.; Boisvert, V.; Brooks, T.; Connelly, I. A.; Cooper-Smith, N. J.; Cowan, G.; Duguid, L.; George, S.; Gibson, S. M.; Kempster, J. J.; Vazquez, J. G. Panduro; Pastore, Fr.; Rose, M.; Teixeira-Dias, P.; Thomas-Wilsker, J.] Royal Holloway Univ London, Dept Phys, Surrey, England. [Bernat, P.; Bieniek, S. P.; Butterworth, J. M.; Campanelli, M.; Casadei, D.; Chislett, R. T.; Cooper, B. D.; Davison, A. R.; Davison, P.; Falla, R. J.; Gregersen, K.; Gutschow, C.; Hesketh, G. G.; Jansen, E.; Konstantinidis, N.; Korn, A.; Lambourne, L.; Leney, K. J. C.; Martyniuk, A. C.; Mcfayden, J. A.; Nurse, E.; Ochoa, M. I.; Pilkington, A. D.; Scanlon, T.; Sherwood, P.; Simmons, B.; Wardrope, D. R.; Waugh, B. M.; Wijeratne, P. A.] UCL, Dept Phys & Astron, London, England. [Bernius, C.; Greenwood, Z. D.; Jana, D. K.; Sawyer, L.; Sircar, A.; Subramaniam, R.] Louisiana Tech Univ, Ruston, LA 71270 USA. [Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; Davignon, O.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Liu, K.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Vannucci, F.; Varouchas, D.] UPMC, Lab Phys Nucl & Hautes Energies, Paris, France. [Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; Davignon, O.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Liu, K.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Vannucci, F.; Varouchas, D.] Univ Paris Diderot, Paris, France. [Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; Davignon, O.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Liu, K.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Vannucci, F.; Varouchas, D.] CNRS, IN2P3, Paris, France. [Akesson, T. P.; Bocchetta, S. S.; Bryngemark, L.; Floderus, A.; Hawkins, A. D.; Hedberg, V.; Ivarsson, J.; Jarlskog, G.; Lytken, E.; Meirose, B.; Mjornmark, J. U.; Smirnova, O.; Viazlo, O.] Lund Univ, Inst Fys, Lund, Sweden. [Arnal, V.; Barreiro, F.; Cantero, J.; De la Torre, H.; Del Peso, J.; Glasman, C.; Merino, J. Llorente; Terron, J.] Univ Autonoma Madrid, Dept Fis Teor C 15, Madrid, Spain. [Aloisio, A.; Blum, W.; Buescher, V.; Caputo, R.; Ellinghaus, F.; Endner, O. C.; Ertel, E.; Fiedler, F.; Torregrosa, E. Fullana; Goeringer, C.; Heck, T.; Hohlfeld, M.; Hsu, P. J.; Huelsing, T. A.; Karnevskiy, M.; Kleinknecht, K.; Koenig, S.; Koepke, L.; Lin, T. H.; Masetti, L.; Mattmann, J.; Meyer, C.; Moreno, D.; Moritz, S.; Mueller, T.; Poettgen, R.; Sander, H. G.; Schaefer, U.; Schmitt, C.; Schott, M.; Schroeder, C.; Schuh, N.; Simioni, E.; Tapprogge, S.; Wollstadt, S. J.; Zimmermann, C.] Johannes Gutenberg Univ Mainz, Inst Phys, D-55122 Mainz, Germany. [Almond, J.; Aloisio, A.; Alonso, A.; Borri, M.; Cox, B. E.; Da Via, C.; Forti, A.; Ponce, J. M. Iturbe; Joshi, K. D.; Klinger, J. A.; Loebinger, F. K.; Marsden, S. P.; Masik, J.; Neep, T. J.; Oh, A.; Owen, M.; Pater, J. R.; Peters, R. F. Y.; Price, D.; Qin, Y.; Queitsch-Maitland, M.; Robinson, J. E. M.; Schwanenberger, C.; Tomlinson, L.; Watts, S.; Webb, S.; Woudstra, M. J.; Wyatt, T. R.; Yang, U. K.] Univ Manchester, Sch Phys & Astron, Manchester, Lancs, England. [Aad, G.; Alio, L.; Barbero, M.; Bertella, C.; Chen, L.; Clemens, J. C.; Coadou, Y.; Diglio, S.; Djama, F.; Feligioni, L.; Gao, J.; Hoffmann, D.; Hubaut, F.; Knoops, E. B. F. G.; Le Guirriec, E.; Li, B.; Madaffari, D.; Mochizuki, K.; Monnier, E.; Muanza, S.; Nagai, Y.; Pralavorio, P.; Rozanov, A.; Serre, T.; Talby, M.; Tiouchichine, E.; Tisserant, S.; Toth, J.; Touchard, F.; Ughetto, M.; Vacavant, L.] Aix Marseille Univ, CPPM, Marseille, France. [Aad, G.; Alio, L.; Barbero, M.; Bertella, C.; Chen, L.; Clemens, J. C.; Coadou, Y.; Diglio, S.; Djama, F.; Feligioni, L.; Gao, J.; Hoffmann, D.; Hubaut, F.; Knoops, E. B. F. G.; Le Guirriec, E.; Li, B.; Madaffari, D.; Mochizuki, K.; Monnier, E.; Muanza, S.; Nagai, Y.; Pralavorio, P.; Rozanov, A.; Serre, T.; Talby, M.; Tiouchichine, E.; Tisserant, S.; Toth, J.; Touchard, F.; Ughetto, M.; Vacavant, L.] CNRS, IN2P3, Marseille, France. [Bellomo, M.; Brau, B.; Colon, G.; Dallapiccola, C.; Daya-Ishmukhametova, R. K.; Meade, A.; Moyse, E. J. W.; Pais, P.; Pueschel, E.; Varol, T.; Ventura, D.; Willocq, S.] Univ Massachusetts, Dept Phys, Amherst, MA 01003 USA. [Belanger-Champagne, C.; Chapleau, B.; Cheatham, S.; Corriveau, F.; Mantifel, R.; Robertson, S. H.; Robichaud-Veronneau, A.; Stockton, M. C.; Stoebe, M.; Vachon, B.; Wang, K.; Warburton, A.] McGill Univ, Dept Phys, Montreal, PQ, Canada. [Aloisio, A.; Barberio, E. L.; Brennan, A. J.; Jennens, D.; Kubota, T.; Limosani, A.; Hanninger, G. Nunes; Nuti, F.; Rados, P.; Spiller, L. A.; Tan, K. G.; Taylor, G. N.; Thong, W. M.; Urquijo, P.; Volpi, M.] Univ Melbourne, Sch Phys, Melbourne, Vic 3010, Australia. [Amidei, D.; Chelstowska, M. A.; Cheng, H. C.; Dai, T.; Diehl, E. B.; Dubbert, J.; Feng, H.; Ferretti, C.; Fleischmann, P.; Goldfarb, S.; Harper, D.; Levin, D.; Liu, L.; Long, J. D.; Lu, N.; Mc Kee, S. P.; McCarn, A.; Neal, H. A.; Panikashvili, N.; Qian, J.; Searcy, J.; Thun, R. P.; Wilson, A.; Wu, Y.; Xu, L.; Yu, J. M.; Zhang, D.; Zhou, B.; Zhu, J.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA. [Abolins, M.; Gonzalez, B. Alvarez; Arabidze, G.; Brock, R.; Bromberg, C.; Caughron, S.; Chegwidden, A.; Fisher, W. C.; Halladjian, G.; Hauser, R.; Hayden, D.; Huston, J.; Koll, J.; Linnemann, J. T.; Martin, B.; Pope, B. G.; Schoenrock, B. D.; Schwienhorst, R.; Ta, D.; Tollefson, K.; True, P.; Willis, C.; Zhang, H.] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA. [Alimonti, G.; Andreazza, A.; Besana, M. I.; Carminati, L.; Cavalli, D.; Citterio, M.; Consonni, S. M.; Costa, G.; Fanti, M.; Giugni, D.; Lari, T.; Mandelli, L.; Meroni, C.; Perini, L.; Pizio, C.; Ragusa, F.; Resconi, S.; Simoniello, R.; Tartarelli, G. F.; Troncon, C.; Turra, R.; Perez, M. Villaplana] Univ Milan, Ist Nazl Fis Nucl, Sez Milano, Milan, Italy. [Andreazza, A.; Carminati, L.; Consonni, S. M.; Fanti, M.; Perini, L.; Pizio, C.; Ragusa, F.; Simoniello, R.; Turra, R.; Perez, M. Villaplana] Univ Milan, Dipartimento Fis, Milan, Italy. [Bogouch, A.; Harkusha, S.; Kulchitsky, Y.; Kurochkin, Y. A.; Tsiareshka, P. V.] Natl Acad Sci Belarus, BI Stepanov Inst Phys, Minsk, Byelarus. [Yanush, S.] Natl Sci & Educ Ctr Particle & High Energy Phys, Minsk, Byelarus. [Taylor, F. E.] MIT, Dept Phys, Cambridge, MA 02139 USA. [Arguin, J-F.; Azuelos, G.; Dallaire, F.; Gauthier, L.; Leroy, C.; Rezvani, R.; Soueid, P.] Univ Montreal, Grp Particle Phys, Montreal, PQ, Canada. [Akimov, A. V.; Baranov, S. P.; Gavrilenko, I. L.; Komar, A. A.; Mashinistov, R.; Mouraviev, S. V.; Nechaeva, P. 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B.; Duckeck, G.; Ebke, J.; Elmsheuser, J.; Heller, C.; Hertenberger, R.; Hoenig, F.; Legger, F.; Lorenz, J.; Mann, A.; Mehlhase, S.; Meineck, C.; Mitrevski, J.; Nunnemann, T.; Rauscher, F.; Ruschke, A.; Sanders, M. P.; Schaile, D.; Schieck, J.; Unverdorben, C.; Vladoiu, D.; Walker, R.; Will, J. Z.; Wittkowski, J.] Univ Munich, Fak Phys, D-81377 Munich, Germany. [Barillari, T.; Bethke, S.; Bronner, J.; Compostella, G.; Cortiana, G.; Flowerdew, M. J.; Goblirsch-Kolb, M.; Ince, T.; Kiryunin, A. E.; Kluth, S.; Kortner, O.; Kortner, S.; Kroha, H.; Macchiolo, A.; Maier, A. A.; Manfredini, A.; Menke, S.; Moser, H. G.; Nagel, M.; Nisius, R.; Nowak, S.; Oberlack, H.; Pahl, C.; Richter, R.; Salihagic, D.; Sandstroem, R.; Schacht, P.; Schwegler, Ph.; Sforza, F.; Spettel, F.; Stern, S.; Stonjek, S.; Terzo, S.; von der Schmitt, H.; Weigell, P.; Wildauer, A.; Zanzi, D.] Max Planck Inst Phys & Astrophys, Werner Heisenberg Inst, Munich, Germany. [Shimojima, M.] Nagasaki Inst Appl Sci, Nagasaki, Japan. [Hasegawa, S.; Horii, Y.; Morvaj, L.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Grad Sch Sci, Nagoya, Aichi 4648601, Japan. [Hasegawa, S.; Horii, Y.; Morvaj, L.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Kobayashi Maskawa Inst, Nagoya, Aichi 4648601, Japan. [Aloisio, A.; Alviggi, M. G.; Canale, V.; Carlino, G.; Chiefari, G.; Conventi, F.; de Asmundis, R.; Della Pietra, M.; Di Donato, C.; Doria, A.; Giordano, R.; Iengo, P.; Izzo, V.; Merola, L.; Patricelli, S.; Rossi, E.; Sanchez, A.; Sekhniaidze, G.; Zurzolo, G.] Univ Naples Federico II, Ist Nazl Fis Nucl, Sez Napoli, Naples, Italy. [Aloisio, A.; Alviggi, M. G.; Canale, V.; Chiefari, G.; Di Donato, C.; Giordano, R.; Merola, L.; Patricelli, S.; Rossi, E.; Sanchez, A.; Zurzolo, G.] Univ Naples Federico II, Dipartimento Fis, Naples, Italy. [Gorelov, I.; Hoeferkamp, M. R.; Seidel, S. C.; Toms, K.; Wang, R.] Univ New Mexico, Dept Phys & Astron, Albuquerque, NM 87131 USA. [Besjes, G. J.; Caron, S.; De Groot, N.; Filthaut, F.; Galea, C.; Klok, P. F.; Konig, A. C.; Salvucci, A.; Struebig, A.] Radboud Univ Nijmegen, Nikhef, Inst Math Astrophys & Particle Phys, NL-6525 ED Nijmegen, Netherlands. [Aben, R.; Angelozzi, I.; Beemster, L. J.; Bentvelsen, S.; Berge, D.; Bobbink, G. J.; Bos, K.; Boterenbrood, H.; Butti, P.; Castelli, A.; Colijn, A. P.; de Jong, P.; De Nooij, L.; Deigaard, I.; Deluca, C.; Deviveiros, P. O.; Dhaliwal, S.; Ferrari, P.; Gadatsch, S.; Geerts, D. A. A.; Hartjes, F.; Hessey, N. P.; Hod, N.; Igonkina, O.; Kluit, P.; Koffeman, E.; Lee, H.; Linde, F.; Mahlstedt, J.; Mechnich, J.; Oussoren, K. P.; Pani, P.; Salek, D.; Valencic, N.; Van Den Wollenberg, W.; Van Der Deijl, P. C.; van der Geer, R.; van der Graaf, H.; Van Der Leeu, R.; van Vulpen, I.; Verkerke, W.; Vermeulen, J. 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A.; Malyshev, V. M.; Maslennikov, A. L.; Maximov, D. A.; Peleganchuk, S. V.; Rezanova, O. L.; Skovpen, K. Yu.; Soukharev, A. M.; Talyshev, A. A.; Tikhonov, Yu. A.] Budker Inst Nucl Phys, SB RAS, Novosibirsk 630090, Russia. [Cranmer, K.; Haas, A.; Heinrich, L.; van Huysduynen, L. Hooft; Kaplan, B.; Karthik, K.; Konoplich, R.; Kreiss, S.; Lewis, G. H.; Mincer, A. I.; Nemethy, P.; Neves, R. M.] NYU, Dept Phys, New York, NY 10003 USA. [Gan, K. K.; Ishmukhametov, R.; Kagan, H.; Kass, R. D.; Merritt, H.; Moss, J.; Nagarkar, A.; Pignotti, D. T.; Tannenwald, B. B.; Yang, Y.] Ohio State Univ, Columbus, OH 43210 USA. [Nakano, I.] Okayama Univ, Fac Sci, Okayama 700, Japan. [Abbott, B.; Bertsche, C.; Bertsche, D.; Gutierrez, P.; Hasib, A.; Norberg, S.; Saleem, M.; Severini, H.; Skubic, P.; Strauss, M.] Univ Oklahoma, Homer L Dodge Dept Phys & Astron, Norman, OK 73019 USA. [Abi, B.; Bousson, N.; Khanov, A.; Rizatdinova, F.; Sidorov, D.; Yu, J.] Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USA. [Chytka, L.; Hamal, P.; Hrabovsky, M.; Kvita, J.; Nozka, L.] Palacky Univ, RCPTM, CR-77147 Olomouc, Czech Republic. [Brau, J. E.; Brost, E.; Majewski, S.; Potter, C. T.; Ptacek, E.; Radloff, P.; Shamim, M.; Sinev, N. B.; Strom, D. M.; Torrence, E.; Wanotayaroj, C.; Winklmeier, F.] Univ Oregon, Ctr High Energy Phys, Eugene, OR 97403 USA. [Khalek, S. Abdel; Bassalat, A.; Becot, C.; Binet, S.; Bourdarios, C.; Charfeddine, D.; De Regie, J. B. De Vivie; Duflot, L.; Escalier, M.; Fayard, L.; Fournier, D.; Grivaz, J. -F.; Guillemin, T.; Hariri, F.; Henrot-Versille, S.; Hrivnac, J.; Iconomidou-Fayard, L.; Kado, M.; Li, Y.; Lounis, A.; Makovec, N.; Poggioli, L.; Puzo, P.; Renaud, A.; Rousseau, D.; Rybkin, G.; Schaffer, A. C.; Scifo, E.; Serin, L.; Simion, S.; Tanaka, R.; Tran, H. L.; Zerwas, D.; Zhang, Z.] Univ Paris 11, LAL, Orsay, France. [Khalek, S. Abdel; Bassalat, A.; Becot, C.; Binet, S.; Bourdarios, C.; Charfeddine, D.; De Regie, J. B. De Vivie; Duflot, L.; Escalier, M.; Fayard, L.; Fournier, D.; Grivaz, J. -F.; Guillemin, T.; Hariri, F.; Henrot-Versille, S.; Hrivnac, J.; Iconomidou-Fayard, L.; Kado, M.; Li, Y.; Lounis, A.; Makovec, N.; Poggioli, L.; Puzo, P.; Renaud, A.; Rousseau, D.; Rybkin, G.; Schaffer, A. C.; Scifo, E.; Serin, L.; Simion, S.; Tanaka, R.; Tran, H. L.; Zerwas, D.; Zhang, Z.] CNRS, IN2P3, F-91405 Orsay, France. [Endo, M.; Hanagaki, K.; Lee, J. S. H.; Nomachi, M.; Okamura, W.; Sugaya, Y.; Teoh, J. J.; Yamaguchi, Y.] Osaka Univ, Grad Sch Sci, Osaka, Japan. [Bugge, L.; Bugge, M. K.; Cameron, D.; Catmore, J. R.; Franconi, L.; Gjelsten, B. K.; Gramstad, E.; Ould-Saada, F.; Pajchel, K.; Pedersen, M.; Read, A. L.; Rohne, O.; Stapnes, S.; Strandlie, A.] Univ Oslo, Dept Phys, Oslo, Norway. [Apolle, R.; Barr, A. J.; Behr, K.; Boddy, C. R.; Buckingham, R. M.; Cooper-Sarkar, A. M.; Ortuzar, M. Crispin; Dafinca, A.; Davies, E.; Gallas, E. J.; Gupta, S.; Gwenlan, C.; Hall, D.; Hays, C. P.; Henderson, J.; Howard, J.; Huffman, T. B.; Issever, C.; Kalderon, C. W.; King, R. S. B.; Kogan, L. A.; Lewis, A.; Livermore, S. S. A.; Nickerson, R. B.; Pachal, K.; Pinder, A.; Ryder, N. C.; Sawyer, C.; Short, D.; Tseng, J. C-L.; Vickey, T.; Viehhauser, G. H. A.; Weidberg, A. R.; Zhong, J.] Univ Oxford, Dept Phys, Oxford OX1 2JD, England. [Conta, C.; Dondero, P.; Ferrari, R.; Fraternali, M.; Gaudio, G.; Livan, M.; Negri, A.; Polesello, G.; Rebuzzi, D. M.; Rimoldi, A.; Vercesi, V.] Univ Pavia, Ist Nazl Fis Nucl, Sez Pavia, I-27100 Pavia, Italy. [Conta, C.; Dondero, P.; Fraternali, M.; Livan, M.; Negri, A.; Rebuzzi, D. M.; Rimoldi, A.] Univ Pavia, Dipartimento Fis, I-27100 Pavia, Italy. [Brendlinger, K.; Heim, S.; Hines, E.; Hong, T. M.; Jackson, B.; Kroll, J.; Kunkle, J.; Lester, C. M.; Lipeles, E.; Meyer, C.; Ospanov, R.; Saxon, J.; Stahlman, J.; Thomson, E.; Tuna, A. N.; Vanguri, R.; Williams, H. H.] Univ Penn, Dept Phys, Philadelphia, PA 19104 USA. [Ezhilov, A.; Fedin, O. L.; Gratchev, V.; Grebenyuk, O. G.; Levchenko, M.; Maleev, V. P.; Ryabov, Y. F.; Schegelsky, V. A.; Sedykh, E.; Seliverstov, D. M.; Solovyev, V.] Petersburg Nucl Phys Inst, Gatchina, Russia. [Beccherle, R.; Bertolucci, F.; Cavasinni, V.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Leone, S.; Roda, C.; Scuri, F.; Volpi, G.; White, S.] Univ Pisa, Ist Nazl Fis Nucl, Sez Pisa, Pisa, Italy. [Beccherle, R.; Bertolucci, F.; Cavasinni, V.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Leone, S.; Roda, C.; Scuri, F.; Volpi, G.; White, S.] Univ Pisa, Dipartimento Fis E Fermi, Pisa, Italy. [Bianchi, R. M.; Boudreau, J.; Cleland, W.; Escobar, C.; Kittelmann, T.; Mueller, J.; Prieur, D.; Sapp, K.; Su, J.; Yoosoofmiya, R.] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA USA. [Aguilar-Saavedra, J. A.; Amor Dos Santos, S. P.; Amorim, A.; Anjos, N.; Araque, J. P.; Cantrill, R.; Carvalho, J.; Castro, N. F.; Muino, P. Conde; Da Cunha Sargedas De Sousa, M. J.; Wemans, A. Do Valle; Fiolhais, M. C. N.; Galhardo, B.; Gomes, A.; Goncalo, R.; Jorge, P. M.; Lopes, L.; Miguens, J. Machado; Maio, A.; Maneira, J.; Marques, C. N.; Onofre, A.; Palma, A.; Pedro, R.; Pina, J.; Pinto, B.; Santos, H.; Saraiva, J. G.; Silva, J.; Delgado, A. Tavares; Veloso, F.; Wolters, H.] Lab Instrument & Fis Expt Particulas LIP, Lisbon, Portugal. [Amorim, A.; Muino, P. Conde; Da Cunha Sargedas De Sousa, M. J.; Gomes, A.; Jorge, P. M.; Miguens, J. Machado; Maio, A.; Maneira, J.; Palma, A.; Pedro, R.; Pina, J.; Delgado, A. Tavares] Univ Lisbon, Fac Ciencias, P-1699 Lisbon, Portugal. [Amor Dos Santos, S. P.; Carvalho, J.; Fiolhais, M. C. N.; Galhardo, B.; Veloso, F.; Wolters, H.] Univ Coimbra, Dept Phys, Coimbra, Portugal. [Gomes, A.; Maio, A.; Pina, J.; Saraiva, J. G.; Silva, J.] Univ Lisbon, Ctr Fis Nucl, P-1699 Lisbon, Portugal. [Onofre, A.] Univ Minho, Dept Fis, Braga, Portugal. [Aguilar-Saavedra, J. A.] Univ Granada, Dept Fis Teor & Cosmos, Granada, Spain. [Aguilar-Saavedra, J. A.] Univ Granada, CAFPE, Granada, Spain. [Wemans, A. Do Valle] Univ Nova Lisboa, Fac Ciencias & Tecnol, Dept Fis, Caparica, Portugal. [Wemans, A. Do Valle] Univ Nova Lisboa, Fac Ciencias & Tecnol, CEFITEC, Caparica, Portugal. [Bohm, J.; Chudoba, J.; Havranek, M.; Hejbal, J.; Jakoubek, T.; Kepka, O.; Kupco, A.; Kus, V.; Lokajicek, M.; Lysak, R.; Marcisovsky, M.; Mikestikova, M.; Nemecek, S.; Sicho, P.; Staroba, P.; Svatos, M.; Tasevsky, M.; Vrba, V.] Acad Sci Czech Republic, Inst Phys, Prague, Czech Republic. [Augsten, K.; Gallus, P.; Gunther, J.; Jakubek, J.; Kohout, Z.; Kral, V.; Myska, M.; Pospisil, S.; Seifert, F.; Simak, V.; Slavicek, T.; Smolek, K.; Solar, M.; Solc, J.; Sopczak, A.; Sopko, B.; Sopko, V.; Suk, M.; Turecek, D.; Vacek, V.; Vlasak, M.; Vokac, P.; Vykydal, Z.; Zeman, M.] Czech Tech Univ, CR-16635 Prague, Czech Republic. [Balek, P.; Berta, P.; Cerny, K.; Chalupkova, I.; Davidek, T.; Dolejsi, J.; Dolezal, Z.; Faltova, J.; Kodys, P.; Leitner, R.; Pleskot, V.; Reznicek, P.; Rybar, M.; Scheirich, D.; Spousta, M.; Sykora, T.; Tas, P.; Todorova-Nova, S.; Valkar, S.; Vorobel, V.] Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic. [Borisov, A.; Denisov, S. P.; Fakhrutdinov, R. M.; Fenyuk, A. B.; Golubkov, D.; Kamenshchikov, A.; Karyukhin, A. N.; Korotkov, V. A.; Kozhin, A. S.; Minaenko, A. A.; Myagkov, A. G.; Nikolaenko, V.; Solodkov, A. A.; Solovyanov, O. V.; Starchenko, E. A.; Zaitsev, A. M.; Zenin, O.] Inst High Energy Phys, State Res Ctr, Protvino, Russia. [Adye, T.; Baines, J. T.; Barnett, B. M.; Burke, S.; Davies, E.; Dewhurst, A.; Dopke, J.; Emeliyanov, D.; Gallop, B. J.; Gee, C. N. P.; Haywood, S. J.; Kirk, J.; Martin-Haugh, S.; McCubbin, N. A.; McMahon, S. J.; Middleton, R. P.; Murray, W. J.; Phillips, P. W.; Rosten, R.; Sankey, D. P. C.; Scott, W. G.; Tyndel, M.; Wickens, F. J.; Wielers, M.] Rutherford Appleton Lab, Particle Phys Dept, Didcot OX11 0QX, Oxon, England. [Benslama, K.] Univ Regina, Dept Phys, Regina, SK S4S 0A2, Canada. [Tanaka, S.] Ritsumeikan Univ, Shiga, Japan. [Anulli, F.; Bagiacchi, P.; Bagnaia, P.; Bini, C.; Ciapetti, G.; De Pedis, D.; De Salvo, A.; Di Domenico, A.; Dionisi, C.; Falciano, S.; Gabrielli, A.; Gauzzi, P.; Gentile, S.; Giagu, S.; Kuna, M.; Lacava, F.; Luci, C.; Luminari, L.; Marzano, F.; Mirabelli, G.; Monzani, S.; Nisati, A.; Pasqualucci, E.; Petrolo, E.; Pontecorvo, L.; Rosati, S.; Tehrani, F. Safai; Sidoti, A.; Vanadia, M.; Vari, R.; Veneziano, S.; Verducci, M.; Zanello, L.] Univ Roma La Sapienza, Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy. [Bagiacchi, P.; Bagnaia, P.; Bini, C.; Ciapetti, G.; Di Domenico, A.; Dionisi, C.; Gabrielli, A.; Gauzzi, P.; Gentile, S.; Giagu, S.; Kuna, M.; Lacava, F.; Luci, C.; Messina, A.; Monzani, S.; Vanadia, M.; Verducci, M.; Zanello, L.] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy. [Aielli, G.; Cardarellia, R.; Cattani, G.; Di Ciaccio, A.; Grossi, G. C.; Iuppa, R.; Liberti, B.; Mazzaferro, L.; Paolozzi, L.; Salamon, A.; Santonico, R.] Univ Roma Tor Vergata, Ist Nazl Fis Nucl, Sez Roma Tor Vergata, Rome, Italy. [Aielli, G.; Cattani, G.; Di Ciaccio, A.; Grossi, G. C.; Iuppa, R.; Mazzaferro, L.; Paolozzi, L.; Santonico, R.] Univ Roma Tor Vergata, Dipartimento Fis, I-00173 Rome, Italy. [Bacci, C.; Baroncelli, A.; Biglietti, M.; Bortolotto, V.; Ceradini, F.; Di Micco, B.; Farilla, A.; Graziani, E.; Iodice, M.; Orestano, D.; Passeri, A.; Pastore, F.; Petrucci, F.; Puddu, D.; Salamanna, G.; Stanescu, C.; Taccini, C.; Trovatelli, M.] Univ Roma Tre, Ist Nazl Fis Nucl, Sez Roma Tre, Rome, Italy. [Bacci, C.; Bortolotto, V.; Ceradini, F.; Di Micco, B.; Orestano, D.; Pastore, F.; Petrucci, F.; Puddu, D.; Salamanna, G.; Taccini, C.; Trovatelli, M.] Univ Roma Tre, Dipartimento Matemat & Fis, Rome, Italy. [Benchekroun, D.; Chafaq, A.; Gouighri, M.; Hoummada, A.] Univ Hassan 2, Reseau Univ Phys Hautes Energies, Fac Sci Ain Chock, Casablanca, Morocco. [Ghazlane, H.] Ctr Natl Energie Sci Tech Nucl, Rabat, Morocco. [El Kacimi, M.; Goujdami, D.] Univ Cadi Ayyad, LPHEA, Fac Sci Semlalia, Marrakech, Morocco. [Boutouil, S.; Derkaoui, J. E.; Ouchrif, M.; Tayalati, Y.] Univ Mohamed Premier, Fac Sci, Oujda, Morocco. [Boutouil, S.; Derkaoui, J. E.; Ouchrif, M.; Tayalati, Y.] LPTPM, Oujda, Morocco. [El Moursli, R. Cherkaoui; Fassi, F.; Haddad, N.] Univ Mohammed V Agdal, Fac Sci, Rabat, Morocco. [Bachacou, H.; Balli, F.; Bauer, F.; Besson, N.; Blanchard, J. -B.; Boonekamp, M.; Calandri, A.; Chevalier, L.; Hoffmann, M. Dano; Deliot, F.; Ernwein, J.; Etienvre, A. I.; Formica, A.; Giraud, P. F.; Da Costa, J. Goncalves Pinto Firmino; Grabas, H. M. X.; Guyot, C.; Hanna, R.; Hassani, S.; Kozanecki, W.; Lancon, E.; Laporte, J. F.; Maiani, C.; Mal, P.; Mansoulie, B.; Martinez, H.; Meric, N.; Meyer, J-P.; Nicolaidou, R.; Ouraou, A.; Protopapadaki, E.; Royon, C. R.; Schoeffel, L.; Schune, Ph.; Schwemling, Ph.; Schwindling, J.; Tsionou, D.; Vranjes, N.; Xiao, M.] CEA Saclay, DSM IRFU, Inst Rech Lois Fondament Univers, Commissariat Energie Atom & Energies Alternat, F-91191 Gif Sur Yvette, France. [Battaglia, M.; Debenedetti, C.; Grillo, A. A.; Kuhl, A.; Law, A. T.; Liang, Z.; Litke, A. M.; Lockman, W. S.; Manning, P. M.; Nielsen, J.; Reece, R.; Rose, P.; Sadrozinski, H. F-W.; Schumm, B. A.; Seiden, A.] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA. [Blackburn, D.; Coccaro, A.; Goussiou, A. G.; Harris, O. M.; Hsu, S. -C.; Lubatti, H. J.; Marx, M.; Rompotis, N.; Rothberg, J.; De Bruin, P. H. Sales; Watts, G.] Univ Washington, Dept Phys, Seattle, WA 98195 USA. [Anastopoulos, C.; Costanzo, D.; Donszelmann, T. Cuhadar; Dawson, I.; Fletcher, G. T.; Hodgkinson, M. C.; Hodgson, P.; Johansson, P.; Korolkova, E. V.; Paredes, B. Lopez; Miyagawa, P. S.; Paganis, E.; Suruliz, K.; Tovey, D. R.] Univ Sheffield, Dept Phys & Astron, Sheffield, S Yorkshire, England. [Hasegawa, Y.; Takeshita, T.] Shinshu Univ, Dept Phys, Nagano, Japan. [Atlay, N. B.; Buchholz, P.; Czirr, H.; Fleck, I.; Gaur, B.; Ibragimov, I.; Ikematsu, K.; Rosenthal, O.; Sipica, V.; Walkowiak, W.; Ziolkowski, M.] Univ Siegen, Fachbereich Phys, D-57068 Siegen, Germany. [Buat, Q.; Dawe, E.; Godfrey, J.; O'Neil, D. C.; Stelzer, B.; Tanasijczuk, A. J.; Torres, H.; Trottier-McDonald, M.; Van Nieuwkoop, J.; Vetterli, M. C.] Simon Fraser Univ, Dept Phys, Burnaby, BC V5A 1S6, Canada. [Aracena, I.; Mayes, J. Backus; Barklow, T.; Bartoldus, R.; Bawa, H. S.; Black, J. E.; Cogan, J. G.; Eifert, T.; Fulsom, B. G.; Gao, Y. S.; Garelli, N.; Grenier, P.; Kagan, M.; Kocian, M.; Koi, T.; Lowe, A. J.; Malone, C.; Mount, R.; Nef, P. D.; Nelson, T. K.; Piacquadio, G.; Salnikov, A.; Schwartzman, A.; Silverstein, D.; Strauss, E.; Su, D.; Swiatlowski, M.; Wittgen, M.; Young, C.] SLAC Natl Accelerator Lab, Stanford, CA USA. [Astalos, R.; Bartos, P.; Blazek, T.; Federic, P.; Plazak, L.; Stavina, P.; Sykora, I.; Tokar, S.; Zenis, T.] Comenius Univ, Fac Math Phys & Informat, Bratislava 80100, Slovakia. [Antos, J.; Bruncko, D.; Kladiva, E.; Strizenec, P.] Slovak Acad Sci, Inst Expt Phys, Dept Subnuclear Phys, Kosice 04353, Slovakia. [Hamilton, A.] Univ Cape Town, Dept Phys, ZA-7925 Cape Town, South Africa. [Aurousseau, M.; Castaneda-Miranda, E.; Connell, S. H.; Yacoob, S.] Univ Johannesburg, Dept Phys, Johannesburg, South Africa. [Bristow, K.; Carrillo-Montoya, D.; Chen, X.; Hamity, G. N.; Hsu, C.; Garcia, B. R. Mellado; Ruan, X.; Boeriu, O. E. Vickey] Univ Witwatersrand, Sch Phys, Johannesburg, South Africa. [Abulaiti, Y.; Akerstedt, H.; Asman, B.; Bendtz, K.; Bertoli, G.; Bessidskaia, O.; Bohm, C.; Clement, C.; Cribbs, W. A.; Eriksson, D.; Gellerstedt, K.; Hellman, S.; Johansson, K. E.; Jon-And, K.; Khandanyan, H.; Kim, H.; Klimek, P.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Petridis, A.; Plucinski, P.; Rossetti, V.; Silverstein, S. B.; Sjolin, J.; Strandberg, S.; Tylmad, M.] Stockholm Univ, Dept Phys, S-10691 Stockholm, Sweden. [Abulaiti, Y.; Akerstedt, H.; Asman, B.; Bendtz, K.; Bertoli, G.; Bessidskaia, O.; Clement, C.; Cribbs, W. A.; Gellerstedt, K.; Hellman, S.; Johansson, K. E.; Jon-And, K.; Khandanyan, H.; Kim, H.; Klimek, P.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Petridis, A.; Rossetti, V.; Sjolin, J.; Strandberg, S.; Tylmad, M.] Oskar Klein Ctr, Stockholm, Sweden. [Jovicevic, J.; Kuwertz, E. S.; Lund-Jensen, B.; Morley, A. K.; Strandberg, J.] Royal Inst Technol, Dept Phys, S-10044 Stockholm, Sweden. [Bee, C. P.; Campoverde, A.; Chen, K.; Engelmann, R.; Grassi, V.; Hobbs, J.; Jia, J.; Li, H.; Lindquist, B. E.; Mastrandrea, P.; McCarthy, R. L.; Puldon, D.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA. [Bee, C. P.; Campoverde, A.; Chen, K.; Engelmann, R.; Grassi, V.; Hobbs, J.; Jia, J.; Li, H.; Lindquist, B. E.; Mastrandrea, P.; McCarthy, R. L.; Puldon, D.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.] SUNY Stony Brook, Dept Chem, Stony Brook, NY 11794 USA. [Bartsch, V.; Cerri, A.; Barajas, C. A. Chavez; De Santo, A.; Grout, Z. J.; Potter, C. J.; Salvatore, F.; Castillo, I. Santoyo; Shehu, C. Y.; Sutton, M. R.] Univ Sussex, Dept Phys & Astron, Brighton, E Sussex, England. [Black, C. W.; Cuthbert, C.; Finelli, K. D.; Jeng, G. -Y.; Patel, N. D.; Saavedra, A. F.; Scarcella, M.; Varvell, K. E.; Watson, I. J.; Yabsley, B.] Univ Sydney, Sch Phys, Sydney, NSW 2006, Australia. [Abdallah, J.; Chu, M. L.; Hou, S.; Jamin, D. O.; Lee, C. A.; Lee, S. C.; Li, B.; Lin, S. C.; Liu, B.; Liu, D.; Lo Sterzo, F.; Mazini, R.; Ren, Z. L.; Shi, L.; Soh, D. A.; Teng, P. K.; Wang, C.; Wang, S. M.; Weng, Z.; Zhang, L.] Acad Sinica, Inst Phys, Taipei, Taiwan. [Abreu, H.; Di Mattia, A.; Kopeliansky, R.; Musto, E.; Rozen, Y.; Tarem, S.] Technion Israel Inst Technol, Dept Phys, IL-32000 Haifa, Israel. [Abramowicz, H.; Alexander, G.; Amram, N.; Ashkenazi, A.; Bella, G.; Benary, O.; Benhammou, Y.; Davies, M.; Etzion, E.; Gershon, A.; Gueta, O.; Guttman, N.; Munwes, Y.; Oren, Y.; Sadeh, I.; Silver, Y.; Soffer, A.; Taiblum, N.] Tel Aviv Univ, Raymond & Beverly Sackler Sch Phys & Astron, IL-69978 Tel Aviv, Israel. [Bachas, K.; Gkaitatzis, S.; Gkialas, I.; Iliadis, D.; Kordas, K.; Kouskoura, V.; Leisos, A.; Papageorgiou, K.; Petridou, C.; Sampsonidis, D.; Sidiropoulou, O.] Aristotle Univ Thessaloniki, Dept Phys, GR-54006 Thessaloniki, Greece. [Akimoto, G.; Asai, S.; Azuma, Y.; Dohmae, T.; Enari, Y.; Hanawa, K.; Kanaya, N.; Kataoka, Y.; Kawamoto, T.; Kazama, S.; Kessoku, K.; Kobayashi, T.; Komori, Y.; Mashimo, T.; Masubuchi, T.; Nakamura, T.; Ninomiya, Y.; Okuyama, T.; Sakamoto, H.; Sasaki, Y.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamaguchi, H.; Yamamoto, S.; Yamamura, T.; Yamanaka, T.; Yoshihara, K.] Univ Tokyo, Int Ctr Elementary Particle Phys, Tokyo, Japan. [Akimoto, G.; Asai, S.; Azuma, Y.; Dohmae, T.; Enari, Y.; Hanawa, K.; Kanaya, N.; Kataoka, Y.; Kawamoto, T.; Kazama, S.; Kessoku, K.; Kobayashi, T.; Komori, Y.; Mashimo, T.; Masubuchi, T.; Nakamura, T.; Ninomiya, Y.; Okuyama, T.; Sakamoto, H.; Sasaki, Y.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamaguchi, H.; Yamamoto, S.; Yamamura, T.; Yamanaka, T.; Yoshihara, K.] Univ Tokyo, Dept Phys, Tokyo 113, Japan. [Bratzler, U.; Fukunaga, C.] Tokyo Metropolitan Univ, Grad Sch Sci & Technol, Tokyo 158, Japan. [Hirose, M.; Ishitsuka, M.; Jinnouchi, O.; Kobayashi, D.; Kuze, M.; Motohashi, K.; Nagai, R.; Nobe, T.; Pettersson, N. E.] Tokyo Inst Technol, Dept Phys, Tokyo 152, Japan. [AbouZeid, O. S.; Brelier, B.; Chau, C. C.; Ilic, N.; Keung, J.; Krieger, P.; Mc Goldrick, G.; Orr, R. S.; Polifka, R.; Rudolph, M. S.; Savard, P.; Schramm, S.; Sinervo, P.; Spreitzer, T.; Taenzer, J.; Teuscher, R. J.; Thompson, P. D.; Trischuk, W.; Venturi, N.] Univ Toronto, Dept Phys, Toronto, ON, Canada. [Azuelos, G.; Canepa, A.; Chekulaev, S. V.; Fortin, D.; Gingrich, D. M.; Koutsman, A.; Oakham, F. G.; Oram, C. J.; Codina, E. Perez; Schouten, D.; Stelzer-Chilton, O.; Tafirout, R.; Trigger, I. M.; Vetterli, M. C.] TRIUMF, Vancouver, BC V6T 2A3, Canada. [Garcia, J. A. Benitez; Bustos, A. C. Florez; Ramos, J. A. Manjarres; Palacino, G.; Qureshi, A.; Taylor, W.] York Univ, Dept Phys & Astron, Toronto, ON M3J 2R7, Canada. [Hara, K.; Hayashi, T.; Kim, S. H.; Kiuchi, K.; Ukegawa, F.] Univ Tsukuba, Fac Pure & Appl Sci, Tsukuba, Ibaraki, Japan. [Beauchemin, P. H.; Hamilton, S.; Meoni, E.; Rolli, S.; Sliwa, K.; Wetter, J.] Tufts Univ, Dept Phys & Astron, Medford, MA 02155 USA. [Losada, M.; Navarro, G.; Sandoval, C.] Univ Antonio Narino, Ctr Invest, Bogota, Colombia. [Corso-Radu, A.; Gerbaudo, D.; Lankford, A. J.; Mete, A. S.; Nelson, A.; Rao, K.; Relich, M.; Scannicchio, D. A.; Schernau, M.; Shimmin, C. O.; Taffard, A.; Unel, G.; Whiteson, D.; Zhou, N.] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA USA. [Acharya, B. S.; Alhroob, M.; Brazzale, S. F.; Cobal, M.; De Sanctis, U.; Giordani, M. P.; Pinamonti, M.; Quayle, W. B.; Shaw, K.; Soualah, R.] Ist Nazl Fis Nucl, Gruppo Collegato Udine, Sez Trieste, Udine, Italy. [Acharya, B. S.; De Sanctis, U.; Quayle, W. B.; Shaw, K.] Abdus Salaam Int Ctr Theoret Phys, Trieste, Italy. [Alhroob, M.; Brazzale, S. F.; Cobal, M.; Giordani, M. P.; Pinamonti, M.; Soualah, R.] Univ Udine, Dipartimento Chim Fis & Ambiente, I-33100 Udine, Italy. [Atkinson, M.; Basye, A.; Benekos, N.; Cavaliere, V.; Chang, P.; Coggeshall, J.; Errede, D.; Errede, S.; Lie, K.; Liss, T. M.; Neubauer, M. S.; Shang, R.; Vichou, I.] Univ Illinois, Dept Phys, Urbana, IL 61801 USA. [Brenner, R.; Buszello, C. P.; Ekelof, T.; Ellert, M.; Ferrari, A.; Isaksson, C.; Madsen, A.; Ohman, H.; Pelikan, D.; Rangel-Smith, C.] Uppsala Univ, Dept Phys & Astron, Uppsala, Sweden. [Cabrera Urban, S.; Castillo Gimenez, V.; Costa, M. J.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Garcia Navarro, J. E.; Gonzalez de la Hoz, S.; Hernandez Jimenez, Y.; Higon-Rodriguez, E.; Irles Quiles, A.; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; March, L.; Marti-Garcia, S.; Mitsou, V. A.; Moles-Valls, R.; Oliver Garcia, E.; Pedraza Lopez, S.; Perez Garcia-Estan, M. T.; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, J.; Sanchez Martinez, V.; Soldevila, U.; Torro Pastor, E.; Valero, A.; Valladolid Gallego, E.; Valls Ferrer, J. A.; Vos, M.] Univ Valencia, Inst Fis Corpuscular, IFIC, Valencia, Spain. [Cabrera Urban, S.; Castillo Gimenez, V.; Costa, M. J.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Garcia Navarro, J. E.; Gonzalez de la Hoz, S.; Hernandez Jimenez, Y.; Higon-Rodriguez, E.; Irles Quiles, A.; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; March, L.; Marti-Garcia, S.; Mitsou, V. A.; Moles-Valls, R.; Oliver Garcia, E.; Pedraza Lopez, S.; Perez Garcia-Estan, M. T.; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, J.; Sanchez Martinez, V.; Soldevila, U.; Torro Pastor, E.; Valero, A.; Valladolid Gallego, E.; Valls Ferrer, J. A.; Vos, M.] Univ Valencia, Dept Fis Atom Mol & Nucl, Valencia, Spain. [Cabrera Urban, S.; Castillo Gimenez, V.; Costa, M. J.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Garcia Navarro, J. E.; Gonzalez de la Hoz, S.; Hernandez Jimenez, Y.; Higon-Rodriguez, E.; Irles Quiles, A.; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; March, L.; Marti-Garcia, S.; Mitsou, V. A.; Moles-Valls, R.; Oliver Garcia, E.; Pedraza Lopez, S.; Perez Garcia-Estan, M. T.; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, J.; Sanchez Martinez, V.; Soldevila, U.; Torro Pastor, E.; Valero, A.; Valladolid Gallego, E.; Valls Ferrer, J. A.; Vos, M.] Univ Valencia, Dept Ingn Elect, Valencia, Spain. [Cabrera Urban, S.; Castillo Gimenez, V.; Costa, M. J.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Garcia Navarro, J. E.; Gonzalez de la Hoz, S.; Hernandez Jimenez, Y.; Higon-Rodriguez, E.; Irles Quiles, A.; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; March, L.; Marti-Garcia, S.; Mitsou, V. A.; Moles-Valls, R.; Oliver Garcia, E.; Pedraza Lopez, S.; Perez Garcia-Estan, M. T.; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, J.; Sanchez Martinez, V.; Soldevila, U.; Torro Pastor, E.; Valero, A.; Valladolid Gallego, E.; Valls Ferrer, J. A.; Vos, M.] Univ Valencia, IMB CNM, Valencia, Spain. [Cabrera Urban, S.; Castillo Gimenez, V.; Costa, M. J.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Garcia Navarro, J. E.; Gonzalez de la Hoz, S.; Hernandez Jimenez, Y.; Higon-Rodriguez, E.; Irles Quiles, A.; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; March, L.; Marti-Garcia, S.; Mitsou, V. A.; Moles-Valls, R.; Oliver Garcia, E.; Pedraza Lopez, S.; Perez Garcia-Estan, M. T.; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, J.; Sanchez Martinez, V.; Soldevila, U.; Torro Pastor, E.; Valero, A.; Valladolid Gallego, E.; Valls Ferrer, J. A.; Vos, M.] CSIC, Valencia, Spain. [Fedorko, W.; Gay, C.; Gecse, Z.; King, S. B.; Lister, A.; Swedish, S.; Viel, S.] Univ British Columbia, Dept Phys, Vancouver, BC, Canada. [Albert, J.; Bansal, V.; Berghaus, F.; Bernlochner, F. U.; David, C.; Fincke-Keeler, M.; Hamano, K.; Hill, E.; Keeler, R.; Kowalewski, R.; Lefebvre, M.; Marino, C. P.; McPherson, R. A.; Ouellette, E. A.; Pearce, J.; Sobie, R.; Venturi, M.] Univ Victoria, Dept Phys & Astron, Victoria, BC, Canada. [Beckingham, M.; Farrington, S. M.; Harrison, P. F.; Janus, M.; Jeske, C.; Jones, G.; Martin, T. A.; Murray, W. J.; Pianori, E.] Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England. [Iizawa, T.; Kimura, N.; Mitani, T.; Sakurai, Y.; Yorita, K.] Waseda Univ, Tokyo, Japan. [Barak, L.; Bressler, S.; Citron, Z. H.; Duchovni, E.; Gabizon, O.; Gross, E.; Groth-Jensen, J.; Lellouch, D.; Levinson, L. J.; Mikenberg, G.; Milov, A.; Milstein, D.; Pitt, M.; Roth, I.; Schaarschmidt, J.; Smakhtin, V.] Weizmann Inst Sci, Dept Particle Phys, IL-76100 Rehovot, Israel. [Banerjee, Sw.; Castillo, L. R. Flores; Hard, A. S.; Heng, Y.; Ji, H.; Ju, X.; Kashif, L.; Kruse, A.; Ming, Y.; Pan, Y. B.; Wang, F.; Wiedenmann, W.; Wu, S. L.; Yang, H.; Zhang, F.; Zobernig, G.] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA. [Redelbach, A.; Schreyer, M.; Siragusa, G.; Stroehmer, R.; Tam, J. Y. C.; Trefzger, T.; Weber, S. W.; Zibell, A.] Univ Wurzburg, Fak Phys & Astron, Wurzburg, Germany. [Bannoura, A. A. E.; Barisonzi, M.; Becker, K.; Beermann, T. A.; Boek, T. T.; Braun, H. M.; Cornelissen, T.; Duda, D.; Ernis, G.; Fischer, J.; Fleischmann, S.; Flick, T.; Hamacher, K.; Harenberg, T.; Heim, T.; Hirschbuehl, D.; Kersten, S.; Khoroshilov, A.; Kohlmann, S.; Lenzen, G.; Maettig, P.; Neumann, M.; Pataraia, S.; Sandhoff, M.; Sartisohn, G.; Wagner, W.; Wicke, D.; Zeitnitz, C.] Berg Univ Wuppertal, Fachbereich Phys C, Wuppertal, Germany. [Adelman, J.; Baker, O. K.; Bedikian, S.; Cummings, J.; Czyczula, Z.; Demers, S.; Erdmann, J.; Garberson, F.; Golling, T.; Guest, D.; Henrichs, A.; Ideal, E.; Lagouri, T.; Leister, A. G.; Loginov, A.; Tipton, P.; Wall, R.; Walsh, B.; Wang, X.] Yale Univ, Dept Phys, New Haven, CT USA. [Hakobyan, H.; Vardanyan, G.] Yerevan Phys Inst, Yerevan 375036, Armenia. [Rahal, G.] IN2P3, Ctr Calcul, Villeurbanne, France. [Acharya, B. S.] Kings Coll London, Dept Phys, London, England. [Bawa, H. S.; Gao, Y. S.; Lowe, A. J.] Calif State Univ Fresno, Dept Phys, Fresno, CA 93740 USA. [Chelkov, G. A.] Tomsk State Univ, Tomsk 634050, Russia. [Conventi, F.; Della Pietra, M.] Univ Napoli Parthenope, Naples, Italy. [Corriveau, F.; McPherson, R. A.; Robertson, S. H.; Sobie, R.; Teuscher, R. J.] IPP, Vancouver, BC, Canada. [Fedin, O. L.] St Petersburg State Polytechn Univ, Dept Phys, St Petersburg, Russia. [Castillo, L. R. Flores] Chinese Univ Hong Kong, Hong Kong, Hong Kong, Peoples R China. [Gkialas, I.; Papageorgiou, K.] Univ Aegean, Dept Financial & Management Engn, Chios, Greece. [Grinstein, S.; Rozas, A. Juste; Martinez, M.] ICREA, Barcelona, Spain. [Ilchenko, Y.; Onyisi, P. U. E.] Univ Texas Austin, Dept Phys, Austin, TX USA. [Jejelava, J.] Ilia State Univ, Inst Theoret Phys, Tbilisi, Rep of Georgia. [Kono, T.] Ochanomizu Univ, Ochadai Acad Prod, Tokyo 112, Japan. [Konoplich, R.] Manhattan Coll, New York, NY USA. [Korol, A. A.; Maximov, D. A.; Rezanova, O. L.; Talyshev, A. A.; Tikhonov, Yu. A.] Novosibirsk State Univ, Novosibirsk 630090, Russia. [Lin, S. C.] Acad Sinica, Inst Phys, Acad Sinica Grid Comp, Taipei, Taiwan. [Mal, P.] Natl Inst Sci Educ & Res, Sch Phys Sci, Bhubaneswar, Orissa, India. [Myagkov, A. G.; Nikolaenko, V.] State Univ, Moscow Inst Phys & Technol, Dolgoprudnyi, Russia. [Pinamonti, M.] Int Sch Adv Studies SISSA, Trieste, Italy. [Purohit, M.] Univ S Carolina, Dept Phys & Astron, Columbia, SC 29208 USA. [Shi, L.; Soh, D. A.; Weng, Z.] Sun Yat Sen Univ, Sch Phys & Engn, Guangzhou 510275, Guangdong, Peoples R China. [Smirnova, L. N.; Turchikhin, S.] Moscow MV Lomonosov State Univ, Fac Phys, Moscow, Russia. [Toth, J.] Inst Particle & Nucl Phys, Wigner Res Ctr Phys, Budapest, Hungary. [Wildt, M. A.] Univ Hamburg, Inst Expt Phys, Hamburg, Germany. [Yacoob, S.] Univ KwaZulu Natal, Discipline Phys, Durban, South Africa. [Yusuff, I.] Univ Malaya, Dept Phys, Kuala Lumpur 59100, Malaysia. RP Aad, G (reprint author), Aix Marseille Univ, CPPM, Marseille, France. RI Connell, Simon/F-2962-2015; Bosman, Martine/J-9917-2014; Joergensen, Morten/E-6847-2015; Mitsou, Vasiliki/D-1967-2009; Riu, Imma/L-7385-2014; Cabrera Urban, Susana/H-1376-2015; Mir, Lluisa-Maria/G-7212-2015; Garcia, Jose /H-6339-2015; Marti-Garcia, Salvador/F-3085-2011; Della Pietra, Massimo/J-5008-2012; Cavalli-Sforza, Matteo/H-7102-2015; Petrucci, Fabrizio/G-8348-2012; Negrini, Matteo/C-8906-2014; Nemecek, Stanislav/G-5931-2014; Gutierrez, Phillip/C-1161-2011; Di Domenico, Antonio/G-6301-2011; Ventura, Andrea/A-9544-2015; Livan, Michele/D-7531-2012; De, Kaushik/N-1953-2013; Smirnova, Oxana/A-4401-2013; Villa, Mauro/C-9883-2009; White, Ryan/E-2979-2015; Wemans, Andre/A-6738-2012; Castro, Nuno/D-5260-2011; Boyko, Igor/J-3659-2013; Brooks, William/C-8636-2013; Gorelov, Igor/J-9010-2015; Gladilin, Leonid/B-5226-2011; Carvalho, Joao/M-4060-2013; Mashinistov, Ruslan/M-8356-2015; Buttar, Craig/D-3706-2011; Gonzalez de la Hoz, Santiago/E-2494-2016; Guo, Jun/O-5202-2015; Aguilar Saavedra, Juan Antonio/F-1256-2016; Leyton, Michael/G-2214-2016; Jones, Roger/H-5578-2011; Pacheco Pages, Andres/C-5353-2011; Vranjes Milosavljevic, Marija/F-9847-2016; Ferrer, Antonio/H-2942-2015; Grancagnolo, Sergio/J-3957-2015; Doyle, Anthony/C-5889-2009; spagnolo, stefania/A-6359-2012; Ciubancan, Liviu Mihai/L-2412-2015; Zhukov, Konstantin/M-6027-2015; Shmeleva, Alevtina/M-6199-2015; Gavrilenko, Igor/M-8260-2015; Tikhomirov, Vladimir/M-6194-2015; Yang, Haijun/O-1055-2015; Chekulaev, Sergey/O-1145-2015; Warburton, Andreas/N-8028-2013; Juste, Aurelio/I-2531-2015; Grinstein, Sebastian/N-3988-2014; Goncalo, Ricardo/M-3153-2016; Gauzzi, Paolo/D-2615-2009; Mindur, Bartosz/A-2253-2017; Fabbri, Laura/H-3442-2012; Solodkov, Alexander/B-8623-2017; Zaitsev, Alexandre/B-8989-2017; Peleganchuk, Sergey/J-6722-2014; Monzani, Simone/D-6328-2017; Li, Liang/O-1107-2015; Fullana Torregrosa, Esteban/A-7305-2016; Perrino, Roberto/B-4633-2010; SULIN, VLADIMIR/N-2793-2015; Nechaeva, Polina/N-1148-2015; Vykydal, Zdenek/H-6426-2016; Olshevskiy, Alexander/I-1580-2016; Snesarev, Andrey/H-5090-2013; BESSON, NATHALIE/L-6250-2015; Vanadia, Marco/K-5870-2016; Ippolito, Valerio/L-1435-2016; Maneira, Jose/D-8486-2011; Prokoshin, Fedor/E-2795-2012; KHODINOV, ALEKSANDR/D-6269-2015; Staroba, Pavel/G-8850-2014 OI Filthaut, Frank/0000-0003-3338-2247; Terzo, Stefano/0000-0003-3388-3906; Smirnov, Sergei/0000-0002-6778-073X; Connell, Simon/0000-0001-6000-7245; Bosman, Martine/0000-0002-7290-643X; Joergensen, Morten/0000-0002-6790-9361; Mitsou, Vasiliki/0000-0002-1533-8886; Riu, Imma/0000-0002-3742-4582; Mir, Lluisa-Maria/0000-0002-4276-715X; Della Pietra, Massimo/0000-0003-4446-3368; Petrucci, Fabrizio/0000-0002-5278-2206; Negrini, Matteo/0000-0003-0101-6963; Di Domenico, Antonio/0000-0001-8078-2759; Ventura, Andrea/0000-0002-3368-3413; Livan, Michele/0000-0002-5877-0062; De, Kaushik/0000-0002-5647-4489; Smirnova, Oxana/0000-0003-2517-531X; Villa, Mauro/0000-0002-9181-8048; White, Ryan/0000-0003-3589-5900; Wemans, Andre/0000-0002-9669-9500; Castro, Nuno/0000-0001-8491-4376; Boyko, Igor/0000-0002-3355-4662; Brooks, William/0000-0001-6161-3570; Farrington, Sinead/0000-0001-5350-9271; Robson, Aidan/0000-0002-1659-8284; Weber, Michele/0000-0002-2770-9031; Wang, Kuhan/0000-0002-6151-0034; Grohsjean, Alexander/0000-0003-0748-8494; La Rosa, Alessandro/0000-0001-6291-2142; Beck, Hans Peter/0000-0001-7212-1096; Vazquez Schroeder, Tamara/0000-0002-9780-099X; Chen, Chunhui /0000-0003-1589-9955; Walsh, Brian/0000-0003-1689-2309; Gorelov, Igor/0000-0001-5570-0133; Gladilin, Leonid/0000-0001-9422-8636; Carvalho, Joao/0000-0002-3015-7821; Mashinistov, Ruslan/0000-0001-7925-4676; Gonzalez de la Hoz, Santiago/0000-0001-5304-5390; Guo, Jun/0000-0001-8125-9433; Aguilar Saavedra, Juan Antonio/0000-0002-5475-8920; Leyton, Michael/0000-0002-0727-8107; Jones, Roger/0000-0002-6427-3513; Pacheco Pages, Andres/0000-0001-8210-1734; Vranjes Milosavljevic, Marija/0000-0003-4477-9733; Ferrer, Antonio/0000-0003-0532-711X; Grancagnolo, Sergio/0000-0001-8490-8304; Doyle, Anthony/0000-0001-6322-6195; spagnolo, stefania/0000-0001-7482-6348; Ciubancan, Liviu Mihai/0000-0003-1837-2841; Tikhomirov, Vladimir/0000-0002-9634-0581; Warburton, Andreas/0000-0002-2298-7315; Cristinziani, Markus/0000-0003-3893-9171; Chromek-Burckhart, Doris/0000-0003-4243-3288; Qian, Jianming/0000-0003-4813-8167; Haas, Andrew/0000-0002-4832-0455; Galhardo, Bruno/0000-0003-0641-301X; Arratia, Miguel/0000-0001-6877-3315; Hays, Chris/0000-0003-2371-9723; Dell'Asta, Lidia/0000-0002-9601-4225; Chen, Hucheng/0000-0002-9936-0115; Sawyer, Lee/0000-0001-8295-0605; Juste, Aurelio/0000-0002-1558-3291; Begel, Michael/0000-0002-1634-4399; Vari, Riccardo/0000-0002-2814-1337; Nisati, Aleandro/0000-0002-5080-2293; Gray, Heather/0000-0002-5293-4716; Mincer, Allen/0000-0002-6307-1418; Grinstein, Sebastian/0000-0002-6460-8694; Leonidopoulos, Christos/0000-0002-7241-2114; Goncalo, Ricardo/0000-0002-3826-3442; Gauzzi, Paolo/0000-0003-4841-5822; Mindur, Bartosz/0000-0002-5511-2611; Fabbri, Laura/0000-0002-4002-8353; Solodkov, Alexander/0000-0002-2737-8674; Zaitsev, Alexandre/0000-0002-4961-8368; Peleganchuk, Sergey/0000-0003-0907-7592; Monzani, Simone/0000-0002-0479-2207; Li, Liang/0000-0001-6411-6107; Troncon, Clara/0000-0002-7997-8524; Fullana Torregrosa, Esteban/0000-0003-3082-621X; Thomson, Mark/0000-0002-2654-9005; Perrino, Roberto/0000-0002-5764-7337; SULIN, VLADIMIR/0000-0003-3943-2495; Vykydal, Zdenek/0000-0003-2329-0672; Olshevskiy, Alexander/0000-0002-8902-1793; Vanadia, Marco/0000-0003-2684-276X; Ippolito, Valerio/0000-0001-5126-1620; Maneira, Jose/0000-0002-3222-2738; Prokoshin, Fedor/0000-0001-6389-5399; KHODINOV, ALEKSANDR/0000-0003-3551-5808; FU ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWF, Austria; FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq, Brazil; FAPESP, Brazil; NSERC, Canada; NRC, Canada; CFI, Canada; CERN; CONICYT, Chile; CAS, China; MOST, China; NSFC, China; COL-CIENCIAS, Colombia; MSMT CR, Czech Republic; MPO CR, Czech Republic; VSC CR, Czech Republic; DNRF, Denmark; DNSRC, Denmark; Lundbeck Foundation, Denmark; EPLANET, European Union; ERC, European Union; NSRF, European Union; IN2P3-CNRS, France; CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, Germany; DFG, Germany; HGF, Germany; MPG, Germany; AvH Foundation, Germany; GSRT, Greece; NSRF, Greece; ISF, Israel; MINERVA, Israel; GIF, Israel; I-CORE, Israel; Benoziyo Center, Israel; INFN, Italy; MEXT, Japan; JSPS, Japan; CNRST, Morocco; FOM, Netherlands; NWO, Netherlands; BRF, Norway; RCN, Norway; MNiSW, Poland; NCN, Poland; GRICES, Portugal; FCT, Portugal; MNE/IFA, Romania; MES of Russia, Russian Federation; ROSATOM, Russian Federation; JINR; MSTD, Serbia; MSSR, Slovakia; ARRS, Slovenia; MIZS, Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC, Sweden; Wallenberg Foundation, Sweden; SER, Geneva, Switzerland; SNSF, Geneva, Switzerland; Cantons of Bern Geneva, Switzerland; NSC, Taiwan; TAEK, Turkey; STFC, United Kingdom; Royal Society and Leverhulme Trust, United Kingdom; DOE, United States of America; NSF, United States of America FX We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWF and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile; CAS, MOST and NSFC, China; COL-CIENCIAS, Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF, DNSRC and Lundbeck Foundation, Denmark; EPLANET, ERC and NSRF, European Union; IN2P3-CNRS, CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, DFG, HGF, MPG and AvH Foundation, Germany; GSRT and NSRF, Greece; ISF, MINERVA, GIF, I-CORE and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; FOM and NWO, Netherlands; BRF and RCN, Norway; MNiSW and NCN, Poland; GRICES and FCT, Portugal; MNE/IFA, Romania; MES of Russia and ROSATOM, Russian Federation; JINR; MSTD, Serbia; MSSR, Slovakia; ARRS and MIZS, Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC and Wallenberg Foundation, Sweden; SER, SNSF and Cantons of Bern and Geneva, Switzerland; NSC, Taiwan; TAEK, Turkey; STFC, the Royal Society and Leverhulme Trust, United Kingdom; DOE and NSF, United States of America. NR 61 TC 43 Z9 43 U1 10 U2 92 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0370-2693 EI 1873-2445 J9 PHYS LETT B JI Phys. Lett. B PD NOV 10 PY 2014 VL 738 BP 68 EP 86 DI 10.1016/j.physletb.2014.09.008 PG 19 WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AT0KK UT WOS:000344624900010 ER PT J AU Abelev, B Adam, J Adamova, D Aggarwal, MM Rinella, GA Agnello, M Agostinelli, A Agrawal, N Ahammed, Z Ahmad, N Ahmed, I Ahn, SU Ahn, SA Aimo, I Aiola, S Ajaz, M Akindinov, A Alam, SN Aleksandrov, D Alessandro, B Alexandre, D Alici, A Alkin, A Alme, J Alt, T Altinpinar, S Altsybeev, I Prado, CAG Andrei, C Andronic, A Anguelov, V Anielski, J Anticic, T Antinori, F Antonioli, P Aphecetche, L Appelshauser, H Arcelli, S Armesto, N Arnaldi, R Aronsson, T Arsene, IC Arslandok, M Augustinus, A Averbeck, R Awes, TC Azmi, MD Bach, M Badala, A Baek, YW Bagnasco, S Bailhache, R Bala, R Baldisseri, A Pedrosa, FBDS Baral, RC Barbera, R Barile, F Barnafoldi, GG Barnby, LS Barret, V Bartke, J Basile, M Bastid, N Basu, S Bathen, B Batigne, G Camejo, AB Batyunya, B Batzing, PC Baumann, C Bearden, IG Beck, H Bedda, C Behera, NK Belikov, I Bellini, F Bellwied, R Belmont-Moreno, E Belmont, R Belyaev, V Bencedi, G Beole, S Berceanu, I Bercuci, A Berdnikov, Y Berenyi, D Berger, ME Bertens, RA Berzano, D Betev, L Bhasin, A Bhat, IR Bhati, AK Bhattacharjee, B Bhom, J Bianchi, L Bianchi, N Bianchin, C Bielcik, J Bielcikovca, J Bilandzic, A Bjelogrlic, S Blanco, F Blau, D Blume, C Bock, F Bogdanov, A Boggild, H Bogolyubsky, M Bohmer, FV Boldizsar, L Bombara, M Book, J Borel, H Borissov, A Bossu, F Botje, M Botta, E Bottger, S Braun-Munzinger, P Bregant, M Breitner, T Broker, TA Browning, TA Broz, M Bruna, E Bruno, GE Budnikov, D Buesching, H Bufalino, S Buncic, P Busch, O Buthelezi, Z Caffarri, D Cai, X Caines, H CaleroDiaz, L Caliva, A Villar, EC Camerini, P Carena, F Carena, W Castellanos, JC Casula, EAR Catanescu, V Cavicchioli, C CeballosSanchez, C Cepila, J Cerello, P Chang, B Chapeland, S Charvet, JL Chattopadhyay, S Chattopadhyay, S Chelnokov, V Cherney, M Cheshkov, C Cheynis, B Barroso, VC Chinellato, DD Chochula, P Chojnacki, M Choudhury, S Christakoglou, P Christensen, CH Christiansen, P Chujo, T Chung, SU Cicalo, C Cifarelli, L Cindolo, F Cleymans, J Colamaria, F Colella, D Collu, A Colocci, M Balbastre, GC del Valle, ZC Connors, ME Contreras, JG Cormier, TM Morales, YC Cortese, P Maldonado, IC Cosentino, MR Costa, F Crochet, P Albino, RC Cuautle, E Cunqueiro, L Dainese, A Dang, R Danu, A Das, D Das, I Das, K Das, S Dash, A Dash, S De, S Delagrange, H Deloff, A Denes, E D'Erasmo, G de Caro, A de Cataldo, G de Cuveland, J De Falco, A De Gruttola, D De Marco, N De Pasquale, S de Rooij, R Corchero, MAD Dietel, T Dillenseger, P Divia, R Bari, D Di Liberto, S Di Mauro, A Di Nezza, P Djuvsland, O Dobrin, A Dobrowolski, T Gimenez, DD Donigus, B Dordic, O Dorheim, S Dubey, AK Dubla, A Ducroux, L Dupieux, P Majumdar, AKD Hilden, TE Ehlers, RJ Elia, D Engel, H Erazmus, B Erdal, HA Eschweiler, D Espagnon, B Esposito, M Estienne, M Esumi, S Evans, D Evdokimov, S Fabris, D Faivre, J Falchieri, D Fantoni, A Fasel, M Fehlker, D Feldkamp, L Felea, D Feliciello, A Feofilov, G Ferencei, J Tellez, AF Ferreiro, EG Ferretti, A Festanti, A Figiel, J Figueredo, MAS Filchagin, S Finogeev, D Fionda, FM Fiore, EM Floratos, E Floris, M Foertsch, S Foka, P Fokin, S Fragiacomo, E Francescon, A Frankenfeld, U Fuchs, U Furget, C FuscoGirard, M Gaardhoje, JJ Gagliardi, M Gago, AM Gallio, M Gangadharan, DR Ganoti, P Gao, C Garabatos, C Garcia-Solis, E Gargiulo, C Garishvili, I Gerhard, J Germain, M Gheata, A Gheata, M Ghidini, B Ghosh, P Ghosh, SK Gianotti, P Giubellino, P Gladysz-Dziadus, E Glassel, P Ramirez, AG Gonzlez-Zamora, P Gorbunov, S Grlich, L Gotovac, S Graczykowski, LK Grelli, A Grigoras, A Grigoras, C Grigoriev, V Grigoryan, A Grigoryan, S Grinyov, B Grion, N Grosse-Oetringhaus, JF Grossiord, JY Grosso, R Guber, F Guernane, R Guerzoni, B Guilbaud, M Gulbrandsen, K Gulkanyan, H Gumbo, M Gunji, T Gupta, A Gupta, R Khan, KH Haake, R Haaland, O Hadjidakis, C Haiduc, M Hamagaki, H Hamar, G Hanratty, LD Hansen, A Harris, JW Hartmann, H Harton, A Hatzifotiadou, D Hayashi, S Heckel, ST Heide, M Helstrup, H Herghelegiu, A Corral, GH Hess, BA Hetland, KF Hippolyte, B Hladky, J Hristov, P Huang, M Humanic, TJ Hussain, N Hutter, D Hwang, DS Ilkaev, R Ilkiv, I Inaba, M Innocenti, GM Ionita, C Ippolitov, M Irfan, M Ivanov, M Ivanov, V Jacholkowski, A Jacobs, PM Jahnke, C Jang, HJ Janik, MA Jayarathna, PHSY Jena, C Jena, S Bustamante, RTJ Jones, PG Jung, H Jusko, A Kadyshevskiy, V Kalcher, S Kalinak, P Kalweit, A Kamin, J Kang, JH Kaplin, V Kar, S Uysal, AK Karavichev, O Karavicheva, T Karpechev, E Kebschull, U Keidel, R Keijdener, DLD Khan, MM Khan, P Khan, SA Khanzadeev, A Kharlov, Y Kileng, B Kim, B Kim, DW Kim, DJ Kim, JS Kim, M Kim, M Kim, S Kim, T Kirsch, S Kisel, I Kiselev, S Kisiel, A Kiss, G Klay, JL Klein, J Klein-Bosing, C Kluge, A Knichel, ML Knospe, AG Kobdaj, C Kofarago, M Khler, MK Kollegger, T Kolojvari, A 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Rettig, F Revol, JP Reygers, K Riabov, V Ricci, RA Richert, T Richter, M Riedler, P Riegler, W Riggi, F Rivetti, A Rocco, E Cahuantzi, MR Manso, AR Roed, K Rogochaya, E Rohni, S Rohr, D Rohrich, D Romita, R Ronchetti, F Ronflette, L Rosnet, P Rossi, A Roukoutakis, F Roy, A Roy, C Roy, P Montero, AJR Rui, R Russo, R Ryabinkin, E Ryabov, Y Rybicki, A Sadovsky, S Safarik, K Sahlmuller, B Sahoo, R Sahu, PK Saini, J Sakai, S Salgado, CA Salzwedel, J Sambyal, S Samsonov, V Castro, XS Rodriguez, FJS Sandor, L Sandoval, A Sano, M Santagati, G Sarkar, D Scapparone, E Scarlassara, F Scharenberg, RP Schiaua, C Schicker, R Schmidt, C Schmidt, HR Schuchmann, S Schukraft, J Schulc, M Schuster, T Schutz, Y Schwarz, K Schweda, K Scioli, G Scomparin, E Scott, R Segato, G Seger, JE Sekiguchi, Y Selyuzhenkov, I Seo, J Serradilla, E Sevcenco, A Shabetai, A Shabratova, G Shahoyan, R Shangaraev, A Sharma, N Sharma, S Shigaki, K Shtejer, K Sibiriak, Y Siddhanta, S Siemiarczuk, T Silvermyr, D Silvestre, C Simatovic, G Singaraju, R Singh, R Singha, S Singhal, V Sinha, BC Sinha, T Sitar, B Sitta, M Skaali, TB Skjerdal, K Slupecki, M Smirnov, N Snellings, RJM Sogaard, C Soltz, R Song, J Song, M Soramel, F Sorensen, S Spacek, M Spiriti, E Sputowska, I Spyropoulou-Stassinaki, M Srivastava, BK Stachel, J Stan, I Stefanek, G Steinpreis, M Stenlund, E Steyn, G Stiller, JH Stocco, D Stolpovskiy, M Strmen, P Suaide, AAP Sugitate, T Suire, C Suleymanov, M Sultanov, R Sumbera, M Susa, T Symons, TJM Szabo, A de Toledo, AS Szarka, I Szczepankiewicz, A Szymanski, M Takahashi, J Tangaro, MA Takaki, JDT Peloni, AT Martinez, AT Tarzila, MG Tauro, A Munoz, GT Telesca, A Terrevoli, C Thader, J Thomas, D Tieulent, R Timmins, AR Toia, A Trubnikov, V Trzaska, H Tsuji, T Tumkin, A Turrisi, R Tveter, TS Ullaland, K Uras, A Usai, GL Vajzer, M Vala, M ValenciaPalomo, L Vallero, S Vyvre, PV Van Der Maarel, J Van Hoorne, JW van Leeuwen, M Vargas, A Vargyas, M Varma, R Vasileiou, M Vasiliev, A Vechernin, V Veldhoen, 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Trubnikov, V. Trzaska, H. Tsuji, T. Tumkin, A. Turrisi, R. Tveter, T. S. Ullaland, K. Uras, A. Usai, G. L. Vajzer, M. Vala, M. ValenciaPalomo, L. Vallero, S. Vyvre, P. Vand Van Der Maarel, J. Van Hoorne, J. W. van Leeuwen, M. Vargas, A. Vargyas, M. Varma, R. Vasileiou, M. Vasiliev, A. Vechernin, V. Veldhoen, M. Velure, A. Venaruzzo, M. Vercellin, E. Vergara Limon, S. Vernet, R. Verweij, M. Vickovic, L. Viesti, G. Viinikainen, J. Vilakazi, Z. Baillie, O. Villalobos Vinogradov, A. Vinogradov, L. Vinogradov, Y. Virgili, T. Viyogi, Y. P. Vodopyanov, A. Voelkl, M. A. Voloshin, K. Voloshin, S. A. Volpe, G. Vonhaller, B. Vorobyev, I. Vranic, D. Vrlalova, J. Vulpescu, B. Vyushin, A. Wagner, B. Wagner, J. Wagner, V. Wang, M. Wang, Y. Watanabe, D. Weber, M. Wessels, J. P. Westerhoff, U. Wiechula, J. Wikne, J. Wilde, M. Wilk, G. Wilkinson, J. Williams, M. C. S. Windelband, B. Winn, M. Yaldo, C. G. Yamaguchi, Y. Yang, H. Yang, P. Yang, S. Yano, S. Yasnopolskiy, S. Yi, J. Yin, Z. Yoo, I. -K. Yushmanov, I. Zaccolo, V. Zach, C. Zaman, A. Zampolli, C. Zaporozhets, S. Zarochentsev, A. Zavada, P. Zaviyalov, N. Zbroszczyk, H. Zgura, I. S. Zhalov, M. Zhang, H. Zhang, X. Zhang, Y. Zhao, C. Zhigareva, N. Zhou, D. Zhou, F. Zhou, Y. Zhou, Zhuo Zhu, H. Zhu, J. Zhu, X. Zichichi, A. Zimmermann, A. Zimmermann, M. B. Zinovjev, G. Zoccarato, Y. Zyzak, M. CA ALICE Collaboration TI Beauty production in pp collisions at root s=2.76 TeV measured via semi-electronic decays SO PHYSICS LETTERS B LA English DT Article DE LHC; ALICE experiment; pp collisions; Single electrons; Heavy flavour production; Beauty production ID QUARK-GLUON PLASMA; LHC; COLLABORATION; PERSPECTIVE; ALICE AB The ALICE Collaboration at the LHC reports measurement of the inclusive production cross section of electrons from semi-leptonic decays of beauty hadrons with rapidity |y| < 0.8 and transverse momentum 1 < p(T)< 10 GeV/c, in pp collisions at root s = 2.76 TeV. Electrons not originating from semi-electronic decay of beauty hadrons are suppressed using the impact parameter of the corresponding tracks. The production cross section of beauty decay electrons is compared to the result obtained with an alternative method which uses the distribution of the azimuthal angle between heavy-flavour decay electrons and charged hadrons. Perturbative QCD predictions agree with the measured cross section within the experimental and theoretical uncertainties. The integrated visible cross section, sigma(b -> e) = 3.47 +/- 0.40(stat)(+1.12)(-1.33)(sys) +/- 0.07(norm) mu b, was extrapolated to full phase space using Fixed Order plus Next-to-Leading Log (FONLL) calculations to obtain the total b (b) over bar production cross section, sigma(b (b) over bar) = 130 +/- 15.1(stat)(+42.1)(-49.8)(sys)(+3.4)(-3.1)(extr) +/- 2.5(norm) +/- 4.4(BR) mu b. (C) 2014 The Authors. Published by Elsevier B.V. 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S.; Kim, S.] Sejong Univ, Dept Phys, Seoul, South Korea. [Arsene, I. C.; Batzing, P. C.; Dordic, O.; Lindal, S.; Mahmood, S. M.; Milosevic, J.; Qvigstad, H.; Richter, M.; Roed, K.; Skaali, T. B.; Tveter, T. S.; Wikne, J.; Zhao, C.] Univ Oslo, Dept Phys, Oslo, Norway. [Meddi, F.] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy. [Casula, E. A. R.; Collu, A.; De Falco, A.; Di Liberto, S.; Mazzoni, M. A.; Puddu, G.; Razazi, V.; Terrevoli, C.; Usai, G. L.] Sezione Ist Nazl Fis Nucl, Rome, Italy. [Casula, E. A. R.; Collu, A.; De Falco, A.; Puddu, G.; Razazi, V.; Terrevoli, C.; Usai, G. L.] Dipartimento Fis Univ, Cagliari, Italy. [Casula, E. A. R.; Cicalo, C.; Collu, A.; De Falco, A.; Lea, R.; Luparello, G.; Margagliotti, G. V.; Masoni, A.; Puddu, G.; Razazi, V.; Rui, R.; Siddhanta, S.; Terrevoli, C.; Usai, G. L.; Venaruzzo, M.] Sezione Ist Nazl Fis Nucl, Cagliari, Italy. [Camerini, P.; Lea, R.; Luparello, G.; Margagliotti, G. V.; Rui, R.; Venaruzzo, M.] Dipartimento Fis Univ, Trieste, Italy. [Camerini, P.; Fragiacomo, E.; Grion, N.; Lea, R.; Luparello, G.; Margagliotti, G. V.; Piano, S.; Rachevski, A.; Rui, R.; Venaruzzo, M.] Sezione Ist Nazl Fis Nucl, Trieste, Italy. [Beole, S.; Berzano, D.; Bianchi, L.; Botta, E.; Morales, Y. Corrales; Ferretti, A.; Gagliardi, M.; Gallio, M.; Innocenti, G. M.; Lattuca, A.; Leoncino, M.; Marchisone, M.; Masera, M.; Russo, R.; Shtejer, K.; Vallero, S.; Vercellin, E.] Dipartimento Fis Univ, Turin, Italy. [Agnello, M.; Aimo, I.; Alessandro, B.; Arnaldi, R.; Bagnasco, S.; Berzano, D.; Bianchi, L.; Botta, E.; Bruna, E.; Bufalino, S.; Cerello, P.; Morales, Y. Corrales; De Marco, N.; Feliciello, A.; Ferretti, A.; Gagliardi, M.; Gallio, M.; Innocenti, G. M.; Lattuca, A.; La Pointe, S. L.; Leoncino, M.; Manceau, L.; Marchisone, M.; Masera, M.; Oppedisano, C.; Prino, F.; Rivetti, A.; Russo, R.; Scomparin, E.; Shtejer, K.; Vallero, S.; Vercellin, E.] Sezione Ist Nazl Fis Nucl, Turin, Italy. [Agostinelli, A.; Arcelli, S.; Basile, M.; Bellini, F.; Cifarelli, L.; Colocci, M.; Falchieri, D.; Guerzoni, B.; Scioli, G.; Zichichi, A.] Univ Bologna, Dipartimento Fis & Astron, Bologna, Italy. [Agostinelli, A.; Alici, A.; Antonioli, P.; Arcelli, S.; Basile, M.; Bellini, F.; Cifarelli, L.; Cindolo, F.; Colocci, M.; Falchieri, D.; Guerzoni, B.; Hatzifotiadou, D.; Margotti, A.; Nania, R.; Noferini, F.; Pesci, A.; Pinazza, O.; Preghenella, R.; Scapparone, E.; Scioli, G.; Williams, M. C. S.; Zampolli, C.; Zichichi, A.] Sezione Ist Nazl Fis Nucl, Bologna, Italy. [Barbera, R.; Jacholkowski, A.; La Rocca, P.; Petta, C.; Riggi, F.; Santagati, G.] Univ Catania, Dipartmento Fis & Astron, Catania, Italy. [Badala, A.; Barbera, R.; Jacholkowski, A.; La Rocca, P.; Palmeri, A.; Pappalardo, G. S.; Petta, C.; Riggi, F.; Santagati, G.] Sezione Ist Nazl Fis Nucl, Catania, Italy. [Festanti, A.; Francescon, A.; Jena, C.; Lunardon, M.; Morando, M.; Moretto, S.; Scarlassara, F.; Segato, G.; Soramel, F.; Viesti, G.] Univ Padua, Dipartimento Fis & Astron, Padua, Italy. [Antinori, F.; Dainese, A.; Fabris, D.; Festanti, A.; Francescon, A.; Jena, C.; Lunardon, M.; Morando, M.; Moretto, S.; Scarlassara, F.; Segato, G.; Soramel, F.; Toia, A.; Turrisi, R.; Viesti, G.] Sezione Ist Nazl Fis Nucl, Padua, Italy. [de Caro, A.; De Gruttola, D.; De Pasquale, S.; FuscoGirard, M.; Pagano, P.; Virgili, T.] Univ Salerno, Dipartimento Fis ER Caianiello, I-84100 Salerno, Italy. [de Caro, A.; De Gruttola, D.; De Pasquale, S.; FuscoGirard, M.; Pagano, P.; Virgili, T.] Grp Coll INFN, I-84100 Salerno, Italy. [Cortese, P.; Ramello, L.; Sitta, M.] Univ Piemonte Orientale, Dipartimento Sci & Innovaz Tecnol, Alessandria, Italy. [Cortese, P.; Ramello, L.; Sitta, M.] Grp Coll INFN, Alessandria, Italy. [Barile, F.; Bruno, G. E.; Colamaria, F.; Colella, D.; D'Erasmo, G.; Di Bari, D.; Fionda, F. M.; Fiore, E. M.; Ghidini, B.; Mastroserio, A.; Tangaro, M. A.] Dipartimento Interateneo Fis M Merlin, Bari, Italy. [Barile, F.; Bruno, G. E.; Colamaria, F.; Colella, D.; D'Erasmo, G.; de Cataldo, G.; Di Bari, D.; Elia, D.; Fionda, F. M.; Fiore, E. M.; Ghidini, B.; Lenti, V.; Manzari, V.; Mastroserio, A.; Nappi, E.; Paticchio, V.; Tangaro, M. A.] Sezione Ist Nazl Fis Nucl, Bari, Italy. [Christiansen, P.; Ljunggren, H. M.; OrtizVelasquez, A.; Oskarsson, A.; Richert, T.; Sogaard, C.; Stenlund, E.] Lund Univ, Div Expt High Energy Phys, Lund, Sweden. [Hess, B. A.; Schmidt, H. R.; Wiechula, J.] Univ Tubingen, Tubingen, Germany. [Rinella, G. Aglieri; Augustinus, A.; Pedrosa, F. Baltasar Dos Santos; Betev, L.; Buncic, P.; Caffarri, D.; Carena, F.; Carena, W.; Cavicchioli, C.; Chapeland, S.; Barroso, V. Chibante; Chochula, P.; Costa, F.; Cunqueiro, L.; Divia, R.; Di Mauro, A.; Erazmus, B.; Esposito, M.; Floris, M.; Francescon, A.; Fuchs, U.; Gargiulo, C.; Gheata, A.; Gheata, M.; Giubellino, P.; Grigoras, A.; Grigoras, C.; Grosse-Oetringhaus, J. F.; Grosso, R.; Hristov, P.; Ionita, C.; Kalweit, A.; Kluge, A.; Kobdaj, C.; Kofarago, M.; Kryshen, E.; Kugathasan, T.; Legrand, I.; Mager, M.; Martinengo, P.; Milano, L.; Morsch, A.; Mueller, H.; Musa, L.; Niculescu, M.; Pinazza, O.; Reidt, F.; Revol, J. -P.; Riedler, P.; Riegler, W.; Rossi, A.; Safarik, K.; Schukraft, J.; Schutz, Y.; Shahoyan, R.; Szczepankiewicz, A.; Martinez, A. Tarazona; Tauro, A.; Telesca, A.; Vyvre, P. Vand; Van Hoorne, J. W.; Volpe, G.; Vonhaller, B.; Vranic, D.; Weber, M.; Zimmermann, M. B.] European Org Nucl Res CERN, Geneva, Switzerland. [Alme, J.; Erdal, H. A.; Helstrup, H.; Hetland, K. F.; Kileng, B.] Bergen Univ Coll, Fac Engn, Bergen, Norway. [Meres, M.; Pikna, M.; Sitar, B.; Strmen, P.; Szabo, A.; Szarka, I.] Comenius Univ, Fac Math Phys & Informat, Bratislava, Slovakia. [Adam, J.; Bielcik, J.; Broz, M.; Cepila, J.; Contreras, J. G.; Krelina, M.; Pachr, M.; Petracek, V.; Petran, M.; Schulc, M.; Spacek, M.; Wagner, V.; Zach, C.] Czech Tech Univ, Fac Nucl Sci & Phys Engn, CR-11519 Prague, Czech Republic. [Bombara, M.; Kravcakova, A.; Vrlalova, J.] Safarik Univ, Fac Sci, Kosice, Slovakia. [Alt, T.; Bach, M.; de Cuveland, J.; Eschweiler, D.; Gerhard, J.; Gorbunov, S.; Hartmann, H.; Hutter, D.; Kalcher, S.; Kirsch, S.; Kisel, I.; Kollegger, T.; Kretz, M.; Krzewicki, M.; Lindenstruth, V.; Painke, F.; Rettig, F.; Rohr, D.] Goethe Univ Frankfurt, Frankfurt Inst Adv Studies, D-60054 Frankfurt, Germany. [Baek, Y. W.; Jung, H.; Kim, D. W.; Kim, J. S.; Kim, M.; Oh, S. K.] Gangneung Wonju Natl Univ, Kangnung, South Korea. [Bhattacharjee, B.; Hussain, N.] Gauhati Univ, Dept Phys, Gauhati, India. [Hilden, T. E.; Pohjoisaho, E. H. O.; Rasanen, S.] Helsinki Inst Phys, Helsinki, Finland. [Shigaki, K.; Sugitate, T.; Yano, S.] Hiroshima Univ, Hiroshima, Japan. [Agrawal, N.; Behera, N. K.; Dash, S.; Meethaleveedu, G. Koyithatta; Kumar, J.; Nandi, B. K.; Pant, D.; Varma, R.] Indian Inst Technol, Bombay 400076, Maharashtra, India. [Mishra, A. N.; Sahoo, P.; Pareek, P.; Roy, A.; Sahoo, R.] Indian Inst Technol, Indore, Madhya Pradesh, India. [Kweon, M. J.] Inha Univ, Inchon, South Korea. [del Valle, Z. Conesa; Das, I.; Espagnon, B.; Hadjidakis, C.; Lakomov, I.; Takaki, J. D. Tapia] Univ Paris 11, CNRS, IN2P3, IPNO, Orsay, France. [Boettger, S.; Breitner, T.; Engel, H.; Ramirez, A. Gomez; Kebschull, U.; Lara, C.] Goethe Univ Frankfurt, Inst Informat, D-60054 Frankfurt, Germany. [Appelshaeuser, H.; Arslandok, M.; Bailhache, R.; Baumann, C.; Beck, H.; Blume, C.; Book, J.; Broker, T. A.; Buesching, H.; Dillenseger, P.; Doenigus, B.; Heckel, S. T.; Kamin, J.; Kulakov, I.; Lehnert, J.; Luettig, P.; Marquard, M.; Ozdemir, M.; Peskov, V.; Rascanu, B. T.; Reichelt, P.; Renfordt, R.; Sahlmuller, B.; Schuchmann, S.; Peloni, A. Tarantola; Toia, A.; Zyzak, M.] Goethe Univ Frankfurt, Inst Kernphys, D-60054 Frankfurt, Germany. [Anielski, J.; Bathen, B.; Dietel, T.; Feldkamp, L.; Haake, R.; Heide, M.; Klein-Boesing, C.; Muehlheim, D.; Passfeld, A.; Wessels, J. P.; Westerhoff, U.; Wilde, M.; Zimmermann, M. B.] Univ Munster, Inst Kernphys, D-48149 Munster, Germany. [Belikov, I.; Hippolyte, B.; Kuhn, C.; Maire, A.; Molnar, L.; Roy, C.; Castro, X. Sanchez] Univ Strasbourg, IN2P3, CNRS, IPHC, Strasbourg, France. [Finogeev, D.; Guber, F.; Karavichev, O.; Karavicheva, T.; Karpechev, E.; Konevskikh, A.; Kurepin, A.; Kurepin, A. B.; Maevskaya, A.; Pshenichnov, I.; Reshetin, A.] Acad Sci, Nucl Res Inst, Moscow, Russia. [Bertens, R. A.; Bianchin, C.; Bjelogrlic, S.; Caliva, A.; de Rooij, R.; Dobrin, A.; Dubla, A.; Grelli, A.; Keijdener, D. L. D.; La Pointe, S. L.; Leogrande, E.; Lodato, D. F.; Luparello, G.; Mischke, A.; Mohammadi, N.; Nooren, G.; Peitzmann, T.; Reicher, M.; Rocco, E.; Snellings, R. J. M.; Thomas, D.; Van Der Maarel, J.; van Leeuwen, M.; Veldhoen, M.; Yang, H.; Zhou, Y.] Univ Utrecht, Inst Subat Phys, Utrecht, Netherlands. [Akindinov, A.; Kiselev, S.; Mal'Kevich, D.; Mikhaylov, K.; Nedosekin, A.; Sultanov, R.; Voloshin, K.; Zhigareva, N.] Inst Theoret & Expt Phys, Moscow 117259, Russia. [Kalinak, P.; Kralik, I.; Krivda, M.; Musinsky, J.; Sandor, L.; Vala, M.] Slovak Acad Sci, Inst Expt Phys, Kosice 04353, Slovakia. [Hladky, J.; Mares, J.; Zavada, P.] Acad Sci Czech Republic, Inst Phys, Prague, Czech Republic. [Baral, R. C.; Mahapatra, D. P.; Sahu, P. K.] Inst Phys, Bhubaneswar 751007, Orissa, India. [Danu, A.; Felea, D.; Gheata, M.; Haiduc, M.; Mitu, C. M.; Niculescu, M.; Sevcenco, A.; Stan, I.; Zgura, I. S.] Inst Space Sci, Bucharest, Romania. [Cuautle, E.; Jimenez Bustamante, R. T.; Ladron de Guevara, P.; Maldonado Cervantes, I.; OrtizVelasquez, A.; Paic, G.] Univ Nacl Autonoma Mexico, Inst Ciencias Nucl, Mexico City 04510, DF, Mexico. [Belmont-Moreno, E.; Menchaca-Rocha, A.; Sandoval, A.; Serradilla, E.] Univ Nacl Autonoma Mexico, Inst Fis, Mexico City 01000, DF, Mexico. [Bossu, F.; Buthelezi, Z.; Foertsch, S.; Steyn, G.; Vilakazi, Z.] Natl Res Fdn, IThemba LABS, Somerset, NJ, South Africa. [Batyunya, B.; Grigoryan, S.; Kadyshevskiy, V.; Malinina, L.; Mikhaylov, K.; Nomokonov, P.; Rogochaya, E.; Shabratova, G.; Vala, M.; Vodopyanov, A.; Zaporozhets, S.] Joint Nucl Res Inst, Dubna, Russia. [Oh, S. K.] Konkuk Univ, Seoul, South Korea. [Ahn, S. U.; Ahn, S. A.; Jang, H. J.; Kim, D. W.] Korea Inst Sci & Technol Informat, Taejon, South Korea. [Uysal, A. Karasu; Okatan, A.] KTO Karatay Univ, Konya, Turkey. [Baek, Y. W.; Barret, V.; Bastid, N.; Camejo, A. Batista; Crochet, P.; Dupieux, P.; Li, S.; Lopez, X.; Manso, F.; Marchisone, M.; Porteboeuf-Houssais, S.; Rosnet, P.; ValenciaPalomo, L.; Vulpescu, B.] Univ Clermont Ferrand, Clermont Univ, IN2P3, CNRS,LPC, Clermont Ferrand, France. [Balbastre, G. Conesa; Faivre, J.; Furget, C.; Guernane, R.; Kox, S.; Real, J. S.; Silvestre, C.] Univ Grenoble Alpes, IN2P3, CNRS, Lab Phys Subatom & Cosmol, Grenoble, France. [Bianchi, N.; CaleroDiaz, L.; Cunqueiro, L.; Di Nezza, P.; Fantoni, A.; Gianotti, P.; Muccifora, V.; Reolon, A. R.; Ronchetti, F.; Sakai, S.; Spiriti, E.] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy. [Ricci, R. A.; Venaruzzo, M.] Ist Nazl Fis Nucl, Lab Nazl Legnaro, I-35020 Legnaro, Italy. [Bock, F.; Gangadharan, D. R.; Jacobs, P. M.; Loizides, C.; Ploskon, M.; Porter, J.; Sakai, S.; Symons, T. J. M.; Zhang, X.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. 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[Bala, R.; Bhasin, A.; Bhat, I. R.; Gupta, A.; Gupta, R.; Potukuchi, B.; Rohni, S.; Sambyal, S.; Sharma, S.; Singh, R.] Univ Jammu, Dept Phys, Jammu 180004, India. [Raniwala, R.; Raniwala, S.] Univ Rajasthan, Dept Phys, Jaipur 302004, Rajasthan, India. [Berger, M. E.; Boehmer, F. V.; Dorheim, S.] Tech Univ Munich, Dept Phys, D-80290 Munich, Germany. [Anguelov, V.; Bock, F.; Busch, O.; Fasel, M.; Glaessel, P.; Klein, J.; Kweon, M. J.; Leardini, L.; Lohner, D.; Lu, X. -G.; Maire, A.; Mercado Perez, J.; Oeschler, H.; Oyama, K.; Pachmayer, Y.; Reygers, K.; Schicker, R.; Stachel, J.; Stiller, J. H.; Vallero, S.; Voelkl, M. A.; Wang, Y.; Wilkinson, J.; Windelband, B.; Winn, M.; Zimmermann, A.] Heidelberg Univ, Physikal Inst, Heidelberg, Germany. [Agnello, M.; Aimo, I.; Bedda, C.] Politecn Torino, Turin, Italy. [Browning, T. A.; Scharenberg, R. P.; Srivastava, B. K.] Purdue Univ, W Lafayette, IN 47907 USA. [Borissov, A.; Chung, S. U.; Seo, J.; Song, J.; Yi, J.; Yoo, I. -K.] Pusan Natl Univ, Pusan 609735, South Korea. [Andronic, A.; Arsene, I. C.; Averbeck, R.; Braun-Munzinger, P.; Foka, P.; Frankenfeld, U.; Garabatos, C.; Ivanov, M.; Knichel, M. L.; Khler, M. K.; Krzewicki, M.; Lippmann, C.; Malzacher, P.; Marin, A.; Martin, N. A.; Masciocchi, S.; Miskowiec, D.; Nicassio, M.; Onderwaater, J.; Otwinowski, J.; Park, W. J.; Schmidt, C.; Schwarz, K.; Schweda, K.; Selyuzhenkov, I.; Thaeder, J.; Vranic, D.; Wagner, J.] GSI Helmholtzzentrum Schwerionenforschung, Div Res, Darmstadt, Germany. [Andronic, A.; Arsene, I. C.; Averbeck, R.; Braun-Munzinger, P.; Foka, P.; Frankenfeld, U.; Garabatos, C.; Ivanov, M.; Knichel, M. L.; Khler, M. K.; Krzewicki, M.; Lippmann, C.; Malzacher, P.; Marin, A.; Martin, N. A.; Masciocchi, S.; Miskowiec, D.; Nicassio, M.; Onderwaater, J.; Otwinowski, J.; Park, W. J.; Schmidt, C.; Schwarz, K.; Schweda, K.; Selyuzhenkov, I.; Thaeder, J.; Vranic, D.; Wagner, J.] GSI Helmholtzzentrum Schwerionenforschung, ExtreMe Matter Inst EMMI, Darmstadt, Germany. [Anticic, T.; Planinic, M.; Poljak, N.; Susa, T.] Rudjer Boskovic Inst, Zagreb, Croatia. [Budnikov, D.; Filchagin, S.; Ilkaev, R.; Kuryakin, A.; Mamonov, A.; Nazarenko, S.; Punin, V.; Tumkin, A.; Vinogradov, Y.; Vyushin, A.; Zaviyalov, N.] Russian Fed Nucl Ctr VNIIEF, Sarov, Russia. [Aleksandrov, D.; Blau, D.; Fokin, S.; Ippolitov, M.; Kucheriaev, Y.; Manko, V.; Nikolaev, S.; Nikulin, S.; Nyanin, A.; Peresunko, D.; Ryabinkin, E.; Sibiriak, Y.; Vasiliev, A.; Vinogradov, A.; Yasnopolskiy, S.; Yushmanov, I.] Russian Res Ctr Kurchatov Inst, Moscow, Russia. [Chattopadhyay, S.; Das, D.; Das, K.; Majumdar, A. K. Dutta; Khan, P.; Paul, B.; Roy, P.; Sinha, T.] Saha Inst Nucl Phys, Kolkata, India. [Alexandre, D.; Barnby, L. S.; Evans, D.; Hanratty, L. D.; Jones, P. G.; Jusko, A.; Krivda, M.; Lee, G. R.; Lietava, R.; Baillie, O. Villalobos] Univ Birmingham, Sch Phys & Astron, Birmingham, W Midlands, England. [Villar, E. Calvo; Gago, A. M.] Pontificia Univ Catolica Peru, Dept Ciencias, Secc Fis, Lima, Peru. [Bogolyubsky, M.; Evdokimov, S.; Kharlov, Y.; Patalakha, D. I.; Polichtchouk, L.; Sadovsky, S.; Shangaraev, A.; Stolpovskiy, M.] NRC Kurchatov Inst, SSC IHEP, Protvino, Russia. [Aphecetche, L.; Batigne, G.; Delagrange, H.; Erazmus, B.; Estienne, M.; Germain, M.; Lardeux, A.; Martiinez Garcia, G.; MartinBlanco, J.; Mas, A.; Massacrier, L.; Morreale, A.; Pillot, P.; Ronflette, L.; Schutz, Y.; Shabetai, A.; Stocco, D.; Wang, M.] Univ Nantes, IN2P3, CNRS, Ecole Mines Nantes,SUBTECH, Nantes, France. [Kobdaj, C.] Suranaree Univ Technol, Nakhon Ratchasima, Thailand. [Gotovac, S.; Mudnic, E.; Vickovic, L.] Tech Univ Split FESB, Split, Croatia. [Bartke, J.; Figiel, J.; Gladysz-Dziadus, E.; Grlich, L.; Kowalski, M.; Matyja, A.; Mayer, C.; Otwinowski, J.; Rybicki, A.; Sputowska, I.] Polish Acad Sci, Henryk Niewodniczanski Inst Nucl Phys, Krakow, Poland. [Knospe, A. G.; Markert, C.] Univ Texas Austin, Dept Phys, Austin, TX 78712 USA. [Leon Monzon, I.; Podesta-Lerma, P. L. M.; Sanchez Rodriguez, F. J.] Univ Autonoma Sinaloa, Culiacan, Mexico. [Alves Garcia Prado, C.; Bregant, M.; Cosentino, M. R.; Domenicis Gimenez, D.; Jahnke, C.; Lagana Fernandes, C.; Moreira De Godoy, D. A.; Munhoz, M. G.; Oliveira Da Silva, A. C.; Pereira De Oliveira Filho, E.; Suaide, A. A. P.; Szanto de Toledo, A.] Univ Sao Paulo, Sao Paulo, Brazil. [Chinellato, D. D.; Dash, A.; Takahashi, J.] Univ Estadual Campinas, Campinas, Brazil. [Bellwied, R.; Chinellato, D. D.; Jayarathna, P. H. S. Y.; Jena, S.; Pinsky, L.; Piyarathna, D. B.; Timmins, A. R.; Weber, M.] Univ Houston, Houston, TX USA. [Chang, B.; Kim, D. J.; Kral, J.; Rak, J.; Slupecki, M.; Trzaska, H.; Vargyas, M.; Viinikainen, J.] Univ Jyvaskyla, Jyvaskyla, Finland. [Figueredo, M. A. S.; Norman, J.; Romita, R.] Univ Liverpool, Liverpool L69 3BX, Merseyside, England. [Martashvili, I.; Mazer, J.; Nattrass, C.; Read, K. F.; Scott, R.; Sharma, N.; Sorensen, S.] Univ Tennessee, Knoxville, TN USA. [Gunji, T.; Hamagaki, H.; Hayashi, S.; Sekiguchi, Y.; Tsuji, T.; Yamaguchi, Y.] Univ Tokyo, Tokyo, Japan. [Bhom, J.; Chujo, T.; Esumi, S.; Inaba, M.; Miake, Y.; Sano, M.; Watanabe, D.] Univ Tsukuba, Tsukuba, Ibaraki, Japan. [Planinic, M.; Poljak, N.; Simatovic, G.] Univ Zagreb, Zagreb 41000, Croatia. [Cheshkov, C.; Cheynis, B.; Ducroux, L.; Grossiord, J. -Y.; Guilbaud, M.; Tieulent, R.; Uras, A.; Zoccarato, Y.] Univ Lyon 1, Univ Lyon, IN2P3, CNRS,IPN Lyon, F-69622 Villeurbanne, France. [Altsybeev, I.; Feofilov, G.; Kolojvari, A.; Kondratiev, V.; Kovalenko, V.; Vechernin, V.; Vinogradov, L.; Vorobyev, I.; Zarochentsev, A.] St Petersburg State Univ, V Fock Inst Phys, St Petersburg 199034, Russia. [Ahammed, Z.; Alam, S. N.; Basu, S.; Chattopadhyay, S.; Choudhury, S.; De, S.; Dubey, A. K.; Ghosh, P.; Kar, S.; Khan, S. A.; Mitra, J.; Mohanty, B.; Muhuri, S.; Mukherjee, M.; Nayak, T. K.; Pal, S. K.; Saini, J.; Sarkar, D.; Singaraju, R.; Singha, S.; Singhal, V.; Sinha, B. C.; Viyogi, Y. P.] Ctr Variable Energy Cyclotron, Kolkata, India. [Langoy, R.; Lien, J.] Vestfold Univ Coll, Tonsberg, Norway. [Graczykowski, L. K.; Janik, M. A.; Kisiel, A.; Oleniacz, J.; Pawlak, T.; Pluta, J.; Szymanski, M.; Zbroszczyk, H.] Warsaw Univ Technol, Warsaw, Poland. [Belmont, R., III; Borissov, A.; Cormier, T. M.; Loggins, R.; Mlynarz, J.; Prasad, S. K.; Pruneau, C. A.; Pujahari, P.; Putschke, J.; Reed, R. J.; Verweij, M.; Voloshin, S. A.; Yaldo, C. G.] Wayne State Univ, Detroit, MI USA. [Barnafoldi, G. G.; Bencedi, G.; Berenyi, D.; Boldizsar, L.; Denes, E.; Hamar, G.; Kiss, G.; Levai, P.; Olah, L.; Pochybova, S.] Hungarian Acad Sci, Wigner Res Ctr Phys, Budapest, Hungary. [Aiola, S.; Aronsson, T.; Caines, H.; Connors, M. E.; Ehlers, R. J.; Harris, J. W.; Ma, R.; Majka, R. D.; Oh, S.; Reed, R. J.; Schuster, T.; Smirnov, N.] Yale Univ, New Haven, CT USA. [Kang, J. H.; Kim, B.; Kim, M.; Kim, T.; Kwon, Y.; Song, M.] Yonsei Univ, Seoul 120749, South Korea. [Keidel, R.] Fachhochschule Worms, Zentrum Technologietransfer & Telekommun, Worms, Germany. [Berdnikov, Y.] St Petersburg State Polytech Univ, St Petersburg, Russia. [Delagrange, H.; Kucheriaev, Y.] Aligarh Muslim Univ, Dept Appl Phys, Aligarh, Uttar Pradesh, India. [Malinina, L.] Moscow MV Lomonosov State Univ, DV Skobeltsyn Inst Nucl Phys, Moscow, Russia. [Milosevic, J.] Univ Belgrade, Fac Phys, Belgrade, Serbia. [Milosevic, J.] Vinca Inst Nucl Sci, Belgrade, Serbia. [Oh, S. K.] Konkuk Univ, Seoul, South Korea. [Redlich, K.] Univ Wroclaw, Inst Theoret Phys, PL-50138 Wroclaw, Poland. [Takaki, J. D. Tapia] Univ Kansas, Lawrence, KS 66045 USA. RP Abelev, B (reprint author), Yerevan Phys Inst Fdn, AI Alikhanyan Natl Sci Lab, Yerevan, Armenia. RI Ahmed, Ijaz/E-9144-2015; Usai, Gianluca/E-9604-2015; Salgado, Carlos A./G-2168-2015; Bregant, Marco/I-7663-2012; Barnby, Lee/G-2135-2010; Barbera, Roberto/G-5805-2012; Bruna, Elena/C-4939-2014; Karasu Uysal, Ayben/K-3981-2015; HAMAGAKI, HIDEKI/G-4899-2014; Pshenichnov, Igor/A-4063-2008; Guber, Fedor/I-4271-2013; Zarochentsev, Andrey/J-6253-2013; Altsybeev, Igor/K-6687-2013; Kovalenko, Vladimir/C-5709-2013; Sumbera, Michal/O-7497-2014; Peitzmann, Thomas/K-2206-2012; Kharlov, Yuri/D-2700-2015; Mitu, Ciprian/E-6733-2011; Sevcenco, Adrian/C-1832-2012; Takahashi, Jun/B-2946-2012; Felea, Daniel/C-1885-2012; Barnafoldi, Gergely Gabor/L-3486-2013; Kucera, Vit/G-8459-2014; Krizek, Filip/G-8967-2014; Vajzer, Michal/G-8469-2014; Wagner, Vladimir/G-5650-2014; Vinogradov, Leonid/K-3047-2013; Kondratiev, Valery/J-8574-2013; Vechernin, Vladimir/J-5832-2013; Janik, Malgorzata/O-7520-2015; Graczykowski, Lukasz/O-7522-2015; feofilov, grigory/A-2549-2013; Adamova, Dagmar/G-9789-2014; Christensen, Christian/D-6461-2012; De Pasquale, Salvatore/B-9165-2008; Chinellato, David/D-3092-2012; Armesto, Nestor/C-4341-2017; Ferretti, Alessandro/F-4856-2013; Martinez Hernandez, Mario Ivan/F-4083-2010; Vickovic, Linda/F-3517-2017; Fernandez Tellez, Arturo/E-9700-2017; Nielsen, Borge S/C-3719-2015; de Cuveland, Jan/H-6454-2016; Kurepin, Alexey/H-4852-2013; Jena, Deepika/P-2873-2015; Jena, Satyajit/P-2409-2015; Akindinov, Alexander/J-2674-2016; Nattrass, Christine/J-6752-2016; Cosentino, Mauro/L-2418-2014; Suaide, Alexandre/L-6239-2016; Castillo Castellanos, Javier/G-8915-2013; Inst. of Physics, Gleb Wataghin/A-9780-2017; Ferreiro, Elena/C-3797-2017 OI Usai, Gianluca/0000-0002-8659-8378; Salgado, Carlos A./0000-0003-4586-2758; Barnby, Lee/0000-0001-7357-9904; Barbera, Roberto/0000-0001-5971-6415; Bruna, Elena/0000-0001-5427-1461; Karasu Uysal, Ayben/0000-0001-6297-2532; Pshenichnov, Igor/0000-0003-1752-4524; Guber, Fedor/0000-0001-8790-3218; Zarochentsev, Andrey/0000-0002-3502-8084; Altsybeev, Igor/0000-0002-8079-7026; Kovalenko, Vladimir/0000-0001-6012-6615; Sumbera, Michal/0000-0002-0639-7323; Peitzmann, Thomas/0000-0002-7116-899X; Sevcenco, Adrian/0000-0002-4151-1056; Takahashi, Jun/0000-0002-4091-1779; Felea, Daniel/0000-0002-3734-9439; Vinogradov, Leonid/0000-0001-9247-6230; Kondratiev, Valery/0000-0002-0031-0741; Vechernin, Vladimir/0000-0003-1458-8055; Janik, Malgorzata/0000-0002-3356-3438; feofilov, grigory/0000-0003-3700-8623; Christensen, Christian/0000-0002-1850-0121; De Pasquale, Salvatore/0000-0001-9236-0748; Chinellato, David/0000-0002-9982-9577; Scarlassara, Fernando/0000-0002-4663-8216; Turrisi, Rosario/0000-0002-5272-337X; D'Erasmo, Ginevra/0000-0003-3407-6962; Beole', Stefania/0000-0003-4673-8038; Fernandez Tellez, Arturo/0000-0001-5092-9748; Armesto, Nestor/0000-0003-0940-0783; Ferretti, Alessandro/0000-0001-9084-5784; Martinez Hernandez, Mario Ivan/0000-0002-8503-3009; Vickovic, Linda/0000-0002-9820-7960; Fernandez Tellez, Arturo/0000-0003-0152-4220; Nielsen, Borge S/0000-0002-0091-1934; Gago Medina, Alberto Martin/0000-0002-0019-9692; Riggi, Francesco/0000-0002-0030-8377; Dainese, Andrea/0000-0002-2166-1874; Paticchio, Vincenzo/0000-0002-2916-1671; de Cuveland, Jan/0000-0003-0455-1398; Kurepin, Alexey/0000-0002-1851-4136; Jena, Deepika/0000-0003-2112-0311; Jena, Satyajit/0000-0002-6220-6982; Akindinov, Alexander/0000-0002-7388-3022; Nattrass, Christine/0000-0002-8768-6468; Cosentino, Mauro/0000-0002-7880-8611; Suaide, Alexandre/0000-0003-2847-6556; Castillo Castellanos, Javier/0000-0002-5187-2779; Ferreiro, Elena/0000-0002-4449-2356 FU State Committee of Science; World Federation of Scientists (WFS); Swiss Fonds Kidagan, Armenia; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq); Financiadora de Estudos e Projetos (FINEP); Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP); National Natural Science Foundation of China (NSFC); Chinese Ministry of Education (CMOE); Ministry of Science and Technology of China (MSTC); Ministry of Education and Youth of the Czech Republic; Danish Natural Science Research Council; Carlsberg Foundation; Danish National Research Foundation; European Research Council under the European Community's Seventh Framework Programme; Helsinki Institute of Physics; Academy of Finland; French CNRS-IN2P3; Region Pays de Loire; Region Alsace; Region Auvergne; CEA, France; German BMBF; Helmholtz Association; General Secretariat for Research and Technology; Ministry of Development, Greece; Hungarian OTKA; National Office for Research and Technology (NKTH); Department of Atomic Energy and Department of Science and Technology of the Government of India; Istituto Nazionale di Fisica Nucleare (INFN); Centro Fermi - Museo Storico della Fisica e Centro Studi e Ricerche "Enrico Fermi", Italy; MEXT; Joint Institute for Nuclear Research, Dubna; National Research Foundation of Korea (NRF); CONACYT; DGAPA, Mexico; ALFA-EC; EPLANET Program (European Particle Physics Latin American Network) Stichting voor Fundamenteel Onderzoek der Materie (FOM); Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Netherlands; Research Council of Norway (NFR); Polish Ministry of Science and Higher Education; National Science Centre, Poland; Ministry of National Education/Institute for Atomic Physics and CNCS-UEFISCDI - Romania; Ministry of Education and Science of Russian Federation; Russian Academy of Sciences; Russian Federal Agency of Atomic Energy; Russian Federal Agency for Science and Innovations; Russian Foundation for Basic Research; Ministry of Education of Slovakia; Department of Science and Technology, South Africa; CIEMAT; EELA; Ministerio de Economia y Competitividad (MINECO) of Spain; Xunta de Galicia (Conselleria de Educacion); CEADEN; Cubaenergia, Cuba; IAEA (International Atomic Energy Agency); Swedish Research Council (VR); Knut & Alice Wallenberg Foundation (KAW); Ukraine Ministry of Education and Science; United Kingdom Science and Technology Facilities Council (STFC); United States Department of Energy; United States National Science Foundation; State of Texas; State of Ohio FX The ALICE Collaboration would like to thank all its engineers and technicians for their invaluable contributions to the construction of the experiment and the CERN accelerator teams for the outstanding performance of the LHC complex. The ALICE Collaboration gratefully acknowledges the resources and support provided by all Grid centres and the Worldwide LHC Computing Grid (WLCG) Collaboration. The ALICE Collaboration acknowledges the following funding agencies for their support in building and running the ALICE detector: State Committee of Science, World Federation of Scientists (WFS) and Swiss Fonds Kidagan, Armenia, Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP); National Natural Science Foundation of China (NSFC), the Chinese Ministry of Education (CMOE) and the Ministry of Science and Technology of China (MSTC); Ministry of Education and Youth of the Czech Republic; Danish Natural Science Research Council, the Carlsberg Foundation and the Danish National Research Foundation; The European Research Council under the European Community's Seventh Framework Programme; Helsinki Institute of Physics and the Academy of Finland; French CNRS-IN2P3, the 'Region Pays de Loire', 'Region Alsace', 'Region Auvergne' and CEA, France; German BMBF and the Helmholtz Association; General Secretariat for Research and Technology, Ministry of Development, Greece; Hungarian OTKA and National Office for Research and Technology (NKTH); Department of Atomic Energy and Department of Science and Technology of the Government of India; Istituto Nazionale di Fisica Nucleare (INFN) and Centro Fermi - Museo Storico della Fisica e Centro Studi e Ricerche "Enrico Fermi", Italy; MEXT Grant-in-Aid for Specially Promoted Research, Japan; Joint Institute for Nuclear Research, Dubna; National Research Foundation of Korea (NRF); CONACYT, DGAPA, Mexico, ALFA-EC and the EPLANET Program (European Particle Physics Latin American Network) Stichting voor Fundamenteel Onderzoek der Materie (FOM) and the Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Netherlands; Research Council of Norway (NFR); Polish Ministry of Science and Higher Education; National Science Centre, Poland; Ministry of National Education/Institute for Atomic Physics and CNCS-UEFISCDI - Romania; Ministry of Education and Science of Russian Federation, Russian Academy of Sciences, Russian Federal Agency of Atomic Energy, Russian Federal Agency for Science and Innovations and The Russian Foundation for Basic Research; Ministry of Education of Slovakia; Department of Science and Technology, South Africa; CIEMAT, EELA, Ministerio de Economia y Competitividad (MINECO) of Spain, Xunta de Galicia (Conselleria de Educacion), CEADEN, Cubaenergia, Cuba, and IAEA (International Atomic Energy Agency); Swedish Research Council (VR) and Knut & Alice Wallenberg Foundation (KAW); Ukraine Ministry of Education and Science; United Kingdom Science and Technology Facilities Council (STFC); The United States Department of Energy, the United States National Science Foundation, the State of Texas, and the State of Ohio. NR 33 TC 18 Z9 18 U1 2 U2 53 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0370-2693 EI 1873-2445 J9 PHYS LETT B JI Phys. Lett. B PD NOV 10 PY 2014 VL 738 BP 97 EP 108 DI 10.1016/j.physletb.2014.09.026 PG 12 WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AT0KK UT WOS:000344624900013 ER PT J AU Dobrescu, BA Hill, CT AF Dobrescu, Bogdan A. Hill, Christopher T. TI Composite vectorlike fermions SO PHYSICS LETTERS B LA English DT Article ID ELECTROWEAK SYMMETRY-BREAKING; T-QUARK; DYNAMICAL MODEL; STANDARD MODEL; SUPERCONDUCTIVITY; CONDENSATION; MECHANISM; ANALOGY; SEARCH; MASSES AB We study a dynamical mechanism that generates a composite vectorlike fermion, formed by the binding of an N-tuplet of elementary chiral fermions to an N-tuplet of scalars. Deriving the properties of the composite fermion in the large N limit, we show that its mass is much smaller than the compositeness scale when the binding coupling is near a critical value. We compute the contact interactions involving four composite fermions, and find that their coefficients scale as 1/N. Physics beyond the Standard Model may include composite vectorlike fermions arising from this mechanism. (C) 2014 The Authors. Published by Elsevier B. V. C1 [Dobrescu, Bogdan A.; Hill, Christopher T.] Fermilab Natl Accelerator Lab, Dept Theoret Phys, Batavia, IL 60510 USA. RP Dobrescu, BA (reprint author), Fermilab Natl Accelerator Lab, Dept Theoret Phys, POB 500, Batavia, IL 60510 USA. FU U.S. Department of Energy [DE-AC02-07CH11359] FX We would like to thank Bill Bardeen for insightful conversations. Fermilab is operated by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the U.S. Department of Energy. NR 32 TC 1 Z9 1 U1 0 U2 1 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0370-2693 EI 1873-2445 J9 PHYS LETT B JI Phys. Lett. B PD NOV 10 PY 2014 VL 738 BP 150 EP 154 DI 10.1016/j.physletb.2014.09.030 PG 5 WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AT0KK UT WOS:000344624900023 ER PT J AU Allison, K Hill, CT Ross, GG AF Allison, Kyle Hill, Christopher T. Ross, Graham G. TI Ultra-weak sector, Higgs boson mass, and the dilaton SO PHYSICS LETTERS B LA English DT Article ID ELECTROWEAK SYMMETRY-BREAKING; DARK-MATTER; AXION AB The Higgs boson mass may arise from a portal coupling to a singlet field sigma which has a very large VEV f >> m(Higgs). This requires a sector of "ultra-weak" couplings zeta(i), where zeta(i) less than or similar to m(Higgs)(2)/f(2). Ultra-weak couplings are technically naturally small due to a custodial shift symmetry of sigma in the zeta(i) -> 0 limit. The singlet field sigma has properties similar to a pseudo-dilaton. We engineer explicit breaking of scale invariance in the ultra-weak sector via a Coleman-Weinberg potential, which requires hierarchies amongst the ultra-weak couplings. (C) 2014 The Authors. Published by Elsevier B.V. C1 [Allison, Kyle; Ross, Graham G.] Univ Oxford, Dept Theoret Phys, Oxford OX1 3NP, England. [Hill, Christopher T.] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA. RP Hill, CT (reprint author), Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA. EM hill@fnal.gov FU Fermi Research Alliance, LLC [DE-AC02-07CH11359]; United States Department of Energy FX For useful discussions, we thank W. Bardeen and Giovanni Villadoro. Fermilab is operated by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the United States Department of Energy. One of us (G. G. R.) would like to thank the Leverhulme foundation for an emeritus fellowship without which this research would not have been initiated. NR 43 TC 18 Z9 18 U1 0 U2 0 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0370-2693 EI 1873-2445 J9 PHYS LETT B JI Phys. Lett. B PD NOV 10 PY 2014 VL 738 BP 191 EP 195 DI 10.1016/j.physletb.2014.09.041 PG 5 WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AT0KK UT WOS:000344624900030 ER PT J AU Murayama, H Nakayama, K Takahashi, F Yanagida, TT AF Murayama, Hitoshi Nakayama, Kazunori Takahashi, Fuminobu Yanagida, Tsutomu T. TI Sneutrino chaotic inflation and landscape SO PHYSICS LETTERS B LA English DT Article ID GRAVITINO DARK-MATTER; SUPERSYMMETRY-BREAKING; GRAND UNIFICATION; SYMMETRY-BREAKING; HIGGS-BOSON; UNIVERSE; MASS; BARYOGENESIS; MODELS; LHC AB The most naive interpretation of the BICEP2 data is the chaotic inflation by an inflaton with a quadratic potential. When combined with supersymmetry, we argue that the inflaton plays the role of right-handed scalar neutrino based on rather general considerations. The framework suggests that the right-handed sneutrino tunneled from a false vacuum in a landscape to our vacuum with a small negative curvature and suppressed scalar perturbations at large scales. (C) 2014 The Authors. Published by Elsevier B.V. C1 [Murayama, Hitoshi] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA. [Murayama, Hitoshi] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Theoret Phys Grp, Berkeley, CA 94720 USA. [Murayama, Hitoshi; Nakayama, Kazunori; Takahashi, Fuminobu; Yanagida, Tsutomu T.] Univ Tokyo, Todai Inst Adv Study, Kavli Inst Phys & Math Univ WPI, Kashiwa, Chiba 2778583, Japan. [Nakayama, Kazunori] Univ Tokyo, Dept Phys, Tokyo 1130033, Japan. [Takahashi, Fuminobu] Tohoku Univ, Dept Phys, Sendai, Miyagi 9808578, Japan. RP Yanagida, TT (reprint author), Univ Tokyo, Todai Inst Adv Study, Kavli Inst Phys & Math Univ WPI, Kashiwa, Chiba 2778583, Japan. EM hitoshi@berkeley.edu; kazunori@hep-th.phys.s.u-tokyo.ac.jp; fumi@tuhep.phys.tohoku.ac.jp; tsutomu.tyanagida@ipmu.jp FU U.S. DOE [DE-AC02-05CH11231]; NSF [PHY-1002399, PHY-1316783]; Inoue Foundation for Science; World Premier International Research Center Initiative (WPI Program), MEXT, Japan; [26400241]; [26800121]; [24740135]; [23104008]; [26287039] FX This work was supported by the U.S. DOE under Contract DE-AC02-05CH11231 [H.M.], by the NSF under grants PHY-1002399 and PHY-1316783 [H.M.], by the Grant-in-Aid for Scientific Research (C) (No. 26400241 [H.M.]), Young Scientists (B) (No. 26800121 [K.N.], No. 24740135 [F.T.]), Scientific Research on Innovative Areas (No. 23104008 [F.T.]), and Scientific Research (B) (No. 26287039 [F.T. and T.T.Y.]), by Inoue Foundation for Science [F.T.], and by World Premier International Research Center Initiative (WPI Program), MEXT, Japan. NR 74 TC 12 Z9 12 U1 0 U2 4 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0370-2693 EI 1873-2445 J9 PHYS LETT B JI Phys. Lett. B PD NOV 10 PY 2014 VL 738 BP 196 EP 200 DI 10.1016/j.physletb.2014.09.045 PG 5 WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AT0KK UT WOS:000344624900031 ER PT J AU Taprogge, J Jungclaus, A Grawe, H Nishimura, S Xu, ZY Doornenbal, P Lorusso, G Nacher, E Simpson, GS Soderstrom, PA Sumikama, T Baba, H Browne, F Fukuda, N Gernhauser, R Gey, G Inabe, N Isobe, T Jung, HS Kameda, D Kim, GD Kim, YK Kojouharov, I Kubo, T Kurz, N Kwon, YK Lin, Z Sakurai, H Schaffner, H Steiger, K Suzuki, H Takeda, H Vajta, Z Watanabe, H Wu, J Yagi, A Yoshinaga, K Benzoni, G Bonig, S Chae, KY Coraggio, L Covello, A Daugas, JM Drouet, F Gadea, A Gargano, A Ilieva, S Kondev, FG Kroll, T Lane, GJ Montaner-Piza, A Moschner, K Mucher, D Naqvi, F Niikura, M Nishibata, H Odahara, A Orlandi, R Patel, Z Podolyak, Z Wendt, A AF Taprogge, J. Jungclaus, A. Grawe, H. Nishimura, S. Xu, Z. Y. Doornenbal, P. Lorusso, G. Nacher, E. Simpson, G. S. Soederstroem, P. -A. Sumikama, T. Baba, H. Browne, F. Fukuda, N. Gernhauser, R. Gey, G. Inabe, N. Isobe, T. Jung, H. S. Kameda, D. Kim, G. D. Kim, Y. -K. Kojouharov, I. Kubo, T. Kurz, N. Kwon, Y. K. Lin, Z. Sakurai, H. Schaffner, H. Steiger, K. Suzuki, H. Takeda, H. Vajta, Zs. Watanabe, H. Wu, J. Yagi, A. Yoshinaga, K. Benzoni, G. Boenig, S. Chae, K. Y. Coraggio, L. Covello, A. Daugas, J. -M. Drouet, F. Gadea, A. Gargano, A. Ilieva, S. Kondev, F. G. Kroell, T. Lane, G. J. Montaner-Piza, A. Moschner, K. Muecher, D. Naqvi, F. Niikura, M. Nishibata, H. Odahara, A. Orlandi, R. Patel, Z. Podolyak, Zs. Wendt, A. TI Identification of a millisecond isomeric state in Cd-129(81) via the detection of internal conversion and Compton electrons SO PHYSICS LETTERS B LA English DT Article DE Isomeric decays; Transition strengths; Shell model calculations ID BETA-DECAY; EURICA; RIKEN AB The decay of an isomeric state in the neutron-rich nucleus Cd-129 has been observed via the detection of internal conversion and Compton electrons providing first experimental information on excited states in this nucleus. The isomer was populated in the projectile fission of a U-238 beam at the Radioactive Isotope Beam Factory at RIKEN. From the measured yields of gamma-rays and internal conversion electrons, a multipolarity of E3 was tentatively assigned to the isomeric transition. A half-life of T-1/2 = 3.6(2) ms was determined for the new state which was assigned a spin of (21/2(+)), based on a comparison to shell model calculations performed using state-of-the-art realistic effective interactions. (C) 2014 The Authors. Published by Elsevier B.V. C1 [Taprogge, J.; Jungclaus, A.] CSIC, Inst Estruct Mat, Madrid 28006, Spain. [Taprogge, J.] Univ Autonoma Madrid, Dept Fis Teor, E-28049 Madrid, Spain. [Taprogge, J.; Nishimura, S.; Xu, Z. Y.; Doornenbal, P.; Lorusso, G.; Soederstroem, P. -A.; Baba, H.; Browne, F.; Fukuda, N.; Gey, G.; Inabe, N.; Isobe, T.; Kameda, D.; Kubo, T.; Sakurai, H.; Suzuki, H.; Takeda, H.; Vajta, Zs.; Watanabe, H.; Wu, J.] RIKEN, Nishina Ctr, Wako, Saitama 3510198, Japan. [Grawe, H.] GSI Helmholtzzentrum Schwerionenforschung GmBH, D-64291 Darmstadt, Germany. [Simpson, G. S.; Gey, G.] Univ Joseph Fourier Grenoble 1, ELPSC, Inst Natl Polytech Grenoble, CNRS IN2P3, F-38026 Grenoble, France. [Sumikama, T.] Tohoku Univ, Dept Phys, Sendai, Miyagi 9808578, Japan. [Sakurai, H.] Univ Tokyo, Dept Phys, Bunkyo Ku, Tokyo 1130033, Japan. [Browne, F.] Univ Brighton, Sch Comp Engn & Math, Brighton BN2 4JG, E Sussex, England. [Gernhauser, R.; Steiger, K.] Tech Univ Munich, Phys Dept E12, D-85748 Garching, Germany. [Gey, G.] Inst Laue Langevin, F-38042 Grenoble 9, France. [Jung, H. S.] Chung Ang Univ, Dept Phys, Seoul 156756, South Korea. [Kim, G. D.; Kwon, Y. K.] Inst for Basic Sci Korea, Rare Isotope Sci Project, Taejon 305811, South Korea. [Kim, Y. -K.] Hanyang Univ, Dept Nucl Engn, Seoul 133791, South Korea. [Lin, Z.; Wu, J.] Peking Univ, Sch Phys, Beijing 100871, Peoples R China. [Lin, Z.; Wu, J.] Peking Univ, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China. [Vajta, Zs.] MTA Atomki, H-4001 Debrecen, Hungary. [Yagi, A.] Osaka Univ, Dept Phys, Osaka, Toyonaka 5600043, Japan. [Yoshinaga, K.] Tokyo Univ Sci, Fac Sci & Technol, Dept Phys, Noda, Chiba 278, Japan. [Benzoni, G.] INFN, Sez Milano, I-20133 Milan, Italy. [Boenig, S.; Ilieva, S.; Kroell, T.; Muecher, D.] Tech Univ Darmstadt, Inst Kernphys, D-64289 Darmstadt, Germany. [Chae, K. Y.] Sungkyunkwan Univ, Dept Phys, Suwon 440746, South Korea. [Coraggio, L.] Complesso Univ Monte S Angelo, Ist Nazl Fis Nucleare, I-80126 Naples, Italy. [Covello, A.] Complesso Univ Monte S Angelo, Univ Naples Federico II, Dipartimento Fis, I-80126 Naples, Italy. [Daugas, J. -M.] CEA, DAM, DIF, F-91297 Arpajon, France. [Gadea, A.; Montaner-Piza, A.] Univ Valencia, CSIC, Inst Fis Corpuscular, E-46980 Paterna, Spain. [Kondev, F. G.] Argonne Natl Lab, Nucl Engn Div, Argonne, IL 60439 USA. [Lane, G. J.] Australian Natl Univ, Res Sch Phys Sci & Engn, Dept Nucl Phys, Canberra, ACT 0200, Australia. [Moschner, K.; Wendt, A.] Univ Cologne, IKP, D-50937 Cologne, Germany. [Naqvi, F.] Yale Univ, Wright Nucl Struct Lab, New Haven, CT 06520 USA. [Orlandi, R.] Katholieke Univ Leuven, Inst Kern Stralingsfys, B-3001 Heverlee, Belgium. [Orlandi, R.] Japan Atom Energy Agcy, Adv Sci Res Ctr, Tokai, Ibaraki 3191195, Japan. [Patel, Z.; Podolyak, Zs.] Univ Surrey, Dept Phys, Guildford GU2 7XH, Surrey, England. RP Jungclaus, A (reprint author), CSIC, Inst Estruct Mat, Madrid 28006, Spain. EM andrea.jungclaus@csic.es RI Lane, Gregory/A-7570-2011; SAKURAI, HIROYOSHI/G-5085-2014; Gadea, Andres/L-8529-2014; Coraggio, Luigi/P-4857-2015 OI Lane, Gregory/0000-0003-2244-182X; Gadea, Andres/0000-0002-4233-1970; Coraggio, Luigi/0000-0002-4327-9107 FU Spanish Ministerio de Ciencia e Innovacion [FPA2009-13377-C02, FPA2011-29854-C04]; Generalitat Valenciana (Spain) [PROMETEO/2010/101]; Japanese government under contract KAKENHI [25247045]; National Research Foundation of Korea (NRF) - Korea government (MEST) [NRF-2012R1A1A1041763]; Priority Centers Research Program in Korea [2009-0093817]; OTKA [K-100835]; European Commission [300096]; U.S. Department of Energy, Office of Nuclear Physics [DE-AC02-06CH11357]; STFC (UK); German BMBF [05P12RDCIA, 05P12RDNUP]; HIC for FAIR FX This experiment was performed at RI Beam Factory operated by RIKEN Nishina Center and CNS, University of Tokyo. We thank the staff of the accelerator complex for providing stable beams with high intensities to the experiment. We acknowledge the EUROBALL Owners Committee for the loan of germanium detectors and the PreSpec Collaboration for the readout electronics of the cluster detectors. This work was supported by the Spanish Ministerio de Ciencia e Innovacion under contracts FPA2009-13377-C02 and FPA2011-29854-C04, the Generalitat Valenciana (Spain) under grant PROMETEO/2010/101, the Japanese government under contract KAKENHI (25247045), the National Research Foundation of Korea (NRF) grant funded by the Korea government (MEST) (No. NRF-2012R1A1A1041763), the Priority Centers Research Program in Korea (2009-0093817), OTKA contract number K-100835, the European Commission through the Marie Curie Actions call FP7-PEOPLE-2011-IEF under Contract No. 300096, the U.S. Department of Energy, Office of Nuclear Physics, under Contract No. DE-AC02-06CH11357, STFC (UK), and the German BMBF (Nos. 05P12RDCIA and 05P12RDNUP) and HIC for FAIR. NR 27 TC 5 Z9 5 U1 3 U2 24 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0370-2693 EI 1873-2445 J9 PHYS LETT B JI Phys. Lett. B PD NOV 10 PY 2014 VL 738 BP 223 EP 227 DI 10.1016/j.physletb.2014.09.047 PG 5 WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AT0KK UT WOS:000344624900036 ER PT J AU Aad, G Abbott, B Abdallah, J Khalek, SA Abdinov, O Aben, R Abi, B Abolins, M AbouZeid, OS Abramowicz, H Abreu, H Abreu, R Abulaiti, Y Acharya, BS Adamczyk, L Adams, DL Adelman, J Adomeit, S Adye, T Agatonovic-Jovin, T Aguilar-Saavedra, JA Agustoni, M Ahlen, SP Ahmadov, F Aielli, G Akerstedt, H Aring;kesson, TPA Akimoto, G Akimov, AV Alberghi, GL Albert, J Albrand, S Verzini, MJA Aleksa, M Aleksandrov, IN Alexa, C Alexander, G Alexandre, G Alexopoulos, T Alhroob, M Alimonti, G Alio, L Alison, J Allbrooke, BMM Allison, LJ Allport, PP Aloisio, A Alonso, A Alonso, F Alpigiani, C Altheimer, A Gonzalez, BA Alviggi, MG Amako, K Coutinho, YA Amelung, C Amidei, D Dos Santos, SPA Amorim, A Amoroso, S Amram, N Amundsen, G Anastopoulos, C Ancu, LS Andari, N Andeen, T 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CA ATLAS Collaboration TI Fiducial and differential cross sections of Higgs boson production measured in the four-lepton decay channel in pp collisions at root s=8 TeV with the ATLAS detector SO PHYSICS LETTERS B LA English DT Article ID HADRON COLLIDERS; QCD CORRECTIONS; MASSLESS PARTICLES; BROKEN SYMMETRIES; NNLO QCD; LHC AB Measurements of fiducial and differential cross sections of Higgs boson production in the H -> ZZ* -> 4l decay channel are presented. The cross sections are determined within a fiducial phase space and corrected for detection efficiency and resolution effects. They are based on 20.3 fb(-1) of pp collision data, produced at root s= 8 TeV centre-of-mass energy at the LHC and recorded by the ATLAS detector. The differential measurements are performed in bins of transverse momentum and rapidity of the four-lepton system, the invariant mass of the subleading lepton pair and the decay angle of the leading lepton pair with respect to the beam line in the four-lepton rest frame, as well as the number of jets and the transverse momentum of the leading jet. The measured cross sections are compared to selected theoretical calculations of the Standard Model expectations. No significant deviation from any of the tested predictions is found. Published by Elsevier B.V. C1 [Jackson, P.; Lee, L.; Soni, N.; White, M. J.] Univ Adelaide, Dept Phys, Adelaide, SA, Australia. [Bouffard, J.; Edson, W.; Ernst, J.; Fischer, A.; Guindon, S.; Jain, V.] SUNY Albany, Dept Phys, Albany, NY 12222 USA. [Butt, A. I.; Czodrowski, P.; Gingrich, D. M.; Moore, R. W.; Pinfold, J. L.; Saddique, A.; Vaque, F. Vives] Univ Alberta, Dept Phys, Edmonton, AB, Canada. [Cakir, I. 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[Angelidakis, S.; Antonaki, A.; Chouridou, S.; Fassouliotis, D.; Giokaris, N.; Ioannou, P.; Iordanidou, K.; Kourkoumelis, C.; Manousakis-Katsikakis, A.; Tsirintanis, N.] Univ Athens, Dept Phys, Athens, Greece. [Alexopoulos, T.; Byszewski, M.; Dris, M.; Gazis, E. N.; Iakovidis, G.; Karakostas, K.; Karastathis, N.; Leontsinis, S.; Maltezos, S.; Ntekas, K.; Panagiotopoulou, E.; Papadopoulou, Th. D.; Tsipolitis, G.; Vlachos, S.] Natl Tech Univ Athens, Dept Phys, Zografos, Greece. [Abdinov, O.; Khalil-zada, F.] Azerbaijan Acad Sci, Inst Phys, Baku 370143, Azerbaijan. [Anjos, N.; Bosman, M.; Armadans, R. Caminal; Casado, M. P.; Casolino, M.; Cavalli-Sforza, M.; Conidi, M. C.; Cortes-Gonzalez, A.; Farooque, T.; Flowerdew, M. J.; Giangiobbe, V.; Parra, G. Gonzalez; Korolkov, I.; Le Menedeu, E.; Paz, I. Lopez; Mir, L. M.; Berlingen, J. Montejo; Pages, A. Pacheco; Aranda, C. Padilla; Bueso, X. Portell; Riu, I.; Rubbo, F.; Sorin, V.; Succurro, A.; Tripiana, M. F.; Tsiskaridze, S.] Univ Autonoma Barcelona, Inst Fis Altes Energies, E-08193 Barcelona, Spain. [Anjos, N.; Bosman, M.; Armadans, R. Caminal; Casado, M. P.; Casolino, M.; Cavalli-Sforza, M.; Conidi, M. C.; Cortes-Gonzalez, A.; Farooque, T.; Flowerdew, M. J.; Giangiobbe, V.; Parra, G. Gonzalez; Korolkov, I.; Le Menedeu, E.; Paz, I. Lopez; Mir, L. M.; Berlingen, J. Montejo; Pages, A. Pacheco; Aranda, C. Padilla; Bueso, X. Portell; Riu, I.; Rubbo, F.; Sorin, V.; Succurro, A.; Tripiana, M. F.; Tsiskaridze, S.] Univ Autonoma Barcelona, Dept Fis, E-08193 Barcelona, Spain. [Agatonovic-Jovin, T.; Bozic, I.; Dimitrievska, A.; Marjanovic, M.; Popovic, D. S.; Sijacki, Dj.; Simic, Lj.; Milosavljevic, M. Vranjes] Univ Belgrade, Inst Phys, Belgrade, Serbia. [Cirkovic, P.; Mamuzic, J.] Univ Belgrade, Vinca Inst Nucl Sci, Belgrade, Serbia. [Buanes, T.; Dale, O.; Eigen, G.; Kastanas, A.; Liebig, W.; Lipniacka, A.; Latour, B. Martin Dit; Rosendahl, P. L.; Sandaker, H.; Sjursen, T. B.; Smestad, L.; Stugu, B.; Ugland, M.] Univ Bergen, Dept Phys & Technol, Bergen, Norway. [Barnett, R. M.; Beringer, J.; Biesiada, J.; Brandt, G.; Brosamer, J.; Calafiura, P.; Caminada, L. M.; Cerutti, F.; Ciocio, A.; Clarke, R. N.; Cooke, M.; Copic, K.; Dube, S.; Einsweiler, K.; Farrell, S.; Garcia-Sciveres, M.; Gilchriese, M.; Haber, C.; Hance, M.; Heinemann, B.; Hinchliffe, I.; Hurwitz, M.; Jeanty, L.; Lavrijsen, W.; Leggett, C.; Loscutoff, P.; Marshall, Z.; Ohm, C. C.; Ovcharova, A.; Griso, S. Pagan; Potamianos, K.; Pranko, A.; Quarrie, D. R.; Shapiro, M.; Sood, A.; Tibbetts, M. J.; Trottier-McDonald, M.; Tsulaia, V.; Virzi, J.; Wang, H.; Yao, W-M.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Phys, Berkeley, CA 94720 USA. [Barnett, R. M.; Beringer, J.; Biesiada, J.; Brandt, G.; Brosamer, J.; Calafiura, P.; Caminada, L. M.; Cerutti, F.; Ciocio, A.; Clarke, R. N.; Cooke, M.; Copic, K.; Dube, S.; Einsweiler, K.; Farrell, S.; Garcia-Sciveres, M.; Gilchriese, M.; Haber, C.; Hance, M.; Heinemann, B.; Hinchliffe, I.; Hurwitz, M.; Jeanty, L.; Lavrijsen, W.; Leggett, C.; Loscutoff, P.; Marshall, Z.; Ohm, C. C.; Ovcharova, A.; Griso, S. Pagan; Potamianos, K.; Pranko, A.; Quarrie, D. R.; Shapiro, M.; Sood, A.; Tibbetts, M. J.; Trottier-McDonald, M.; Tsulaia, V.; Virzi, J.; Wang, H.; Yao, W-M.] Univ Calif Berkeley, Berkeley, CA 94720 USA. [Giorgi, F. M.; Grancagnolo, S.; Herbert, G. H.; Herrberg-Schubert, R.; Hristova, I.; Kind, O.; Kolanoski, H.; Lacker, H.; Lohse, T.; Nikiforov, A.; Rehnisch, L.; Rieck, P.; Schulz, H.; Stamm, S.; Wendland, D.; Nedden, M. zur] Humboldt Univ, Dept Phys, Berlin, Germany. [Agustoni, M.; Beck, H. P.; Cervelli, A.; Ereditato, A.; Gallo, V.; Haug, S.; Kruker, T.; Marti, L. F.; Meloni, F.; Schneider, B.; Sciacca, F. G.; Stramaglia, M. E.; Stucci, S. A.; Weber, M. S.] Univ Bern, Albert Einstein Ctr Fundamental Phys, Bern, Switzerland. [Agustoni, M.; Beck, H. P.; Cervelli, A.; Ereditato, A.; Gallo, V.; Haug, S.; Kruker, T.; Marti, L. F.; Meloni, F.; Schneider, B.; Sciacca, F. G.; Stramaglia, M. E.; Stucci, S. A.; Weber, M. S.] Univ Bern, High Energy Phys Lab, Bern, Switzerland. [Arik, M.; Istin, S.; Ozcan, V. E.] Bogazici Univ, Dept Phys, Istanbul, Turkey. [Istin, S.] Dogus Univ, Dept Phys, Istanbul, Turkey. [Beddall, A. J.; Beddall, A.; Bingul, A.] Gaziantep Univ, Dept Engn Phys, Gaziantep, Turkey. [Alberghi, G. L.; Bellagamba, L.; Boscherini, D.; Bruni, A.; Bruni, G.; Bruschi, M.; Caforio, D.; Corradi, M.; De Castro, S.; Di Sipio, R.; Fabbri, L.; Forti, A.; Gabrielli, A.; Giacobbe, B.; Giorgi, F. M.; Grafstroem, P.; Manghi, F. Lasagni; Massa, I.; Massa, L.; Mengarelli, A.; Negrini, M.; Piccinini, M.; Polini, A.; Rinaldi, L.; Romano, M.; Sbarra, C.; Sbrizzi, A.; Semprini-Cesari, N.; Spighi, R.; Tupputi, S. A.; Valentinetti, S.; Villa, M.; Zoccoli, A.] Ist Nazl Fis Nucl, Sez Bol, I-40126 Bologna, Italy. [Alberghi, G. L.; Caforio, D.; De Castro, S.; Di Sipio, R.; Fabbri, L.; Forti, A.; Gabrielli, A.; Grafstroem, P.; Manghi, F. Lasagni; Massa, I.; Massa, L.; Mengarelli, A.; Piccinini, M.; Romano, M.; Sbrizzi, A.; Semprini-Cesari, N.; Tupputi, S. A.; Valentinetti, S.; Villa, M.; Zoccoli, A.] Univ Bologna, Dipartimento Fis & Astron, Bologna, Italy. [Arslan, O.; Bechtle, P.; Brock, I.; Cristinziani, M.; Davey, W.; Desch, K.; Dingfelder, J.; Ehrenfeld, W.; Gaycken, G.; Geich-Gimbel, Ch.; Gonella, L.; Haefner, P.; Hageboeck, S.; Hellmich, D.; Hillert, S.; Huegging, F.; Janssen, J.; Khoriauli, G.; Koevesarki, P.; Kostyukhin, V. V.; Kraus, J. K.; Kroseberg, J.; Krueger, H.; Lapoire, C.; Lehmacher, M.; Lenz, T.; Leyko, A. M.; Liebal, J.; Limbach, C.; Loddenkoetter, T.; Mergelmeyer, S.; Mijovic, L.; Mueller, K.; Nanava, G.; Nattermann, T.; Obermann, T.; Pohl, D.; Sarrazin, B.; Schaepe, S.; Schultens, M. J.; Schwindt, T.; Scutti, F.; Stillings, J. A.; Tannoury, N.; Therhaag, J.; Uchida, K.; Uhlenbrock, M.; Vogel, A.; von Toerne, E.; Wagner, P.; Wang, T.; Wermes, N.; Wienemann, P.; Wiik-Fuchs, L. A. M.; Winter, B. T.; Wong, K. H. Yau; Zimmermann, R.; Zimmermann, S.] Univ Bonn, Inst Phys, Bonn, Germany. [Ahlen, S. P.; Bernard, C.; Black, K. M.; Butler, J. M.; Dell'Asta, L.; Helary, L.; Kruskal, M.; Long, B. A.; Shank, T.; Yan, Z.] Boston Univ, Dept Phys, Boston, MA 02215 USA. [Amelung, C.; Amundsen, G.; Artoni, G.; Bensinger, J. R.; Bianchini, L.; Blocker, C.; Coffey, L.; Gozpinar, S.; Sciolla, G.; Venturini, A.; Zengel, K.] Brandeis Univ, Dept Phys, Waltham, MA 02254 USA. [Coutinho, Y. Amaral; Caloba, L. P.; Graber, L.; Maidantchik, C.; Marroquim, F.; Nepomuceno, A. A.; Seixas, J. M.] Univ Fed Rio de Janeiro, COPPE EE IF, Rio De Janeiro, Brazil. [Cerqueira, A. S.; de Andrade Filho, L. Manhaes] Fed Univ Juiz de Fora UFJF, Juiz De Fora, Brazil. [do Vale, M. A. B.] Fed Univ Sao Joao del Rei UFSJ, Sao Joao Del Rei, Brazil. [Donadelli, M.; Leite, M. A. L.] Univ Sao Paulo, Inst Fis, BR-01498 Sao Paulo, Brazil. [Adams, D. L.; Assamagan, K.; Begel, M.; Chen, H.; Chernyatin, V.; Debbe, R.; Ernst, M.; Gibbard, B.; Gordon, H. A.; Klimentov, A.; Kravchenko, A.; Lanni, F.; Lissauer, D.; Lynn, D.; Ma, H.; Maeno, T.; Metcalfe, J.; Mountricha, E.; Nevski, P.; Okawa, H.; Damazio, D. Oliveira; Paige, F.; Panitkin, S.; Perepelitsa, D. V.; Pleier, M. -A.; Polychronakos, V.; Protopopescu, S.; Purohit, M.; Radeka, V.; Rajagopalan, S.; Redlinger, G.; Schovancova, J.; Snyder, S.; Steinberg, P.; Takai, H.; Undrus, A.; Wenaus, T.; Ye, S.] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. [Alexa, C.; Boldea, V.; Buda, S. I.; Caprini, I.; Caprini, M.; Chitan, A.; Ciubancan, M.; Constantinescu, S.; Cuciuc, C. -M.; Dita, P.; Dita, S.; Ducua, O. A.; Jinaru, A.; Maurer, J.; Olariu, A.; Pantea, D.; Rotaru, M.; Stoicea, G.; Tudorache, A.; Tudorache, V.] Natl Inst Phys & Nucl Engn, Bucharest, Romania. [Popeneciu, G. A.] Natl Inst Res & Dev Isotop & Mol Technol, Dept Phys, Cluj Napoca, Romania. Univ Politeh Bucharest, Bucharest, Romania. West Univ Timisoara, Timisoara, Romania. [Garzon, G. Otero y; Piegaia, R.; Reisin, H.; Sacerdoti, S.] Univ Buenos Aires, Dept Fis, Buenos Aires, DF, Argentina. [Arratia, M.; Barlow, N.; Batley, J. R.; Brochu, F. M.; Buttinger, W.; Carter, J. R.; Chapman, J. D.; Cottin, G.; Franchino, S.; French, S. T.; Frost, J. A.; Gillam, T. P. S.; Hill, J. C.; Kaneti, S.; Khoo, T. J.; Lester, C. G.; Mueller, T.; Parker, M. A.; Robinson, D.; Sandoval, T.; Thomson, M.; Ward, C. P.; Williams, S.] Univ Cambridge, Cavendish Lab, Cambridge CB3 0HE, England. [Bellerive, A.; Cree, G.; Di Valentino, D.; Koffas, T.; Lacey, J.; Leight, W. A.; Marchand, J. F.; McCarthy, T. G.; Nomidis, I.; Pasztor, G.; Tarrade, F.; Ueno, R.; Vincter, M. G.; Whalen, K.] Carleton Univ, Dept Phys, Ottawa, ON K1S 5B6, Canada. [Abreu, R.; Aleksa, M.; Andari, N.; Anders, G.; Anghinolfi, F.; Armbruster, A. J.; Arnaez, O.; Avolio, G.; Baak, M. A.; Backes, M.; Mayes, J. Backus; Battistin, M.; Beltramello, O.; Bianco, M.; Bogaerts, J. A.; Boyd, J.; Burckhart, H.; Campana, S.; Garrido, M. D. M. Capeans; Carli, T.; Catinaccio, A.; Cattai, A.; Cerv, M.; Chromek-Burckhart, D.; Dell'Acqua, A.; Di Girolamo, A.; Di Girolamo, B.; Dittus, F.; Dobos, D.; Dudarev, A.; Duhrssen, M.; Ellis, N.; Elsing, M.; Farthouat, P.; Fassnacht, P.; Feigl, S.; Perez, S. Fernandez; Fortin, D.; Fournier, D.; Franklin, M.; Froidevaux, D.; Garonne, V.; Gianotti, F.; Gillberg, D.; Glatzer, J.; Godlewski, J.; Goossens, L.; Gorini, B.; Gray, H. M.; Hauschild, M.; Hawkings, R. J.; Heller, M.; Helsens, C.; Correia, A. M. Henriques; Hervas, L.; Hoecker, A.; Hubacek, Z.; Huhtinen, M.; Jaekel, M. R.; Jakobsen, S.; Jansen, H.; Jungst, R. M.; Kaneda, M.; Klioutchnikova, T.; Krasznahorkay, A.; Lantzsch, K.; Lassnig, M.; Miotto, G. Lehmann; Lenzi, B.; Lichard, P.; Macina, D.; Malyukov, S.; Mandelli, B.; Mapelli, L.; Martin, B.; Marzin, A.; Messina, A.; Meyer, J.; Milic, A.; Mornacchi, G.; Nairz, A. M.; Nakahama, Y.; Negri, G.; Nicquevert, B.; Nordberg, M.; Palestini, S.; Pauly, T.; Pernegger, H.; Peters, K.; Petersen, B. A.; Pommes, K.; Poppleton, A.; Poulard, G.; Prasad, S.; Rammensee, M.; Raymond, M.; Rembser, C.; Rodrigues, L.; Roe, S.; Ruiz-Martinez, A.; Salzburger, A.; Savu, D. O.; Schaefer, D.; Schlenker, S.; Schmieden, K.; Serfon, C.; Sfyrla, A.; Solans, C. A.; Spigo, G.; Stelzer, H. J.; Teischinger, F. A.; Ten Kate, H.; Tremblet, L.; Tricoli, A.; Tsarouchas, C.; Unal, G.; van der Ster, D.; van Eldik, N.; van Woerden, M. C.; Vandelli, W.; Vigne, R.; Voss, R.; Vuillermet, R.; Wells, P. S.; Wengler, T.; Wenig, S.; Werner, P.; Wilkens, H. G.; Wotschack, J.; Young, J. S.; Zwalinski, L.] CERN, Geneva, Switzerland. [Alison, J.; Anderson, K. J.; Boveia, A.; Cheng, Y.; Facini, G.; Fiascaris, M.; Gardner, R. W.; Kapliy, A.; Li, H. L.; Meehan, S.; Melachrinos, C.; Merritt, F. S.; Miller, D. W.; Okumura, Y.; Oreglia, M. J.; Penning, B.; Phillips, P. W.; Pilcher, J. E.; Shochet, M. J.; Tompkins, L.; Vukotic, I.; Webster, J. S.] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA. [Carquin, E.; Diaz, M. A.; Vogel, M.] Pontificia Univ Catolica Chile, Dept Fis, Santiago, Chile. [Brooks, W. K.; Kuleshov, S.; Pezoa, R.; Prokoshin, F.; White, R.] Univ Tecn Federico Santa Maria, Valparaiso, Chile. [Bai, Y.; Fang, Y.; Jin, S.; Lu, F.; Ouyang, Q.; Ren, H.; Shan, L. Y.; Sun, X.; Wang, J.; Xu, D.; Yao, L.; Zhu, H.; Zhuang, X.] Chinese Acad Sci, Inst High Energy Phys, Beijing, Peoples R China. [Gao, J.; Guan, L.; Han, L.; Li, B.; Liu, J. B.; Liu, K.; Liu, M.; Peng, H.; Song, H. Y.; Xu, L.] Shanghai Jiao Tong Univ, Dept Modern Phys, Shanghai 200030, Anhui, Peoples R China. [Chen, S.; Li, Y.] Nanjing Univ, Dept Phys, Nanjing, Jiangsu, Peoples R China. [Chen, L.; Feng, C.; Ge, P.; Ma, L. L.; Peng, H.; Zhang, X.; Zhu, C. G.] Shandong Univ, Sch Phys, Jinan, Shandong, Peoples R China. [Li, L.; Yang, H.] Shanghai Jiao Tong Univ, Dept Phys, Shanghai 200030, Peoples R China. [Chen, X.] Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China. [Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Dubreuil, E.; Ghodbane, N.; Gilles, G.; Gris, Ph.; Guicheney, C.; Liao, H.; Pallin, D.; Podlyski, F.; Santoni, C.; Theveneaux-Pelzer, T.; Valery, L.; Vazeille, F.] Clermont Univ, Lab Phys Corpusculaire, Clermont Ferrand, France. [Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Dubreuil, E.; Ghodbane, N.; Gilles, G.; Gris, Ph.; Guicheney, C.; Liao, H.; Pallin, D.; Podlyski, F.; Santoni, C.; Theveneaux-Pelzer, T.; Valery, L.; Vazeille, F.] Univ Clermont Ferrand, Clermont Ferrand, France. [Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Dubreuil, E.; Ghodbane, N.; Gilles, G.; Gris, Ph.; Guicheney, C.; Liao, H.; Pallin, D.; Podlyski, F.; Santoni, C.; Theveneaux-Pelzer, T.; Valery, L.; Vazeille, F.] CNRS IN2P3, Clermont Ferrand, France. [Altheimer, A.; Andeen, T.; Angerami, A.; Bain, T.; Brooijmans, G.; Chen, Y.; Cole, B.; Guo, J.; Hu, D.; Hughes, E. W.; Mohapatra, S.; Nikiforou, N.; Parsons, J. A.; Reale, V. Perez; Scherzer, M. I.; Thompson, E. N.; Tian, F.; Tuts, P. M.; Urbaniec, D.; Wulf, E.; Zhou, L.] Columbia Univ, Nevis Lab, Irvington, NY USA. [Boyko, I. R.; Dam, M.; Galster, G.; Hansen, J. B.; Hansen, J. D.; Hansen, P. H.; Joergensen, M. D.; Loevschall-Jensen, A. E.; Monk, J.; Pedersen, L. E.; Petersen, T. C.; Pingel, A.; Simonyan, M.; Thomsen, L. A.; Wiglesworth, C.; Xella, S.] Univ Copenhagen, Niels Bohr Inst, Copenhagen, Denmark. [Capua, M.; Chen, Y.; Crosetti, G.; La Rotonda, L.; Mastroberardino, A.; Policicchio, A.; Salvatore, D.; Scarfone, V.; Schioppa, M.; Susinno, G.; Tassi, E.] Ist Nazl Fis Nucl, Grp Collegato Cosenza, Lab Nazl Frascati, Naples, Italy. [Capua, M.; Chen, Y.; Crosetti, G.; La Rotonda, L.; Mastroberardino, A.; Policicchio, A.; Salvatore, D.; Scarfone, V.; Schioppa, M.; Susinno, G.; Tassi, E.] Univ Calabria, Dipartmento Fis, I-87036 Arcavacata Di Rende, Italy. [Adamczyk, L.; Bold, T.; Dabrowski, W.; Dwuznik, M.; Dyndal, M.; Grabowska-Bolda, I.; Kisielewska, D.; Koperny, S.; Kowalski, T. Z.; Mindur, B.; Przybycien, M.; Zemla, A.] AGH Univ Sci & Technol, Fac Phys & Appl Comp Sci, Krakow, Poland. [Palka, M.] Jagiellonian Univ, Marian Smoluchowski Inst Phys, Krakow, Poland. [Banas, E.; de Renstrom, P. A. Bruckman; Chwastowski, J. J.; Derendarz, D.; Gornicki, E.; Hajduk, Z.; Iwanski, W.; Kaczmarska, A.; Korcyl, K.; Malecki, Pa.; Olszewski, A.; Olszowska, J.; Stanecka, E.; Staszewski, R.; Trzebinski, M.; Trzupek, A.; Wolter, M. W.; Wosiek, B. K.; Wozniak, K. W.; Zabinski, B.] Polish Acad Sci, Henryk Niewodniczanski Inst Nucl Phys, Krakow, Poland. [Cao, T.; Firan, A.; Hoffman, J.; Kama, S.; Kehoe, R.; Randle-Conde, A. S.; Sekula, S. J.; Stroynowski, R.; Turvey, A. J.; Wang, H.; Ye, J.] So Methodist Univ, Dept Phys, Dallas, TX 75275 USA. [Izen, J. M.; Leyton, M.; Lou, X.; Namasivayam, H.; Reeves, K.] Univ Texas Dallas, Dept Phys, Richardson, TX 75083 USA. [Argyropoulos, S.; Asbah, N.; Bessner, M.; Bloch, I.; Borroni, S.; Camarda, S.; Dassoulas, J. A.; Deterre, C.; Dietrich, J.; Filipuzzi, M.; Francis, D.; Friedrich, C.; Glazov, A.; Fajardo, L. S. Gomez; Grahn, K-J.; Gregor, I. M.; Grohsjean, A.; Haleem, M.; Hamnett, P. G.; Hengler, C.; Hiller, K. H.; Howarth, J.; Huang, Y.; Belenguer, M. Jimenez; Katzy, J.; Keller, J. S.; Kondrashova, N.; Kuhl, T.; Lisovyi, M.; Lobodzinska, E.; Lohwasser, K.; Medinnis, M.; Moenig, K.; Naumann, T.; Peschke, R.; Petit, E.; Radescu, V.; Rubinskiy, I.; Schaefer, R.; Sedov, G.; Shushkevich, S.; South, D.; Stanescu-Bellu, M.; Stanitzki, M. M.; Starovoitov, P.; Styles, N. A.; Tackmann, K.; Vankov, P.; Wang, J.; Wasicki, C.; Yatsenko, E.; Yildirim, E.] DESY, Hamburg, Germany. [Burmeister, I.; Esch, H.; Gossling, C.; Jentzsch, J.; Jung, C. A.; Klingenberg, R.; Wittig, T.] Tech Univ Dortmund, Inst Experimentelle Phys 6, Dortmund, Germany. [Anger, P.; Franconi, L.; Friedrich, F.; Grohs, J. P.; Gumpert, C.; Kobel, M.; Mader, W. F.; Morgenstern, M.; Novgorodova, O.; Rudolph, C.; Schnoor, U.; Siegert, F.; Socher, F.; Staerz, S.; Straessner, A.; Vest, A.; Wahrmund, S.] Tech Univ Dresden, Inst Kern & Teilchenphys, D-01062 Dresden, Germany. [Arce, A. T. H.; Benjamin, D. P.; Bocci, A.; Cerio, B. C.; Kajomovitz, E.; Kotwal, A.; Kruse, M. C.; Li, L.; Li, S.; Liu, M.; Oh, S. H.; Pollard, C. S.; Wang, C.] Duke Univ, Dept Phys, Durham, NC 27706 USA. [Bhimji, W.; Bristow, T. M.; Clark, P. J.; Dias, F. A.; Edwards, N. C.; Walls, F. M. Garay; Glaysher, P. C. F.; Harrington, R. D.; Leonidopoulos, C.; Martin, V. J.; Mills, C.; O'Brien, B. J.; Pino, S. A. Olivares; Proissl, M.; Selbach, K. E.; Smart, B. H.; Washbrook, A.; Wynne, B. M.] Univ Edinburgh, SUPA Sch Phys & Astron, Edinburgh, Midlothian, Scotland. [Annovi, A.; Antonelli, M.; Bilokon, H.; Chiarella, V.; Curatolo, M.; D'Onofrio, M.; Di Nardo, R.; Esposito, B.; Gatti, C.; Laurelli, P.; Maccarrone, G.; Mancini, G.; Prokofiev, K.; Sansoni, A.; Testa, M.; Vilucchi, E.] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy. [Amoroso, S.; Arnold, H.; Betancourt, C.; Boehler, M.; Bruneliere, R.; Buehrer, F.; Buescher, D.; Coniavitis, E.; Consorti, V.; Dao, V.; Di Simone, A.; Fehling-Kaschek, M.; Giuliani, C.; Herten, G.; Jakobs, K.; Javurek, T.; Jenni, P.; Kiss, F.; Koeneke, K.; Kopp, A. K.; Kuehn, S.; Lai, S.; Landgraf, U.; Madar, R.; Mahboubi, K.; Mohr, W.; Pagacova, M.; Parzefall, U.; Rave, T. C.; Ronzani, M.; Ruhr, F.; Rurikova, Z.; Ruthmann, N.; Schillo, C.; Schumacher, M.; Sommer, P.; Sundermann, J. E.; Temming, K. K.; Tsiskaridze, V.; Ungaro, F. C.; von Radziewski, H.; Anh, T. Vu; Warsinsky, M.; Weiser, C.; Werner, M.; Zimmermann, S.] Univ Freiburg, Fak Math & Phys, D-79106 Freiburg, Germany. [Alexandre, G.; Ancu, L. S.; Barone, G.; Bell, J.; Bell, W. H.; Noccioli, E. Benhar; De Mendizabal, J. Bilbao; Bucci, F.; Toro, R. Camacho; Clark, A.; Delitzsch, C. M.; della Volpe, D.; Doglioni, C.; Ferrere, D.; Gadomski, S.; Gonzalez-Sevilla, S.; Goulette, M. P.; Gramling, J.; Iacobucci, G.; Katre, A.; La Rosa, A.; Mermod, P.; Miucci, A.; Muenstermann, D.; Nektarijevic, S.; Nikolics, K.; Picazio, A.; Pohl, M.; Rosbach, K.; Tykhonov, A.; Vallecorsa, S.; Wu, X.] Univ Geneva, Sect Phys, Geneva, Switzerland. [Barberis, D.; Darbo, G.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Gemme, C.; Guido, E.; Morettinia, P.; Osculati, B.; Parodi, F.; Passaggio, S.; Rossi, L. P.; Schiavi, C.] Ist Nazl Fis Nucl, Sez Genova, Milan, Italy. [Barberis, D.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Guido, E.; Osculati, B.; Parodi, F.; Schiavi, C.] Univ Genoa, Dipartimento Fis, Genoa, Italy. [Jejelava, J.; Tskhadadze, E. G.] Javakhishvili Tbilisi State Univ, E Andronikashvili Inst Phys 6, Tbilisi, Rep of Georgia. [Djobava, T.; Durglishvili, A.; Jejelava, J.; Khubua, J.; Mosidze, M.] Tbilisi State Univ, Inst High Energy Phys, Tbilisi, Rep of Georgia. [Dueren, M.; Kreutzfeldt, K.; Stenzel, H.] Univ Giessen, Inst Phys 2, Giessen, Germany. [Bates, R. L.; Britton, D.; Buckley, A. G.; Bussey, P.; Buttar, C. M.; Buzatu, A.; Cinca, D.; D'Auria, S.; Doherty, T.; Doyle, A. T.; Ferrag, S.; Ferrando, J.; de Lima, D. E. Ferreira; Gemmell, A.; Gul, U.; Ortiz, N. G. Gutierrez; Kar, D.; Knue, A.; O'Shea, V.; Barrera, C. Oropeza; Qin, G.; Quilty, D.; Ravenscroft, T.; Robson, A.; Saxon, D. H.; Smith, K. M.; Denis, R. D. St.; Stewart, G. A.; Thompson, A. S.; Wright, M.] Univ Glasgow, SUPA Sch Phys & Astron, Glasgow, Lanark, Scotland. [Bierwagen, K.; Bindi, M.; Blumenschein, U.; George, M.; Grosse-Knetter, J.; Hamer, M.; Kareem, J.; Kawamura, G.; Keil, M.; Kroeninger, K.; Lemmer, B.; Magradze, E.; Llacer, M. Moreno; Musheghyan, H.; Nackenhorst, O.; Nadal, J.; Quadt, A.; Rieger, J.; Schorlemmer, A. L. S.; Serkin, L.; Shabalina, E.; Stolte, P.; Schroeder, T. Vazquez; Weingarten, J.; Zinonos, Z.] Univ Gottingen, Inst Phys 2, Gottingen, Germany. [Albrand, S.; Brown, J.; Collot, J.; Crepe-Renaudin, G.; Dechenaux, B.; Delsart, P. A.; Gabaldon, C.; Genest, M. H.; Hostachy, J-Y.; Ledroit-Guillon, F.; Lleres, A.; Lucotte, A.; Malek, F.; Monini, C.; Stark, J.; Trocme, B.; Wu, M.] Univ Grenoble Alpes, Lab Phys Subatom & Cosmol, CNRS IN2P3, Grenoble, France. [McFarlane, K. W.] Hampton Univ, Dept Phys, Hampton, VA 23668 USA. [da Costa, J. Barreiro Guimaraes; Butler, B.; Catastini, P.; Conti, G.; Fracchia, S.; Huth, J.; Ippolito, V.; Mateos, D. Lopez; Mchedlidze, G.; Mercurio, K. M.; Morii, M.; Skottowe, H. P.; Spearman, W. R.; Sun, S.; Tolley, E.; Yen, A. L.; della Porta, G. Zevi] Harvard Univ, Lab Particle Phys & Cosmol, Cambridge, MA 02138 USA. [Andrei, V.; Baas, A. E.; Badescu, E.; Brandt, O.; Davygora, Y.; Dietzsch, T. A.; Djuvsland, J. I.; Dunforda, M.; Hanke, P.; Jongmanns, J.; Khomich, A.; Kluge, E. -E.; Laier, H.; Lang, V. S.; Meier, K.; Mueller, F.; Poddar, S.; Scharf, V.; Schultz-Coulon, H. -C.; Stamen, R.; Wessels, M.] Heidelberg Univ, Kirchhoff Inst fr Phys, D-69115 Heidelberg, Germany. [Giulini, M.; Kasieczka, G.; Narayan, R.; Schaetzel, S.; Schmitt, S.; Schoening, A.] Heidelberg Univ, Inst Phys, D-69115 Heidelberg, Germany. [Colombo, T.; Kugel, A.] Heidelberg Univ, ZITI Inst Tech Informat, Mannheim, Germany. [Nagasaka, Y.] Hiroshima Inst Technol, Fac Appl Informat Sci, Hiroshima, Japan. [Fleischmann, P.] Chinese Univ Hong Kong, Dept Phys, Shatin, Hong Kong, Peoples R China. Univ Hong Kong, Dept Phys, Hong Kong, Hong Kong, Peoples R China. Hong Kong Univ Sci & Technol, Dept Phys, Kowloon, Hong Kong, Peoples R China. [Brunet, S.; Dattagupta, A.; Evans, H.; Gagnon, P.; Lammers, S.; Martinez, N. Lorenzo; Luehring, F.; Ogren, H.; Penwell, J.; Poveda, J.; Weinert, B.; Zieminska, D.] Indiana Univ, Dept Phys, Bloomington, IN 47405 USA. [Francavilla, P.; Franz, S.; Jussel, P.; Kneringer, E.; Lukas, W.; Nagai, K.; Ritsch, E.; Usanova, A.] Leopold Franzens Univ, Inst Astro & Teilchenphys, Innsbruck, Austria. [Mallik, U.; Mandrysch, R.; Morange, N.; Zaidan, R.] Univ Iowa, Iowa City, IA USA. [Chen, C.; Cochran, J.; De Lorenzi, F.; Donini, J.; Dudziak, F.; Krumnack, N.; Pluth, D.; Prell, S.; Shrestha, S.; Yamamoto, K.] Iowa State Univ, Dept Phys & Astron, Ames, IA USA. [Aleksandrov, I. N.; Bednyakov, V. A.; Budagov, I. A.; Cheplakov, A.; Chizhov, M. V.; Dedovich, D. V.; Demichev, M.; Glonti, G. L.; Gostkin, M. I.; Karpov, S. N.; Karpova, Z. M.; Kazarinov, M. Y.; Khramov, E.; Kotov, V. M.; Kruchonak, U.; Krumshteyn, Z. V.; Kukhtin, V.; Ladygin, E.; Minashvili, I. A.; Mineev, M.; Olchevski, A. G.; Peshekhonov, V. D.; Plotnikova, E.; Potrap, I. N.; Pozdnyakov, V.; Rusakovich, N. A.; Sadykov, R.; Sapronov, A.; Shiyakova, M.; Sisakyan, A. N.; Soloshenko, A.; Sumida, T.; Topilin, N. D.; Vinogradov, V. B.; Yeletskikh, I.; Zhemchugov, A.; Zimine, N. I.] JINR Dubna, Joint Inst Nucl Res, Dubna, Russia. [Alonso, A.; Amako, K.; Aoki, M.; Arai, Y.; Ikegami, Y.; Ikeno, M.; Iwasaki, H.; Kanzaki, J.; Kohriki, T.; Kondo, T.; Kono, T.; Makida, Y.; Mitsui, S.; Nagano, K.; Nakamura, K.; Nozaki, M.; Odaka, S.; Sasaki, O.; Suzuki, Y.; Takubo, Y.; Tanaka, S.; Terada, S.; Tokushuku, K.; Tsuno, S.; Unno, Y.; Yamada, M.; Yamamoto, A.; Yasu, Y.] KEK, High Energy Accelerator Res Org, Tsukuba, Ibaraki, Japan. [Hasegawa, M.; Inamaru, Y.; Kishimoto, T.; Kurashige, H.; Kurumida, R.; Ochi, A.; Shimizu, S.; Takeda, H.; Yakabe, R.; Yamazaki, Y.; Yuan, L.] Kobe Univ, Grad Sch Sci, Kobe, Hyogo 657, Japan. [Ishino, M.; Tashiro, T.] Kobe Univ, Fac Sci, Kobe, Hyogo 657, Japan. [Takashima, R.] Kyoto Univ, Kyoto 612, Japan. [Kawagoe, K.; Oda, S.; Otono, H.; Tojo, J.] Kyushu Univ, Dept Phys, Fukuoka 812, Japan. [Verzini, M. J. Alconada; Alonso, F.; Anduaga, X. S.; Dova, M. T.; Monticelli, F.; Wahlberg, H.] Univ Nacl La Plata, Inst Fis La Plata, La Plata, Argentina. [Verzini, M. J. Alconada; Alonso, F.; Anduaga, X. S.; Dova, M. T.; Monticelli, F.; Wahlberg, H.] Consejo Nacl Invest Cient & Tecn, La Plata, Argentina. [Allison, L. J.; Barton, A. E.; Beattie, M. D.; Borissov, G.; Bouhova-Thacker, E. V.; Dearnaley, W. J.; Bustos, A. C. Florez; Grimm, K.; Henderson, R. C. W.; Hughes, G.; Jones, R. W. L.; Kartvelishvili, V.; Long, R. E.; Love, P. A.; Maddocks, H. J.; Smizanska, M.; Walder, J.] Univ Lancaster, Dept Phys, Lancaster, England. [Chiodini, G.; Gorini, E.; Orlando, N.; Perrino, R.; Primavera, M.; Spagnolo, S.; Ventura, A.] Ist Nazl Fis Nucl, Sez Lecce, I-73100 Lecce, Italy. [Gorini, E.; Orlando, N.; Spagnolo, S.; Ventura, A.] Univ Salento, Dipartimento Matemat & Fis, Lecce, Italy. [Allport, P. P.; Bundock, A. C.; Burdin, S.; Dervan, P.; Gwilliam, C. B.; Hayward, H. S.; Jackson, M.; Jones, T. J.; King, B. T.; Klein, M.; Klein, U.; Kretzschmar, J.; Laycock, P.; Lehan, A.; Mahmoud, S.; Maxfield, S. J.; Mehta, A.; Migas, S.; Price, J.; Readioff, N. P.; Schnellbach, Y. J.; Sellers, G.; Vossebeld, J. H.; Waller, P.] Univ Liverpool, Oliver Lodge Lab, Liverpool L69 3BX, Merseyside, England. [Chilingarov, A.; Cindro, V.; Deliyergiyev, M.; Filipcic, A.; Gorisek, A.; Kersevan, B. P.; Kramberger, G.; Mandic, I.; Mikuz, M.; Sfiligoj, T.] Jozef Stefan Inst, Dept Phys, Ljubljana, Slovenia. [Chilingarov, A.; Cindro, V.; Deliyergiyev, M.; Filipcic, A.; Gorisek, A.; Kersevan, B. P.; Kramberger, G.; Mandic, I.; Mikuz, M.; Sfiligoj, T.] Univ Ljubljana, Ljubljana, Slovenia. [Alpigiani, C.; Bona, M.; Bret, M. Cano; Cerrito, L.; Fitzgerald, E. A.; Goddard, J. R.; Hickling, R.; Landon, M. P. J.; Morris, J. D.; Piccaro, E.; Rizvi, E.; Sandbach, R. L.; Snidero, G.; Castanheira, M. Teixeira Dias] Queen Mary Univ London, Sch Phys & Astron, London, England. [Berry, T.; Boisvert, V.; Brooks, T.; Connelly, I. A.; Cooper-Smith, N. J.; Cowan, G.; Duguid, L.; George, S.; Gibson, S. M.; Kempster, J. J.; Vazquez, J. G. Panduro; Pastore, Fr.; Rose, M.; Spano, F.; Teixeira-Dias, P.; Thomas-Wilsker, J.] Royal Holloway Univ London, Dept Phys, Surrey, England. [Bernat, P.; Bieniek, S. P.; Butterworth, J. M.; Campanelli, M.; Casadei, D.; Chislett, R. T.; Cooper, B. D.; Davison, A. R.; Davison, P.; Falla, R. J.; Gregersen, K.; Gutschow, C.; Hesketh, G. G.; Jansen, E.; Konstantinidis, N.; Korn, A.; Kucuk, H.; Lambourne, L.; Leney, K. J. C.; Martyniuk, A. C.; Mcfayden, J. A.; Nurse, E.; Ochoa, M. I.; Pilkington, A. D.; Scanlon, T.; Sherwood, P.; Simmons, B.; Wardrope, D. R.; Waugh, B. M.; Wijeratne, P. A.] UCL, Dept Phys & Astron, London, England. [Bernius, C.; Jana, D. K.; Lloyd, S. L.; Sircar, A.; Subramaniam, R.] Louisiana Tech Univ, Ruston, LA 71270 USA. [Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; Davignon, O.; De Cecco, S.; Demilly, A.; Derue, F.; Formica, A.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Liu, K.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Vannucci, F.; Varouchas, D.] UPMC, Lab Phys Nucl & Hautes Energies, Paris, France. [Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; Davignon, O.; De Cecco, S.; Demilly, A.; Derue, F.; Formica, A.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Liu, K.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Vannucci, F.; Varouchas, D.] Univ Paris Diderot, Paris, France. [Bomben, M.; Calderini, G.; Crescioli, F.; Davignon, O.; De Cecco, S.; Demilly, A.; Derue, F.; Formica, A.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Liu, K.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Vannucci, F.; Varouchas, D.] CNRS IN2P3, Paris, France. [Akesson, T. P. A.; Bocchetta, S. S.; Bryngemark, L.; Fleck, I.; Hawkins, A. D.; Hedberg, V.; Ivarsson, J.; Jarlskog, G.; Lytken, E.; Meirose, B.; Mjoernmark, J. U.; Smirnova, O.; Viazlo, O.] Lund Univ, Fysiska Inst, Lund, Sweden. [Arnal, V.; Barreiro, F.; Cantero, J.; De la Torre, H.; Del Peso, J.; Glasman, C.; Merino, J. Llorente; Terron, J.] Univ Autonoma Madrid, Dept Fis Teor C 15, Madrid, Spain. [Blum, W.; Buescher, V.; Caputo, R.; Caudron, J.; Ellinghaus, F.; Endner, O. C.; Ertel, E.; Fiedler, F.; Torregrosa, E. Fullana; Goeringer, C.; Heck, T.; Hohlfeld, M.; Hsu, P. J.; Huelsing, T. A.; Karnevskiy, M.; Kleinknecht, K.; Koenig, S.; Koepke, L.; Lin, T. H.; Lungwitz, M.; Masetti, L.; Mattmann, J.; Meyer, C.; Moreno, D.; Moritz, S.; Mueller, T.; Poettgen, R.; Sander, H. G.; Schaefer, U.; Schmitt, C.; Schott, M.; Schroeder, C.; Schuh, N.; Simioni, E.; Tapprogge, S.; Wollstadt, S. J.; Zimmermann, C.] Johannes Gutenberg Univ Mainz, Inst Phys, Mainz, Germany. [Borri, M.; Cox, B. E.; Da Via, C.; Flick, T.; Ponce, J. M. Iturbe; Joshi, K. D.; Klinger, J. A.; Loebinger, F. K.; Marsden, S. P.; Masik, J.; Neep, T. J.; Oh, A.; Owen, M.; Pater, J. R.; Peters, R. F. Y.; Price, D.; Qin, Y.; Queitsch-Maitland, M.; Robinson, J. E. M.; Schwanenberger, C.; Thompson, R. J.; Tomlinson, L.; Watts, S.; Webb, S.; Woudstra, M. J.; Wyatt, T. R.; Yang, U. K.] Univ Manchester, Sch Phys & Astron, Manchester, Lancs, England. [Aad, G.; Alio, L.; Barbero, M.; Bertella, C.; Clemens, J. C.; Coadou, Y.; Diglio, S.; Djama, F.; Feligioni, L.; Hoffmann, D.; Hubaut, F.; Knoops, E. B. F. G.; Le Guirriec, E.; Li, B.; Madaffari, D.; Mochizuki, K.; Monnier, E.; Muanza, S.; Nagai, Y.; Pralavorio, P.; Rozanov, A.; Serre, T.; Talby, M.; Tiouchichine, E.; Tisserant, S.; Toth, J.; Touchard, F.; Ughetto, M.; Vacavant, L.] Aix Marseille Univ, CPPM, Marseille, France. [Aad, G.; Alio, L.; Barbero, M.; Bertella, C.; Clemens, J. C.; Coadou, Y.; Diglio, S.; Djama, F.; Feligioni, L.; Hoffmann, D.; Hubaut, F.; Knoops, E. B. F. G.; Le Guirriec, E.; Li, B.; Madaffari, D.; Mochizuki, K.; Monnier, E.; Muanza, S.; Nagai, Y.; Pralavorio, P.; Rozanov, A.; Serre, T.; Talby, M.; Tiouchichine, E.; Tisserant, S.; Toth, J.; Touchard, F.; Ughetto, M.; Vacavant, L.] CNRS IN2P3, Marseille, France. [Bellomo, M.; Brau, B.; Colon, G.; Dallapiccola, C.; Daya-Ishmukhametova, R. K.; Moyse, E. J. W.; Pais, P.; Pueschel, E.; Varol, T.; Ventura, D.; Willocq, S.] Univ Massachusetts, Dept Phys, Amherst, MA USA. [Belanger-Champagne, C.; Chapleau, B.; Cheatham, S.; Mantifel, R.; Robichaud-Veronneau, A.; Stockton, M. C.; Stoebe, M.; Vachon, B.; Wang, K.; Warburton, A.] McGill Univ, Dept Phys, Montreal, PQ, Canada. [Barberio, E. L.; Brennan, A. J.; Jennens, D.; Kubota, T.; Limosani, A.; Hanninger, G. Nunes; Nuti, F.; Rados, P.; Spiller, L. A.; Tan, K. G.; Taylor, G. N.; Thong, W. M.; Urquijo, P.; Volpi, M.; Zanzi, D.] Univ Melbourne, Sch Phys, Melbourne, Vic 3010, Australia. [Amidei, D.; Chelstowska, M. A.; Cheng, H. C.; Dai, T.; Diehl, E. B.; Dubbert, J.; Feng, H.; Ferretti, C.; Goldfarb, S.; Harper, D.; Hu, X.; Levin, D.; Liu, L.; Long, J. D.; Lu, N.; Mc Kee, S. P.; McCarn, A.; Neal, H. A.; Panikashvili, N.; Qian, J.; Schwarz, T. A.; Searcy, J.; Thun, R. P.; Wilson, A.; Wu, Y.; Xu, L.; Yu, J. M.; Zhang, D.; Zhou, B.; Zhu, J.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA. [Abolins, M.; Gonzalez, B. Alvarez; Arabidze, G.; Brock, R.; Bromberg, C.; Chegwidden, A.; Fisher, W. C.; Halladjian, G.; Hauser, R.; Hayden, D.; Huston, J.; Koll, J.; Linnemann, J. T.; Martin, B.; Pope, B. G.; Schoenrock, B. D.; Schwienhorst, R.; Ta, D.; Tollefson, K.; True, P.; Willis, C.; Zhang, H.] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA. [Alimonti, G.; Andreazza, A.; Besana, M. I.; Carminati, L.; Cavallia, D.; Citterio, M.; Consonni, S. M.; Costa, G.; Fanti, M.; Giugni, D.; Lari, T.; Mandelli, L.; Meroni, C.; Perini, L.; Pizio, C.; Ragusa, F.; Resconi, S.; Simoniello, R.; Tartarelli, G. F.; Troncon, C.; Turra, R.; Perez, M. Villaplana] Ist Nazl Fis Nucl, Sez Milano, I-20133 Milan, Italy. [Andreazza, A.; Carminati, L.; Consonni, S. M.; Fanti, M.; Perini, L.; Pizio, C.; Ragusa, F.; Simoniello, R.; Turra, R.; Perez, M. Villaplana] Univ Milan, Dipartimento Fis, Milan, Italy. [Bogouch, A.; Harkusha, S.; Kulchitsky, Y.; Kurochkin, Y. A.; Tsiareshka, P. V.] Natl Acad Sci Belarus, BI Stepanov Inst Phys, Minsk, Byelarus. 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G.; Nagel, M.; Nisius, R.; Nowak, S.; Oberlack, H.; Pahl, C.; Richter, R.; Salihagic, D.; Sandstroem, R.; Schacht, P.; Schwegler, Ph.; Sforza, F.; Spettel, F.; Stern, S.; Stonjek, S.; Terzo, S.; von der Schmitt, H.; Weigell, P.; Wildauer, A.] Max Planck Inst Phys & Astrophys, Werner Heisenberg Inst, D-80805 Munich, Germany. [Shimojima, M.] Nagasaki Inst Appl Sci, Nagasaki, Japan. [Hasegawa, S.; Horii, Y.; Morvaj, L.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Grad Sch Sci, Nagoya, Aichi 4648601, Japan. [Hasegawa, S.; Horii, Y.; Morvaj, L.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Kobayashi Maskawa Inst, Nagoya, Aichi 4648601, Japan. [Aloisio, A.; Alviggi, M. G.; Canale, V.; Carlino, G.; Chiefari, G.; Conventi, F.; de Asmundis, R.; Della Pietra, M.; Di Donato, C.; Doria, A.; Giordano, R.; Iengo, P.; Izzo, V.; Merola, L.; Patricelli, S.; Perrella, S.; Rossi, E.; Sanchez, A.; Sekhniaidze, G.; Zurzolo, G.] Ist Nazl Fis Nucl, Sez Napoli, I-80125 Naples, Italy. [Aloisio, A.; Alviggi, M. G.; Canale, V.; Chiefari, G.; Di Donato, C.; Giordano, R.; Merola, L.; Patricelli, S.; Perrella, S.; Rossi, E.; Sanchez, A.; Zurzolo, G.] Univ Naples Federico II, Dipartimento Fis, Naples, Italy. [Gorelov, I.; Hoeferkamp, M. R.; Seidel, C.; Toms, K.; Wang, R.] Univ New Mexico, Dept Phys & Astron, Albuquerque, NM 87131 USA. [Besjes, G. J.; Caron, S.; Croft, V.; De Groot, N.; Filthaut, F.; Galea, C.; Klok, P. F.; Koenig, A. C.; Salvucci, A.; Strubig, A.] Radboud Univ Nijmegen, Inst Math Astrophys & Particle Phys, NL-6525 ED Nijmegen, Netherlands. [Aben, R.; Angelozzi, I.; Beemster, L. J.; Bentvelsen, S.; Berge, D.; Bobbink, G. J.; Bos, K.; Boterenbrood, H.; Butti, P.; Castelli, A.; Colijn, A. P.; de Jong, P.; De Nooij, L.; Deigaard, I.; Deluca, C.; Deviveiros, P. O.; Dhaliwal, S.; Ferrari, P.; Gadatsch, S.; Geerts, D. A. A.; Hartjes, F.; Hessey, N. P.; Hod, N.; Igonkina, O.; Kluit, P.; Koffeman, E.; Lee, H.; Linde, F.; Mahlstedt, J.; Mechnich, J.; Oussoren, K. P.; Pani, P.; Sabato, G.; Salek, D.; Slawinska, M.; Valencic, N.; Van Den Wollenberg, W.; Van der Deijl, P. C.; van der Geer, R.; van der Graaf, H.; Van Der Leeuw, R.; van Vulpen, I.; Verkerke, W.; Vermeulen, J. C.; Vreeswijk, M.; Weits, H.] Nikhef Natl Inst Subat Phys, Amsterdam, Netherlands. [Burghgrave, B.; Calkins, R.; Chakraborty, D.; Cole, S.; Suhr, C.; Yurkewicz, A.; Zutshi, V.] No Illinois Univ, Dept Phys, De Kalb, IL 60115 USA. [Anisenkov, V.; Bobrovnikov, V. S.; Bogdanchikov, A. G.; Kazanin, V. F.; Korol, A. A.; Malyshev, V. M.; Maslennikov, A. L.; Maximov, D. A.; Peleganchuk, S. V.; Rezanova, O. L.; Skovpen, K. Yu.; Soukharev, M.; Talyshev, A. A.; Tikhonov, Yu. A.] SB RAS, Budker Inst Nucl Phys, Novosibirsk 630090, Russia. [Cranmer, K.; Haas, A.; Heinrich, L.; van Huysduynen, L. Hooft; Kaplan, B.; Karthik, K.; Kreiss, S.; Lewis, G. H.; Mincer, A. I.; Nemethy, P.; Neves, R. M.] NYU, Dept Phys, New York, NY 10003 USA. [Gan, K. K.; Ishmukhametov, R.; Kagan, H.; Kass, R. D.; Merritt, H.; Moss, J.; Nagarkar, A.; Pignotti, D. T.; Tannenwald, B. B.; Yang, Y.] Ohio State Univ, Columbus, OH 43210 USA. [Nakano, I.] Okayama Univ, Fac Sci, Okayama 700, Japan. [Abbott, B.; Bertsche, C.; Bertsche, D.; Gutierrez, P.; Hasib, A.; Norberg, S.; Saleem, M.; Severini, H.; Skubic, P.; Strauss, M.] Univ Oklahoma, Homer L Dodge Dept Phys & Astron, Norman, OK 73019 USA. [Abi, B.; Bousson, N.; Khanov, A.; Rizatdinova, F.; Sidorov, D.; Yu, J.] Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USA. [Chytka, L.; Hamal, P.; Hrabovsky, M.; Kvita, J.; Nozka, L.] Palacky Univ, RCPTM, CR-77147 Olomouc, Czech Republic. [Brau, J. E.; Brost, E.; Hopkins, W. H.; Majewski, S.; Potter, C. T.; Ptacek, E.; Radloff, P.; Shamim, M.; Sinev, N. B.; Strom, D. M.; Torrence, E.; Wanotayaroj, C.; Winklmeier, F.] Univ Oregon, Ctr High Energy Phys, Eugene, OR 97403 USA. [Khalek, S. Abdel; Bassalat, A.; Becot, C.; Binet, S.; Bourdarios, C.; Braun, H. M.; Charfeddine, D.; De Regie, J. B. De Vivie; Duflot, L.; Escalier, M.; Fayard, L.; Castillo, L. R. Flores; Grivaz, J. -F.; Guillemin, T.; Henrot-Versille, S.; Hrivnac, J.; Iconomidou-Fayard, L.; Kado, M.; Lounis, A.; Makovec, N.; Nellist, C.; Poggioli, L.; Puzo, P.; Renaud, A.; Rousseau, D.; Rybkin, G.; Schaffer, A. C.; Scifo, E.; Serin, L.; Simion, S.; Tanaka, R.; Tran, H. L.; Zerwas, D.; Zhang, Z.] Univ Paris 11, LAL, Orsay, France. [Khalek, S. Abdel; Bassalat, A.; Becot, C.; Binet, S.; Bourdarios, C.; Braun, H. M.; Charfeddine, D.; De Regie, J. B. De Vivie; Duflot, L.; Escalier, M.; Fayard, L.; Castillo, L. R. Flores; Grivaz, J. -F.; Guillemin, T.; Henrot-Versille, S.; Hrivnac, J.; Iconomidou-Fayard, L.; Kado, M.; Lounis, A.; Makovec, N.; Nellist, C.; Poggioli, L.; Puzo, P.; Renaud, A.; Rousseau, D.; Rybkin, G.; Schaffer, A. C.; Scifo, E.; Serin, L.; Simion, S.; Tanaka, R.; Tran, H. L.; Zerwas, D.; Zhang, Z.] CNRS IN2P3, Orsay, France. [Endo, M.; Hanagaki, K.; Lee, J. S. H.; Nomachi, M.; Okamura, W.; Sugaya, Y.; Teoh, J. J.; Yamaguchi, Y.] Osaka Univ, Grad Sch Sci, Osaka, Japan. [Bugge, L.; Bugge, M. K.; Cameron, D.; Catmore, J. R.; Fox, H.; Gjelsten, B. K.; Gramstad, E.; Ould-Saada, F.; Pajchel, K.; Pedersen, M.; Read, A. L.; Rohne, O.; Stapnes, S.; Strandlie, A.] Univ Oslo, Dept Phys, Oslo, Norway. [Barr, A. J.; Behr, K.; Boddy, C. R.; Buckingham, R. M.; Cooper-Sarkar, A. M.; Ortuzar, M. Crispin; Dafinca, A.; Gallas, E. J.; Gupta, S.; Gwenlan, C.; Hall, D.; Hays, C. P.; Henderson, J.; Howard, J.; Huffman, T. B.; Issever, C.; Kalderon, C. W.; King, R. S. B.; Kogan, L. A.; Lewis, A.; Livermore, S. S. A.; Nickerson, R. B.; Pachal, K.; Pinder, A.; Ryder, N. C.; Sawyer, C.; Short, D.; Tseng, J. C-L.; Viehhauser, G. H. A.; Weidberg, A. R.; Zhong, J.] Univ Oxford, Dept Phys, Oxford, England. [Conta, C.; Dondero, P.; Ferrari, R.; Franchini, M.; Fraternali, M.; Gaudio, G.; Livan, M.; Negri, A.; Polesello, G.; Rebuzzi, D. M.; Rimoldi, A.; Vercesi, V.] Ist Nazl Fis Nucl, Sez Pavia, I-27100 Pavia, Italy. [Conta, C.; Dondero, P.; Franchini, M.; Fraternali, M.; Livan, M.; Negri, A.; Rebuzzi, D. M.; Rimoldi, A.] Univ Pavia, Dipartimento Fis, I-27100 Pavia, Italy. [Brendlinger, K.; Heim, S.; Hines, E.; Hong, T. M.; Jackson, B.; Kroll, J.; Kunkle, J.; Lester, C. M.; Lipeles, E.; Meyer, C.; Ospanov, R.; Saxon, J.; Stahlman, J.; Thomson, E.; Tuna, A. N.; Vanguri, R.; Williams, H. H.] Univ Penn, Dept Phys, Philadelphia, PA 19104 USA. [Ezhilov, A.; Gratchev, V.; Grebenyuk, O. G.; Levchenko, M.; Maleev, V. P.; Ryabov, Y. F.; Schegelsky, V. A.; Sedykh, E.; Seliverstov, D. M.; Solovyev, V.] Petersburg Nucl Phys Inst, Gatchina, Russia. [Beccherle, R.; Bertolucci, F.; Bini, C.; Cavasinni, V.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Leone, S.; Roda, C.; Scuri, F.; Volpi, G.; White, S.] Ist Nazl Fis Nucl, Sez Pisa, I-56010 Pisa, Italy. [Beccherle, R.; Bertolucci, F.; Bini, C.; Cavasinni, V.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Leone, S.; Roda, C.; Scuri, F.; Volpi, G.; White, S.] Univ Pisa, Dipartimento Fis E Fermi, Pisa, Italy. [Bianchi, R. M.; Boudreau, J.; Cleland, W.; Escobar, C.; Kittelmann, T.; Mueller, J.; Prieur, D.; Sapp, K.; Su, J.; Yoosoofmiya, R.] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA. [Aguilar-Saavedra, J. A.; Dos Santos, S. P. Amor; Amorim, A.; Araque, J. P.; Cantrill, R.; Carvalho, J.; Castro, N. F.; Muino, P. Conde; Sargedas De Sousa, M. J. Da Cunha; Wemans, A. Do Valle; Fiolhais, M. C. N.; Galhardo, B.; Gomes, A.; Goncalo, R.; Jorge, P. M.; Lopes, L.; Miguens, J. Machado; Maio, A.; Maneira, J.; Marques, C. N.; Onofre, A.; Palma, A.; Pedro, R.; Pina, J.; Pinto, B.; Santos, H.; Saraiva, J. G.; Silva, J.; Delgado, A. Tavares; Veloso, F.; Wolters, H.] Lab Instrument & Fis Expt Particulas LIP, Lisbon, Portugal. [Amorim, A.; Muino, P. Conde; Sargedas De Sousa, M. J. Da Cunha; Gomes, A.; Jorge, P. M.; Miguens, J. Machado; Maio, A.; Maneira, J.; Palma, A.; Pedro, R.; Pina, J.; Saraiva, J. G.; Silva, J.; Delgado, A. Tavares] Univ Lisbon, Fac Ciencias, Lisbon, Portugal. [Dos Santos, S. P. Amor; Carvalho, J.; Fiolhais, M. C. N.; Galhardo, B.; Veloso, F.; Wolters, H.] Univ Coimbra, Dept Phys, Coimbra, Portugal. [Gomes, A.; Maio, A.; Pina, J.] Univ Lisbon, Ctr Fis ca Nucl, P-1699 Lisbon, Portugal. [Onofre, A.] Univ Minho, Dept Fis, Braga, Portugal. [Aguilar-Saavedra, J. A.] Univ Granada, Dept Fis Teor & Cosmos, Granada, Spain. [Aguilar-Saavedra, J. A.] Univ Granada, CAFPE, Granada, Spain. [Wemans, A. Do Valle] Univ Nova Lisboa, Dep Fis, Caparica, Portugal. [Wemans, A. Do Valle] Univ Nova Lisboa, CEFITEC, Fac Ciencias & Tecnol, Caparica, Portugal. [Bohm, J.; Chudoba, J.; Havranek, M.; Jakoubek, T.; Kepka, O.; Kupco, A.; Kus, V.; Lokajicek, M.; Lysak, R.; Marcisovsky, M.; Mikestikova, M.; Nemecek, S.; Sicho, P.; Staroba, P.; Svatos, M.; Tasevsky, M.; Vrba, V.] Acad Sci Czech Republic, Inst Phys, Prague, Czech Republic. [Augsten, K.; Gallus, P.; Guenther, J.; Hejbal, J.; Jakubek, J.; Kohout, Z.; Kral, V.; Myska, M.; Pospisil, S.; Seifert, F.; Simak, V.; Slavicek, T.; Smolek, K.; Solar, M.; Solc, J.; Sopczak, A.; Sopko, B.; Sopko, V.; Suk, M.; Turecek, D.; Vacek, V.; Vlasak, M.; Vokac, P.; Vykydal, Z.; Zeman, M.] Czech Tech Univ, CR-16635 Prague, Czech Republic. [Balek, P.; Berta, P.; Cerny, K.; Chalupkova, I.; Davidek, T.; Dolejsi, J.; Dolezal, Z.; Faltova, J.; Kodys, P.; Leitner, R.; Pleskot, V.; Reznicek, P.; Rybar, M.; Scheirich, D.; Spousta, M.; Sykora, T.; Tas, P.; Todorova-Nova, S.; Valkar, S.; Vorobel, V.] Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic. [Borisov, A.; Denisov, S. P.; Fakhrutdinov, R. M.; Fenyuk, A. B.; Golubkov, D.; Kamenshchikov, A.; Karyukhin, A. N.; Korotkov, V. A.; Kozhin, A. S.; Minaenko, A. A.; Myagkov, A. G.; Nikolaenko, V.; Solodkov, A. A.; Solovyanov, O. V.; Starchenko, E. A.; Zaitsev, A. M.; Zenin, O.] State Res Ctr Inst High Energy Phys, Protvino, Russia. [Adye, T.; Apolle, R.; Baines, J. T.; Barnett, M.; Burke, S.; Davies, E.; Dewhurst, A.; Dopke, J.; Emeliyanov, D.; Gallop, B. J.; Gee, C. N. P.; Haywood, S. J.; Kirk, J.; Martin-Haugh, S.; McCubbin, N. A.; McMahon, S. J.; Middleton, R. P.; Murray, W. J.; Sankey, D. P. C.; Scott, W. G.; Tyndel, M.; Wickens, F. J.; Wielers, M.] Rutherford Appleton Lab, Particle Phys Dept, Didcot OX11 0QX, Oxon, England. [Benslama, K.] Univ Regina, Dept Phys, Regina, SK S4S 0A2, Canada. [Tanaka, S.] Ritsumeikan Univ, Kusatsu, Shiga, Japan. [Anulli, F.; Bagiacchi, P.; Bagnaia, P.; Bini, C.; Ciapetti, G.; De Pedis, D.; De Salvo, A.; Di Domenico, A.; Dionisi, C.; Falcianoa, S.; Gabrielli, A.; Gauzzi, P.; Gentile, S.; Giagu, S.; Giannetti, P.; Kuna, M.; Lacava, F.; Luci, C.; Luminari, L.; Marzano, F.; Mirabelli, G.; Monzani, S.; Nisati, A.; Pasqualucci, E.; Petrolo, E.; Pontecorvo, L.; Rescigno, M.; Rosati, S.; Tehrani, F. Safai; Sidoti, A.; Vanadia, M.; Vari, R.; Veneziano, S.; Verducci, M.; Zanello, L.] Ist Nazl Fis Nucl, Sez Roma, Rome, Italy. [Bagiacchi, P.; Bagnaia, P.; Bini, C.; Ciapetti, G.; Di Domenico, A.; Dionisi, C.; Gabrielli, A.; Gauzzi, P.; Gentile, S.; Giagu, S.; Giannetti, P.; Kuna, M.; Lacava, F.; Luci, C.; Messina, A.; Monzani, S.; Vanadia, M.; Verducci, M.; Zanello, L.] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy. [Aielli, G.; Cardarelli, R.; Cattani, G.; Di Ciaccio, A.; Di Domenico, A.; Grossi, G. C.; Iuppa, R.; Liberti, B.; Mazzaferro, L.; Paolozzi, L.; Salamon, A.; Santonico, R.] Ist Nazl Fis Nucl, Sez Roma Tor Vergata, Rome, Italy. [Aielli, G.; Cattani, G.; Di Ciaccio, A.; Di Domenico, A.; Grossi, G. C.; Iuppa, R.; Mazzaferro, L.; Paolozzi, L.; Santonico, R.] Univ Roma Tor Vergata, Dipartimento Fis, I-00173 Rome, Italy. [Bacci, C.; Bagiacchi, P.; Baroncelli, A.; Biglietti, M.; Bortolotto, V.; Ceradini, F.; Di Micco, B.; Farilla, A.; Graziani, E.; Iodice, M.; Orestano, D.; Passeri, A.; Pastore, F.; Petrucci, F.; Puddu, D.; Salamanna, G.; Stanescu, C.; Taccini, C.; Delgado, A. Tavares; Trovatelli, M.] Ist Nazl Fis Nucl, Sez Roma Tre, Rome, Italy. [Bacci, C.; Bagiacchi, P.; Bortolotto, V.; Ceradini, F.; Di Micco, B.; Orestano, D.; Pastore, F.; Petrucci, F.; Puddu, D.; Salamanna, G.; Taccini, C.; Delgado, A. Tavares; Trovatelli, M.] Univ Roma Tre, Dipartimento Matemat & Fis, Rome, Italy. [Benchekroun, D.; Chafaq, A.; Chang, P.; Gouighri, M.; Hoummada, A.] Univ Hassan 2, Reseau Univ Phys Hautes Energies, Fac Sci Ain Chock, Casablanca, Morocco. [Ghazlane, H.] Ctr Natl Energie Sci Techn Nucl, Rabat, Morocco. [El Kacimi, M.; Goujdami, D.] Univ Cadi Ayyad, LPHEA, Fac Sci Semlalia, Marrakech, Morocco. [Boutouil, S.; Derkaoui, J. E.; Ouchrif, M.; Tayalati, Y.] Univ Mohamed Premier, Fac Sci, Oujda, Morocco. [Boutouil, S.; Derkaoui, J. E.; Ouchrif, M.; Tayalati, Y.] LPTPM, Oujda, Morocco. [El Moursli, R. Cherkaoui; Fassi, F.; Haddad, N.; Idrissi, Z.] Univ Mohammed V Agdal, Fac Sci, Rabat, Morocco. [Bachacou, H.; Balli, F.; Bauer, F.; Besson, N.; Blanchard, J. -B.; Boonekamp, M.; Calandri, A.; Chevalier, L.; Hoffmann, M. Dano; Ernwein, J.; Etienvre, A. I.; Fletcher, G.; Giraud, P. F.; Da Costa, J. Goncalves Pinto Firmino; Grabas, H. M. X.; Guyot, C.; Hanna, R.; Hassani, S.; Kozanecki, W.; Lancon, E.; Laporte, J. F.; Maiani, C.; Mal, P.; Mansoulie, B.; Martinez, H.; Meric, N.; Meyer, J-P.; Nicolaidou, R.; Ouraou, A.; Protopapadaki, E.; Royon, C. R.; Schoeffel, L.; Schune, Ph.; Schwemling, Ph.; Schwindling, J.; Tsionou, D.; Vranjes, N.; Xiao, M.] CEA Saclay, DSM IRFU, Inst Rech Lois Fondament Univers, Commissariat Energie Atom & Energies Alternat, F-91191 Gif Sur Yvette, France. [Battaglia, M.; Debenedetti, C.; Deliot, F.; Grillo, A. A.; Kuhl, A.; Law, A. T.; Liang, Z.; Litke, A. M.; Lockman, W. S.; Manning, P. M.; Nielsen, J.; Reece, R.; Rose, P.; Sadrozinski, H. F-W.; Schumm, B. A.; Seiden, A.] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA. [Blackburn, D.; Coccaro, A.; Goussiou, A. G.; Harris, O. M.; Hsu, S. -C.; Lubatti, H. J.; Marx, M.; Rompotis, N.; Rosten, R.; Rothberg, J.; De Bruin, P. H. Sales; Watts, G.] Univ Washington, Dept Phys, Seattle, WA 98195 USA. [Anastopoulos, C.; Costanzo, D.; Donszelmann, T. Cuhadar; Dawson, I.; Hodgkinson, M. C.; Hodgson, P.; Johansson, P.; Korolkova, E. V.; Paredes, B. Lopez; Miyagawa, P. S.; Paganis, E.; Suruliz, K.; Tovey, D. R.] Univ Sheffield, Dept Phys & Astron, Sheffield, S Yorkshire, England. [Hasegawa, Y.; Takeshita, T.] Shinshu Univ, Dept Phys, Nagano, Japan. [Atlay, N. B.; Buchholz, P.; Czirr, H.; Gaur, B.; Ibragimov, I.; Ikematsu, K.; Rosenthal, O.; Sipica, V.; Walkowiak, W.; Ziolkowski, M.] Univ Siegen, Fachbereich Phys, D-57068 Siegen, Germany. [Buat, Q.; Dawe, E.; O'Neil, D. C.; Stelzer, B.; Tanasijczuk, A. J.; Torres, H.; Van Nieuwkoop, J.] Simon Fraser Univ, Dept Phys, Burnaby, BC V5A 1S6, Canada. [Astalos, R.; Bartos, P.; Blazek, T.; Federic, P.; Plazak, L.; Stavina, P.; Sykora, I.; Tokar, S.; Zenis, T.] Comenius Univ, Fac Math Phys & Informat, Bratislava, Slovakia. [Antos, J.; Bruncko, D.; Kladiva, E.; Strizenec, P.] Slovak Acad Sci, Inst Expt Phys, Dept Subnuclear Phys, Kosice 04353, Slovakia. [Hamiltona, A.] Univ Cape Town, Dept Phys, ZA-7925 Cape Town, South Africa. [Castaneda-Miranda, E.; Connell, S. H.; Yacoob, S.] Univ Johannesburg, Dept Phys, Johannesburg, South Africa. [Bristow, K.; Carrillo-Montoya, G. D.; Hamity, G. N.; Hsuc, C.; March, L.; Ruan, X.; Vickey, T.; Boeriu, O. E. Vickey] Univ Johannesburg, Sch Phys, Johannesburg, South Africa. [Abulaiti, Y.; Akerstedt, H.; Asman, B.; Bendtz, K.; Bertoli, G.; Bessidskaia, O.; Bohm, C.; Clement, C.; Cribbs, W. A.; Erikssona, D.; Gellerstedt, K.; Hellman, S.; Johansson, K. E.; Jon-And, K.; Khandanyan, H.; Kim, H.; Klimek, P.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Petridis, A.; Plucinski, P.; Rossetti, V.; Silverstein, S. B.; Sjlin, J.; Strandberg, S.; Tylmad, M.] Stockholm Univ, Dept Phys, S-10691 Stockholm, Sweden. [Abulaiti, Y.; Akerstedt, H.; Asman, B.; Bendtz, K.; Bertoli, G.; Bessidskaia, O.; Clement, C.; Cribbs, W. A.; Gellerstedt, K.; Hellman, S.; Johansson, K. E.; Jon-And, K.; Khandanyan, H.; Kim, H.; Klimek, P.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Petridis, A.; Plucinski, P.; Rossetti, V.; Sjlin, J.; Strandberg, S.; Tylmad, M.] Oskar Klein Ctr, Stockholm, Sweden. [Jovicevic, J.; Kuwertz, E. S.; Lund-Jensen, B.; Morley, A. K.; Strandberg, J.] Royal Inst Technol, Dept Phys, S-10044 Stockholm, Sweden. [Bee, C. P.; Campoverde, A.; Chen, K.; Engelmann, R.; Grassi, V.; Hobbs, J.; Jia, J.; Li, H.; Lindquist, B. E.; Mastrandrea, P.; McCarthy, R. L.; Puldon, D.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.] SUNY Stony Brook, Dept Phys, Stony Brook, NY 11794 USA. [Bee, C. P.; Campoverde, A.; Chen, K.; Engelmann, R.; Hobbs, J.; Jia, J.; Li, H.; Lindquist, B. E.; Mastrandrea, P.; McCarthy, R. L.; Puldon, D.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.] SUNY Stony Brook, Dept Astron & Chem, Stony Brook, NY 11794 USA. [Bartsch, V.; Cerri, A.; Barajas, C. A. Chavez; De Sanctis, U.; De Santo, A.; Grout, Z. J.; Potter, C. J.; Salvatore, F.; Castillo, I. Santoyo; Shehu, C. Y.; Sutton, M. R.; Vivarelli, I.] Univ Sussex, Dept Phys & Astron, Brighton, E Sussex, England. [Black, C. W.; Cuthbert, C.; Finelli, K. D.; Jeng, G. -Y.; Patel, N. D.; Saavedra, A. F.; Scarcella, M.; Varvell, K. E.; Watson, I. J.; Yabsley, B.] Univ Sydney, Sch Phys, Sydney, NSW 2006, Australia. [Abdallah, J.; Chu, M. L.; Hou, S.; Jamin, D. O.; Lee, C. A.; Lee, S. C.; Lin, S. C.; Liu, B.; Liu, D.; Lo Sterzo, F.; Mazini, R.; Ren, Z. L.; Shi, L.; Soh, A.; Teng, P. K.; Wang, C.; Wang, S. M.; Weng, Z.; Zhang, L.] Acad Sinica, Inst Phys, Taipei, Taiwan. [Abreu, H.; Di Mattia, A.; Kopeliansky, R.; Musto, E.; Rozen, Y.; Tarem, S.] Technion Israel Inst Technol, Dept Phys, IL-32000 Haifa, Israel. [Abramowicz, H.; Alexander, G.; Amram, N.; Ashkenazi, A.; Bella, G.; Benary, O.; Benhammou, Y.; Davies, M.; Etzion, E.; Gershon, A.; Gueta, O.; Guttman, N.; Munwes, Y.; Oren, Y.; Sadeh, I.; Silver, Y.; Soffer, A.; Taiblum, N.] Tel Aviv Univ, Raymond & Beverly Sackler Sch Phys & Astro, Tel Aviv, Israel. [Bachas, K.; Gkaitatzis, S.; Gkialas, I.; Iliadis, D.; Kordas, K.; Kouskoura, V.; Leisos, A.; Papageorgiou, K.; Hernandez, D. Paredes; Petridou, C.; Sampsonidis, D.; Sidiropoulou, O.] Aristotle Univ Thessaloniki, Dept Phys, Thessaloniki, Greece. [Akimoto, G.; Asai, S.; Azuma, Y.; Backhaus, M.; Dohmae, T.; Enari, Y.; Hanawa, K.; Kanaya, N.; Kataoka, Y.; Kawamoto, T.; Kazama, S.; Kessoku, K.; Kobayashi, T.; Komori, Y.; Mashimo, T.; Masubuchi, T.; Minami, Y.; Nakamura, T.; Ninomiya, Y.; Okuyama, T.; Sakamoto, H.; Sasaki, Y.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamaguchi, H.; Yamamoto, S.; Yamamura, T.; Yamanaka, T.; Yoshihara, K.] Univ Tokyo, Int Ctr Elementary Particle Phys, Tokyo, Japan. [Akimoto, G.; Asai, S.; Azuma, Y.; Backhaus, M.; Dohmae, T.; Enari, Y.; Hanawa, K.; Kanaya, N.; Kataoka, Y.; Kawamoto, T.; Kazama, S.; Kessoku, K.; Kobayashi, T.; Komori, Y.; Mashimo, T.; Masubuchi, T.; Minami, Y.; Nakamura, T.; Ninomiya, Y.; Okuyama, T.; Sakamoto, H.; Sasaki, Y.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamaguchi, H.; Yamamoto, S.; Yamamura, T.; Yamanaka, T.; Yoshihara, K.] Univ Tokyo, Dept Phys, Tokyo 113, Japan. [Bratzler, U.] Tokyo Metropolitan Univ, Grad Sch Sci & Technol, Tokyo 158, Japan. [Fukunaga, C.; Hirose, M.; Ishitsuka, M.; Jinnouchi, O.; Kobayashi, D.; Kuze, M.; Motohashi, K.; Nagai, R.; Nobe, T.; Pettersson, N. E.] Tokyo Inst Technol, Dept Phys, Tokyo 152, Japan. [AbouZeid, O. S.; Brelier, B.; Chau, C. C.; Ilic, N.; Keung, J.; Krieger, P.; Mc Coldrick, G.; Orr, R. S.; Polifka, R.; Rudolph, M. S.; Savard, P.; Schramm, S.; Sinervo, P.; Spreitzer, T.; Taenzer, J.; Teuscher, R. J.; Thompson, P. 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[Conventi, F.; Della Pietra, M.] Univ Napoli Parthenope, Naples, Italy. [Fedin, O. L.] St Petersburg State Polytech Univ, Dept Phys, St Petersburg, Russia. [Gkialas, I.] Univ Aegean, Dept Financial & Management Engn, Chios, Greece. [Greenwood, Z. D.; Sawyer, L.] Louisiana Tech Univ, Ruston, LA 71270 USA. [Grinstein, S.; Rozas, A. Juste; Martinez, M.] Inst Catalana Recerca & Estudis Avancats ICREA, Barcelona, Spain. [Ilchenko, Y.; Onyisi, P. U. E.] Univ Texas Austin, Dept Phys, Austin, TX 78712 USA. [Jejelava, J.] Ilia State Univ, Inst Theoret Phys, Tbilisi, Rep of Georgia. [Jenni, P.] CERN, Geneva, Switzerland. Ochanomizu Univ, Ochadai Acad Prod, Tokyo 112, Japan. Manhattan Coll, New York, NY USA. [Li, Y.] Univ Paris 11, LAL, Orsay, France. [Li, Y.] CNRS IN2P3, Orsay, France. [Lin, S. C.] Acad Sinica, Inst Phys, Acad Sinica Grid Comp, Taipei 115, Taiwan. [Mal, P.] Natl Inst Sci Educ & Res, Sch Phys Sci, Bhubaneswar, Orissa, India. [Myagkov, A. G.; Nikolaenko, V.; Zaitsev, A. M.] State Univ, Moscow Inst Phys & Technol, Dolgoprudnyi, Russia. [Nessi, M.] Univ Geneva, Sect Phys, Geneva, Switzerland. [Pinamonti, M.] Int Sch Adv Studies SISSA, Trieste, Italy. [Purohit, M.] Univ S Carolina, Dept Phys & Astron, Columbia, SC 29208 USA. [Shi, L.; Soh, A.] Sun Yat Sen Univ, Sch Phys & Engn, Guangzhou 510275, Guangdong, Peoples R China. [Smirnova, L. N.; Turchikhin, S.] Moscow MV Lomonosov State Univ, Fac Phys, Moscow, Russia. [Tikhomirov, V. O.] Natl Res Nucl Univ MEPhI, Moscow, Russia. [Toth, J.] Wigner Res Ctr Phys, Inst Particle & Nucl Phys, Budapest, Hungary. [Wang, C.] Nanjing Univ, Dept Phys, Nanjing, Jiangsu, Peoples R China. [Wildt, M. A.] Univ Hamburg, Inst Experimentalphys, Hamburg, Germany. Univ Michigan, Ann Arbor, MI USA. [Yacoob, S.] Univ Kwazulu Natal, Discipline Phys, Durban, South Africa. [Yusuff, I.] Univ Malaya, Dept Phys, Kuala Lumpur 59100, Malaysia. RP Dolgoshein, BA (reprint author), Natl Res Nucl Univ MEPhI, Moscow, Russia. RI SULIN, VLADIMIR/N-2793-2015; Nechaeva, Polina/N-1148-2015; Vykydal, Zdenek/H-6426-2016; Olshevskiy, Alexander/I-1580-2016; Snesarev, Andrey/H-5090-2013; BESSON, NATHALIE/L-6250-2015; Vanadia, Marco/K-5870-2016; Ippolito, Valerio/L-1435-2016; Maneira, Jose/D-8486-2011; Prokoshin, Fedor/E-2795-2012; KHODINOV, ALEKSANDR/D-6269-2015; Staroba, Pavel/G-8850-2014; Tartarelli, Giuseppe Francesco/A-5629-2016; Fassi, Farida/F-3571-2016; la rotonda, laura/B-4028-2016; Goncalo, Ricardo/M-3153-2016; Gauzzi, Paolo/D-2615-2009; Mindur, Bartosz/A-2253-2017; Fabbri, Laura/H-3442-2012; Solodkov, Alexander/B-8623-2017; Zaitsev, Alexandre/B-8989-2017; Peleganchuk, Sergey/J-6722-2014; Li, Liang/O-1107-2015; Monzani, Simone/D-6328-2017; Korol, Aleksandr/A-6244-2014; Capua, Marcella/A-8549-2015; Connell, Simon/F-2962-2015; Bosman, Martine/J-9917-2014; Joergensen, Morten/E-6847-2015; Mitsou, Vasiliki/D-1967-2009; Riu, Imma/L-7385-2014; Mir, Lluisa-Maria/G-7212-2015; Marti-Garcia, Salvador/F-3085-2011; Della Pietra, Massimo/J-5008-2012; Cavalli-Sforza, Matteo/H-7102-2015; Petrucci, Fabrizio/G-8348-2012; Negrini, Matteo/C-8906-2014; Ferrer, Antonio/H-2942-2015; White, Ryan/E-2979-2015; Brooks, William/C-8636-2013; Wemans, Andre/A-6738-2012; Castro, Nuno/D-5260-2011; Boyko, Igor/J-3659-2013; Nemecek, Stanislav/G-5931-2014; Gutierrez, Phillip/C-1161-2011; Di Domenico, Antonio/G-6301-2011; Ventura, Andrea/A-9544-2015; Livan, Michele/D-7531-2012; De, Kaushik/N-1953-2013; Smirnova, Oxana/A-4401-2013; Villa, Mauro/C-9883-2009; Grancagnolo, Sergio/J-3957-2015; Doyle, Anthony/C-5889-2009; spagnolo, stefania/A-6359-2012; Ciubancan, Liviu Mihai/L-2412-2015; Zhukov, Konstantin/M-6027-2015; Shmeleva, Alevtina/M-6199-2015; Gavrilenko, Igor/M-8260-2015; Tikhomirov, Vladimir/M-6194-2015; Yang, Haijun/O-1055-2015; Chekulaev, Sergey/O-1145-2015; Warburton, Andreas/N-8028-2013; Gorelov, Igor/J-9010-2015; Gladilin, Leonid/B-5226-2011; Carvalho, Joao/M-4060-2013; Mashinistov, Ruslan/M-8356-2015; Buttar, Craig/D-3706-2011; Gonzalez de la Hoz, Santiago/E-2494-2016; Guo, Jun/O-5202-2015; Aguilar Saavedra, Juan Antonio/F-1256-2016; Leyton, Michael/G-2214-2016; Jones, Roger/H-5578-2011; Pacheco Pages, Andres/C-5353-2011; Vranjes Milosavljevic, Marija/F-9847-2016; Perrino, Roberto/B-4633-2010 OI SULIN, VLADIMIR/0000-0003-3943-2495; Vykydal, Zdenek/0000-0003-2329-0672; Olshevskiy, Alexander/0000-0002-8902-1793; Vanadia, Marco/0000-0003-2684-276X; Ippolito, Valerio/0000-0001-5126-1620; Maneira, Jose/0000-0002-3222-2738; Prokoshin, Fedor/0000-0001-6389-5399; KHODINOV, ALEKSANDR/0000-0003-3551-5808; Di Micco, Biagio/0000-0002-4067-1592; Tartarelli, Giuseppe Francesco/0000-0002-4244-502X; Fassi, Farida/0000-0002-6423-7213; la rotonda, laura/0000-0002-6780-5829; Osculati, Bianca Maria/0000-0002-7246-060X; Amorim, Antonio/0000-0003-0638-2321; Giorgi, Filippo Maria/0000-0003-1589-2163; Coccaro, Andrea/0000-0003-2368-4559; Goncalo, Ricardo/0000-0002-3826-3442; Gauzzi, Paolo/0000-0003-4841-5822; Mindur, Bartosz/0000-0002-5511-2611; Fabbri, Laura/0000-0002-4002-8353; Solodkov, Alexander/0000-0002-2737-8674; Zaitsev, Alexandre/0000-0002-4961-8368; Peleganchuk, Sergey/0000-0003-0907-7592; Li, Liang/0000-0001-6411-6107; Monzani, Simone/0000-0002-0479-2207; Korol, Aleksandr/0000-0001-8448-218X; Giordani, Mario/0000-0002-0792-6039; Capua, Marcella/0000-0002-2443-6525; Connell, Simon/0000-0001-6000-7245; Bosman, Martine/0000-0002-7290-643X; Joergensen, Morten/0000-0002-6790-9361; Mitsou, Vasiliki/0000-0002-1533-8886; Riu, Imma/0000-0002-3742-4582; Mir, Lluisa-Maria/0000-0002-4276-715X; Della Pietra, Massimo/0000-0003-4446-3368; Petrucci, Fabrizio/0000-0002-5278-2206; Negrini, Matteo/0000-0003-0101-6963; Ferrer, Antonio/0000-0003-0532-711X; White, Ryan/0000-0003-3589-5900; Brooks, William/0000-0001-6161-3570; Wemans, Andre/0000-0002-9669-9500; Castro, Nuno/0000-0001-8491-4376; Boyko, Igor/0000-0002-3355-4662; Di Domenico, Antonio/0000-0001-8078-2759; Ventura, Andrea/0000-0002-3368-3413; Livan, Michele/0000-0002-5877-0062; De, Kaushik/0000-0002-5647-4489; Smirnova, Oxana/0000-0003-2517-531X; Villa, Mauro/0000-0002-9181-8048; Grancagnolo, Sergio/0000-0001-8490-8304; Doyle, Anthony/0000-0001-6322-6195; spagnolo, stefania/0000-0001-7482-6348; Ciubancan, Liviu Mihai/0000-0003-1837-2841; Tikhomirov, Vladimir/0000-0002-9634-0581; Warburton, Andreas/0000-0002-2298-7315; Gorelov, Igor/0000-0001-5570-0133; Gladilin, Leonid/0000-0001-9422-8636; Carvalho, Joao/0000-0002-3015-7821; Mashinistov, Ruslan/0000-0001-7925-4676; Gonzalez de la Hoz, Santiago/0000-0001-5304-5390; Guo, Jun/0000-0001-8125-9433; Aguilar Saavedra, Juan Antonio/0000-0002-5475-8920; Leyton, Michael/0000-0002-0727-8107; Jones, Roger/0000-0002-6427-3513; Pacheco Pages, Andres/0000-0001-8210-1734; Vranjes Milosavljevic, Marija/0000-0003-4477-9733; Perrino, Roberto/0000-0002-5764-7337 FU ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; ANAS, Azerbaijan; SSTC, Belarus; CNPq; FAPESP, Brazil; BMWF; FWF, Austria; NSERC; NRC; CFI, Canada; CERN; CONICYT, Chile; CAS; MOST; NSFC, China; COL-CIENCIAS, Colombia; MSMT CR; MPO CR; VSC CR, Czech Republic; DNRF; DNSRC; Lundbeck Foundation, Denmark; EPLANET; ERC; NSRF; European Union; IN2P3-CNRS; CEA-DSM/IRFU, France; GNSF, Georgia; BMBF; DFG; HGF; MPG; AvH Foundation, Germany; GSRT; NSRF, Greece; ISF; MINERVA; GIF; DIP; Benoziyo Center, Israel; INFN, Italy; MEXT; JSPS, Japan; CNRST, Morocco; FOM; NWO, Netherlands; BRF; RCN, Norway; MNiSW, Poland; GRICES; FCT, Portugal; MERYS (MECTS), Romania; MES of Russia; ROSATOM; Russian Federation; Russian Federation; JINR; MSTD, Serbia; MSSR, Slovakia; ARRS; MIZS, Slovenia; DST/NRF, South Africa; MICINN, Spain; SRC; Wallenberg Foundation, Sweden; SER; SNSF; Cantons of Bern and Geneva, Switzerland; NSC, Taiwan; TAEK, Turkey; STFC; Royal Society and Leverhulme Trust, United Kingdom; DOE; NSF, United States of America FX We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWF and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile; CAS, MOST and NSFC, China; COL-CIENCIAS, Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF, DNSRC and Lundbeck Foundation, Denmark; EPLANET, ERC and NSRF, European Union; IN2P3-CNRS, CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, DFG, HGF, MPG and AvH Foundation, Germany; GSRT and NSRF, Greece; ISF, MINERVA, GIF, DIP and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; FOM and NWO, Netherlands; BRF and RCN, Norway; MNiSW, Poland; GRICES and FCT, Portugal; MERYS (MECTS), Romania; MES of Russia and ROSATOM, Russian Federation; JINR; MSTD, Serbia; MSSR, Slovakia; ARRS and MIZS, Slovenia; DST/NRF, South Africa; MICINN, Spain; SRC and Wallenberg Foundation, Sweden; SER, SNSF and Cantons of Bern and Geneva, Switzerland; NSC, Taiwan; TAEK, Turkey; STFC, the Royal Society and Leverhulme Trust, United Kingdom; DOE and NSF, United States of America. NR 69 TC 31 Z9 31 U1 8 U2 90 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0370-2693 EI 1873-2445 J9 PHYS LETT B JI Phys. Lett. B PD NOV 10 PY 2014 VL 738 BP 234 EP 253 DI 10.1016/j.physletb.2014.09.054 PG 20 WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AT0KK UT WOS:000344624900038 ER PT J AU Jimenez-Delgado, P Avakian, H Melnitchouk, W AF Jimenez-Delgado, P. Avakian, H. Melnitchouk, W. CA Jefferson Lab Angular Momentum JAM TI Constraints on spin-dependent parton distributions at large x from global QCD analysis SO PHYSICS LETTERS B LA English DT Article ID DEEP-INELASTIC SCATTERING; POLARIZED HE-3; FORM-FACTORS; QUARK; DUALITY AB We investigate the behavior of spin-dependent parton distribution functions (PDFs) at large parton momentum fractions x in the context of global QCD analysis. We explore the constraints from existing deep-inelastic scattering data, and from theoretical expectations for the leading x -> 1 behavior based on hard gluon exchange in perturbative QCD. Systematic uncertainties from the dependence of the PDFs on the choice of parametrization are studied by considering functional forms motivated by orbital angular momentum arguments. Finally, we quantify the reduction in the PDF uncertainties that may be expected from future high-x data from Jefferson Lab at 12 GeV. (C) 2014 The Authors. Published by Elsevier B.V. C1 [Jimenez-Delgado, P.; Avakian, H.; Melnitchouk, W.] Jefferson Lab, Newport News, VA 23606 USA. RP Melnitchouk, W (reprint author), Jefferson Lab, Newport News, VA 23606 USA. FU DOE Contract under Jefferson Science Associates, LLC operates Jefferson Lab [DE-AC05-06OR23177] FX We thank A. Accardi for helpful discussions, and J.-P. Chen, S. Kuhn, G. Schnell, B. Wojtsekhowski and X. Zheng for communications about existing and future polarization asymmetry experiments. This work was supported by the DOE Contract No. DE-AC05-06OR23177, under which Jefferson Science Associates, LLC operates Jefferson Lab. NR 35 TC 5 Z9 5 U1 0 U2 2 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0370-2693 EI 1873-2445 J9 PHYS LETT B JI Phys. Lett. B PD NOV 10 PY 2014 VL 738 BP 263 EP 267 DI 10.1016/j.physletb.2014.09.049 PG 5 WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AT0KK UT WOS:000344624900041 ER PT J AU Khachatryan, V Sirunyan, AM Tumasyan, A Adam, W Bergauer, T Dragicevic, M Ero, J Fabjan, C Friedl, M Fruhwirth, R Ghete, VM Hartl, C Hormann, N Hrubec, J Jeitler, M Kiesenhofer, W Knunz, V Krammer, M Kratschmer, I Liko, D Mikulec, I Rabady, D Rahbaran, B Rohringer, H Schofbeck, R Strauss, J Taurok, A Treberer-Treberspurg, W Waltenberger, W Wulz, CE Mossolov, V Shumeiko, N Gonzalez, JS Alderweireldt, S Bansal, M Bansal, S Cornelis, T De Wolf, EA Janssen, X Knutsson, A Luyckx, S Ochesanu, S Roland, B Rougny, R De Klundert, MV Van Haevermaet, H Van Mechelen, P Van Remortel, N Van Spilbeeck, A Blekman, F Blyweert, S D'Hondt, J Daci, N Heracleous, N Keaveney, J Kim, TJ Lowette, S Maes, M Olbrechts, A Python, Q Strom, D Tavernier, S Van Doninck, W Van Mulders, 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Lath, A. Panwalkar, S. Park, M. Patel, R. Rekovic, V. Salur, S. Schnetzer, S. Seitz, C. Somalwar, S. Stone, R. Thomas, S. Thomassen, P. Walker, M. Rose, K. Spanier, S. York, A. Bouhali, O. Eusebi, R. Flanagan, W. Gilmore, J. Kamon, T. Khotilovich, V. Krutelyov, V. Montalvo, R. Osipenkov, I. Pakhotin, Y. Perloff, A. Roe, J. Rose, A. Safonov, A. Sakuma, T. Suarez, I. Tatarinov, A. Akchurin, N. Cowden, C. Damgov, J. Dragoiu, C. Dudero, P. R. Faulkner, J. Kovitanggoon, K. Kunori, S. Lee, S. W. Libeiro, T. Volobouev, I. Appelt, E. Delannoy, A. G. Greene, S. Gurrola, A. Johns, W. Maguire, C. Mao, Y. Melo, A. Sharma, M. Sheldon, P. Snook, B. Tuo, S. Velkovska, J. Arenton, M. W. Boutle, S. Cox, B. Francis, B. Goodell, J. Hirosky, R. Ledovskoy, A. Li, H. Lin, C. Neu, C. Wood, J. Harr, R. Karchin, P. E. Don, C. Kottachchi Kankanamge Lamichhane, P. Sturdy, J. Belknap, D. A. Carlsmith, D. Cepeda, M. Dasu, S. Duric, S. Friis, E. Hall-Wilton, R. Herndon, M. Herve, A. Klabbers, P. Lanaro, A. Lazaridis, C. Levine, A. Loveless, R. Mohapatra, A. Ojalvo, I. Perry, T. Pierro, G. A. Polese, G. Ross, I. Sarangi, T. Savin, A. Smith, W. H. Woods, N. CA CMS Collaboration TI Search for excited quarks in the gamma plus jet final state in proton-proton collisions at root s=8 TeV SO PHYSICS LETTERS B LA English DT Article DE CMS; Physics; Photon; Jet ID PARTON DISTRIBUTIONS; HADRON COLLIDERS; LHC AB A search for excited quarks decaying into the gamma + jet final state is presented. The analysis is based on data corresponding to an integrated luminosity of 19.7 fb(-1) collected by the CMS experiment in proton-proton collisions at root s = 8 TeV at the LHC. Events with photons and jets with high transverse momenta are selected and the gamma + jet invariant mass distribution is studied to search for a resonance peak. The 95% confidence level upper limits on the product of cross section and branching fraction are evaluated as a function of the excited quark mass. 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A.; Dell'Orso, R.; Donato, S.; Fiori, F.; Foa, L.; Giassi, A.; Grippo, M. T.; Ligabue, F.; Lomtadze, T.; Martini, L.; Messineo, A.; Moon, C. S.; Palla, F.; Rizzi, A.; Savoy-Navarro, A.; Serban, A. T.; Spagnolo, P.; Squillacioti, P.; Tenchini, R.; Tonelli, G.; Venturi, A.; Verdini, P. G.; Vernieri, C.] Ist Nazl Fis Nucl, Sez Pisa, Pisa, Italy. [Martini, L.; Messineo, A.; Rizzi, A.; Tonelli, G.] Univ Pisa, Pisa, Italy. [Broccolo, G.; Donato, S.; Fiori, F.; Foa, L.; Ligabue, F.; Vernieri, C.] Scuola Normale Super Pisa, Pisa, Italy. [Barone, L.; Cavallari, F.; Del Re, D.; Diemoz, M.; Grassi, M.; Jorda, C.; Longo, E.; Margaroli, F.; Meridiani, P.; Micheli, F.; Nourbakhsh, S.; Organtini, G.; Paramatti, R.; Rahatlou, S.; Rovelli, C.; Santanastasio, F.; Soffi, L.; Traczyk, P.] Ist Nazl Fis Nucl, Sez Roma, Rome, Italy. [Barone, L.; Del Re, D.; Grassi, M.; Longo, E.; Margaroli, F.; Micheli, F.; Nourbakhsh, S.; Organtini, G.; Rahatlou, S.; Santanastasio, F.; Soffi, L.; Traczyk, P.] Univ Rome, Rome, Italy. [Amapane, N.; Arcidiacono, R.; Argiro, S.; Arneodo, M.; Bellan, R.; Biino, C.; Cartiglia, N.; Casasso, S.; Costa, M.; Degano, A.; Demaria, N.; Finco, L.; Mariotti, C.; Maselli, S.; Migliore, E.; Monaco, V.; Musich, M.; Obertino, M. M.; Ortona, G.; Pacher, L.; Pastrone, N.; Pelliccioni, M.; Angioni, G. L. Pinna; Potenza, A.; Romero, A.; Ruspa, M.; Sacchi, R.; Solano, A.; Staiano, A.; Tamponi, U.] Ist Nazl Fis Nucl, Sez Torino, I-10125 Turin, Italy. [Amapane, N.; Argiro, S.; Bellan, R.; Casasso, S.; Costa, M.; Degano, A.; Finco, L.; Migliore, E.; Monaco, V.; Ortona, G.; Angioni, G. L. Pinna; Potenza, A.; Romero, A.; Sacchi, R.; Solano, A.] Univ Turin, Turin, Italy. [Arcidiacono, R.; Arneodo, M.; Obertino, M. M.; Ruspa, M.] Univ Piemonte Orientale Novara, Turin, Italy. [Giammanco, A.; Belforte, S.; Candelise, V.; Casarsa, M.; Cossutti, F.; Della Ricca, G.; Gobbo, B.; La Licata, C.; Marone, M.; Montanino, D.; Schizzi, A.; Umer, T.; Zanetti, A.] Ist Nazl Fis Nucl, Sez Trieste, Trieste, Italy. [Candelise, V.; Della Ricca, G.; La Licata, C.; Marone, M.; Montanino, D.; Schizzi, A.; Umer, T.] Univ Trieste, Trieste, Italy. [Chang, S.; Kropivnitskaya, A.; Nam, S. K.] Kangwon Natl Univ, Chunchon, South Korea. [Kim, D. H.; Kim, G. N.; Kim, M. S.; Kong, D. J.; Lee, S.; Oh, Y. D.; Park, H.; Sakharov, A.; Son, D. C.; Kamon, T.] Kyungpook Natl Univ, Taegu, South Korea. [Kim, J. Y.; Song, S.] Chonnam Natl Univ, Inst Univ & Elementary Particles, Kwangju, South Korea. [Choi, S.; Gyun, D.; Hong, B.; Jo, M.; Kim, H.; Kim, Y.; Lee, B.; Lee, K. S.; Park, S. K.; Roh, Y.] Korea Univ, Seoul, South Korea. [Choi, M.; Kim, J. H.; Park, I. C.; Park, S.; Ryu, G.; Ryu, M. S.] Univ Seoul, Seoul, South Korea. [Choi, Y.; Choi, Y. K.; Goh, J.; Kwon, E.; Lee, J.; Seo, H.; Yu, I.] Sungkyunkwan Univ, Suwon, South Korea. [Juodagalvis, A.] Vilnius State Univ, Vilnius, Lithuania. [Komaragiri, J. R.] Univ Malaya, Natl Ctr Particle Phys, Kuala Lumpur, Malaysia. [Castilla-Valdez, H.; De La Cruz-Burelo, E.; Heredia-de La Cruz, I.; Lopez-Fernandez, R.; Sanchez-Hernandez, A.] IPN, Ctr Invest & Estudios Avanzados, Mexico City 07738, DF, Mexico. [Carrillo Moreno, S.; Vazquez Valencia, F.] Univ Iberoamer, Mexico City, DF, Mexico. [Pedraza, I.; Salazar Ibarguen, H. A.] Univ Autonoma San Luis Potosi, San Luis Potosi, Mexico. [Krofcheck, D.] Univ Auckland, Auckland 1, New Zealand. [Butler, P. H.; Reucroft, S.] Univ Canterbury, Christchurch 1, New Zealand. [Ahmad, A.; Ahmad, M.; Hassan, Q.; Hoorani, H. R.; Khalid, S.; Khan, W. A.; Khurshid, T.; Shah, M. A.; Shoaib, M.] Quaid I Azam Univ, Natl Ctr Phys, Islamabad, Pakistan. [Bialkowska, H.; Bluj, M.; Boimska, B.; Frueboes, T.; Gorski, M.; Kazana, M.; Nawrocki, K.; Romanowska-Rybinska, K.; Szleper, M.; Zalewski, P.] Natl Ctr Nucl Res, Otwock, Poland. [Brona, G.; Bunkowski, K.; Cwiok, M.; Dominik, W.; Doroba, K.; Kalinowski, A.; Konecki, M.; Krolikowski, J.; Misiura, M.; Olszewski, M.; Wolszczak, W.] Univ Warsaw, Fac Phys, Inst Expt Phys, Warsaw, Poland. [Bargassa, P.; Beirao Da Cruz E Silva, C.; Faccioli, P.; Parracho, P. G. Ferreira; Gallinaro, M.; Nguyen, F.; Rodrigues Antunes, J.; Seixas, J.; Varela, J.; Vischia, P.] Lab Instrumentacao & Fisica Expt Particulas, Lisbon, Portugal. [Finger, M., Jr.; Bunin, P.; Gavrilenko, M.; Golutvin, I.; Kamenev, A.; Karjavin, V.; Konoplyanikov, V.; Lanev, A.; Malakhov, A.; Matveev, V.; Moisenz, P.; Palichik, V.; Perelygin, V.; Savina, M.; Shmatov, S.; Shulha, S.; Skatchkov, N.; Smirnov, V.; Zarubin, A.] Joint Inst Nucl Res, Dubna, Russia. [Golovtsov, V.; Ivanov, Y.; Kim, V.; Levchenko, P.; Murzin, V.; Oreshkin, V.; Smirnov, I.; Sulimov, V.; Uvarov, L.; Vavilov, S.; Vorobyev, A.; Vorobyev, An.] Petersburg Nucl Phys Inst, St Petersburg, Russia. [Matveev, V.; Andreev, Yu.; Dermenev, A.; Gninenko, S.; Golubev, N.; Kirsanov, M.; Krasnikov, N.; Pashenkov, A.; Tlisov, D.; Toropin, A.; Musienko, Y.] Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia. [Epshteyn, V.; Gavrilov, V.; Lychkovskaya, N.; Popov, V.; Safronov, G.; Semenov, S.; Spiridonov, A.; Stolin, V.; Vlasov, E.; Zhokin, A.; Starodumov, A.; Nikitenko, A.] Inst Theoret & Expt Phys, Moscow 117259, Russia. [Andreev, V.; Azarkin, M.; Dremin, I.; Kirakosyan, M.; Leonidov, A.; Mesyats, G.; Rusakov, S. V.; Vinogradov, A.] PN Lebedev Phys Inst, Moscow 117924, Russia. [Popov, A.; Zhukov, V.; Katkov, I.; Belyaev, A.; Boos, E.; Bunichev, V.; Dubinin, M.; Dudko, L.; Ershov, A.; Klyukhin, V.; Kodolova, O.; Lokhtin, I.; Obraztsov, S.; Petrushanko, S.; Savrin, V.; Snigirev, A.] Lomonosov Moscow State Univ, Skobeltsyn Inst Nucl Phys, Moscow, Russia. [Azhgirey, I.; Bayshev, I.; Bitioukov, S.; Kachanov, V.; Kalinin, A.; Konstantinov, D.; Krychkine, V.; Petrov, V.; Ryutin, R.; Sobol, A.; Tourtchanovitch, L.; Troshin, S.; Tyurin, N.; Uzunian, A.; Volkov, A.] Inst High Energy Phys, State Res Ctr Russian Federat, Protvino, Russia. [Adzic, P.; Dordevic, M.; Ekmedzic, M.; Milosevic, J.; Milenovic, P.] Univ Belgrade, Fac Phys, Belgrade 11001, Serbia. [Adzic, P.; Dordevic, M.; Ekmedzic, M.; Milosevic, J.; Milenovic, P.] Vinca Inst Nucl Sci, Belgrade, Serbia. [Alcaraz Maestre, J.; Battilana, C.; Calvo, E.; Cerrada, M.; Chamizo Llatas, M.; Colino, N.; De La Cruz, B.; Delgado Peris, A.; Dominguez Vazquez, D.; Escalante Del Valle, A.; Fernandez Bedoya, C.; Fernandez Ramos, J. P.; Flix, J.; Fouz, M. C.; Garcia-Abia, P.; Gonzalez Lopez, O.; Lopez, S. Goy; Hernandez, J. M.; Josa, M. I.; Merino, G.; Navarro De Martino, E.; Perez-Calero Yzquierdo, A.; Puerta Pelayo, J.; Quintario Olmeda, A.; Redondo, I.; Romero, L.; S. Soares, M.] Ctr Invest Energet Medioambient Tecnol CIEMAT, Madrid, Spain. [Albajar, C.; de Troconiz, J. F.; Missiroli, M.] Univ Autonoma Madrid, Madrid, Spain. [Brun, H.; Cuevas, J.; Fernandez Menendez, J.; Folgueras, S.; Gonzalez Caballero, I.; Lloret Iglesias, L.] Univ Oviedo, Oviedo, Spain. [Brochero Cifuentes, J. A.; Cabrillo, I. J.; Calderon, A.; Duarte Campderros, J.; Fernandez, M.; Gomez, G.; Graziano, A.; Lopez Virto, A.; Marco, J.; Marco, R.; Martinez Rivero, C.; Matorras, F.; Munoz Sanchez, F. J.; Piedra Gomez, J.; Rodrigo, T.; Rodriguez-Marrero, A. Y.; Ruiz-Jimeno, A.; Scodellaro, L.; Vila, I.; Vilar Cortabitarte, R.] Univ Cantabria, CSIC, Inst Fis Cantabria IFCA, E-39005 Santander, Spain. [Rabady, D.; Pernie, L.; Genchev, V.; Boudoul, G.; Contardo, D.; Lingemann, J.; Hartmann, F.; Hauth, T.; Kornmayer, A.; Mohanty, A. K.; Radogna, R.; Silvestris, L.; Masetti, G.; Costa, S.; Fiorendi, S.; Gennai, S.; Geros, R.; Lucchini, M. T.; Micheli, F.; Argiro, S.; Obertino, M. M.; Schizzi, A.; Abbaneo, D.; Auffray, E.; Auzinger, G.; Bachtis, M.; Baillon, P.; Ball, A. H.; Barney, D.; Benaglia, A.; Bendavid, J.; Benhabib, L.; Benitez, J. F.; Bernet, C.; Bianchi, G.; Bloch, P.; Bocci, A.; Bonato, A.; Bondu, O.; Botta, C.; Breuker, H.; Camporesi, T.; Cerminara, G.; Colafranceschi, S.; D'Alfonso, M.; d'Enterria, D.; Dabrowski, A.; David, A.; De Guio, F.; De Roeck, A.; De Visscher, S.; Dobson, M.; Dupont-Sagorin, N.; Elliott-Peisert, A.; Eugster, J.; Franzoni, G.; Funk, W.; Gigi, D.; Gill, K.; Giordano, D.; Girone, M.; Glege, F.; Guida, R.; Gundacker, S.; Guthoff, M.; Hammer, J.; Hansen, M.; Harris, P.; Hegeman, J.; Innocente, V.; Janot, P.; Kousouris, K.; Krajczar, K.; Lecoq, P.; Lourenco, C.; Magini, N.; Malgeri, L.; Mannelli, M.; Marrouche, J.; Masetti, L.; Meijers, F.; Mersi, S.; Meschi, E.; Moortgat, F.; Morovic, S.; Mulders, M.; Musella, P.; Orsini, L.; Pape, L.; Perez, E.; Perrozzi, L.; Petrilli, A.; Petrucciani, G.; Pfeiffer, A.; Pierini, M.; Pimiae, M.; Piparo, D.; Plagge, M.; Racz, A.; Rolandi, G.; Rovere, M.; Sakulin, H.; Schaefer, C.; Schwick, C.; Sekmen, S.; Sharma, A.; Siegrist, P.; Silva, P.; Simon, M.; Sphicas, P.; Spiga, D.; Steggemann, J.; Stieger, B.; Stoye, M.; Treille, D.; Tsirou, A.; Veres, G. 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Millan; Ngadiuba, J.; Robmann, P.; Ronga, F. J.; Snoek, H.; Taroni, S.; Verzetti, M.; Yang, Y.] Univ Zurich, Zurich, Switzerland. [Cardaci, M.; Chen, K. H.; Ferro, C.; Kuo, C. M.; Lin, W.; Lu, Y. J.; Volpe, R.; Yu, S. S.] Natl Cent Univ, Chungli 32054, Taiwan. [Chang, P.; Chang, Y. H.; Chang, Y. W.; Chao, Y.; Chen, K. F.; Chen, P. H.; Dietz, C.; Grundler, U.; Hou, W. -S.; Kao, K. Y.; Lei, Y. J.; Liu, Y. F.; Lu, R. -S.; Majumder, D.; Petrakou, E.; Tzeng, Y. M.; Wilken, R.] Natl Taiwan Univ, Taipei 10764, Taiwan. [Asavapibhop, B.; Srimanobhas, N.; Suwonjandee, N.] Chulalongkorn Univ, Bangkok, Thailand. [Adiguzel, A.; Bakirci, M. N.; Cerci, S.; Dozen, C.; Dumanoglu, I.; Eskut, E.; Girgis, S.; Gokbulut, G.; Gurpinar, E.; Hos, I.; Kangal, E. E.; Topaksu, A. Kayis; Onengut, G.; Ozdemir, K.; Ozturk, S.; Polatoz, A.; Sogut, K.; Cerci, D. Sunar; Tali, B.; Topakli, H.; Vergili, M.] Cukurova Univ, Adana, Turkey. [Akin, I. V.; Bilin, B.; Bilmis, S.; Gamsizkan, H.; Karapinar, G.; Ocalan, K.; Surat, U. E.; Yalvac, M.; Zeyrek, M.] Middle E Tech Univ, Dept Phys, TR-06531 Ankara, Turkey. [Gulmez, E.; Isildak, B.; Kaya, M.; Kaya, O.] Bogazici Univ, Istanbul, Turkey. [Bahtiyar, H.; Barlas, E.; Cankocak, K.; Vardarli, F. I.; Yucel, M.] Istanbul Tech Univ, TR-80626 Istanbul, Turkey. [Levchuk, L.; Sorokin, P.] Kharkov Phys & Technol Inst, Natl Sci Ctr, UA-310108 Kharkov, Ukraine. [Brooke, J. J.; Clement, E.; Cussans, D.; Flacher, H.; Frazier, R.; Goldstein, J.; Grimes, M.; Heath, G. P.; Heath, H. F.; Jacob, J.; Kreczko, L.; Lucas, C.; Meng, Z.; Newbold, D. M.; Paramesvaran, S.; Poll, A.; Senkin, S.; Smith, V. J.; Williams, T.] Univ Bristol, Bristol, Avon, England. [Newbold, D. M.; Brew, C.; Brown, R. M.; Cockerill, D. J. A.; Coughlan, J. A.; Harder, K.; Harper, S.; Olaiya, E.; Petyt, D.; Shepherd-Themistocleous, C. H.; Thea, A.; Tomalin, I. R.; Womersley, W. J.; Worm, S. D.; Lucas, R.] Rutherford Appleton Lab, Didcot OX11 0QX, Oxon, England. [Baber, M.; Bainbridge, R.; Buchmuller, O.; Burton, D.; Colling, D.; Cripps, N.; Cutajar, M.; Dauncey, P.; Davies, G.; Della Negra, M.; Dunne, P.; Ferguson, W.; Fulcher, J.; Futyan, D.; Gilbert, A.; Hall, G.; Iles, G.; Jarvis, M.; Karapostoli, G.; Kenzie, M.; Lane, R.; Lucas, R.; Lyons, L.; Magnan, A. -M.; Malik, S.; Mathias, B.; Nash, J.; Nikitenko, A.; Pela, J.; Pesaresi, M.; Petridis, K.; Raymond, D. M.; Rogerson, S.; Rose, A.; Seez, C.; Sharp, P.; Tapper, A.; Acosta, M. Vazquez; Virdee, T.] Univ London Imperial Coll Sci Technol & Med, London, England. [Cole, J. E.; Hobson, P. R.; Khan, A.; Kyberd, P.; Leggat, D.; Leslie, D.; Martin, W.; Reid, I. D.; Symonds, P.; Teodorescu, L.; Turner, M.] Brunel Univ, Uxbridge UB8 3PH, Middx, England. [Dittmann, J.; Hatakeyama, K.; Kasmi, A.; Liu, H.; Scarborough, T.] Baylor Univ, Waco, TX 76798 USA. [Charaf, O.; Cooper, S. I.; Henderson, C.; Rumerio, P.] Univ Alabama, Tuscaloosa, AL USA. [Avetisyan, A.; Bose, T.; Fantasia, C.; Heister, A.; Lawson, P.; Richardson, C.; Rohlf, J.; Sperka, D.; St John, J.; Sulak, L.] Boston Univ, Boston, MA 02215 USA. [Alimena, J.; Berry, E.; Bhattacharya, S.; Christopher, G.; Cutts, D.; Demiragli, Z.; Ferapontov, A.; Garabedian, A.; Heintz, U.; Jabeen, S.; Kukartsev, G.; Laird, E.; Landsberg, G.; Luk, M.; Narain, M.; Segala, M.; Sinthuprasith, T.; Speer, T.; Swanson, J.] Brown Univ, Providence, RI 02912 USA. [Breedon, R.; Breto, G.; Sanchez, M. Calderon De La Barca; Chauhan, S.; Chertok, M.; Conway, J.; Conway, R.; Cox, P. T.; Erbacher, R.; Gardner, M.; Ko, W.; Lander, R.; Miceli, T.; Mulhearn, M.; Pellett, D.; Pilot, J.; Ricci-Tam, F.; Searle, M.; Shalhout, S.; Smith, J.; Squires, M.; Stolp, D.; Tripathi, M.; Wilbur, S.; Yohay, R.] Univ Calif Davis, Davis, CA 95616 USA. [Cousins, R.; Everaerts, P.; Farrell, C.; Hauser, J.; Ignatenko, M.; Rakness, G.; Takasugi, E.; Valuev, V.; Weber, M.] Univ Calif Los Angeles, Los Angeles, CA USA. [Babb, J.; Burt, K.; Clare, R.; Ellison, J.; Gary, J. W.; Hanson, G.; Heilman, J.; IvovaRikova, M.; Jandir, P.; Kennedy, E.; Lacroix, F.; Liu, H.; Long, O. R.; Luthra, A.; Malberti, M.; Nguyen, H.; Shrinivas, A.; Sumowidagdo, S.; Wimpenny, S.] Univ Calif Riverside, Riverside, CA 92521 USA. [Abdulsalam, A.; Barge, D.; Bradmiller-Feld, J.; Campagnari, C.; Danielson, T.; Dishaw, A.; Flowers, K.; Sevilla, M. Franco; Geffert, P.; George, C.; Golf, F.; Gouskos, L.; Incandela, J.; Justus, C.; Mccoll, N.; Richman, J.; Stuart, D.; To, W.; West, C.] Univ Calif Santa Barbara, Santa Barbara, CA 93106 USA. [Dias, F. A.; Dubinin, M.; Apresyan, A.; Bornheim, A.; Bunn, J.; Chen, Y.; Di Marco, E.; Duarte, J.; Mott, A.; Newman, H. B.; Pena, C.; Rogan, C.; Spiropulu, M.; Timciuc, V.; Wilkinson, R.; Xie, S.; Zhu, R. Y.] CALTECH, Pasadena, CA USA. [Azzolini, V.; Calamba, A.; Ferguson, T.; Iiyama, Y.; Paulini, M.; Russ, J.; Vogel, H.; Vorobiev, I.] Carnegie Mellon Univ, Pittsburgh, PA 15213 USA. [Cumalat, J. P.; Drell, B. R.; Ford, W. T.; Gaz, A.; Lopez, E. Luiggi; Nauenberg, U.; Smith, J. G.; Stenson, K.; Ulmer, K. A.; Wagner, S. R.] Univ Colorado, Boulder, CO 80309 USA. [Alexander, J.; Chatterjee, A.; Chu, J.; Dittmer, S.; Eggert, N.; Mirman, N.; Kaufman, G. Nicolas; Patterson, J. R.; Ryd, A.; Salvati, E.; Skinnari, L.; Sun, W.; Teo, W. D.; Thom, J.; Thompson, J.; Tucker, J.; Weng, Y.; Winstrom, L.; Wittich, P.] Cornell Univ, Ithaca, NY USA. [Winn, D.] Fairfield Univ, Fairfield, CT 06430 USA. [Abdullin, S.; Albrow, M.; Anderson, J.; Apollinari, G.; Bauerdick, L. A. T.; Beretvas, A.; Berryhill, J.; Bhat, P. C.; Burkett, K.; Butler, J. N.; Cheung, H. W. K.; Chlebana, F.; Cihangir, S.; Elvira, V. D.; Fisk, I.; Freeman, J.; Gao, Y.; Gottschalk, E.; Gray, L.; Green, D.; Gruenendahl, S.; Gutsche, O.; Hanlon, J.; Hare, D.; Harris, R. M.; Hirschauer, J.; Hooberman, B.; Jindariani, S.; Johnson, M.; Joshi, U.; Kaadze, K.; Klima, B.; Kreis, B.; Kwan, S.; Linacre, J.; Lincoln, D.; Lipton, R.; Liu, T.; Lykken, J.; Maeshima, K.; Marraffino, J. M.; Outschoorn, V. I. Martinez; Maruyama, S.; Mason, D.; McBride, P.; Mishra, K.; Mrenna, S.; Musienko, Y.; Nahn, S.; Newman-Holmes, C.; O'Dell, V.; Prokofyev, O.; Sexton-Kennedy, E.; Sharma, S.; Soha, A.; Spalding, W. J.; Spiegel, L.; Taylor, L.; Tkaczyk, S.; Tran, N. V.; Uplegger, L.; Vaandering, E. W.; Vidal, R.; Whitbeck, A.; Whitmore, J.; Yang, F.] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA. [Acosta, D.; Avery, P.; Bourilkov, D.; Carver, M.; Cheng, T.; Curry, D.; Das, S.; De Gruttola, M.; Di Giovanni, G. P.; Field, R. D.; Fisher, M.; Furic, I. K.; Hugon, J.; Konigsberg, J.; Korytov, A.; Kypreos, T.; Low, J. F.; Matchev, K.; Milenovic, P.; Mitselmakher, G.; Muniz, L.; Rinkevicius, A.; Shchutska, L.; Skhirtladze, N.; Snowball, M.; Yelton, J.; Zakaria, M.] Univ Florida, Gainesville, FL USA. [Hewamanage, S.; Linn, S.; Markowitz, P.; Martinez, G.; Rodriguez, J. L.] Florida Int Univ, Miami, FL 33199 USA. [Adams, T.; Askew, A.; Bochenek, J.; Diamond, B.; Haas, J.; Hagopian, S.; Hagopian, V.; Johnson, K. F.; Prosper, H.; Veeraraghavan, V.; Weinberg, M.] Florida State Univ, Tallahassee, FL 32306 USA. [Baarmand, M. M.; Hohlmann, M.; Kalakhety, H.; Yumiceva, F.] Florida Inst Technol, Melbourne, FL 32901 USA. [Adams, M. R.; Apanasevich, L.; Bazterra, V. E.; Berry, D.; Betts, R. R.; Bucinskaite, I.; Cavanaugh, R.; Evdokimov, O.; Gauthier, L.; Gerber, C. E.; Hofman, D. J.; Khalatyan, S.; Kurt, P.; Moon, D. H.; O'Brien, C.; Silkworth, C.; Turner, P.; Varelas, N.] Univ Illinois, Chico, CA USA. [Albayrak, E. A.; Bilki, B.; Clarida, W.; Dilsiz, K.; Duru, F.; Haytmyradov, M.; Merlo, J. -P.; Mermerkaya, H.; Mestvirishvili, A.; Moeller, A.; Nachtman, J.; Ogul, H.; Onel, Y.; Ozok, F.; Penzo, A.; Rahmat, R.; Sen, S.; Tan, P.; Tiras, E.; Wetzel, J.; Yetkin, T.; Yi, K.] Univ Iowa, Iowa City, IA USA. [Sibille, J.; Barnett, B. A.; Blumenfeld, B.; Bolognesi, S.; Fehling, D.; Gritsan, A. V.; Maksimovic, P.; Martin, C.; Swartz, M.] Univ Kansas, Lawrence, KS 66045 USA. [Barfuss, A. F.; Chakaberia, I.; Ivanov, A.; Khalil, S.; Makouski, M.; Maravin, Y.; Saini, L. K.; Shrestha, S.; Svintradze, I.] Kansas State Univ, Manhattan, KS 66506 USA. [Gronberg, J.; Lange, D.; Rebassoo, F.; Wright, D.] Lawrence Livermore Natl Lab, Livermore, CA USA. [Baden, A.; Calvert, B.; Eno, S. C.; Gomez, J. A.; Hadley, N. J.; Kellogg, R. G.; Kolberg, T.; Lu, Y.; Marionneau, M.; Mignerey, A. C.; Pedro, K.; Skuja, A.; Tonjes, M. B.; Tonwar, S. C.] Univ Maryland, College Pk, MD 20742 USA. [Apyan, A.; Barbieri, R.; Bauer, G.; Busza, W.; Cali, I. A.; Chan, M.; Di Matteo, L.; Dutta, V.; Ceballos, G. Gomez; Goncharov, M.; Gulhan, D.; Klute, M.; Lai, Y. S.; Lee, Y. -J.; Levin, A.; Luckey, P. D.; Ma, T.; Paus, C.; Ralph, D.; Roland, C.; Roland, G.; Stephans, G. S. F.; Stoeckli, F.; Sumorok, K.; Velicanu, D.; Veverka, J.; Wyslouch, B.; Yang, M.; Zanetti, M.; Zhukova, V.] MIT, Cambridge, MA 02139 USA. [Dahmes, B.; Gude, A.; Kao, S. C.; Klapoetke, K.; Kubota, Y.; Mans, J.; Pastika, N.; Rusack, R.; Singovsky, A.; Tambe, N.; Turkewitz, J.] Univ Minnesota, Minneapolis, MN USA. [Acosta, J. G.; Oliveros, S.] Univ Mississippi, Oxford, MS USA. [Avdeeva, E.; Bloom, K.; Bose, S.; Claes, D. R.; Dominguez, A.; Suarez, R. Gonzalez; Keller, J.; Knowlton, D.; Kravchenko, I.; Lazo-Flores, J.; Malik, S.; Meier, F.; Snow, G. R.] Univ Nebraska, Lincoln, NE USA. [Dolen, J.; Godshalk, A.; Iashvili, I.; Kharchilava, A.; Kumar, A.; Rappoccio, S.] SUNY Buffalo, Buffalo, NY 14260 USA. 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[Heredia-de La Cruz, I.] Univ Michoacana, Morelia, Michoacan, Mexico. [Kim, V.] St Petersburg State Polytech Univ, St Petersburg, Russia. [Colafranceschi, S.] Univ Rome, Fac Ingn, Rome, Italy. [Rolandi, G.] Ist Nazl Fis Nucl, Scuola Normale & Sez, Pisa, Italy. [Amsler, C.] Albert Einstein Ctr Fundamental Phys, Bern, Switzerland. [Bakirci, M. N.; Ozturk, S.; Topakli, H.] Gaziosmanpasa Univ, Tokat, Turkey. [Cerci, S.; Cerci, D. Sunar; Tali, B.] Adiyaman Univ, Adiyaman, Turkey. [Onengut, G.] Cag Univ, Mersin, Turkey. [Sogut, K.] Mersin Univ, Mersin, Turkey. [Karapinar, G.] Izmir Inst Technol, Izmir, Turkey. [Isildak, B.] Ozyegin Univ, Istanbul, Turkey. [Kaya, M.; Kaya, O.] Kafkas Univ, Kars, Turkey. [Bahtiyar, H.; Albayrak, E. A.; Ozok, F.] Mimar Sinan Univ, Istanbul, Turkey. [Brown, R. M.] Univ Southampton, Sch Phys & Astron, Southampton, Hants, England. [Bilki, B.] Argonne Natl Lab, Argonne, IL 60439 USA. [Mermerkaya, H.] Erzincan Univ, Erzincan, Turkey. [Yetkin, T.] Yildiz Tekn Univ, Istanbul, Turkey. [Bouhali, O.] Texas A&M Univ Qatar, Doha, Qatar. RP Khachatryan, V (reprint author), Yerevan Phys Inst, Yerevan 375036, Armenia. RI Trocsanyi, Zoltan/A-5598-2009; Montanari, Alessandro/J-2420-2012; Hernandez Calama, Jose Maria/H-9127-2015; ciocci, maria agnese /I-2153-2015; My, Salvatore/I-5160-2015; Lo Vetere, Maurizio/J-5049-2012; Ragazzi, Stefano/D-2463-2009; Rovelli, Tiziano/K-4432-2015; Dremin, Igor/K-8053-2015; Hoorani, Hafeez/D-1791-2013; Leonidov, Andrey/M-4440-2013; Andreev, Vladimir/M-8665-2015; Haj Ahmad, Wael/E-6738-2016; Konecki, Marcin/G-4164-2015; Xie, Si/O-6830-2016; Leonardo, Nuno/M-6940-2016; Goh, Junghwan/Q-3720-2016; Ruiz, Alberto/E-4473-2011; Govoni, Pietro/K-9619-2016; Tuominen, Eija/A-5288-2017; Yazgan, Efe/C-4521-2014; Paulini, Manfred/N-7794-2014; Inst. of Physics, Gleb Wataghin/A-9780-2017; Chinellato, Jose Augusto/I-7972-2012; Leonidov, Andrey/P-3197-2014; Benussi, Luigi/O-9684-2014; Petrushanko, Sergey/D-6880-2012; Bernardes, Cesar Augusto/D-2408-2015; Raidal, Martti/F-4436-2012; Calderon, Alicia/K-3658-2014; VARDARLI, Fuat Ilkehan/B-6360-2013; Sen, Sercan/C-6473-2014; Wulz, Claudia-Elisabeth/H-5657-2011; Belyaev, Alexander/F-6637-2015; Stahl, Achim/E-8846-2011; Della Ricca, Giuseppe/B-6826-2013; Tomei, Thiago/E-7091-2012; Dubinin, Mikhail/I-3942-2016; Kirakosyan, Martin/N-2701-2015; Gulmez, Erhan/P-9518-2015; Tinoco Mendes, Andre David/D-4314-2011; Vilela Pereira, Antonio/L-4142-2016; Sznajder, Andre/L-1621-2016; Da Silveira, Gustavo Gil/N-7279-2014; Mundim, Luiz/A-1291-2012; Ozdemir, Kadri/P-8058-2014; da Cruz e Silva, Cristovao/K-7229-2013; vilar, rocio/P-8480-2014; Grandi, Claudio/B-5654-2015; Gonzalez Caballero, Isidro/E-7350-2010; Lokhtin, Igor/D-7004-2012; Manganote, Edmilson/K-8251-2013; Codispoti, Giuseppe/F-6574-2014; Yazgan, Efe/A-4915-2015; Scodellaro, Luca/K-9091-2014; Cerrada, Marcos/J-6934-2014; Dahms, Torsten/A-8453-2015; Ferguson, Thomas/O-3444-2014; Cakir, Altan/P-1024-2015; Matorras, Francisco/I-4983-2015; TUVE', Cristina/P-3933-2015; Dudko, Lev/D-7127-2012; KIM, Tae Jeong/P-7848-2015; Paganoni, Marco/A-4235-2016; Azarkin, Maxim/N-2578-2015; de Jesus Damiao, Dilson/G-6218-2012; Calvo Alamillo, Enrique/L-1203-2014; Flix, Josep/G-5414-2012; Perez-Calero Yzquierdo, Antonio/F-2235-2013; Novaes, Sergio/D-3532-2012 OI Trocsanyi, Zoltan/0000-0002-2129-1279; Montanari, Alessandro/0000-0003-2748-6373; Hernandez Calama, Jose Maria/0000-0001-6436-7547; ciocci, maria agnese /0000-0003-0002-5462; My, Salvatore/0000-0002-9938-2680; Lo Vetere, Maurizio/0000-0002-6520-4480; Ragazzi, Stefano/0000-0001-8219-2074; Rovelli, Tiziano/0000-0002-9746-4842; Haj Ahmad, Wael/0000-0003-1491-0446; Konecki, Marcin/0000-0001-9482-4841; Xie, Si/0000-0003-2509-5731; Leonardo, Nuno/0000-0002-9746-4594; Goh, Junghwan/0000-0002-1129-2083; Ruiz, Alberto/0000-0002-3639-0368; Govoni, Pietro/0000-0002-0227-1301; Tuominen, Eija/0000-0002-7073-7767; Yazgan, Efe/0000-0001-5732-7950; Paulini, Manfred/0000-0002-6714-5787; Chinellato, Jose Augusto/0000-0002-3240-6270; Benussi, Luigi/0000-0002-2363-8889; Sen, Sercan/0000-0001-7325-1087; Wulz, Claudia-Elisabeth/0000-0001-9226-5812; Belyaev, Alexander/0000-0002-1733-4408; Stahl, Achim/0000-0002-8369-7506; Della Ricca, Giuseppe/0000-0003-2831-6982; Tomei, Thiago/0000-0002-1809-5226; Dubinin, Mikhail/0000-0002-7766-7175; Gulmez, Erhan/0000-0002-6353-518X; Tinoco Mendes, Andre David/0000-0001-5854-7699; Vilela Pereira, Antonio/0000-0003-3177-4626; Sznajder, Andre/0000-0001-6998-1108; Da Silveira, Gustavo Gil/0000-0003-3514-7056; Mundim, Luiz/0000-0001-9964-7805; Ozdemir, Kadri/0000-0002-0103-1488; Grandi, Claudio/0000-0001-5998-3070; Gonzalez Caballero, Isidro/0000-0002-8087-3199; Codispoti, Giuseppe/0000-0003-0217-7021; Scodellaro, Luca/0000-0002-4974-8330; Cerrada, Marcos/0000-0003-0112-1691; Dahms, Torsten/0000-0003-4274-5476; Ferguson, Thomas/0000-0001-5822-3731; Matorras, Francisco/0000-0003-4295-5668; TUVE', Cristina/0000-0003-0739-3153; Dudko, Lev/0000-0002-4462-3192; KIM, Tae Jeong/0000-0001-8336-2434; Paganoni, Marco/0000-0003-2461-275X; de Jesus Damiao, Dilson/0000-0002-3769-1680; Calvo Alamillo, Enrique/0000-0002-1100-2963; Flix, Josep/0000-0003-2688-8047; Perez-Calero Yzquierdo, Antonio/0000-0003-3036-7965; Novaes, Sergio/0000-0003-0471-8549 FU BMWFW (Austria); FWF (Austria); FNRS (Belgium); FWO (Belgium); CNPq (Brazil); CAPES (Brazil); FAPERJ (Brazil); FAPESP (Brazil); MES (Bulgaria); CERN (China); CAS (China); MoST (China); NSFC (China); COLCIENCIAS (Colombia); MSES (Croatia); CSF (Croatia); RPF (Cyprus); ERDF (Estonia); MoER (Estonia); ERC IUT (Estonia); Academy of Finland (Finland); MEC (Finland); HIP (Finland); CEA(France); CNRS/IN2P3 (France); BMBF (Germany); DFG (Germany); HGF (Germany); GSRT (Greece); OTKA (Hungary); NIH (Hungary); DAE (India); DST (India); IPM (Iran); SFI (Ireland); INFN (Italy); NRF (Republic of Korea); WCU (Republic of Korea); LAS (Lithuania); MOE (Malaysia); UM (Malaysia); CINVESTAV (Mexico); CONACYT (Mexico); SEP (Mexico); UASLP-FAI (Mexico); MBIE (New Zealand); PAEC (Pakistan); MSHE (Poland); NSC (Poland); FCT (Portugal); JINR (Dubna); MON (Russia); RosAtom (Russia); RAS (Russia); RFBR (Russia); MESTD (Serbia); SEIDI (Spain); CPAN (Spain); Swiss Funding Agencies (Switzerland); MST (Taipei); ThEPCenter (Thailand); IPST (Thailand); STAR (Thailand); NSTDA (Thailand); TUBITAK (Turkey); TAEK (Turkey); NASU (Ukraine); SFFR (Ukraine); STFC (United Kingdom); DOE (USA); NSF (USA) FX We thank Debajyoti Choudhury for inspiring this work and continuing to provide theoretical insight throughout its course. We congratulate our colleagues in the CERN accelerator departments for the excellent performance of the LHC and thank the technical and administrative staffs at CERN and at other CMS institutes for their contributions to the success of the CMS effort. In addition, we gratefully acknowledge the computing centres and personnel of the Worldwide LHC Computing Grid for delivering so effectively the computing infrastructure essential to our analyses. Finally, we acknowledge the enduring support for the construction and operation of the LHC and the CMS detector provided by the following funding agencies: BMWFW and FWF (Austria); FNRS and FWO (Belgium); CNPq, CAPES, FAPERJ, and FAPESP (Brazil); MES (Bulgaria); CERN; CAS, MoST, and NSFC (China); COLCIENCIAS (Colombia); MSES and CSF (Croatia); RPF (Cyprus); MoER, ERC IUT and ERDF (Estonia); Academy of Finland, MEC, and HIP (Finland); CEA and CNRS/IN2P3 (France); BMBF, DFG, and HGF (Germany); GSRT (Greece); OTKA and NIH (Hungary); DAE and DST (India); IPM (Iran); SFI (Ireland); INFN (Italy); NRF and WCU (Republic of Korea); LAS (Lithuania); MOE and UM (Malaysia); CINVESTAV, CONACYT, SEP, and UASLP-FAI (Mexico); MBIE (New Zealand); PAEC (Pakistan); MSHE and NSC (Poland); FCT (Portugal); JINR (Dubna); MON, RosAtom, RAS and RFBR (Russia); MESTD (Serbia); SEIDI and CPAN (Spain); Swiss Funding Agencies (Switzerland); MST (Taipei); ThEPCenter, IPST, STAR and NSTDA (Thailand); TUBITAK and TAEK (Turkey); NASU and SFFR (Ukraine); STFC (United Kingdom); DOE and NSF (USA). NR 38 TC 16 Z9 17 U1 9 U2 69 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0370-2693 EI 1873-2445 J9 PHYS LETT B JI Phys. Lett. B PD NOV 10 PY 2014 VL 738 BP 274 EP 293 DI 10.1016/j.physletb.2014.09.048 PG 20 WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AT0KK UT WOS:000344624900043 ER PT J AU Abelev, B Adam, J Adamova, D Aggarwal, MM Agnello, M Agostinelli, A Agrawal, N Ahammed, Z Ahmad, N Ahmed, I Ahn, SU Ahn, SA Aimo, I Aiola, S Ajaz, M Akindinov, A Alam, SN Aleksandrov, D Alessandro, B Alexandre, D Alici, A Alkin, A Alme, J Alt, T Altinpinar, S Altsybeev, I Prado, CAG Andrei, C Andronic, A Anguelov, V Anielski, J Anticic, T Antinori, F Antonioli, P Aphecetche, L Appelshauser, H Arcelli, S Armesto, N Arnaldi, R Aronsson, T Arsene, IC Arslandok, M Augustinus, A Averbeck, R Awes, TC Azmi, MD Bach, M Badala, A Baek, YW Bagnasco, S Bailhache, R Bala, R Baldisseri, A Pedrosa, FBD Baral, RC Barbera, R Barile, F Barnaflodi, GG Barnby, LS Barret, V Bartke, J Basile, M Bastid, N Basu, S Bathen, B Batigne, G Batyunya, B Batzing, PC Baumann, C 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W. van Leeuwen, M. Vargas, A. Vargyas, M. Varma, R. Vasileiou, M. Vasiliev, A. Vechernin, V. Veldhoen, M. Velure, A. Venaruzzo, M. Vercellin, E. Limon, S. Vergara Vernet, R. Vickovic, L. Viesti, G. Viinikainen, J. Vilakazi, Z. Baillie, O. Villalobos Vinogradov, A. Vinogradov, L. Vinogradov, Y. Virgili, T. Viyogi, Y. P. Vodopyanov, A. Voelkl, M. A. Voloshin, K. Voloshin, S. A. Volpe, G. von Haller, B. Vorobyev, I. Vranic, D. Vrlakova, J. Vulpescu, B. Vyushin, A. Wagner, B. Wagner, J. Wagner, V. Wang, M. Wang, Y. Watanabe, D. Weber, M. Weber, S. G. Wessels, J. P. Westerhoff, U. Wiechula, J. Wikne, J. Wilde, M. Wilk, G. Wilkinson, J. Williams, M. C. S. Windelband, B. Winn, M. Yaldo, C. G. Yamaguchi, Y. Yang, H. Yang, P. Yang, S. Yano, S. Yasnopolskiy, S. Yi, J. Yin, Z. Yoo, I. -K. Yushmanov, I. Zaccolo, V. Zach, C. Zaman, A. Zampolli, C. Zaporozhets, S. Zarochentsev, A. Zavada, P. Zaviyalov, N. Zbroszczyk, H. Zgura, I. S. Zhalov, M. Zhang, H. Zhang, X. Zhang, Y. Zhao, C. Zhigareva, N. Zhou, D. Zhou, F. Zhou, Y. Zhou, Zhuo Zhu, H. Zhu, J. Zhu, X. Zichichi, A. Zimmermann, A. Zimmermann, M. B. Zinovjev, G. Zoccarato, Y. Zyzak, M. CA ALICE Collaboration TI Suppression of Upsilon(1S) at forward rapidity in Pb-Pb collisions at root s(NN)=2.76 TeV SO PHYSICS LETTERS B LA English DT Article ID QUARK-GLUON PLASMA; J/PSI SUPPRESSION; NUCLEON; PSI' AB We report on the measurement of the inclusive Upsilon(1S) production in Pb-Pb collisions at root s(NN) = 2.76 TeV carried out at forward rapidity (2.5 < y < 4) and down to zero transverse momentum using its mu(+)mu(-) decay channel with the ALICE detector at the Large Hadron Collider. Astrong suppression of the inclusive Upsilon(1S) yield is observed with respect to pp collisions scaled by the number of independent nucleo-nnucleon collisions. The nuclear modification factor, for events in the 0-90% centrality range, amounts to 0.30 +/- 0.05(stat) +/- 0.04(syst). 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[Bartke, J.; Figiel, J.; Gladysz-Dziadus, E.; Gorlich, L.; Kowalski, M.; Matyja, A.; Mayer, C.; Rybicki, A.; Sputowska, I.] Polish Acad Sci, Henryk Niewodniczanski Inst Nucl Phys, Krakow, Poland. [Knospe, A. G.; Markert, C.] Univ Texas Austin, Dept Phys, Austin, TX 78712 USA. [Monzon, I. Leon; Podesta-Lerma, P. L. M.; Rodriguez, F. J. Sanchez] Univ Autonoma Sinaloa, Culiacan, Mexico. [Prado, C. Alves Garcia; Bregant, M.; Cosentino, M. R.; Gimenez, D. Domenicis; Jahnke, C.; Fernandes, C. Lagana; De Godoy, D. A. Moreira; Munhoz, M. G.; Da Silva, A. C. Oliveira; Pereira De Oliveira Filho, E.; Suaide, A. A. P.; Szanto de Toledo, A.] Univ Sao Paulo, BR-09500900 Sao Paulo, Brazil. [Chinellato, D. D.; Dash, A.; Takahashi, J.] Univ Estadual Campinas, Campinas, SP, Brazil. [Bellwied, R.; Chinellato, D. D.; Jayarathna, P. H. S. Y.; Jena, S.; Pinsky, L.; Piyarathna, D. B.; Timmins, A. R.; Weber, M.] Univ Houston, Houston, TX USA. [Chang, B.; Kim, D. J.; Kral, J.; Rak, J.; Trzaska, W. 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[Keidel, R.] ZTT, Worms, Germany. [Berdnikov, Y.] St Petersburg State Polytech Univ, St Petersburg, Russia. [Khan, M. M.] Aligarh Muslim Univ, Dept Appl Phys, Aligarh, Uttar Pradesh, India. [Iv, L. Malinina] Moscow MV Lomonosov State Univ, DV Skobeltsyn Inst Nucl Phys, Moscow, Russia. [Milosevic, J.] Univ Belgrade, Fac Phys, Belgrade 11001, Serbia. [Milosevic, J.] Vinca Inst Nucl Sci, Belgrade 11001, Serbia. [Redlich, K.; Takaki, J. D. Tapia] Univ Wroclaw, Inst Theoret Phys, PL-50138 Wroclaw, Poland. [Takaki, J. D. Tapia] Univ Kansas, Lawrence, KS 66045 USA. RP Abelev, B (reprint author), Lawrence Livermore Natl Lab, Livermore, CA 94550 USA. RI Armesto, Nestor/C-4341-2017; Ferretti, Alessandro/F-4856-2013; Martinez Hernandez, Mario Ivan/F-4083-2010; Vickovic, Linda/F-3517-2017; Fernandez Tellez, Arturo/E-9700-2017; Kovalenko, Vladimir/C-5709-2013; Sevcenco, Adrian/C-1832-2012; Takahashi, Jun/B-2946-2012; Felea, Daniel/C-1885-2012; Kucera, Vit/G-8459-2014; Krizek, Filip/G-8967-2014; Bielcikova, Jana/G-9342-2014; Vajzer, Michal/G-8469-2014; Wagner, Vladimir/G-5650-2014; Sumbera, Michal/O-7497-2014; Peitzmann, Thomas/K-2206-2012; Kharlov, Yuri/D-2700-2015; Mitu, Ciprian/E-6733-2011; Ahmed, Ijaz/E-9144-2015; Usai, Gianluca/E-9604-2015; Salgado, Carlos A./G-2168-2015; Bregant, Marco/I-7663-2012; Barnby, Lee/G-2135-2010; Barbera, Roberto/G-5805-2012; Bruna, Elena/C-4939-2014; Karasu Uysal, Ayben/K-3981-2015; HAMAGAKI, HIDEKI/G-4899-2014; Pshenichnov, Igor/A-4063-2008; Guber, Fedor/I-4271-2013; Zarochentsev, Andrey/J-6253-2013; Altsybeev, Igor/K-6687-2013; Vinogradov, Leonid/K-3047-2013; Kondratiev, Valery/J-8574-2013; Vechernin, Vladimir/J-5832-2013; Janik, Malgorzata/O-7520-2015; Graczykowski, Lukasz/O-7522-2015; feofilov, grigory/A-2549-2013; Adamova, Dagmar/G-9789-2014; Christensen, Christian/D-6461-2012; De Pasquale, Salvatore/B-9165-2008; Chinellato, David/D-3092-2012; de Cuveland, Jan/H-6454-2016; Kurepin, Alexey/H-4852-2013; Jena, Deepika/P-2873-2015; Jena, Satyajit/P-2409-2015; Akindinov, Alexander/J-2674-2016; Nattrass, Christine/J-6752-2016; Cosentino, Mauro/L-2418-2014; Suaide, Alexandre/L-6239-2016; Castillo Castellanos, Javier/G-8915-2013; Inst. of Physics, Gleb Wataghin/A-9780-2017; Ferreiro, Elena/C-3797-2017 OI Armesto, Nestor/0000-0003-0940-0783; Ferretti, Alessandro/0000-0001-9084-5784; Martinez Hernandez, Mario Ivan/0000-0002-8503-3009; Vickovic, Linda/0000-0002-9820-7960; Fernandez Tellez, Arturo/0000-0003-0152-4220; Kovalenko, Vladimir/0000-0001-6012-6615; Sevcenco, Adrian/0000-0002-4151-1056; Takahashi, Jun/0000-0002-4091-1779; Felea, Daniel/0000-0002-3734-9439; Sumbera, Michal/0000-0002-0639-7323; Peitzmann, Thomas/0000-0002-7116-899X; Usai, Gianluca/0000-0002-8659-8378; Salgado, Carlos A./0000-0003-4586-2758; Barnby, Lee/0000-0001-7357-9904; Barbera, Roberto/0000-0001-5971-6415; Bruna, Elena/0000-0001-5427-1461; Karasu Uysal, Ayben/0000-0001-6297-2532; Pshenichnov, Igor/0000-0003-1752-4524; Guber, Fedor/0000-0001-8790-3218; Zarochentsev, Andrey/0000-0002-3502-8084; Altsybeev, Igor/0000-0002-8079-7026; Vinogradov, Leonid/0000-0001-9247-6230; Kondratiev, Valery/0000-0002-0031-0741; Vechernin, Vladimir/0000-0003-1458-8055; Janik, Malgorzata/0000-0002-3356-3438; feofilov, grigory/0000-0003-3700-8623; Christensen, Christian/0000-0002-1850-0121; De Pasquale, Salvatore/0000-0001-9236-0748; Chinellato, David/0000-0002-9982-9577; de Cuveland, Jan/0000-0003-0455-1398; Kurepin, Alexey/0000-0002-1851-4136; Jena, Deepika/0000-0003-2112-0311; Jena, Satyajit/0000-0002-6220-6982; Akindinov, Alexander/0000-0002-7388-3022; Nattrass, Christine/0000-0002-8768-6468; Cosentino, Mauro/0000-0002-7880-8611; Suaide, Alexandre/0000-0003-2847-6556; Castillo Castellanos, Javier/0000-0002-5187-2779; Ferreiro, Elena/0000-0002-4449-2356 FU State Committee of Science; World Federation of Scientists (WFS); Swiss Fonds Kidagan, Armenia; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq); Financiadora de Estudos e Projetos (FINEP); Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP); National Natural Science Foundation of China (NSFC); Chinese Ministry of Education (CMOE); Ministry of Science and Technology of China (MSTC); Ministry of Education and Youth of the Czech Republic; Danish Natural Science Research Council; Carlsberg Foundation; Danish National Research Foundation; European Research Council under the European Community; Helsinki Institute of Physics; Academy of Finland; French CNRS-IN2P3; Region Pays de Loire; Region Alsace; Region Auvergne; CEA, France; German BMBF; Helmholtz Association; General Secretariat for Research and Technology, Greece; Ministry of Development, Greece; Hungarian OTKA; National Office for Research and Technology (NKTH); Department of Atomic Energy; Department of Science and Technology of the Government of India; Istituto Nazionale di Fisica Nucleare (INFN); Centro Fermi - Museo Storico della Fisica e Centro Studi e Ricerche "Enrico Fermi", Italy; MEXT, Japan; Joint Institute for Nuclear Research, Dubna; National Research Foundation of Korea (NRF); CONACYT; DGAPA Mexico; ALFA-EC; EPLANET Program (European Particle Physics Latin American Network); Stichting voor Fundamenteel Onderzoek der Materie (FOM); Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Netherlands; Research Council of Norway (NFR); Polish Ministry of Science and Higher Education; National Authority for Scientific Research - NASR (Autoritatea Nationala pentru Cercetare, Stiintifica-ANCS); Ministry of Education and Science of the Russian Federation; Russian Academy of Sciences; Russian Federal Agency of Atomic Energy; Russian Federal Agency for Science and Innovations; Russian Foundation for Basic Research; Ministry of Education of Slovakia; Department of Science and Technology, Republic of South Africa; CIEMAT, Cuba; EELA, Cuba; Ministerio de Economia y Competitividad (MINECO) of Spain; Xunta de Galicia (Conselleria de Educacion); CEADEN; Cubaenergia, Cuba; IAEA (International Atomic Energy Agency); Swedish Research Council (VR); Knut and Alice Wallenberg Foundation (KAW); Ukraine Ministry of Education and Science; United Kingdom Science and Technology Facilities Council (STFC); U.S. Department of Energy; United States National Science Foundation; State of Texas; State of Ohio FX The ALICE Collaboration acknowledges the following funding agencies for their support in building and running the ALICE detector: State Committee of Science, World Federation of Scientists (WFS) and Swiss Fonds Kidagan, Armenia, Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP); National Natural Science Foundation of China (NSFC), the Chinese Ministry of Education (CMOE) and the Ministry of Science and Technology of China (MSTC); Ministry of Education and Youth of the Czech Republic; Danish Natural Science Research Council, the Carlsberg Foundation and the Danish National Research Foundation; The European Research Council under the European Community's Seventh Framework Programme; Helsinki Institute of Physics and the Academy of Finland; French CNRS-IN2P3, the 'Region Pays de Loire', 'Region Alsace', 'Region Auvergne' and CEA, France; German BMBF and the Helmholtz Association; General Secretariat for Research and Technology, Ministry of Development, Greece; Hungarian OTKA and National Office for Research and Technology (NKTH); Department of Atomic Energy and Department of Science and Technology of the Government of India; Istituto Nazionale di Fisica Nucleare (INFN) and Centro Fermi - Museo Storico della Fisica e Centro Studi e Ricerche "Enrico Fermi", Italy; MEXT Grant-in-Aid for Specially Promoted Research, Japan; Joint Institute for Nuclear Research, Dubna; National Research Foundation of Korea (NRF); CONACYT, DGAPA, Mexico, ALFA-EC and the EPLANET Program (European Particle Physics Latin American Network); Stichting voor Fundamenteel Onderzoek der Materie (FOM) and the Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Netherlands; Research Council of Norway (NFR); Polish Ministry of Science and Higher Education; National Authority for Scientific Research - NASR (Autoritatea Nationala pentru Cercetare, Stiintifica-ANCS); Ministry of Education and Science of the Russian Federation, Russian Academy of Sciences, Russian Federal Agency of Atomic Energy, Russian Federal Agency for Science and Innovations and the Russian Foundation for Basic Research; Ministry of Education of Slovakia; Department of Science and Technology, Republic of South Africa; CIEMAT, EELA, Ministerio de Economia y Competitividad (MINECO) of Spain, Xunta de Galicia (Conselleria de Educacion), CEADEN, Cubaenergia, Cuba, and IAEA (International Atomic Energy Agency); Swedish Research Council (VR) and Knut and Alice Wallenberg Foundation (KAW); Ukraine Ministry of Education and Science; United Kingdom Science and Technology Facilities Council (STFC); The U.S. Department of Energy, the United States National Science Foundation, the State of Texas, and the State of Ohio. NR 52 TC 18 Z9 18 U1 1 U2 49 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0370-2693 EI 1873-2445 J9 PHYS LETT B JI Phys. Lett. B PD NOV 10 PY 2014 VL 738 BP 361 EP 372 DI 10.1016/j.physletb.2014.10.001 PG 12 WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AT0KK UT WOS:000344624900054 ER PT J AU Staszczak, A Wong, CY AF Staszczak, Andrzej Wong, Cheuk-Yin TI A region of high-spin toroidal isomers SO PHYSICS LETTERS B LA English DT Article DE Toroidal light nuclei; High-K isomeric states ID SKYRMES INTERACTION; ANGULAR-MOMENTUM; NUCLEI; FISSION; BUBBLE AB The combined considerations of both the bulk liquid-drop-type behavior and the quantized angular momentum reveal that high-spin toroidal isomeric states may have general occurrences for light nuclei with 28 <= A <= 52. High-spin N = Ztoroidal isomers in this mass region have been located theoretically using cranked self-consistent constraint Skyrme-Hartree-Fock model calculations. (C) 2014 The Authors. Published by Elsevier B. V. This is an open access article under the CC BY license (http://creativecommons. org/licenses/by/3.0/). Funded by SCOAP(3). C1 [Staszczak, Andrzej] Marie Curie Sklodowska Univ, Inst Phys, PL-20031 Lublin, Poland. [Wong, Cheuk-Yin] Oak Ridge Natl Lab, Div Phys, Oak Ridge, TN 37831 USA. RP Staszczak, A (reprint author), Marie Curie Sklodowska Univ, Inst Phys, Pl M Curie Sklodowskiej 1, PL-20031 Lublin, Poland. EM stas@tytan.umcs.lublin.pl; wongc@ornl.gov FU Division of Nuclear Physics, U.S. Department of Energy, U.S.A. [DE-AC05-00OR22725] FX The authors wish to thank Drs. Jerzy Dudek, Vince Cianciolo, and I-Yang Lee for helpful discussions. This work was supported in part by the Division of Nuclear Physics, U.S. Department of Energy, U.S.A., Contract No. DE-AC05-00OR22725. NR 23 TC 3 Z9 3 U1 0 U2 4 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0370-2693 EI 1873-2445 J9 PHYS LETT B JI Phys. Lett. B PD NOV 10 PY 2014 VL 738 BP 401 EP 404 DI 10.1016/j.physletb.2014.10.013 PG 4 WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AT0KK UT WOS:000344624900060 ER PT J AU Aad, G Abbott, B Abdallah, J Khalek, SA Abdinov, O Aben, R Abi, B Abolins, M AbouZeid, OS Abramowicz, H Abreu, H Abreu, R Abulaiti, Y Acharya, BS Adamczyk, L Adams, DL Adelman, J Adomeit, S Adye, T Agatonovic-Jovin, T Aguilar-Saavedra, JA Agustoni, M Ahlen, SP Ahmadov, F Aielli, G Akerstedt, H Akesson, TPA Akimoto, G Akimov, AV Alberghi, GL Albert, J Albrand, S Verzini, MJA Aleksa, M Aleksandrov, IN Alexa, C Alexander, G Alexandre, G Alexopoulos, T Alhroob, M Alimonti, G Alio, L Alison, J Allbrooke, BMM Allison, LJ Allport, PP Almond, J Aloisio, A Alonso, A Alonso, F Alpigiani, C Altheimer, A Gonzalez, BA Alviggi, MG Amako, K Coutinho, YA Amelung, C Amidei, D Dos Santos, SPA Amorim, A Amoroso, S Amram, N Amundsen, G Anastopoulos, C Ancu, LS Andari, N 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CA ATLAS Collaboration TI Search for new resonances in W gamma and Z gamma final states in pp collisions at root s=8 TeV with the ATLAS detector SO PHYSICS LETTERS B LA English DT Article ID PARTON DISTRIBUTIONS; DIMENSIONAL ANALYSIS; LHC; TECHNICOLOR; PARTICLE; BOSON AB This Letter presents a search for new resonances decaying to final states with a vector boson produced in association with a high transverse momentum photon, V gamma, with V = W(-> l nu) or Z(-> l(+)l(-)), where l = mu or mu. The measurements use 20.3fb(-1) of proton-proton collision data at a center-of-mass energy of root s = 8 TeV recorded with the ATLAS detector. No deviations from the Standard Model expectations are found, and production cross section limits are set at 95% confidence level. Masses of the hypothetical a(T) and omega(T) states of a benchmark Low Scale Technicolor model are excluded in the ranges [275, 960] GeV and [200, 700]boolean OR[750, 890] GeV, respectively. 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P.; Maidantchik, C.; Marroquim, F.; Nepomuceno, A. A.; Seixas, J. M.] Univ Fed Rio de Janeiro, COPPE, EE, IF, Rio De Janeiro, Brazil. [Cerqueira, A. S.; Manhaes de Andrade Filho, L.] Univ Fed Juiz de Fora, Juiz de Fora, Brazil. [do Vale, M. A. B.] Fed Univ Sao Joao Rei UFSJ, Sao Joao Del Rei, Brazil. [Donadelli, M.; Leite, M. A. L.] Univ Sao Paulo, Inst Fis, BR-01498 Sao Paulo, Brazil. [Adams, D. L.; Assamagan, K.; Begel, M.; Chen, H.; Chernyatin, V.; Debbe, R.; Ernst, M.; Gibbard, B.; Gordon, H. A.; Hu, X.; Klimentov, A.; Kravchenko, A.; Lanni, F.; Lissauer, D.; Lynn, D.; Ma, H.; Maeno, T.; Metcalfe, J.; Mountricha, E.; Nevski, P.; Okawa, H.; Damazio, D. Oliveira; Paige, F.; Panitkin, S.; Perepelitsa, D. V.; Pleier, M. -A.; Polychronakos, V.; Protopopescu, S.; Purohit, M.; Radeka, V.; Rajagopalan, S.; Redlinger, G.; Schovancova, J.; Snyder, S.; Steinberg, P.; Takai, H.; Undrus, A.; Wenaus, T.; Ye, S.] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. [Alexa, C.; Badescu, E.; Boldea, V.; Buda, S. I.; Caprini, I.; Caprini, M.; Chitan, A.; Ciubancan, M.; Constantinescu, S.; Cuciuc, C. -M.; Dita, P.; Dita, S.; Ducu, O. A.; Jinaru, A.; Maurer, J.; Olariu, A.; Pantea, D.; Popeneciu, G. A.; Rotaru, M.; Stoicea, G.; Tudorache, A.; Tudorache, V.] Natl Inst Phys & Nucl Engn, Bucharest, Romania. [Popeneciu, G. A.] Natl Inst Res & Dev Isotop & Mol Technol, Dept Phys, Cluj Napoca, Romania. Univ Politehn Bucuresti, Bucharest, Romania. West Univ Timisoara, Timisoara, Romania. [Otero y Garzon, G.; Piegaia, R.; Reisin, H.; Sacerdoti, S.] Univ Buenos Aires, Dept Fis, Buenos Aires, DF, Argentina. [Arratia, M.; Barlow, N.; Batley, J. R.; Brochu, F. M.; Buttinger, W.; Carter, J. R.; Chapman, J. D.; Cottin, G.; French, S. T.; Frost, J. A.; Gillam, T. P. S.; Hill, J. C.; Kaneti, S.; Khoo, T. J.; Lester, C. G.; Mueller, T.; Parker, M. A.; Robinson, D.; Sandoval, T.; Thomson, M.; Ward, C. P.; Williams, S.; Yusuff, I.] Univ Cambridge, Cavendish Lab, Cambridge CB3 0HE, England. [Bellerive, A.; Cree, G.; Di Valentino, D.; Koffas, T.; Lacey, J.; Leight, W. A.; Marchand, J. F.; McCarthy, T. G.; Nomidis, I.; Oakham, F. G.; Pasztor, G.; Tarrade, F.; Ueno, R.; Vincter, M. G.; Whalen, K.] Carleton Univ, Dept Phys, Ottawa, ON K1S 5B6, Canada. [Abreu, R.; Aleksa, M.; Andari, N.; Anders, G.; Anghinolfi, F.; Armbruster, A. J.; Arnaez, O.; Avolio, G.; Baak, M. A.; Backes, M.; Backhaus, M.; Battistin, M.; Beltramello, O.; Bianco, M.; Bogaerts, J. A.; Boyd, J.; Burckhart, H.; Campana, S.; Garrido, M. D. M. Capeans; Carli, T.; Catinaccio, A.; Cattai, A.; Cerv, M.; Chromek-Burckhart, D.; Dell'Acqua, A.; Di Girolamo, A.; Di Girolamo, B.; Dittus, F.; Dobos, D.; Dudarev, A.; Duehrssen, M.; Ellis, N.; Elsing, M.; Farthouat, P.; Fassnacht, P.; Feigl, S.; Perez, S. Fernandez; Franchino, S.; Francis, D.; Froidevaux, D.; Garonne, V.; Gianotti, F.; Gillberg, D.; Glatzer, J.; Godlewski, J.; Goossens, L.; Gorini, B.; Gray, H. M.; Hauschild, M.; Hawkings, R. J.; Heller, M.; Helsens, C.; Correia, A. M. Henriques; Hervas, L.; Hoecker, A.; Hubacek, Z.; Huhtinen, M.; Jaekel, M. R.; Jakobsen, S.; Jansen, H.; Jungst, R. M.; Kaneda, M.; Klioutchnikova, T.; Krasznahorkay, A.; Lantzsch, K.; Lassnig, M.; Miotto, G. Lehmann; Lenzi, B.; Lichard, P.; Macina, D.; Malyukov, S.; Mandelli, B.; Mapelli, L.; Martin, B.; Marzin, A.; Messina, A.; Meyer, J.; Milic, A.; Mornacchi, G.; Nairz, A. M.; Nakahama, Y.; Negri, G.; Nessi, M.; Nicquevert, B.; Nordberg, M.; Palestini, S.; Pauly, T.; Pernegger, H.; Peters, K.; Petersen, B. A.; Pommes, K.; Poppleton, A.; Poulard, G.; Prasad, S.; Rammensee, M.; Raymond, M.; Rembser, C.; Rodrigues, L.; Roe, S.; Ruiz-Martinez, A.; Salzburger, A.; Savu, D. O.; Schaefer, D.; Schlenker, S.; Schmieden, K.; Serfon, C.; Sfyrla, A.; Solans, C. A.; Spigo, G.; Stelzer, H. J.; Teischinger, F. A.; Ten Kate, H.; Tremblet, L.; Tricoli, A.; Tsarouchas, C.; Unal, G.; van der Ster, D.; van Eldik, N.; van Woerden, M. C.; Vandelli, W.; Vigne, R.; Voss, R.; Vuillermet, R.; Wells, P. S.; Wengler, T.; Wenig, S.; Werner, P.; Wilkens, H. G.; Wotschack, J.; Young, C. J. S.; Zwalinski, L.] CERN, Geneva, Switzerland. [Alison, J.; Anderson, K. J.; Boveia, A.; Cheng, Y.; Facini, G.; Fiascaris, M.; Gardner, R. W.; Ilchenko, Y.; Kapliy, A.; Li, H. L.; Meehan, S.; Melachrinos, C.; Merritt, F. S.; Miller, D. W.; Okumura, Y.; Onyisi, P. U. E.; Oreglia, M. J.; Penning, B.; Pilcher, J. E.; Shochet, M. J.; Tompkins, L.; Vukotic, I.; Webster, J. S.] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA. [Carquin, E.; Diaz, M. A.; Vogel, M.] Pontificia Univ Catolica Chile, Dept Fis, Santiago, Chile. [Brooks, W. K.; Kuleshov, S.; Pezoa, R.; Prokoshin, F.; White, R.] Univ Tecn Federico Santa Maria, Dept Fis, Valparaiso, Chile. [Bai, Y.; Fang, Y.; Jin, S.; Lu, F.; Ouyang, Q.; Ren, H.; Shan, L. Y.; Sun, X.; Wang, J.; Xu, D.; Yao, L.; Zhu, H.; Zhuang, X.] Chinese Acad Sci, Inst High Energy Phys, Beijing, Peoples R China. [Gao, J.; Guan, L.; Han, L.; Jiang, Y.; Li, B.; Liu, J. B.; Liu, K.; Liu, M.; Liu, Y.; Peng, H.; Song, H. Y.; Xu, L.; Zhao, Z.; Zhu, Y.] Univ Sci & Technol China, Dept Modern Phys, Hefei, Anhui, Peoples R China. [Chen, S.; Li, Y.; Wang, C.] Nanjing Univ, Dept Phys, Nanjing, Jiangsu, Peoples R China. [Chen, L.; Feng, C.; Ge, P.; Ma, L. L.; Zhang, X.; Zhu, C. G.] Shandong Univ, Sch Phys, Jinan, Shandong, Peoples R China. [Li, L.; Yang, H.] Shanghai Jiao Tong Univ, Dept Phys, Shanghai 200030, Peoples R China. [Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Donini, J.; Dubreuil, E.; Ghodbane, N.; Gilles, G.; Gris, Ph.; Guicheney, C.; Liao, H.; Pallin, D.; Hernandez, D. Paredes; Podlyski, F.; Santoni, C.; Theveneaux-Pelzer, T.; Valery, L.; Vazeille, F.] Clermont Univ, Phys Corpusculaire Lab, Clermont Ferrand, France. [Altheimer, A.; Andeen, T.; Angerami, A.; Bain, T.; Brooijmans, G.; Chen, Y.; Cole, B.; Guo, J.; Hu, D.; Hughes, E. W.; Mohapatra, S.; Nikiforou, N.; Parsons, J. A.; Reale, V. Perez; Scherzer, M. I.; Thompson, E. N.; Tian, F.; Tuts, P. M.; Urbaniec, D.; Wulf, E.; Zhou, L.] Columbia Univ, Nevis Lab, Irvington, NY USA. [Alonso, A.; Dam, M.; Galster, G.; Hansen, J. B.; Hansen, J. D.; Hansen, P. H.; Joergensen, M. D.; Loevschall-Jensen, A. E.; Monk, J.; Pedersen, L. E.; Petersen, T. C.; Pingel, A.; Simonyan, M.; Thomsen, L. A.; Wiglesworth, C.; Xella, S.] Univ Copenhagen, Niels Bohr Inst, Copenhagen, Denmark. [Capua, M.; Crosetti, G.; La Rotonda, L.; Mastroberardino, A.; Policicchio, A.; Salvatore, D.; Scarfone, V.; Schioppa, M.; Susinno, G.; Tassi, E.] INFN Grp Collegato Cosenza, Nazl Frascati Lab, Frascati, Italy. [Capua, M.; Crosetti, G.; La Rotonda, L.; Mastroberardino, A.; Policicchio, A.; Salvatore, D.; Scarfone, V.; Schioppa, M.; Susinno, G.; Tassi, E.] Univ Calabria, Dipartimento Fis, I-87030 Commenda Di Rende, Italy. [Adamczyk, L.; Bold, T.; Dabrowski, W.; Dwuznik, M.; Dyndal, M.; Grabowska-Bold, I.; Kisielewska, D.; Koperny, S.; Kowalski, T. Z.; Mindur, B.; Przybycien, M.; Zemla, A.] AGH Univ Sci & Technol, Fac Phys & Appl Comp Sci, Krakow, Poland. [Palka, M.] Jagiellonian Univ, Marian Smoluchowski Inst Phys, Krakow, Poland. [Banas, E.; de Renstrom, P. A. Bruckman; Chwastowski, J. J.; Derendarz, D.; Gornicki, E.; Hajduk, Z.; Iwanski, W.; Kaczmarska, A.; Korcyl, K.; Malecki, Pa.; Olszewski, A.; Olszowska, J.; Stanecka, E.; Staszewski, R.; Trzebinski, M.; Trzupek, A.; Wolter, M. W.; Wosiek, B. K.; Wozniak, K. W.; Zabinski, B.] Polish Acad Sci, Henryk Niewodniczanski Inst Nucl Phys, Krakow, Poland. [Cao, T.; Firan, A.; Hoffman, J.; Kama, S.; Kehoe, R.; Randle-Conde, A. S.; Sekula, S. J.; Stroynowski, R.; Wang, H.; Ye, J.] So Methodist Univ, Dept Phys, Dallas, TX 75275 USA. [Izen, J. M.; Leyton, M.; Lou, X.; Namasivayam, H.; Reeves, K.] Univ Texas Dallas, Dept Phys, Richardson, TX USA. [Argyropoulos, S.; Asbah, N.; Bessner, M.; Bloch, I.; Borroni, S.; Camarda, S.; Dassoulas, J. A.; Deterre, C.; Dietrich, J.; Filipuzzi, M.; Friedrich, C.; Glazov, A.; Fajardo, L. S. Gomez; Grahn, K-J.; Gregor, I. M.; Grohsjean, A.; Haleem, M.; Hamnett, P. G.; Hengler, C.; Hiller, K. H.; Howarth, J.; Huang, Y.; Belenguer, M. Jimenez; Katzy, J.; Keller, J. S.; Kondrashova, N.; Kuhl, T.; Lisovyi, M.; Lobodzinska, E.; Lohwasser, K.; Medinnis, M.; Moenig, K.; Naumann, T.; Peschke, R.; Petit, E.; Radescu, V.; Rubinskiy, I.; Schaefer, R.; Sedov, G.; Shushkevich, S.; South, D.; Stanescu-Bellu, M.; Stanitzki, M. M.; Starovoitov, P.; Styles, N. A.; Tackmann, K.; Vankov, P.; Wang, J.; Wasicki, C.; Wildt, M. A.; Yatsenko, E.; Yildirim, E.] DESY, Hamburg & Zeuthen, Hamburg, Germany. [Burmeister, I.; Esch, H.; Goessling, C.; Jentzsch, J.; Jung, C. A.; Klingenberg, R.; Wittig, T.] Tech Univ Dortmund, Inst Expt Phys 4, Dortmund, Germany. [Anger, P.; Friedrich, F.; Grohs, J. P.; Gumpert, C.; Kobel, M.; Mader, W. F.; Morgenstern, M.; Novgorodova, O.; Rudolph, C.; Schnoor, U.; Siegert, F.; Socher, F.; Staerz, S.; Straessner, A.; Vest, A.; Wahrmund, S.] Tech Univ Dresden, Inst Kern & Teilchenphys, D-01062 Dresden, Germany. [Arce, A. T. H.; Benjamin, D. P.; Bocci, A.; Cerio, B.; Kajomovitz, E.; Kotwal, A.; Kruse, M. C.; Li, L.; Li, S.; Liu, M.; Oh, S. H.; Pollard, C. S.; Wang, C.] Duke Univ, Dept Phys, Durham, NC 27706 USA. [Bhimji, W.; Bristow, T. M.; Clark, P. J.; Dias, F. A.; Edwards, N. C.; Walls, F. M. Garay; Glaysher, P. C. F.; Harrington, R. D.; Leonidopoulos, C.; Mills, C.; O'Brien, B. J.; Pino, S. A. Olivares; Proissl, M.; Selbach, K. E.; Smart, B. H.; Washbrook, A.; Wynne, B. M.] Univ Edinburgh, SUPA Sch Phys & Astron, Edinburgh, Midlothian, Scotland. [Annovi, A.; Antonelli, M.; Bilokon, H.; Chiarella, V.; Curatolo, M.; Di Nardo, R.; Esposito, B.; Gatti, C.; Laurelli, P.; Maccarrone, G.; Prokofiev, K.; Sansoni, A.; Testa, M.; Vilucchi, E.] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy. [Amoroso, S.; Arnold, H.; Betancourt, C.; Boehler, M.; Bruneliere, R.; Buehrer, F.; Buescher, D.; Coniavitis, E.; Consorti, V.; Dao, V.; Di Simone, A.; Fehling-Kaschek, M.; Flechl, M.; Giuliani, C.; Herten, G.; Jakobs, K.; Javurek, T.; Jenni, P.; Kiss, F.; Koeneke, K.; Kopp, A. K.; Kuehn, S.; Lai, S.; Landgraf, U.; Madar, R.; Mahboubi, K.; Mohr, W.; Pagacova, M.; Parzefall, U.; Rave, T. C.; Ronzani, M.; Ruehr, F.; Rurikova, Z.; Ruthmann, N.; Schillo, C.; Schmidt, E.; Schumacher, M.; Sommer, P.; Sundermann, J. E.; Temming, K. K.; Tsiskaridze, V.; Ungaro, F. C.; von Radziewski, H.; Anh, T. Vu; Warsinsky, M.; Weiser, C.; Werner, M.; Zimmermann, S.] Univ Freiburg, Fak Math & Phys, D-79106 Freiburg, Germany. [Alexandre, G.; Ancu, L. S.; Barone, G.; Bell, P. J.; Bell, W. H.; Noccioli, E. Benhar; De Mendizabal, J. Bilbao; Bucci, F.; Toro, R. Camacho; Clark, A.; Delitzsch, C. M.; della Volpe, D.; Doglioni, C.; Ferrere, D.; Gadomski, S.; Gonzalez-Sevilla, S.; Goulette, M. P.; Gramling, J.; Guescini, F.; Iacobucci, G.; Katre, A.; La Rosa, A.; Mermod, P.; Miucci, A.; Muenstermann, D.; Nektarijevic, S.; Nikolics, K.; Picazio, A.; Pohl, M.; Rosbach, K.; Tykhonov, A.; Vallecorsa, S.; Wu, X.] Univ Geneva, Sect Phys, Geneva, Switzerland. [Barberis, D.; Darbo, G.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Gemme, C.; Guido, E.; Morettini, P.; Osculati, B.; Parodi, F.; Passaggio, S.; Rossi, L. P.; Schiavi, C.] Ist Nazl Fis Nucl, Sez Genova, Genoa, Italy. [Barberis, D.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Guido, E.; Osculati, B.; Parodi, F.; Schiavi, C.] Univ Genoa, Dipartimento Fis, Genoa, Italy. [Jejelava, J.; Tskhadadze, E. G.] Iv Javakhishvili Tbilisi State Univ, E Andronikashvili Inst Phys, Tbilisi, Rep of Georgia. [Djobava, T.; Durglishvili, A.; Khubua, J.; Mosidze, M.] Tbilisi State Univ, Inst High Energy Phys, Tbilisi, Rep of Georgia. [Dueren, M.; Kreutzfeldt, K.; Stenzel, H.] Univ Giessen, Inst Phys 2, Giessen, Germany. [Bates, R. L.; Britton, D.; Buckley, A. G.; Bussey, P.; Buttar, C. M.; Buzatu, A.; Cinca, D.; D'Auria, S.; Doherty, T.; Doyle, A. T.; Ferrag, S.; Ferrando, J.; de Lima, D. E. Ferreira; Gemmell, A.; Gul, U.; Ortiz, N. G. Gutierrez; Kar, D.; Knue, A.; O'Shea, V.; Barrera, C. Oropeza; Qin, G.; Quilty, D.; Ravenscroft, T.; Robson, A.; Saxon, D. H.; Smith, K. M.; St Denis, R. D.; Stewart, G. A.; Thompson, A. S.; Wright, M.] Univ Glasgow, SUPA Sch Phys & Astron, Glasgow, Lanark, Scotland. [Bierwagen, K.; Bindi, M.; George, M.; Graber, L.; Grosse-Knetter, J.; Hamer, M.; Hensel, C.; Kareem, M. J.; Kawamura, G.; Keil, M.; Kroeninger, K.; Lemmer, B.; Magradze, E.; Mchedlidze, G.; Llacer, M. Moreno; Musheghyan, H.; Nackenhorst, O.; Nadal, J.; Quadt, A.; Rieger, J.; Schorlemmer, A. L. S.; Serkin, L.; Shabalina, E.; Stolte, P.; Weingarten, J.] Univ Gottingen, Inst Phys 2, Gottingen, Germany. [Albrand, S.; Brown, J.; Collot, J.; Crepe-Renaudin, S.; Dechenaux, B.; Delsart, P. A.; Gabaldon, C.; Genest, M. H.; Hostachy, J-Y.; Ledroit-Guillon, F.; Lleres, A.; Lucotte, A.; Malek, F.; Monini, C.; Stark, J.; Trocme, B.; Wu, M.] Univ Grenoble Alpes, CNRS, IN2P3, Lab Phys Subatom & Cosmol, Grenoble, France. [McFarlane, K. W.] Hampton Univ, Dept Phys, Hampton, VA 23668 USA. [da Costa, J. Barreiro Guimaraes; Butler, B.; Catastini, P.; Conti, G.; Franklin, M.; Huth, J.; Ippolito, V.; Mateos, D. Lopez; Mercurio, K. M.; Morii, M.; Skottowe, H. P.; Spearman, W. R.; Sun, S.; Tolley, E.; Yen, A. L.; della Porta, G. Zevi] Harvard Univ, Lab Particle Phys & Cosmol, Cambridge, MA 02138 USA. [Andrei, V.; Baas, A.; Brandt, O.; Davygora, Y.; Dietzsch, T. A.; Dunford, M.; Hanke, P.; Hofmann, J. I.; Jongmanns, J.; Khomich, A.; Kluge, E. -E.; Laier, H.; Lang, V. S.; Meier, K.; Mueller, F.; Poddar, S.; Scharf, V.; Schultz-Coulon, H. -C.; Stamen, R.; Wessels, M.] Heidelberg Univ, Kirchhoff Inst Phys, Heidelberg, Germany. [Anders, C. F.; Giulini, M.; Kasieczka, G.; Narayan, R.; Schaetzel, S.; Schmitt, S.; Schoening, A.] Heidelberg Univ, Inst Phys, Heidelberg, Germany. [Colombo, T.; Kretz, M.; Kugel, A.] Heidelberg Univ, ZITI Inst Tech Informat, Mannheim, Germany. [Nagasaka, Y.] Hiroshima Inst Technol, Fac Appl Informat Sci, Hiroshima, Japan. [Brunet, S.; Dattagupta, A.; Evans, H.; Gagnon, P.; Lammers, S.; Martinez, N. Lorenzo; Luehring, F.; Ogren, H.; Penwell, J.; Poveda, J.; Weinert, B.; Zieminska, D.] Indiana Univ, Dept Phys, Bloomington, IN 47405 USA. [Franz, S.; Jussel, P.; Kneringer, E.; Lukas, W.; Nagai, K.; Ritsch, E.; Usanova, A.] Leopold Franzens Univ, Inst Astro & Teilchenphys, Innsbruck, Austria. [Mallik, U.; Mandrysch, R.; Morange, N.; Zaidan, R.] Univ Iowa, Iowa City, IA USA. [Chen, C.; Cochran, J.; De Lorenzi, F.; Dudziak, F.; Krumnack, N.; Prell, S.; Shrestha, S.; Yamamoto, K.] Iowa State Univ, Dept Phys & Astron, Ames, IA USA. [Ahmadov, F.; Aleksandrov, I. N.; Boyko, I. R.; Budagov, I. A.; Chelkov, G. A.; Cheplakov, A.; Chizhov, M. V.; Corso-Radu, A.; Dedovich, D. V.; Demichev, M.; Glonti, G. L.; Gostkin, M. I.; Huseynov, N.; Javadov, N.; Karpov, S. N.; Kazarinov, M. Y.; Khramov, E.; Kruchonak, U.; Kukhtin, V.; Ladygin, E.; Minashvili, I. A.; Mineev, M.; Olchevski, A. G.; Plotnikova, E.; Potrap, I. N.; Rusakovich, N. A.; Sadykov, R.; Sapronov, A.; Shiyakova, M.; Sisakyan, A. N.; Soloshenko, A.; Topilin, N. D.; Yeletskikh, I.; Zhemchugov, A.; Zimine, N. I.] JINR Dubna, Dubna, Russia. [Amako, K.; Aoki, M.; Arai, Y.; Ikegami, Y.; Ikeno, M.; Iwasaki, H.; Kanzaki, J.; Kohriki, T.; Kondo, T.; Kono, T.; Makida, Y.; Mitsui, S.; Nagano, K.; Nakamura, K.; Nozaki, M.; Odaka, S.; Sasaki, O.; Suzuki, Y.; Takubo, Y.; Tanaka, S.; Terada, S.; Tokushuku, K.; Tsuno, S.; Unno, Y.; Yamada, M.; Yamamoto, A.; Yasu, Y.] High Energy Accelerator Res Org, KEK, Tsukuba, Ibaraki, Japan. [Chen, Y.; Hasegawa, M.; Inamaru, Y.; Kishimoto, T.; Kurashige, H.; Kurumida, R.; Ochi, A.; Shimizu, S.; Takeda, H.; Yakabe, R.; Yamazaki, Y.; Yuan, L.] Kobe Univ, Grad Sch Sci, Kobe, Hyogo 657, Japan. [Ishino, M.; Sumida, T.; Tashiro, T.] Kyoto Univ, Fac Sci, Kyoto, Japan. [Takashima, R.] Kyoto Univ, Kyoto 612, Japan. [Kawagoe, K.; Oda, S.; Otono, H.; Tojo, J.] Kyushu Univ, Dept Phys, Fukuoka 812, Japan. [Alconada Verzini, M. J.; Alonso, F.; Anduaga, X. S.; Dova, M. T.; Monticelli, F.; Wahlberg, H.] Univ Nacl La Plata, Inst Fis La Plata, La Plata, Argentina. [Alconada Verzini, M. J.; Alonso, F.; Anduaga, X. S.; Dova, M. T.; Monticelli, F.; Wahlberg, H.] Consejo Nacl Invest Cient & Tecn, La Plata, Argentina. [Allison, L. J.; Barton, A. E.; Beattie, M. D.; Borissov, G.; Bouhova-Thacker, E. V.; Chilingarov, A.; Dearnaley, W. J.; Fox, H.; Grimm, K.; Henderson, R. C. W.; Hughes, G.; Jones, R. W. L.; Kartvelishvili, V.; Long, R. E.; Love, P. A.; Maddocks, H. J.; Smizanska, M.; Walder, J.] Univ Lancaster, Dept Phys, Lancaster, England. [Chiodini, G.; Gorini, E.; Orlando, N.; Perrino, R.; Primavera, M.; Spagnolo, S.; Ventura, A.] Ist Nazl Fis Nucl, Sez Lecce, Lecce, Italy. [Gorini, E.; Orlando, N.; Spagnolo, S.; Ventura, A.] Univ Salento, Dipartimento Matemat & Fis, Lecce, Italy. [Allport, P. P.; Bundock, A. C.; Burdin, S.; D'Onofrio, M.; Dervan, P.; Gwilliam, C. B.; Hayward, H. S.; Jackson, M.; Jones, T. J.; King, B. T.; Klein, M.; Klein, U.; Kretzschmar, J.; Laycock, P.; Lehan, A.; Mahmoud, S.; Maxfield, S. J.; Mehta, A.; Migas, S.; Price, J.; Readioff, N. P.; Schnellbach, Y. J.; Sellers, G.; Vossebeld, J. H.; Waller, P.] Univ Liverpool, Oliver Lodge Lab, Liverpool L69 3BX, Merseyside, England. [Cindro, V.; Deliyergiyev, M.; Filipcic, A.; Gorisek, A.; Kersevan, B. P.; Kramberger, G.; Mandic, I.; Mikuz, M.; Sfiligoj, T.] Jozef Stefan Inst, Dept Phys, Ljubljana, Slovenia. [Cindro, V.; Deliyergiyev, M.; Filipcic, A.; Gorisek, A.; Kersevan, B. P.; Kramberger, G.; Mandic, I.; Mikuz, M.; Sfiligoj, T.] Univ Ljubljana, Ljubljana, Slovenia. [Alpigiani, C.; Bona, M.; Bret, M. Cano; Cerrito, L.; Fletcher, G.; Goddard, J. R.; Hickling, R.; Landon, M. P. J.; Lloyd, S. L.; Morris, J. D.; Piccaro, E.; Rizvi, E.; Sandbach, R. L.; Snidero, G.; Castanheira, M. Teixeira Dias] Queen Mary Univ London, Sch Phys & Astron, London, England. [Berry, T.; Boisvert, V.; Brooks, T.; Connelly, I. A.; Cooper-Smith, N. J.; Cowan, G.; Duguid, L.; George, S.; Gibson, S. M.; Kempster, J. J.; Vazquez, J. G. Panduro; Pastore, Fr.; Rose, M.; Spano, F.; Teixeira-Dias, P.; Thomas-Wilsker, J.] Royal Holloway Univ London, Dept Phys, Surrey, England. [Bernat, P.; Bieniek, S. P.; Butterworth, J. M.; Campanelli, M.; Casadei, D.; Chislett, R. T.; Cooper, B. D.; Davison, A. R.; Davison, P.; Falla, R. J.; Gregersen, K.; Gutschow, C.; Hesketh, G. G.; Jansen, E.; Konstantinidis, N.; Korn, A.; Lambourne, L.; Leney, K. J. C.; Martyniuk, A. C.; Mcfayden, J. A.; Nurse, E.; Ochoa, M. I.; Pilkington, A. D.; Scanlon, T.; Sherwood, P.; Simmons, B.; Wardrope, D. R.; Waugh, B. M.; Wijeratne, P. A.] UCL, Dept Phys & Astron, London, England. [Bernius, C.; Greenwood, Z. D.; Jana, D. K.; Sawyer, L.; Sircar, A.; Subramaniam, R.] Louisiana Tech Univ, Ruston, LA 71270 USA. [Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; Davignon, O.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Liu, K.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Vannucci, F.; Varouchas, D.] Univ Paris 06, Lab Phys Nucl & Hautes Energies, Paris, France. [Bomben, M.; Calderini, G.; Crescioli, F.; Demilly, A.; Derue, F.; Lacour, D.; Laforge, B.; Lefebvre, G.; Liu, K.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Roos, L.; Vannucci, F.; Varouchas, D.] Univ Paris 07, Paris, France. [Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; Davignon, O.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Liu, K.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Vannucci, F.; Varouchas, D.] CNRS, IN2P3, Paris, France. [Akesson, T. P. A.; Bocchetta, S. S.; Bryngemark, L.; Floderus, A.; Hawkins, A. D.; Hedberg, V.; Ivarsson, J.; Jarlskog, G.; Lytken, E.; Meirose, B.; Mjornmark, J. U.; Smirnova, O.; Viazlo, O.] Lund Univ, Inst Fys, Lund, Sweden. [Arnal, V.; Barreiro, F.; Cantero, J.; De la Torre, H.; Del Peso, J.; Glasman, C.; Llorente Merino, J.; Terron, J.] Univ Autonoma Madrid, Dept Fis Teor C 15, Madrid, Spain. [Blum, W.; Buescher, V.; Caputo, R.; Ellinghaus, F.; Endner, O. C.; Ertel, E.; Fiedler, F.; Torregrosa, E. Fullana; Goeringer, C.; Heck, T.; Hohlfeld, M.; Hsu, P. J.; Huelsing, T. A.; Karnevskiy, M.; Kleinknecht, K.; Koenig, S.; Koepke, L.; Lin, T. H.; Lungwitz, M.; Masetti, L.; Mattmann, J.; Meyer, C.; Moreno, D.; Moritz, S.; Mueller, T.; Poettgen, R.; Sander, H. G.; Schaefer, U.; Schmitt, C.; Schott, M.; Schroeder, C.; Schuh, N.; Simioni, E.; Tapprogge, S.; Wollstadt, S. J.; Zimmermann, C.] Johannes Gutenberg Univ Mainz, Inst Phys, Mainz, Germany. [Almond, J.; Borri, M.; Cox, B. E.; Da Via, C.; Forti, A.; Ponce, J. M. Iturbe; Joshi, K. D.; Klinger, J. A.; Loebinger, F. K.; Marsden, S. P.; Masik, J.; Neep, T. J.; Oh, A.; Owen, M.; Pater, J. R.; Peters, R. F. Y.; Price, D.; Qin, Y.; Queitsch-Maitland, M.; Robinson, J. E. M.; Schwanenberger, C.; Thompson, R. J.; Tomlinson, L.; Watts, S.; Webb, S.; Woudstra, M. J.; Wyatt, T. R.; Yang, U. K.] Univ Manchester, Sch Phys & Astron, Manchester, Lancs, England. [Aad, G.; Alio, L.; Barbero, M.; Bertella, C.; Chen, L.; Clemens, J. C.; Coadou, Y.; Diglio, S.; Djama, F.; Feligioni, L.; Gao, J.; Hoffmann, D.; Hubaut, F.; Knoops, E. B. F. G.; Le Guirriec, E.; Li, B.; Madaffari, D.; Mochizuki, K.; Monnier, E.; Muanza, S.; Nagai, Y.; Pralavorio, P.; Rozanov, A.; Serre, T.; Talby, M.; Tiouchichine, E.; Tisserant, S.; Toth, J.; Touchard, F.; Ughetto, M.; Vacavant, L.] Aix Marseille Univ, CPPM, Marseille, France. [Aad, G.; Alio, L.; Aloisio, A.; Barbero, M.; Bertella, C.; Chen, L.; Clemens, J. C.; Coadou, Y.; Diglio, S.; Djama, F.; Feligioni, L.; Gao, J.; Hoffmann, D.; Hubaut, F.; Knoops, E. B. F. G.; Le Guirriec, E.; Li, B.; Madaffari, D.; Mochizuki, K.; Monnier, E.; Muanza, S.; Nagai, Y.; Pralavorio, P.; Rozanov, A.; Serre, T.; Talby, M.; Tiouchichine, E.; Tisserant, S.; Toth, J.; Touchard, F.; Ughetto, M.; Vacavant, L.] CNRS, IN2P3, Marseille, France. [Bellomo, M.; Brau, B.; Colon, G.; Dallapiccola, C.; Daya-Ishmukhametova, R. K.; Moyse, E. J. W.; Pais, P.; Pueschel, E.; Varol, T.; Ventura, D.; Willocq, S.] Univ Massachusetts, Dept Phys, Amherst, MA 01003 USA. [Belanger-Champagne, C.; Chapleau, B.; Cheatham, S.; Corriveau, F.; Mantifel, R.; Robertson, S. H.; Robichaud-Veronneau, A.; Stockton, M. C.; Stoebe, M.; Vachon, B.; Wang, K.; Warburton, A.] McGill Univ, Dept Phys, Montreal, PQ, Canada. [Barberio, E. L.; Brennan, A. J.; Jennens, D.; Kubota, T.; Limosani, A.; Hanninger, G. Nunes; Nuti, F.; Rados, P.; Spiller, L. A.; Tan, K. G.; Taylor, G. N.; Thong, W. M.; Urquijo, P.; Volpi, M.] Univ Melbourne, Sch Phys, Melbourne, Vic 3010, Australia. [Amidei, D.; Chelstowska, M. A.; Cheng, H. C.; Dai, T.; Diehl, E. B.; Dubbert, J.; Feng, H.; Ferretti, C.; Fleischmann, P.; Goldfarb, S.; Harper, D.; Levin, D.; Liu, L.; Long, J. D.; Lu, N.; Mc Kee, S. P.; McCarn, A.; Neal, H. A.; Panikashvili, N.; Qian, J.; Schwarz, T. A.; Searcy, J.; Thun, R. P.; Wilson, A.; Wu, Y.; Yu, J. M.; Zhang, D.; Zhou, B.; Zhu, J.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA. [Abolins, M.; Gonzalez, B. Alvarez; Arabidze, G.; Brock, R.; Bromberg, C.; Chegwidden, A.; Fisher, W. C.; Halladjian, G.; Hauser, R.; Hayden, D.; Huston, J.; Koll, J.; Linnemann, J. T.; Martin, B.; Pope, B. G.; Schoenrock, B. D.; Schwienhorst, R.; Ta, D.; Tollefson, K.; True, P.; Willis, C.; Zhang, H.] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA. [Alimonti, G.; Andreazza, A.; Besana, M. I.; Carminati, L.; Cavalli, D.; Citterio, M.; Consonni, S. M.; Costa, G.; Fanti, M.; Giugni, D.; Lari, T.; Mandelli, L.; Meroni, C.; Perini, L.; Pizio, C.; Ragusa, F.; Resconi, S.; Simoniello, R.; Tartarelli, G. F.; Troncon, C.; Turra, R.; Perez, M. Villaplana] Ist Nazl Fis Nucl, Sez Milano, Milan, Italy. [Andreazza, A.; Carminati, L.; Consonni, S. M.; Fanti, M.; Perini, L.; Pizio, C.; Ragusa, F.; Simoniello, R.; Turra, R.; Perez, M. Villaplana] Univ Milan, Dipartimento Fis, Milan, Italy. [Bogouch, A.; Harkusha, S.; Kulchitsky, Y.; Kurochkin, Y. A.; Tsiareshka, P. V.] Natl Acad Sci Belarus, BI Stepanov Phys Inst, Minsk, Byelarus. [Fitzgerald, E. A.; Yanush, S.] Natl Sci & Educ Ctr Particle & High Energy Phys, Minsk, Byelarus. [Taylor, F. E.] MIT, Dept Phys, Cambridge, MA 02139 USA. [Arguin, J-F.; Azuelos, G.; Dallaire, F.; Gauthier, L.; Leroy, C.; Rezvani, R.; Soueid, P.] Univ Montreal, Grp Particle Phys, Montreal, PQ, Canada. [Akimov, A. V.; Baranov, S. P.; Gavrilenko, I. L.; Komar, A. A.; Mashinistov, R.; Mouraviev, S. V.; Nechaeva, P. Yu.; Shmeleva, A.; Snesarev, A. A.; Sulin, V. V.; Tikhomirov, V. O.; Zhukov, K.] Acad Sci, PN Lebedev Phys Inst, Moscow, Russia. [Artamonov, A.; Gorbounov, P. A.; Khovanskiy, V.; Shatalov, P. B.; Tsukerman, I. I.] Inst Theoret & Expt Phys, Moscow 117259, Russia. [Antonov, A.; Belotskiy, K.; Bulekov, O.; Dolgoshein, B. A.; Kantserov, V. A.; Khodinov, A.; Krasnopevtsev, D.; Romaniouk, A.; Shulga, E.; Smirnov, S. Yu.; Smirnov, Y.; Soldatov, E. Yu.; Tikhomirov, V. O.; Timoshenko, S.; Vorobev, K.] Moscow Engn & Phys Inst MEPhI, Moscow, Russia. [Boldyrev, A. S.; Gladilin, L. K.; Grishkevich, Y. V.; Kramarenko, V. A.; Maevskiy, A.; Rud, V. I.; Sivoklokov, S. Yu.; Smirnova, L. N.; Turchikhin, S.] Moscow MV Lomonosov State Univ, DV Skobeltsyn Inst Nucl Phys, Moscow, Russia. [Adomeit, S.; Becker, S.; Biebel, O.; Bock, C.; Bortfeldt, J.; Calfayan, P.; Chow, B. K. B.; Duckeck, G.; Ebke, J.; Elmsheuser, J.; Heller, C.; Hertenberger, R.; Hoenig, F.; Legger, F.; Lorenz, J.; Mann, A.; Mehlhase, S.; Meineck, C.; Mitrevski, J.; Nunnemann, T.; Rauscher, F.; Ruschke, A.; Sanders, M. P.; Schaile, D.; Schieck, J.; Unverdorben, C.; Vladoiu, D.; Walker, R.; Will, J. Z.; Wittkowski, J.] Univ Munich, Fak Phys, Munich, Germany. [Barillari, T.; Bethke, S.; Bronner, J.; Compostella, G.; Cortiana, G.; Flowerdew, M. J.; Goblirsch-Kolb, M.; Ince, T.; Kiryunin, A. E.; Kluth, S.; Kortner, O.; Kortner, S.; Kroha, H.; Macchiolo, A.; Maier, A. A.; Manfredini, A.; Menke, S.; Moser, H. G.; Nagel, M.; Nisius, R.; Nowak, S.; Oberlack, H.; Pahl, C.; Richter, R.; Salihagic, D.; Sandstroem, R.; Schacht, P.; Schwegler, Ph.; Sforza, F.; Spettel, F.; Stern, S.; Stonjek, S.; Terzo, S.; von der Schmitt, H.; Weigell, P.; Wildauer, A.; Zanzi, D.] Max Planck Inst Phys & Astrophys, Werner Heisenberg Inst, Munich, Germany. [Shimojima, M.] Nagasaki Inst Appl Sci, Nagasaki, Japan. [Hasegawa, S.; Horii, Y.; Morvaj, L.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Grad Sch Sci, Nagoya, Aichi 4648601, Japan. [Hasegawa, S.; Horii, Y.; Morvaj, L.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Kobayashi Maskawa Inst, Nagoya, Aichi 4648601, Japan. [Aloisio, A.; Alviggi, M. G.; Canale, V.; Carlino, G.; Chiefari, G.; Conventi, F.; de Asmundis, R.; Della Pietra, M.; Di Donato, C.; Doria, A.; Giordano, R.; Iengo, P.; Izzo, V.; Merola, L.; Patricelli, S.; Perrella, S.; Rossi, E.; Sanchez, A.; Sekhniaidze, G.; Zurzolo, G.] Ist Nazl Fis Nucl, Sez Napoli, I-80125 Naples, Italy. [Aloisio, A.; Alviggi, M. G.; Canale, V.; Chiefari, G.; Di Donato, C.; Giordano, R.; Merola, L.; Patricelli, S.; Perrella, S.; Rossi, E.; Sanchez, A.; Zurzolo, G.] Univ Naples Federico II, Dipartimento Fis, Naples, Italy. [Gorelov, I.; Hoeferkamp, M. R.; Seidel, S. C.; Toms, K.; Wang, R.] Univ New Mexico, Dept Phys & Astron, Albuquerque, NM 87131 USA. [Besjes, G. J.; Caron, S.; Croft, V.; De Groot, N.; Filthaut, F.; Galea, C.; Klok, P. F.; Konig, A. C.; Salvucci, A.; Struebig, A.] Radboud Univ Nijmegen, Nikhef, Inst Math Astrophys & Particle Phys, NL-6525 ED Nijmegen, Netherlands. [Aben, R.; Angelozzi, I.; Beemster, L. J.; Bentvelsen, S.; Berge, D.; Bobbink, G. J.; Bos, K.; Boterenbrood, H.; Butti, P.; Castelli, A.; Colijn, A. P.; de Jong, P.; De Nooij, L.; Deigaard, I.; Deluca, C.; Deviveiros, P. O.; Dhaliwal, S.; Ferrari, P.; Gadatsch, S.; Geerts, D. A. A.; Hartjes, F.; Hessey, N. P.; Hod, N.; Igonkina, O.; Kluit, P.; Koffeman, E.; Lee, H.; Linde, F.; Mahlstedt, J.; Mechnich, J.; Oussoren, K. P.; Pani, P.; Salek, D.; Valencic, N.; Van den Wollenberg, W.; Van der Deijl, P. C.; van der geer, R.; van der Graaf, H.; Van der Leeuw, R.; van Vulpen, I.; Verkerke, W.; Vermeulen, J. C.; Vreeswijk, M.; Weits, H.] Nikhef Natl Inst Subatom Phys, Amsterdam, Netherlands. [Angelozzi, I.; Berge, D.; Bobbink, G. J.; Bos, K.; Boterenbrood, H.; Castelli, A.; Colijn, A. P.; Deigaard, I.; Deluca, C.; Geerts, D. A. A.; Hartjes, F.; Koffeman, E.; Lee, H.; Linde, F.; Mahlstedt, J.; Mechnich, J.; Oussoren, K. P.; Salek, D.; van der Graaf, H.; van Vulpen, I.; Vermeulen, J. C.; Weits, H.] Univ Amsterdam, Amsterdam, Netherlands. [Burghgrave, B.; Calkins, R.; Chakraborty, D.; Cole, S.; Suhr, C.; Yurkewicz, A.; Zutshi, V.] No Illinois Univ, Dept Phys, De Kalb, IL 60115 USA. [Anisenkov, A. V.; Bobrovnikov, V. S.; Bogdanchikov, A. G.; Kazanin, V. F.; Korol, A. A.; Malyshev, V. M.; Maslennikov, A. L.; Maximov, D. A.; Peleganchuk, S. V.; Rezanova, O. L.; Skovpen, K. Yu.; Soukharev, A. M.; Talyshev, A. A.; Tikhonov, Yu. A.] SB RAS, Budker Inst Nucl Phys, Novosibirsk, Russia. [Cranmer, K.; Haas, A.; Heinrich, L.; van Huysduynen, L. Hooft; Kaplan, B.; Karthik, K.; Konoplich, R.; Kreiss, S.; Lewis, G. H.; Mincer, A. I.; Nemethy, P.; Neves, R. M.] NYU, Dept Phys, New York, NY 10003 USA. [Gan, K. K.; Ishmukhametov, R.; Kagan, H.; Kass, R. D.; Merritt, H.; Moss, J.; Nagarkar, A.; Pignotti, D. T.; Tannenwald, B. B.; Yang, Y.] Ohio State Univ, Columbus, OH 43210 USA. [Nakano, I.] Okayama Univ, Fac Sci, Okayama 700, Japan. [Abbott, B.; Bertsche, C.; Gutierrez, P.; Hasib, A.; Norberg, S.; Saleem, M.; Severini, H.; Skubic, P.; Strauss, M.] Univ Oklahoma, Homer L Dodge Dept Phys & Astron, Norman, OK 73019 USA. [Abi, B.; Bousson, N.; Khanov, A.; Rizatdinova, F.; Sidorov, D.; Yu, J.] Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USA. [Chytka, L.; Hamal, P.; Hrabovsky, M.; Kvita, J.; Nozka, L.] Palacky Univ, RCPTM, CR-77147 Olomouc, Czech Republic. [Brau, J. E.; Brost, E.; Hopkins, W. H.; Majewski, S.; Potter, C. T.; Ptacek, E.; Radloff, P.; Shamim, M.; Sinev, N. B.; Strom, D. M.; Torrence, E.; Wanotayaroj, C.; Winklmeier, F.] Univ Oregon, Ctr High Energy Phys, Eugene, OR 97403 USA. [Khalek, S. Abdel; Bassalat, A.; Becot, C.; Binet, S.; Bourdarios, C.; Charfeddine, D.; De Regie, J. B. De Vivie; Duflot, L.; Escalier, M.; Fayard, L.; Fournier, D.; Grivaz, J. -F.; Guillemin, T.; Hariri, F.; Henrot-Versille, S.; Hrivnac, J.; Iconomidou-Fayard, L.; Kado, M.; Li, Y.; Lounis, A.; Makovec, N.; Poggioli, L.; Puzo, P.; Renaud, A.; Rousseau, D.; Rybkin, G.; Schaffer, A. C.; Scifo, E.; Serin, L.; Simion, S.; Tanaka, R.; Tran, H. L.; Zerwas, D.; Zhang, Z.] Univ Paris 11, LAL, Orsay, France. [Khalek, S. Abdel; Bassalat, A.; Becot, C.; Binet, S.; Bourdarios, C.; Charfeddine, D.; De Regie, J. B. De Vivie; Duflot, L.; Escalier, M.; Fayard, L.; Fournier, D.; Grivaz, J. -F.; Guillemin, T.; Hariri, F.; Henrot-Versille, S.; Hrivnac, J.; Iconomidou-Fayard, L.; Kado, M.; Li, Y.; Lounis, A.; Makovec, N.; Poggioli, L.; Puzo, P.; Renaud, A.; Rousseau, D.; Rybkin, G.; Schaffer, A. C.; Scifo, E.; Serin, L.; Simion, S.; Tanaka, R.; Tran, H. L.; Zerwas, D.; Zhang, Z.] CNRS, IN2P3, F-91405 Orsay, France. [Endo, M.; Hanagaki, K.; Lee, J. S. H.; Nomachi, M.; Okamura, W.; Sugaya, Y.; Teoh, J. J.; Yamaguchi, Y.] Osaka Univ, Grad Sch Sci, Osaka, Japan. [Bugge, L.; Bugge, M. K.; Cameron, D.; Catmore, J. R.; Franconi, L.; Gjelsten, B. K.; Gramstad, E.; Ould-Saada, F.; Pajchel, K.; Pedersen, M.; Read, A. L.; Rohne, O.; Stapnes, S.; Strandlie, A.] Univ Oslo, Dept Phys, Oslo, Norway. [Apolle, R.; Barr, A. J.; Behr, K.; Boddy, C. R.; Buckingham, R. M.; Cooper-Sarkar, A. M.; Ortuzar, M. Crispin; Dafinca, A.; Davies, E.; Gallas, E. J.; Gupta, S.; Gwenlan, C.; Hall, D.; Hays, C. P.; Henderson, J.; Howard, J.; Huffman, T. B.; Issever, C.; Kalderon, C. W.; King, R. S. B.; Kogan, L. A.; Lewis, A.; Livermore, S. S. A.; Nickerson, R. B.; Pachal, K.; Pinder, A.; Ryder, N. C.; Sawyer, C.; Short, D.; Tseng, J. C-L.; Vickey, T.; Viehhauser, G. H. A.; Weidberg, A. R.; Zhong, J.] Univ Oxford, Dept Phys, Oxford, England. [Conta, C.; Dondero, P.; Ferrari, R.; Fraternali, M.; Gaudio, G.; Livan, M.; Negri, A.; Polesello, G.; Rebuzzi, D. M.; Rimoldi, A.; Vercesi, V.] Ist Nazl Fis Nucl, Sez Pavia, Pavia, Italy. [Conta, C.; Dondero, P.; Fraternali, M.; Livan, M.; Negri, A.; Rebuzzi, D. M.; Rimoldi, A.] Univ Pavia, Dipartimento Fis, I-27100 Pavia, Italy. [Brendlinger, K.; Heim, S.; Hines, E.; Hong, T. M.; Jackson, B.; Kroll, J.; Kunkle, J.; Lester, C. M.; Lipeles, E.; Meyer, C.; Ospanov, R.; Saxon, J.; Stahlman, J.; Thomson, E.; Tuna, A. N.; Vanguri, R.; Williams, H. H.] Univ Penn, Dept Phys, Philadelphia, PA 19104 USA. [Ezhilov, A.; Fedin, O. L.; Gratchev, V.; Grebenyuk, O. G.; Levchenko, M.; Maleev, V. P.; Ryabov, Y. F.; Schegelsky, V. A.; Sedykh, E.; Seliverstov, D. M.; Solovyev, V.] Petersburg Nucl Phys Inst, Gatchina, Russia. [Beccherle, R.; Bertolucci, F.; Cavasinni, V.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Leone, S.; Roda, C.; Scuri, F.; Volpi, G.; White, S.] Ist Nazl Fis Nucl, Sez Pisa, Pisa, Italy. [Beccherle, R.; Bertolucci, F.; Cavasinni, V.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Leone, S.; Roda, C.; Scuri, F.; Volpi, G.; White, S.] Univ Pisa, Dipartimento Fis E Fermi, Pisa, Italy. [Bianchi, R. M.; Boudreau, J.; Cleland, W.; Escobar, C.; Kittelmann, T.; Mueller, J.; Prieur, D.; Sapp, K.; Su, J.; Yoosoofmiya, R.] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA. [Aguilar-Saavedra, J. A.; Amorim, A.; Anjos, N.; Araque, J. P.; Cantrill, R.; Carvalho, J.; Castro, N. F.; Conde Muino, P.; Da Cunha Sargedas De Sousa, M. J.; Do Valle Wemans, A.; Fiolhais, M. C. N.; Galhardo, B.; Gomes, A.; Goncalo, R.; Jorge, P. M.; Lopes, L.; Machado Miguens, J.; Maio, A.; Maneira, J.; Marques, C. N.; Onofre, A.; Palma, A.; Pedro, R.; Pina, J.; Pinto, B.; Santos, H.; Saraiva, J. G.; Silva, J.; Tavares Delgado, A.; Veloso, F.; Wolters, H.] Lab Instrumentacao & Fis Expt Particulas LIP, Lisbon, Portugal. [Amorim, A.; Conde Muino, P.; Da Cunha Sargedas De Sousa, M. J.; Gomes, A.; Jorge, P. M.; Machado Miguens, J.; Maio, A.; Maneira, J.; Palma, A.; Pedro, R.; Pina, J.; Tavares Delgado, A.] Univ Lisbon, Fac Ciencias, Lisbon, Portugal. [Amor Dos Santos, S. P.; Carvalho, J.; Fiolhais, M. C. N.; Galhardo, B.; Veloso, F.; Wolters, H.] Univ Coimbra, Dept Phys, Coimbra, Portugal. [Gomes, A.; Maio, A.; Pina, J.; Saraiva, J. G.; Silva, J.] Univ Lisbon, Ctr Fis Nucl, P-1699 Lisbon, Portugal. [Onofre, A.] Univ Minho, Dept Fis, Braga, Portugal. [Aguilar-Saavedra, J. A.] Univ Granada, Dept Fis Teor & Cosmos, Granada, Spain. [Aguilar-Saavedra, J. A.] Univ Granada, CAFPE, Granada, Spain. [Do Valle Wemans, A.] Univ Nova Lisboa, Dept Fis, Caparica, Portugal. [Chen, L.; Gao, J.] Univ Nova Lisboa, CEFITEC Fac Ciencias & Tecnol, Caparica, Portugal. [Bohm, J.; Chudoba, J.; Havranek, M.; Hejbal, J.; Jakoubek, T.; Kepka, O.; Kupco, A.; Kus, V.; Lokajicek, M.; Lysak, R.; Marcisovsky, M.; Mikestikova, M.; Nemecek, S.; Sicho, P.; Staroba, P.; Svatos, M.; Tasevsky, M.; Vrba, V.] Acad Sci Czech Republic, Inst Phys, Prague, Czech Republic. [Augsten, K.; Gallus, P.; Gunther, J.; Jakubek, J.; Kohout, Z.; Kral, V.; Myska, M.; Pospisil, S.; Seifert, F.; Simak, V.; Slavicek, T.; Smolek, K.; Solar, M.; Solc, J.; Sopczak, A.; Sopko, B.; Sopko, V.; Suk, M.; Turecek, D.; Vacek, V.; Vlasak, M.; Vokac, P.; Vykydal, Z.; Zeman, M.] Czech Tech Univ, Prague, Czech Republic. [Balek, P.; Berta, P.; Cerny, K.; Chalupkova, I.; Davidek, T.; Dolejsi, J.; Dolezal, Z.; Faltova, J.; Kodys, P.; Leitner, R.; Pleskot, V.; Reznicek, P.; Rybar, M.; Scheirich, D.; Spousta, M.; Sykora, T.; Tas, P.; Todorova-Nova, S.; Valkar, S.; Vorobel, V.] Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic. [Borisov, A.; Denisov, S. P.; Fakhrutdinov, R. M.; Fenyuk, A. B.; Golubkov, D.; Kamenshchikov, A.; Karyukhin, A. N.; Korotkov, V. A.; Kozhin, A. S.; Minaenko, A. A.; Myagkov, A. G.; Nikolaenko, V.; Solodkov, A. A.; Solovyanov, O. V.; Starchenko, E. A.; Zaitsev, A. M.; Zenin, O.] State Res Ctr Inst High Energy Phys, Protvino, Russia. [Apolle, R.; Barnett, B. M.; Davies, E.; Dewhurst, A.; Emeliyanov, D.; Gallop, B. J.; Gee, C. N. P.; Sankey, D. P. C.] Rutherford Appleton Lab, Particle Phys Dept, Didcot OX11 0QX, Oxon, England. [Benslama, K.] Univ Regina, Dept Phys, Regina, SK S4S 0A2, Canada. [Tanaka, S.] Ritsumeikan Univ, Kusatsu, Shiga, Japan. 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[Bacci, C.; Baroncelli, A.; Biglietti, M.; Bortolotto, V.; Ceradini, F.; Di Micco, B.; Farilla, A.; Graziani, E.; Iodice, M.; Orestano, D.; Passeri, A.; Pastore, F.; Petrucci, F.; Puddu, D.; Salamanna, G.; Stanescu, C.; Taccini, C.; Trovatelli, M.] Ist Nazl Fis Nucl, Sez Roma Tre, Rome, Italy. [Bacci, C.; Bortolotto, V.; Ceradini, F.; Di Micco, B.; Orestano, D.; Pastore, F.; Petrucci, F.; Puddu, D.; Salamanna, G.; Taccini, C.; Trovatelli, M.] Univ Roma Tre, Dipartimento Matemat & Fis, Rome, Italy. [Benchekroun, D.; Chafaq, A.; Gouighri, M.; Hoummada, A.] Univ Hassan 2, Reseau Univ Phys Hautes Energies, Fac Sci Ain Chock, Casablanca, Morocco. [Ghazlane, H.] Ctr Natl Energie Sci Tech Nucl, Rabat, Morocco. [El Kacimi, M.; Goujdami, D.] Univ Cadi Ayyad, LPHEA, Fac Sci Semlalia, Marrakech, Morocco. [Boutouil, S.; Derkaoui, J. E.; Ouchrif, M.; Tayalati, Y.] Univ Mohamed Premier, Fac Sci, Oujda, Morocco. [Boutouil, S.; Derkaoui, J. E.; Ouchrif, M.; Tayalati, Y.] LPTPM, Oujda, Morocco. 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A.; Seiden, A.] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA. [Blackburn, D.; Coccaro, A.; Goussiou, A. G.; Harris, O. M.; Hsu, S. -C.; Lubatti, H. J.; Marx, M.; Rompotis, N.; Rosten, R.; Rothberg, J.; De Bruin, P. H. Sales; Watts, G.] Univ Washington, Dept Phys, Seattle, WA 98195 USA. [Anastopoulos, C.; Costanzo, D.; Donszelmann, T. Cuhadar; Dawson, I.; Fletcher, G. T.; Hodgkinson, M. C.; Hodgson, P.; Johansson, P.; Korolkova, E. V.; Paredes, B. Lopez; Miyagawa, P. S.; Paganis, E.; Suruliz, K.; Tovey, D. R.] Univ Sheffield, Dept Phys & Astron, Sheffield, S Yorkshire, England. [Hasegawa, Y.; Takeshita, T.] Shinshu Univ, Dept Phys, Nagano, Japan. [Atlay, N. B.; Buchholz, P.; Czirr, H.; Fleck, I.; Gaur, B.; Ibragimov, I.; Ikematsu, K.; Rosenthal, O.; Sipica, V.; Walkowiak, W.; Ziolkowski, M.] Univ Siegen, Fachbereich Phys, D-57068 Siegen, Germany. [Buat, Q.; Dawe, E.; O'Neil, D. C.; Stelzer, B.; Tanasijczuk, A. J.; Torres, H.; Van Nieuwkoop, J.; Vetterli, M. C.] Simon Fraser Univ, Dept Phys, Burnaby, BC V5A 1S6, Canada. [Aracena, I.; Mayes, J. Backus; Barklow, T.; Bartoldus, R.; Bawa, H. S.; Black, J. E.; Cogan, J. G.; Eifert, T.; Fulsom, B. G.; Gao, Y. S.; Garelli, N.; Grenier, P.; Kagan, M.; Kocian, M.; Koi, T.; Lowe, A. J.; Malone, C.; Mount, R.; Nef, P. D.; Nelson, T. K.; Piacquadio, G.; Salnikov, A.; Schwartzman, A.; Silverstein, D.; Strauss, E.; Su, D.; Swiatlowski, M.; Wittgen, M.; Young, C.] SLAC Natl Accelerator Lab, Stanford, CA USA. [Astalos, R.; Bartos, P.; Blazek, T.; Federic, P.; Plazak, L.; Stavina, P.; Sykora, I.; Tokar, S.; Zenis, T.] Comenius Univ, Fac Math Phys & Informat, Bratislava, Slovakia. [Antos, J.; Bruncko, D.; Kladiva, E.; Strizenec, P.] Slovak Acad Sci, Inst Expt Phys, Dept Subnucl Phys, Kosice 04353, Slovakia. [Hamilton, A.] Univ Cape Town, Dept Phys, ZA-7925 Cape Town, South Africa. [Aurousseau, M.; Castaneda-Miranda, E.; Connell, S. H.; Yacoob, S.] Univ Johannesburg, Dept Phys, Johannesburg, South Africa. [Bristow, K.; Carrillo-Montoya, G. D.; Chen, X.; Hamity, G. N.; Hsu, C.; Garcia, B. R. Mellado; Ruan, X.; Vickey, T.; Boeriu, O. E. Vickey] Univ Witwatersrand, Sch Phys, Johannesburg, South Africa. [Abulaiti, Y.; Akerstedt, H.; Asman, B.; Bendtz, K.; Bertoli, G.; Bessidskaia, O.; Bohm, C.; Clement, C.; Cribbs, W. A.; Eriksson, D.; Gellerstedt, K.; Hellman, S.; Johansson, K. E.; Jon-And, K.; Khandanyan, H.; Kim, H.; Klimek, P.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Petridis, A.; Plucinski, P.; Rossetti, V.; Silverstein, S. B.; Sjolin, J.; Strandberg, S.; Tylmad, M.] Stockholm Univ, Dept Phys, Stockholm, Sweden. [Abulaiti, Y.; Akerstedt, H.; Asman, B.; Bendtz, K.; Bertoli, G.; Bessidskaia, O.; Clement, C.; Cribbs, W. A.; Gellerstedt, K.; Hellman, S.; Johansson, K. E.; Jon-And, K.; Khandanyan, H.; Kim, H.; Klimek, P.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Petridis, A.; Plucinski, P.; Rossetti, V.; Sjolin, J.; Strandberg, S.; Tylmad, M.] Oskar Klein Ctr, Stockholm, Sweden. [Jovicevic, J.; Kuwertz, E. S.; Lund-Jensen, B.; Morley, A. K.; Strandberg, J.] Royal Inst Technol, Dept Phys, S-10044 Stockholm, Sweden. [Bee, C. P.; Campoverde, A.; Chen, K.; Engelmann, R.; Grassi, V.; Hobbs, J.; Jia, J.; Li, H.; Lindquist, B. E.; Mastrandrea, P.; McCarthy, R. L.; Puldon, D.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA. [Bartsch, V.; Cerri, A.; Barajas, C. A. Chavez; De Sanctis, U.; De Santo, A.; Grout, Z. J.; Potter, C. J.; Salvatore, F.; Castillo, I. Santoyo; Shehu, C. Y.; Sutton, M. R.; Vivarelli, I.] Univ Sussex, Dept Phys & Astron, Brighton, E Sussex, England. [Black, C. W.; Cuthbert, C.; Finelli, K. D.; Jeng, G. -Y.; Patel, N. D.; Saavedra, A. F.; Scarcella, M.; Varvell, K. E.; Watson, I. J.; Yabsley, B.] Univ Sydney, Sch Phys, Sydney, NSW 2006, Australia. [Abdallah, J.; Chu, M. L.; Hou, S.; Jamin, D. O.; Lee, C. A.; Lee, S. C.; Lin, S. C.; Liu, B.; Liu, D.; Lo Sterzo, F.; Mazini, R.; Ren, Z. L.; Shi, L.; Soh, D. A.; Teng, P. K.; Wang, C.; Wang, S. M.; Weng, Z.; Zhang, L.] Acad Sinica, Inst Phys, Taipei, Taiwan. [Abreu, H.; Di Mattia, A.; Kopeliansky, R.; Musto, E.; Rozen, Y.; Tarem, S.] Technion Israel Inst Technol, Dept Phys, IL-32000 Haifa, Israel. [Abramowicz, H.; Alexander, G.; Amram, N.; Ashkenazi, A.; Bella, G.; Benary, O.; Benhammou, Y.; Davies, M.; Etzion, E.; Gershon, A.; Gueta, O.; Guttman, N.; Munwes, Y.; Oren, Y.; Sadeh, I.; Silver, Y.; Soffer, A.; Taiblum, N.] Tel Aviv Univ, Raymond & Beverly Sackler Sch Phys & Astron, IL-69978 Tel Aviv, Israel. [Bachas, K.; Gkaitatzis, S.; Gkialas, I.; Iliadis, D.; Kordas, K.; Kouskoura, V.; Leisos, A.; Papageorgiou, K.; Petridou, C.; Sampsonidis, D.; Sidiropoulou, O.] Aristotle Univ Thessaloniki, Dept Phys, GR-54006 Thessaloniki, Greece. [Akimoto, G.; Asai, S.; Azuma, Y.; Dohmae, T.; Enari, Y.; Hanawa, K.; Kanaya, N.; Kataoka, Y.; Kawamoto, T.; Kazama, S.; Kessoku, K.; Kobayashi, T.; Komori, Y.; Mashimo, T.; Masubuchi, T.; Nakamura, T.; Ninomiya, Y.; Okuyama, T.; Sakamoto, H.; Sasaki, Y.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamaguchi, H.; Yamamoto, S.; Yamamura, T.; Yamanaka, T.; Yoshihara, K.] Univ Tokyo, Int Ctr Elementary Particle Phys, Tokyo, Japan. [Akimoto, G.; Asai, S.; Azuma, Y.; Dohmae, T.; Enari, Y.; Hanawa, K.; Kanaya, N.; Kataoka, Y.; Kawamoto, T.; Kazama, S.; Kessoku, K.; Kobayashi, T.; Komori, Y.; Mashimo, T.; Masubuchi, T.; McFarlane, K. W.; Nakamura, T.; Ninomiya, Y.; Okuyama, T.; Sakamoto, H.; Sasaki, Y.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamaguchi, H.; Yamamoto, S.; Yamamura, T.; Yamanaka, T.; Yoshihara, K.] Univ Tokyo, Dept Phys, Tokyo 113, Japan. [Bratzler, U.; Fukunaga, C.] Tokyo Metropolitan Univ, Grad Sch Sci & Technol, Tokyo 158, Japan. [Hirose, M.; Ishitsuka, M.; Jinnouchi, O.; Kobayashi, D.; Kuze, M.; Motohashi, K.; Nagai, R.; Nobe, T.; Pettersson, N. E.] Tokyo Inst Technol, Dept Phys, Tokyo 152, Japan. [AbouZeid, O. S.; Brelier, B.; Chau, C. C.; Ilic, N.; Keung, J.; Krieger, P.; Mc Goldrick, G.; Orr, R. S.; Polifka, R.; Rudolph, M. S.; Savard, P.; Schramm, S.; Sinervo, P.; Spreitzer, T.; Taenzer, J.; Teuscher, R. J.; Thompson, P. D.; Trischuk, W.; Venturi, N.] Univ Toronto, Dept Phys, Toronto, ON, Canada. [Azuelos, G.; Canepa, A.; Chekulaev, S. V.; Fortin, D.; Gingrich, D. M.; Koutsman, A.; Oakham, F. G.; Oram, C. J.; Codina, E. Perez; Savard, P.; Schouten, D.; Seuster, R.; Stelzer-Chilton, O.; Tafirout, R.; Trigger, I. M.; Vetterli, M. C.] TRIUMF, Vancouver, BC V6T 2A3, Canada. [Garcia, J. A. Benitez; Bustos, A. C. Florez; Ramos, J. A. Manjarres; Palacino, G.; Qureshi, A.; Taylor, W.] York Univ, Dept Phys & Astron, Toronto, ON M3J 2R7, Canada. [Hara, K.; Hayashi, T.; Kim, S. H.; Kiuchi, K.; Ukegawa, F.] Univ Tsukuba, Fac Pure & Appl Sci, Tsukuba, Ibaraki, Japan. [Beauchemin, P. H.; Hamilton, S.; Meoni, E.; Rolli, S.; Sliwa, K.; Wetter, J.] Tufts Univ, Dept Phys & Astron, Medford, MA 02155 USA. [Losada, M.; Navarro, G.; Sandoval, C.] Univ Antonio Narino, Ctr Invest, Bogota, Colombia. [Corso-Radu, A.; Gerbaudo, D.; Lankford, A. J.; Mete, A. S.; Nelson, A.; Rao, K.; Relich, M.; Scannicchio, D. A.; Schernau, M.; Shimmin, C. O.; Taffard, A.; Unel, G.; Whiteson, D.; Zhou, N.] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA USA. [Acharya, B. S.; Alhroob, M.; Brazzale, S. F.; Cobal, M.; Giordani, M. P.; Pinamonti, M.; Quayle, W. B.; Shaw, K.; Soualah, R.] Ist Nazl Fis Nucl, Grp Collegato Udine, Sez Trieste, Udine, Italy. [Acharya, B. S.; Quayle, W. B.; Shaw, K.] Abdus Salaam Int Ctr Theoret Phys, Trieste, Italy. [Alhroob, M.; Brazzale, S. F.; Cobal, M.; Giordani, M. P.; Pinamonti, M.; Soualah, R.] Univ Udine, Dipartimento Chim Fis & Ambiente, I-33100 Udine, Italy. [Atkinson, M.; Basye, A.; Benekos, N.; Cavaliere, V.; Chang, P.; Coggeshall, J.; Errede, D.; Errede, S.; Lie, K.; Liss, T. M.; Neubauer, M. S.; Shang, R.; Vichou, I.] Univ Illinois, Dept Phys, Urbana, IL 61801 USA. [Brenner, R.; Buszello, C. P.; Ekelof, T.; Ellert, M.; Ferrari, A.; Isaksson, C.; Madsen, A.; Ohman, H.; Pelikan, D.; Rangel-Smith, C.] Uppsala Univ, Dept Phys & Astron, Uppsala, Sweden. [Cabrera Urban, S.; Castillo Gimenez, V.; Costa, M. J.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Hernandez Jimenez, Y.; Higon-Rodriguez, E.; Irles Quiles, A.; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; March, L.; Marti-Garcia, S.; Mitsou, V. A.; Moles-Valls, R.; Oliver Garcia, E.; Pedraza Lopez, S.; Perez Garcia-Estan, M. T.; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, J.; Sanchez Martinez, V.; Soldevila, U.; Torro Pastor, E.; Valero, A.; Valladolid Gallego, E.; Valls Ferrer, J. A.; Vos, M.] Univ Valencia, Inst Fis Corpuscular IFIC, Valencia, Spain. [Cabrera Urban, S.; Castillo Gimenez, V.; Costa, M. J.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Hernandez Jimenez, Y.; Higon-Rodriguez, E.; Irles Quiles, A.; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; March, L.; Marti-Garcia, S.; Mitsou, V. A.; Moles-Valls, R.; Oliver Garcia, E.; Pedraza Lopez, S.; Perez Garcia-Estan, M. T.; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, J.; Sanchez Martinez, V.; Soldevila, U.; Torro Pastor, E.; Valero, A.; Valladolid Gallego, E.; Valls Ferrer, J. A.; Vos, M.] Univ Valencia, Dept Fis Atom Mol & Nucl, Valencia, Spain. [Cabrera Urban, S.; Castillo Gimenez, V.; Costa, M. J.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Hernandez Jimenez, Y.; Higon-Rodriguez, E.; Irles Quiles, A.; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; March, L.; Marti-Garcia, S.; Mitsou, V. A.; Moles-Valls, R.; Oliver Garcia, E.; Pedraza Lopez, S.; Perez Garcia-Estan, M. T.; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, J.; Sanchez Martinez, V.; Soldevila, U.; Torro Pastor, E.; Valero, A.; Valladolid Gallego, E.; Valls Ferrer, J. A.; Vos, M.] Univ Valencia, Dept Ingn Elect, Valencia, Spain. [Cabrera Urban, S.; Castillo Gimenez, V.; Costa, M. J.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Hernandez Jimenez, Y.; Higon-Rodriguez, E.; Irles Quiles, A.; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; March, L.; Marti-Garcia, S.; Mitsou, V. A.; Moles-Valls, R.; Oliver Garcia, E.; Pedraza Lopez, S.; Perez Garcia-Estan, M. T.; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, J.; Sanchez Martinez, V.; Soldevila, U.; Torro Pastor, E.; Valero, A.; Valladolid Gallego, E.; Valls Ferrer, J. A.; Vos, M.] Univ Valencia, CNM, IMB, Valencia, Spain. [Cabrera Urban, S.; Castillo Gimenez, V.; Costa, M. J.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Hernandez Jimenez, Y.; Higon-Rodriguez, E.; Irles Quiles, A.; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; March, L.; Marti-Garcia, S.; Mitsou, V. A.; Moles-Valls, R.; Oliver Garcia, E.; Pedraza Lopez, S.; Perez Garcia-Estan, M. T.; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, J.; Sanchez Martinez, V.; Soldevila, U.; Torro Pastor, E.; Valero, A.; Valladolid Gallego, E.; Valls Ferrer, J. A.; Vos, M.] CSIC, Valencia, Spain. [Fedorko, W.; Gay, C.; Gecse, Z.; King, S. B.; Lister, A.; Swedish, S.; Viel, S.] Univ British Columbia, Dept Phys, Vancouver, BC, Canada. [Albert, J.; Bansal, V.; Berghaus, F.; Bernlochner, F. U.; David, C.; Fincke-Keeler, M.; Hamano, K.; Hill, E.; Keeler, R.; Kowalewski, R.; Lefebvre, M.; Marino, C. P.; McPherson, R. A.; Ouellette, E. A.; Pearce, J.; Sobie, R.; Venturi, M.] Univ Victoria, Dept Phys & Astron, Victoria, BC, Canada. [Beckingham, M.; Farrington, S. M.; Harrison, P. F.; Janus, M.; Jeske, C.; Jones, G.; Martin, T. A.; Murray, W. J.; Pianori, E.] Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England. [Iizawa, T.; Kimura, N.; Mitani, T.; Sakurai, Y.; Yorita, K.] Waseda Univ, Tokyo, Japan. [Barak, L.; Bressler, S.; Citron, Z. H.; Duchovni, E.; Gabizon, O.; Gross, E.; Groth-Jensen, J.; Lellouch, D.; Levinson, L. J.; Mikenberg, G.; Milov, A.; Milstein, D.; Pitt, M.; Roth, I.; Schaarschmidt, J.; Smakhtin, V.] Weizmann Inst Sci, Dept Particle Phys, IL-76100 Rehovot, Israel. [Banerjee, Sw.; Castillo, L. R. Flores; Hard, A. S.; Heng, Y.; Ji, H.; Ju, X.; Kashif, L.; Kruse, A.; Ming, Y.; Pan, Y. B.; Wang, F.; Wiedenmann, W.; Wu, S. L.; Yang, H.; Zhang, F.; Zobernig, G.] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA. [Redelbach, A.; Schreyer, M.; Siragusa, G.; Stroehmer, R.; Tam, J. Y. C.; Trefzger, T.; Weber, S. W.; Zibell, A.] Univ Wurzburg, Fak Phys & Astron, D-97070 Wurzburg, Germany. [Bannoura, A. A. E.; Barisonzi, M.; Becker, K.; Beermann, T. A.; Boek, T. T.; Braun, H. 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[Kono, T.] Ochanomizu Univ, Ochadai Acad Prod, Tokyo 112, Japan. [Konoplich, R.] Manhattan Coll, New York, NY USA. [Korol, A. A.; Maximov, D. A.; Rezanova, O. L.; Talyshev, A. A.; Tikhonov, Yu. A.] Novosibirsk State Univ, Novosibirsk 630090, Russia. [Li, B.] Acad Sinica, Inst Phys, Taipei, Taiwan. [Lin, S. C.] Acad Sinica, Inst Phys, Acad Sinica Grid Comp, Taipei, Taiwan. [Mal, P.] Natl Inst Sci Educ & Res, Sch Phys Sci, Bhubaneswar, Orissa, India. [Messina, A.] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy. [Myagkov, A. G.; Nikolaenko, V.; Zaitsev, A. M.] Moscow Inst Phys & Technol, Dolgoprudnyi, Russia. [Nessi, M.] Univ Geneva, Sect Phys, Geneva, Switzerland. [Pinamonti, M.] Int Sch Adv Studies SISSA, Trieste, Italy. [Purohit, M.] Univ S Carolina, Dept Phys & Astron, Columbia, SC 29208 USA. [Shi, L.; Soh, D. A.; Weng, Z.] Sun Yat Sen Univ, Sch Phys & Engn, Guangzhou 510275, Guangdong, Peoples R China. [Smirnova, L. N.; Turchikhin, S.] Moscow MV Lomonosov State Univ, Fac Phys, Moscow, Russia. [Toth, J.] Inst Particle & Nucl Phys, Wigner Res Ctr Phys, Budapest, Hungary. [Wildt, M. A.] Univ Hamburg, Inst Expt Phys, Hamburg, Germany. [Xu, L.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA. [Yacoob, S.] Univ KwaZulu Natal, Discipline Phys, Durban, South Africa. [Yusuff, I.] Univ Malaya, Dept Phys, Kuala Lumpur 59100, Malaysia. RP Blum, W (reprint author), Johannes Gutenberg Univ Mainz, Inst Phys, Mainz, Germany. RI Connell, Simon/F-2962-2015; Bosman, Martine/J-9917-2014; Joergensen, Morten/E-6847-2015; Mitsou, Vasiliki/D-1967-2009; Riu, Imma/L-7385-2014; Cabrera Urban, Susana/H-1376-2015; Mir, Lluisa-Maria/G-7212-2015; Marti-Garcia, Salvador/F-3085-2011; Della Pietra, Massimo/J-5008-2012; Cavalli-Sforza, Matteo/H-7102-2015; Petrucci, Fabrizio/G-8348-2012; Negrini, Matteo/C-8906-2014; Tartarelli, Giuseppe Francesco/A-5629-2016; Fassi, Farida/F-3571-2016; la rotonda, laura/B-4028-2016; White, Ryan/E-2979-2015; Wemans, Andre/A-6738-2012; Castro, Nuno/D-5260-2011; Boyko, Igor/J-3659-2013; Brooks, William/C-8636-2013; Nemecek, Stanislav/G-5931-2014; Gutierrez, Phillip/C-1161-2011; Di Domenico, Antonio/G-6301-2011; Ventura, Andrea/A-9544-2015; Livan, Michele/D-7531-2012; De, Kaushik/N-1953-2013; Smirnova, Oxana/A-4401-2013; Villa, Mauro/C-9883-2009; Goncalo, Ricardo/M-3153-2016; Gauzzi, Paolo/D-2615-2009; Mindur, Bartosz/A-2253-2017; Fabbri, Laura/H-3442-2012; Solodkov, Alexander/B-8623-2017; Zaitsev, Alexandre/B-8989-2017; Peleganchuk, Sergey/J-6722-2014; Li, Liang/O-1107-2015; Monzani, Simone/D-6328-2017; Korol, Aleksandr/A-6244-2014; Capua, Marcella/A-8549-2015; Perrino, Roberto/B-4633-2010; SULIN, VLADIMIR/N-2793-2015; Nechaeva, Polina/N-1148-2015; Vykydal, Zdenek/H-6426-2016; Olshevskiy, Alexander/I-1580-2016; Snesarev, Andrey/H-5090-2013; BESSON, NATHALIE/L-6250-2015; Vanadia, Marco/K-5870-2016; Ippolito, Valerio/L-1435-2016; Maneira, Jose/D-8486-2011; Prokoshin, Fedor/E-2795-2012; KHODINOV, ALEKSANDR/D-6269-2015; Staroba, Pavel/G-8850-2014; Gorelov, Igor/J-9010-2015; Gladilin, Leonid/B-5226-2011; Carvalho, Joao/M-4060-2013; Mashinistov, Ruslan/M-8356-2015; Buttar, Craig/D-3706-2011; Gonzalez de la Hoz, Santiago/E-2494-2016; Guo, Jun/O-5202-2015; Aguilar Saavedra, Juan Antonio/F-1256-2016; Leyton, Michael/G-2214-2016; Jones, Roger/H-5578-2011; Pacheco Pages, Andres/C-5353-2011; Vranjes Milosavljevic, Marija/F-9847-2016; Ferrer, Antonio/H-2942-2015; Grancagnolo, Sergio/J-3957-2015; Doyle, Anthony/C-5889-2009; spagnolo, stefania/A-6359-2012; Ciubancan, Liviu Mihai/L-2412-2015; Zhukov, Konstantin/M-6027-2015; Shmeleva, Alevtina/M-6199-2015; Gavrilenko, Igor/M-8260-2015; Tikhomirov, Vladimir/M-6194-2015; Yang, Haijun/O-1055-2015; Chekulaev, Sergey/O-1145-2015; Warburton, Andreas/N-8028-2013 OI Connell, Simon/0000-0001-6000-7245; Bosman, Martine/0000-0002-7290-643X; Joergensen, Morten/0000-0002-6790-9361; Mitsou, Vasiliki/0000-0002-1533-8886; Riu, Imma/0000-0002-3742-4582; Mir, Lluisa-Maria/0000-0002-4276-715X; Della Pietra, Massimo/0000-0003-4446-3368; Petrucci, Fabrizio/0000-0002-5278-2206; Negrini, Matteo/0000-0003-0101-6963; Di Micco, Biagio/0000-0002-4067-1592; Tartarelli, Giuseppe Francesco/0000-0002-4244-502X; Fassi, Farida/0000-0002-6423-7213; la rotonda, laura/0000-0002-6780-5829; Osculati, Bianca Maria/0000-0002-7246-060X; Amorim, Antonio/0000-0003-0638-2321; Giorgi, Filippo Maria/0000-0003-1589-2163; Coccaro, Andrea/0000-0003-2368-4559; White, Ryan/0000-0003-3589-5900; Wemans, Andre/0000-0002-9669-9500; Castro, Nuno/0000-0001-8491-4376; Boyko, Igor/0000-0002-3355-4662; Brooks, William/0000-0001-6161-3570; Di Domenico, Antonio/0000-0001-8078-2759; Ventura, Andrea/0000-0002-3368-3413; Livan, Michele/0000-0002-5877-0062; De, Kaushik/0000-0002-5647-4489; Smirnova, Oxana/0000-0003-2517-531X; Villa, Mauro/0000-0002-9181-8048; Goncalo, Ricardo/0000-0002-3826-3442; Gauzzi, Paolo/0000-0003-4841-5822; Mindur, Bartosz/0000-0002-5511-2611; Fabbri, Laura/0000-0002-4002-8353; Solodkov, Alexander/0000-0002-2737-8674; Zaitsev, Alexandre/0000-0002-4961-8368; Peleganchuk, Sergey/0000-0003-0907-7592; Li, Liang/0000-0001-6411-6107; Monzani, Simone/0000-0002-0479-2207; Korol, Aleksandr/0000-0001-8448-218X; Giordani, Mario/0000-0002-0792-6039; Capua, Marcella/0000-0002-2443-6525; Perrino, Roberto/0000-0002-5764-7337; SULIN, VLADIMIR/0000-0003-3943-2495; Vykydal, Zdenek/0000-0003-2329-0672; Olshevskiy, Alexander/0000-0002-8902-1793; Vanadia, Marco/0000-0003-2684-276X; Ippolito, Valerio/0000-0001-5126-1620; Maneira, Jose/0000-0002-3222-2738; Prokoshin, Fedor/0000-0001-6389-5399; KHODINOV, ALEKSANDR/0000-0003-3551-5808; Gorelov, Igor/0000-0001-5570-0133; Gladilin, Leonid/0000-0001-9422-8636; Carvalho, Joao/0000-0002-3015-7821; Mashinistov, Ruslan/0000-0001-7925-4676; Gonzalez de la Hoz, Santiago/0000-0001-5304-5390; Guo, Jun/0000-0001-8125-9433; Aguilar Saavedra, Juan Antonio/0000-0002-5475-8920; Leyton, Michael/0000-0002-0727-8107; Jones, Roger/0000-0002-6427-3513; Pacheco Pages, Andres/0000-0001-8210-1734; Vranjes Milosavljevic, Marija/0000-0003-4477-9733; Ferrer, Antonio/0000-0003-0532-711X; Grancagnolo, Sergio/0000-0001-8490-8304; Doyle, Anthony/0000-0001-6322-6195; spagnolo, stefania/0000-0001-7482-6348; Ciubancan, Liviu Mihai/0000-0003-1837-2841; Tikhomirov, Vladimir/0000-0002-9634-0581; Warburton, Andreas/0000-0002-2298-7315 FU ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWFW, Austria; FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq, Brazil; FAPESP, Brazil; NSERC, Canada; NRC, Canada; CFI, Canada; CERN; CONICYT, Chile; CAS, China; MOST, China; NSFC, China; COLCIENCIAS, Colombia; MSMT CR, Czech Republic; MPO CR, Czech Republic; VSC CR, Czech Republic; DNRF, Denmark; DNSRC, Denmark; Lundbeck Foundation, Denmark; EPLANET, European Union; ERC, European Union; NSRF, European Union; IN2P3-CNRS, France; CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, Germany; DFG, Germany; MPG, Germany; AvH Foundation, Germany; GSRT, Greece; NSRF, Greece; ISF, Israel; MINERVA, Israel; GIF, Israel; I-CORE, Israel; Benoziyo Center, Israel; INFN, Italy; MEXT, Japan; JSPS, Japan; CNRST, Morocco; FOM, Netherlands; NWO, Netherlands; BRF, Norway; RCN, Norway; MNiSW, Poland; NCN, Poland; GRICES, Portugal; FCT, Portugal; MNE/IFA, Romania; MES of Russia; ROSATOM, Russian Federation; JINR; MSTD, Serbia; MSSR, Slovakia; ARRS, Slovenia; MIZS, Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC, Sweden; Wallenberg Foundation, Sweden; SER, Switzerland; SNSF, Switzerland; Canton of Bern, Switzerland; Canton of Geneva, Switzerland; NSC, Taiwan; TAEK, Turkey; STFC, United Kingdom; Royal Society, United Kingdom; Leverhulme Trust, United Kingdom; DOE, United States of America; NSF, United States of America FX We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWFW and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile; CAS, MOST and NSFC, China; COLCIENCIAS, Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF, DNSRC and Lundbeck Foundation, Denmark; EPLANET, ERC and NSRF, European Union; IN2P3-CNRS, CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, DFG, HGF, MPG and AvH Foundation, Germany; GSRT and NSRF, Greece; ISF, MINERVA, GIF, I-CORE and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; FOM and NWO, Netherlands; BRF and RCN, Norway; MNiSW and NCN, Poland; GRICES and FCT, Portugal; MNE/IFA, Romania; MES of Russia and ROSATOM, Russian Federation; JINR; MSTD, Serbia; MSSR, Slovakia; ARRS and MIZS, Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC and Wallenberg Foundation, Sweden; SER, SNSF and Cantons of Bern and Geneva, Switzerland; NSC, Taiwan; TAEK, Turkey; STFC, the Royal Society and Leverhulme Trust, United Kingdom; DOE and NSF, United States of America. NR 46 TC 88 Z9 88 U1 10 U2 86 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0370-2693 EI 1873-2445 J9 PHYS LETT B JI Phys. Lett. B PD NOV 10 PY 2014 VL 738 BP 428 EP 447 DI 10.1016/j.physletb.2014.10.002 PG 20 WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AT0KK UT WOS:000344624900065 ER PT J AU Shi, C Chang, L Roberts, CD Schmidt, SM Tandy, PC Zong, HS AF Shi, Chao Chang, Lei Roberts, Craig D. Schmidt, Sebastian M. Tandy, Peter C. Zong, Hong-shi TI Flavour symmetry breaking in the kaon parton distribution amplitude SO PHYSICS LETTERS B LA English DT Article DE Dynamical chiral symmetry breaking; Dyson-Schwinger equations; Factorisation in heavy-meson decays; Flavour symmetry breaking; Light pseudoscalar mesons; Parton distribution amplitudes; Strange quarks ID DYSON-SCHWINGER EQUATIONS; PION FORM-FACTOR; QUANTUM CHROMODYNAMICS; EXCLUSIVE PROCESSES; SU(3) BREAKING; QCD; MESONS; FACTORIZATION; CONFINEMENT; BEHAVIOR AB We compute the kaon's valence-quark (twist-two parton) distribution amplitude (PDA) by projecting its Poincare-covariant Bethe-Salpeter wave-function onto the light-front. At a scale zeta = 2GeV, the PDA is abroad, concave and asymmetric function, whose peak is shifted 12-16% away from its position in QCD's conformal limit. These features are a clear expression of SU(3)-flavour-symmetry breaking. They show that the heavier quark in the kaon carries more of the bound-state's momentum than the lighter quark and also that emergent phenomena in QCD modulate the magnitude of flavour-symmetry breaking: it is markedly smaller than one might expect based on the difference between light-quark current masses. Our results add to a body of evidence which indicates that at any energy scale accessible with existing or foreseeable facilities, a reliable guide to the interpretation of experiment requires the use of such nonperturbatively broadened PDAs in leading-order, leading-twist formulae for hard exclusive processes instead of the asymptotic PDA associated with QCD's conformal limit. We illustrate this via the ratio of kaon and pion electromagnetic form factors: using our nonperturbative PDAs in the appropriate formulae, F-K/F-pi = 1.23 at spacelike-Q(2) = 17 GeV2, which compares satisfactorily with the value of 0.92(5) inferred in e(+)e(-) annihilation at s = 17GeV(2). (C) 2014 Argonne National Laboratory and the authors. Published by Elsevier B. V. C1 [Shi, Chao] Nanjing Univ, Inst Acoust, Key Lab Modern Acoust, MOE, Nanjing 210093, Jiangsu, Peoples R China. [Shi, Chao; Zong, Hong-shi] Nanjing Univ, Dept Phys, Nanjing 210093, Jiangsu, Peoples R China. [Chang, Lei] Univ Adelaide, Sch Chem & Phys, CSSM, Adelaide, SA 5005, Australia. [Roberts, Craig D.] Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA. [Tandy, Peter C.] Kent State Univ, Ctr Rech Nucl, Dept Phys, Kent, OH USA. [Schmidt, Sebastian M.] Forschungszentrum Julich, Inst Adv Simulat, D-52425 Julich, Germany. [Zong, Hong-shi] Chinese Acad Sci, Inst Theoret Phys, State Key Lab Theoret Phys, Beijing 100190, Peoples R China. [Zong, Hong-shi] Joint Ctr Particle Nucl Phys & Cosmol, Nanjing 210093, Jiangsu, Peoples R China. [Schmidt, Sebastian M.] JARA, D-52425 Julich, Germany. RP Roberts, CD (reprint author), Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA. FU International Fellow Award from the Helmholtz Association; National Natural Science Foundation of China [11275097, 11274166]; National Basic Research Program of China [2012CB921504]; Research Fund for the Doctoral Program of Higher Education (China) [2012009111002]; University of Adelaide; Australian Research Council [FL0992247]; Department of Energy, Office of Nuclear Physics [DE-AC02-06CH11357]; Forschungszentrum Julich GmbH; National Science Foundation [NSF-PHY1206187] FX We benefited from insightful comments by I. C. Cloet, B. El-Bennich, R.J. Holt, G. Krein, J. Segovia and A. W. Thomas; and from the opportunity to participate (L. C., C. D. R., P. C. T.) in the workshops "Many Manifestations of Nonperturbative QCD under the Southern Cross", Ubatuba, Sao Paulo, and (C. D. R., P. C. T.) the "2nd Workshop on Perspectives in Nonperturbative QCD" at IFT-UNESP, Sao Paulo, during both of which a substantial body of this work was completed. C. D. R. acknowledges support from an International Fellow Award from the Helmholtz Association; and research otherwise supported by: the National Natural Science Foundation of China (grant Nos. 11275097 and 11274166); the National Basic Research Program of China (grant No. 2012CB921504); the Research Fund for the Doctoral Program of Higher Education (China, grant No. 2012009111002); University of Adelaide and Australian Research Council through grant No. FL0992247; Department of Energy, Office of Nuclear Physics, contract No. DE-AC02-06CH11357; Forschungszentrum Julich GmbH; and National Science Foundation, grant No. NSF-PHY1206187. NR 66 TC 11 Z9 11 U1 0 U2 2 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0370-2693 EI 1873-2445 J9 PHYS LETT B JI Phys. Lett. B PD NOV 10 PY 2014 VL 738 BP 512 EP 518 DI 10.1016/j.physletb.2014.07.057 PG 7 WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AT0KK UT WOS:000344624900077 ER PT J AU Campione, S de Ceglia, D Guclu, C Vincenti, MA Scalora, M Capolino, F AF Campione, Salvatore de Ceglia, Domenico Guclu, Caner Vincenti, Maria A. Scalora, Michael Capolino, Filippo TI Fano collective resonance as complex mode in a two-dimensional planar metasurface of plasmonic nanoparticles SO APPLIED PHYSICS LETTERS LA English DT Article ID LEAKY MODES; NANOCLUSTERS; NANOSPHERES; CLUSTERS AB Fano resonances are features in transmissivity/reflectivity/absorption that owe their origin to the interaction between a broad bright resonance and a dark (i.e., sub-radiant) narrower one. They may emerge in the optical properties of planar two-dimensional (2D) periodic arrays (metasurfaces) of plasmonic nanoparticles. In this letter, we provide a thorough assessment of their nature for the general case of normal and oblique plane wave incidence, highlighting when a Fano resonance is affected by the mutual coupling in an array and its capability to support free modal solutions. We analyze the representative case of a metasurface of plasmonic nanoshells at ultraviolet frequencies and compute its absorption under TE- and TM-polarized, oblique plane-wave incidence. In particular, we find that plasmonic metasurfaces display two distinct types of resonances observable as absorption peaks: one is related to the Mie electric dipolar resonance of each nanoparticle and the other is due to the forced excitation of free modes with small attenuation constant, usually found at oblique incidence. The latter is thus an array-induced collective Fano resonance. This realization opens up to manifold flexible designs at optical frequencies mixing individual and collective resonances. We explain the physical origin of such Fano resonances using the modal analysis through which we calculate the free modes with complex wavenumber supported by the metasurface. We define equivalent array dipolar polarizabilities that are directly related to the absorption physics at oblique incidence and show a direct dependence between array modal phase and attenuation constants and Fano resonances. We thus provide a more complete picture of Fano resonances that may lead to the design of filters, energy-harvesting devices, photodetectors, and sensors at ultraviolet frequencies. Similar resonances may be also extended to the visible range with an appropriate choice of geometries and materials. (C) 2014 AIP Publishing LLC. C1 [Campione, Salvatore; Guclu, Caner; Capolino, Filippo] Univ Calif Irvine, Dept Elect Engn & Comp Sci, Irvine, CA 92697 USA. [de Ceglia, Domenico; Vincenti, Maria A.] Natl Res Council AMRDEC, Charles M Bowden Res Lab, Redstone Arsenal, AL 35898 USA. [Scalora, Michael] US Army RDECOM, AMRDEC, Charles M Bowden Res Lab, Redstone Arsenal, AL 35898 USA. RP Campione, S (reprint author), Sandia Natl Labs, Ctr Integrated Nanotechnol, POB 5800, Albuquerque, NM 87185 USA. EM sncampi@sandia.gov; f.capolino@uci.edu RI Campione, Salvatore/A-2349-2015 OI Campione, Salvatore/0000-0003-4655-5485 FU National Science Foundation [CM.MI-1101074]; National Research Council Research Associateship award at the U.S. Army Aviation and Missile Research Development and Engineering Center FX S.C., C. G., and F. C. acknowledge partial support from the National Science Foundation under Grant No. CM.MI-1101074. This research was performed while the authors D.d.C. and M. A. V. held a National Research Council Research Associateship award at the U.S. Army Aviation and Missile Research Development and Engineering Center. NR 32 TC 8 Z9 8 U1 7 U2 80 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0003-6951 EI 1077-3118 J9 APPL PHYS LETT JI Appl. Phys. Lett. PD NOV 10 PY 2014 VL 105 IS 19 AR 191107 DI 10.1063/1.4901183 PG 5 WC Physics, Applied SC Physics GA AT8YZ UT WOS:000345216100007 ER PT J AU Kanesue, T Fuwa, Y Kondo, K Okamura, M AF Kanesue, Takeshi Fuwa, Yasuhiro Kondo, Kotaro Okamura, Masahiro TI Laser ion source with solenoid field SO APPLIED PHYSICS LETTERS LA English DT Article ID MAGNETIC-FIELD; PLASMA AB Pulse length extension of highly charged ion beam generated from a laser ion source is experimentally demonstrated. The laser ion source (LIS) has been recognized as one of the most powerful heavy ion source. However, it was difficult to provide long pulse beams. By applying a solenoid field (90 mT, 1m) at plasma drifting section, a pulse length of carbon ion beam reached 3.2 mu s which was 4.4 times longer than the width from a conventional LIS. The particle number of carbon ions accelerated by a radio frequency quadrupole linear accelerator was 1.2 x 10(11), which was provided by a single 1 J Nd-YAG laser shot. A laser ion source with solenoid field could be used in a next generation heavy ion accelerator. (C) 2014 AIP Publishing LLC. C1 [Kanesue, Takeshi; Okamura, Masahiro] Brookhaven Natl Lab, Collider Accelerator Dept, Upton, NY 11973 USA. [Fuwa, Yasuhiro] Kyoto Univ, Grad Sch Sci, Sakyo Ku, Kyoto 6067501, Japan. [Fuwa, Yasuhiro] RIKEN, Wako, Saitama 3510198, Japan. [Kondo, Kotaro] Tokyo Inst Technol, Nucl Reactors Res Lab, Meguro Ku, Tokyo 1528550, Japan. RP Kanesue, T (reprint author), Brookhaven Natl Lab, Collider Accelerator Dept, Upton, NY 11973 USA. EM tkanesue@bnl.gov FU U.S. Department of Energy; RIKEN; Japan Society for Promotion of Science FX This work was supported by U.S. Department of Energy, RIKEN, and Japan Society for Promotion of Science. NR 17 TC 6 Z9 6 U1 1 U2 4 PU AMER INST PHYSICS PI MELVILLE PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA SN 0003-6951 EI 1077-3118 J9 APPL PHYS LETT JI Appl. Phys. Lett. PD NOV 10 PY 2014 VL 105 IS 19 AR 193506 DI 10.1063/1.4902021 PG 4 WC Physics, Applied SC Physics GA AT8YZ UT WOS:000345216100080 ER PT J AU Lindemann, WR Wang, WJ Fungura, F Shinar, J Shinar, R Vaknin, D AF Lindemann, William R. Wang, Wenjie Fungura, Fadzai Shinar, Joseph Shinar, Ruth Vaknin, David TI The effect of cesium carbonate on 1-(3-methoxycarbonyl)propyl-1-phenyl[6,6]C-61 aggregation in films SO APPLIED PHYSICS LETTERS LA English DT Article ID HETEROJUNCTION SOLAR-CELLS; C-60-PROPYLAMINE ADDUCT MONOLAYERS; CATHODE INTERFACIAL LAYER; SHORT-CIRCUIT CURRENT; X-RAY; ORGANIC PHOTOVOLTAICS; POLYMER; EFFICIENCY; NEUTRON AB Surface-pressure versus molecular area isotherms, X-ray reflectivity, and X-ray near-total reflection fluorescence were used to study the properties of 1-(3-methoxycarbonyl)propyl-1-phenyl[6,6]C-61 (PCBM) that was pre-mixed with cesium carbonate and spread as a film at the air-water interface. The pre-mixed PCBM with cesium carbonate demonstrated a strikingly strong effect on the organization of the film. Whereas films formed from pure PCBM solution were rough due to strong inter-molecular interactions, the films formed from the mixture were much smoother. This indicates that the cesium carbonate moderates the inter-molecular interactions among PCBM molecules, hinting that the cesium diffusion observed in inverted organic photovoltaic structures and the likely ensuing ionic Cs-PCBM interaction decrease aggregation tendency of PCBM. This implies that the use of cesium salts affects the morphology of the organic layer and consequently improves the efficiency of these devices. (C) 2014 AIP Publishing LLC. C1 [Lindemann, William R.; Wang, Wenjie; Shinar, Joseph; Vaknin, David] Iowa State Univ, Ames Lab, Ames, IA 50011 USA. [Lindemann, William R.; Wang, Wenjie; Shinar, Joseph; Vaknin, David] Iowa State Univ, Dept Phys & Astron, Ames, IA 50011 USA. [Fungura, Fadzai; Shinar, Ruth] Iowa State Univ, Microelect Res Ctr, Ames, IA 50011 USA. [Fungura, Fadzai; Shinar, Ruth] Iowa State Univ, Dept Elect & Comp Engn, Ames, IA 50011 USA. RP Shinar, R (reprint author), Iowa State Univ, Microelect Res Ctr, Ames, IA 50011 USA. EM rshinar@iastate.edu; vaknin@ameslab.gov RI Vaknin, David/B-3302-2009; OI Vaknin, David/0000-0002-0899-9248; Lindemann, William/0000-0002-5967-3192 FU Office of Basic Energy Sciences, U.S. Department of Energy [DE-AC02-07CH11358]; U.S. Department of Energy Science Undergraduate Laboratory Internship (SULI) Program under Iowa State University [DE-AC02-07CH11358]; Iowa Energy Center FX We thank Eric Grieser for help with experiments. The work at Ames Laboratory was supported by the Office of Basic Energy Sciences, U.S. Department of Energy under Contract No. DE-AC02-07CH11358 and by the U.S. Department of Energy Science Undergraduate Laboratory Internship (SULI) Program under its contract with Iowa State University, Contract No. DE-AC02-07CH11358. William Lindemann is grateful to the DOE for the assistantship and opportunity to participate in the SULI program. R. Shinar acknowledges partial support of the Iowa Energy Center. NR 28 TC 0 Z9 0 U1 0 U2 5 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0003-6951 EI 1077-3118 J9 APPL PHYS LETT JI Appl. Phys. Lett. PD NOV 10 PY 2014 VL 105 IS 19 AR 191605 DI 10.1063/1.4901444 PG 5 WC Physics, Applied SC Physics GA AT8YZ UT WOS:000345216100024 ER PT J AU Yang, SM Okatan, MB Paranthaman, MP Jesse, S Noh, TW Kalinin, SV AF Yang, Sang Mo Okatan, M. Baris Paranthaman, M. Parans Jesse, Stephen Noh, Tae Won Kalinin, Sergei V. TI Second harmonic detection in the electrochemical strain microscopy of Ag-ion conducting glass SO APPLIED PHYSICS LETTERS LA English DT Article ID NANOSCALE; RESOLUTION; DIFFUSION; AGI-AGPO3; SOLIDS AB The first and second harmonic electromechanical responses and their cross-correlation in Ag-ion conducting glass were investigated using band-excitation electrochemical strain microscopy (ESM). Consecutive ESM images with increasing magnitudes of the applied AC voltage allowed observation of not only reversible surface displacement but also irreversible silver nanoparticle formation above a certain threshold voltage. The second harmonic ESM response was anti-correlated with the first harmonic response in many local regions. Furthermore, the nucleation sites of silver nanoparticles were closely related to the anti-correlated regions, specifically, with low second harmonic and high first harmonic ESM responses. The possible origins of the second harmonic ESM response are discussed. (C) 2014 AIP Publishing LLC. C1 [Yang, Sang Mo; Noh, Tae Won] Inst for Basic Sci Korea, Ctr Correlated Electron Syst, Seoul 151742, South Korea. [Yang, Sang Mo; Noh, Tae Won] Seoul Natl Univ, Dept Phys & Astron, Seoul 151742, South Korea. [Yang, Sang Mo; Okatan, M. Baris; Jesse, Stephen; Kalinin, Sergei V.] Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA. [Paranthaman, M. Parans] Oak Ridge Natl Lab, Div Chem Sci, Oak Ridge, TN 37831 USA. RP Yang, SM (reprint author), Inst for Basic Sci Korea, Ctr Correlated Electron Syst, Seoul 151742, South Korea. EM yangs@ornl.gov RI Paranthaman, Mariappan/N-3866-2015; Yang, Sang Mo/Q-2455-2015; Kalinin, Sergei/I-9096-2012; Jesse, Stephen/D-3975-2016; Okatan, M. Baris/E-1913-2016 OI Paranthaman, Mariappan/0000-0003-3009-8531; Yang, Sang Mo/0000-0003-1809-2938; Kalinin, Sergei/0000-0001-5354-6152; Jesse, Stephen/0000-0002-1168-8483; Okatan, M. Baris/0000-0002-9421-7846 FU Center for Nanophase Materials Sciences, which is a DOE Office of Science User Facility; DOE Presidential Early Career for Scientists and Engineers; Materials Sciences and Engineering Division, Office of Basic Energy Sciences, U.S. Department of Energy [IBS-R009-D1] FX This research was conducted at and partially supported by (M.B.O., S.J., and S. V. K.) the Center for Nanophase Materials Sciences, which is a DOE Office of Science User Facility. Support (S.M.Y. and S. V. K.) was also provided by a DOE Presidential Early Career for Scientists and Engineers. This research was also partially supported (S.M.Y. and T.W.N.) by IBS-R009-D1, Korea. Materials synthesis work (M. P. P.) was sponsored by the Materials Sciences and Engineering Division, Office of Basic Energy Sciences, U.S. Department of Energy. Thanks are due to Dr. Zhonghe Bi for initial help with synthesis and Dr. Miaofang Chi with microscopy work. NR 29 TC 4 Z9 4 U1 2 U2 24 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0003-6951 EI 1077-3118 J9 APPL PHYS LETT JI Appl. Phys. Lett. PD NOV 10 PY 2014 VL 105 IS 19 AR 193106 DI 10.1063/1.4901736 PG 5 WC Physics, Applied SC Physics GA AT8YZ UT WOS:000345216100066 ER PT J AU Yu, WL Jiang, YX Huan, C Chen, XC Jiang, ZG Hawkins, SD Klem, JF Pan, W AF Yu, Wenlong Jiang, Yuxuan Huan, Chao Chen, Xunchi Jiang, Zhigang Hawkins, Samuel D. Klem, John F. Pan, Wei TI Superconducting proximity effect in inverted InAs/GaSb quantum well structures with Ta electrodes SO APPLIED PHYSICS LETTERS LA English DT Article ID MAJORANA FERMIONS; CONDUCTANCE; NANOWIRE; JUNCTIONS; SIGNATURE AB We present our recent electronic transport results in top-gated InAs/GaSb quantum well hybrid structures with superconducting Ta electrodes. We show that the transport across the InAs-Ta junction depends largely on the interfacial transparency, exhibiting distinct zero-bias behavior. For a relatively resistive interface, a broad conductance peak is observed at zero bias. When a transparent InAs-Ta interface is achieved, a zero-bias conductance dip appears with two coherent-peak-like features forming at bias voltages corresponding to the superconducting gap of Ta. The conductance spectra of the transparent InAs-Ta junction at different gate voltages can be fit well using the standard Blonder-Tinkham-Klapwijk theory. (C) 2014 AIP Publishing LLC. C1 [Yu, Wenlong; Jiang, Yuxuan; Huan, Chao; Chen, Xunchi; Jiang, Zhigang] Georgia Inst Technol, Sch Phys, Atlanta, GA 30332 USA. [Hawkins, Samuel D.; Klem, John F.; Pan, Wei] Sandia Natl Labs, Albuquerque, NM 87185 USA. RP Jiang, ZG (reprint author), Georgia Inst Technol, Sch Phys, Atlanta, GA 30332 USA. EM zhigang.jiang@physics.gatech.edu; wpan@sandia.gov FU LDRD at Sandia; U.S. Department of Energy, Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division; U.S. Department of Energy, Office of Basic Energy Sciences user facility at Los Alamos National Laboratory [DE-AC52-06NA25396]; Sandia National Laboratories [DE-AC04-94AL85000]; United States Department of Energy's National Nuclear Security Administration [DE-AC04-94AL85000] FX We thank Rui-Rui Du for helpful discussions and Mark Overberg for wafer growth. This work is jointly supported by LDRD at Sandia and by the U.S. Department of Energy, Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division. Device fabrication was performed, in part, at the Center for Integrated Nanotechnologies, a U.S. Department of Energy, Office of Basic Energy Sciences user facility at Los Alamos National Laboratory (Contract DE-AC52-06NA25396) and Sandia National Laboratories (Contract DE-AC04-94AL85000). Sandia National Laboratories is a multi-program laboratory managed and operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the United States Department of Energy's National Nuclear Security Administration under Contract No. DE-AC04-94AL85000. NR 34 TC 1 Z9 1 U1 3 U2 15 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0003-6951 EI 1077-3118 J9 APPL PHYS LETT JI Appl. Phys. Lett. PD NOV 10 PY 2014 VL 105 IS 19 AR 192107 DI 10.1063/1.4901965 PG 5 WC Physics, Applied SC Physics GA AT8YZ UT WOS:000345216100045 ER PT J AU Zhivun, E Wickenbrock, A Patton, B Budker, D AF Zhivun, Elena Wickenbrock, Arne Patton, Brian Budker, Dmitry TI Alkali-vapor magnetic resonance driven by fictitious radiofrequency fields SO APPLIED PHYSICS LETTERS LA English DT Article ID ATOMIC VAPOR; GROUND-STATE; LIGHT SHIFTS; LASER; STABILIZATION; ECHOES; SODIUM; DIODE AB We demonstrate an all-optical Cs-133 scalar magnetometer, operating in nonzero magnetic field, in which the magnetic resonance is driven by an effective oscillating magnetic field provided by the AC Stark shift of an intensity-modulated laser beam. We achieve a projected shot-noise-limited sensitivity of 1.7fT/root Hz and measure a technical noise floor of 40fT/root Hz. These results are essentially identical to a coil-driven scalar magnetometer using the same setup. This all-optical scheme offers advantages over traditional coil-driven magnetometers for use in arrays and in magnetically sensitive fundamental physics experiments, e. g., searches for a permanent electric dipole moment of the neutron. (C) 2014 AIP Publishing LLC. C1 [Zhivun, Elena; Patton, Brian; Budker, Dmitry] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA. [Wickenbrock, Arne] Johannes Gutenberg Univ Mainz, Inst Phys, D-55128 Mainz, Germany. [Patton, Brian] Tech Univ Munich, Phys Dept, D-85748 Garching, Germany. [Budker, Dmitry] Johannes Gutenberg Univ Mainz, Helmholtz Inst, D-55099 Mainz, Germany. [Budker, Dmitry] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Nucl Sci, Berkeley, CA 94720 USA. RP Wickenbrock, A (reprint author), Johannes Gutenberg Univ Mainz, Inst Phys, D-55128 Mainz, Germany. EM wickenbr@uni-mainz.de RI Budker, Dmitry/F-7580-2016 OI Budker, Dmitry/0000-0002-7356-4814 FU Marie Curie International Research Staff Exchange Scheme Fellowship, FP7 "Coherent optics sensors for medical applications-COSMA"; DFG [SPP1491] FX A.W. was supported by the Marie Curie International Research Staff Exchange Scheme Fellowship, FP7 "Coherent optics sensors for medical applications-COSMA." B.P. was supported by DFG Priority Program SPP1491, Precision Measurements with Cold and Ultracold Neutrons. Dedicated to Professor William Happer on the occasion of his 75th birthday. NR 38 TC 4 Z9 4 U1 0 U2 19 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0003-6951 EI 1077-3118 J9 APPL PHYS LETT JI Appl. Phys. Lett. PD NOV 10 PY 2014 VL 105 IS 19 AR 192406 DI 10.1063/1.4902028 PG 4 WC Physics, Applied SC Physics GA AT8YZ UT WOS:000345216100051 ER PT J AU Vinson, J Jach, T Elam, WT Denlinger, JD AF Vinson, John Jach, Terrence Elam, W. T. Denlinger, J. D. TI Origins of extreme broadening mechanisms in near-edge x-ray spectra of nitrogen compounds SO PHYSICAL REVIEW B LA English DT Article ID DENSITY-FUNCTIONAL THEORY; MOLECULES; PSEUDOPOTENTIALS; PHOTOEMISSION; SPECTROSCOPY; EXCITATIONS; ABSORPTION AB We demonstrate the observation of many-body lifetime effects in valence-band x-ray emission. A comparison of the N K alpha emission of crystalline ammonium nitrate to molecular-orbital calculations revealed an unexpected, extreme broadening of the NO sigma recombination-so extensively as to virtually disappear. GW calculations establish that this disappearance is due to a large imaginary component of the self-energy associated with the NO s orbitals. Building upon density-functional theory, we have calculated radiative transitions from the nitrogen 1s level of ammonium nitrate and ammonium chloride using a Bethe-Salpeter method to include electron-hole interactions. The absorption and emission spectra of both crystals evince large, orbital-dependent sensitivity to molecular dynamics. We demonstrate that many-body effects as well as thermal and zero-point motion are vital for understanding observed spectra. A computational approach using average atomic positions and uniform broadening to account for lifetime and phonon effects is unsatisfactory. C1 [Vinson, John; Jach, Terrence] NIST, Mat Measurement Lab, Gaithersburg, MD 20899 USA. [Elam, W. T.] Univ Washington, Appl Phys Lab, Seattle, WA 98195 USA. [Denlinger, J. D.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94720 USA. RP Vinson, J (reprint author), NIST, Mat Measurement Lab, Gaithersburg, MD 20899 USA. OI Vinson, John/0000-0002-7619-7060 FU Office of Naval Research [N00014-05-1-0843]; Office of Science, Office of Basic Energy Sciences, of the U.S. Department of Energy [DE-AC02-05CH11231] FX This work was supported in part by the Office of Naval Research under Grant No. N00014-05-1-0843 (W.T.E.). The Advanced Light Source is supported by the Director, Office of Science, Office of Basic Energy Sciences, of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. The authors wish to thank Dr. Eric Shirley for helpful discussions. Certain software packages are identified in this paper to foster understanding. Such identification does not imply recommendation or endorsement by the National Institute of Standards and Technology, nor does it imply that these are necessarily the best available for the purpose. NR 43 TC 3 Z9 3 U1 3 U2 27 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 2469-9950 EI 2469-9969 J9 PHYS REV B JI Phys. Rev. B PD NOV 10 PY 2014 VL 90 IS 20 AR 205207 DI 10.1103/PhysRevB.90.205207 PG 6 WC Physics, Condensed Matter SC Physics GA AT4NK UT WOS:000344915800008 ER PT J AU Massarczyk, R Rusev, G Schwengner, R Donau, F Bhatia, C Gooden, ME Kelley, JH Tonchev, AP Tornow, W AF Massarczyk, R. Rusev, G. Schwengner, R. Doenau, F. Bhatia, C. Gooden, M. E. Kelley, J. H. Tonchev, A. P. Tornow, W. TI Magnetic dipole strength in Xe-128 and Xe-134 in the spin-flip resonance region SO PHYSICAL REVIEW C LA English DT Article ID NUCLEI; NEUTRON; DEFORMATION; EXCITATIONS; ISOTOPES; FACILITY; SM-154; WIDTH AB The magnetic dipole strength in the energy region of the spin-flip resonance is investigated in Xe-128 and Xe-134 using quasimonoenergetic and linearly polarized gamma-ray beams at the High-Intensity gamma-Ray Source facility in Durham, North Carolina, USA. Absorption cross sections were deduced for the magnetic and electric and dipole strength distributions separately for various intervals of excitation energy, including the strength of states in the unresolved quasicontinuum. The magnetic dipole strength distributions show structures resembling a resonance in the spin-flip region around an excitation energy of 8 MeV. The electric dipole strength distributions obtained from the present experiments are in agreement with the ones deduced from an earlier experiment using broad-band bremsstrahlung instead of a quasimonoenergetic beam. The experimental magnetic and electric dipole strength distributions are compared with phenomenological approximations and with predictions of a quasiparticle random phase approximation in a deformed basis. C1 [Massarczyk, R.; Schwengner, R.; Doenau, F.] Helmholtz Zentrum Dresden Rossendorf, D-01328 Dresden, Germany. [Massarczyk, R.] Tech Univ Dresden, D-01062 Dresden, Germany. [Rusev, G.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA. [Bhatia, C.] McMaster Univ, Hamilton, ON L8S 4L8, Canada. [Gooden, M. E.; Kelley, J. H.; Tornow, W.] Triangle Univ Nucl Lab, Durham, NC 27708 USA. [Gooden, M. E.; Kelley, J. H.] N Carolina State Univ, Raleigh, NC 27695 USA. [Tonchev, A. P.] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA. [Tornow, W.] Duke Univ, Durham, NC 27708 USA. RP Massarczyk, R (reprint author), Los Alamos Natl Lab, POB 1663, Los Alamos, NM 87545 USA. EM r.massarczyk@hzdr.de OI Rusev, Gencho/0000-0001-7563-1518 FU German Research Foundation (DFG) [SCHW883/1-1]; EURATOM FP7 Project ERINDA [FP7-269499]; U.S. Department of Energy, Office of Nuclear Physics [DE-FG02-97ER41033, DE-FG02-97ER41042] FX We thank A. Hartmann for the target preparation and the crew of the HI gamma S facility for their collaboration during the experiments. This work was supported by the German Research Foundation (DFG), Project No. SCHW883/1-1 and EURATOM FP7 Project ERINDA (FP7-269499). Partial support was also given by the U.S. Department of Energy, Office of Nuclear Physics, under Grants No. DE-FG02-97ER41033 and No. DE-FG02-97ER41042. NR 44 TC 4 Z9 4 U1 0 U2 5 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0556-2813 EI 1089-490X J9 PHYS REV C JI Phys. Rev. C PD NOV 10 PY 2014 VL 90 IS 5 AR 054310 DI 10.1103/PhysRevC.90.054310 PG 6 WC Physics, Nuclear SC Physics GA AT4NO UT WOS:000344916400005 ER PT J AU Cherwinka, J Grant, D Halzen, F Heeger, KM Hsu, L Hubbard, AJF Karle, A Kauer, M Kudryavtsev, VA Macdonald, C Maruyama, RH Paling, S Pettus, W Pierpoint, ZP Reilly, BN Robinson, M Sandstrom, P Spooner, NJC Telfer, S Yang, L AF Cherwinka, J. Grant, D. Halzen, F. Heeger, K. M. Hsu, L. Hubbard, A. J. F. Karle, A. Kauer, M. Kudryavtsev, V. A. Macdonald, C. Maruyama, R. H. Paling, S. Pettus, W. Pierpoint, Z. P. Reilly, B. N. Robinson, M. Sandstrom, P. Spooner, N. J. C. Telfer, S. Yang, L. CA DM Ice Collaboration TI First data from DM-Ice17 SO PHYSICAL REVIEW D LA English DT Article ID DARK-MATTER CANDIDATES; NAIAD EXPERIMENT; CROSS-SECTIONS; ICECUBE; CONSTRAINTS; PARTICLES; SCINTILLATION; PERFORMANCE; DAMA/LIBRA; MODULATION AB We report the first analysis of background data from DM-Ice17, a direct-detection dark matter experiment consisting of 17 kg of NaI(Tl) target material. It was codeployed with IceCube 2457 m deep in the South Pole glacial ice in December 2010 and is the first such detector operating in the Southern Hemisphere. The background rate in the 6.5-8.0 keV(ee) region is measured to be 7.9 +/- 0.4 counts/day/keV/kg. This is consistent with the expected background from the detector assemblies with negligible contributions from the surrounding ice. The successful deployment and operation of DM-Ice17 establishes the South Pole ice as a viable location for future underground, low-background experiments in the Southern Hemisphere. The detector assembly and deployment are described here, as well as the analysis of the DM-Ice17 backgrounds based on data from the first two years of operation after commissioning, July 2011-June 2013. C1 [Cherwinka, J.] Univ Wisconsin, Phys Sci Lab, Stoughton, WI 53589 USA. [Grant, D.] Univ Alberta, Dept Phys, Edmonton, AB, Canada. [Halzen, F.; Hubbard, A. J. F.; Karle, A.; Kauer, M.; Pettus, W.; Pierpoint, Z. P.; Reilly, B. N.; Sandstrom, P.] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA. [Halzen, F.; Hubbard, A. J. F.; Karle, A.; Kauer, M.; Pettus, W.; Pierpoint, Z. P.; Reilly, B. N.; Sandstrom, P.] Univ Wisconsin, Wisconsin IceCube Particle Astrophys Ctr, Madison, WI 53706 USA. [Heeger, K. M.; Hubbard, A. J. F.; Kauer, M.; Maruyama, R. H.; Pettus, W.; Pierpoint, Z. P.; Reilly, B. N.] Yale Univ, Dept Phys, New Haven, CT 06520 USA. [Hsu, L.] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA. [Kudryavtsev, V. A.; Macdonald, C.; Robinson, M.; Spooner, N. J. C.; Telfer, S.] Univ Sheffield, Dept Phys & Astron, Sheffield, S Yorkshire, England. [Paling, S.] STFC Boulby Underground Sci Facil, Boulby Mine, Cleveland, England. [Yang, L.] Univ Illinois, Dept Phys, Urbana, IL 61801 USA. RP Cherwinka, J (reprint author), Univ Wisconsin, Phys Sci Lab, Stoughton, WI 53589 USA. EM reina.maruyama@yale.edu RI Maruyama, Reina/A-1064-2013; OI Maruyama, Reina/0000-0003-2794-512X; Pettus, Walter/0000-0003-4947-7400; Kudryavtsev, Vitaly/0000-0002-7018-5827 FU NSF [PLR-1046816, PHY-1151795]; Wisconsin IceCube Particle Astrophysics Center; Wisconsin Alumni Research Foundation; Yale University; Natural Sciences and Engineering Research Council of Canada; Fermilab; Fermi Research Alliance, LLC [DE-AC02-07CH11359]; U.S. Department of Energy; DOE/NNSA Stewardship Science Graduate Fellowship [DE-FC52-08NA28752]; NSF Graduate Research Fellowship [DGE-1256259] FX We thank the IceCube Collaboration and construction team for their support in the successful deployment of the detector and on-going detector monitoring and data management. We thank the support from SNOLAB for their efforts on the low-background measurements, and STFC and the Boulby mine company CPL for support of low-background measurements of NaI. This work was supported by the NSF Grants No. PLR-1046816 and No. PHY-1151795, Wisconsin IceCube Particle Astrophysics Center, the Wisconsin Alumni Research Foundation, Yale University, the Natural Sciences and Engineering Research Council of Canada, and Fermilab, operated by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the U.S. Department of Energy. W. P. and A. H. are supported by the DOE/NNSA Stewardship Science Graduate Fellowship (Grant No. DE-FC52-08NA28752) and NSF Graduate Research Fellowship (Grant No. DGE-1256259), respectively. NR 62 TC 18 Z9 18 U1 0 U2 4 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 2470-0010 EI 2470-0029 J9 PHYS REV D JI Phys. Rev. D PD NOV 10 PY 2014 VL 90 IS 9 AR 092005 DI 10.1103/PhysRevD.90.092005 PG 13 WC Astronomy & Astrophysics; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AT4NT UT WOS:000344917200003 ER PT J AU Roberts, BM Stadnik, YV Dzuba, VA Flambaum, VV Leefer, N Budker, D AF Roberts, B. M. Stadnik, Y. V. Dzuba, V. A. Flambaum, V. V. Leefer, N. Budker, D. TI Parity-violating interactions of cosmic fields with atoms, molecules, and nuclei: Concepts and calculations for laboratory searches and extracting limits SO PHYSICAL REVIEW D LA English DT Article ID ELECTRIC-DIPOLE MOMENT; HIGH-PRECISION MEASUREMENT; HIGH-ACCURACY CALCULATION; BODY-PERTURBATION-THEORY; STRONG CP PROBLEM; ANAPOLE MOMENT; SOLAR AXIONS; CONFIGURATION-INTERACTION; HYPERFINE-STRUCTURE; OPTICAL-ROTATION AB We propose methods and present calculations that can be used to search for evidence of cosmic fields by investigating the parity-violating effects, including parity nonconservation amplitudes and electric dipole moments, that they induce in atoms. The results are used to constrain important fundamental parameters describing the strength of the interaction of various cosmic fields with electrons, protons, and neutrons. Candidates for such fields are dark matter (including axions) and dark energy, as well as several more exotic sources described by standard-model extensions. Calculations of the effects induced by pseudoscalar and pseudovector fields are performed for H, Li, Na, K, Cu, Rb, Ag, Cs, Ba, Ba+, Dy, Yb, Au, Tl, Fr, and Ra+. Existing parity nonconservation experiments in Cs, Dy, Yb, and Tl are combined with these calculations to directly place limits on the interaction strength between the temporal component, b(0), of a static pseudovector cosmic field and the atomic electrons, with the most stringent limit of vertical bar b(0)(e)vertical bar < 7 x 10(-15) GeV, in the laboratory frame of reference, coming from Dy. From a measurement of the nuclear anapole moment of Cs, and a limit on its value for Tl, we also extract limits on the interaction strength between the temporal component of this cosmic field, as well as a related tensor cosmic-field component d(00), with protons and neutrons. The most stringent limits of vertical bar b(0)(p)vertical bar < 4 x 10(-8) GeV and vertical bar d(00)(p)vertical bar < 5 x 10(-8) for protons and vertical bar b(0)(n)vertical bar < 2 x 10(-7) GeV and vertical bar d(00)(n)vertical bar < 2 x 10(-7) for neutrons (in the laboratory frame) come from the results using Cs. Axions may induce oscillating parity-and time reversal-violating effects in atoms and molecules through the generation of oscillating nuclear magnetic quadrupole and Schiff moments, which arise from P- and T-odd intranuclear forces and from the electric dipole moments of constituent nucleons. Nuclear spin-independent parity nonconservation effects may be enhanced in diatomic molecules possessing close pairs of opposite-parity levels in the presence of time-dependent interactions. C1 [Roberts, B. M.; Stadnik, Y. V.; Dzuba, V. A.] Univ New S Wales, Sch Phys, Sydney, NSW 2052, Australia. [Leefer, N.; Budker, D.] Johannes Gutenberg Univ Mainz, Helmholtz Inst Mainz, D-55099 Mainz, Germany. [Budker, D.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA. [Budker, D.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Nucl Sci, Berkeley, CA 94720 USA. RP Roberts, BM (reprint author), Univ New S Wales, Sch Phys, Sydney, NSW 2052, Australia. EM b.roberts@unsw.edu.au; y.stadnik@unsw.edu.au RI Stadnik, Yevgeny/L-4065-2014; Roberts, Benjamin/C-1284-2013; Budker, Dmitry/F-7580-2016 OI Roberts, Benjamin/0000-0002-0345-6375; Budker, Dmitry/0000-0002-7356-4814 FU Australian Research Council; NSF [PHY-1068875]; Perimeter Institute for Theoretical Physics; Government of Canada through Industry Canada; Province of Ontario through the Ministry of Economic Development and Innovation; Humboldt foundation; Marie Curie International Incoming Fellowship within the 7th European Community Framework Programme FX The authors would like to acknowledge Michael Hohensee, Iosif B. Khriplovich, Derek Jackson Kimball, Mikhail Kozlov, Maxim Pospelov, Arkady Vainshtein, and Vladimir G. Zelevinsky for valuable discussions. We are particularly grateful to V. Alan Kostelecky for pointing out that our methods in Ref. [1] could be extended to place constraints on the d00p parameter. This work was supported in part by the Australian Research Council, by NSF Grant No. PHY-1068875, and by the Perimeter Institute for Theoretical Physics. Research at the Perimeter Institute is supported by the Government of Canada through Industry Canada and by the Province of Ontario through the Ministry of Economic Development and Innovation. V. V. Flambaum would also like to acknowledge the Humboldt foundation for support in the form of the Humboldt Award, and the MBN Research Center, where part of this work was conducted, for hospitality. N. Leefer was supported by a Marie Curie International Incoming Fellowship within the 7th European Community Framework Programme. NR 150 TC 21 Z9 21 U1 3 U2 16 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1550-7998 EI 1550-2368 J9 PHYS REV D JI Phys. Rev. D PD NOV 10 PY 2014 VL 90 IS 9 AR 096005 DI 10.1103/PhysRevD.90.096005 PG 18 WC Astronomy & Astrophysics; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AT4NT UT WOS:000344917200008 ER PT J AU Zhu, HY Sigdel, A Zhang, S Su, D Xi, Z Li, Q Sun, SH AF Zhu, Huiyuan Sigdel, Aruna Zhang, Sen Su, Dong Xi, Zheng Li, Qing Sun, Shouheng TI Core/Shell Au/MnO Nanoparticles Prepared Through Controlled Oxidation of AuMn as an Electrocatalyst for Sensitive H2O2 Detection SO ANGEWANDTE CHEMIE-INTERNATIONAL EDITION LA English DT Article DE gold; hydrogen peroxide; manganese; nanoparticles; sensors ID OXYGEN REDUCTION REACTION; MODIFIED ITO ELECTRODE; HYDROGEN-PEROXIDE; ALLOY NANOPARTICLES; CO OXIDATION; COMPOSITE; CATALYSIS; NANORODS; CELLS; ACID AB Monodisperse 5nm AuMn nanoparticles were synthesized by hydride reduction of manganese acetylacetonate in the presence of Au nanoparticles. The alloy was formed through fast Mn diffusion into the Au structure. The AuMn nanoparticles were converted to Au-MnO composite particles through air annealing at 170 degrees C. These Au-MnO particles, especially the core/shell Au/MnO nanoparticles, were active for the electrochemical reduction of H2O2, with a detection limit reaching 8nM. This highly sensitive electrochemical sensor based on the Au/MnO nanoparticles was used to monitor H2O2 concentrations released from living cells, from which tumorigenic cells were discovered to release higher levels of H2O2 than the non-tumorigenic cells. C1 [Zhu, Huiyuan; Sigdel, Aruna; Zhang, Sen; Xi, Zheng; Li, Qing; Sun, Shouheng] Brown Univ, Dept Chem, Providence, RI 02912 USA. [Su, Dong] Brookhaven Natl Lab, Ctr Funct Nanomat, Upton, NY 11973 USA. RP Sun, SH (reprint author), Brown Univ, Dept Chem, Providence, RI 02912 USA. EM ssun@brown.edu RI Zhang, Sen/E-4226-2015; Li, Qing/G-4502-2011 OI Li, Qing/0000-0003-4807-030X FU U.S. Army Research Laboratory; U.S. Army Research Office under the Multi University Research Initiative (MURI) [W911NF-11-1-0353]; U.S. Department of Energy, Office of Basic Energy Sciences [DE-AC02-98CH10886] FX Supported by the U.S. Army Research Laboratory and the U.S. Army Research Office under the Multi University Research Initiative (MURI, grant number W911NF-11-1-0353) on "Stress-Controlled Catalysis via Engineered Nanostructures". Electron microscopy work carried out at the Center for Functional Nanomaterials, Brookhaven National Laboratory was supported by the U.S. Department of Energy, Office of Basic Energy Sciences under Contract No. DE-AC02-98CH10886. We thank Dr. L. Chen of the Department of Polymer Science and Engineering, University of Massachusetts-Amherst for collecting XPS data. NR 34 TC 21 Z9 21 U1 21 U2 160 PU WILEY-V C H VERLAG GMBH PI WEINHEIM PA BOSCHSTRASSE 12, D-69469 WEINHEIM, GERMANY SN 1433-7851 EI 1521-3773 J9 ANGEW CHEM INT EDIT JI Angew. Chem.-Int. Edit. PD NOV 10 PY 2014 VL 53 IS 46 SI SI BP 12508 EP 12512 DI 10.1002/anie.201406281 PG 5 WC Chemistry, Multidisciplinary SC Chemistry GA AT0UJ UT WOS:000344649900026 PM 25155180 ER PT J AU Osterwalder, M Speziale, D Shoukry, M Mohan, R Ivanek, R Kohler, M Beisel, C Wen, XH Scales, SJ Christoffels, VM Visel, A Lopez-Rios, J Zeller, R AF Osterwalder, Marco Speziale, Dario Shoukry, Malak Mohan, Rajiv Ivanek, Robert Kohler, Manuel Beisel, Christian Wen, Xiaohui Scales, Suzie J. Christoffels, Vincent M. Visel, Axel Lopez-Rios, Javier Zeller, Rolf TI HAND2 Targets Define a Network of Transcriptional Regulators that Compartmentalize the Early Limb Bud Mesenchyme SO DEVELOPMENTAL CELL LA English DT Article ID RETINOIC ACID SYNTHESIS; VERTEBRATE LIMB; POLARIZING ACTIVITY; GENE-EXPRESSION; SHH EXPRESSION; MOUSE LIMB; GLI3; BINDING; DHAND; DIFFERENTIATION AB The genetic networks that govern vertebrate development are well studied, but how the interactions of trans-acting factors with cis-regulatory modules (CRMs) are integrated into spatiotemporal regulation of gene expression is not clear. The transcriptional regulator HAND2 is required during limb, heart, and branchial arch development. Here, we identify the genomic regions enriched in HAND2 chromatin complexes from mouse embryos and limb buds. Then we analyze the HAND2 target CRMs in the genomic landscapes encoding transcriptional regulators required in early limb buds. HAND2 controls the expression of genes functioning in the proximal limb bud and orchestrates the establishment of anterior and posterior polarity of the nascent limb bud mesenchyme by impacting Gli3 and Tbx3 expression. TBX3 is required downstream of HAND2 to refine the posterior Gli3 expression boundary. Our analysis uncovers the transcriptional circuits that function in establishing distinct mesenchymal compartments downstream of HAND2 and upstream of SHH signaling. C1 [Osterwalder, Marco; Speziale, Dario; Ivanek, Robert; Lopez-Rios, Javier; Zeller, Rolf] Univ Basel, Dept Biomed, CH-4058 Basel, Switzerland. [Shoukry, Malak; Visel, Axel] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Genom Div, Berkeley, CA 94720 USA. [Mohan, Rajiv; Christoffels, Vincent M.] Univ Amsterdam, Acad Med Ctr, Heart Failure Res Ctr, Dept Anat Embryol & Physiol, NL-1100 DD Amsterdam, Netherlands. [Kohler, Manuel; Beisel, Christian] Fed Inst Technol Zurich, Dept Biosyst Sci & Engn, CH-4058 Basel, Switzerland. [Wen, Xiaohui; Scales, Suzie J.] Genentech Inc, Dept Mol Biol, San Francisco, CA 94080 USA. [Visel, Axel] US DOE, Joint Genome Inst, Walnut Creek, CA 94598 USA. [Visel, Axel] Univ Calif Merced, Sch Nat Sci, Merced, CA 95343 USA. RP Lopez-Rios, J (reprint author), Univ Basel, Dept Biomed, CH-4058 Basel, Switzerland. EM javier.lopez-rios@unibas.ch; rolf.zeller@unibas.ch RI Lopez-Rios, Javier/D-8094-2014; Zeller, Rolf /C-2610-2013; Visel, Axel/A-9398-2009; OI Lopez-Rios, Javier/0000-0001-6731-3798; Visel, Axel/0000-0002-4130-7784; Zeller, Rolf/0000-0002-3186-7403 FU Swiss National Science Foundation [31003A_130803/146248]; EU [PERG-GA-2009-246576]; Netherlands Heart Foundation [2010B205]; NIH [R01HG003988, U01DE020060]; Department of Energy, University of California [DE-AC02-05CH11231] FX We wish to thank the mouse transgenic core facility of the University of Basel for generation of chimeric mice and A. Offinger and her team for excellent animal care. Frederic Laurent is thanked for performing the OPT analysis. We are grateful to Jennifer Akiyama for generation of constructs, Ina Nissen (D-BSSE) for the preparation of the ChIP-seq library, and Isabelle Ginez for preparing the tissue sections. This research was supported by Swiss National Science Foundation grants (31003A_130803/146248) and both cantons of Basel (to R.Z.), an EU Reintegration grant (PERG-GA-2009-246576 to J.L.-R.), a Netherlands Heart Foundation grant (2010B205) (to V.M.C.), and NIH grants (R01HG003988 and U01DE020060) (to A.V.). A.V.'s research was conducted at the E.O. Lawrence Berkeley National Laboratory and performed under a Department of Energy Contract (DE-AC02-05CH11231), University of California. X.W. and S.J.S. are employees of Genentech, a member of the Roche group. NR 51 TC 18 Z9 18 U1 3 U2 12 PU CELL PRESS PI CAMBRIDGE PA 600 TECHNOLOGY SQUARE, 5TH FLOOR, CAMBRIDGE, MA 02139 USA SN 1534-5807 EI 1878-1551 J9 DEV CELL JI Dev. Cell PD NOV 10 PY 2014 VL 31 IS 3 BP 345 EP 357 DI 10.1016/j.devcel.2014.09.018 PG 13 WC Cell Biology; Developmental Biology SC Cell Biology; Developmental Biology GA AT3OD UT WOS:000344843000011 PM 25453830 ER PT J AU Nguyen, SC Lomont, JP Zoerb, MC Pham, PV Cahoon, JF Harris, CB AF Nguyen, Son C. Lomont, Justin P. Zoerb, Matthew C. Pham, Phong V. Cahoon, James F. Harris, Charles B. TI Direct Observation of Metal Ketenes Formed by Photoexcitation of a Fischer Carbene using Ultrafast Infrared Spectroscopy SO ORGANOMETALLICS LA English DT Article ID MATRIX-ISOLATION; COMPLEX PHOTOCHEMISTRY; CYCLIZATION REACTIONS; FLASH-PHOTOLYSIS; MECHANISM; IMINES; PHOTOCARBONYLATION; TUNGSTEN AB Fischer carbenes are commonly used as reagents in the synthesis of new carboncarbon bonds, a reaction made possible by the unique chemistry of the formal metalcarbon double bond. Nevertheless, the photoinduced reactions of these complexes are relatively poorly understood. For instance, it has been postulated but not confirmed that visible irradiation leads to photocarbonylation, in which a CO ligand inserts into the metalcarbon bond to form a metal ketene intermediate. Here, we report the first direct observation of this intermediate following 400 nm photoexcitation of the model group 6 Fischer carbene Cr(CO)(5)[CCH3(OCH3)]. Using ultrafast time-resolved infrared spectroscopy (TRIR), we observe the formation of three distinct metal ketene structures, which we assign as a singlet and two isoenergetic triplet excited-state structures. The singlet relaxes to the ground state on a time scale of similar to 35 ps, whereas the two triplets are long-lived (>2 ns). TRIR of the tungsten analogue yields no evidence for a metal ketene structure, consistent with the limited reactivity of this complex. The results directly elucidate the fundamental role of triplet metal ketenes in the photoreactivity of Fischer carbene complexes. C1 [Nguyen, Son C.; Lomont, Justin P.; Zoerb, Matthew C.; Pham, Phong V.; Harris, Charles B.] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA. [Nguyen, Son C.; Lomont, Justin P.; Zoerb, Matthew C.; Pham, Phong V.; Harris, Charles B.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA. [Cahoon, James F.] Univ N Carolina, Dept Chem, Chapel Hill, NC 27599 USA. RP Harris, CB (reprint author), Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA. EM cbharris@berkeley.edu FU NSF [CHE-1213135]; Molecular Graphics and Computation Facility at UC-Berkeley [CHE-0840505, CHE-0233882]; Office of Science of the U.S. DOE [DE-AC02-05CH11231]; VIED fellowship; NSF graduate research fellowship; VNU Dept. of Chem. research fellowship FX This work was supported by NSF grant CHE-1213135. The authors acknowledge use of the Molecular Graphics and Computation Facility at UC-Berkeley (grants CHE-0840505 and CHE-0233882) and the National Energy Research Scientific Computing Center, supported by the Office of Science of the U.S. DOE under Contract No. DE-AC02-05CH11231. S.C.N. acknowledges support through a VIED fellowship. J.P.L. acknowledges support through an NSF graduate research fellowship. P.V.P. acknowledges support through a VNU Dept. of Chem. research fellowship. NR 32 TC 4 Z9 4 U1 1 U2 18 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0276-7333 EI 1520-6041 J9 ORGANOMETALLICS JI Organometallics PD NOV 10 PY 2014 VL 33 IS 21 BP 6149 EP 6153 DI 10.1021/om500795b PG 5 WC Chemistry, Inorganic & Nuclear; Chemistry, Organic SC Chemistry GA AT1WO UT WOS:000344722000034 ER PT J AU Lomont, JP Nguyen, SC Harris, CB AF Lomont, Justin P. Nguyen, Son C. Harris, Charles B. TI Exploring the Utility of Tandem Thermal Photochemical CO Delivery with CORM-2 SO ORGANOMETALLICS LA English DT Article ID MONOXIDE-RELEASING MOLECULES; TRANSITION-METAL-COMPLEXES; GAUSSIAN-BASIS SETS; CARBON-MONOXIDE; STRUCTURAL-CHARACTERIZATION; CORRELATION-ENERGY; INFRARED-SPECTRA; AQUEOUS-SOLUTION; WAVE-FUNCTIONS; CHEMISTRY AB Among the most popular and widely studied CO-releasing molecules (CO-RMs) for biological research is Ru2Cl4(CO)(6) (CORM-2). When dissolved in DMSO (the solubilizing agent used in preclinical trials), the dimer cleaves into monomeric DMSO-ligated Ru subunits; the rate of this reaction and behavior of the products formed are thus highly relevant to the efficacy of CORM-2 in vivo. FT-IR spectroscopy was used to monitor this reaction in DMSO and also to monitor the reactivity of CORM-2 and of the monomeric DMSO-ligated derivatives in mouse serum. While the CORM-2 dimer readily liberates CO in mouse serum under ambient conditions, the monomeric Ru subunits formed in DMSO solution do not. This demonstrates that a substantial fraction of the CO-delivery agent being introduced via DMSO solutions would appear to be, in fact, inactive. Photochemical irradiation readily liberates CO from the inactive species, and thus a combined thermalphotochemical approach can greatly improve the yield of CO delivery. Ultrafast experiments indicate that CO loss from the DMSO-ligated monomers is a primary photochemical process. Viewing these results for the popular CORM-2 as a series of proof-of-principle observations, these results demonstrate that predissolution of a CO-RM in any solvent may generate products that are no longer physiologically active, and thus the time between dissolution and injection should always be carefully monitored; this has been seldom reported or considered in CO-RM studies to date. Although a combined thermalphotochemical CO-release approach has not been taken previously, we demonstrate that such an approach is practically quite useful for one of the most popular CO-RMs currently being studied, and thus it is clear that such an approach will be needed to achieve the full potential of many current and future CO-RMs. C1 [Harris, Charles B.] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA. Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA. RP Harris, CB (reprint author), Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA. EM cbharris@berkeley.edu FU NSF [CHE-1213135]; Molecular Graphics and Computation Facility at UC-Berkeley [CHE-0840505, CHE-0233882]; VIED fellowship; NSF graduate research fellowship FX This work was supported by NSF Grant CHE-1213135. The authors acknowledge use of the Molecular Graphics and Computation Facility at UC-Berkeley (grants CHE-0840505, CHE-0233882). S.C.N. acknowledges support through a VIED fellowship. J.P.L. acknowledges support through an NSF graduate research fellowship. The authors thank Dr. Keary Mark Engle for helpful discussions. NR 50 TC 0 Z9 0 U1 5 U2 27 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0276-7333 EI 1520-6041 J9 ORGANOMETALLICS JI Organometallics PD NOV 10 PY 2014 VL 33 IS 21 BP 6179 EP 6185 DI 10.1021/om500859c PG 7 WC Chemistry, Inorganic & Nuclear; Chemistry, Organic SC Chemistry GA AT1WO UT WOS:000344722000038 ER PT J AU Lin, YZ Cohen, RE Stackhouse, S Driver, KP Militzer, B Shulenburger, L Kim, J AF Lin, Yangzheng Cohen, R. E. Stackhouse, Stephen Driver, Kevin P. Militzer, Burkhard Shulenburger, Luke Kim, Jeongnim TI Equations of state and stability of MgSiO3 perovskite and post-perovskite phases from quantum Monte Carlo simulations SO PHYSICAL REVIEW B LA English DT Article ID EARTHS LOWERMOST MANTLE; V-T EQUATION; OF-STATE; HIGH-PRESSURE; THERMOELASTIC PROPERTIES; (MG,FE)SIO3 PEROVSKITE; THERMAL EXPANSIVITY; CRYSTAL-CHEMISTRY; ELECTRON-GAS; 30 GPA AB We have performed quantum Monte Carlo (QMC) simulations and density functional theory calculations to study the equations of state of MgSiO3 perovskite (Pv, bridgmanite) and post-perovskite (PPv) up to the pressure and temperature conditions of the base of Earth's lower mantle. The ground-state energies were derived using QMC simulations and the temperature-dependent Helmholtz free energies were calculated within the quasiharmonic approximation and density functional perturbation theory. The equations of state for both phases of MgSiO3 agree well with experiments, and better than those from generalized gradient approximation calculations. The Pv-PPv phase boundary calculated from our QMC equations of state is also consistent with experiments, and better than previous local density approximation calculations. We discuss the implications for double crossing of the Pv-PPv boundary in the Earth. C1 [Lin, Yangzheng; Cohen, R. E.] Carnegie Inst Sci, Geophys Lab, Washington, DC 20015 USA. [Cohen, R. E.] UCL, Dept Earth Sci, London WC1E 6BT, England. [Stackhouse, Stephen; Driver, Kevin P.; Militzer, Burkhard] Univ Calif Berkeley, Dept Earth & Planetary Sci, Berkeley, CA 94720 USA. [Stackhouse, Stephen] Univ Leeds, Sch Earth & Environm, Leeds LS2 9JT, W Yorkshire, England. [Militzer, Burkhard] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA. [Shulenburger, Luke] Sandia Natl Labs, Albuquerque, NM 87185 USA. [Kim, Jeongnim] Oak Ridge Natl Lab, Oak Ridge, TN 37830 USA. RP Lin, YZ (reprint author), Carnegie Inst Sci, Geophys Lab, 5251 Broad Branch Rd NW, Washington, DC 20015 USA. EM rcohen@carnegiescience.edu OI Lin, Yangzheng/0000-0003-3913-5298 FU National Science Foundation [DMS-1025370, EAR-1214807, OCI1053575]; Carnegie Institution; European Research Council advanced grant ToMCaT; Office of Science of the U.S. Department of Energy [DE-AC05-00OR22725]; Innovative and Novel Computational Impact on Theory and Experiment (INCITE) program [CPH103geo]; U.S. Department of Energy [DE-SC0010517]; Predictive Theory and Modeling for Materials; Chemical Science program by the Office of Basic Energy Sciences (BES), Department of Energy (DOE); U.S. Department of Energy's National Nuclear Security Administration [DE-AC04-94AL85000] FX This work is supported by National Science Foundation Grants No. DMS-1025370 and No. EAR-1214807. R.E.C. was supported by the Carnegie Institution and by the European Research Council advanced grant ToMCaT. This work used the Extreme Science and Engineering Discovery Environment (XSEDE) computers, which are supported by the National Science Foundation Grant No. OCI1053575, and computers at the Oak Ridge Leadership Computing Facility at the Oak Ridge National Laboratory, which is supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC05-00OR22725. An award of computer time was provided by the Innovative and Novel Computational Impact on Theory and Experiment (INCITE) program with Project CPH103geo. K.D. and B.M. acknowledge support from the U.S. Department of Energy under Contract No. DE-SC0010517. L.S. was supported through the Predictive Theory and Modeling for Materials and Chemical Science program by the Office of Basic Energy Sciences (BES), Department of Energy (DOE). Sandia National Laboratories is a multiprogram laboratory managed and operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the U.S. Department of Energy's National Nuclear Security Administration under Contract No. DE-AC04-94AL85000. We thank Jane Robb for assistance with editing the manuscript. NR 94 TC 4 Z9 4 U1 2 U2 34 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1098-0121 EI 1550-235X J9 PHYS REV B JI Phys. Rev. B PD NOV 10 PY 2014 VL 90 IS 18 AR 184103 DI 10.1103/PhysRevB.90.184103 PG 11 WC Physics, Condensed Matter SC Physics GA AT4ND UT WOS:000344915100002 ER PT J AU Lees, JP Poireau, V Tisserand, V Grauges, E Palano, A Eigen, G Stugu, B Brown, DN Feng, M Kerth, LT Kolomensky, YG Lee, MJ Lynch, G Koch, H Schroeder, T Hearty, C Mattison, TS McKenna, JA So, RY Khan, A Blinov, VE Buzykaev, AR Druzhinin, VP Golubev, VB Kravchenko, EA Onuchin, AP Serednyakov, SI Skovpen, YI Solodov, EP Todyshev, KY Lankford, AJ Mandelkern, M Dey, B Gary, JW Long, O Campagnari, C Sevilla, MF Hong, TM Kovalskyi, D Richman, JD West, CA Eisner, AM Lockman, WS Vazquez, WP Schumm, BA Seiden, A Chao, DS Cheng, CH Echenard, B Flood, KT Hitlin, DG Miyashita, TS Ongmongkolkul, P Porter, FC Andreassen, R Huard, Z Meadows, BT Pushpawela, BG Sokoloff, MD Sun, L Bloom, PC Ford, WT Gaz, A Smith, JG Wagner, SR Ayad, R Toki, WH Spaan, B Bernard, D Verderi, M Playfer, S Bettoni, D Bozzi, C Calabrese, R Cibinetto, G Fioravanti, E Garzia, I Luppi, E Piemontese, L Santoro, V Calcaterra, A de Sangro, R Finocchiaro, G Martellotti, S Patteri, P Peruzzi, IM Piccolo, M Rama, M Zallo, A Contri, R Lo Vetere, M Monge, MR Passaggio, S Patrignani, C Robutti, E Bhuyan, B Prasad, V Adametz, A Uwer, U Lacker, HM Dauncey, PD Mallik, U Chen, C Cochran, J Prell, S Ahmed, H Gritsan, AV Arnaud, N Davier, M Derkach, D Grosdidier, G Le Diberder, F Lutz, AM Malaescu, B Roudeau, P Stocchi, A Wormser, G Lange, DJ Wright, DM Coleman, JP Fry, JR Gabathuler, E Hutchcroft, DE Payne, DJ Touramanis, C Bevan, AJ Di Lodovico, F Sacco, R Cowan, G Bougher, J Brown, DN Davis, CL Denig, AG Fritsch, M Gradl, W Griessinger, K Hafner, A Schubert, KR Barlow, RJ Lafferty, GD Cenci, R Hamilton, B Jawahery, A Roberts, DA Cowan, R Sciolla, G Cheaib, R Patel, PM Robertson, SH Neri, N Palombo, F Cremaldi, L Godang, R Sonnek, P Summers, DJ Simard, M Taras, P De Nardo, G Onorato, G Sciacca, C Martinelli, M Raven, G Jessop, CP LoSecco, JM Honscheid, K Kass, R Feltresi, E Margoni, M Morandin, M Posocco, M Rotondo, M Simi, G Simonetto, F Stroili, R Akar, S Ben-Haim, E Bomben, M Bonneaud, GR Briand, H Calderini, G Chauveau, J Leruste, P Marchiori, G Ocariz, J Biasini, M Manoni, E Pacetti, S Rossi, A Angelini, C Batignani, G Bettarini, S Carpinelli, M Casarosa, G Cervelli, A Chrzaszcz, M Forti, F Giorgi, MA Lusiani, A Oberhof, B Paoloni, E Perez, A Rizzo, G Walsh, JJ Pegna, DL Olsen, J Smith, AJS Faccini, R Ferrarotto, F Ferroni, F Gaspero, M Gioi, LL Pilloni, A Piredda, G Bunger, C Dittrich, S Grunberg, O Hartmann, T Hess, M Leddig, T Voss, C Waldi, R Adye, T Olaiya, EO Wilson, FF Emery, S Vasseur, G Anulli, F Aston, D Bard, DJ Cartaro, C Convery, MR Dorfan, J Dubois-Felsmann, GP Dunwoodie, W Ebert, M Field, RC Fulsom, BG Graham, MT Hast, C Innes, WR Kim, P Leith, DWGS Lewis, P Lindemann, D Luitz, S Luth, V Lynch, HL MacFarlane, DB Muller, DR Neal, H Perl, M Pulliam, T Ratcliff, BN Roodman, A Salnikov, AA Schindler, RH Snyder, A Su, D Sullivan, MK Va'vra, J Wisniewski, WJ Wulsin, HW Purohit, MV White, RM Wilson, JR Randle-Conde, A Sekula, SJ Bellis, M Burchat, PR Puccio, EMT Alam, MS Ernst, JA Gorodeisky, R Guttman, N Peimer, DR Soffer, A Spanier, SM Ritchie, JL Ruland, AM Schwitters, RF Wray, BC Izen, JM Lou, XC Bianchi, F De Mori, F Filippi, A Gamba, D Lanceri, L Vitale, L Martinez-Vidal, F Oyanguren, A Villanueva-Perez, P Albert, J Banerjee, S Beaulieu, A Bernlochner, FU Choi, HHF King, GJ Kowalewski, R Lewczuk, MJ Lueck, T Nugent, IM Roney, JM Sobie, RJ Tasneem, N Gershon, TJ Harrison, PF Latham, TE Band, HR Dasu, S Pan, Y Prepost, R Wu, SL AF Lees, J. P. Poireau, V. Tisserand, V. Grauges, E. Palano, A. Eigen, G. Stugu, B. Brown, D. N. Feng, M. Kerth, L. T. Kolomensky, Yu. G. Lee, M. J. Lynch, G. Koch, H. Schroeder, T. Hearty, C. Mattison, T. S. McKenna, J. A. So, R. Y. Khan, A. Blinov, V. E. Buzykaev, A. R. Druzhinin, V. P. Golubev, V. B. Kravchenko, E. A. Onuchin, A. P. Serednyakov, S. I. Skovpen, Yu. I. Solodov, E. P. Todyshev, K. Yu. Lankford, A. J. Mandelkern, M. Dey, B. Gary, J. W. Long, O. Campagnari, C. Sevilla, M. Franco Hong, T. M. Kovalskyi, D. Richman, J. D. West, C. A. Eisner, A. M. Lockman, W. S. Vazquez, W. Panduro Schumm, B. A. Seiden, A. Chao, D. S. Cheng, C. H. Echenard, B. Flood, K. T. Hitlin, D. G. Miyashita, T. S. Ongmongkolkul, P. Porter, F. C. Andreassen, R. Huard, Z. Meadows, B. T. Pushpawela, B. G. Sokoloff, M. D. Sun, L. Bloom, P. C. Ford, W. T. Gaz, A. Smith, J. G. Wagner, S. R. Ayad, R. Toki, W. H. Spaan, B. Bernard, D. Verderi, M. Playfer, S. Bettoni, D. Bozzi, C. Calabrese, R. Cibinetto, G. Fioravanti, E. Garzia, I. Luppi, E. Piemontese, L. Santoro, V. Calcaterra, A. de Sangro, R. Finocchiaro, G. Martellotti, S. Patteri, P. Peruzzi, I. M. Piccolo, M. Rama, M. Zallo, A. Contri, R. Lo Vetere, M. Monge, M. R. Passaggio, S. Patrignani, C. Robutti, E. Bhuyan, B. Prasad, V. Adametz, A. Uwer, U. Lacker, H. M. Dauncey, P. D. Mallik, U. Chen, C. Cochran, J. Prell, S. Ahmed, H. Gritsan, A. V. Arnaud, N. Davier, M. Derkach, D. Grosdidier, G. Le Diberder, F. Lutz, A. M. Malaescu, B. Roudeau, P. Stocchi, A. Wormser, G. Lange, D. J. Wright, D. M. Coleman, J. P. Fry, J. R. Gabathuler, E. Hutchcroft, D. E. Payne, D. J. Touramanis, C. Bevan, A. J. Di Lodovico, F. Sacco, R. Cowan, G. Bougher, J. Brown, D. N. Davis, C. L. Denig, A. G. Fritsch, M. Gradl, W. Griessinger, K. Hafner, A. Schubert, K. R. Barlow, R. J. Lafferty, G. D. Cenci, R. Hamilton, B. Jawahery, A. Roberts, D. A. Cowan, R. Sciolla, G. Cheaib, R. Patel, P. M. Robertson, S. H. Neri, N. Palombo, F. Cremaldi, L. Godang, R. Sonnek, P. Summers, D. J. Simard, M. Taras, P. De Nardo, G. Onorato, G. Sciacca, C. Martinelli, M. Raven, G. Jessop, C. P. LoSecco, J. M. Honscheid, K. Kass, R. Feltresi, E. Margoni, M. Morandin, M. Posocco, M. Rotondo, M. Simi, G. Simonetto, F. Stroili, R. Akar, S. Ben-Haim, E. Bomben, M. Bonneaud, G. R. Briand, H. Calderini, G. Chauveau, J. Leruste, Ph. Marchiori, G. Ocariz, J. Biasini, M. Manoni, E. Pacetti, S. Rossi, A. Angelini, C. Batignani, G. Bettarini, S. Carpinelli, M. Casarosa, G. Cervelli, A. Chrzaszcz, M. Forti, F. Giorgi, M. A. Lusiani, A. Oberhof, B. Paoloni, E. Perez, A. Rizzo, G. Walsh, J. J. Pegna, D. Lopes Olsen, J. Smith, A. J. S. Faccini, R. Ferrarotto, F. Ferroni, F. Gaspero, M. Gioi, L. Li Pilloni, A. Piredda, G. Buenger, C. Dittrich, S. Gruenberg, O. Hartmann, T. Hess, M. Leddig, T. Voss, C. Waldi, R. Adye, T. Olaiya, E. O. Wilson, F. F. Emery, S. Vasseur, G. Anulli, F. Aston, D. Bard, D. J. Cartaro, C. Convery, M. R. Dorfan, J. Dubois-Felsmann, G. P. Dunwoodie, W. Ebert, M. Field, R. C. Fulsom, B. G. Graham, M. T. Hast, C. Innes, W. R. Kim, P. Leith, D. W. G. S. Lewis, P. Lindemann, D. Luitz, S. Luth, V. Lynch, H. L. MacFarlane, D. B. Muller, D. R. Neal, H. Perl, M. Pulliam, T. Ratcliff, B. N. Roodman, A. Salnikov, A. A. Schindler, R. H. Snyder, A. Su, D. Sullivan, M. K. Va'vra, J. Wisniewski, W. J. Wulsin, H. W. Purohit, M. V. White, R. M. Wilson, J. R. Randle-Conde, A. Sekula, S. J. Bellis, M. Burchat, P. R. Puccio, E. M. T. Alam, M. S. Ernst, J. A. Gorodeisky, R. Guttman, N. Peimer, D. R. Soffer, A. Spanier, S. M. Ritchie, J. L. Ruland, A. M. Schwitters, R. F. Wray, B. C. Izen, J. M. Lou, X. C. Bianchi, F. De Mori, F. Filippi, A. Gamba, D. Lanceri, L. Vitale, L. Martinez-Vidal, F. Oyanguren, A. Villanueva-Perez, P. Albert, J. Banerjee, Sw. Beaulieu, A. Bernlochner, F. U. Choi, H. H. F. King, G. J. Kowalewski, R. Lewczuk, M. J. Lueck, T. Nugent, I. M. Roney, J. M. Sobie, R. J. Tasneem, N. Gershon, T. J. Harrison, P. F. Latham, T. E. Band, H. R. Dasu, S. Pan, Y. Prepost, R. Wu, S. L. CA BABAR Collaboration TI Search for a Dark Photon in e(+)e(-) Collisions at BABAR SO PHYSICAL REVIEW LETTERS LA English DT Article ID BHABHA SCATTERING; DETECTOR; ENERGIES; BOSON AB Dark sectors charged under a new Abelian interaction have recently received much attention in the context of dark matter models. These models introduce a light new mediator, the so-called dark photon (A'), connecting the dark sector to the standard model. We present a search for a dark photon in the reaction e(+)e(-) ->gamma A', A' -> e(+)e(-), mu(+) mu(-) using 514 fb(-1) of data collected with the BABAR detector. We observe no statistically significant deviations from the standard model predictions, and we set 90% confidence level upper limits on the mixing strength between the photon and dark photon at the level of 10(-4) - 10(-3) for dark photon masses in the range 0.02-10.2 GeV. 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A.; Schindler, R. H.; Snyder, A.; Su, D.; Sullivan, M. K.; Wisniewski, W. J.; Wulsin, H. W.] SLAC Natl Accelerator Lab, Stanford, CA 94309 USA. [Purohit, M. V.; White, R. M.; Wilson, J. R.] Univ S Carolina, Columbia, SC 29208 USA. [Randle-Conde, A.; Sekula, S. J.] So Methodist Univ, Dallas, TX 75275 USA. [Bellis, M.; Burchat, P. R.; Puccio, E. M. T.] Stanford Univ, Stanford, CA 94305 USA. [Alam, M. S.; Ernst, J. A.] SUNY Albany, Albany, NY 12222 USA. [Gorodeisky, R.; Guttman, N.; Peimer, D. R.; Soffer, A.] Tel Aviv Univ, Sch Phys & Astron, IL-69978 Tel Aviv, Israel. [Spanier, S. M.] Univ Tennessee, Knoxville, TN 37996 USA. [Ritchie, J. L.; Ruland, A. M.; Schwitters, R. F.; Wray, B. C.] Univ Texas Austin, Austin, TX 78712 USA. [Izen, J. M.; Lou, X. C.] Univ Texas Dallas, Richardson, TX 75083 USA. [Bianchi, F.; De Mori, F.; Filippi, A.; Gamba, D.] Ist Nazl Fis Nucl, Sez Torino, I-10125 Turin, Italy. [Bianchi, F.; De Mori, F.; Gamba, D.] Univ Turin, Dipartimento Fis, I-10125 Turin, Italy. [Lanceri, L.; Vitale, L.] Ist Nazl Fis Nucl, Sez Trieste, I-34127 Trieste, Italy. [Lanceri, L.; Vitale, L.] Univ Trieste, Dipartimento Fis, I-34127 Trieste, Italy. [Martinez-Vidal, F.; Oyanguren, A.; Villanueva-Perez, P.] Univ Valencia, CSIC, IFIC, E-46071 Valencia, Spain. [Albert, J.; Banerjee, Sw.; Beaulieu, A.; Bernlochner, F. U.; Choi, H. H. F.; King, G. J.; Kowalewski, R.; Lewczuk, M. J.; Lueck, T.; Nugent, I. M.; Roney, J. M.; Sobie, R. J.; Tasneem, N.] Univ Victoria, Victoria, BC V8W 3P6, Canada. [Gershon, T. J.; Harrison, P. F.; Latham, T. E.] Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England. [Band, H. R.; Dasu, S.; Pan, Y.; Prepost, R.; Wu, S. L.] Univ Wisconsin, Madison, WI 53706 USA. [Carpinelli, M.] Univ Sassari, I-07100 Sassari, Italy. RP Lees, JP (reprint author), Univ Savoie, Lab Annecy le Vieux Phys Particules LAPP, IN2P3, CNRS, F-74941 Annecy Le Vieux, France. RI Morandin, Mauro/A-3308-2016; Lusiani, Alberto/A-3329-2016; Di Lodovico, Francesca/L-9109-2016; Kolomensky, Yury/I-3510-2015; Martinez Vidal, F*/L-7563-2014; Oyanguren, Arantza/K-6454-2014; Monge, Maria Roberta/G-9127-2012; Lo Vetere, Maurizio/J-5049-2012; Lusiani, Alberto/N-2976-2015; Calcaterra, Alessandro/P-5260-2015; Patrignani, Claudia/C-5223-2009; Luppi, Eleonora/A-4902-2015; White, Ryan/E-2979-2015; Kravchenko, Evgeniy/F-5457-2015; Calabrese, Roberto/G-4405-2015; Rizzo, Giuliana/A-8516-2015; OI Morandin, Mauro/0000-0003-4708-4240; Lusiani, Alberto/0000-0002-6876-3288; Di Lodovico, Francesca/0000-0003-3952-2175; Lanceri, Livio/0000-0001-8220-3095; Sciacca, Crisostomo/0000-0002-8412-4072; Ebert, Marcus/0000-0002-3014-1512; Paoloni, Eugenio/0000-0001-5969-8712; Bettarini, Stefano/0000-0001-7742-2998; Cibinetto, Gianluigi/0000-0002-3491-6231; Kolomensky, Yury/0000-0001-8496-9975; Martinez Vidal, F*/0000-0001-6841-6035; Oyanguren, Arantza/0000-0002-8240-7300; Monge, Maria Roberta/0000-0003-1633-3195; Lo Vetere, Maurizio/0000-0002-6520-4480; Lusiani, Alberto/0000-0002-6876-3288; Calcaterra, Alessandro/0000-0003-2670-4826; Patrignani, Claudia/0000-0002-5882-1747; Luppi, Eleonora/0000-0002-1072-5633; White, Ryan/0000-0003-3589-5900; Calabrese, Roberto/0000-0002-1354-5400; Pacetti, Simone/0000-0002-6385-3508; Rizzo, Giuliana/0000-0003-1788-2866; Faccini, Riccardo/0000-0003-2613-5141; Martinelli, Maurizio/0000-0003-4792-9178; Pilloni, Alessandro/0000-0003-4257-0928; Raven, Gerhard/0000-0002-2897-5323; Bellis, Matthew/0000-0002-6353-6043 FU DOE; NSF (U. S.); NSERC (Canada); CEA (France); CNRS-IN2P3 (France); BMBF (Germany); DFG (Germany); INFN (Italy); FOM (Netherlands); NFR (Norway); MES (Russia); MICIIN (Spain); STFC (United Kingdom); Marie Curie EIF (European Union); A. P. Sloan Foundation (U. S.); Binational Science Foundation (U.S.- Israel) FX The authors wish to thank Rouven Essig and Sarah Andreas for providing the constraints derived from existing experiments. We also thank Rouven Essig, Philip Schuster, and Natalia Toro for useful discussions and for providing us with their MADGRAPH code to simulate dark photon processes. We are grateful for the excellent luminosity and machine conditions provided by our PEP-II2 colleagues, and for the substantial dedicated effort from the computing organizations that support BABAR. The collaborating institutions wish to thank SLAC for its support and kind hospitality. This work is supported by DOE and NSF (U.S.), NSERC (Canada), CEA and CNRS-IN2P3 (France), BMBF and DFG (Germany), INFN (Italy), FOM (Netherlands), NFR (Norway), MES (Russia), MICIIN (Spain), STFC (United Kingdom). Individuals have received support from the Marie Curie EIF (European Union), the A. P. Sloan Foundation (U. S.), and the Binational Science Foundation (U.S.- Israel). NR 37 TC 75 Z9 79 U1 2 U2 28 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0031-9007 EI 1079-7114 J9 PHYS REV LETT JI Phys. Rev. Lett. PD NOV 10 PY 2014 VL 113 IS 20 AR 201801 DI 10.1103/PhysRevLett.113.201801 PG 8 WC Physics, Multidisciplinary SC Physics GA AT4OL UT WOS:000344919200001 PM 25432035 ER PT J AU Lilova, KI Pearce, CI Rosso, KM Navrotsky, A AF Lilova, Kristina I. Pearce, Carolyn I. Rosso, Kevin M. Navrotsky, Alexandra TI Energetics of Spinels in the Fe-Ti-O System at the Nanoscale SO CHEMPHYSCHEM LA English DT Article DE nanosized solid solution; spinel phases; surface energy; thermodynamics; titanomagnetites ID OXIDATION-REDUCTION EQUILIBRIA; HIGH-TEMPERATURE CALORIMETRY; MAGNETITE NANOPARTICLES; SOLID-SOLUTIONS; THERMODYNAMICS; MAGHEMITE; OXIDES; SIZE; TITANOMAGNETITE; FE3O4-FE2TIO4 AB The energetics of nanosized Fe/Ti spinel oxides was studied using high-temperature oxide melt solution calorimetry. The mixing properties of the solid solution in the system were obtained, and through comparison to macroscopic materials the effect of particle size on the thermodynamics was assessed. The surface energies of the nanosized materials are similar within the errors regardless of the composition, and are consistent with those determined for other spinels. The enthalpies of oxidation to hematite plus rutile of the iron titanium spinels follow a linear trend with the Fe2+ content, which allows them to be calculated for any composition or particle size. The heat of formation of the macroscopic and nanosized titanomagnetites was fit as a polynomial function and the numerical coefficients are presented. The enthalpies of mixing in the titanomagnetite and titanomaghemite solid solutions are similar at the macroscopic and nanoscale. C1 [Lilova, Kristina I.; Navrotsky, Alexandra] Univ Calif Davis, Peter A Rock Thermochem Lab, Davis, CA 95616 USA. [Lilova, Kristina I.; Navrotsky, Alexandra] Univ Calif Davis, NEAT ORU, Davis, CA 95616 USA. [Pearce, Carolyn I.; Rosso, Kevin M.] Pacific NW Natl Lab, Richland, WA 99352 USA. [Pearce, Carolyn I.] Univ Manchester, Sch Chem, Manchester M13 9PL, Lancs, England. RP Navrotsky, A (reprint author), Univ Calif Davis, Peter A Rock Thermochem Lab, Davis, CA 95616 USA. EM anavrotsky@ucdavis.edu FU Pacific Northwest National Laboratory Science Focus Area (SFA) Subsurface Biogeochemical Research (SBR) Program of the U.S. Department of Energy (DOE) Office of Science; DOE Office of Science, Office of Basic Energy Sciences [DE-AC02-05CH11231]; PNNL [DEAC02-98CH10886]; UCD [DEAC02-98CH10886] FX We gratefully acknowledge support from the Pacific Northwest National Laboratory Science Focus Area (SFA) Subsurface Biogeochemical Research (SBR) Program of the U.S. Department of Energy (DOE) Office of Science. We acknowledge Elke Arenholz for her assistance with XA and XMCD measurements. XA and XMCD measurements were performed at the Advance Light Source supported by the DOE Office of Science, Office of Basic Energy Sciences under contract no. DE-AC02-05CH11231. Calorimetry was supported by contract DEAC02-98CH10886 between PNNL and UCD. NR 44 TC 3 Z9 3 U1 8 U2 37 PU WILEY-V C H VERLAG GMBH PI WEINHEIM PA BOSCHSTRASSE 12, D-69469 WEINHEIM, GERMANY SN 1439-4235 EI 1439-7641 J9 CHEMPHYSCHEM JI ChemPhysChem PD NOV 10 PY 2014 VL 15 IS 16 BP 3655 EP 3662 DI 10.1002/cphc.201402441 PG 8 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AS6JW UT WOS:000344370900031 PM 25178637 ER PT J AU Rasthofer, U Burton, GC Wall, WA Gravemeier, V AF Rasthofer, U. Burton, G. C. Wall, W. A. Gravemeier, V. TI An algebraic variational multiscale-multigrid-multifractal method (AVM(4)) for large-eddy simulation of turbulent variable-density flow at low Mach number SO INTERNATIONAL JOURNAL FOR NUMERICAL METHODS IN FLUIDS LA English DT Article DE large-eddy simulation; turbulent variable-density flow; multifractal subgrid-scale modeling; algebraic-multigrid scale separation; turbulent channel flow; backward-facing step ID BACKWARD-FACING STEP; NAVIER-STOKES EQUATIONS; FINITE-ELEMENT-METHOD; DIRECT NUMERICAL-SIMULATION; SUBGRID-SCALE MODEL; HEAT-TRANSFER; CHANNEL FLOW; SHEAR FLOWS; A-PRIORI; DOWNSTREAM AB An algebraic variational multiscale-multigrid-multifractal method is proposed for large-eddy simulation of turbulent variable-density flow at low Mach number. In the multifractal subgrid-scale modeling approach, the subgrid-scale quantities are explicitly evaluated from a multifractal description of associated gradient fields. The multifractal subgrid-scale modeling approach is embedded into a residual-based form of the variational multiscale method. A particular feature of the proposed form of the multifractal subgrid-scale modeling approach is scale separation by level-transfer operators from plain aggregation algebraic multigrid methods to identify the required smaller resolved scales. In this study, we introduce a novel development of the multifractal subgrid-scale modeling approach for application to turbulent variable-density flow at low Mach number. Based on the physical background, we derive a variable-density extension of the multifractal subgrid-scale modeling approach to recover the subgrid-scale velocity and temperature field. The proposed method is validated via two numerical test cases. First, turbulent flow in a channel with a heated and a cooled wall is considered for two different temperature ratios. Second, turbulent flow over a backward-facing step with heating is investigated. The results obtained with the algebraic variational multiscale-multigrid-multifractal method are compared with results obtained with the widely-used dynamic Smagorinsky model and a residual-based variational multiscale method. Particularly, the results obtained for turbulent flow in a channel with a heated and a cooled wall indicate the excellent prediction quality achievable by the proposed method for turbulent variable-density flow at low Mach number. Copyright (C) 2014 John Wiley & Sons, Ltd. C1 [Rasthofer, U.; Wall, W. A.; Gravemeier, V.] Tech Univ Munich, Inst Computat Mech, D-85748 Garching, Germany. [Burton, G. C.] Lawrence Livermore Natl Lab, Turbulence Anal & Simulat Ctr, Thermal Fluids Grp, Computat Engn Div, Livermore, CA 94551 USA. [Wall, W. A.; Gravemeier, V.] AdCo EngineeringGW GmbH, D-85748 Garching, Germany. RP Gravemeier, V (reprint author), Tech Univ Munich, Inst Computat Mech, Boltzmannstr 15, D-85748 Garching, Germany. EM vgravem@lnm.mw.tum.de FU Leibniz Supercomputing Center [pr83te] FX Computational resources provided by the Leibniz Supercomputing Center under the project pr83te are gratefully acknowledged. NR 71 TC 3 Z9 3 U1 1 U2 8 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0271-2091 EI 1097-0363 J9 INT J NUMER METH FL JI Int. J. Numer. Methods Fluids PD NOV 10 PY 2014 VL 76 IS 7 BP 416 EP 449 DI 10.1002/fld.3940 PG 34 WC Computer Science, Interdisciplinary Applications; Mathematics, Interdisciplinary Applications; Mechanics; Physics, Fluids & Plasmas SC Computer Science; Mathematics; Mechanics; Physics GA AQ4TV UT WOS:000342793500002 ER PT J AU Zalupski, PR McDowell, R Dutech, G AF Zalupski, Peter R. McDowell, Rocklan Dutech, Guy TI The Adsorption of Gold, Palladium, and Platinum from Acidic Chloride Solutions on Mesoporous Carbons SO SOLVENT EXTRACTION AND ION EXCHANGE LA English DT Article DE adsorption; Mesoporous carbon; palladium; gold; electronic scrap; platinum ID SELECTIVE RECOVERY; ACTIVATED CARBON; PRECIOUS METALS; PERSIMMON TANNIN; NANOPARTICLES; NANOTUBES; SORPTION; WASTE; IONS; GELS AB Studies on the adsorption characteristics of gold, palladium, and platinum on mesoporous carbon (CMK-3) and sulfur-impregnated mesoporous carbon (CMK-3/S) evaluated the benefits/drawbacks of the presence of a layer of elemental sulfur inside mesoporous carbon structures. Adsorption isotherms collected for Au(III), Pd(II), and Pt(IV) on those materials suggest that sulfur does enhance the adsorption of those metal ions in mildly acidic environment (pH 3). The isotherms collected in 1 M HCl show that the benefit of sulfur disappears due to the competing influence of large concentration of chloride ions on the ion-exchanging mechanism of metal ions sorption on mesoporous carbon surfaces. The collected acid dependencies illustrate similar adsorption characteristics for CMK-3 and CMK-3/S in 1-5 M HCl concentration range. Sorption of metal ions from diluted aqueous acidic mixtures of actual leached electronic waste demonstrated the feasibility of recovery of gold from such liquors. C1 [Zalupski, Peter R.; McDowell, Rocklan; Dutech, Guy] Idaho Natl Lab, Aqueous Separat & Radiochem Dept, Idaho Falls, ID 83415 USA. RP Zalupski, PR (reprint author), Idaho Natl Lab, Aqueous Separat & Radiochem Dept, Idaho Falls, ID 83415 USA. EM Peter.Zalupski@inl.gov FU Laboratory Directed Research and Development Program, U.S. Department of Energy, under DOE Idaho Operations Office [DE-AC07-05ID14517]; Idaho National Laboratory FX This research was sponsored by the Laboratory Directed Research and Development Program, U.S. Department of Energy, under DOE Idaho Operations Office contract DE-AC07-05ID14517 with Idaho National Laboratory, managed by Battelle Energy Alliance, LLC. NR 27 TC 1 Z9 1 U1 7 U2 45 PU TAYLOR & FRANCIS INC PI PHILADELPHIA PA 530 WALNUT STREET, STE 850, PHILADELPHIA, PA 19106 USA SN 0736-6299 EI 1532-2262 J9 SOLVENT EXTR ION EXC JI Solvent Extr. Ion Exch. PD NOV 10 PY 2014 VL 32 IS 7 BP 737 EP 748 DI 10.1080/07366299.2014.951278 PG 12 WC Chemistry, Multidisciplinary SC Chemistry GA AQ5FJ UT WOS:000342831700005 ER PT J AU Zapol, B Zapol, P AF Zapol, Boris Zapol, Peter TI Explicit expressions for totally symmetric spherical functions and symmetry-dependent properties of multipoles SO PROCEEDINGS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES LA English DT Article DE symmetric function; point group; projection operator; multipole; selection rule ID ICOSAHEDRAL GROUP; ADAPTED FUNCTIONS; MOMENTS; BASES AB Closed expressions for matrix elements < lm'|A(G)|lm >, where |lm > are spherical functions and A(G) is the average of all symmetry operators of point group G, are derived for all point groups (PGs) and then used to obtain linear combinations of spherical functions that are totally symmetric under all symmetry operations of G. In the derivation, we exploit the product structure of the groups. The obtained expressions are used to explore properties of multipoles of symmetric charge distributions. We produce complete lists of selection rules for multipoles Q(l) and their moments Q(lm), as well as of numbers of independent moments in a multipole, for any l and m and for all PGs. Periodicities and other trends in these properties are revealed. C1 [Zapol, Boris] Univ Latvia, Inst Chem Phys, LV-1586 Riga, Latvia. [Zapol, Peter] Argonne Natl Lab, Div Mat Sci, Argonne, IL 60439 USA. RP Zapol, B (reprint author), Univ Latvia, Inst Chem Phys, 19 Raina Blvd, LV-1586 Riga, Latvia. EM bpz7x11x13@gmail.com FU U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, Materials Sciences and Engineering Division [DE-AC02-06CH11357] FX P.Z. is supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, Materials Sciences and Engineering Division under Contract No. DE-AC02-06CH11357. NR 27 TC 0 Z9 0 U1 0 U2 2 PU ROYAL SOC PI LONDON PA 6-9 CARLTON HOUSE TERRACE, LONDON SW1Y 5AG, ENGLAND SN 1364-5021 EI 1471-2946 J9 P ROY SOC A-MATH PHY JI Proc. R. Soc. A-Math. Phys. Eng. Sci. PD NOV 8 PY 2014 VL 470 IS 2171 AR 20140435 DI 10.1098/rspa.2014.0435 PG 17 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA CQ4WM UT WOS:000360605300004 ER PT J AU Weinstein, M Heifetz, A Klann, R AF Weinstein, Marvin Heifetz, Alexander Klann, Raymond TI Detection of nuclear sources in search survey using dynamic quantum clustering of gamma-ray spectral data SO EUROPEAN PHYSICAL JOURNAL PLUS LA English DT Article ID SPECTROMETRY AB In a search scenario, nuclear background spectra are continuously measured in short acquisition intervals with a mobile detector-spectrometer. Detecting sources from measured data is difficult because of low signal-to-noise ratio (S/N) of spectra, large and highly varying background due to naturally occurring radioactive material (NORM), and line broadening due to limited spectral resolution of nuclear detector. We have invented a method for detection of sources using clustering of spectral data. Our method takes advantage of the physical fact that a source not only produces counts in the region of its spectral emission, but also has the effect on the entire detector spectrum via Compton continuum. This allows characterizing the low S/N spectrum without distinct isotopic lines using multiple data features. We have shown that noisy spectra with low S/N can be grouped by overall spectral shape similarity using a data clustering technique called Dynamic Quantum Clustering (DQC). The spectra in the same cluster can then be averaged to enhance S/N of the isotopic spectral line. This would allow for increased accuracy of isotopic identification and lower false alarm rate. Our method was validated in a proof-of-principle study using a data set of spectra measured in one-second intervals with sodium iodide detector. The data set consisted of over 7000 spectra obtained in urban background measurements, and approximately 70 measurements of Cs-137 and Co-60 sources. Using DQC analysis, we have observed that all spectra containing Cs-137 and Co-60 signal cluster away from the background. C1 [Weinstein, Marvin] Quantum Insights LLC, Palo Alto, CA 94303 USA. [Weinstein, Marvin] Stanford Linear Accelerator Ctr, Menlo Pk, CA 94025 USA. [Heifetz, Alexander; Klann, Raymond] Argonne Natl Lab, Nucl Engn Div, Lemont, IL 60439 USA. RP Weinstein, M (reprint author), Quantum Insights LLC, 3845 Nathan Way, Palo Alto, CA 94303 USA. EM aheifetz@anl.gov FU National Science Foundation Cyber-Physical Systems grant [CNS-1329657]; Argonne, a U.S. Department of Energy Office of Science laboratory [DE-AC02-06CH11357] FX This work was supported in part by the National Science Foundation Cyber-Physical Systems grant CNS-1329657. The submitted manuscript has been created by UChicago Argonne, LLC, Operator of Argonne National Laboratory ("Argonne"). Argonne, a U.S. Department of Energy Office of Science laboratory, is operated under Contract No. DE-AC02-06CH11357. NR 17 TC 1 Z9 1 U1 1 U2 2 PU SPRINGER HEIDELBERG PI HEIDELBERG PA TIERGARTENSTRASSE 17, D-69121 HEIDELBERG, GERMANY SN 2190-5444 J9 EUR PHYS J PLUS JI Eur. Phys. J. Plus PD NOV 7 PY 2014 VL 129 IS 11 AR 239 DI 10.1140/epjp/i2014-14239-3 PG 11 WC Physics, Multidisciplinary SC Physics GA CH0RA UT WOS:000353728700001 ER PT J AU Beck, AR Bernhardt, B Warrick, ER Wu, MX Chen, S Gaarde, MB Schafer, KJ Neumark, DM Leone, SR AF Beck, Annelise R. Bernhardt, Birgitta Warrick, Erika R. Wu, Mengxi Chen, Shaohao Gaarde, Mette B. Schafer, Kenneth J. Neumark, Daniel M. Leone, Stephen R. TI Attosecond transient absorption probing of electronic superpositions of bound states in neon: detection of quantum beats SO NEW JOURNAL OF PHYSICS LA English DT Article DE attosecond transient absorption; quantum beating; electronic wavepackets ID TRANSITION-PROBABILITIES; OSCILLATOR-STRENGTHS; PULSES; LINES; NEI; LIFETIMES; DYNAMICS; LIGHT; NE(I) AB Electronic wavepackets composed of multiple bound excited states of atomic neon lying between 19.6 and 21.5 eV are launched using an isolated attosecond pulse. Individual quantum beats of the wavepacket are detected by perturbing the induced polarization of the medium with a time-delayed few-femtosecond near-infrared (NIR) pulse via coupling the individual states to multiple neighboring levels. All of the initially excited states are monitored simultaneously in the attosecond transient absorption spectrum, revealing Lorentzian to Fano lineshape spectral changes as well as quantum beats. The most prominent beating of the several that were observed was in the spin-orbit split 3d absorption features, which has a 40 femtosecond period that corresponds to the spin-orbit splitting of 0.1 eV. The few-level models and multilevel calculations confirm that the observed magnitude of oscillation depends strongly on the spectral bandwidth and tuning of the NIR pulse and on the location of possible coupling states. C1 [Beck, Annelise R.; Bernhardt, Birgitta; Warrick, Erika R.; Neumark, Daniel M.; Leone, Stephen R.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Chem Sci, Ultrafast Xray Sci Lab, Berkeley, CA 94720 USA. [Beck, Annelise R.; Bernhardt, Birgitta; Warrick, Erika R.; Neumark, Daniel M.; Leone, Stephen R.] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA. [Wu, Mengxi; Chen, Shaohao; Gaarde, Mette B.; Schafer, Kenneth J.] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA. [Leone, Stephen R.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA. RP Beck, AR (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Chem Sci, Ultrafast Xray Sci Lab, Berkeley, CA 94720 USA. EM srl@berkeley.edu RI Bernhardt, Birgitta/L-9424-2015; Neumark, Daniel/B-9551-2009; OI Bernhardt, Birgitta/0000-0001-7537-4689; Neumark, Daniel/0000-0002-3762-9473; Warrick, Erika/0000-0003-0637-7645 FU Director, Office of Science, Office of Basic Energy Sciences; Division of Chemical Sciences, Geosciences, and Biosciences of the US Department of Energy at LBNL [DE-AC02-05CH11231]; LSU [DE-FG02-13ER16403]; NSF-GRFP; Alexander von Humboldt Foundation; National Security Science and Engineering Faculty Fellowship FX This work was supported by the Director, Office of Science, Office of Basic Energy Sciences and by the Division of Chemical Sciences, Geosciences, and Biosciences of the US Department of Energy at LBNL under contract nos. DE-AC02-05CH11231 and at LSU under contract no. DE-FG02-13ER16403. ARB acknowledges funding from NSF-GRFP. BB acknowledges support from the Alexander von Humboldt Foundation. SRL acknowledges the support of a National Security Science and Engineering Faculty Fellowship. The authors thank Camila Bacellar, Adam Chatterley, Mike Ziemkiewicz and He Wang for the loan of optics. NR 39 TC 24 Z9 24 U1 1 U2 39 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 1367-2630 J9 NEW J PHYS JI New J. Phys. PD NOV 7 PY 2014 VL 16 AR 113016 DI 10.1088/1367-2630/16/11/113016 PG 12 WC Physics, Multidisciplinary SC Physics GA AX1NH UT WOS:000346713100003 ER PT J AU Wang, SY Tan, LZ Wang, WH Louie, SG Lin, NA AF Wang, Shiyong Tan, Liang Z. Wang, Weihua Louie, Steven G. Lin, Nian TI Manipulation and Characterization of Aperiodical Graphene Structures Created in a Two-Dimensional Electron Gas SO PHYSICAL REVIEW LETTERS LA English DT Article ID MASSLESS DIRAC FERMIONS; EDGE STATES; NANORIBBONS AB We demonstrate that Dirac fermions can be created and manipulated in a two-dimensional electron gas (2DEG). Using a cryogenic scanning tunneling microscope, we arranged coronene molecules one by one on a Cu(111) surface to construct artificial graphene nanoribbons with perfect zigzag (ZGNRs) or arm chairedges and confirmed that new states localized along the edges emerge only in the ZGNRs. We further made and studied several typical defects, such as single vacancies, Stone-Wales defects, and dislocation lines, and found that all these defects introduce localized states at or near the Dirac point in the quasiparticle spectra. Our results confirm that artificial systems built on a 2DEG provide rigorous experimental verifications for several long-sought theoretical predications of aperiodic graphene structures. C1 [Wang, Shiyong; Wang, Weihua; Lin, Nian] Hong Kong Univ Sci & Technol, Dept Phys, Hong Kong, Hong Kong, Peoples R China. [Tan, Liang Z.; Louie, Steven G.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA. [Tan, Liang Z.; Louie, Steven G.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA. [Louie, Steven G.] Hong Kong Univ Sci & Technol, Inst Adv Study, Hong Kong, Hong Kong, Peoples R China. RP Lin, NA (reprint author), Hong Kong Univ Sci & Technol, Dept Phys, Hong Kong, Hong Kong, Peoples R China. EM phnlin@ust.hk RI Wang, Weihua/K-1297-2012; OI Wang, Weihua/0000-0002-2269-1952; Tan, Liang Z/0000-0003-4724-6369 FU Hong Kong RGC [602712]; National Science Foundation [DMR 10-1006184]; Director, Office of Science, Office of Basic Energy Sciences, Material Sciences and Engineering Division; U.S. Department of Energy [DE-AC02-05CH11231]; Simons Foundation Fellowship in Theoretical Physics; NICS (Kraken); National Science Foundation FX This work is supported by the Hong Kong RGC (No. 602712), the National Science Foundation Grant No. DMR 10-1006184 and by the Director, Office of Science, Office of Basic Energy Sciences, Material Sciences and Engineering Division, U.S. Department of Energy under Contract No. DE-AC02-05CH11231. S. G. L. acknowledges support from a Simons Foundation Fellowship in Theoretical Physics. We acknowledge the assistance of the XSEDE computational cluster resource provided by NICS (Kraken), supported by the National Science Foundation. NR 34 TC 9 Z9 9 U1 5 U2 29 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0031-9007 EI 1079-7114 J9 PHYS REV LETT JI Phys. Rev. Lett. PD NOV 7 PY 2014 VL 113 IS 19 AR 196803 DI 10.1103/PhysRevLett.113.196803 PG 5 WC Physics, Multidisciplinary SC Physics GA AU1CG UT WOS:000345358100011 PM 25415917 ER PT J AU Whitmer, JK Chiu, CC Joshi, AA de Pablo, JJ AF Whitmer, Jonathan K. Chiu, Chi-cheng Joshi, Abhijeet A. de Pablo, Juan J. TI Basis Function Sampling: A New Paradigm for Material Property Computation SO PHYSICAL REVIEW LETTERS LA English DT Article ID HISTOGRAM ANALYSIS METHOD; FREE-ENERGY CALCULATIONS; DENSITY-OF-STATES; MOLECULAR-DYNAMICS; MONTE-CARLO; PHASE-TRANSITIONS; LIQUID-CRYSTALS; SIMULATION; METADYNAMICS; LANDSCAPE AB Wang-Landau sampling, and the associated class of flat histogram simulation methods have been remarkably helpful for calculations of the free energy in a wide variety of physical systems. Practically, convergence of these calculations to a target free energy surface is hampered by reliance on parameters which are unknown a priori. Here, we derive and implement a method built upon orthogonal functions which is fast, parameter-free, and (importantly) geometrically robust. The method is shown to be highly effective in achieving convergence. An important feature of this method is its ability to attain arbitrary levels of description for the free energy. It is thus ideally suited to in silico measurement of elastic moduli and other material properties related to free energy perturbations. We demonstrate the utility of such applications by applying our method to calculate the Frank elastic constants of the Lebwohl-Lasher model of liquid crystals. C1 [Whitmer, Jonathan K.; Chiu, Chi-cheng; de Pablo, Juan J.] Univ Chicago, Inst Mol Engn, Chicago, IL 60637 USA. [Whitmer, Jonathan K.; Chiu, Chi-cheng; de Pablo, Juan J.] Argonne Natl Lab, Div Mat Sci, Argonne, IL 60439 USA. [Joshi, Abhijeet A.] Univ Wisconsin, Dept Chem & Biol Engn, Madison, WI 53706 USA. RP Whitmer, JK (reprint author), Univ Notre Dame, Dept Chem & Biomol Engn, Notre Dame, IN 46556 USA. FU University of Wisconsin Materials Science and Engineering Center (UW-MRSEC) under National Science Foundation [DMR-1121288]; Innovative and Novel Computational Impact on Theory and Experiment (INCITE) program of the Argonne Leadership Computing Facility at Argonne National Laboratory [DMR-1121288] FX We wish to thank S. Singh, M. McGovern, and T. F. Roberts for helpful discussions. The algorithm development presented within this work was supported by the U. S. Department of Energy, Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division. The calculation of elastic constants for liquid crystals was supported by the University of Wisconsin Materials Science and Engineering Center (UW-MRSEC) under National Science Foundation Grant No. DMR-1121288. An award of computer time was provided by the Innovative and Novel Computational Impact on Theory and Experiment (INCITE) program of the Argonne Leadership Computing Facility at Argonne National Laboratory. Additional development work was performed using the Argonne Laboratory Resource Computing Center (LCRC) and University of Chicago Midway cluster. NR 45 TC 3 Z9 3 U1 2 U2 26 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0031-9007 EI 1079-7114 J9 PHYS REV LETT JI Phys. Rev. Lett. PD NOV 7 PY 2014 VL 113 IS 19 AR 190602 DI 10.1103/PhysRevLett.113.190602 PG 5 WC Physics, Multidisciplinary SC Physics GA AU1CG UT WOS:000345358100002 PM 25415892 ER PT J AU Rozema, LA Mahler, DH Blume-Kohout, R Steinberg, AM AF Rozema, Lee A. Mahler, Dylan H. Blume-Kohout, Robin Steinberg, Aephraim M. TI Optimizing the Choice of Spin-Squeezed States for Detecting and Characterizing Quantum Processes SO PHYSICAL REVIEW X LA English DT Article ID COHERENT; SUBSYSTEMS; LIGHT AB Quantum metrology uses quantum states with no classical counterpart to measure a physical quantity with extraordinary sensitivity or precision. Most such schemes characterize a dynamical process by probing it with a specially designed quantum state. The success of such a scheme usually relies on the process belonging to a particular one-parameter family. If this assumption is violated, or if the goal is to measure more than one parameter, a different quantum state may perform better. In the most extreme case, we know nothing about the process and wish to learn everything. This requires quantum process tomography, which demands an informationally complete set of probe states. It is very convenient if this set is group covariant-i.e., each element is generated by applying an element of the quantum system's natural symmetry group to a single fixed fiducial state. In this paper, we consider metrology with 2-photon ("biphoton") states and report experimental studies of different states' sensitivity to small, unknown collective SU(2) rotations ["SU(2) jitter"]. Maximally entangled N00N states are the most sensitive detectors of such a rotation, yet they are also among the worst at fully characterizing an a priori unknown process. We identify (and confirm experimentally) the best SU(2)-covariant set for process tomography; these states are all less entangled than the N00N state, and are characterized by the fact that they form a 2-design. C1 [Rozema, Lee A.; Mahler, Dylan H.; Steinberg, Aephraim M.] Univ Toronto, Dept Phys, Ctr Quantum Informat & Quantum Control, Toronto, ON M5S 1A7, Canada. [Rozema, Lee A.; Mahler, Dylan H.; Steinberg, Aephraim M.] Univ Toronto, Inst Opt Sci, Toronto, ON M5S 1A7, Canada. [Blume-Kohout, Robin] Sandia Natl Labs, Comp Sci Res Inst, Albuquerque, NM 87123 USA. [Steinberg, Aephraim M.] Canadian Inst Adv Res, Toronto, ON M5G 1Z8, Canada. RP Rozema, LA (reprint author), Univ Toronto, Dept Phys, Ctr Quantum Informat & Quantum Control, 60 St George St, Toronto, ON M5S 1A7, Canada. RI Steinberg, Aephraim/C-3226-2008 FU Natural Sciences and Engineering Research Council of Canada (NSERC); Canadian Institute for Advanced Research (CIFAR); U.S. Department of Energy's National Nuclear Security Administration [DE-AC04-94AL85000] FX We thank Natural Sciences and Engineering Research Council of Canada (NSERC) and Canadian Institute for Advanced Research (CIFAR) for financial support. We also thank Peter Turner and Steven Flammia for helpful discussions. Sandia National Laboratories is a multiprogram laboratory operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the U.S. Department of Energy's National Nuclear Security Administration under Contract No. DE-AC04-94AL85000. NR 39 TC 4 Z9 4 U1 0 U2 8 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 2160-3308 J9 PHYS REV X JI Phys. Rev. X PD NOV 7 PY 2014 VL 4 IS 4 AR 041025 DI 10.1103/PhysRevX.4.041025 PG 9 WC Physics, Multidisciplinary SC Physics GA AU1BS UT WOS:000345356700001 ER PT J AU Jin, XG Cotta, AAC Chen, G Diaye, ATN Schmid, AK Yamamoto, N AF Jin, Xiuguang Cotta, Alexandre A. C. Chen, Gong Diaye, Alpha T. N. Schmid, Andreas K. Yamamoto, Naoto TI Low energy electron microscopy and Auger electron spectroscopy studies of Cs-O activation layer on p-type GaAs photocathode SO JOURNAL OF APPLIED PHYSICS LA English DT Article ID WORK-FUNCTION; ADSORPTION; AFFINITY; GAAS(100); SURFACES; BEAMS; LEED AB Work function, photoemission yield, and Auger electron spectra were measured on (001) p-type GaAs during negative electron affinity (NEA) surface preparation, surface degradation, and heating processes. The emission current sensitively depends on work function change and its dependence allows us to determine that the shape of the vacuum barrier was close to double triangular. Regarding the NEA surface degradation during photoemission, we discuss the importance of residual gas components the oxygen and hydrogen. We also found that gentle annealing (<= 100 degrees C) of aged photocathodes results in a lower work function and may offer a patch to reverse the performance degradation. (C) 2014 AIP Publishing LLC. C1 [Jin, Xiuguang] Nagoya Univ, Inst Adv Res, Nagoya, Aichi 4648603, Japan. [Cotta, Alexandre A. C.; Chen, Gong; Diaye, Alpha T. N.; Schmid, Andreas K.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, NCEM, Berkeley, CA 94720 USA. [Cotta, Alexandre A. C.] Univ Fed Minas Gerais, Dept Fis, ICEx, BR-31270901 Belo Horizonte, MG, Brazil. [Yamamoto, Naoto] Nagoya Univ, Synchrotron Radiat Res Ctr, Nagoya, Aichi 4648603, Japan. RP Jin, XG (reprint author), Nagoya Univ, Inst Adv Res, Nagoya, Aichi 4648603, Japan. RI Chen, Gong/H-3074-2015; Foundry, Molecular/G-9968-2014; OI Cotta, Alexandre/0000-0002-4464-1091 FU Office Science, Office of Basic Energy Sciences, of the U.S. Department of Energy [DE-AC02-05CH 11231]; Japan Society for the Promotion of Science (JSPS) [23246003, 25390066] FX This work was performed at the Molecular Foundry, National Center for Electron Microscopy, supported by the Office Science, Office of Basic Energy Sciences, of the U.S. Department of Energy under Contract No. DE-AC02-05CH 11231. This work was also supported by the Grants-in-Aid for Scientific Research (A) (23246003) and Grants-in-Aid for Scientific Research (C) (25390066) from the Japan Society for the Promotion of Science (JSPS). The authors are thankful to Dr. Weishi Wan (Lawrence Berkeley National Lab) for fruitful discussion and we thank Arantzazu Mascaraque (U. Complutense de Madrid) and Enriques Garcia Michel (U Autonoma de Madrid) for their helpful comments. NR 26 TC 1 Z9 1 U1 1 U2 26 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0021-8979 EI 1089-7550 J9 J APPL PHYS JI J. Appl. Phys. PD NOV 7 PY 2014 VL 116 IS 17 AR 174509 DI 10.1063/1.4901201 PG 6 WC Physics, Applied SC Physics GA AT7ZH UT WOS:000345152900065 ER PT J AU Kaur, M Jiang, WL Qiang, Y Burks, EC Liu, K Namavar, F McCloy, JS AF Kaur, Maninder Jiang, Weilin Qiang, You Burks, Edward C. Liu, Kai Namavar, Fereydoon McCloy, John S. TI Exchange bias in polycrystalline magnetite films made by ion-beam assisted deposition SO JOURNAL OF APPLIED PHYSICS LA English DT Article ID THIN-FILMS; MAGNETORESISTANCE; ARRAYS AB Iron oxide films were produced using ion-beam-assisted deposition, and Raman spectroscopy and x-ray diffraction indicate single-phase magnetite. However, incorporation of significant fractions of argon in the films from ion bombardment is evident from chemical analysis, and Fe/O ratios are lower than expected from pure magnetite, suggesting greater than normal disorder. Low temperature magnetometry and first-order reversal curve measurements show strong exchange bias, which likely arises from defects at grain boundaries, possibly amorphous, creating frustrated spins. Since these samples contain grains similar to 6 nm, a large fraction of the material consists of grain boundaries, where spins are highly disordered and reverse independently with external field. (C) 2014 AIP Publishing LLC. C1 [Kaur, Maninder; Qiang, You] Univ Idaho, Dept Phys, Moscow, ID 83844 USA. [Jiang, Weilin; McCloy, John S.] Pacific NW Natl Lab, Richland, WA 99352 USA. [Burks, Edward C.; Liu, Kai] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA. [Namavar, Fereydoon] Univ Nebraska Med Ctr, Omaha, NE 68198 USA. [McCloy, John S.] Washington State Univ, Sch Mech & Mat Engn, Pullman, WA 98163 USA. RP Kaur, M (reprint author), Univ Idaho, Dept Phys, Moscow, ID 83844 USA. RI Liu, Kai/B-1163-2008; OI Liu, Kai/0000-0001-9413-6782; Jiang, Weilin/0000-0001-8302-8313; McCloy, John/0000-0001-7476-7771 FU Laboratory Directed Research Development; NSF [DMR-1008791]; U.S. Department of Energy (DOE) [DE-AC05-76RL01830]; DOE's Office of Biological and Environmental Research located at PNNL FX This work was supported in part by Laboratory Directed Research & Development and in part by NSF (DMR-1008791). The Pacific Northwest National Laboratory (PNNL) is operated for the U.S. Department of Energy (DOE) by Battelle under Contract DE-AC05-76RL01830. Some of the research was performed using the Environmental Molecular Sciences Laboratory (EMSL), sponsored by the DOE's Office of Biological and Environmental Research and located at PNNL. The authors thank the following for assistance with characterization and helpful discussions: Alicia Certain and Matt Olszta for FIB/TEM, A. Scott Lea for MFM, Paul Gassman for Raman, Tim Droubay for magnetometry, and Tamas Varga for XRD data analysis. NR 27 TC 3 Z9 3 U1 0 U2 21 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0021-8979 EI 1089-7550 J9 J APPL PHYS JI J. Appl. Phys. PD NOV 7 PY 2014 VL 116 IS 17 AR 173902 DI 10.1063/1.4900747 PG 6 WC Physics, Applied SC Physics GA AT7ZH UT WOS:000345152900033 ER PT J AU Popovic, S Upadhyay, J Mammosser, J Nikolic, M Vuskovic, L AF Popovic, S. Upadhyay, J. Mammosser, J. Nikolic, M. Vuskovic, L. TI Resonant-frequency discharge in a multi-cell radio frequency cavity SO JOURNAL OF APPLIED PHYSICS LA English DT Article ID GLOW-DISCHARGE; PLASMA; ITER AB We are reporting experimental results on a microwave discharge operating at resonant frequency in a multi-cell radio frequency (RF) accelerator cavity. Although the discharge operated at room temperature, the setup was constructed so that it could be used for plasma generation and processing in fully assembled active superconducting radio-frequency cryo-module. This discharge offers a mechanism for removal of a variety of contaminants, organic or oxide layers, and residual particulates from the interior surface of RF cavities through the interaction of plasma-generated radicals with the cavity walls. We describe resonant RF breakdown conditions and address the issues related to resonant detuning due to sustained multi-cell cavity plasma. We have determined breakdown conditions in the cavity, which was acting as a plasma vessel with distorted cylindrical geometry. We discuss the spectroscopic data taken during plasma removal of contaminants and use them to evaluate plasma parameters, characterize the process, and estimate the volatile contaminant product removal. (C) 2014 AIP Publishing LLC. C1 [Popovic, S.; Upadhyay, J.; Nikolic, M.; Vuskovic, L.] Old Dominion Univ, Dept Phys, Ctr Accelerator Sci, Norfolk, VA 23529 USA. [Mammosser, J.] Thomas Jefferson Natl Accelerator Facil, Newport News, VA 23606 USA. RP Popovic, S (reprint author), Old Dominion Univ, Dept Phys, Ctr Accelerator Sci, Norfolk, VA 23529 USA. OI Popovic, Svetozar/0000-0002-3668-4841 FU JSA/DOE [DE-AC05-060R23177]; Accelerator Division, Thomas Jefferson National Accelerator Facility under JSA/DOE FX This work was supported by JSA/DOE Contract No. DE-AC05-060R23177. J. Upadhyay acknowledges the financial support from the Accelerator Division, Thomas Jefferson National Accelerator Facility under the same contract. NR 22 TC 0 Z9 0 U1 0 U2 3 PU AMER INST PHYSICS PI MELVILLE PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA SN 0021-8979 EI 1089-7550 J9 J APPL PHYS JI J. Appl. Phys. PD NOV 7 PY 2014 VL 116 IS 17 AR 173301 DI 10.1063/1.4900994 PG 7 WC Physics, Applied SC Physics GA AT7ZH UT WOS:000345152900010 ER PT J AU Samolyuk, GD Ujfalussy, B Stocks, GM AF Samolyuk, G. D. Ujfalussy, B. Stocks, G. M. TI The distribution alloying elements in alnico 8 and 9 magnets: Site preference of ternary Ti, Fe, Co, and Ni additions in DO3 Fe3Al, Co3Al, and Ni3Al based intermetallic phases SO JOURNAL OF APPLIED PHYSICS LA English DT Article ID EFFECTIVE FORMATION ENERGIES; ATOMIC DEFECTS; POINT-DEFECTS; PERMANENT-MAGNETS; AB-INITIO; 1ST-PRINCIPLES; PSEUDOPOTENTIALS AB Recently, interest in alnico magnetic alloys has been rekindled due to their potential to substitute for rare-earth based permanent magnets provided modest improvements in their coercivity can be achieved without loss of saturation magnetization. Recent experimental studies have indicated that atomic and magnetic structure of the two phases (one AlNi-based, the other FeCo-based) that comprise these spinodally decomposed alloy is not as simple as previously thought. A key issue that arises is the distribution of Fe, Co, and Ti within the AlNi-based matrix phase. In this paper, we report the results of first-principles calculations of the site preference of ternary alloying additions in DO3 Fe3Al, Co3Al, and Ni3Al alloys, as models for the aluminide phase. For compound compositions that are Al rich, which correspond to experimental situation, Ti and Fe are found to occupy the alpha sites, while Co and Ni prefer the gamma sites of the DO3 lattice. An important finding is that the magnetic moments of transition metals in Fe3Al and Co3Al are ordered ferromagnetically, whereas the Ni3Al were found to be nonmagnetic unless the Fe or Co is added as a ternary element. (C) 2014 AIP Publishing LLC. C1 [Samolyuk, G. D.; Stocks, G. M.] Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA. [Ujfalussy, B.] Hungarian Acad Sci, Wigner Res Ctr Phys, H-1121 Budapest, Hungary. RP Samolyuk, GD (reprint author), Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA. RI Ujfalussy, Balazs/A-8155-2013; Stocks, George Malcollm/Q-1251-2016 OI Ujfalussy, Balazs/0000-0003-3338-4699; Stocks, George Malcollm/0000-0002-9013-260X FU U.S. Department of Energy, Office of Energy Efficiency and Renewable Energy (EERE), under its Vehicle Technologies Program, through the Ames Laboratory; Hungarian National Science Foundation [OTKA 84078]; [DE-AC02-07CH11358] FX One of the authors (G. S.) is grateful to Dr. C. L. Fu and Dr. A. Barashev for useful discussions. G. S. and G. M. S. were supported by the U.S. Department of Energy, Office of Energy Efficiency and Renewable Energy (EERE), under its Vehicle Technologies Program, through the Ames Laboratory. Ames Laboratory is operated by Iowa State University under Contract No. DE-AC02-07CH11358. B. U. was supported by the Hungarian National Science Foundation under OTKA 84078. NR 31 TC 1 Z9 1 U1 6 U2 45 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0021-8979 EI 1089-7550 J9 J APPL PHYS JI J. Appl. Phys. PD NOV 7 PY 2014 VL 116 IS 17 AR 173908 DI 10.1063/1.4901229 PG 12 WC Physics, Applied SC Physics GA AT7ZH UT WOS:000345152900039 ER PT J AU Karkehabadi, S Helmich, KE Kaper, T Hansson, H Mikkelsen, NE Gudmundsson, M Piens, K Fujdala, M Banerjee, G Scott-Craig, JS Walton, JD Phillips, GN Sandgren, M AF Karkehabadi, Saeid Helmich, Kate E. Kaper, Thijs Hansson, Henrik Mikkelsen, Nils-Egil Gudmundsson, Mikael Piens, Kathleen Fujdala, Meredith Banerjee, Goutami Scott-Craig, John S. Walton, Jonathan D. Phillips, George N., Jr. Sandgren, Mats TI Biochemical Characterization and Crystal Structures of a Fungal Family 3 beta-Glucosidase, Cel3A from Hypocrea jecorina SO JOURNAL OF BIOLOGICAL CHEMISTRY LA English DT Article ID SUBSTRATE-BINDING REGION; TRICHODERMA-REESEI; MACROMOLECULAR STRUCTURES; 3-DIMENSIONAL STRUCTURE; FUNCTIONAL EXPRESSION; STRUCTURE REFINEMENT; STRUCTURE VALIDATION; MAXIMUM-LIKELIHOOD; DIFFRACTION DATA; HYDROLASE AB Cellulase mixtures from Hypocrea jecorina are commonly used for the saccharification of cellulose in biotechnical applications. The most abundant beta-glucosidase in the mesophilic fungus Hypocrea jecorina is HjCel3A, which hydrolyzes the beta-linkage between two adjacent molecules in dimers and short oligomers of glucose. It has been shown that enhanced levels of HjCel3A in H. jecorina cellulase mixtures benefit the conversion of cellulose to glucose. Biochemical characterization of HjCel3A shows that the enzyme efficiently hydrolyzes (1,4)-as well as (1,2)-, (1,3)-, and (1,6)-beta-D-linked disaccharides. For crystallization studies, HjCel3A was produced in both H. jecorina (HjCel3A) and Pichia pastoris (Pp-HjCel3A). Whereas the thermostabilities of HjCel3A and Pp-HjCel3A are the same, Pp-HjCel3A has a higher degree of N-linked glycosylation. Here, we present x-ray structures of HjCel3A with and without glucose bound in the active site. The structures have a three-domain architecture as observed previously for other glycoside hydrolase family 3 beta-glucosidases. Both production hosts resulted in HjCel3A structures that have N-linked glycosylations at Asn(208) and Asn(310). In H. jecorina-produced HjCel3A, a single N-acetylglucosamine is present at both sites, whereas in Pp-HjCel3A, the P. pastoris-produced HjCel3A enzyme, the glycan chains consist of 8 or 4 saccharides. The glycosylations are involved in intermolecular contacts in the structures derived from either host. Due to the different sizes of the glycosylations, the interactions result in different crystal forms for the two protein forms. C1 [Karkehabadi, Saeid; Hansson, Henrik; Mikkelsen, Nils-Egil; Gudmundsson, Mikael; Piens, Kathleen; Sandgren, Mats] Swedish Univ Agr Sci, Dept Chem & Biotechnol, SE-75007 Uppsala, Sweden. [Helmich, Kate E.; Phillips, George N., Jr.] Univ Wisconsin, Dept Energy, Great Lakes Bioenergy Res Ctr, Madison, WI 53706 USA. [Helmich, Kate E.; Phillips, George N., Jr.] Univ Wisconsin, Dept Biochem, Madison, WI 53706 USA. [Kaper, Thijs; Fujdala, Meredith] DuPont Ind Biosci, Palo Alto, CA 94304 USA. [Banerjee, Goutami; Scott-Craig, John S.; Walton, Jonathan D.] Michigan State Univ, Dept Energy, Great Lakes Bioenergy Res Ctr, E Lansing, MI 48824 USA. [Phillips, George N., Jr.] Rice Univ, Dept Biochem & Cell Biol, Houston, TX 77251 USA. [Phillips, George N., Jr.] Rice Univ, Dept Chem, Houston, TX 77251 USA. RP Phillips, GN (reprint author), Rice Univ, Dept Biochem & Cell Biol, POB 1892, Houston, TX 77251 USA. EM georgep@rice.edu; mats.sandgren@slu.se FU Faculty for Natural Resources and Agriculture at the Swedish University of Agricultural Sciences; United States Department of Energy Great Lakes Bioenergy Research Center (Department of Energy Office of Science Biological and Environmental Research (BER) [DE-FC02-07ER64494] FX This work was supported in part by the Faculty for Natural Resources and Agriculture at the Swedish University of Agricultural Sciences through the research program "MicroDrivE." Work in the laboratories of J. D. W. and G. N. P. was supported by the United States Department of Energy Great Lakes Bioenergy Research Center (Department of Energy Office of Science Biological and Environmental Research (BER) Grant DE-FC02-07ER64494). NR 70 TC 15 Z9 15 U1 4 U2 49 PU AMER SOC BIOCHEMISTRY MOLECULAR BIOLOGY INC PI BETHESDA PA 9650 ROCKVILLE PIKE, BETHESDA, MD 20814-3996 USA SN 0021-9258 EI 1083-351X J9 J BIOL CHEM JI J. Biol. Chem. PD NOV 7 PY 2014 VL 289 IS 45 BP 31624 EP 31637 DI 10.1074/jbc.M114.587766 PG 14 WC Biochemistry & Molecular Biology SC Biochemistry & Molecular Biology GA AS9GA UT WOS:000344549900062 PM 25164811 ER PT J AU Brown, TN O'Donovan, M Hasselquist, L Corner, B Schiffman, JM AF Brown, Tyler N. O'Donovan, Meghan Hasselquist, Leif Corner, Brian Schiffman, Jeffrey M. TI Soldier-relevant loads impact lower limb biomechanics during anticipated and unanticipated single-leg cutting movements SO JOURNAL OF BIOMECHANICS LA English DT Article DE Joint power; Kinematics; Kinetics; Locomotion; Backpack; Stance time ID LOWER-EXTREMITY BIOMECHANICS; CRUCIATE LIGAMENT INJURY; JOINT COORDINATE SYSTEM; GROUND REACTION FORCES; KNEE-JOINT; SPATIOTEMPORAL PARAMETERS; DROP-LANDINGS; BACKPACK LOAD; ACL INJURY; KINEMATICS AB This study quantified how body borne load impacts hip and knee biomechanics during anticipated and unanticipated single-leg cutting maneuvers. Fifteen male military personnel performed a series of single-leg cutting maneuvers with three different load configurations (light, similar to 6 kg, medium, similar to 20 kg, and heavy, similar to 40 kg). Subject-based means of the specific lower limb biomechanical variables were submitted to repeated measures ANOVA to test the main and interaction effects of body borne load and movement type. With body borne load, stance time (P<0.001) increased, while larger hip (P=0.027) and knee flexion (P=0.004), and hip adduction (P<0.001) moments, and decreased hip (P=0.002) and knee flexion (P<0.001), and hip adduction (P=0.003) postures were evident. Further, the hip (P<0.001) and ankle (P=0.024) increased energy absorption, while the knee (P=0.020) increased energy generation with body borne load. During the unanticipated maneuvers, the hip (P=0.009) and knee (P=0.032) increased energy generation, and peak hip flexion moment (P=0.002) increased relative to the anticipated movements. With the body borne load, participants adopted biomechanical patterns that decreased their locomotive ability including larger moments and reduced flexion postures of the lower limb. During the single-leg cut, participants used greater energy absorption from the large, proximal muscles of the hip and greater energy generation from the knee with the addition of load. Participant's performance when carrying a range of loads was not compromised by anticipation, as they did not exhibit the hip and knee kinetic and kinematic adaptations previously demonstrated when reacting to an unplanned stimulus. Published by Elsevier Ltd. C1 [Brown, Tyler N.] Oak Ridge Inst Sci & Educ, Belcamp, MD USA. [Brown, Tyler N.; O'Donovan, Meghan; Hasselquist, Leif; Corner, Brian; Schiffman, Jeffrey M.] US Army, Natick Soldier Res Dev & Engn Ctr, Natick, MA 01760 USA. [Schiffman, Jeffrey M.] Liberty Mutual Res Inst Safety, Hopkinton, MA USA. RP Brown, TN (reprint author), Natick Soldier RD & E Ctr, Dept Army, 15 Kansas St, Natick, MA 01760 USA. EM tyler.n.brown4.civ@mail.mil FU Competitive In-house Laboratory Independent Research (ILIR) Award program from the Department of the Army, Office of the Assistant Secretary of the Army - Acquisition Logistics and Technology FX This work was supported by a FY 2012-2014 Competitive In-house Laboratory Independent Research (ILIR) Award program from the Department of the Army, Office of the Assistant Secretary of the Army - Acquisition Logistics and Technology. The authors thank Ms. Marina Carboni and Mr. Albert Adams for their assistance with this study. NR 47 TC 5 Z9 5 U1 0 U2 15 PU ELSEVIER SCI LTD PI OXFORD PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, OXON, ENGLAND SN 0021-9290 EI 1873-2380 J9 J BIOMECH JI J. Biomech. PD NOV 7 PY 2014 VL 47 IS 14 BP 3494 EP 3501 DI 10.1016/j.jbiomech.2014.09.002 PG 8 WC Biophysics; Engineering, Biomedical SC Biophysics; Engineering GA AT8KZ UT WOS:000345183500010 PM 25257813 ER PT J AU Adare, A Afanasiev, S Aidala, C Ajitanand, NN Akiba, Y Akimoto, R Al-Bataineh, H Alexander, J Alfred, M Angerami, A Aoki, K Apadula, N Aphecetche, L Aramaki, Y Armendariz, R Aronson, SH Asai, J Asano, H Atomssa, ET Averbeck, R Awes, TC Azmoun, B Babintsev, V Bai, M Baksay, G Baksay, L Baldisseri, A Bandara, NS Bannier, B Barish, KN Barnes, PD Bassalleck, B Basye, AT Bathe, S Batsouli, S Baublis, V Baumann, C Bazilevsky, A Beaumier, M Beckman, S Belikov, S Belmont, R Bennett, R Berdnikov, A Berdnikov, Y Bhom, JH Bickley, AA Black, D Blau, DS Boissevain, JG Bok, JS Borel, H Boyle, K Brooks, ML Bryslawskyj, J Buesching, H Bumazhnov, V Bunce, G Butsyk, S Campbell, S Caringi, A Chang, BS Charvet, JL Chen, CH Chernichenko, S Chi, CY Chiba, J Chiu, M Choi, IJ Choi, JB Choudhury, RK Christiansen, P Chujo, T Chung, P Churyn, A Chvala, O Cianciolo, V Citron, Z Cleven, CR Cole, BA Comets, MP del Valle, ZC Connors, M Constantin, P Csanad, M Csorgo, T Dahms, T Dairaku, S Danchev, I Das, K Datta, A Daugherity, MS David, G Dayananda, MK Deaton, MB DeBlasio, K Dehmelt, K Delagrange, H Denisov, A d'Enterria, D Deshpande, A Desmond, EJ Dharmawardane, KV Dietzsch, O Ding, L Dion, A Do, JH Donadelli, M Drapier, O Drees, A Drees, KA Dubey, AK Durham, JM Durum, A Dutta, D Dzhordzhadze, V D'Orazio, L Edwards, S Efremenko, YV Egdemir, J Ellinghaus, F Emam, WS Engelmore, T Enokizono, A En'yo, H Esumi, S Eyser, KO Fadem, B Feege, N Fields, DE Finger, M Finger, M Fleuret, F Fokin, SL Fraenkel, Z Frantz, JE Franz, A Frawley, AD Fujiwara, K Fukao, Y Fusayasu, T Gadrat, S Gal, C Gallus, P Garg, P Garishvili, I Ge, H Giordano, F Glenn, A Gong, H Gonin, M Gosset, J Goto, Y de Cassagnac, RG Grau, N Greene, SV Grim, G Perdekamp, MG Gu, Y Gunji, T Guragain, H Gustafsson, HA Hachiya, T Henni, AH Haegemann, C Haggerty, JS Hahn, KI Hamagaki, H Hamblen, J Han, R Han, SY Hanks, J Harada, H Hartouni, EP Haruna, K Hasegawa, S Haslum, E Hayano, R He, X Heffner, M Hemmick, TK Hester, T Hiejima, H Hill, JC Hobbs, R Hohlmann, M Hollis, RS Holzmann, W Homma, K Hong, B Horaguchi, T Hornback, D Hoshino, T Huang, S Ichihara, T Ichimiya, R Iinuma, H Ikeda, Y Imai, K Imazu, Y Inaba, M Inoue, Y Iordanova, A Isenhower, D Isenhower, L Ishihara, M Isobe, T Issah, M Isupov, A Ivanischev, D Ivanishchev, D Iwanaga, Y Jacak, BV Jeon, SJ Jezghani, M Jia, J Jiang, X Jin, J Jinnouchi, O Johnson, BM Jones, T Joo, E Joo, KS Jouan, D Jumper, DS Kajihara, F Kametani, S Kamihara, N Kamin, J Kaneta, M Kang, JH Kang, JS Kanou, H Kapustinsky, J Karatsu, K Kasai, M Kawall, D Kawashima, M Kazantsev, AV Kempel, T Key, JA Khachatryan, V Khanzadeev, A Kihara, K Kijima, KM Kikuchi, J Kim, A Kim, BI Kim, C Kim, DH Kim, DJ Kim, E Kim, EJ Kim, HJ Kim, M Kim, YJ Kim, YK Kinney, E Kiss, A Kistenev, E Kiyomichi, A Klatsky, J Klay, J Klein-Boesing, C Kleinjan, D Kline, P Koblesky, T Kochenda, L Kochetkov, V Kofarago, M Komkov, B Konno, M Koster, J Kotchetkov, D Kotov, D Kozlov, A Kral, A Kravitz, A Kubart, J Kunde, GJ Kurihara, N Kurita, K Kurosawa, M Kweon, MJ Kwon, Y Kyle, GS Lacey, R Lai, YS Lajoie, JG Lebedev, A Lee, DM Lee, J Lee, KB Lee, KS Lee, MK Lee, SH Lee, T Leitch, MJ Leite, MAL Leitgab, M Lenzi, B Li, X Lichtenwalner, P Liebing, P Lim, SH Levy, LAL Liska, T Litvinenko, A Liu, H Liu, MX Love, B Lynch, D Maguire, CF Makdisi, YI Makek, M Malakhov, A Malik, MD Manion, A Manko, VI Mannel, E Mao, Y Masek, L Masui, H Matathias, F McCumber, M McGaughey, PL McGlinchey, D McKinney, C Means, N Meles, A Mendoza, M Meredith, B Miake, Y Mibe, T Mignerey, AC Mikes, P Miki, K Miller, AJ Miller, TE Milov, A Mioduszewski, S Mishra, DK Mishra, M Mitchell, JT Mitrovski, M Miyasaka, S Mizuno, S Mohanty, AK Montuenga, P Moon, HJ Moon, T Morino, Y Morreale, A Morrison, DP Moukhanova, TV Mukhopadhyay, D Murakami, T Murata, J Mwai, A Nagamiya, S Nagata, Y Nagle, JL Naglis, M Nagy, MI Nakagawa, I Nakagomi, H Nakamiya, Y Nakamura, KR Nakamura, T Nakano, K Nam, S Nattrass, C Netrakanti, PK Newby, J Nguyen, M Nihashi, M Niida, T Norman, BE Nouicer, R Novitzky, N Nyanin, AS Oakley, C O'Brien, E Oda, SX Ogilvie, CA Ohnishi, H Oka, M Okada, K Omiwade, OO Onuki, Y Koop, JDO Oskarsson, A Ouchida, M Ozaki, H Ozawa, K Pak, R Pal, D Palounek, APT Pantuev, V Papavassiliou, V Park, IH Park, J Park, S Park, SK Park, WJ Pate, SF Patel, L Patel, M Pei, H Peng, JC Pereira, H Perepelitsa, DV Perera, GDN Peresedov, V Peressounko, DY Perry, J Petti, R Pinkenburg, C Pinson, R Pisani, RP Proissl, M Purschke, ML Purwar, AK Qu, H Rak, J Rakotozafindrabe, A Ravinovich, I Read, KF Rembeczki, S Reuter, M Reygers, K Reynolds, D Riabov, V Riabov, Y Richardson, E Riveli, N Roach, D Roche, G Rolnick, SD Romana, A Rosati, M Rosen, CA Rosendahl, SSE Rosnet, P Rowan, Z Rubin, JG Rukoyatkin, P Ruzicka, P Rykov, VL Sahlmueller, B Saito, N Sakaguchi, T Sakai, S Sakashita, K Sakata, H Sako, H Samsonov, V Sano, S Sarsour, M Sato, S Sato, T Sawada, S Schaefer, B Schmoll, BK Sedgwick, K Seele, J Seidl, R Semenov, V Sen, A Seto, R Sett, P Sexton, A Sharma, D Shein, I Shevel, A Shibata, TA Shigaki, K Shimomura, M Shoji, K Shukla, P Sickles, A Silva, CL Silvermyr, D Silvestre, C Sim, KS Singh, BK Singh, CP Singh, V Skutnik, S Slunecka, M Soldatov, A Soltz, RA Sondheim, WE Sorensen, SP Sourikova, IV Staley, F Stankus, PW Stenlund, E Stepanov, M Ster, A Stoll, SP Sugitate, T Suire, C Sukhanov, A Sumita, T Sun, J Sziklai, J Tabaru, T Takagi, S Takagui, EM Takahara, A Taketani, A Tanabe, R Tanaka, Y Taneja, S Tanida, K Tannenbaum, MJ Tarafdar, S Taranenko, A Tarjan, P Themann, H Thomas, D Thomas, TL Timilsina, A Todoroki, T Togawa, M Toia, A Tojo, J Tomasek, L Tomasek, M Torii, H Towell, M Towell, R Towell, RS Tram, VN Tserruya, I Tsuchimoto, Y Vale, C Valle, H van Hecke, HW Vargyas, M Vazquez-Zambrano, E Veicht, A Velkovska, J Vertesi, R Vinogradov, AA Virius, M Vrba, V Vznuzdaev, E Wagner, M Walker, D Wang, XR Watanabe, D Watanabe, K Watanabe, Y Watanabe, YS Wei, F Wei, R Wessels, J Whitaker, S White, SN Winter, D Wolin, S Woody, CL Wright, RM Wysocki, M Xia, B Xie, W Xue, L Yalcin, S Yamaguchi, YL Yamaura, K Yang, R Yanovich, A Yasin, Z Ying, J Yokkaichi, S Yoon, I You, Z Young, GR Younus, I Yushmanov, IE Zajc, WA Zaudtke, O Zelenski, A Zhang, C Zhou, S Zimanyi, J Zolin, L AF Adare, A. Afanasiev, S. Aidala, C. Ajitanand, N. N. Akiba, Y. Akimoto, R. Al-Bataineh, H. Alexander, J. Alfred, M. Angerami, A. Aoki, K. Apadula, N. Aphecetche, L. Aramaki, Y. Armendariz, R. Aronson, S. H. Asai, J. Asano, H. Atomssa, E. T. Averbeck, R. Awes, T. C. Azmoun, B. Babintsev, V. Bai, M. Baksay, G. Baksay, L. Baldisseri, A. Bandara, N. S. Bannier, B. Barish, K. N. Barnes, P. D. Bassalleck, B. Basye, A. T. Bathe, S. Batsouli, S. Baublis, V. Baumann, C. Bazilevsky, A. Beaumier, M. Beckman, S. Belikov, S. Belmont, R. Bennett, R. Berdnikov, A. Berdnikov, Y. Bhom, J. H. Bickley, A. A. Black, D. Blau, D. S. Boissevain, J. G. Bok, J. S. Borel, H. Boyle, K. Brooks, M. L. Bryslawskyj, J. Buesching, H. Bumazhnov, V. Bunce, G. Butsyk, S. Campbell, S. Caringi, A. Chang, B. S. Charvet, J. -L. Chen, C. -H. Chernichenko, S. Chi, C. Y. Chiba, J. Chiu, M. Choi, I. J. Choi, J. B. Choudhury, R. K. Christiansen, P. Chujo, T. Chung, P. Churyn, A. Chvala, O. Cianciolo, V. Citron, Z. Cleven, C. R. Cole, B. 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McKinney, C. Means, N. Meles, A. Mendoza, M. Meredith, B. Miake, Y. Mibe, T. Mignerey, A. C. Mikes, P. Miki, K. Miller, A. J. Miller, T. E. Milov, A. Mioduszewski, S. Mishra, D. K. Mishra, M. Mitchell, J. T. Mitrovski, M. Miyasaka, S. Mizuno, S. Mohanty, A. K. Montuenga, P. Moon, H. J. Moon, T. Morino, Y. Morreale, A. Morrison, D. P. Moukhanova, T. V. Mukhopadhyay, D. Murakami, T. Murata, J. Mwai, A. Nagamiya, S. Nagata, Y. Nagle, J. L. Naglis, M. Nagy, M. I. Nakagawa, I. Nakagomi, H. Nakamiya, Y. Nakamura, K. R. Nakamura, T. Nakano, K. Nam, S. Nattrass, C. Netrakanti, P. K. Newby, J. Nguyen, M. Nihashi, M. Niida, T. Norman, B. E. Nouicer, R. Novitzky, N. Nyanin, A. S. Oakley, C. O'Brien, E. Oda, S. X. Ogilvie, C. A. Ohnishi, H. Oka, M. Okada, K. Omiwade, O. O. Onuki, Y. Koop, J. D. Orjuela Oskarsson, A. Ouchida, M. Ozaki, H. Ozawa, K. Pak, R. Pal, D. Palounek, A. P. T. Pantuev, V. Papavassiliou, V. Park, I. H. Park, J. Park, S. Park, S. K. Park, W. J. Pate, S. F. Patel, L. Patel, M. Pei, H. Peng, J. -C. Pereira, H. Perepelitsa, D. V. Perera, G. D. N. Peresedov, V. Peressounko, D. Yu. Perry, J. Petti, R. Pinkenburg, C. Pinson, R. Pisani, R. P. Proissl, M. Purschke, M. L. Purwar, A. K. Qu, H. Rak, J. Rakotozafindrabe, A. Ravinovich, I. Read, K. F. Rembeczki, S. Reuter, M. Reygers, K. Reynolds, D. Riabov, V. Riabov, Y. Richardson, E. Riveli, N. Roach, D. Roche, G. Rolnick, S. D. Romana, A. Rosati, M. Rosen, C. A. Rosendahl, S. S. E. Rosnet, P. Rowan, Z. Rubin, J. G. Rukoyatkin, P. Ruzicka, P. Rykov, V. L. Sahlmueller, B. Saito, N. Sakaguchi, T. Sakai, S. Sakashita, K. Sakata, H. Sako, H. Samsonov, V. Sano, S. Sarsour, M. Sato, S. Sato, T. Sawada, S. Schaefer, B. Schmoll, B. K. Sedgwick, K. Seele, J. Seidl, R. Semenov, V. Sen, A. Seto, R. Sett, P. Sexton, A. Sharma, D. Shein, I. Shevel, A. Shibata, T. -A. Shigaki, K. Shimomura, M. Shoji, K. Shukla, P. Sickles, A. Silva, C. L. Silvermyr, D. Silvestre, C. Sim, K. S. Singh, B. K. Singh, C. P. Singh, V. Skutnik, S. Slunecka, M. Soldatov, A. Soltz, R. A. Sondheim, W. E. Sorensen, S. P. Sourikova, I. V. Staley, F. Stankus, P. W. Stenlund, E. Stepanov, M. Ster, A. Stoll, S. P. Sugitate, T. Suire, C. Sukhanov, A. Sumita, T. Sun, J. Sziklai, J. Tabaru, T. Takagi, S. Takagui, E. M. Takahara, A. Taketani, A. Tanabe, R. Tanaka, Y. Taneja, S. Tanida, K. Tannenbaum, M. J. Tarafdar, S. Taranenko, A. Tarjan, P. Themann, H. Thomas, D. Thomas, T. L. Timilsina, A. Todoroki, T. Togawa, M. Toia, A. Tojo, J. Tomasek, L. Tomasek, M. Torii, H. Towell, M. Towell, R. Towell, R. S. Tram, V-N. Tserruya, I. Tsuchimoto, Y. Vale, C. Valle, H. van Hecke, H. W. Vargyas, M. Vazquez-Zambrano, E. Veicht, A. Velkovska, J. Vertesi, R. Vinogradov, A. A. Virius, M. Vrba, V. Vznuzdaev, E. Wagner, M. Walker, D. Wang, X. R. Watanabe, D. Watanabe, K. Watanabe, Y. Watanabe, Y. S. Wei, F. Wei, R. Wessels, J. Whitaker, S. White, S. N. Winter, D. Wolin, S. Woody, C. L. Wright, R. M. Wysocki, M. Xia, B. Xie, W. Xue, L. Yalcin, S. Yamaguchi, Y. L. Yamaura, K. Yang, R. Yanovich, A. Yasin, Z. Ying, J. Yokkaichi, S. Yoon, I. You, Z. Young, G. R. Younus, I. Yushmanov, I. E. Zajc, W. A. Zaudtke, O. Zelenski, A. Zhang, C. Zhou, S. Zimanyi, J. Zolin, L. CA PHENIX Collaboration TI Measurement of K-S(0) and K*(0) in p plus p, d plus Au, and Cu plus Cu collisions at root s(NN)=200 GeV SO PHYSICAL REVIEW C LA English DT Article ID LARGE TRANSVERSE-MOMENTUM; QUARK-GLUON PLASMA; CENTRALITY DEPENDENCE; PBPB COLLISIONS; PHENIX; DETECTORS; MATTER; TEV; QCD AB The PHENIX experiment at the Relativistic Heavy Ion Collider has performed a systematic study of K-S(0) and K*(0) meson production at midrapidity in p + p, d + Au, and Cu + Cu collisions at root s(NN) = 200 GeV. The K-S(0) and K*(0) mesons are reconstructed via their K-S(0) -> pi(0)(-> gamma gamma) pi(0)(-> gamma gamma) and K*(0) -> K-+/-pi(-/+) decay modes, respectively. The measured transverse-momentum spectra are used to determine the nuclear modification factor of K-S(0) and K*(0) mesons in d + Au and Cu + Cu collisions at different centralities. In the d + Au collisions, the nuclear modification factor of K-S(0) and K*(0) mesons is almost constant as a function of transverse momentum and is consistent with unity, showing that cold-nuclear-matter effects do not play a significant role in the measured kinematic range. In Cu + Cu collisions, within the uncertainties no nuclear modification is registered in peripheral collisions. In central collisions, both mesons show suppression relative to the expectations from the p + p yield scaled by the number of binary nucleon-nucleon collisions in the Cu + Cu system. In the p(T) range 2-5 GeV/c, the strange mesons (K-S(0), K*(0)) similarly to the phi meson with hidden strangeness, showan intermediate suppression between the more suppressed light quark mesons (pi(0)) and the nonsuppressed baryons (p, (p) over bar). At higher transverse momentum, p(T) > 5 GeV/c, production of all particles is similarly suppressed by a factor of approximate to 2. C1 [Basye, A. T.; Daugherity, M. S.; Deaton, M. B.; Isenhower, D.; Isenhower, L.; Jones, T.; Jumper, D. S.; Miller, A. J.; Omiwade, O. O.; Pinson, R.; Thomas, D.; Towell, M.; Towell, R.; Towell, R. S.; Wright, R. M.] Abilene Christian Univ, Abilene, TX 79699 USA. [Grau, N.] Augustana Coll, Dept Phys, Sioux Falls, SD 57197 USA. [Garg, P.; Mishra, M.; Singh, B. K.; Singh, C. P.; Singh, V.; Tarafdar, S.] Banaras Hindu Univ, Dept Phys, Varanasi 221005, Uttar Pradesh, India. [Choudhury, R. K.; Dutta, D.; Mishra, D. K.; Mohanty, A. K.; Netrakanti, P. K.; Sett, P.; Shukla, P.] Bhabha Atom Res Ctr, Bombay 400085, Maharashtra, India. [Bathe, S.; Bryslawskyj, J.; Rowan, Z.] CUNY Bernard M Baruch Coll, New York, NY 10010 USA. [Bai, M.; Drees, K. A.; Makdisi, Y. I.; Zelenski, A.] Brookhaven Natl Lab, Collider Accelerator Dept, Upton, NY 11973 USA. [Aronson, S. H.; Azmoun, B.; Bazilevsky, A.; Belikov, S.; Buesching, H.; Bunce, G.; Chiu, M.; David, G.; Desmond, E. J.; Franz, A.; Haggerty, J. S.; Jia, J.; Johnson, B. M.; Kistenev, E.; Lynch, D.; Mannel, E.; Milov, A.; Mioduszewski, S.; Mitchell, J. T.; Morrison, D. P.; Nouicer, R.; O'Brien, E.; Pak, R.; Perepelitsa, D. V.; Pinkenburg, C.; Pisani, R. P.; Purschke, M. L.; Sakaguchi, T.; Sickles, A.; Sourikova, I. V.; Stoll, S. P.; Sukhanov, A.; Tannenbaum, M. J.; Vale, C.; White, S. N.; Woody, C. L.] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. [Barish, K. N.; Bathe, S.; Beaumier, M.; Black, D.; Chvala, O.; Dzhordzhadze, V.; Emam, W. S.; Eyser, K. O.; Hester, T.; Hollis, R. S.; Iordanova, A.; Kleinjan, D.; Kotchetkov, D.; Mendoza, M.; Morreale, A.; Rolnick, S. D.; Sedgwick, K.; Seto, R.; Yasin, Z.] Univ Calif Riverside, Riverside, CA 92521 USA. [Finger, M.; Finger, M., Jr.; Kubart, J.; Masek, L.; Mikes, P.; Slunecka, M.] Charles Univ Prague, CR-11636 Prague 1, Czech Republic. [Choi, J. B.; Kim, E. -J.] Chonbuk Natl Univ, Jeonju 561756, South Korea. [Li, X.; Zhou, S.] China Inst Atom Energy, Sci & Technol Nucl Data Lab, Beijing 102413, Peoples R China. [Akimoto, R.; Aramaki, Y.; Gunji, T.; Hamagaki, H.; Hayano, R.; Isobe, T.; Kajihara, F.; Kametani, S.; Kurihara, N.; Morino, Y.; Oda, S. X.; Ozawa, K.; Sano, S.; Takahara, A.; Yamaguchi, Y. L.] Univ Tokyo, Grad Sch Sci, Ctr Nucl Study, Bunkyo Ku, Tokyo 1130033, Japan. [Adare, A.; Beckman, S.; Bickley, A. A.; Ellinghaus, F.; Glenn, A.; Kinney, E.; Koblesky, T.; Levy, L. A. Linden; McGlinchey, D.; Nagle, J. L.; Koop, J. D. Orjuela; Rosen, C. A.; Seele, J.; Wysocki, M.] Univ Colorado, Boulder, CO 80309 USA. [Aidala, C.; Angerami, A.; Chi, C. Y.; Cole, B. A.; d'Enterria, D.; Engelmore, T.; Hanks, J.; Holzmann, W.; Jia, J.; Jin, J.; Kravitz, A.; Lai, Y. S.; Mannel, E.; Matathias, F.; Meredith, B.; Perepelitsa, D. V.; Vazquez-Zambrano, E.; Winter, D.; Zajc, W. A.] Columbia Univ, New York, NY 10027 USA. [Aidala, C.; Angerami, A.; Chi, C. Y.; Cole, B. A.; d'Enterria, D.; Engelmore, T.; Grau, N.; Hanks, J.; Holzmann, W.; Jin, J.; Kravitz, A.; Lai, Y. S.; Mannel, E.; Matathias, F.; Meredith, B.; Perepelitsa, D. V.; Vazquez-Zambrano, E.; Winter, D.; Zajc, W. A.] Nevis Labs, Irvington, NY 10533 USA. [Gallus, P.; Kral, A.; Liska, T.; Tomasek, M.; Virius, M.; Vrba, V.] Czech Tech Univ, Prague 16636 6, Czech Republic. [Baldisseri, A.; Borel, H.; Charvet, J. -L.; Gosset, J.; Pereira, H.; Silvestre, C.; Staley, F.] CEA Saclay, Dapnia, F-91191 Gif Sur Yvette, France. [Tarjan, P.; Vertesi, R.] Univ Debrecen, H-4010 Debrecen, Hungary. [Csanad, M.; Kiss, A.; Kofarago, M.; Nagy, M. 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[Dietzsch, O.; Donadelli, M.; Leite, M. A. L.; Lenzi, B.; Silva, C. L.; Takagui, E. M.] Univ Sao Paulo, Inst Fis, BR-05315970 Sao Paulo, Brazil. [Kim, E.; Kim, M.; Lee, T.; Park, S.; Tanida, K.; Yoon, I.] Seoul Natl Univ, Dept Phys & Astron, Seoul 151742, South Korea. [Ajitanand, N. N.; Alexander, J.; Chung, P.; Gu, Y.; Holzmann, W.; Issah, M.; Jia, J.; Lacey, R.; Mitrovski, M.; Mwai, A.; Reynolds, D.; Shevel, A.; Taranenko, A.; Wei, R.] SUNY Stony Brook, Dept Chem, Stony Brook, NY 11794 USA. [Apadula, N.; Atomssa, E. T.; Averbeck, R.; Bannier, B.; Bennett, R.; Boyle, K.; Butsyk, S.; Campbell, S.; Chen, C. -H.; Citron, Z.; Connors, M.; Dahms, T.; Dehmelt, K.; Deshpande, A.; Dion, A.; Drees, A.; Durham, J. M.; Egdemir, J.; Feege, N.; Frantz, J. E.; Gal, C.; Ge, H.; Gong, H.; Hanks, J.; Hemmick, T. K.; Jacak, B. V.; Kamin, J.; Khachatryan, V.; Kline, P.; Lee, S. 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[Chujo, T.; Esumi, S.; Ikeda, Y.; Inaba, M.; Kihara, K.; Konno, M.; Masui, H.; Miake, Y.; Miki, K.; Mizuno, S.; Nagata, Y.; Nakagomi, H.; Niida, T.; Oka, M.; Ozaki, H.; Sakai, S.; Shimomura, M.; Tanabe, R.; Todoroki, T.; Watanabe, K.] Univ Tsukuba, Inst Phys, Tsukuba, Ibaraki 305, Japan. [Belmont, R.; Chujo, T.; Danchev, I.; Greene, S. V.; Huang, S.; Issah, M.; Love, B.; Maguire, C. F.; Miller, T. E.; Mukhopadhyay, D.; Pal, D.; Roach, D.; Schaefer, B.; Valle, H.; Velkovska, J.] Vanderbilt Univ, Nashville, TN 37235 USA. [Kametani, S.; Kikuchi, J.; Sano, S.; Yamaguchi, Y. L.] Waseda Univ, Adv Res Inst Sci & Engn, Shinjuku Ku, Tokyo 1620044, Japan. [Citron, Z.; Dubey, A. K.; Fraenkel, Z.; Kozlov, A.; Makek, M.; Milov, A.; Naglis, M.; Ravinovich, I.; Sharma, D.; Tarafdar, S.; Tserruya, I.] Weizmann Inst Sci, IL-76100 Rehovot, Israel. [Csoergo, T.; Nagy, M. I.; Ster, A.; Vargyas, M.; Vertesi, R.; Zimanyi, J.] Hungarian Acad Sci, Wigner Res Ctr Phys, Inst Particle & Nucl Phys, Wigner RCP,RMKI, H-1525 Budapest, Hungary. [Bhom, J. H.; Bok, J. S.; Chang, B. S.; Choi, I. J.; Do, J. H.; Kang, J. H.; Kim, D. J.; Kim, H. -J.; Kwon, Y.; Lee, M. K.; Lim, S. H.; Moon, T.] Yonsei Univ, IPAP, Seoul 120749, South Korea. [Makek, M.] Univ Zagreb, Fac Sci, Dept Phys, HR-10002 Zagreb, Croatia. RP Morrison, DP (reprint author), Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. EM morrison@bnl.gov; jamie.nagle@colorado.edu RI Dahms, Torsten/A-8453-2015; En'yo, Hideto/B-2440-2015; Taketani, Atsushi/E-1803-2017; Hayano, Ryugo/F-7889-2012; HAMAGAKI, HIDEKI/G-4899-2014; Gu, Yi/B-6101-2016; Semenov, Vitaliy/E-9584-2017; Durum, Artur/C-3027-2014; Sen, Abhisek/J-1157-2016; Nattrass, Christine/J-6752-2016; Sorensen, Soren /K-1195-2016; Yokkaichi, Satoshi/C-6215-2017 OI Dahms, Torsten/0000-0003-4274-5476; Taketani, Atsushi/0000-0002-4776-2315; Hayano, Ryugo/0000-0002-1214-7806; Gu, Yi/0000-0003-4467-697X; Sen, Abhisek/0000-0003-1192-3938; Nattrass, Christine/0000-0002-8768-6468; Sorensen, Soren /0000-0002-5595-5643; FU Office of Nuclear Physics in the Office of Science of the Department of Energy; National Science Foundation; Abilene Christian University Research Council; Research Foundation of SUNY; Dean of the College of Arts and Sciences; Vanderbilt University (USA); Ministry of Education, Culture, Sports, Science, and Technology; Japan Society for the Promotion of Science (Japan); Conselho Nacional de Desenvolvimento Cientifico e Tecnologico and Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (Brazil); Natural Science Foundation of China (P.R. China); Ministry of Science, Education, and Sports (Croatia); Ministry of Education, Youth and Sports (Czech Republic); Centre National de la Recherche Scientifique; Commissariat a l'Energie Atomique; Institut National de Physique Nucleaire et de Physique des Particules (France); Bundesministerium fur Bildung und Forschung; Deutscher Akademischer Austausch Dienst; Alexander von Humboldt Stiftung (Germany); OTKA [NK 101 428]; Ch. Simonyi Fund (Hungary); Department of Atomic Energy and Department of Science and Technology (India); Israel Science Foundation (Israel); National Research Foundation of Korea of the Ministry of Science, ICT, and Future Planning (Korea); Physics Department, Lahore University of Management Sciences (Pakistan); Ministry of Education and Science, Russian Academy of Sciences, Federal Agency of Atomic Energy (Russia); VR; Wallenberg Foundation (Sweden); US Civilian Research and Development Foundation for the Independent States of the Former Soviet Union; Hungarian American Enterprise Scholarship Fund; US-Israel Binational Science Foundation FX We thank the staff of the Collider-Accelerator and Physics Departments at Brookhaven National Laboratory and the staff of the other PHENIX participating institutions for their vital contributions. We acknowledge support from the Office of Nuclear Physics in the Office of Science of the Department of Energy, the National Science Foundation, Abilene Christian University Research Council, Research Foundation of SUNY, and Dean of the College of Arts and Sciences, Vanderbilt University (USA); Ministry of Education, Culture, Sports, Science, and Technology and the Japan Society for the Promotion of Science (Japan); Conselho Nacional de Desenvolvimento Cientifico e Tecnologico and Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (Brazil); Natural Science Foundation of China (P.R. China), Ministry of Science, Education, and Sports (Croatia); Ministry of Education, Youth and Sports (Czech Republic); Centre National de la Recherche Scientifique, Commissariat a l'Energie Atomique, and Institut National de Physique Nucleaire et de Physique des Particules (France); Bundesministerium fur Bildung und Forschung, Deutscher Akademischer Austausch Dienst, and Alexander von Humboldt Stiftung (Germany); OTKA Grant No. NK 101 428 and the Ch. Simonyi Fund (Hungary); Department of Atomic Energy and Department of Science and Technology (India); Israel Science Foundation (Israel); National Research Foundation of Korea of the Ministry of Science, ICT, and Future Planning (Korea); Physics Department, Lahore University of Management Sciences (Pakistan); Ministry of Education and Science, Russian Academy of Sciences, Federal Agency of Atomic Energy (Russia); VR and Wallenberg Foundation (Sweden); the US Civilian Research and Development Foundation for the Independent States of the Former Soviet Union; the Hungarian American Enterprise Scholarship Fund; and the US-Israel Binational Science Foundation. NR 58 TC 4 Z9 4 U1 7 U2 29 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0556-2813 EI 1089-490X J9 PHYS REV C JI Phys. Rev. C PD NOV 7 PY 2014 VL 90 IS 5 AR 054905 DI 10.1103/PhysRevC.90.054905 PG 18 WC Physics, Nuclear SC Physics GA AT9NH UT WOS:000345253400003 ER PT J AU Kim, JB Weichman, ML Neumark, DM AF Kim, Jongjin B. Weichman, Marissa L. Neumark, Daniel M. TI Slow photoelectron velocity-map imaging spectroscopy of the Fe3O- and Co3O- anions SO JOURNAL OF CHEMICAL PHYSICS LA English DT Article ID DENSITY-FUNCTIONAL THEORY; IRON-OXIDE CLUSTERS; NATURAL-POPULATION ANALYSIS; TRANSITION-METAL OXIDES; DIOXIDE BOND-ENERGIES; GUIDED ION-BEAM; NEGATIVE-IONS; VIBRATIONAL SPECTROSCOPY; MAGNETIC-PROPERTIES; ELECTRONIC-STRUCTURE AB We report high-resolution photoelectron spectra of the transition metal suboxide clusters Fe3O- and Co3O-. The combination of slow electron velocity-map imaging and cryogenic cooling yields vibrationally well-resolved spectra, from which we obtain precise values of 1.4408(3) and 1.3951(4) eV for the electron affinities of Fe3O and Co3O. Several vibrational frequencies of the neutral ground state Fe3O and Co3O clusters are assigned for the first time, and a low-lying excited state of Fe3O is observed. The experimental results are compared with density functional electronic structure calculations and Franck-Condon spectral simulations, enabling identification of the structural isomer and electronic states. As has been found in photoelectron spectra of other trimetal oxo species, Fe3O0/- and Co3O0/- are assigned to a mu(2)-oxo isomer with planar C-2v symmetry. We identify the ground states of Fe3O- and Co3O- as (12)A(1) and B-9(2) states, respectively. From these states we observe photodetachment to the B-11(2) ground and (13)A(1) excited states of Fe3O, as well as to the (8)A(1) ground state of Co3O. (C) 2014 AIP Publishing LLC. C1 [Neumark, Daniel M.] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA. Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA. RP Neumark, DM (reprint author), Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA. EM dneumark@berkeley.edu RI Neumark, Daniel/B-9551-2009; OI Neumark, Daniel/0000-0002-3762-9473; Weichman, Marissa/0000-0002-2551-9146 FU Air Force Office of Scientific Research [FA9550-12-1-0160]; Defense University Research Instrumentation Program [FA9550-11-1-0330]; National Science Foundation FX This work is funded by the Air Force Office of Scientific Research under Grant No. FA9550-12-1-0160 and the Defense University Research Instrumentation Program under Grant No. FA9550-11-1-0330. M. L. W. thanks the National Science Foundation for a graduate research fellowship. We thank Nicholas J. Mayhall for a useful discussion of electronic structure methods for transition metal species. NR 82 TC 3 Z9 3 U1 1 U2 37 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0021-9606 EI 1089-7690 J9 J CHEM PHYS JI J. Chem. Phys. PD NOV 7 PY 2014 VL 141 IS 17 AR 174307 DI 10.1063/1.4900646 PG 11 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AT2RL UT WOS:000344782200022 PM 25381514 ER PT J AU Markutsya, S Lamm, MH AF Markutsya, Sergiy Lamm, Monica H. TI A coarse-graining approach for molecular simulation that retains the dynamics of the all-atom reference system by implementing hydrodynamic interactions SO JOURNAL OF CHEMICAL PHYSICS LA English DT Article ID BROWNIAN DYNAMICS; FORCE-FIELD; INTERACTION POTENTIALS; WATER MODELS; MOTION; ALGORITHM; SCALE; CRYSTALLINE; EXTENSION; RECEPTOR AB We report on a new approach for deriving coarse-grained intermolecular forces that retains the frictional contribution that is often discarded by conventional coarse-graining methods. The approach is tested for water and an aqueous glucose solution, and the results from the new implementation for coarse-grained molecular dynamics simulation show remarkable agreement with the dynamics obtained from reference all-atom simulations. The agreement between the structural properties observed in the coarse-grained and all-atom simulations is also preserved. We discuss how this approach may be applied broadly to any existing coarse-graining method where the coarse-grained models are rigorously derived from all-atom reference systems. (C) 2014 AIP Publishing LLC. C1 [Markutsya, Sergiy; Lamm, Monica H.] Iowa State Univ, Ames Lab, Ames, IA 50011 USA. [Lamm, Monica H.] Iowa State Univ, Dept Chem & Biol Engn, Ames, IA 50011 USA. RP Lamm, MH (reprint author), Iowa State Univ, Ames Lab, Ames, IA 50011 USA. EM mhlamm@iastate.edu FU (U.S.) Department of Energy (DOE) SciDAC program through the Office of Advanced Scientific Computing Research (ASCR) and Biological and Environmental Research (BER); US-DOE [DE-AC02-07CH11358] FX This research was sponsored by the (U.S.) Department of Energy (DOE) SciDAC program through the Office of Advanced Scientific Computing Research (ASCR) and Biological and Environmental Research (BER), and was performed at the Ames Laboratory, FWP AL-08-330-039. Ames Laboratory is managed by Iowa State University for the US-DOE under Contract No. DE-AC02-07CH11358. The authors gratefully acknowledge G. A. Voth for providing the multi-scale coarse-graining (MS-CG) software, J. C. Smith for providing the parameters for the CHARMM36 potential used in the all-atom simulations, and M. S. Gordon, R. D. Vigil, and B. H. Shanks for discussion. NR 70 TC 5 Z9 5 U1 1 U2 29 PU AMER INST PHYSICS PI MELVILLE PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA SN 0021-9606 EI 1089-7690 J9 J CHEM PHYS JI J. Chem. Phys. PD NOV 7 PY 2014 VL 141 IS 17 AR 174107 DI 10.1063/1.4898625 PG 10 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AT2RL UT WOS:000344782200010 PM 25381502 ER PT J AU Tulk, CA Machida, S Klug, DD Lu, H Guthrie, M Molaison, J AF Tulk, C. A. Machida, S. Klug, D. D. Lu, H. Guthrie, M. Molaison, J. TI The structure of CO2 hydrate between 0.7 and 1.0 GPa SO JOURNAL OF CHEMICAL PHYSICS LA English DT Article ID HIGH-PRESSURE; MOLECULAR-DYNAMICS; CARBON-DIOXIDE; METHANE; TEMPERATURE; DIFFRACTION; BEHAVIOR; SYSTEM; VI AB A deuterated sample of CO2 structure I (sI) clathrate hydrate (CO2 center dot 8.3 D2O) has been formed and neutron diffraction experiments up to 1.0 GPa at 240 K were performed. The sI CO2 hydrate transformed at 0.7 GPa into the high pressure phase that had been observed previously by Hirai et al. [J. Phys. Chem. 133, 124511 (2010)] and Bollengier et al. [Geochim. Cosmochim. Acta 119, 322 (2013)], but which had not been structurally identified. The current neutron diffraction data were successfully fitted to a filled ice structure with CO2 molecules filling the water channels. This CO2+ water system has also been investigated using classical molecular dynamics and density functional ab initio methods to provide additional characterization of the high pressure structure. Both models indicate the water network adapts a MH-III "like" filled ice structure with considerable disorder of the orientations of the CO2 molecule. Furthermore, the disorder appears to be a direct result of the level of proton disorder in the water network. In contrast to the conclusions of Bollengier et al., our neutron diffraction data show that the filled ice phase can be recovered to ambient pressure (0.1 MPa) at 96 K, and recrystallization to sI hydrate occurs upon subsequent heating to 150 K, possibly by first forming low density amorphous ice. Unlike other clathrate hydrate systems, which transform from the sI or sII structure to the hexagonal structure (sH) then to the filled ice structure, CO2 hydrate transforms directly from the sI form to the filled ice structure. (C) 2014 AIP Publishing LLC. C1 [Tulk, C. A.; Machida, S.; Molaison, J.] Oak Ridge Natl Lab, Neutron Scattering Sci Div, Oak Ridge, TN 37831 USA. [Machida, S.; Guthrie, M.] Carnegie Inst Sci, Geophys Lab, Washington, DC 20015 USA. [Klug, D. D.; Lu, H.] Natl Res Council Canada, Ottawa, ON K1A 0R6, Canada. RP Tulk, CA (reprint author), Oak Ridge Natl Lab, Neutron Scattering Sci Div, Oak Ridge, TN 37831 USA. RI Tulk, Chris/R-6088-2016 OI Tulk, Chris/0000-0003-3400-3878 FU EFree, an Energy Frontier Research Center - U.S. Department of Energy (DOE), Office of Science, Office of Basic Energy Science (BES) [DE-SC0001057]; Scientific User Facilities Division, Office of Basic Energy Sciences, (U.S.) Department of Energy (DOE) FX We would like to acknowledge important discussions with Serge Desgrenier of the University of Ottawa. This work was supported by EFree, an Energy Frontier Research Center Funded by the U.S. Department of Energy (DOE), Office of Science, Office of Basic Energy Science (BES) under award No. DE-SC0001057. The neutron diffraction experiments and analysis portion of the research conducted at ORNL's Spallation Neutron Source, was sponsored by the Scientific User Facilities Division, Office of Basic Energy Sciences, (U.S.) Department of Energy (DOE). NR 39 TC 3 Z9 3 U1 2 U2 40 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0021-9606 EI 1089-7690 J9 J CHEM PHYS JI J. Chem. Phys. PD NOV 7 PY 2014 VL 141 IS 17 AR 174503 DI 10.1063/1.4899265 PG 8 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AT2RL UT WOS:000344782200035 PM 25381527 ER PT J AU Ziemkiewicz, MP Bacellar, C Siefermann, KR Leone, SR Neumark, DM Gessner, O AF Ziemkiewicz, Michael P. Bacellar, Camila Siefermann, Katrin R. Leone, Stephen R. Neumark, Daniel M. Gessner, Oliver TI Femtosecond time-resolved XUV plus UV photoelectron imaging of pure helium nanodroplets SO JOURNAL OF CHEMICAL PHYSICS LA English DT Article ID ELECTRONICALLY EXCITED-STATES; LIQUID-HELIUM; SMALL CLUSTERS; HE DROPLETS; SPECTROSCOPY; MOLECULES; DYNAMICS; ATOMS; ION; PHOTOIONIZATION AB Liquid helium nanodroplets, consisting of on average 2 x 106 atoms, are examined using femtosecond time-resolved photoelectron imaging. The droplets are excited by an extreme ultraviolet light pulse centered at 23.7 eV photon energy, leading to states within a band that is associated with the 1s3p and 1s4p Rydberg levels of free helium atoms. The initially excited states and subsequent relaxation dynamics are probed by photoionizing transient species with a 3.2 eV pulse and using velocity map imaging to measure time-dependent photoelectron kinetic energy distributions. Significant differences are seen compared to previous studies with a lower energy (1.6 eV) probe pulse. Three distinct time-dependent signals are analyzed by global fitting. A broad intense signal, centered at an electron kinetic energy (eKE) of 2.3 eV, grows in faster than the experimental time resolution and decays in similar to 100 fs. This feature is attributed to the initially excited droplet state. A second broad transient feature, with eKE ranging from 0.5 to 4 eV, appears at a rate similar to the decay of the initially excited state and is attributed to rapid atomic reconfiguration resulting in Franck-Condon overlap with a broader range of cation geometries, possibly involving formation of a Rydberg-excited (He-n)* core within the droplet. An additional relaxation pathway leads to another short-lived feature with vertical binding energies greater than or similar to 2.4 eV, which is identified as a transient population within the lower-lying 1s2p Rydberg band. Ionization at 3.2 eV shows an enhanced contribution from electronically excited droplet states compared to ejected Rydberg atoms, which dominate at 1.6 eV. This is possibly the result of increased photoelectron generation from the bulk of the droplet by the more energetic probe photons. (C) 2014 AIP Publishing LLC. C1 [Ziemkiewicz, Michael P.; Bacellar, Camila; Siefermann, Katrin R.; Leone, Stephen R.; Neumark, Daniel M.; Gessner, Oliver] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Chem Sci, Ultrafast Xray Sci Lab, Berkeley, CA 94720 USA. [Ziemkiewicz, Michael P.; Bacellar, Camila; Leone, Stephen R.; Neumark, Daniel M.] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA. [Leone, Stephen R.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA. RP Ziemkiewicz, MP (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Chem Sci, Ultrafast Xray Sci Lab, Berkeley, CA 94720 USA. RI Neumark, Daniel/B-9551-2009 OI Neumark, Daniel/0000-0002-3762-9473 FU U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-AC02-05CH11231] FX This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences under Contract No. DE-AC02-05CH11231. The authors would also like to thank Ming-Fu Lin, Oleg Kornilov, Darcy Peterka, and Chia Wang for helpful discussions in the course of writing this paper. NR 48 TC 4 Z9 4 U1 4 U2 52 PU AMER INST PHYSICS PI MELVILLE PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA SN 0021-9606 EI 1089-7690 J9 J CHEM PHYS JI J. Chem. Phys. PD NOV 7 PY 2014 VL 141 IS 17 AR 174306 DI 10.1063/1.4900503 PG 9 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AT2RL UT WOS:000344782200021 PM 25381513 ER PT J AU Weber, AZ Kusoglu, A AF Weber, Adam Z. Kusoglu, Ahmet TI Unexplained transport resistances for low-loaded fuel-cell catalyst layers SO JOURNAL OF MATERIALS CHEMISTRY A LA English DT Article ID NAFION THIN-FILMS; OXYGEN-TRANSPORT; WATER-UPTAKE; SURFACE-AREA; PROTON CONDUCTIVITY; CONFINEMENT; PERFORMANCE; MEMBRANE; PEMFC; REDUCTION AB For next-generation polymer-electrolyte fuel cells, material solutions are being sought to decrease the cost of the cell components, and, in particular, the amount of catalyst, without sacrificing performance and lifetime. However, as recently shown, this cannot be achieved in practice due most likely to limitations caused by the ionomer thin-film surrounding the catalyst sites, where confinement and substrate interactions dominate and result in increased mass-transport limitations. Mitigation of this issue is paramount to the future commercial viability of polymer-electrolyte fuel cells. C1 [Weber, Adam Z.; Kusoglu, Ahmet] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Environm Energy Technol Div, Berkeley, CA 94720 USA. RP Weber, AZ (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Environm Energy Technol Div, Berkeley, CA 94720 USA. EM azweber@lbl.gov OI Kusoglu, Ahmet/0000-0002-2761-1050 NR 61 TC 20 Z9 20 U1 13 U2 76 PU ROYAL SOC CHEMISTRY PI CAMBRIDGE PA THOMAS GRAHAM HOUSE, SCIENCE PARK, MILTON RD, CAMBRIDGE CB4 0WF, CAMBS, ENGLAND SN 2050-7488 EI 2050-7496 J9 J MATER CHEM A JI J. Mater. Chem. A PD NOV 7 PY 2014 VL 2 IS 41 BP 17207 EP 17211 DI 10.1039/c4ta02952f PG 5 WC Chemistry, Physical; Energy & Fuels; Materials Science, Multidisciplinary SC Chemistry; Energy & Fuels; Materials Science GA AQ4JW UT WOS:000342763300001 ER PT J AU Simmonds, PJ Sun, M Laghumavarapu, RB Liang, BL Norman, AG Luo, JW Huffaker, DL AF Simmonds, Paul J. Sun, Meng Laghumavarapu, Ramesh Babu Liang, Baolai Norman, Andrew G. Luo, Jun-Wei Huffaker, Diana L. TI Improved quantum dot stacking for intermediate band solar cells using strain compensation SO NANOTECHNOLOGY LA English DT Article DE strain compensation; tensile strain; self-assembled quantum dots; InAs/AlAsSb; intermediate band solar cells ID INP; EFFICIENCY; ISLANDS AB We use thin tensile-strained AlAs layers to manage compressive strain in stacked layers of InAs/AlAsSb quantum dots (QDs). The AlAs layers allow us to reduce residual strain in the QD stacks, suppressing strain-related defects. AlAs layers 2.4 monolayers thick are sufficient to balance the strain in the structures studied, in agreement with theory. Strain balancing improves material quality and helps increase QD uniformity by preventing strain accumulation and ensuring that each layer of InAs experiences the same strain. Stacks of 30 layers of strain-balanced QDs exhibit carrier lifetimes as long as 9.7 ns. QD uniformity is further enhanced by vertical ABAB... ordering of the dots in successive layers. Strain compensated InAs/AlAsSb QD stacks show great promise for intermediate band solar cell applications. C1 [Simmonds, Paul J.; Liang, Baolai; Huffaker, Diana L.] Univ Calif Los Angeles, Calif NanoSyst Inst, Los Angeles, CA 90095 USA. [Sun, Meng; Laghumavarapu, Ramesh Babu; Huffaker, Diana L.] Univ Calif Los Angeles, Dept Elect Engn, Los Angeles, CA 90095 USA. [Norman, Andrew G.; Luo, Jun-Wei] Natl Renewable Energy Lab, Golden, CO 80401 USA. RP Simmonds, PJ (reprint author), Univ Calif Los Angeles, Calif NanoSyst Inst, Los Angeles, CA 90095 USA. EM p.j.simmonds.03@cantab.net RI Norman, Andrew/F-1859-2010; Simmonds, Paul/M-8377-2013 OI Norman, Andrew/0000-0001-6368-521X; Simmonds, Paul/0000-0001-5524-0835 FU Department of Energy [DE-EE0005325] FX This material is based upon work supported by the Department of Energy under Award Number DE-EE0005325. The authors at UCLA gratefully acknowledge the use of the Nano and Pico Characterization Lab in the California NanoSystems Institute, and the XRD resources made available by Mark Goorsky. We thank Seth Hubbard for useful discussions. NR 26 TC 7 Z9 7 U1 0 U2 30 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0957-4484 EI 1361-6528 J9 NANOTECHNOLOGY JI Nanotechnology PD NOV 7 PY 2014 VL 25 IS 44 AR 445402 DI 10.1088/0957-4484/25/44/445402 PG 7 WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied SC Science & Technology - Other Topics; Materials Science; Physics GA AS3ET UT WOS:000344160000011 PM 25319397 ER PT J AU Tselev, A Morozovska, AN Udod, A Eliseev, EA Kalinin, SV AF Tselev, Alexander Morozovska, Anna N. Udod, Alexei Eliseev, Eugene A. Kalinin, Sergei V. TI Self-consistent modeling of electrochemical strain microscopy of solid electrolytes SO NANOTECHNOLOGY LA English DT Article DE scanning probe microscopy; ionic processes; chemical strain; electrochemical strain microscopy; numerical simulations; frequency response ID LITHIUM-ION BATTERY; NANOSCALE; CONDUCTORS; RESISTANCE; DIFFUSION; TRANSPORT; CATHODE AB Electrochemical strain microscopy (ESM) employs a strong electromechanical coupling in solid ionic conductors to map ionic transport and electrochemical processes with nanometer-scale spatial resolution. To elucidate the mechanisms of the ESM image formation, we performed self-consistent numerical modeling of the electromechanical response in solid electrolytes under the probe tip in a linear, small-signal regime using the Boltzmann-Planck-Nernst-Einstein theory and Vegard's law while taking account of the electromigration and diffusion. The characteristic time scales involved in the formation of the ESM response were identified. It was found that the dynamics of the charge carriers in the tip-electrolyte system with blocking interfaces can be described as charging of the diffuse layer at the tip-electrolyte interface through the tip contact spreading resistance. At the high frequencies used in the detection regime, the distribution of the charge carriers under the tip is governed by evanescent concentration waves generated at the tip-electrolyte interface. The ion drift length in the electric field produced by the tip determines the ESM response at high frequencies, which follows a 1/f asymptotic law. The electronic conductivity, as well as the electron transport through the electrode-electrolyte interface, do not have a significant effect on the ESM signal in the detection regime. The results indicate, however, that for typical solid electrolytes at room temperature, the ESM response originates at and contains information about the very surface layer of a sample, and the properties of the one-unit-cell-thick surface layer may significantly contribute to the ESM response, implying a high surface sensitivity and a high lateral resolution of the technique. On the other hand, it follows that a rigorous analysis of the ESM signals requires techniques that account for the discrete C1 [Tselev, Alexander; Kalinin, Sergei V.] Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA. [Morozovska, Anna N.] Natl Acad Sci Ukraine, Inst Phys, UA-03028 Kiev, Ukraine. [Udod, Alexei] Taras Shevchenko Kiev Natl Univ, Radiophys Fac, UA-03022 Kiev, Ukraine. [Eliseev, Eugene A.] Natl Acad Sci Ukraine, Inst Problems Mat Sci, UA-03142 Kiev, Ukraine. RP Tselev, A (reprint author), Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA. EM tseleva@ornl.gov; morozo@i.com.ua RI Tselev, Alexander/L-8579-2015; Kalinin, Sergei/I-9096-2012 OI Tselev, Alexander/0000-0002-0098-6696; Kalinin, Sergei/0000-0001-5354-6152 FU Scientific User Facilities Division, Office of Basic Energy Sciences, US Department of Energy FX A portion of this research (AT, SVK) was conducted at the Center for Nanophase Materials Sciences, which is sponsored at Oak Ridge National Laboratory by the Scientific User Facilities Division, Office of Basic Energy Sciences, US Department of Energy. NR 36 TC 6 Z9 6 U1 5 U2 44 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0957-4484 EI 1361-6528 J9 NANOTECHNOLOGY JI Nanotechnology PD NOV 7 PY 2014 VL 25 IS 44 AR 445701 DI 10.1088/0957-4484/25/44/445701 PG 11 WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied SC Science & Technology - Other Topics; Materials Science; Physics GA AS3ET UT WOS:000344160000018 PM 25302673 ER PT J AU Xu, YT Ke, X Yu, CC Liu, SF Zhao, J Cui, GF Higgins, D Chen, ZW Li, Q Wu, G AF Xu, Yantong Ke, Xi Yu, Changchun Liu, Shaofang Zhao, Jie Cui, Guofeng Higgins, Drew Chen, Zhongwei Li, Qing Wu, Gang TI A strategy for fabricating nanoporous gold films through chemical dealloying of electrochemically deposited Au-Sn alloys SO NANOTECHNOLOGY LA English DT Article DE nanoporous gold; electrodeposition; chemical dealloying ID RAMAN-SPECTROSCOPY; LOW-TEMPERATURE; SURFACE-AREA; NANOWIRES; MICROSTRUCTURE; ELECTRODES; MONOLAYERS; EVOLUTION; NANORODS; CO AB We report a novel strategy for the fabrication of nanoporous gold (NPG) films. The fabrication process involves the electrodeposition of a gold-tin alloy, followed by subsequent chemical dealloying of tin. Scanning electron microscopy (SEM) images show a bicontinuous nanoporous structure formed on the substrates after chemical dealloying. Energy dispersive x-ray (EDX) analysis indicates that there are no impurities in the Au-Sn alloy film with an average composition of 58 at. % Au and 42 at. % Sn. After dealloying, only gold remains in the NPG film indicating the effectiveness of this technique. X-ray diffraction (XRD) results reveal that the as-prepared Au-Sn alloy film is composed of two phases (Au5Sn and AuSn), while the NPG film is composed of a single phase (Au). We demonstrate that this approach enables the fabrication of NPG films, either freestanding or supported on various conductive substrates such as copper foil, stainless steel sheet and nickel foam. The resulting NPG electrode exhibits enhanced electrocatalytic activity toward both H2O2 reduction and methanol oxidation compared to the polished Au disc electrode. Our strategy provides a general method to fabricate high quality NPG films on conductive substrates, which will broaden the application potential of NPG or NPG-based materials in various fields such as catalysis, optics and sensor technology. C1 [Xu, Yantong; Ke, Xi; Liu, Shaofang; Cui, Guofeng] Sun Yat Sen Univ, Sch Chem & Chem Engn, Elect Packaging Electrochem Lab, Guangzhou 510275, Guangdong, Peoples R China. [Yu, Changchun; Zhao, Jie] S China Univ Technol, Sch Mech & Automot Engn, Guangzhou 510640, Peoples R China. [Higgins, Drew; Li, Qing] Los Alamos Natl Lab, Mat Phys & Applicat Div, Los Alamos, NM 87545 USA. [Higgins, Drew; Chen, Zhongwei] Univ Waterloo, Waterloo Inst Sustainable Energy, Waterloo Inst Nanotechnol, Dept Chem Engn, Waterloo, ON N2L 3G1, Canada. [Wu, Gang] SUNY Buffalo, Dept Chem & Biol Engn, Buffalo, NY 14260 USA. RP Xu, YT (reprint author), Sun Yat Sen Univ, Sch Chem & Chem Engn, Elect Packaging Electrochem Lab, Guangzhou 510275, Guangdong, Peoples R China. EM xikeciac@gmail.com; cuigf@mail.sysu.edu.cn RI Wu, Gang/E-8536-2010; Ke, Xi/P-8335-2014; Li, Qing/G-4502-2011; chen, zhongwei/A-5605-2015 OI Wu, Gang/0000-0003-4956-5208; Ke, Xi/0000-0002-0737-4174; Li, Qing/0000-0003-4807-030X; FU National Natural Science Foundation of China [51271205, 50801070]; Guangzhou Pearl Technology the Nova Special Project [2012J2200058]; Excellent Young College Teachers Development Program in Guangdong Province [Yq2013006]; Research and Application of Key Technologies Oriented the Industrial Development [90035-3283309, 90035-3283321]; Science and Technology Plan Project of Guangzhou city [2013Y2-00102]; Science and Technology Plan Project of Huizhou city [2012B050013012]; DaYa Gulf district of Huizhou city [20110108, 20120212]; China Postdoctoral Science Foundation [2014M562234] FX G F Cui gratefully acknowledges the financial support by National Natural Science Foundation of China (51271205, 50801070), Guangzhou Pearl Technology the Nova Special Project (2012J2200058), Excellent Young College Teachers Development Program in Guangdong Province (Yq2013006), Research and Application of Key Technologies Oriented the Industrial Development (90035-3283309, 90035-3283321), Science and Technology Plan Projects of Guangzhou city (2013Y2-00102), Huizhou city (2012B050013012) and DaYa Gulf district of Huizhou city (20110108, 20120212). Dr X Ke acknowledges the support from China Postdoctoral Science Foundation (2014M562234). NR 36 TC 4 Z9 4 U1 15 U2 124 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0957-4484 EI 1361-6528 J9 NANOTECHNOLOGY JI Nanotechnology PD NOV 7 PY 2014 VL 25 IS 44 AR 445602 DI 10.1088/0957-4484/25/44/445602 PG 7 WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied SC Science & Technology - Other Topics; Materials Science; Physics GA AS3ET UT WOS:000344160000016 PM 25325248 ER PT J AU Woyke, T Rubin, EM AF Woyke, Tanja Rubin, Edward M. TI Searching for new branches on the tree of life SO SCIENCE LA English DT Editorial Material ID LINEAGES; HYDROGEN C1 [Woyke, Tanja] US DOE, Joint Genome Inst, Walnut Creek, CA 94598 USA. Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. RP Woyke, T (reprint author), US DOE, Joint Genome Inst, Walnut Creek, CA 94598 USA. EM emrubin@lbl.gov NR 15 TC 5 Z9 5 U1 4 U2 43 PU AMER ASSOC ADVANCEMENT SCIENCE PI WASHINGTON PA 1200 NEW YORK AVE, NW, WASHINGTON, DC 20005 USA SN 0036-8075 EI 1095-9203 J9 SCIENCE JI Science PD NOV 7 PY 2014 VL 346 IS 6210 BP 698 EP 699 DI 10.1126/science.1258871 PG 2 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AT1JT UT WOS:000344690100020 PM 25378606 ER PT J AU Samanta, A Tuckerman, ME Yu, TQ E, WN AF Samanta, Amit Tuckerman, Mark E. Yu, Tang-Qing E, Weinan TI Microscopic mechanisms of equilibrium melting of a solid SO SCIENCE LA English DT Article ID CRYSTAL INSTABILITY; COLLOIDAL CRYSTALS; STABILITY LIMIT; GERM-FORMATION; STRING METHOD; NUCLEATION; ENERGY; TEMPERATURE; LINDEMANN; METALS AB The melting of a solid, like other first-order phase transitions, exhibits an intrinsic time-scale disparity: The time spent by the system in metastable states is orders of magnitude longer than the transition times between the states. Using rare-event sampling techniques, we find that melting of representative solids-here, copper and aluminum-occurs via multiple, competing pathways involving the formation and migration of point defects or dislocations. Each path is characterized by multiple barrier-crossing events arising from multiple metastable states within the solid basin. At temperatures approaching superheating, melting becomes a single barrier-crossing process, and at the limit of superheating, the melting mechanism is driven by a vibrational instability. Our findings reveal the importance of nonlocal behavior, suggesting a revision of the perspective of classical nucleation theory. C1 [Samanta, Amit] Lawrence Livermore Natl Lab, Condensed Matter & Mat Div, Livermore, CA 94550 USA. [Samanta, Amit; E, Weinan] Princeton Univ, Program Appl & Computat Math, Princeton, NJ 08544 USA. [Tuckerman, Mark E.] NYU, Dept Chem, New York, NY 10003 USA. [Tuckerman, Mark E.; Yu, Tang-Qing] NYU, Courant Inst Math Sci, New York, NY 10012 USA. [Tuckerman, Mark E.] NYU East China Normal Univ Ctr Computat Chem, NYU Shanghai, Shanghai 200062, Peoples R China. [E, Weinan] Peking Univ, Beijing Int Ctr Math Res, Beijing 100871, Peoples R China. [E, Weinan] Peking Univ, Sch Math Sci, Beijing 100871, Peoples R China. [E, Weinan] Princeton Univ, Dept Math, Princeton, NJ 08544 USA. RP Samanta, A (reprint author), Lawrence Livermore Natl Lab, Condensed Matter & Mat Div, Livermore, CA 94550 USA. EM asamanta@math.princeton.edu; mark.tuckerman@nyu.edu; weinan@math.princeton.edu RI Yu, Tang-Qing/C-5437-2011 FU U.S. Department of Energy (DOE) [DE-SC0009248]; National Natural Science Foundation of China [9130005]; DOE by Lawrence Livermore National Laboratory [DE-AC52-07NA27344]; NSF [CHE-1301314] FX Work by W. E and A. S. at Princeton was supported by the U.S. Department of Energy (DOE) (grant DE-SC0009248) and in Beijing by the National Natural Science Foundation of China (9130005). This work was partially performed under the auspices of DOE by Lawrence Livermore National Laboratory under contract DE-AC52-07NA27344. Work by M. E. T. was supported by NSF grant CHE-1301314. NR 29 TC 22 Z9 22 U1 9 U2 104 PU AMER ASSOC ADVANCEMENT SCIENCE PI WASHINGTON PA 1200 NEW YORK AVE, NW, WASHINGTON, DC 20005 USA SN 0036-8075 EI 1095-9203 J9 SCIENCE JI Science PD NOV 7 PY 2014 VL 346 IS 6210 BP 729 EP 732 DI 10.1126/science.1253810 PG 4 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AT1JT UT WOS:000344690100035 PM 25378619 ER PT J AU Zemcov, M Smidt, J Arai, T Bock, J Cooray, A Gong, Y Kim, MG Korngut, P Lam, A Lee, DH Matsumoto, T Matsuura, S Nam, UW Roudier, G Tsumura, K Wada, T AF Zemcov, Michael Smidt, Joseph Arai, Toshiaki Bock, James Cooray, Asantha Gong, Yan Kim, Min Gyu Korngut, Phillip Lam, Anson Lee, Dae Hee Matsumoto, Toshio Matsuura, Shuji Nam, Uk Won Roudier, Gael Tsumura, Kohji Wada, Takehiko TI On the origin of near-infrared extragalactic background light anisotropy SO SCIENCE LA English DT Article ID EXPERIMENT CIBER; POPULATION-III; FLUCTUATIONS; SKY; SPECTRUM; STARS; 2MASS AB Extragalactic background light (EBL) anisotropy traces variations in the total production of photons over cosmic history and may contain faint, extended components missed in galaxy point-source surveys. Infrared EBL fluctuations have been attributed to primordial galaxies and black holes at the epoch of reionization (EOR) or, alternately, intrahalo light (IHL) from stars tidally stripped from their parent galaxies at low redshift. We report new EBL anisotropy measurements from a specialized sounding rocket experiment at 1.1 and 1.6 micrometers. The observed fluctuations exceed the amplitude from known galaxy populations, are inconsistent with EOR galaxies and black holes, and are largely explained by IHL emission. The measured fluctuations are associated with an EBL intensity that is comparable to the background from known galaxies measured through number counts and therefore a substantial contribution to the energy contained in photons in the cosmos. C1 [Zemcov, Michael; Bock, James; Korngut, Phillip; Lam, Anson] CALTECH, Dept Phys Math & Astron, Pasadena, CA 91125 USA. [Zemcov, Michael; Bock, James; Korngut, Phillip; Roudier, Gael] NASA, JPL, Pasadena, CA 91109 USA. [Smidt, Joseph] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA. [Smidt, Joseph; Cooray, Asantha; Gong, Yan] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA. [Arai, Toshiaki; Matsumoto, Toshio; Matsuura, Shuji; Wada, Takehiko] Japan Aerosp Explorat Agcy JAXA, ISAS, Dept Space Astron & Astrophys, Sagamihara, Kanagawa 2525210, Japan. [Arai, Toshiaki] Univ Tokyo, Grad Sch Sci, Dept Phys, Tokyo 1130033, Japan. [Kim, Min Gyu] Seoul Natl Univ, Dept Phys & Astron, Seoul 151742, South Korea. [Lam, Anson] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA. [Lee, Dae Hee; Nam, Uk Won] Korea Astron & Space Sci Inst KASI, Taejon 305348, South Korea. [Matsumoto, Toshio] Acad Sinica, Inst Astron & Astrophys, Taipei 10617, Taiwan. [Tsumura, Kohji] Tohoku Univ, Frontier Res Inst Interdisciplinary Sci, Sendai, Miyagi 9808578, Japan. RP Bock, J (reprint author), CALTECH, Dept Phys Math & Astron, Pasadena, CA 91125 USA. EM jjb@astro.caltech.edu RI Matsuura, Shuji/B-5658-2016 OI Matsuura, Shuji/0000-0002-5698-9634 FU NASA APRA [NNX07AI54G, NNG05WC18G, NNX07AG43G, NNX07AJ24G, NNX10AE12G]; Jet Propulsion Laboratory's Director's Research and Development Fund; KAKENHI from Japan Society for the Promotion of Science (JSPS) [20.34, 18204018, 19540250, 21340047, 21111004]; Ministry of Education, Culture, Sports, Science and Technology (MEXT); Pioneer Project from Korea Astronomy and Space Science Institute (KASI); NASA Postdoctoral Program; NSF CAREER [AST-0645427]; NSF [AST-1313319]; JSPS Research Fellowship for Young Scientists; National Aeronautics and Space Administration; National Science Foundation FX Our thanks to O. Dore, J. Filippini, and K. Ganga for useful conversations and comments throughout the course of this work and K. Helgason for kindly providing models of the statistics of the near-infrared CIB. The authors acknowledge the excellent support from the NASA sounding rockets program that was essential in developing, testing, qualifying, launching, and recovering our payloads. The CIBER auto-and cross-power spectra are available for public download at http://ciber.caltech.edu/zemcovetal. This work was supported by NASA APRA research grants NNX07AI54G, NNG05WC18G, NNX07AG43G, NNX07AJ24G, and NNX10AE12G. Initial support was provided by an award to J. B. from the Jet Propulsion Laboratory's Director's Research and Development Fund. Japanese participation in CIBER was supported by KAKENHI (20.34, 18204018, 19540250, 21340047, and 21111004) from Japan Society for the Promotion of Science (JSPS) and the Ministry of Education, Culture, Sports, Science and Technology (MEXT). Korean participation in CIBER was supported by the Pioneer Project from Korea Astronomy and Space Science Institute (KASI). M.Z. and P. K. acknowledge support from NASA Postdoctoral Program fellowships, A. C. acknowledges support from an NSF CAREER award AST-0645427 and NSF AST-1313319, and K. T. acknowledges support from the JSPS Research Fellowship for Young Scientists. This publication makes use of data products from the Two Micron All Sky Survey (2MASS), which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. This work made use of images and/or data products provided by the National Optical Astronomy Observatory (NOAO) Deep Wide-Field Survey (NDWFS), which is supported by NOAO, operated by AURA, Inc., under a cooperative agreement with the National Science Foundation. NR 28 TC 24 Z9 24 U1 2 U2 19 PU AMER ASSOC ADVANCEMENT SCIENCE PI WASHINGTON PA 1200 NEW YORK AVE, NW, WASHINGTON, DC 20005 USA SN 0036-8075 EI 1095-9203 J9 SCIENCE JI Science PD NOV 7 PY 2014 VL 346 IS 6210 BP 732 EP 735 DI 10.1126/science.1258168 PG 4 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AT1JT UT WOS:000344690100036 PM 25378620 ER PT J AU Moses, WW Peng, Q AF Moses, W. W. Peng, Q. TI Artifacts in digital coincidence timing SO PHYSICS IN MEDICINE AND BIOLOGY LA English DT Article DE timing resolution; artifacts; digital timing methods; timing optimization ID TIME-OF-FLIGHT; PET AB Digital methods are becoming increasingly popular for measuring time differences, and are the de facto standard in PET cameras. These methods usually include a master system clock and a (digital) arrival time estimate for each detector that is obtained by comparing the detector output signal to some reference portion of this clock (such as the rising edge). Time differences between detector signals are then obtained by subtracting the digitized estimates from a detector pair. A number of different methods can be used to generate the digitized arrival time of the detector output, such as sending a discriminator output into a time to digital converter (TDC) or digitizing the waveform and applying a more sophisticated algorithm to extract a timing estimator. All measurement methods are subject to error, and one generally wants to minimize these errors and so optimize the timing resolution. A common method for optimizing timing methods is to measure the coincidence timing resolution between two timing signals whose time difference should be constant (such as detecting gammas from positron annihilation) and selecting the method that minimizes the width of the distribution (i.e. the timing resolution). Unfortunately, a common form of error (a nonlinear transfer function) leads to artifacts that artificially narrow this resolution, which can lead to erroneous selection of the 'optimal' method. The purpose of this note is to demonstrate the origin of this artifact and suggest that caution should be used when optimizing time digitization systems solely on timing resolution minimization. C1 [Moses, W. W.; Peng, Q.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. RP Moses, WW (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. EM wwmoses@lbl.gov FU Office of Science, Office of Biological and Environmental Research, Medical Science Division of the U.S. Department of Energy [DE-AC02-05CH11231]; National Institutes of Health, National Institute of Biomedical Imaging and Bioengineering [R01-EB006085] FX We would like to thank Dr William Ashmanskas of the University of Pennsylvania for the discussions that stimulated this work. This work is supported in part by the Director, Office of Science, Office of Biological and Environmental Research, Medical Science Division of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231, and in part by the National Institutes of Health, National Institute of Biomedical Imaging and Bioengineering under grant No. R01-EB006085. NR 10 TC 0 Z9 0 U1 0 U2 10 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0031-9155 EI 1361-6560 J9 PHYS MED BIOL JI Phys. Med. Biol. PD NOV 7 PY 2014 VL 59 IS 21 BP N181 EP N185 DI 10.1088/0031-9155/59/21/N181 PG 5 WC Engineering, Biomedical; Radiology, Nuclear Medicine & Medical Imaging SC Engineering; Radiology, Nuclear Medicine & Medical Imaging GA AQ8QD UT WOS:000343092900001 PM 25321885 ER PT J AU van Veelen, M Luo, SS Simon, B AF van Veelen, Matthijs Luo, Shishi Simon, Burton TI A simple model of group selection that cannot be analyzed with inclusive fitness SO JOURNAL OF THEORETICAL BIOLOGY LA English DT Article DE Kin selection; Equivalence; Social evolution; Cooperation; Multi-level selection ID KIN SELECTION; MULTILEVEL SELECTION; SOCIAL SEMANTICS; CONNECTED WORLD; EVOLUTION; ALTRUISM; COOPERATION; RULE; EQUIVALENT AB A widespread claim in evolutionary theory is that every group selection model can be recast in terms of inclusive fitness. Although there are interesting classes of group selection models for which this is possible, we show that it is not true in general. With a simple set of group selection models, we show two distinct limitations that prevent recasting in terms of inclusive fitness. The first is a limitation across models. We show that if inclusive fitness is to always give the correct prediction, the definition of relatedness needs to change, continuously, along with changes in the parameters of the model. This results in infinitely many different definitions of relatedness - one for every parameter value - which strips relatedness of its meaning. The second limitation is across time. We show that one can find the trajectory for the group selection model by solving a partial differential equation, and that it is mathematically impossible to do this using inclusive fitness. (C) 2014 Elsevier Ltd. All rights reserved. C1 [van Veelen, Matthijs] Univ Amsterdam, Dept Econ & Business, NL-1018 WB Amsterdam, Netherlands. [van Veelen, Matthijs] Harvard Univ, Program Evolutionary Dynam, Cambridge, MA 02138 USA. [Luo, Shishi] Los Alamos Natl Lab, Theoret Biol & Biophys T6, Los Alamos, NM 87545 USA. [Luo, Shishi] Los Alamos Natl Lab, Ctr Nonlinear Studies, Los Alamos, NM 87545 USA. [Simon, Burton] Univ Colorado, Dept Math & Stat Sci, Denver, CO 80202 USA. RP van Veelen, M (reprint author), Univ Amsterdam, Dept Econ & Business, Roeters Str 11, NL-1018 WB Amsterdam, Netherlands. EM c.m.vanveelen@uva.nl; shishi@lanl.gov; Burt.Simon@ucdenver.edu RI van Veelen, Matthijs/G-5365-2014 OI van Veelen, Matthijs/0000-0002-8290-9212 FU Duke Stern Fellowship; US Department of Energy through the LANL/LDRD Program FX S.L. was supported by the Duke Stern Fellowship and the US Department of Energy through the LANL/LDRD Program. NR 43 TC 8 Z9 8 U1 3 U2 51 PU ACADEMIC PRESS LTD- ELSEVIER SCIENCE LTD PI LONDON PA 24-28 OVAL RD, LONDON NW1 7DX, ENGLAND SN 0022-5193 EI 1095-8541 J9 J THEOR BIOL JI J. Theor. Biol. PD NOV 7 PY 2014 VL 360 BP 279 EP 289 DI 10.1016/j.jtbi.2014.07.004 PG 11 WC Biology; Mathematical & Computational Biology SC Life Sciences & Biomedicine - Other Topics; Mathematical & Computational Biology GA AP1BE UT WOS:000341800600029 PM 25034338 ER PT J AU Kennedy, BK Berger, SL Brunet, A Campisi, J Cuervo, AM Epel, ES Franceschi, C Lithgow, GJ Morimoto, RI Pessin, JE Rando, TA Richardson, A Schadt, EE Wyss-Coray, T Sierra, F AF Kennedy, Brian K. Berger, Shelley L. Brunet, Anne Campisi, Judith Cuervo, Ana Maria Epel, Elissa S. Franceschi, Claudio Lithgow, Gordon J. Morimoto, Richard I. Pessin, Jeffrey E. Rando, Thomas A. Richardson, Arlan Schadt, Eric E. Wyss-Coray, Tony Sierra, Felipe TI Geroscience: Linking Aging to Chronic Disease SO CELL LA English DT Editorial Material ID LIFE-SPAN; LONGEVITY; CELLS AB Mammalian aging can be delayed with genetic, dietary, and pharmacologic approaches. Given that the elderly population is dramatically increasing and that aging is the greatest risk factor for a majority of chronic diseases driving both morbidity and mortality, it is critical to expand geroscience research directed at extending human healthspan. C1 [Kennedy, Brian K.; Campisi, Judith; Lithgow, Gordon J.] Buck Inst Res Aging, Novato, CA USA. [Berger, Shelley L.] Univ Penn, Perelman Sch Med, Penn Epigenet Program, Philadelphia, PA 19104 USA. [Berger, Shelley L.] Univ Penn, Perelman Sch Med, Dept Cell & Dev Biol, Philadelphia, PA 19104 USA. [Berger, Shelley L.] Univ Penn, Perelman Sch Med, Dept Genet, Philadelphia, PA 19104 USA. [Berger, Shelley L.] Univ Penn, Perelman Sch Med, Dept Biol, Philadelphia, PA 19104 USA. [Brunet, Anne] Stanford Univ, Dept Genet, Stanford, CA 94305 USA. [Brunet, Anne; Rando, Thomas A.] Stanford Univ, Glenn Ctr Biol Aging, Stanford, CA 94305 USA. [Campisi, Judith] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Life Sci, Berkeley, CA 94720 USA. [Cuervo, Ana Maria] Albert Einstein Coll Med, Dept Dev & Mol Biol, Bronx, NY 10461 USA. [Cuervo, Ana Maria] Albert Einstein Coll Med, Inst Aging Studies, Bronx, NY 10461 USA. [Epel, Elissa S.] Univ Calif San Francisco, Sch Med, Dept Psychiat, San Francisco, CA 94143 USA. [Franceschi, Claudio] Bellaria Hosp, IRCCS Inst Neurol Sci Bologna, Bologna, Italy. [Franceschi, Claudio] Univ Bologna, CIG, Interdept Ctr L Galvani Integrated Studies Bioinf, Bologna 3, Italy. [Franceschi, Claudio] Univ Bologna, Dept Expt Diagnost & Specialty Med, DIMES, Bologna 3, Italy. [Morimoto, Richard I.] Northwestern Univ, Rice Inst Biomed Res, Dept Biochem Mol Biol & Cell Biol, Evanston, IL 60208 USA. [Pessin, Jeffrey E.] Albert Einstein Coll Med, Dept Med & Mol Pharmacol, Bronx, NY 10461 USA. [Rando, Thomas A.; Wyss-Coray, Tony] Stanford Univ, Sch Med, Dept Neurol & Neurol Sci, Stanford, CA 94305 USA. [Rando, Thomas A.; Wyss-Coray, Tony] Vet Adm Palo Alto Hlth Care Syst, Ctr Tissue Regenerat Repair & Restorat, Palo Alto, CA 94304 USA. [Richardson, Arlan] Univ Oklahoma, Hlth Sci Ctr, Oklahoma City, OK 73104 USA. [Richardson, Arlan] Oklahoma City VA Med Ctr, Oklahoma City, OK 73104 USA. [Schadt, Eric E.] Icahn Sch Med Mt Sinai, Dept Genet & Genom Sci, New York, NY 10029 USA. [Schadt, Eric E.] Icahn Sch Med Mt Sinai, Icahn Inst Genom & Multiscale Biol, New York, NY 10029 USA. [Sierra, Felipe] NIA, Div Aging Biol, Bethesda, MD 20892 USA. RP Kennedy, BK (reprint author), Buck Inst Res Aging, Novato, CA USA. EM bkennedy@buckinstitute.org FU NIA NIH HHS [P01 AG031782, P01 AG036695, R01 AG024287, R01 AG033373, R01 AG043080] NR 14 TC 97 Z9 98 U1 3 U2 21 PU CELL PRESS PI CAMBRIDGE PA 600 TECHNOLOGY SQUARE, 5TH FLOOR, CAMBRIDGE, MA 02139 USA SN 0092-8674 EI 1097-4172 J9 CELL JI Cell PD NOV 6 PY 2014 VL 159 IS 4 BP 708 EP 712 DI 10.1016/j.cell.2014.10.039 PG 5 WC Biochemistry & Molecular Biology; Cell Biology SC Biochemistry & Molecular Biology; Cell Biology GA AS8TY UT WOS:000344522000002 PM 25417146 ER PT J AU Rotavera, B Zador, J Welz, O Sheps, L Scheer, AM Savee, JD Ali, MA Lee, TS Simmons, BA Osborn, DL Violi, A Taatjes, CA AF Rotavera, Brandon Zador, Judit Welz, Oliver Sheps, Leonid Scheer, Adam M. Savee, John D. Ali, Moharnad Akbar Lee, Taek Soon Simmons, Blake A. Osborn, David L. Violi, Angela Taatjes, Craig A. TI Photoionization Mass Spectrometric Measurements of Initial Reaction Pathways in Low-Temperature Oxidation of 2,5-Dimethylhexane SO JOURNAL OF PHYSICAL CHEMISTRY A LA English DT Article ID GAS-PHASE OXIDATION; PRESSURE RATE RULES; COMBUSTION CHEMISTRY; ELEMENTARY REACTIONS; CHEMICAL-DYNAMICS; BIOFUELS PATHWAYS; RATE CONSTANTS; KINETICS; HYDROCARBONS; RADICALS AB Product formation from R + O-2 reactions relevant to low-temperature autoignition chemistry was studied for 2,5-dimethylhexane, a symmetrically branched octane isomer, at 550 and 650 K using Cl-atom initiated oxidation and multiplexed photoionization mass spectrometry (MPIMS). Interpretation of time- and photon-energy-resolved mass spectra led to three specific results important to characterizing the initial oxidation steps: (1) quantified isomer-resolved branching ratios for HO2+ alkene channels; (2) 2,2,5,5-tetramethyltetrahydrofuran is formed in substantial yield from addition of O2 to tertiary 2,5-dimethylhex-2-yl followed by isomerization of the resulting ROO adduct to tertiary hydroperoxyalkyl (QOOH) and exhibits a positive dependence on temperature over the range covered leading to a higher flux relative to aggregate cyclic ether yield. The higher relative flux is explained by a 1,5-hydrogen atom shift reaction that converts the initial primary alkyl radical (2,5-dimethylhex-1-yl) to the tertiary alkyl radical 2,5-dimethylhex-2-yl, providing an additional source of tertiary alkyl radicals. Quantum-chemical and master-equation calculations of the unimolecular decomposition of the primary alkyl radical reveal that isomerization to the tertiary alkyl radical is the most favorable pathway, and is favored over O2-addition at 650 K under the conditions herein. The isomerization pathway to tertiary alkyl radicals therefore contributes an additional mechanism to 2,2,5,5-tetramethyltetrahydrofuran formation; (3) carbonyl species (acetone, propanal, and methylpropanal) consistent with beta-scission of QOOH radicals were formed in significant yield, indicating unimolecular QOOH decomposition into carbonyl + alkene + OH. C1 [Rotavera, Brandon; Zador, Judit; Welz, Oliver; Sheps, Leonid; Scheer, Adam M.; Savee, John D.; Osborn, David L.; Taatjes, Craig A.] Sandia Natl Labs, Combust Res Facil, Combust Chem Dept, Livermore, CA 94550 USA. [Ali, Moharnad Akbar; Violi, Angela] Univ Michigan, Dept Mech Engn, Ann Arbor, MI 48109 USA. [Lee, Taek Soon; Simmons, Blake A.] Joint BioEnergy Inst, Emeryville, CA 94608 USA. [Simmons, Blake A.] Sandia Natl Labs, Biofuels & Biomat Sci & Technol Dept, Livermore, CA 94551 USA. RP Rotavera, B (reprint author), Sandia Natl Labs, Combust Res Facil, Combust Chem Dept, Livermore, CA 94550 USA. EM BRotave@Sandia.gov; CATaatj@Sandia.gov RI Zador, Judit/A-7613-2008; Welz, Oliver/C-1165-2013; OI Zador, Judit/0000-0002-9123-8238; Welz, Oliver/0000-0003-1978-2412; Simmons, Blake/0000-0002-1332-1810 FU Department of Energy by the U.S-China Clean Energy Research Center (CERC) Clean Vehicle Consortium [DE-PI0000012]; U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences; DOE Office of Science User Facility at Lawrence Berkeley National Laboratory [DE-AC02-05CH11231]; National Nuclear Security Administration [DE-AC04-94-AL85000]; Office of Science, Office of Biological and Environmental Research, of the United States Department of Energy [DE-AC02-05CH11231] FX The authors acknowledge financial support from the Department of Energy under Award Number DE-PI0000012, supported by the U.S-China Clean Energy Research Center (CERC) Clean Vehicle Consortium. J.Z., O.W., L.S., A.M.S., J.D.S, D.L.O., and the development and maintenance of the MPIMS kinetics machine are supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences. The research conducted used resources of the Advanced Light Source, which is a DOE Office of Science User Facility at Lawrence Berkeley National Laboratory under Contract DE-AC02-05CH11231. Sandia is a multiprogram laboratory operated by Sandia Corporation, a Lockheed Martin Company, for the National Nuclear Security Administration under contract DE-AC04-94-AL85000. The portion of work conducted by the Joint BioEnergy Institute was supported by the Office of Science, Office of Biological and Environmental Research, of the United States Department of Energy under Contract No. DE-AC02-05CH11231. NR 37 TC 3 Z9 3 U1 2 U2 41 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1089-5639 J9 J PHYS CHEM A JI J. Phys. Chem. A PD NOV 6 PY 2014 VL 118 IS 44 BP 10188 EP 10200 DI 10.1021/jp507811d PG 13 WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical SC Chemistry; Physics GA AS9RK UT WOS:000344579100004 PM 25234586 ER PT J AU Grimes, TS Zalupski, PR Martin, LR AF Grimes, Travis S. Zalupski, Peter R. Martin, Leigh R. TI Features of the Thermodynamics of Trivalent Lanthanide/Actinide Distribution Reactions by Tri-n-octylphosphine Oxide and Bis(2-ethylhexyl) Phosphoric Acid SO JOURNAL OF PHYSICAL CHEMISTRY B LA English DT Article ID LIQUID-LIQUID-EXTRACTION; NITRIC-ACID; TRIOCTYLPHOSPHINE OXIDE; SOLVENT-EXTRACTION; TRANSPLUTONIUM ELEMENTS; SELECTIVE EXTRACTION; STABILITY CONSTANTS; OXIDIZED AMERICIUM; ORGANIC-COMPOUNDS; NITRATE AB A new methodology has been developed to study the thermochemical features of the biphasic transfer reactions of trisnitrato complexes of lanthanides and americium by a monofunctional solvating ligand (tri-n-octylphosphine oxide, TOPO). Stability constants for successive nitrato complexes (M(NO3)(x)(3-x)(aq) where M is Eu3+, Am3+, or Cm3+) were determined to assist in the calculation of the extraction constant, Kex, for the metal ions under study. Enthalpies of extraction (triangle H-extr) for the lanthanide series (excluding Pm3+) and Am3+ by TOPO have been measured using isothermal titration calorimetry. The observed ?Hextr were found to be constant at similar to 29 kJ mol(-1) across the series from La3+ to Er3+, with a slight decrease observed from Tm3+ to Lu3+. These heats were found to be consistent with enthalpies determined using van't Hoff analysis of temperature dependent extraction studies. A complete set of thermodynamic parameters (triangle G, triangle H, triangle S) was calculated for Eu(NO3)(3), Am(NO3)(3), and Cm(NO3)(3) extraction by TOPO and Am3+ and Cm3+ extraction by bis(2-ethylhexyl) phosphoric acid (HDEHP). A discussion comparing the energetics of these systems is offered. The measured biphasic extraction heats for the transplutonium elements, triangle H-extr, presented in these studies are the first ever direct measurements offered using two-phase calorimetric techniques. C1 [Grimes, Travis S.; Zalupski, Peter R.; Martin, Leigh R.] Idaho Natl Lab, Aqueous Separat & Radiochem Dept, Idaho Falls, ID 83415 USA. RP Martin, LR (reprint author), Idaho Natl Lab, Aqueous Separat & Radiochem Dept, POB 1625, Idaho Falls, ID 83415 USA. EM Leigh.Martin@inl.gov RI Martin, Leigh/P-3167-2016 OI Martin, Leigh/0000-0001-7241-7110 FU Department of Energy, Nuclear Energy Fuel Cycle Research and Development, Thermodynamics and Kinetics program under DOE Idaho Operations Office [DE-AC07-05ID14517] FX This work was funded by the Department of Energy, Nuclear Energy Fuel Cycle Research and Development, Thermodynamics and Kinetics program under DOE Idaho Operations Office Contract DE-AC07-05ID14517. NR 41 TC 3 Z9 3 U1 1 U2 13 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1520-6106 J9 J PHYS CHEM B JI J. Phys. Chem. B PD NOV 6 PY 2014 VL 118 IS 44 BP 12725 EP 12733 DI 10.1021/jp507727v PG 9 WC Chemistry, Physical SC Chemistry GA AS9RS UT WOS:000344579900015 PM 25315891 ER PT J AU Mercado, CC Zalcutayev, A Zhu, K Flynn, CJ Cahoon, JF Nozik, AJ AF Mercado, Candy C. Zalcutayev, Andriy Zhu, Kai Flynn, Cory J. Cahoon, James F. Nozik, Arthur J. TI Sensitized Zinc-Cobalt-Oxide Spinel p-Type Photoelectrode SO JOURNAL OF PHYSICAL CHEMISTRY C LA English DT Article ID NANOCRYSTALLINE TIO2 ELECTRODES; SOLAR-CELLS; ELECTRICAL-PROPERTIES; CONVERSION EFFICIENCY; DEFECT STRUCTURE; COUMARIN DYES; NICKEL-OXIDE; NIO; FILMS; RECOMBINATION AB Tandem dye-sensitized solar cells that use nickel oxide as a hole-transport layer have limited performance due to the poor transport properties of NiO; alternative p-type oxides with the correct band alignment, good hole mobility, and stability in corrosive electrolyte must be identified. In this paper, we present our study on the ternary oxide material (zinccobaltoxide spinel) as a hole conductor in a sensitized architecture. Zinc substitution for cobalt in cobalt(II,III) oxide results in good p-type conductivity and a spinel crystal structure. The flatband potential of ZnCoO thin films was determined to be around 0.7 V vs NHE (pH 5) and varies slightly depending on the conducting substrate. The films were used as the hole-transport layer in a dye-sensitized solar cell, and the hole-injection current was generated upon sensitization by coumarin-343. The cells exhibited an IQE of >90% and an open-circuit voltage of around 260 mV. The increase in photon-to-electron conversion efficiency of ZnCoO over NiO was due to an increased diffusion length, lower recombination, and better transport within the semiconductor-electrolyte device. Although the films were assembled here as liquid electrolyte dye-sensitized photovoltaic devices, they are also applicable to dye-sensitized photoelectrochemical cells for solar fuels. C1 [Mercado, Candy C.; Nozik, Arthur J.] Univ Colorado, Renewable & Sustainable Energy Inst, Boulder, CO 80309 USA. [Nozik, Arthur J.] Univ Colorado, Dept Chem & Biochem, Boulder, CO 80309 USA. [Zalcutayev, Andriy; Zhu, Kai; Nozik, Arthur J.] Natl Renewable Energy Lab, Golden, CO 80401 USA. [Flynn, Cory J.; Cahoon, James F.] Univ N Carolina, Dept Chem, Chapel Hill, NC 27599 USA. RP Mercado, CC (reprint author), 027 UCB,Suite 208,Fleming Bldg, Boulder, CO 80309 USA. EM candy.mercado@colorado.edu RI Nozik, Arthur/A-1481-2012; Nozik, Arthur/P-2641-2016; OI Flynn, Cory/0000-0002-3175-6770; Zakutayev, Andriy/0000-0002-3054-5525 FU UNC Center for Solar Fuels, an Energy Frontier Research Center - U.S. Department of Energy, Office of Science [DE-SC0001011]; Center for Inverse Design Energy Frontier Research Center [DE-AC36-08GO28308]; Division of Chemical Sciences, Geosciences, and Biosciences, Office of Basic Energy Sciences, U.S. Department of Energy [DE-AC36-08GO28308]; National Renewable Energy Laboratory FX This research was primarily supported by the UNC Center for Solar Fuels, an Energy Frontier Research Center funded by the U.S. Department of Energy, Office of Science, under Award DE-SC0001011 supporting C.C.M, C.J.F., J.F.C., and A.J.N. The sputtering and crystallinity and composition characterization of the films were done by A.Z. as a part of Center for Inverse Design Energy Frontier Research Center under Contact DE-AC36-08GO28308 to NREL. K.Z. was supported by the Division of Chemical Sciences, Geosciences, and Biosciences, Office of Basic Energy Sciences, U.S. Department of Energy, under Contract DE-AC36-08GO28308 with the National Renewable Energy Laboratory and measured the IMVS and IMPS. NR 43 TC 8 Z9 8 U1 6 U2 74 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1932-7447 J9 J PHYS CHEM C JI J. Phys. Chem. C PD NOV 6 PY 2014 VL 118 IS 44 BP 25340 EP 25349 DI 10.1021/jp508153j PG 10 WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Chemistry; Science & Technology - Other Topics; Materials Science GA AS9RM UT WOS:000344579300006 ER PT J AU Velasco-Velez, JJ Wu, CH Wang, BY Sun, Y Zhang, Y Guo, JH Salmeron, M AF Velasco-Velez, J. J. Wu, C. H. Wang, B. Y. Sun, Y. Zhang, Y. Guo, J. -H. Salmeron, M. TI Polarized X-ray Absorption Spectroscopy Observation of Electronic and Structural Changes of Chemical Vapor Deposition Graphene in Contact with Water SO JOURNAL OF PHYSICAL CHEMISTRY C LA English DT Article ID NEAR-EDGE; FILMS; RAMAN AB The interaction of chemical vapor deposition (CVD)-grown graphene films with water was studied by means of in situ angle-dependent X-ray absorption spectroscopy (XAS). We found that when the graphene layer is in contact with water there is a reduction in the pi* peak intensity in the carbon K-edge absorption spectra, accompanied by an extension of the pi* peak to lower energies, which are indicative of chemical modifications of the graphene and a reduction in the number of unsaturated carbon bonds due to the covalent attachment of contaminant species. In addition to the chemical changes a decrease in the dichroic ratio measured by polarized XAS measurements was observed, which indicates an increase on the nanometer scale corrugation. These changes can strongly influence the electronic properties, mechanical robustness, and resistance to sloughing, as well as graphene reactivity C1 [Velasco-Velez, J. J.; Wu, C. H.; Sun, Y.; Zhang, Y.; Salmeron, M.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA. [Wu, C. H.] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA. [Wang, B. Y.; Guo, J. -H.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94720 USA. [Salmeron, M.] Univ Calif Berkeley, Dept Mat Sci & Engn, Berkeley, CA 94720 USA. RP Salmeron, M (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA. EM mbsalmeron@lbl.gov RI Zhang, Y/E-6600-2011; Wu, Cheng Hao/C-9565-2014; Foundry, Molecular/G-9968-2014 OI Zhang, Y/0000-0003-0344-8399; FU U.S. Department of Energy (DOE), Office of Basic Energy Sciences (BES), Materials Sciences and Engineering (MSE) Division [DE-AC02-05CH11231]; Alexander von Humboldt foundation FX This work was supported by the U.S. Department of Energy (DOE), Office of Basic Energy Sciences (BES), Materials Sciences and Engineering (MSE) Division, under Contract No. DE-AC02-05CH11231. J.J. Velasco-Velez gratefully acknowledges financial support from the Alexander von Humboldt foundation. Y. Zhang and the graphene synthesis work were supported by the Molecular Foundry. The ALS and Molecular Foundry are User Facilities of the DOE, Office of Science. NR 18 TC 5 Z9 5 U1 4 U2 42 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1932-7447 J9 J PHYS CHEM C JI J. Phys. Chem. C PD NOV 6 PY 2014 VL 118 IS 44 BP 25456 EP 25459 DI 10.1021/jp507405z PG 4 WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Chemistry; Science & Technology - Other Topics; Materials Science GA AS9RM UT WOS:000344579300018 ER PT J AU Gong, Y Joly, AG El-Khoury, PZ Hess, WP AF Gong, Yu Joly, Alan G. El-Khoury, Patrick Z. Hess, Wayne P. TI Nonlinear Photoemission Electron Micrographs of Plasmonic Nanoholes in Gold Thin Films SO JOURNAL OF PHYSICAL CHEMISTRY C LA English DT Article ID SURFACE-PLASMONS; OPTICAL-TRANSMISSION; LIGHT; PROPAGATION; POLARITONS; NANOWIRES; MICROSCOPY AB Nonlinear photoemission electron microscopy of isolated nanoholes in gold thin films maps propagating surface plasmon polaritons (SPPs) launched from the lithographically patterned plasmonic structures. A damped elongated ringlike photoemission beat pattern is observed from the nanoholes, following low angle of incidence irradiation of these structures with sub-15 fs 780 nm laser pulses. A notable agreement between finite difference time domain simulations and experiment corroborates our assignment of the observed photoemission patterns to SPPs launched from isolated nanoholes and probed through nonlinear photoemission. We also demonstrate how the efficiency of coupling light waves into isolated plasmonic holes can be tuned by varying hole diameter. In this regard, a simple intuitive geometrical model, which accounts for the observed and simulated diameter dependent plasmonic response, is proposed. Overall, this study paves the way for designing nanohole assemblies where optical coupling and subsequent plasmon propagation can be rationally controlled through 2D SPP interferometry. C1 [Gong, Yu; Joly, Alan G.; El-Khoury, Patrick Z.; Hess, Wayne P.] Pacific NW Natl Lab, Div Phys Sci, Richland, WA 99352 USA. RP Hess, WP (reprint author), Pacific NW Natl Lab, Div Phys Sci, POB 999, Richland, WA 99352 USA. EM wayne.hess@pnnl.gov RI Gong, Yu /I-9950-2014 OI Gong, Yu /0000-0002-9357-9503 FU U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, Division of Chemical Sciences, Geosciences Biosciences; Laboratory Directed Research and Development Program through a Linus Pauling Fellowship at Pacific Northwest National Laboratory (PNNL); Department of Energy's Office of Biological and Environmental Research located at PNNL FX This work was supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, Division of Chemical Sciences, Geosciences & Biosciences. P.Z.E.-K. acknowledges support from the Laboratory Directed Research and Development Program through a Linus Pauling Fellowship at Pacific Northwest National Laboratory (PNNL), a multi-program national laboratory operated for DOE by Battelle. The research was performed using EMSL, a national scientific user facility sponsored by the Department of Energy's Office of Biological and Environmental Research and located at PNNL. NR 35 TC 8 Z9 8 U1 1 U2 22 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1932-7447 J9 J PHYS CHEM C JI J. Phys. Chem. C PD NOV 6 PY 2014 VL 118 IS 44 BP 25671 EP 25676 DI 10.1021/jp509900h PG 6 WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Chemistry; Science & Technology - Other Topics; Materials Science GA AS9RM UT WOS:000344579300042 ER PT J AU Li, X Eilam, A Shapiro, M AF Li, Xuan Eilam, Asaf Shapiro, Moshe TI Complete Quantum State Selectivity in Cold Molecular Beams Using Deflection-Resistant Dark States in a STIRAP Configuration SO JOURNAL OF PHYSICAL CHEMISTRY LETTERS LA English DT Article ID ELECTROMAGNETICALLY INDUCED TRANSPARENCY; POPULATION TRANSFER; TRANSITIONS; SCATTERING; PULSES; ATOMS; LIGHT AB One of the main goals of chemical dynamics is the creation of molecular beams composed of a single (vibrational, rotational, and magnetic) quantum state of choice. In this Letter, we propose a method to achieve complete quantum state selectivity by producing resistance to electromagnetically induced deflection (EID) and that the state to be selected can be "dialed in" at will. We illustrate the method by showing in detail how to purify thermal beams of the LiRb and IF molecules to yield molecular beams composed of a variety of prechosen single internal quantum states and/or superpositions of such states. We expect that this method will be implemented in all subsequent explorations of the fundamentals of chemical reactions and their control and the use of cold molecules as a vehicle for studying some of the most profound issues of quantum dynamics. [GRAPHICS] C1 [Li, Xuan] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Chem Sci & Ultrafast Xray Sci Lab, Berkeley, CA 94720 USA. [Eilam, Asaf; Shapiro, Moshe] Univ British Columbia, Dept Chem, Vancouver, BC V6T 1Z1, Canada. RP Li, X (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Chem Sci & Ultrafast Xray Sci Lab, Berkeley, CA 94720 USA. EM xuanli@lbl.gov; easaf@chem.ubc.ca FU "Major Thematic Grant" of the Peter Wall Institute for Advanced Studies of the University of British Columbia; NSERC Discovery Grant; US-DoD DTRA Program FX This work was supported by a "Major Thematic Grant" of the Peter Wall Institute for Advanced Studies of the University of British Columbia, by a NSERC Discovery Grant, and by the US-DoD DTRA Program. NR 37 TC 0 Z9 0 U1 2 U2 14 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1948-7185 J9 J PHYS CHEM LETT JI J. Phys. Chem. Lett. PD NOV 6 PY 2014 VL 5 IS 21 BP 3620 EP 3624 DI 10.1021/jz501852p PG 5 WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Atomic, Molecular & Chemical SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AS9RO UT WOS:000344579500016 PM 26278728 ER PT J AU Yin, WJ Yan, YF Wei, SH AF Yin, Wan-Jian Yan, Yanfa Wei, Su-Huai TI Anomalous Alloy Properties in Mixed Halide Perovskites SO JOURNAL OF PHYSICAL CHEMISTRY LETTERS LA English DT Article ID LEAD IODIDE PEROVSKITE; HYBRID SOLAR-CELLS; QUASI-RANDOM STRUCTURES; WAVE BASIS-SET; OPTICAL-PROPERTIES; 1ST-PRINCIPLES CALCULATION; SEQUENTIAL DEPOSITION; BROMIDE PEROVSKITE; CHARGE-TRANSPORT; HIGH-PERFORMANCE AB Engineering halide perovskite through mixing halogen elements, such as CH3NH3PbI3-xClx and CH3NH3PbI3-xBrx, is a viable way to tune its electronic and optical properties. Despite many emerging experiments on mixed halide perovskites, the basic electronic and structural properties of the alloys have not been understood and some crucial questions remain, for example, how much Cl can be incorporated into CH3NH3PbI3 is still unclear. In this Letter, we chose CsPbX3 (X = I, Br, Cl) as an example and use a first-principle calculation together with cluster-expansion methods to systematically study the structural, electronic, and optical properties of mixed halide perovskites and find that unlike conventional semiconductor alloys, they exhibit many anomalous alloy properties such as small or even negative formation energies at some concentrations and negligible or even negative band gap bowing parameters at high temperature. We further show that mixed-(I,Cl) perovskite is hard to form at temperature below 625 K, whereas forming mixed-(Br,Cl) and (I,Br) alloys are easy at room temperature. C1 [Yin, Wan-Jian; Wei, Su-Huai] Natl Renewable Energy Lab, Golden, CO 80401 USA. [Yin, Wan-Jian; Yan, Yanfa] Univ Toledo, Dept Phys & Astron, Toledo, OH 43606 USA. [Yin, Wan-Jian; Yan, Yanfa] Univ Toledo, Wright Ctr Photovolta Innovat & Commercializat, Toledo, OH 43606 USA. RP Yin, WJ (reprint author), Natl Renewable Energy Lab, Golden, CO 80401 USA. EM yinwanjian@gmail.com; yanfa.yan@utoledo.edu; suhuai.wei@nrel.gov RI Yin, Wanjian/F-6738-2013 FU U.S. Department of Energy [DE-AC36-08GO28308]; Office of Science of the U.S. Department of Energy [DE-AC02-05CH11231]; Ohio Research Scholar Program FX This research was funded by the U.S. Department of Energy under the Grant No. DE-AC36-08GO28308 to NREL. It used the resources of the Ohio Supercomputer Center and the National Energy Research Scientific Computing Center, which is supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. Y.Y. acknowledges the support of the Ohio Research Scholar Program. NR 58 TC 30 Z9 30 U1 17 U2 153 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1948-7185 J9 J PHYS CHEM LETT JI J. Phys. Chem. Lett. PD NOV 6 PY 2014 VL 5 IS 21 BP 3625 EP 3631 DI 10.1021/jz501896w PG 7 WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Atomic, Molecular & Chemical SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AS9RO UT WOS:000344579500028 PM 26278729 ER PT J AU Markus, IM Lin, F Kam, KC Asta, M Doeff, MM AF Markus, Isaac M. Lin, Feng Kam, Kinson C. Asta, Mark Doeff, Marca M. TI Computational and Experimental Investigation of Ti Substitution in Li-1(NixMnxCo1-2x-yTiy)O-2 for Lithium Ion Batteries SO JOURNAL OF PHYSICAL CHEMISTRY LETTERS LA English DT Article ID TOTAL-ENERGY CALCULATIONS; AUGMENTED-WAVE METHOD; ELECTROCHEMICAL PROPERTIES; CATHODE MATERIALS; ELECTRODE MATERIALS; STRUCTURAL-CHANGES; LI BATTERIES; BASIS-SET; LINI1/3CO1/3MN1/3O2; OXIDE AB Aliovalent substitutions in layered transition-metal cathode materials has been demonstrated to improve the energy densities of lithium ion batteries, with the mechanisms underlying such effects incompletely understood. Performance enhancement associated with Ti substitution of Co in the cathode material Li-1(NixMnxCo1-2x)O-2 were investigated using density functional theory calculations, including Hubbard-U corrections. An examination of the structural and electronic modifications revealed that Ti substitution reduces the structural distortions occurring during delithiation due to the larger cation radius of Ti4+ relative to Co3+ and the presence of an electron polaron on Mn cations induced by aliovalent Ti substitution. The structural differences were found to correlate with a decrease in the lithium intercalation voltage at lower lithium concentrations, which is consistent with quasi-equilibrium voltages obtained by integrating data from stepped potential experiments. Further, Ti is found to suppress the formation of a secondary rock salt phase at high voltage. Our results provide insights into how selective substitutions can enhance the performance of cathodes, maximizing the energy density and lifetime of current Li ion batteries. C1 [Markus, Isaac M.; Asta, Mark] Univ Calif Berkeley, Mat Sci & Engn Dept, Berkeley, CA 94720 USA. [Markus, Isaac M.; Lin, Feng; Doeff, Marca M.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Environm Energy Technol Div, Berkeley, CA 94720 USA. [Asta, Mark] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA. [Kam, Kinson C.] Haldor Topsoe Res Labs, DK-2800 Lyngby, Denmark. RP Markus, IM (reprint author), Univ Calif Berkeley, Mat Sci & Engn Dept, Berkeley, CA 94720 USA. EM isaac.markus@berkeley.edu; mmdoeff@lbl.gov FU Office of Vehicle Technologies of the U.S. Department of Energy [DE-AC02-05CH11231]; Office of Science of the U.S. Department of Energy [DE-AC03-76SF00098]; National Science Foundation [ACI-1053575]; NSF graduate research fellowship program FX This work was supported by the Assistant Secretary for Energy Efficiency and Renewable Energy, Office of Vehicle Technologies of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231 under the Batteries for Advanced Transportation Technologies (BATT) Program. This work made use of computational resources provided by the National Energy Research Supercomputer Center (NERSC), which is supported by the Office of Science of the U.S. Department of Energy under Contract DE-AC03-76SF00098. This work also used the Extreme Science and Engineering Discovery Environment (XSEDE), which is supported by National Science Foundation Grant Number ACI-1053575. I.M.M acknowledges the support of the NSF graduate research fellowship program and Dr. Kristin Persson for useful discussions and feedback. NR 48 TC 14 Z9 15 U1 8 U2 70 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1948-7185 J9 J PHYS CHEM LETT JI J. Phys. Chem. Lett. PD NOV 6 PY 2014 VL 5 IS 21 BP 3649 EP 3655 DI 10.1021/jz5017526 PG 7 WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Atomic, Molecular & Chemical SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AS9RO UT WOS:000344579500029 PM 26278733 ER PT J AU Zhang, Y Biggs, JD Govind, N Mukamel, S AF Zhang, Yu Biggs, Jason D. Govind, Niranjan Mukamel, Shaul TI Monitoring Long-Range Electron Transfer Pathways in Proteins by Stimulated Attosecond Broadband X-ray Raman Spectroscopy SO JOURNAL OF PHYSICAL CHEMISTRY LETTERS LA English DT Article ID TRYPTOPHAN; FLOW; DNA; CHEMISTRY; OXIDASE AB Long-range electron transfer (ET) is a crucial step in many energy conversion processes and biological redox reactions in living organisms. We show that newly developed X-ray pulses can directly probe the evolving oxidation states and the electronic structure around selected atoms with detail not available through conventional time-resolved infrared or optical techniques. This is demonstrated in a simulation study of the stimulated X-ray Raman (SXRS) signals in Re-modified azurin, which serves as a benchmark system for photoinduced ET in proteins. Nonlinear SXRS signals offer a direct novel window into the long-range ET mechanism. [GRAPHICS] C1 [Zhang, Yu; Biggs, Jason D.; Mukamel, Shaul] Univ Calif Irvine, Dept Chem, Irvine, CA 92697 USA. [Govind, Niranjan] Pacific NW Natl Lab, William R Wiley Environm Mol Sci Lab, Richland, WA 99352 USA. RP Mukamel, S (reprint author), Univ Calif Irvine, Dept Chem, 450 Rowland Hall, Irvine, CA 92697 USA. EM smukamel@uci.edu FU Chemical Sciences, Geosciences and Biosciences Division, Office of Basic Energy Sciences, Office of Science, U.S. Department of Energy; National Science Foundation [CHE-1361516]; National Institutes of Health [GM-59230]; Department of Energy's Office of Biological and Environmental Research located at Pacific Northwest National Laboratory FX The support of the Chemical Sciences, Geosciences and Biosciences Division, Office of Basic Energy Sciences, Office of Science, U.S. Department of Energy is gratefully acknowledged. We also gratefully acknowledge the support of the National Science Foundation (Grant CHE-1361516), and the National Institutes of Health (Grant GM-59230). A portion of the research was performed using EMSL, a national scientific user facility sponsored by the Department of Energy's Office of Biological and Environmental Research and located at Pacific Northwest National Laboratory. The authors wish to thank Prof. Harry B. Gray for most useful discussions. NR 32 TC 4 Z9 4 U1 0 U2 13 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1948-7185 J9 J PHYS CHEM LETT JI J. Phys. Chem. Lett. PD NOV 6 PY 2014 VL 5 IS 21 BP 3656 EP 3661 DI 10.1021/jz501966h PG 6 WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Atomic, Molecular & Chemical SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AS9RO UT WOS:000344579500011 PM 25400875 ER PT J AU Kawarai, Y Weber, T Azuma, Y Winstead, C McKoy, V Belkacem, A Slaughter, DS AF Kawarai, Y. Weber, Th. Azuma, Y. Winstead, C. McKoy, V. Belkacem, A. Slaughter, D. S. TI Dynamics of the Dissociating Uracil Anion Following Resonant Electron Attachment SO JOURNAL OF PHYSICAL CHEMISTRY LETTERS LA English DT Article ID IMAGING TECHNIQUE; SPECTROSCOPY; NCO AB We report a combined experimental and theoretical investigation of dissociative electron attachment (DEA) to the nucleobase uracil. Using ion momentum imaging experiments employing a DEA reaction microscope we have measured 3-dimensional momentum distributions of specific anionic fragments following DEA to uracil by 6 eV electrons. From the measured anion fragment kinetic energy we determine the possible dissociation pathways and the total kinetic energy release. We employ electronic structure and electron scattering calculations to determine the probability for electron attachment in the molecular frame. Combining these calculations with the imaging measurements, we reveal several key features of the coupled electronic and nuclear dynamics of DEA. [GRAPHICS] C1 [Kawarai, Y.; Azuma, Y.] Sophia Univ, Fac Sci & Technol, Dept Mat & Life Sci, Chiyoda Ku, Tokyo 1028554, Japan. [Kawarai, Y.; Weber, Th.; Belkacem, A.; Slaughter, D. S.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA. [Winstead, C.; McKoy, V.] CALTECH, Arthur Amos Noyes Lab Chem Phys, Pasadena, CA 91125 USA. RP Slaughter, DS (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA. EM DSSlaughter@lbl.gov OI Slaughter, Daniel/0000-0002-4621-4552 FU U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences; Division of Chemical Sciences, Geo-sciences, and Biosciences [DE-AC02-05CH11231, DE-FG02-97ER14814]; Japan Society for the Promotion of Science [23600009] FX This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, and by the Division of Chemical Sciences, Geo-sciences, and Biosciences under Contracts No. DE-AC02-05CH11231 (LBNL) and DE-FG02-97ER14814 (California Institute of Technology). The work of V.M. and C.W. made use of the Jet Propulsion Laboratory's Supercomputing and Visualization Facility. Y.A. acknowledges the Japan Society for the Promotion of Science for support through Grants-in-Aid for Scientific Research (No. 23600009). NR 34 TC 4 Z9 4 U1 1 U2 12 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1948-7185 J9 J PHYS CHEM LETT JI J. Phys. Chem. Lett. PD NOV 6 PY 2014 VL 5 IS 21 BP 3854 EP 3858 DI 10.1021/jz501907d PG 5 WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Atomic, Molecular & Chemical SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AS9RO UT WOS:000344579500023 PM 26278760 ER PT J AU Biffin, A Johnson, RD Kimchi, I Morris, R Bombardi, A Analytis, JG Vishwanath, A Coldea, R AF Biffin, A. Johnson, R. D. Kimchi, I. Morris, R. Bombardi, A. Analytis, J. G. Vishwanath, A. Coldea, R. TI Noncoplanar and Counterrotating Incommensurate Magnetic Order Stabilized by Kitaev Interactions in gamma-Li2IrO3 SO PHYSICAL REVIEW LETTERS LA English DT Article AB Materials that realize Kitaev spin models with bond-dependent anisotropic interactions have long been searched for, as the resulting frustration effects are predicted to stabilize novel forms of magnetic order or quantum spin liquids. Here, we explore the magnetism of gamma-Li2IrO3, which has the topology of a three-dimensional Kitaev lattice of interconnected Ir honeycombs. Using magnetic resonant x-ray diffraction, we find a complex, yet highly symmetric incommensurate magnetic structure with noncoplanar and counterrotating Ir moments. We propose a minimal Kitaev-Heisenberg Hamiltonian that naturally accounts for all key features of the observed magnetic structure. Our results provide strong evidence that gamma-Li2IrO3 realizes a spin Hamiltonian with dominant Kitaev interactions. C1 [Biffin, A.; Johnson, R. D.; Morris, R.; Coldea, R.] Univ Oxford, Clarendon Lab, Oxford OX1 3PU, England. [Kimchi, I.; Analytis, J. G.; Vishwanath, A.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA. [Bombardi, A.] Diamond Light Source Ltd, Didcot OX11 0DE, Oxon, England. [Analytis, J. G.; Vishwanath, A.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA. RP Biffin, A (reprint author), Univ Oxford, Clarendon Lab, Parks Rd, Oxford OX1 3PU, England. FU EPSRC (U.K.) [EP/H014934/1, EP/J003557/1]; U.S. Department of Energy, Office of Basic Energy Sciences, Materials Sciences and Engineering Division [DE-AC02-05CH11231] FX This work was supported by EPSRC (U.K.) under Grants No. EP/H014934/1 and No. EP/J003557/1, and by the U.S. Department of Energy, Office of Basic Energy Sciences, Materials Sciences and Engineering Division, under Contract No. DE-AC02-05CH11231. We thank A. Coldea for technical help with the micro-calorimeter specific heat measurements. NR 19 TC 35 Z9 35 U1 4 U2 32 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0031-9007 EI 1079-7114 J9 PHYS REV LETT JI Phys. Rev. Lett. PD NOV 6 PY 2014 VL 113 IS 19 AR 197201 DI 10.1103/PhysRevLett.113.197201 PG 5 WC Physics, Multidisciplinary SC Physics GA AS8HJ UT WOS:000344490100008 PM 25415919 ER PT J AU Zhang, H Ming, FF Kim, HJ Zhu, HB Zhang, Q Weitering, HH Xiao, XD Zeng, CG Cho, JH Zhang, ZY AF Zhang, Hui Ming, Fangfei Kim, Hyun-Jung Zhu, Hongbin Zhang, Qiang Weitering, Hanno H. Xiao, Xudong Zeng, Changgan Cho, Jun-Hyung Zhang, Zhenyu TI Stabilization and Manipulation of Electronically Phase-Separated Ground States in Defective Indium Atom Wires on Silicon SO PHYSICAL REVIEW LETTERS LA English DT Article ID CHARGE-DENSITY-WAVE; QUANTUM CHAINS; SURFACE; SUPERCONDUCTIVITY; TRANSITION; MANGANITE AB Exploration and manipulation of electronic states in low-dimensional systems are of great importance in the fundamental and practical aspects of nanomaterial and nanotechnology. Here, we demonstrate that the incorporation of vacancy defects into monatomic indium wires on n-type Si(111) can stabilize electronically phase-separated ground states where the insulating 8 x 2 and metallic 4 x 1 phases coexist. Furthermore, the areal ratio of the two phases in the phase-separated states can be tuned reversibly by electric field or charge doping, and such tunabilities can be quantitatively captured by first principles-based modeling and simulations. The present results extend the realm of electronic phase separation from strongly correlated d-electron materials typically in bulk form to weakly interacting sp-electron systems in reduced dimensionality. C1 [Zhang, Hui; Zhu, Hongbin; Zhang, Qiang; Zeng, Changgan] Univ Sci & Technol China, Hefei Natl Lab Phys Sci Microscale HFNL, Hefei 230026, Anhui, Peoples R China. [Zhang, Hui; Zhu, Hongbin; Zhang, Qiang; Zeng, Changgan] Univ Sci & Technol China, Dept Phys, Hefei 230026, Anhui, Peoples R China. [Ming, Fangfei; Xiao, Xudong] Chinese Univ Hong Kong, Dept Phys, Shatin, Hong Kong, Peoples R China. [Kim, Hyun-Jung; Cho, Jun-Hyung] Hanyang Univ, Dept Phys, Seoul 133791, South Korea. [Weitering, Hanno H.] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA. [Weitering, Hanno H.] Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37831 USA. [Xiao, Xudong] Chinese Acad Sci, Shenzhen Inst Adv Technol, Shenzhen 518055, Peoples R China. [Zeng, Changgan; Zhang, Zhenyu] Univ Sci & Technol China, Int Ctr Quantum Design Funct Mat ICQD, HFNL, Hefei 230026, Anhui, Peoples R China. [Zeng, Changgan; Zhang, Zhenyu] Univ Sci & Technol China, Synerget Innovat Ctr Quantum Informat & Quantum P, Hefei 230026, Anhui, Peoples R China. RP Zeng, CG (reprint author), Univ Sci & Technol China, Hefei Natl Lab Phys Sci Microscale HFNL, Hefei 230026, Anhui, Peoples R China. EM cgzeng@ustc.edu.cn; chojh@hanyang.ac.kr RI Hyun-Jung, Kim/E-8074-2011; Cho, Jun-Hyung/R-7256-2016; OI Hyun-Jung, Kim/0000-0002-5602-1404; Cho, Jun-Hyung/0000-0002-1785-1835; Ming, Fangfei/0000-0003-4630-1653 FU NSFC [11434009, 11374279, 11034006]; NKBRPC [2014CB921102]; CAS [XDB01020000]; SRFDP [20113402110046]; FRFCU [WK2340000035, WK2340000011]; NRF [2014M2B2A9032247]; KISTI supercomputing center through the strategic support program [KSC-2013-C3-043]; NSF [DMR-1005488] FX H. Z., F. M., and H.-J. K contributed equally to this work. This work was supported in part by the NSFC (Grants No. 11434009, No. 11374279, and No. 11034006), NKBRPC (Grant No. 2014CB921102), CAS (Grant No. XDB01020000), SRFDP (Grant No. 20113402110046), FRFCU (Grants No. WK2340000035 and No. WK2340000011), the NRF (Grant No. 2014M2B2A9032247), and the KISTI supercomputing center through the strategic support program (No. KSC-2013-C3-043). H. H. W. acknowledges support from NSF Grant No. DMR-1005488. NR 39 TC 8 Z9 8 U1 4 U2 56 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0031-9007 EI 1079-7114 J9 PHYS REV LETT JI Phys. Rev. Lett. PD NOV 6 PY 2014 VL 113 IS 19 AR 196802 DI 10.1103/PhysRevLett.113.196802 PG 5 WC Physics, Multidisciplinary SC Physics GA AS8HJ UT WOS:000344490100006 PM 25415916 ER PT J AU Schunck, N Duke, D Carr, H Knoll, A AF Schunck, N. Duke, D. Carr, H. Knoll, A. TI Description of induced nuclear fission with Skyrme energy functionals: Static potential energy surfaces and fission fragment properties SO PHYSICAL REVIEW C LA English DT Article ID INITIO MOLECULAR-DYNAMICS; HARMONIC-OSCILLATOR BASIS; HARTREE-FOCK; SELF-CONSISTENT; MEAN-FIELD; KINETIC-ENERGY; DENSITY; MASS; EQUATIONS; BARRIERS AB Eighty years after its experimental discovery, a description of induced nuclear fission based solely on the interactions between neutrons and protons and quantum many-body methods still poses formidable challenges. The goal of this paper is to contribute to the development of a predictive microscopic framework for the accurate calculation of static properties of fission fragments for hot fission and thermal or slow neutrons. To this end, we focus on the Pu-239(n, f) reaction and employ nuclear density functional theory with Skyrme energy densities. Potential energy surfaces are computed at the Hartree-Fock-Bogoliubov approximation with up to five collective variables. We find that the triaxial degree of freedom plays an important role, both near the fission barrier and at scission. The impact of the parametrization of the Skyrme energy density and the role of pairing correlations on deformation properties from the ground state up to scission are also quantified. We introduce a general template for the quantitative description of fission fragment properties. It is based on the careful analysis of scission configurations, using both advanced topological methods and recently proposed quantum many-body techniques. We conclude that an accurate prediction of fission fragment properties at low incident neutron energies, although technologically demanding, should be within the reach of current nuclear density functional theory. C1 [Schunck, N.] Lawrence Livermore Natl Lab, Div Phys, Livermore, CA 94551 USA. [Duke, D.; Carr, H.] Univ Leeds, Sch Comp, Leeds, W Yorkshire, England. [Knoll, A.] Argonne Natl Lab, Argonne, IL 60439 USA. RP Schunck, N (reprint author), Lawrence Livermore Natl Lab, Div Phys, Livermore, CA 94551 USA. OI Schunck, Nicolas/0000-0002-9203-6849 FU U.S. Department of Energy by Lawrence Livermore National Laboratory [DE-AC52-07NA27344]; U.S. Department of Energy Office of Science, Nuclear Physics Program [DE-AC52-07NA27344 Clause B-9999, Clause H-9999]; American Recovery and Reinvestment Act, Pub. L. 111-5; Office of Science of the Department of Energy [DE-AC05-00OR22725]; UK Engineering and Physical Sciences Research Council [EP/J013072/1] FX We express our deepest gratitude to W. Younes and D. Gogny for many stimulating and enlightening discussions, and for explaining us the details of their quantum localization method. We are also thankful to N. Dubray, W. Nazarewicz and J. Pei for useful comments. Special thanks are addressed to J. McDonnell for a careful reading of the manuscript. This work was partly performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract No. DE-AC52-07NA27344. Funding was also provided by the U.S. Department of Energy Office of Science, Nuclear Physics Program pursuant to Contract No. DE-AC52-07NA27344 Clause B-9999, Clause H-9999, and the American Recovery and Reinvestment Act, Pub. L. 111-5. An award of computer time under the name "Computational Nuclear Structure" was provided by the Innovative and Novel Computational Impact on Theory and Experiment (INCITE) program. This research used resources of the Oak Ridge Leadership Computing Facility located in the Oak Ridge National Laboratory, which is supported by the Office of Science of the Department of Energy under Contract DE-AC05-00OR22725. It also used an award under the Annual Computing Grand Challenge Program at LLNL. Thanks are also due to the UK Engineering and Physical Sciences Research Council, under Grant No. EP/J013072/1. NR 108 TC 17 Z9 17 U1 2 U2 10 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0556-2813 EI 1089-490X J9 PHYS REV C JI Phys. Rev. C PD NOV 6 PY 2014 VL 90 IS 5 AR 054305 DI 10.1103/PhysRevC.90.054305 PG 18 WC Physics, Nuclear SC Physics GA AS7AS UT WOS:000344410700002 ER PT J AU Kumah, DP Malashevich, A Disa, AS Arena, DA Walker, FJ Ismail-Beigi, S Ahn, CH AF Kumah, Divine P. Malashevich, Andrei Disa, Ankit S. Arena, Dario A. Walker, Frederick J. Ismail-Beigi, Sohrab Ahn, Charles H. TI Effect of Surface Termination on the Electronic Properties of LaNiO3 Films SO PHYSICAL REVIEW APPLIED LA English DT Article ID METAL-INSULATOR-TRANSITION; OXIDE INTERFACES; PIXEL DETECTOR; RNIO3 R; FERROELECTRICITY; MULTIFERROICS; SYSTEMS; PHYSICS AB The electronic and structural properties of thin LaNiO3 films grown by using molecular beam epitaxy are studied as a function of the net ionic charge of the surface terminating layer. We demonstrate that electronic transport in nickelate heterostructures can be manipulated through changes in the surface termination due to a strong coupling of the surface electrostatic properties to the structural properties of the Ni-O bonds that govern electronic conduction. We observe experimentally and from first-principles theory an asymmetric response of the structural properties of the films to the sign of the surface charge, which results from a strong interplay between electrostatic and mechanical boundary conditions governing the system. The structural response results in ionic buckling in the near-surface NiO2 planes for films terminated with negatively charged NiO2 and bulklike NiO2 planes for films terminated with positively charged LaO planes. The ability to modify transport properties by the deposition of a single atomic layer can be used as a guiding principle for nanoscale device fabrication. C1 [Kumah, Divine P.; Malashevich, Andrei; Disa, Ankit S.; Walker, Frederick J.; Ismail-Beigi, Sohrab; Ahn, Charles H.] Yale Univ, Ctr Res Interface Struct & Phenomena, New Haven, CT 06520 USA. [Kumah, Divine P.; Malashevich, Andrei; Disa, Ankit S.; Walker, Frederick J.; Ismail-Beigi, Sohrab; Ahn, Charles H.] Yale Univ, Dept Appl Phys, New Haven, CT 06520 USA. [Arena, Dario A.] Brookhaven Natl Lab, Upton, NY 11973 USA. [Ismail-Beigi, Sohrab; Ahn, Charles H.] Yale Univ, Dept Mech Engn & Mat Sci, New Haven, CT 06520 USA. RP Kumah, DP (reprint author), Yale Univ, Ctr Res Interface Struct & Phenomena, New Haven, CT 06520 USA. EM divine.kumah@yale.edu RI Ismail-Beigi, Sohrab/F-2382-2014; Kumah, Divine/A-7031-2011; OI Ismail-Beigi, Sohrab/0000-0002-7331-9624; Kumah, Divine/0000-0003-0715-1285; Disa, Ankit/0000-0002-7762-3244; Walker, Frederick/0000-0002-8094-249X FU NSF MRSEC [DMR-1119826]; U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-AC02-06CH11357, DE-AC02-98CH10886]; NSF [CNS 08-21132]; NSF XSEDE [TG-MCA08X007] FX The work at Yale is supported by NSF MRSEC DMR-1119826 (CRISP). Use of the Advanced Photon Source is supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract No. DE-AC02-06CH11357. Use of the National Synchrotron Light Source, Brookhaven National Laboratory, is supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract No. DE-AC02-98CH10886. Partial personnel and facilities support is provided by NSF Grant No. CNS 08-21132 and by the facilities and staff of the Yale University Faculty of Arts and Sciences High Performance Computing Center. Additional computations are carried out via the NSF XSEDE resources through Grant No. TG-MCA08X007. NR 51 TC 4 Z9 4 U1 2 U2 51 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 2331-7019 J9 PHYS REV APPL JI Phys. Rev. Appl. PD NOV 6 PY 2014 VL 2 IS 5 AR 054004 DI 10.1103/PhysRevApplied.2.054004 PG 7 WC Physics, Applied SC Physics GA AS5ZG UT WOS:000344344300001 ER PT J AU Lees, JP Poireau, V Tisserand, V Grauges, E Palano, A Eigen, G Stugu, B Brown, DN Kerth, LT Kolomensky, YG Lee, MJ Lynch, G Koch, H Schroeder, T Hearty, C Mattison, TS McKenna, JA So, RY Khan, A Blinov, VE Buzykaev, AR Druzhinin, VP Golubev, VB Kravchenko, EA Onuchin, AP Serednyakov, SI Skovpen, YI Solodov, EP Todyshev, KY Yushkov, AN Kirkby, D Lankford, AJ Mandelkern, M Dey, B Gary, JW Long, O Campagnari, C Sevilla, MF Hong, TM Kovalskyi, D Richman, JD West, CA Eisner, AM Lockman, WS Schumm, BA Seiden, A Chao, DS Cheng, CH Echenard, B Flood, KT Hitlin, DG Ongmongkolkul, P Porter, FC Andreassen, R Huard, Z Meadows, BT Pushpawela, BG Sokoloff, MD Sun, L Bloom, PC Ford, WT Gaz, A Nauenberg, U Smith, JG Wagner, SR Ayad, R Toki, WH Spaan, B Schwierz, R Bernard, D Verderi, M Playfer, S Bettoni, D Bozzi, C Calabrese, R Cibinetto, G Fioravanti, E Garzia, I Luppi, E Piemontese, L Santoro, V Baldini-Ferroli, R Calcaterra, A de Sangro, R Finocchiaro, G Martellotti, S Patteri, P Peruzzi, IM Piccolo, M Rama, M Zallo, A Contri, R Guido, E Lo Vetere, M Monge, MR Passaggio, S Patrignani, C Robutti, E Bhuyan, B Prasad, V Morii, M Adametz, A Uwer, U Lacker, HM Dauncey, PD Mallik, U Chen, C Cochran, J Meyer, WT Prell, S Ahmed, H Gritsan, AV Arnaud, N Davier, M Derkach, D Grosdidier, G Le Diberder, F Lutz, AM Malaescu, B Roudeau, P Stocchi, A Wormser, G Lange, DJ Wright, DM Coleman, JP Fry, JR Gabathuler, E Hutchcroft, DE Payne, DJ Touramanis, C Bevan, AJ Di Lodovico, F Sacco, R Cowan, G Bougher, J Brown, DN Davis, CL Denig, AG Fritsch, M Gradl, W Griessinger, K Hafner, A Prencipe, E Schubert, KR Barlow, RJ Lafferty, GD Behn, E Cenci, R Hamilton, B Jawahery, A Roberts, DA Cowan, R Dujmic, D Sciolla, G Cheaib, R Patel, PM Robertson, SH Biassoni, P Neri, N Palombo, F Cremaldi, L Godang, R Sonnek, P Summers, DJ Simard, M Taras, P De Nardo, G Monorchio, D Onorato, G Sciacca, C Martinelli, M Raven, G Jessop, CP LoSecco, JM Honscheid, K Kass, R Brau, J Frey, R Sinev, NB Strom, D Torrence, E Ahmed, H Feltresi, E Margoni, M Morandin, M Posocco, M Rotondo, M Simi, G Simonetto, F Stroili, R Akar, S Ben-Haim, E Bomben, M Bonneaud, GR Briand, H Calderini, G Chauveau, J Leruste, P Marchiori, G Ocariz, J Sitt, S Biasini, M Manoni, E Pacetti, S Rossi, A Angelini, C Batignani, G Bettarini, S Carpinelli, M Casarosa, G Cervelli, A Forti, F Giorgi, MA Lusiani, A Oberhof, B Paoloni, E Perez, A Rizzo, G Walsh, JJ Pegna, DL Olsen, J Smith, AJS Faccini, R Ferrarotto, F Ferroni, F Gaspero, M Gioi, LL Piredda, G Bunger, C Grunberg, O Hartmann, T Leddig, T Voss, C Waldi, R Adye, T Olaiya, EO Wilson, FF Emery, S de Monchenault, GH Vasseur, G Yeche, C Anulli, F Aston, D Bard, DJ Benitez, JF Cartaro, C Convery, MR Dorfan, J Dubois-Felsmann, GP Dunwoodie, W Ebert, M Field, RC Fulsom, BG Gabareen, AM Graham, MT Hast, C Innes, WR Kim, P Kocian, ML Leith, DWGS Lewis, P Lindemann, D Lindquist, B Luitz, S Luth, V Lynch, HL MacFarlane, DB Muller, DR Neal, H Nelson, S Perl, M Pulliam, T Ratcliff, BN Roodman, A Salnikov, AA Schindler, RH Snyder, A Su, D Sullivan, MK Va'vra, J Wagner, AP Wang, WF Wisniewski, WJ Wittgen, M Wright, DH Wulsin, HW Ziegler, V Park, W Purohit, MV White, RM Wilson, JR Randle-Conde, A Sekula, SJ Bellis, M Burchat, PR Miyashita, TS Puccio, EMT Alam, MS Ernst, JA Gorodeisky, R Guttman, N Peimer, DR Soffer, A Spanier, SM Ritchie, JL Ruland, AM Schwitters, RF Wray, BC Izen, JM Lou, XC Bianchi, F De Mori, F Filippi, A Gamba, D Zambito, S Lanceri, L Vitale, L Martinez-Vidal, F Oyanguren, A Villanueva-Perez, P Albert, J Banerjee, S Bernlochner, FU Choi, HHF King, GJ Kowalewski, R Lewczuk, MJ Lueck, T Nugent, IM Roney, JM Sobie, RJ Tasneem, N Gershon, TJ Harrison, PF Latham, TE Band, HR Dasu, S Pan, Y Prepost, R Wu, SL AF Lees, J. P. Poireau, V. Tisserand, V. Grauges, E. Palano, A. Eigen, G. Stugu, B. Brown, D. N. Kerth, L. T. Kolomensky, Yu. G. Lee, M. J. Lynch, G. Koch, H. Schroeder, T. Hearty, C. Mattison, T. S. McKenna, J. A. So, R. Y. Khan, A. Blinov, V. E. Buzykaev, A. R. Druzhinin, V. P. Golubev, V. B. Kravchenko, E. A. Onuchin, A. P. Serednyakov, S. I. Skovpen, Yu. I. Solodov, E. P. Todyshev, K. Yu. Yushkov, A. N. Kirkby, D. Lankford, A. J. Mandelkern, M. Dey, B. Gary, J. W. Long, O. Campagnari, C. Sevilla, M. Franco Hong, T. M. Kovalskyi, D. Richman, J. D. West, C. A. Eisner, A. M. Lockman, W. S. Schumm, B. A. Seiden, A. Chao, D. S. Cheng, C. H. Echenard, B. Flood, K. T. Hitlin, D. G. Ongmongkolkul, P. Porter, F. C. Andreassen, R. Huard, Z. Meadows, B. T. Pushpawela, B. G. Sokoloff, M. D. Sun, L. Bloom, P. C. Ford, W. T. Gaz, A. Nauenberg, U. Smith, J. G. Wagner, S. R. Ayad, R. Toki, W. H. Spaan, B. Schwierz, R. Bernard, D. Verderi, M. Playfer, S. Bettoni, D. Bozzi, C. Calabrese, R. Cibinetto, G. Fioravanti, E. Garzia, I. Luppi, E. Piemontese, L. Santoro, V. Baldini-Ferroli, R. Calcaterra, A. de Sangro, R. Finocchiaro, G. Martellotti, S. Patteri, P. Peruzzi, I. M. Piccolo, M. Rama, M. Zallo, A. Contri, R. Guido, E. Lo Vetere, M. Monge, M. R. Passaggio, S. Patrignani, C. Robutti, E. Bhuyan, B. Prasad, V. Morii, M. Adametz, A. Uwer, U. Lacker, H. M. Dauncey, P. D. Mallik, U. Chen, C. Cochran, J. Meyer, W. T. Prell, S. Ahmed, H. Gritsan, A. V. Arnaud, N. Davier, M. Derkach, D. Grosdidier, G. Le Diberder, F. Lutz, A. M. Malaescu, B. Roudeau, P. Stocchi, A. Wormser, G. Lange, D. J. Wright, D. M. Coleman, J. P. Fry, J. R. Gabathuler, E. Hutchcroft, D. E. Payne, D. J. Touramanis, C. Bevan, A. J. Di Lodovico, F. Sacco, R. Cowan, G. Bougher, J. Brown, D. N. Davis, C. L. Denig, A. G. Fritsch, M. Gradl, W. Griessinger, K. Hafner, A. Prencipe, E. Schubert, K. R. Barlow, R. J. Lafferty, G. D. Behn, E. Cenci, R. Hamilton, B. Jawahery, A. Roberts, D. A. Cowan, R. Dujmic, D. Sciolla, G. Cheaib, R. Patel, P. M. Robertson, S. H. Biassoni, P. Neri, N. Palombo, F. Cremaldi, L. Godang, R. Sonnek, P. Summers, D. J. Simard, M. Taras, P. De Nardo, G. Monorchio, D. Onorato, G. Sciacca, C. Martinelli, M. Raven, G. Jessop, C. P. LoSecco, J. M. Honscheid, K. Kass, R. Brau, J. Frey, R. Sinev, N. B. Strom, D. Torrence, E. Ahmed, H. Feltresi, E. Margoni, M. Morandin, M. Posocco, M. Rotondo, M. Simi, G. Simonetto, F. Stroili, R. Akar, S. Ben-Haim, E. Bomben, M. Bonneaud, G. R. Briand, H. Calderini, G. Chauveau, J. Leruste, Ph. Marchiori, G. Ocariz, J. Sitt, S. Biasini, M. Manoni, E. Pacetti, S. Rossi, A. Angelini, C. Batignani, G. Bettarini, S. Carpinelli, M. Casarosa, G. Cervelli, A. Forti, F. Giorgi, M. A. Lusiani, A. Oberhof, B. Paoloni, E. Perez, A. Rizzo, G. Walsh, J. J. Pegna, D. Lopes Olsen, J. Smith, A. J. S. Faccini, R. Ferrarotto, F. Ferroni, F. Gaspero, M. Gioi, L. Li Piredda, G. Buenger, C. Gruenberg, O. Hartmann, T. Leddig, T. Voss, C. Waldi, R. Adye, T. Olaiya, E. O. Wilson, F. F. Emery, S. de Monchenault, G. Hamel Vasseur, G. Yeche, Ch. Anulli, F. Aston, D. Bard, D. J. Benitez, J. F. Cartaro, C. Convery, M. R. Dorfan, J. Dubois-Felsmann, G. P. Dunwoodie, W. Ebert, M. Field, R. C. Fulsom, B. G. Gabareen, A. M. Graham, M. T. Hast, C. Innes, W. R. Kim, P. Kocian, M. L. Leith, D. W. G. S. Lewis, P. Lindemann, D. Lindquist, B. Luitz, S. Luth, V. Lynch, H. L. MacFarlane, D. B. Muller, D. R. Neal, H. Nelson, S. Perl, M. Pulliam, T. Ratcliff, B. N. Roodman, A. Salnikov, A. A. Schindler, R. H. Snyder, A. Su, D. Sullivan, M. K. Va'vra, J. Wagner, A. P. Wang, W. F. Wisniewski, W. J. Wittgen, M. Wright, D. H. Wulsin, H. W. Ziegler, V. Park, W. Purohit, M. V. White, R. M. Wilson, J. R. Randle-Conde, A. Sekula, S. J. Bellis, M. Burchat, P. R. Miyashita, T. S. Puccio, E. M. T. Alam, M. S. Ernst, J. A. Gorodeisky, R. Guttman, N. Peimer, D. R. Soffer, A. Spanier, S. M. Ritchie, J. L. Ruland, A. M. Schwitters, R. F. Wray, B. C. Izen, J. M. Lou, X. C. Bianchi, F. De Mori, F. Filippi, A. Gamba, D. Zambito, S. Lanceri, L. Vitale, L. Martinez-Vidal, F. Oyanguren, A. Villanueva-Perez, P. Albert, J. Banerjee, Sw. Bernlochner, F. U. Choi, H. H. F. King, G. J. Kowalewski, R. Lewczuk, M. J. Lueck, T. Nugent, I. M. Roney, J. M. Sobie, R. J. Tasneem, N. Gershon, T. J. Harrison, P. F. Latham, T. E. Band, H. R. Dasu, S. Pan, Y. Prepost, R. Wu, S. L. TI Measurements of direct CP asymmetries in B -> X-s gamma decays using sum of exclusive decays SO PHYSICAL REVIEW D LA English DT Article ID BABAR DETECTOR; PHYSICS AB We measure the direct CP violation asymmetry, A(CP), in B -> X-s gamma and the isospin difference of the asymmetry, Delta A(CP), using 429 fb(-1) of data collected at Upsilon(4S) resonance with the BABAR detector at the PEP- II asymmetric- energy e(+)e(-) storage rings operating at the SLAC National Accelerator Laboratory. B mesons are reconstructed from ten charged B final states and six neutral B final states. We find A(CP) = +(1.7 +/- 1.9 +/- 1.0)%, which is in agreement with the Standard Model prediction and provides an improvement on the world average. Moreover, we report the first measurement of the difference between A(CP) for charged and neutral decay modes, Delta A(CP) = +(5.0 +/- 3.9 +/- 1.5)%. Using the value of Delta A(CP), we also provide 68% and 90% confidence intervals on the imaginary part of the ratio of theWilson coefficients corresponding to the chromomagnetic dipole and the electromagnetic dipole transitions. C1 [Lees, J. P.; Poireau, V.; Tisserand, V.] Univ Savoie, CNRS, IN2P3, Lab Annecy Le Vieux Phys Particules, F-74941 Annecy Le Vieux, France. [Grauges, E.] Univ Barcelona, Fac Fis, Dept ECM, E-08028 Barcelona, Spain. [Palano, A.] Ist Nazl Fis Nucl, Sez Bari, I-70126 Bari, Italy. [Palano, A.] Univ Bari, Dipartmento Fis, I-70126 Bari, Italy. [Eigen, G.; Stugu, B.] Univ Bergen, Inst Phys, N-5007 Bergen, Norway. [Brown, D. N.; Kerth, L. T.; Kolomensky, Yu. G.; Lee, M. J.; Lynch, G.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Brown, D. N.; Kerth, L. T.; Kolomensky, Yu. G.; Lee, M. J.; Lynch, G.] Univ Calif Berkeley, Berkeley, CA 94720 USA. [Koch, H.; Schroeder, T.] Ruhr Univ Bochum, Inst Expt Phys 1, D-44780 Bochum, Germany. [Hearty, C.; Mattison, T. S.; McKenna, J. A.; So, R. Y.] Univ British Columbia, Vancouver, BC V6T 1Z1, Canada. [Khan, A.] Brunel Univ, Uxbridge UB8 3PH, Middx, England. [Blinov, V. E.; Buzykaev, A. R.; Druzhinin, V. P.; Golubev, V. B.; Kravchenko, E. A.; Onuchin, A. P.; Serednyakov, S. I.; Skovpen, Yu. I.; Solodov, E. P.; Todyshev, K. Yu.; Yushkov, A. N.] RAS, SB, Budker Inst Nucl Phys, Novosibirsk 630090, Russia. [Druzhinin, V. P.; Golubev, V. B.; Kravchenko, E. A.; Serednyakov, S. I.; Skovpen, Yu. I.; Solodov, E. P.; Todyshev, K. Yu.] Novosibirsk State Univ, Novosibirsk 630090, Russia. [Blinov, V. E.; Onuchin, A. P.] Novosibirsk State Tech Univ, Novosibirsk 630092, Russia. [Kirkby, D.; Lankford, A. J.; Mandelkern, M.] Univ Calif Irvine, Irvine, CA 92697 USA. [Dey, B.; Gary, J. W.; Long, O.] Univ Calif Riverside, Riverside, CA 92521 USA. [Campagnari, C.; Sevilla, M. Franco; Hong, T. M.; Kovalskyi, D.; Richman, J. D.; West, C. A.] Univ Calif Santa Barbara, Santa Barbara, CA 93106 USA. [Eisner, A. M.; Lockman, W. S.; Schumm, B. A.; Seiden, A.] Univ Calif Santa Cruz, Inst Particle Phys, Santa Cruz, CA 95064 USA. [Chao, D. S.; Cheng, C. H.; Echenard, B.; Flood, K. T.; Hitlin, D. G.; Ongmongkolkul, P.; Porter, F. C.] CALTECH, Pasadena, CA 91125 USA. [Andreassen, R.; Huard, Z.; Meadows, B. T.; Pushpawela, B. G.; Sokoloff, M. D.; Sun, L.] Univ Cincinnati, Cincinnati, OH 45221 USA. [Bloom, P. C.; Ford, W. T.; Gaz, A.; Nauenberg, U.; Smith, J. G.; Wagner, S. R.] Univ Colorado, Boulder, CO 80309 USA. [Ayad, R.; Toki, W. H.] Colorado State Univ, Ft Collins, CO 80523 USA. [Spaan, B.] Tech Univ Dortmund, Fak Phys, D-44221 Dortmund, Germany. [Schwierz, R.] Tech Univ Dresden, Inst Kern & Teilchenphys, D-01062 Dresden, Germany. [Bernard, D.] Ecole Polytech, CNRS, IN2P3, Lab Leprince Ringuet, F-91128 Palaiseau, France. [Playfer, S.] Univ Edinburgh, Edinburgh EH9 3JZ, Midlothian, Scotland. [Bettoni, D.; Bozzi, C.; Calabrese, R.; Cibinetto, G.; Fioravanti, E.; Garzia, I.; Luppi, E.; Piemontese, L.; Santoro, V.] Ist Nazl Fis Nucl, Sez Ferrara, I-44122 Ferrara, Italy. [Calabrese, R.; Cibinetto, G.; Fioravanti, E.; Garzia, I.; Luppi, E.] Univ Ferrara, Dipartimento Fis & Sci Terra, I-44122 Ferrara, Italy. [Baldini-Ferroli, R.; Calcaterra, A.; de Sangro, R.; Finocchiaro, G.; Martellotti, S.; Patteri, P.; Peruzzi, I. M.; Piccolo, M.; Rama, M.; Zallo, A.] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy. [Contri, R.; Guido, E.; Lo Vetere, M.; Monge, M. R.; Passaggio, S.; Patrignani, C.; Robutti, E.] Ist Nazl Fis Nucl, Sez Genova, I-16146 Genoa, Italy. [Contri, R.; Guido, E.; Lo Vetere, M.; Monge, M. R.; Patrignani, C.] Univ Genoa, Dipartimento Fis, I-16146 Genoa, Italy. [Bhuyan, B.; Prasad, V.] Indian Inst Technol Guwahati, Gauhati 781039, Assam, India. [Morii, M.] Harvard Univ, Cambridge, MA 02138 USA. [Adametz, A.; Uwer, U.] Heidelberg Univ, Inst Phys, D-69120 Heidelberg, Germany. [Lacker, H. M.] Humboldt Univ, Inst Phys, D-12489 Berlin, Germany. [Dauncey, P. D.] Univ London Imperial Coll Sci Technol & Med, London SW7 2AZ, England. [Mallik, U.] Univ Iowa, Iowa City, IA 52242 USA. [Chen, C.; Cochran, J.; Meyer, W. T.; Prell, S.] Iowa State Univ, Ames, IA 50011 USA. [Ahmed, H.] Jazan Univ, Jazan 22822, Saudi Arabia. [Gritsan, A. V.] Johns Hopkins Univ, Baltimore, MD 21218 USA. [Arnaud, N.; Davier, M.; Derkach, D.; Grosdidier, G.; Le Diberder, F.; Lutz, A. M.; Malaescu, B.; Roudeau, P.; Stocchi, A.; Wormser, G.] CNRS, IN2P3, Lab Accelerateur Lineaire, F-91898 Orsay, France. [Arnaud, N.; Davier, M.; Derkach, D.; Grosdidier, G.; Le Diberder, F.; Lutz, A. 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[Anulli, F.; Aston, D.; Bard, D. J.; Benitez, J. F.; Cartaro, C.; Convery, M. R.; Dorfan, J.; Dubois-Felsmann, G. P.; Dunwoodie, W.; Ebert, M.; Field, R. C.; Fulsom, B. G.; Gabareen, A. M.; Graham, M. T.; Hast, C.; Innes, W. R.; Kim, P.; Kocian, M. L.; Leith, D. W. G. S.; Lewis, P.; Lindemann, D.; Lindquist, B.; Luitz, S.; Luth, V.; Lynch, H. L.; MacFarlane, D. B.; Muller, D. R.; Neal, H.; Nelson, S.; Perl, M.; Pulliam, T.; Ratcliff, B. N.; Roodman, A.; Salnikov, A. A.; Schindler, R. H.; Snyder, A.; Su, D.; Sullivan, M. K.; Va'vra, J.; Wagner, A. P.; Wang, W. F.; Wisniewski, W. J.; Wittgen, M.; Wright, D. H.; Wulsin, H. W.; Ziegler, V.] Stanford Linear Accelerator Ctr, Natl Accelerator Lab, Stanford, CA 94309 USA. [Park, W.; Purohit, M. V.; White, R. M.; Wilson, J. R.] Univ S Carolina, Columbia, SC 29208 USA. [Randle-Conde, A.; Sekula, S. J.] So Methodist Univ, Dallas, TX 75275 USA. [Bellis, M.; Burchat, P. R.; Miyashita, T. S.; Puccio, E. M. T.] Stanford Univ, Stanford, CA 94305 USA. [Alam, M. S.; Ernst, J. A.] SUNY Albany, Albany, NY 12222 USA. [Gorodeisky, R.; Guttman, N.; Peimer, D. R.; Soffer, A.] Tel Aviv Univ, Sch Phys & Astron, IL-69978 Tel Aviv, Israel. [Spanier, S. M.] Univ Tennessee, Knoxville, TN 37996 USA. [Ritchie, J. L.; Ruland, A. M.; Schwitters, R. F.; Wray, B. C.] Univ Texas Austin, Austin, TX 78712 USA. [Izen, J. M.; Lou, X. C.] Univ Texas Dallas, Richardson, TX 75083 USA. [Bianchi, F.; De Mori, F.; Filippi, A.; Gamba, D.; Zambito, S.] Ist Nazl Fis Nucl, Sez Torino, I-10125 Turin, Italy. [Bianchi, F.; De Mori, F.; Gamba, D.; Zambito, S.] Univ Torino, Dipartimento Fis, I-10125 Turin, Italy. [Lanceri, L.; Vitale, L.] Ist Nazl Fis Nucl, Sez Trieste, I-34127 Trieste, Italy. [Lanceri, L.; Vitale, L.] Univ Trieste, Dipartimento Fis, I-34127 Trieste, Italy. [Martinez-Vidal, F.; Oyanguren, A.; Villanueva-Perez, P.] Univ Valencia, CSIC, IFIC, E-46071 Valencia, Spain. [Albert, J.; Banerjee, Sw.; Bernlochner, F. U.; Choi, H. H. F.; King, G. J.; Kowalewski, R.; Lewczuk, M. J.; Lueck, T.; Nugent, I. M.; Roney, J. M.; Sobie, R. J.; Tasneem, N.] Univ Victoria, Victoria, BC V8W 3P6, Canada. [Gershon, T. J.; Harrison, P. F.; Latham, T. E.] Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England. [Band, H. R.; Dasu, S.; Pan, Y.; Prepost, R.; Wu, S. L.] Univ Wisconsin, Madison, WI 53706 USA. [Godang, R.] Univ Sassari, I-07100 Sassari, Italy. RP Lees, JP (reprint author), Univ Savoie, CNRS, IN2P3, Lab Annecy Le Vieux Phys Particules, F-74941 Annecy Le Vieux, France. RI Oyanguren, Arantza/K-6454-2014; Monge, Maria Roberta/G-9127-2012; Lo Vetere, Maurizio/J-5049-2012; Patrignani, Claudia/C-5223-2009; Luppi, Eleonora/A-4902-2015; White, Ryan/E-2979-2015; Lusiani, Alberto/N-2976-2015; Calcaterra, Alessandro/P-5260-2015; Kravchenko, Evgeniy/F-5457-2015; Calabrese, Roberto/G-4405-2015; Kolomensky, Yury/I-3510-2015; Martinez Vidal, F*/L-7563-2014; Rizzo, Giuliana/A-8516-2015; Morandin, Mauro/A-3308-2016; Lusiani, Alberto/A-3329-2016; Di Lodovico, Francesca/L-9109-2016; Frey, Raymond/E-2830-2016; OI Oyanguren, Arantza/0000-0002-8240-7300; Monge, Maria Roberta/0000-0003-1633-3195; Lo Vetere, Maurizio/0000-0002-6520-4480; Patrignani, Claudia/0000-0002-5882-1747; Luppi, Eleonora/0000-0002-1072-5633; White, Ryan/0000-0003-3589-5900; Lusiani, Alberto/0000-0002-6876-3288; Calcaterra, Alessandro/0000-0003-2670-4826; Calabrese, Roberto/0000-0002-1354-5400; Kolomensky, Yury/0000-0001-8496-9975; Martinez Vidal, F*/0000-0001-6841-6035; Pacetti, Simone/0000-0002-6385-3508; Sciacca, Crisostomo/0000-0002-8412-4072; Rizzo, Giuliana/0000-0003-1788-2866; Faccini, Riccardo/0000-0003-2613-5141; Martinelli, Maurizio/0000-0003-4792-9178; Raven, Gerhard/0000-0002-2897-5323; Morandin, Mauro/0000-0003-4708-4240; Lusiani, Alberto/0000-0002-6876-3288; Di Lodovico, Francesca/0000-0003-3952-2175; Frey, Raymond/0000-0003-0341-2636; Paoloni, Eugenio/0000-0001-5969-8712; Bettarini, Stefano/0000-0001-7742-2998; Lanceri, Livio/0000-0001-8220-3095; Ebert, Marcus/0000-0002-3014-1512; Cibinetto, Gianluigi/0000-0002-3491-6231 FU U.S. Department of Energy and National Science Foundation; Natural Sciences and Engineering Research Council (Canada); Commissariat a l'Energie Atomique and Institut National de Physique Nucleaire et de Physique des Particules (France); Bundesministerium fur Bildung und Forschung and Deutsche Forschungsgemeinscha (Germany); Istituto Nazionale di Fisica Nucleare (Italy); Foundation for Fundamental Research on Matter (The Netherlands); Research Council of Norway; Ministry of Education and Science of the Russian Federation; Ministerio de Economia y Competitividad (Spain); Science and Technology Facilities Council (United Kingdom); Binational Science Foundation (U.S.-Israel); Marie-Curie IEF program (European Union); A. P. Sloan Foundation (USA) FX We would like to thank Gil Paz for very useful discussions. We are grateful for the extraordinary contributions of our PEP-II colleagues in achieving the excellent luminosity and machine conditions that have made this work possible. The success of this project also relies critically on the expertise and dedication of the computing organizations that support BABAR. The collaborating institutions wish to thank SLAC for its support and the kind hospitality extended to them. This work is supported by the U.S. Department of Energy and National Science Foundation, the Natural Sciences and Engineering Research Council (Canada), the Commissariat a l'Energie Atomique and Institut National de Physique Nucleaire et de Physique des Particules (France), the Bundesministerium fur Bildung und Forschung and Deutsche Forschungsgemeinschaft (Germany), the Istituto Nazionale di Fisica Nucleare (Italy), the Foundation for Fundamental Research on Matter (The Netherlands), the Research Council of Norway, the Ministry of Education and Science of the Russian Federation, Ministerio de Economia y Competitividad (Spain), the Science and Technology Facilities Council (United Kingdom), and the Binational Science Foundation (U.S.-Israel). Individuals have received support from the Marie-Curie IEF program (European Union) and the A. P. Sloan Foundation (USA). NR 27 TC 5 Z9 5 U1 0 U2 17 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1550-7998 EI 1550-2368 J9 PHYS REV D JI Phys. Rev. D PD NOV 5 PY 2014 VL 90 IS 9 AR 092001 DI 10.1103/PhysRevD.90.092001 PG 12 WC Astronomy & Astrophysics; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AT8HE UT WOS:000345173600001 ER PT J AU Schatschneider, B Mathers, RT Gee, RH Wonderling, NM AF Schatschneider, Bohdan Mathers, Robert T. Gee, Richard H. Wonderling, Nichole M. TI Exploration of the transition temperatures and crystal structure of highly crystalline poly(1,3-cyclohexadiene): An experimental and computational investigation SO POLYMER LA English DT Article DE Molecular dynamics; Polycyclohexadiene; DSC ID MOLECULAR-DYNAMICS SIMULATION; CONFORMATIONAL DYNAMICS; BLOCK-COPOLYMERS; POLYMER MELTS; MAIN-CHAIN; CATALYSTS; 1,3-CYCLOHEXADIENE; MICROSTRUCTURE; POLYETHYLENE; RELAXATION AB Experimental determination of transition temperatures for highly crystalline polymers such as poly-1,3-cyclohexadiene (PCHD) can be difficult due to reduced solubility and thermalization processes which occur during data acquisition. In order to facilitate further understanding of these processes for PCHD, density functional theory (DFT) and molecular dynamics (MD) were used in conjunction with differential scanning calorimetry (DSC) and powder X-ray diffraction (XRD) to explore the oligomer microstructures, the crystal structure, and the temperature dependence of the specific volume (1/rho). DFT geometry minimizations on isolated oligomers were used to identify the lowest energy confirmer; revealing that alternating R,R and S,S chiral bonds between monomer units afford the lowest energy structure. MD simulations of crystalline PCHD were constructed so as to replicate the experimental XRD pattern of crystalline PCHD, with the best fit producing a monoclinic crystal structure. The temperature dependence of the specific volume derived from MD simulations provided insight into the glass/vitrification T-g and melting (T-m) transition temperatures. Comparison of the simulation transition temperatures with differential scanning calorimetry data of PCHD polymerized with Ni(acac)(2)/MAO shows good agreement and solidifies the fidelity of the newly defined PCHD crystalline structure. (C) 2014 Elsevier Ltd. All rights reserved. C1 [Schatschneider, Bohdan] Penn State Univ, Dept Chem, Lemont Furnace, PA 15401 USA. [Mathers, Robert T.] Penn State Univ, Dept Chem, New Kensington, PA 15068 USA. [Gee, Richard H.] Lawrence Livermore Natl Lab, Livermore, CA 94551 USA. [Wonderling, Nichole M.] Penn State Univ, Mat Res Inst, University Pk, PA 16802 USA. RP Schatschneider, B (reprint author), Penn State Univ, Dept Chem, Eberly Campus, Lemont Furnace, PA 15401 USA. EM bxs54@psu.edu FU U.S. Department of Energy [DE-AC52-07NA27344]; Eberly Science Foundation; United Soybean Board FX This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344. B.S. would like to thank the Eberly Science Foundation for their support of this work. RTM thanks the United Soybean Board for financial support. NR 54 TC 0 Z9 0 U1 4 U2 23 PU ELSEVIER SCI LTD PI OXFORD PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, OXON, ENGLAND SN 0032-3861 EI 1873-2291 J9 POLYMER JI Polymer PD NOV 5 PY 2014 VL 55 IS 23 SI SI BP 6085 EP 6090 DI 10.1016/j.polymer.2014.09.055 PG 6 WC Polymer Science SC Polymer Science GA AU0JW UT WOS:000345310100029 ER PT J AU Appy, D Lei, HP Han, Y Wang, CZ Tringides, MC Shao, DH Kwolek, EJ Evans, JW Thiel, PA AF Appy, David Lei, Huaping Han, Yong Wang, Cai-Zhuang Tringides, Michael C. Shao, Dahai Kwolek, Emma J. Evans, J. W. Thiel, P. A. TI Determining whether metals nucleate homogeneously on graphite: A case study with copper SO PHYSICAL REVIEW B LA English DT Article ID ORIENTED PYROLYTIC-GRAPHITE; SURFACE-DEFECTS; GROWTH; HOPG; DEPOSITION; MORPHOLOGY; PARTICLES; DENSITY; ENERGY; PLANE AB We observe that Cu clusters grow on surface terraces of graphite as a result of physical vapor deposition in ultrahigh vacuum. We show that the observation is incompatible with a variety of models incorporating homogeneous nucleation and calculations of atomic-scale energetics. An alternative explanation, ion-mediated heterogeneous nucleation, is proposed and validated, both with theory and experiment. This serves as a case study in identifying when and whether the simple, common observation of metal clusters on carbon-rich surfaces can be interpreted in terms of homogeneous nucleation. We describe a general approach for making system-specific and laboratory-specific predictions. C1 [Appy, David; Lei, Huaping; Han, Yong; Wang, Cai-Zhuang; Tringides, Michael C.; Shao, Dahai; Evans, J. W.; Thiel, P. A.] Ames Lab, Ames, IA 50011 USA. [Appy, David; Shao, Dahai; Kwolek, Emma J.; Thiel, P. A.] Iowa State Univ, Dept Chem, Ames, IA 50011 USA. [Lei, Huaping; Han, Yong; Tringides, Michael C.; Evans, J. W.] Iowa State Univ, Dept Phys & Astron, Ames, IA 50011 USA. [Thiel, P. A.] Iowa State Univ, Dept Mat Sci & Engn, Ames, IA 50011 USA. RP Thiel, PA (reprint author), Ames Lab, Ames, IA 50011 USA. EM thiel@ameslab.gov FU Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division of the US Department of Energy (USDOE) [DE-AC02-07CH11358]; US Department of Energy; NSF [CHE-1111500] FX The experimental and DFT components of this work were supported by the Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division of the US Department of Energy (USDOE), under Contract No. DE-AC02-07CH11358 with the US Department of Energy. Y.H. and J.W.E. were supported by NSF Grant CHE-1111500 for modeling and KMC simulation. We thank R. S. Houk, A. Schmid, and M. Schmid for useful insights, and J. Anderegg for HOPG samples. NR 34 TC 6 Z9 6 U1 1 U2 22 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1098-0121 EI 1550-235X J9 PHYS REV B JI Phys. Rev. B PD NOV 5 PY 2014 VL 90 IS 19 AR 195406 DI 10.1103/PhysRevB.90.195406 PG 6 WC Physics, Condensed Matter SC Physics GA AT8GC UT WOS:000345170900006 ER PT J AU Shi, HL Du, MH AF Shi, Hongliang Du, Mao-Hua TI Shallow halogen vacancies in halide optoelectronic materials SO PHYSICAL REVIEW B LA English DT Article ID PEROVSKITE SOLAR-CELLS; AUGMENTED-WAVE METHOD; X-RAY; THALLIUM; DETECTORS; TRANSPORT; CRYSTALS; LENGTHS AB Halogen vacancies (V-H) are usually deep color centers (F centers) in halides and can act as major electron traps or recombination centers. The deep V-H contributes to the typically poor carrier transport properties in halides. However, several halides have recently emerged as excellent optoelectronic materials, e. g., CH3NH3PbI3 and TlBr. Both CH3NH3PbI3 and TlBr have been found to have shallow V-H, in contrast to commonly seen deep V-H in halides. In this paper, several halide optoelectronic materials, i.e., CH3NH3PbI3, CH3NH3SnI3 (photovoltaic materials), TlBr, and CsPbBr3 (gamma-ray detection materials) are studied to understand the material chemistry and structure that determine whether V-H is a shallow or deep defect in a halide material. It is found that crystal structure and chemistry of ns(2) ions both play important roles in creating shallow V-H in halides such as CH3NH3PbI3, CH3NH3SnI3, and TlBr. The key to identifying halides with shallow V-H is to find the right crystal structures and compounds that suppress cation orbital hybridization at V-H, such as those with large cation-cation distances and low anion coordination numbers and those with crystal symmetry that prevents strong hybridization of cation dangling bond orbitals at V-H. The results of this paper provide insight and guidance to identifying halides with shallow V-H as good electronic and optoelectronic materials. C1 [Du, Mao-Hua] Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37831 USA. Oak Ridge Natl Lab, Ctr Radiat Detect Mat & Syst, Oak Ridge, TN 37831 USA. RP Du, MH (reprint author), Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37831 USA. EM mhdu@ornl.gov RI Shi, Hongliang/A-7568-2010; Du, Mao-Hua/B-2108-2010 OI Shi, Hongliang/0000-0003-0713-4688; Du, Mao-Hua/0000-0001-8796-167X FU Department of Homeland Security, Domestic Nuclear Detection Office [HSHQDC-14-R-B0009] FX Work on halide perovskites was supported by the Department of Energy, Basic Energy Sciences, Materials Sciences and Engineering Division, while work on halides for radiation detection was supported by the Department of Homeland Security, Domestic Nuclear Detection Office (Grant No. HSHQDC-14-R-B0009). NR 45 TC 16 Z9 16 U1 13 U2 83 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 2469-9950 EI 2469-9969 J9 PHYS REV B JI Phys. Rev. B PD NOV 5 PY 2014 VL 90 IS 17 AR 174103 DI 10.1103/PhysRevB.90.174103 PG 6 WC Physics, Condensed Matter SC Physics GA AT8FU UT WOS:000345170200002 ER PT J AU Sreedhar, B Hobbs, DT Kawajiri, Y AF Sreedhar, Balamurali Hobbs, David T. Kawajiri, Yoshiaki TI Simulated moving bed chromatography designs for lanthanide and actinide separations using Reillex HPQ (TM) resin SO SEPARATION AND PURIFICATION TECHNOLOGY LA English DT Article DE Actinide; Lanthanide; Simulated moving bed; Chromatography; Modeling; Nuclear fuel ID CATION-EXCHANGE CHROMATOGRAPHY; SPENT NUCLEAR-FUELS; ANION-EXCHANGE; EXTRACTION CHROMATOGRAPHY; MINOR ACTINIDES; OPTIMIZATION; AMERICIUM; HPQ AB In this work, we investigated simulated moving bed (SMB) chromatography designs for purifying lanthanides (Ln) and actinides (An). SMB is a technique where chromatographic columns are arranged in a semi-closed-loop manner to separate feed into two product streams efficiently with minimal use of the eluent. Using neodymium (Nd) and samarium (Sm) as representative Ln elements and surrogates for minor actinides such as americium (Am) and curium (Cm), we investigated SMB designs with the Reillex HPQ.im resin. Using a chromatographic column packed with the resin, model parameters for the SMB design were obtained from the UV-VIS responses of pulse injections of the pure components. The mobile phase used was 0.5-3.0 M nitric acid. A mathematical model based optimization was used to theoretically predict the optimal purification rates for an equimolar mixture of the two components resulting in product purities of up to 99.5%. (C) 2014 Elsevier B.V. All rights reserved. C1 [Sreedhar, Balamurali; Kawajiri, Yoshiaki] Georgia Inst Technol, Sch Chem & Biomol Engn, Atlanta, GA 30332 USA. [Hobbs, David T.] Savannah River Natl Lab, Aiken, SC USA. RP Kawajiri, Y (reprint author), Georgia Inst Technol, Sch Chem & Biomol Engn, Atlanta, GA 30332 USA. EM ykawajiri@chbe.gatech.edu FU Strategic Energy Institute at Georgia Institute of Technology FX We greatly acknowledge the financial support from the Strategic Energy Institute at Georgia Institute of Technology. We would also like to thank Dr. Thomas Shehee and Dr. William Wilmarth of Savannah River National Laboratory for fruitful discussions. NR 43 TC 0 Z9 0 U1 3 U2 22 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 1383-5866 EI 1873-3794 J9 SEP PURIF TECHNOL JI Sep. Purif. Technol. PD NOV 5 PY 2014 VL 136 BP 50 EP 57 DI 10.1016/j.seppur.2014.08.006 PG 8 WC Engineering, Chemical SC Engineering GA AT3JJ UT WOS:000344831100007 ER PT J AU Cohen, T D'Agnolo, RT Hance, M Lou, HK Wacker, JG AF Cohen, Timothy D'Agnolo, Raffaele Tito Hance, Mike Lou, Hou Keong Wacker, Jay G. TI Boosting stop searches with a 100 TeV proton collider SO JOURNAL OF HIGH ENERGY PHYSICS LA English DT Article DE Hadronic Colliders ID SUPERSYMMETRY BREAKING AB A proton-proton collider with center of mass energy around 100TeV is the energy frontier machine that is likely to succeed the LHC. One of the primary physics goals will be the continued exploration of weak scale naturalness. Here we focus on the pair-production of stops that decay to a top and a neutralino. Most of the heavy stop parameter space results in highly boosted tops, populating kinematic regimes inaccessible at the LHC. New strategies for boosted top-tagging are needed and a simple, detector-independent tagger can be constructed by requiring a muon inside a jet. Assuming 20% systematic uncertainties, this future collider can discover (exclude) stops with masses up to 5.5 (8) TeV with 3000 fb(-1) of integrated luminosity. Studying how the exclusion limits scale with luminosity motivates going beyond this benchmark in order to saturate the discovery potential of the machine. C1 [Cohen, Timothy] SLAC Natl Accelerator Lab, Theory Grp, Menlo Pk, CA 94025 USA. [D'Agnolo, Raffaele Tito] Inst Adv Study, Sch Nat Sci, Princeton, NJ 08540 USA. [Hance, Mike] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Lou, Hou Keong] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA. [Wacker, Jay G.] Quora, Mountain View, CA 94041 USA. [Wacker, Jay G.] Stanford Univ, Stanford Inst Theoret Phhys, Dept Phys, Stanford, CA 94305 USA. RP Cohen, T (reprint author), SLAC Natl Accelerator Lab, Theory Grp, Menlo Pk, CA 94025 USA. EM timcohen@slac.stanford.edu; dagnolo@ias.edu; mhance@lbl.gov; hlou@princeton.edu; jay@quora.com FU DoE [DE-AC02-76SF00515, DE-AC02-05CH11231]; NSF [NSF PHY11-25915, PHY-0907744]; DOE SCG Fellowship FX We thank Nima Arkani-Hamed, Andy Haas, Stephanie Majewski, Gigi Rolandi, Maurizio Pierini, Michele Selvaggi, Anyes Taffard, Daniel Whiteson. We thank Christoph Borschensky, Michael Kranmer and Tilman Plehn for providing the NLL + NLO stop production cross sections. TC is supported by DoE contract number DE-AC02-76SF00515 and in part by the NSF grant NSF PHY11-25915. RTD is supported by the NSF grant PHY-0907744. MH is supported by DoE contract number DE-AC02-05CH11231. HKL is supported by the DOE SCG Fellowship. NR 68 TC 18 Z9 18 U1 0 U2 0 PU SPRINGER PI NEW YORK PA 233 SPRING ST, NEW YORK, NY 10013 USA SN 1029-8479 J9 J HIGH ENERGY PHYS JI J. High Energy Phys. PD NOV 5 PY 2014 IS 11 AR 021 DI 10.1007/JHEP11(2014)021 PG 19 WC Physics, Particles & Fields SC Physics GA AT3WO UT WOS:000344864700001 ER PT J AU Papucci, M Vichi, A Zurek, KM AF Papucci, Michele Vichi, Alessandro Zurek, Kathryn M. TI Monojet versus the rest of the world I: t-channel SO JOURNAL OF HIGH ENERGY PHYSICS LA English DT Article DE Exotics; Hadron-Hadron Scattering; Particle and resonance production ID DARK-MATTER; SUPERLIGHT GRAVITINO; HADRON COLLIDERS; LHC; SIGNALS AB Monojet searches using Effective Field Theory (EFT) operators are usually interpreted as a robust and model independent constraint on direct detection (DD) scattering cross-sections. At the same time, a mediator particle must be present to produce the dark matter (DM) at the LHC. This mediator particle may be produced on shell, so that direct searches for the mediating particle can constrain the effective operator being applied to monojet constraints. In this first paper, we do a case study on t-channel models in monojet searches, where the (Standard Model singlet) DM is pair produced via a t-channel mediating particle, whose supersymmetric analogue is the squark. We compare monojet constraints to direct constraints on single or pair production of the mediator from multi-jets plus missing energy searches and we identify the regions where the latter dominate over the former. We show that computing bounds using supersymmetric simplified models and in the narrow width approximation, as done in previous work in the literature, misses important quantitative effects. We perform a full event simulation and statistical analysis, and we compute the effects of both on-and off-shell production of the mediating particle, showing that for both the monojet and multi-jets plus missing energy searches, previously derived bounds provided more conservative bounds than what can be extracted by including all relevant processes in the simulation. Monojets and searches for super-symmetry (SUSY) provide comparable bounds on a wide range of the parameter space, with SUSY searches usually providing stronger bounds, except in the regions where the DM particle and the mediator are very mass degenerate. The EFT approximation rarely is able to reproduce the actual limits. In a second paper to follow, we consider the case of s-channel mediators. C1 [Papucci, Michele; Zurek, Kathryn M.] Univ Michigan, Michigan Ctr Theoret Phys, Ann Arbor, MI 48109 USA. [Vichi, Alessandro] Univ Calif Berkeley, Berkeley Ctr Theoret Phys, Berkeley, CA 94720 USA. [Vichi, Alessandro] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Theoret Phys Grp, Berkeley, CA 94720 USA. RP Papucci, M (reprint author), Univ Michigan, Michigan Ctr Theoret Phys, Ann Arbor, MI 48109 USA. EM mpapucci@umich.edu; avichi@lbl.gov; kzurek@umich.edu FU Office of Science of the U.S. Department of Energy [DE-AC02-05CH1123]; NSF CAREER [PHY 1049896] FX We would like to thank S. Alioli for helpful discussions. This research used resources of the National Energy Research Scientific Computing Center, which is supported, as the work of AV, by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH1123. KZ is supported by NSF CAREER award PHY 1049896. MP would like to thank the CERN TH group for its warm hospitality, and MP and KZ would like to thank the Aspen Center for Physics where part of this work was completed. NR 52 TC 33 Z9 33 U1 1 U2 2 PU SPRINGER PI NEW YORK PA 233 SPRING ST, NEW YORK, NY 10013 USA SN 1029-8479 J9 J HIGH ENERGY PHYS JI J. High Energy Phys. PD NOV 5 PY 2014 IS 11 AR 024 DI 10.1007/JHEP11(2014)024 PG 26 WC Physics, Particles & Fields SC Physics GA AT2TH UT WOS:000344788500003 ER PT J AU Doris, SE Lynch, JJ Li, CY Wills, AW Urban, JJ Helms, BA AF Doris, Sean E. Lynch, Jared J. Li, Changyi Wills, Andrew W. Urban, Jeffrey J. Helms, Brett A. TI Mechanistic Insight into the Formation of Cationic Naked Nanocrystals Generated under Equilibrium Control SO JOURNAL OF THE AMERICAN CHEMICAL SOCIETY LA English DT Article ID FIELD-EFFECT TRANSISTORS; ATOMIC-LIGAND PASSIVATION; QUANTUM-DOT SOLIDS; COLLOIDAL NANOCRYSTALS; SURFACE-CHEMISTRY; CDSE NANOCRYSTALS; PBSE NANOCRYSTALS; ELECTRONIC TRANSPORT; MESOPOROUS MATERIALS; CHARGE-TRANSPORT AB Cationic naked nanocrystals (NCs) are useful building units for assembling hierarchical mesostructured materials. Until now, their preparation required strongly electrophilic reagents that irreversibly sever bonds between native organic ligands and the NC surface. Colloidal instabilities can occur during ligand stripping if exposed metal cations desorb from the surface. We hypothesized that cation desorption could be avoided were we able to stabilize the surface during ligand stripping via ion pairing. We were successful in this regard by carrying out ligand stripping under equilibrium control with Lewis acidbase adducts of BF3. To better understand the microscopic processes involved, we studied the reaction pathway in detail using in situ NMR experiments and electrospray ionization mass spectrometry. As predicted, we found that cationic NC surfaces are transiently stabilized post-stripping by physisorbed anionic species that arise from the reaction of BF3 with native ligands. This stabilization allows polar dispersants to reach the NC surface before cation desorption can occur. The mechanistic insights gained in this work provide a much-needed framework for understanding the interplay between NC surface chemistry and colloidal stability. These insights enabled the preparation of stable naked NC inks of desorption-susceptible NC compositions such as PbSe, which were easily assembled into new mesostructured films and polymer-nanocrystal composites with wide-ranging technological applications. C1 [Doris, Sean E.; Lynch, Jared J.; Li, Changyi; Wills, Andrew W.; Urban, Jeffrey J.; Helms, Brett A.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Mol Foundry, Berkeley, CA 94720 USA. [Doris, Sean E.] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA. [Li, Changyi] Univ Calif Berkeley, Dept Chem & Biomol Engn, Berkeley, CA 94720 USA. RP Helms, BA (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Mol Foundry, One Cyclotron Rd, Berkeley, CA 94720 USA. EM bahelms@lbl.gov RI Foundry, Molecular/G-9968-2014; OI Doris, Sean/0000-0002-4285-7999; Helms, Brett/0000-0003-3925-4174 FU Joint Center for Energy Storage Research, an Energy Innovation Hub - U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences; Department of Defense through the National Defense Science & Engineering Graduate Fellowship program; AFOSR MURI [FA9550-12-1-0002]; Office of Science, Office of Basic Energy Sciences, of the U.S. Department of Energy [DE-AC02-05CH11231] FX We thank N. Su and T. Williams for supplying Ni nanocrystals and block copolymer architecture-directing agents, respectively, A. Hexemer for assistance with GISAXS, P. Frischmann for assistance with ESI-MS, and L. Gerber for helpful discussions. All work with PbSe, TiO2, ZnO, and Mn3O4 was performed by S.E.D, C.L., A.W.W., and B.A.H.. C.L. and B.A.H. were supported by the Joint Center for Energy Storage Research, an Energy Innovation Hub funded by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences. S.E.D. was supported by the Department of Defense through the National Defense Science & Engineering Graduate Fellowship program. J.J.L. and J.J.U. carried out all experiments with Ni and Cu1.7Se, acknowledging support from the AFOSR MURI program under FA9550-12-1-0002. Portions of the work-including nanocrystal synthesis, characterization, and chemical transformations thereof were carried out as User Projects at the Molecular Foundry, which is supported by the Office of Science, Office of Basic Energy Sciences, of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. GISAXS was carried out at Beamline 7.3.3 of the Advanced Light Source, which is supported by the Director of the Office of Science, Office of Basic Energy Sciences, of the U.S. Department of Energy under the same contract. NR 73 TC 17 Z9 17 U1 2 U2 61 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0002-7863 J9 J AM CHEM SOC JI J. Am. Chem. Soc. PD NOV 5 PY 2014 VL 136 IS 44 BP 15702 EP 15710 DI 10.1021/ja508675T PG 9 WC Chemistry, Multidisciplinary SC Chemistry GA AS8RT UT WOS:000344516600042 PM 25302526 ER PT J AU Marshall, MSJ Malashevich, A Disa, AS Han, MG Chen, HH Zhu, YM Ismail-Beigi, S Walker, FJ Ahn, CH AF Marshall, Matthew S. J. Malashevich, Andrei Disa, Ankit S. Han, Myung-Geun Chen, Hanghui Zhu, Yimei Ismail-Beigi, Sohrab Walker, Frederick J. Ahn, Charles H. TI Conduction at a Ferroelectric Interface SO PHYSICAL REVIEW APPLIED LA English DT Article ID WANNIER FUNCTIONS; METAL; ENHANCEMENT; TRANSITION; SYSTEMS AB Typical logic elements utilizing the field effect rely on the change in carrier concentration due to the field in the channel region of the device. Ferroelectric-field-effect devices provide a nonvolatile version of this effect due to the stable polarization order parameter in the ferroelectric. In this work, we describe an oxide/oxide ferroelectric heterostructure device based on (001)-oriented PbZr0.2Ti0.8O3-LaNiO3 where the dominant change in conductivity is a result of a significant mobility change in the interfacial channel region. The effect is confined to a few atomic layers at the interface and is reversible by switching the ferroelectric polarization. More interestingly, in one polarization state, the field effect induces a 1.7-eV shift of the interfacial bands to create a new conducting channel in the interfacial PbO layer of the ferroelectric. C1 [Marshall, Matthew S. J.; Malashevich, Andrei; Disa, Ankit S.; Chen, Hanghui; Ismail-Beigi, Sohrab; Walker, Frederick J.; Ahn, Charles H.] Yale Univ, CRISP, New Haven, CT 06520 USA. [Marshall, Matthew S. J.; Malashevich, Andrei; Disa, Ankit S.; Chen, Hanghui; Ismail-Beigi, Sohrab; Walker, Frederick J.; Ahn, Charles H.] Yale Univ, Dept Appl Phys, New Haven, CT 06520 USA. [Han, Myung-Geun; Zhu, Yimei] Brookhaven Natl Lab, Condensed Matter Phys & Mat Sci Dept, Upton, NY 11973 USA. [Ahn, Charles H.] Yale Univ, Dept Mech Engn & Mat Sci, New Haven, CT 06520 USA. RP Marshall, MSJ (reprint author), Yale Univ, CRISP, New Haven, CT 06520 USA. EM charles.ahn@yale.edu RI Ismail-Beigi, Sohrab/F-2382-2014; OI Ismail-Beigi, Sohrab/0000-0002-7331-9624; Disa, Ankit/0000-0002-7762-3244; Walker, Frederick/0000-0002-8094-249X FU Office of Naval Research; NSF [DMR 1119826, CNS 08-21132]; NSF XSEDE [TG-MCA08X007]; U.S. Department of Energy, Office of Basic Energy Sciences Division of Materials Science and Engineering [DE-AC02-98CH10886] FX Work at Yale is supported by the Office of Naval Research and NSF DMR 1119826 (CRISP). Computational facilities were supported by NSF Grant No. CNS 08-21132, by the facilities and staff of the Yale University Faculty of Arts and Sciences High Performance Computing Center, and by the NSF XSEDE resources through Grant No. TG-MCA08X007. Work at the Condensed Matter Physics & Materials Science Department, Brookhaven National Laboratory is supported by the U.S. Department of Energy, Office of Basic Energy Sciences Division of Materials Science and Engineering, under Contract No. DE-AC02-98CH10886. TEM sample preparation was performed at the Center for Functional Nanomaterials, Brookhaven National Laboratory. The authors thank Eric Altman and Divine Kumah for helpful discussions. NR 34 TC 12 Z9 12 U1 2 U2 40 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 2331-7019 J9 PHYS REV APPL JI Phys. Rev. Appl. PD NOV 5 PY 2014 VL 2 IS 5 AR 051001 DI 10.1103/PhysRevApplied.2.051001 PG 6 WC Physics, Applied SC Physics GA AS5ZF UT WOS:000344344200001 ER PT J AU Aad, G Abajyan, T Abbott, B Abdallah, J Khalek, SA Abdinov, O Aben, R Abi, B Abolins, M AbouZeid, OS Abramowicz, H Abreu, H Abulaitia, Y Acharya, BS Adamczyk, L Adams, DL Addy, TN Adelman, J Adomeit, S Adye, T Agatonovic-Jovin, T Aguilar-Saavedra, JA Agustoni, M Ahlen, SP Ahmadov, F Aielli, G Akesson, TP Akimoto, G Akimov, AV Albert, J Albrand, S Verzini, MJA Aleksa, M Aleksandrov, IN Alexa, C Alexander, G Alexandre, G Alexopoulos, T Alhroob, M Alimonti, G Alio, L Alison, J Allbrooke, BMM Allison, LJ Allport, PP Allwood-Spiers, SE Almond, J Aloisio, A Alon, R Alonso, A Alonso, F Alpigiani, C Altheimer, A Gonzalez, BA Alviggi, MG Amako, K Coutinho, YA Amelung, C Ammosov, VV Dos Santos, SPA Amorim, A Amoroso, S Amram, N Amundsen, G Anastopoulos, C Ancu, LS Andari, N Andeen, T Anders, CF Anders, G Anderson, KJ Andreazza, A Andrei, V Anduaga, XS Angelidakis, S Anger, P Angerami, A Anghinolfi, F Anisenkov, AV Anjos, N Annovi, A Antonaki, A Antonelli, M Antonov, A Antos, J Anulli, F Aoki, M Bella, LA Apolle, R Arabidze, G Aracena, I Arai, Y Arce, ATH Arguin, JF Argyropoulos, S Arik, E Arik, M Armbruster, AJ Arnaez, O Arnal, V Arslan, O Artamonov, A Artoni, G Asai, S Asbah, N Ask, S Asman, B Asquith, L Assamagan, K Astalos, R Astbury, A Atkinson, M Atlay, NB Auerbach, B Auge, E Augsten, K Aurousseau, M Avolio, G Azuelos, G Azuma, Y Baak, MA Bacci, C Bach, AM Bachacou, H Bachas, K Backes, M Backhaus, M Mayes, JB Badescua, E Bagiacchi, P Bagnaia, P Bai, Y Bailey, DC Bain, T Baines, JT Baker, OK Baker, S Balek, P Balli, F Banas, E Banerjee, S Bangert, A Bansal, V Bansil, HS Barak, L Baranov, SP Barber, T Barberio, EL Barberis, D Barbero, M Barillari, T Barisonzi, M Barklow, T Barlow, N Barnett, BM Barnett, RM Baroncelli, A Barone, G Barr, AJ Barreiro, F Da Costa, JBG Bartoldus, R Barton, AE Bartos, P Bartsch, V Bassalat, A Basye, A Bates, RL Batkova, L Batley, JR Battistin, M Bauer, F Bawa, HS Beau, T Beauchemin, PH Beccherle, R Bechtle, P Beck, HP Becker, K Becker, S Beckingham, M Beddall, AJ Beddall, A Bedikian, S Bednyakov, VA Bee, CP Beemster, LJ Beermann, TA Begel, M Behr, K Belanger-Champagne, C Bell, PJ Bell, WH Bella, G Bellagamba, L Bellerive, A Bellomo, M Belloni, A Belotskiy, K Beltramello, O Benary, O Benchekroun, D Bendtz, K Benekos, N Benhammou, Y Noccioli, EB Garcia, JAB Benjamin, DP Bensinger, JR Benslama, K Bentvelsen, S Berge, D Kuutmann, EB Berger, N Berghaus, F Berglund, E Beringer, J Bernard, C Bernat, P Bernius, C Bernlochner, FU Berry, T Berta, P Bertella, C Bertolucci, F Besana, MI Besjes, GJ Bessidskaia, O Besson, N Betancourt, C Bethke, S Bhimji, W Bianchi, RM Bianchini, L Bianco, M Biebel, O Bieniek, SP Bierwagen, K Biesiada, J Biglietti, M De Mendizabal, JB Bilokon, H Bindi, M Binet, S Bingul, A Bini, C Black, CW Black, JE Black, KM Blackburn, D Blair, RE Blanchard, JB Blazeka, T Bloch, I Blocker, C Blum, W Blumenschein, U Bobbink, GJ Bobrovnikov, VS Bocchetta, SS Bocci, A Boddy, CR Boehler, M Boek, J Boek, TT Bogaerts, JA Bogdanchikov, AG Bogouch, A Bohm, C Bohm, J Boisvert, V Bold, T Boldea, V Boldyrev, AS Bolnet, NM Bomben, M Bona, M Boonekamp, M Borisov, A Borissov, G Borri, M Borroni, S Bortfeldt, J Bortolotto, V Bos, K Boscherini, D Bosman, M Boterenbrood, H Boudreau, J Bouffard, J Bouhova-Thacker, EV Boumediene, D Bourdarios, C Bousson, N Boutouil, S Boveia, A Boyd, J Boyko, IR Bozovic-Jelisavcic, I Bracinik, J Branchini, P Brandt, A Brandt, G Brandta, O Bratzler, U Brau, B Brau, JE Braun, HM Brazzale, SF Brelier, B Brendlinger, K Brennan, AJ Brenner, R Bressler, S Bristow, K Bristow, TM Britton, D Brochu, FM Brock, I Brock, R Bromberg, C Bronner, J Brooijmans, G Brooks, T Brooks, WK Brosamer, J Brost, E Brown, G Brown, J de Renstrom, PAB Bruncko, D Bruneliere, R Brunet, S Bruni, A Bruni, G Bruschi, M Bryngemark, L Buanes, T Buat, Q Bucci, F Buchholz, P Buckingham, RM Buckley, AG Buda, SI Budagov, IA Buehrer, F Bugge, L Bugge, MK Bulekov, O Bundock, AC Burckhart, H Burdin, S Burghgrave, B Burke, S Burmeister, I Busato, E Buscher, V Bussey, P Buszello, CP Butler, B Butler, JM Butt, AI Buttar, CM Butterworth, JM Buttinger, W Buzatu, A Byszewski, M Urban, SC Caforio, D Cakir, O Calafiura, P Calderini, G Calfayan, P Calkins, R Caloba, LP Caloi, R Calvet, D Calvet, S Toro, RC Cameron, D Caminada, LM Armadans, RC Campana, S Campanelli, M Campoverde, A Canale, V Canelli, F Canepa, A Cantero, J Cantrill, R Cao, T Garrido, MDMC Caprini, I Caprini, M Capua, M Caputo, R Cardarelli, R Carli, T Carlino, G Carminati, L Caron, S Carquin, E Carrillo-Montoya, GD Carter, JR Carvalho, J Casadei, D Casado, MP Castaneda-Miranda, E Castelli, A Gimenez, VC Castro, NF Catastini, P Catinaccio, A Catmore, JR Cattai, A Cattani, G Caughron, S Cavaliere, V Cavalli, D Cavalli-Sforza, M Cavasinni, V Ceradini, F Cerio, B Cerny, K Cerqueira, AS Cerri, A Cerrito, L Cerutti, F Cerv, M Cervelli, A Cetin, SA Chafaq, A Chakraborty, D Chalupkova, I Chan, K Chang, P Chapleau, B Chapman, JD Charfeddine, D Charlton, DG Barajas, CAC Cheatham, S Chekanov, S Chekulaev, SV Chelkov, GA Chelstowska, MA Chen, C Chen, H Chen, K Chen, L Chen, S Chen, X Chen, Y Cheng, HC Cheng, Y Cheplakov, A El Moursli, R El Moursli, A Chernyatin, V Cheu, E Chevalier, L Chiarella, V Chiefari, G Childers, JT Chilingarov, A Chiodini, G Chisholm, AS Chislett, RT Chitan, A Chizhov, MV Chouridou, S Chow, BKB Christidi, IA Chromek-Burckhart, D Chu, ML Chudoba, J Ciapetti, G Ciftci, AK Ciftci, R Cinca, D Cindro, V Ciocio, A Cirkovic, P Citron, ZH Citterio, M Ciubancan, M Clark, A Clark, PJ Clarke, RN Cleland, W Clemens, JC Clement, B Clement, C Coadou, Y Cobal, M Coccaro, A Cochran, J Coffey, L Cogan, JG Coggeshall, J Cole, B Cole, S Colijn, AP Collins-Tooth, C Collot, J Colombo, T Colon, G Compostella, G Muino, PC Coniavitis, E Conidi, MC Connelly, IA Consonni, SM Consorti, V Constantinescu, S Conta, C Conti, G Conventi, F Cooke, M Cooper, BD Cooper-Sarkar, AM Cooper-Smith, NJ Copic, K Cornelissen, T Corradi, M Corriveau, F Corso-Radu, A Cortes-Gonzalez, A Cortiana, G Costa, G Costa, MJ Costanzo, D Cote, D Cottin, G Cowan, G Cox, BE Cranmer, K Cree, G Crepe-Renaudin, S Crescioli, F Ortuzar, MC Cristinziani, M Crosetti, G Cuciuc, CM Donszelmann, TC Cummings, J Curatolo, M Cuthbert, C Czirr, H Czodrowski, P Czyczula, Z D'Auria, S D'Onofrio, M De Sousa, MJDCS Da Via, C Dabrowski, W Dafinca, A Dai, T Dale, O Dallaire, F Dallapiccola, C Dam, M Daniells, AC Hoffmann, MD Dao, V Darbo, G Darlea, GL Darmora, S Dassoulas, JA Davey, W David, C Davidek, T Davies, E Davies, M Davignon, O Davison, AR Davison, P Davygora, Y Dawe, E Dawson, I Daya-Ishmukhametova, RK De, K de Asmundis, R De Castro, S De Cecco, S de Graat, J De Groot, N de Jong, P De la Taille, C De la Torre, H De Lorenzi, F De Nooij, L De Pedis, D De Salvo, A De Sanctis, U De Santo, A De Regie, JBD De Zorzi, G Dearnaley, WJ Debbe, R Debenedetti, C Dechenaux, B Dedovich, DV Degenhardt, J Deigaard, I Del Peso, J Del Prete, T Delemontex, T Deliot, F Deliyergiyev, M Dell'Acqua, A Dell'Asta, L Della Pietra, M della Volpe, D Delmastro, M Delsart, PA Deluca, C Demers, S Demichev, M Demilly, A Demirkoz, B Denisov, SP Derendarz, D Derkaoui, JE Derue, F Dervan, P Desch, K Deviveiros, PO Dewhurst, A Dhaliwal, S Di Ciaccio, A Di Ciaccio, L Di Domenico, A Di Donato, C Di Girolamo, A Di Girolamo, B Di Mattia, A Di Micco, B Di Nardo, R Di Simone, A Di Sipio, R Di Valentino, D Diaz, MA Diehl, EB Dietrich, J Dietzsch, TA Diglio, S Dimitrievska, A Dingfelder, J Dionisi, C Dita, P Dita, S Dittus, F Djama, F Djobava, T do Vale, MAB Wemans, ADV Doan, TKO Dobos, D Dobson, E Doglioni, C Doherty, T Dohmae, T Dolejsi, J Dolezal, Z Dolgoshein, BA Donadelli, M Donati, S Dondero, P Donini, J Dopke, J Doria, A Dotti, A Dova, MT Doyle, AT Dris, M Dubbert, J Dube, S Dubreuil, E Duchovni, E Duckeck, G Ducu, OA Duda, D Dudarev, A Dudziak, F Duflot, L Duguid, L Duhrssen, M Dunford, M Yildiz, HD Duren, M Dwuznik, M Ebke, J Edson, W Edwards, NC Ehrenfeld, W Eifert, T Eigen, G Einsweiler, K Ekelof, T Kacimi, M Ellert, M Elles, S Ellinghaus, F Ellis, N Elmsheuser, J Elsing, M Emeliyanov, D Enari, Y Endner, OC Endo, M Engelmann, R Erdmann, J Ereditato, A Eriksson, D Ernis, G Ernst, J Ernst, M Ernwein, J Errede, D Errede, S Ertel, E Escalier, M Esch, H Escobar, C Curull, XE Esposito, B Etienne, F Etienvre, AI Etzion, E Evans, H Fabbri, L Facini, G Fakhrutdinov, RM Falciano, S Faltova, J Fang, Y Fanti, M Farbin, A Farilla, A Farooque, T Farrell, S Farrington, SM Farthouat, P Fassi, F Fassnacht, P Fassouliotis, D Favareto, A Fayard, L Federic, P Fedin, OL Fedorko, W Fehling-Kaschek, M Feigl, S Feligioni, L Feng, C Feng, EJ Feng, H Fenyuk, AB Perez, SF Fernando, W Ferrag, S Ferrando, J Ferrara, V Ferrari, A Ferrari, P Ferrari, R de Lima, DEF Ferrer, A Ferrere, D Ferretti, C Parodi, AF Fiascaris, M 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Zhu, J. Zhu, Y. Zhuang, X. Zibell, A. Zieminska, D. Zimine, N. I. Zimmermann, C. Zimmermann, R. Zimmermann, S. Zimmermann, S. Zinonos, Z. Ziolkowski, M. Zitoun, R. Zobernig, G. Zoccoli, A. Nedden, M. zur Zurzolo, G. Zutshi, V. Zwalinski, L. CA ATLAS Collaboration TI Measurement of the cross-section of high transverse momentum vector bosons reconstructed as single jets and studies of jet substructure in pp collisions at root s=7TeV with the ATLAS detector SO NEW JOURNAL OF PHYSICS LA English DT Article DE hadronic W; boosted; jet substructure ID MODEL AB This paper presents a measurement of the cross-section for high transverse momentum W and Z bosons produced in pp collisions and decaying to allhadronic final states. The data used in the analysis were recorded by the ATLAS detector at the CERN Large Hadron Collider at a centre-of-mass energy of root s = 7 TeV and correspond to an integrated luminosity of 4.6 fb(-1). The measurement is performed by reconstructing the boosted W or Z bosons in single jets. The reconstructed jet mass is used to identify the W and Z bosons, and a jet substructure method based on energy cluster information in the jet centre-ofmass frame is used to suppress the large multi-jet background. The cross-section for events with a hadronically decaying W or Z boson, with transverse momentum p(T) > 320 GeV and pseudorapidity |eta| < 1.9, is measured to be sigma W+ Z= 8.5 +/- 1.7 pb and is compared to next-to-leading-order calculations. The selected events are further used to study jet grooming techniques.This paper presents a measurement of the cross-section for high transverse momentum W and Z bosons produced in pp collisions and decaying to allhadronic final states. The data used in the analysis were recorded by the ATLAS detector at the CERN Large Hadron Collider at a centre-of-mass energy of root s = 7 TeV and correspond to an integrated luminosity of 4.6 fb(-1). The measurement is performed by reconstructing the boosted W or Z bosons in single jets. The reconstructed jet mass is used to identify the W and Z bosons, and a jet substructure method based on energy cluster information in the jet centre-ofmass frame is used to suppress the large multi-jet background. The cross-section for events with a hadronically decaying W or Z boson, with transverse momentum p(T) > 320 GeV and pseudorapidity |eta| < 1.9, is measured to be sigma W+ Z= 8.5 +/- 1.7 pb and is compared to next-to-leading-order calculations. The selected events are further used to study jet grooming techniques. C1 [Jackson, P.; Soni, N.; White, M. J.] Univ Adelaide, Dept Phys, Adelaide, SA, Australia. [Bouffard, J.; Edson, W.; Ernst, J.; Guindon, S.; Jain, V.] SUNY Albany, Dept Phys, Albany, NY 12222 USA. [Butt, A. I.; Chan, K.; Czodrowski, P.; Gingrich, D. M.; Moore, R. W.; Pinfold, J. L.; Saddique, A.; Sbrizzi, A.; Subramania, H. S.; Vaque, F. 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A.; Backes, M.; Beltramello, O.; Bianco, M.; Cattai, A.; Cerv, M.; Chromek-Burckhart, D.; Dell'Acqua, A.; Di Girolamo, A.; Di Girolamo, B.; Dittus, F.; Dobos, D.; Dopke, J.; Dudarev, A.; Ellis, N.; Elsing, M.; Facini, G.; Farthouat, P.; Feigl, S.; Froidevaux, D.; Garonne, V.; Godlewski, J.; Gorini, B.; Hauschild, M.; Hawkings, R. J.; Heller, C.; Hoecker, A.; Hubacek, Z.; Huhtinen, M.; Jaekel, M. R.; Jansen, E.; Jungst, R. M.; Kaneda, M.; Klioutchnikova, T.; Krasznahorkay, A.; Lampen, C. L.; Lantzsch, K.; Lichard, P.; Macina, D.; Mandelli, B.; Mapelli, L.; Martin, B.; Messina, A.; Meyer, C.; Mornacchi, G.; Nairz, A. M.; Nessi, M.; Nicquevert, B.; Nordberg, M.; Ohm, C. C.; Palestini, S.; Pauly, T.; Pernegger, H.; Petersen, B. A.; Pommes, K.; Poulard, G.; Prasad, S.; Rammes, M.; Rodrigues, L.; Roe, S.; Salzburger, A.; Savu, D. O.; Scanlon, T.; Schlenker, S.; Serfon, C.; Solans, C. A.; Spigo, G.; Stelzer, B.; Unal, G.; van der Ster, D.; van Eldik, N.; van Woerden, M. C.; Vigne, R.; Voss, R.; Vuillermet, R.; Wells, P. S.; Wengler, T.; Wenig, S.; Werner, M.; Wilkens, H. G.; Wotschack, J.; Young, C. J. S.; Zwalinski, L.] CERN, Geneva, Switzerland. [Alison, J.; Anderson, K. J.; Boveia, A.; Cheng, Y.; Fiascaris, M.; Gardner, R. W.; Kapliy, A.; Li, B.; Meehan, S.; Melachrinos, C.; Merritt, F. S.; Meyer, C.; Miller, D. W.; Okumura, Y.; Onyisi, P. U. E.; Oreglia, M. J.; Penning, B.; Pilcher, J. E.; Shochet, M. J.; Tompkins, L.; Vukotic, I.; Webster, J. S.] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA. [Carquin, E.; Diaz, M. A.] Pontificia Univ Catolica Chile, Dept Fis, Santiago, Chile. [Brooks, W. K.; Kuleshov, S.; Pezoa, R.; Prokoshin, F.; White, R.] Univ Tecn Federico Santa Maria, Dept Fis, Valparaiso, Chile. [Bai, Y.; Fang, Y.; Jin, S.; Lu, F.; Ouyang, Q.; Shan, L. Y.; Sun, X.; Wang, J.; Xu, D.; Yao, L.; Zhu, H.; Zhuang, X.] Chinese Acad Sci, Inst High Energy Phys, Beijing, Peoples R China. [Gaob, J.; Guan, L.; Han, L.; Jiang, Y.; Li, B.; Liu, K.; Liu, M.; Liu, Y.; Peng, H.; Xu, L.; Zhao, Z.; Zhu, Y.] Univ Sci & Technol China, Dept Modern Phys, Hefei, Anhui, Peoples R China. [Chen, S.] Nanjing Univ, Dept Phys, Nanjing, Jiangsu, Peoples R China. [Chen, L.; Feng, C.; Ge, P.; Marti, L. F.; Zhang, X.; Zhu, C. G.] Shandong Univ, Sch Phys, Jinan, Shandong, Peoples R China. [Yang, H.] Shanghai Jiao Tong Univ, Dept Phys, Shanghai 200030, Peoples R China. [Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Donini, J.; Dubreuil, E.; Ghodbane, N.; Gris, Ph; Guicheney, C.; Liao, H.; Pallin, D.; Hernandez, D. Paredes; Podlyski, F.; Santoni, C.; Theveneaux-Pelzer, T.; Valery, L.; Vazeille, F.] Univ Clermont Ferrand, Phys Corpusculaire Lab, Clermont Ferrand, France. [Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Donini, J.; Dubreuil, E.; Ghodbane, N.; Gris, Ph; Guicheney, C.; Liao, H.; Pallin, D.; Hernandez, D. Paredes; Podlyski, F.; Santoni, C.; Theveneaux-Pelzer, T.; Valery, L.; Vazeille, F.] Univ Clermont Ferrand, Clermont Ferrand, France. [Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Donini, J.; Dubreuil, E.; Ghodbane, N.; Gris, Ph; Paredes, B. Lopez; Pallin, D.; Hernandez, D. Paredes; Podlyski, F.; Theveneaux-Pelzer, T.; Valero, A.; Vazeille, F.] Univ Clermont Ferrand, Photochim Mol & Macromol Lab, CNRS, IN2P3, F-63177 Clermont Ferrand, France. [Altheimer, A.; Andeen, T.; Angerami, A.; Bain, T.; Brooijmans, G.; Chen, Y.; Cole, B.; Guo, J.; Hu, D.; Hughes, G.; Mohapatra, S.; Nikiforou, N.; Parsons, J. A.; Reale, V. Perez; Scherzer, M. I.; Thompson, E. N.; Tian, F.; Tuts, P. M.; Urbaniec, D.; Wulf, E.; Zhou, L.] Columbia Univ, Nevis Lab, Irvington, NY USA. [Alonso, A.; Dam, M.; Galster, G.; Gregersen, K.; Hansen, J. B.; Hansen, J. D.; Hansen, P. H.; Heisterkamp, S.; Jakobsen, S.; Joergensen, M. D.; Klinkby, E. B.; Loevschall-Jensen, A. E.; Mehlhase, S.; Monk, J.; Petersen, T. C.; Pingel, A.; Simonyan, M.; Thomsen, L. A.; Wiglesworth, C.; Xella, S.] Univ Copenhagen, Niels Bohr Inst, Copenhagen, Denmark. [Capua, M.; Crosetti, G.; La Rotonda, L.; Lavorini, V.; Mastroberardino, A.; Policicchio, A.; Salvatore, D.; Schioppa, M.; Susinno, G.; Tassi, E.] Ist Nazl Fis Nucl, Grp Collegato Cosenza, Lab Nazl Frascati, Milan, Italy. [Capua, M.; Crosetti, G.; La Rotonda, L.; Lavorini, V.; Mastroberardino, A.; Policicchio, A.; Salvatore, D.; Schioppa, M.; Susinno, G.; Tassi, E.] Univ Calabria, Dipartmento Fis, I-87036 Arcavacata Di Rende, Italy. [Adamczyk, L.; Bold, T.; Dabrowski, W.; Dwuznik, M.; Grabowska-Bold, I.; Kisielewska, D.; Koperny, S.; Kowalewski, R.; Kowalski, T. Z.; Mindur, B.; Przybycien, M.; Zemla, A.] AGH Univ Sci & Technol, Fac Phys & Appl Comp Sci, Krakow, Poland. Jagiellonian Univ, Marian Smoluchowski Inst Phys, Krakow, Poland. [Banas, E.; de Renstrom, P. A. Bruckman; Derendarz, D.; Gornicki, E.; Hajduk, Z.; Iwanski, W.; Kaczmarska, A.; Korcyl, K.; Malecki, Pa; Olszewski, A.; Olszowska, J.; Stanecka, E.; Staszewski, R.; Trzebinski, M.; Trzupek, A.; Wolter, M. W.; Wosiek, B. K.; Wozniak, K. W.; Zabinski, B.] Polish Acad Sci, Henryk Niewodniczanski Inst Nucl Phys, Krakow, Poland. [Cao, T.; Firan, A.; Hoffman, J.; Kama, S.; Kehoe, R.; Randle-Conde, A. S.; Sekula, S. J.; Stroynowski, R.; Wang, H.; Ye, J.] So Methodist Univ, Dept Phys, Dallas, TX 75275 USA. [Izen, J. M.; Leyton, M.; Lou, X.; Namasivayam, H.; Reeves, K.] Univ Texas Dallas, Dept Phys, Richardson, TX 75083 USA. [Argyropoulos, S.; Bloch, I.; Borroni, S.; Dassoulas, J. A.; Dietrich, J.; Ferrara, V.; Filipuzzi, M.; Friedrich, C.; Glazov, A.; Fajardo, L. S. Gomez; Da Costa, J. Goncalves Pinto Firmino; Grahn, K-J; Gregor, I. M.; Haleem, M.; Grohsjean, A.; Hengler, C.; Hernandez Jimenez, Y.; Hiller, K. H.; Howard, J.; Howarth, J.; Belenguer, M. Jimenez; Katzy, J.; Kuhl, A.; Lange, C.; Lisovyi, M.; Lobodzinska, E.; Maeno, M.; Medinnis, M.; Radeka, V.; Rubinskiy, I.; Sedov, G.; Shushkevich, S.; South, D.; Stanescu-Bellu, M.; Stanitzki, M. M.; Starovoitov, P.; Styles, N. A.; Tackmann, K.; Vankov, P.; Wang, J.; Wasicki, C.; Wildt, M. A.; Yatsenko, E.; Yildirim, E.] DESY, Hamburg, Germany. [Argyropoulos, S.; Bloch, I.; Borroni, S.; Toro, R. Camacho; Dassoulas, J. A.; Ferrara, V.; Filipuzzi, M.; Friedrich, C.; Glazov, A.; Fajardo, L. S. Gomez; Da Costa, J. Goncalves Pinto Firmino; Grahn, K-J; Gregor, I. M.; Haleem, M.; Grohsjean, A.; Howarth, J.; Belenguer, M. Jimenez; Katzy, J.; Keller, J. S.; Kuhl, A.; Lisovyi, M.; Lobodzinska, E.; Medinnis, M.; Piec, S. M.; Radescu, V.; Rubinskiy, I.; Schaelicke, A.; Sedov, G.; Shushkevich, S.; South, D.; Stanescu-Bellu, M.; Stanitzki, M. M.; Starovoitov, P.; Styles, N. A.; Tackmann, K.; Vankov, P.; Wang, J.; Wasicki, C.; Wildt, M. A.; Yatsenko, E.; Yildirim, E.] DESY, Zeuthen, Germany. [Burmeister, I.; Esch, H.; Goessling, C.; Jentzsch, J.; Jung, C. A.; Klingenberg, R.; Wittig, T.] Tech Univ Dortmund, Inst Expt Phys 4, Dortmund, Germany. [Anger, P.; Friedrich, F.; Grohs, J. P.; Gumpert, C.; Kobel, M.; Leonhardt, K.; Mader, W. F.; Morgenstern, M.; Rudolph, M. S.; Schnoor, U.; Strandberg, S.; Vest, A.; Wahrmund, S.] Tech Univ Dresden, Inst Kern & Teilchenphys, D-01062 Dresden, Germany. [Arce, A. T. H.; Benjamin, D. P.; Bocci, A.; Cerio, B.; Kajomovitz, E.; Kotwal, A.; Krstic, J.; Li, S.; Liu, M.; Oh, S. H.; Pollard, C. S.; Wang, C.] Duke Univ, Dept Phys, Durham, NC 27706 USA. [Bhimji, W.; Bristow, T. M.; Clark, P. J.; Debenedetti, C.; Edwards, N. C.; Walls, F. M. Garay; Harrington, R. D.; Martin, B.; Pino, S. A. Olivares; Proissl, M.; Schaelicke, A.; Selbach, K. E.; Smart, B. H.; Washbrook, A.; Wynne, B. M.] Univ Edinburgh, Sch Phys & Astron, SUPA, Edinburgh, Midlothian, Scotland. [Annovi, A.; Antonelli, M.; Bilokon, H.; Chiarella, V.; Curatolo, M.; Di Nardo, R.; Esposito, B.; Gatti, C.; Laurelli, P.; Maccarrone, G.; Sansoni, A.; Testa, M.; Vilucchi, E.; Volpi, G.] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy. [Amoroso, S.; Barber, T.; Betancourt, C.; Boehler, M.; Buehrer, F.; Consonni, S. M.; Fehling-Kaschek, M.; Flechl, M.; Giuliani, C.; Jakobs, K.; Jenni, P.; Kiss, F.; Kopp, A. K.; Kuehn, S.; Lai, S.; Landgraf, U.; Madar, R.; Mohr, W.; Paganis, E.; Rave, T. C.; Rurikova, Z.; Schmitt, C.; Sommer, P.; Stoerig, K.; Sundermann, J. E.; Temming, K. K.; Thoma, S.; Tsiskaridze, S.; Ungaro, F. C.; Ventura, A.; von Radziewski, H.; Warsinsky, M.; Weiser, C.; Werner, M.; Winkelmann, S.; Zimmermann, S.] Univ Freiburg, Fak Math & Phys, D-79106 Freiburg, Germany. [Alexandre, G.; Barone, G.; Bell, P. J.; Noccioli, E. Benhar; De Mendizabal, J. Bilbao; Bucci, F.; Toro, R. Camacho; Clark, A.; della Volpe, D.; Doglioni, C.; Ferrere, D.; Gadomski, S.; Gonzalez-Sevilla, S.; Goulette, M. P.; Iacobucci, G.; Katre, A.; La Rosa, A.; Latour, B. Martin dit; Nikolics, K.; Picazio, A.; Pohl, D.; Pohl, M.; Rosbach, K.; Vallecorsa, S.; Wu, X.] Univ Geneva, Sect Phys, Geneva, Switzerland. [Barberis, D.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Gemme, C.; Guido, E.; Morettini, P.; Osculati, B.; Parodi, F.; Passaggio, S.; Rossi, L. P.] Ist Nazl Fis Nucl, Sez Genova, Milan, Italy. [Barberis, D.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Guido, E.; Osculati, B.; Parodi, F.; Schiavi, C.] Univ Genoa, Dipartimento Fis, Genoa, Italy. [Tskhadadze, E. G.] Iv Javakhishvili Tbilisi State Univ, E Andronikashvili Inst Phys, Tbilisi, Rep of Georgia. [Djobava, T.; Khubua, J.; Mosidzeb, M.] Tbilisi State Univ, Inst High Energy Phys, Tbilisi, Rep of Georgia. [Dueren, M.; Kreutzfeldt, K.; Stenzel, H.] Univ Giessen, Inst Phys 2, Giessen, Germany. [Allwood-Spiers, S. E.; Altheimer, A.; Bates, R. L.; Britton, D.; Buckley, A. G.; Bussey, P.; Buttar, C. M.; Collins-Tooth, C.; D'Auria, S.; Doherty, T.; Doyle, A. T.; Ferrag, S.; de Lima, D. E. Ferreira; Gemmell, A.; Gul, U.; Ortiz, N. G. Gutierrez; Kar, D.; Knue, A.; Moraes, A.; O'Shea, V.; Barrera, C. Oropeza; Quilty, D.; Ravenscroft, T.; Robson, A.; Saxon, J.; Smith, K. M.; St Denis, R. D.; Steele, G.; Stewart, G. A.; Valls Ferrer, J. A.] Univ Glasgow, Sch Phys & Astron, SUPA, Glasgow, Lanark, Scotland. [Bierwagen, K.; Bindi, M.; Blumenschein, U.; George, M.; Graber, L.; Grosse-Knetter, J.; Hamer, M.; Hensel, C.; Kawamura, G.; Keil, M.; Kroeninger, K.; Lemmer, B.; Magradze, E.; Mchedlidze, G.; Morel, J.; Llacer, M. Moreno; Nackenhorst, O.; Nadal, J.; Quadt, A.; Schorlemmer, A. L. S.; Serkin, L.; Shabalina, E.; Weingarten, J.; Zinonos, Z.] Univ Gottingen, Inst Phys 2, Gottingen, Germany. [Albrand, S.; Brown, G.; Clement, B.; Collot, J.; Crepe-Renaudin, S.; Dechenaux, B.; Gabaldon, C.; Genest, M. H.; Hostachy, J-Y; Le, B. T.; Ledroit-Guillon, F.; Lleres, A.; Lucotte, A.; Malek, F.; Monini, C.; Stark, J.; Trocme, B.] Univ Grenoble Alpes, Lab Phys Subatom & Cosmol, CNRS, IN2P3, Grenoble, France. [Addy, T. N.; Harvey, A.; McFarlane, K. W.] Hampton Univ, Dept Phys, Hampton, VA 23668 USA. [Da Costa, J. Barreiro Guimaraes; Belloni, A.; Butler, B.; Catastini, P.; Conti, G.; Franklin, M.; Huth, J.; Ippolito, V.; Lopez Mateos, D.; Mercurio, K. M.; Morii, M.; Skottowe, H. P.; Spearman, W. R.; Yen, A. L.; della Porta, G. Zevi] Harvard Univ, Lab Particle Phys & Cosmol, Cambridge, MA 02138 USA. [Andrei, V.; Brandta, O.; Davygora, Y.; Dietzsch, T. A.; Dunford, M.; Hanke, P.; Hofmann, J. I.; Khomich, A.; Kluge, E-E; Meier, K.; Mueller, F.; Scharf, V.; Stamen, R.; Wessels, M.] Heidelberg Univ, Kirchhoff Inst Phys, Heidelberg, Germany. [Anders, C. F.; Giunta, M.; Kasieczka, G.; Narayan, R.; Schaetzel, S.; Schmitt, S.; Schoening, A.] Heidelberg Univ, Inst Phys, Heidelberg, Germany. [Colombo, T.; Kretz, M.; Kugel, A.] Heidelberg Univ, ZITI Inst Tech Informat, Heidelberg, Germany. [Nagasaka, Y.] Hiroshima Inst Technol, Fac Appl Informat Sci, Hiroshima, Japan. [Brunet, S.; Evans, H.; Gagnon, P.; Martinez, N. Lorenzo; Luehring, F.; Ogren, H.; Penwell, J.; Poveda, J.; Zieminska, D.] Indiana Univ, Dept Phys, Bloomington, IN 47405 USA. [Franz, S.; Jussel, P.; Kneringer, E.; Lukas, W.; Nagai, K.; Ritsch, E.; Usanova, A.] Leopold Franzens Univ, Inst fur Astro & Teilchenphys, Innsbruck, Austria. [Cinca, D.; Gandrajula, R. P.; Limper, M.; Mallik, U.; Mandrysch, R.; Morange, N.; Pylypchenko, Y.; Zaidan, R.] Univ Iowa, Iowa City, IA USA. [Chen, C.; Cochran, J.; De Lorenzi, F.; Dudziak, F.; Krumnack, N.; Prell, S.; Ruiz-Martinez, A.; Shrestha, S.; Yamamoto, K.] Iowa State Univ, Dept Phys & Astron, Ames, IA USA. [Ahmadov, F.; Aleksandrov, I. N.; Bednyakov, V. A.; Boyko, I. R.; Buda, S. I.; Chizhov, M. V.; Dedovich, D. V.; Demilly, A.; Glonti, G. L.; Huseynov, N.; Khramov, E.; Kotov, V. M.; Kruchonak, U.; Krumshteyn, Z. V.; Kukhtin, V.; Ladygin, E.; Mineev, M.; Olchevski, A. G.; Peshekhonov, V. D.; Plotnikova, E.; Potrap, I. N.; Pozdnyakov, V.; Pueschel, E.; Rusakovich, N. A.; Sisakyan, A. N.; Topilin, N. D.; Vinogradov, V. B.; Zhemchugov, A.; Zimine, N. I.] Joint Inst Nucl Res Dubna, Dubna, Russia. [Amako, K.; Aoki, M.; Arai, Y.; Ikegami, Y.; Iwasaki, H.; Kohriki, T.; Kondo, T.; Kono, T.; Nagano, K.; Nakamura, K.; Nozaki, M.; Takubo, Y.; Tanaka, S.; Terada, S.; Tsuno, S.; Yamada, M.; Yamamoto, A.; Yasu, Y.] High Energy Accelerator Res Org, KEK, Tsukuba, Ibaraki, Japan. [Inamaru, Y.; Kishimoto, T.; Kitamura, T.; Kurashige, H.; Matsushita, T.; Ochi, A.; Takeda, H.; Tani, K.; Watanabe, I.; Yamazaki, Y.; Yuan, L.] Kobe Univ, Grad Sch Sci, Kobe, Hyogo 657, Japan. [Ishino, M.; Sumida, T.; Tashiro, T.] Kyoto Univ, Fac Sci, Kyoto, Japan. [Takashima, R.] Kyoto Univ, Kyoto 612, Japan. [Kawagoe, K.; Oda, S.; Otono, H.; Tojo, J.] Kyushu Univ, Dept Phys, Fukuoka 812, Japan. [Alconada Verzini, M. J.; Alonso, F.; Anduaga, X. S.; Dova, M. T.; Monticelli, F.; Tripiana, M. F.] Univ Nacl La Plata, Inst Fis La Plata, La Plata, Argentina. [Alconada Verzini, M. J.; Alonso, F.; Anduaga, X. S.; Dova, M. T.; Monticelli, F.; Tripiana, M. F.] Consejo Nacl Invest Cient & Tecn, La Plata, Argentina. [Allison, L. J.; Barton, A. E.; Borissov, G.; Bouhova-Thacker, E. V.; Catmore, J. R.; Chilingarov, A.; Dearnaley, W. J.; Fox, H.; Grimm, K.; Henderson, R. C. W.; Hughes, G.; Jones, R. W. L.; Kartvelishvili, V.; Long, J. D.; Love, P. A.; Maddocks, H. J.; Smizanska, M.; Walder, J.] Univ Lancaster, Dept Phys, Lancaster, England. [Chiodini, G.; Gorini, E.; Grancagnolo, F.; Orlando, N.; Perrino, R.; Primavera, M.; Spagnolo, S.; Ventura, A.] Ist Nazl Fis Nucl, Sez Lecce, I-73100 Lecce, Italy. [Gorini, E.; Orlando, N.; Spagnolo, S.; Ventura, A.] Univ Salento, Dipartimento Matemat & Fis, Lecce, Italy. [Allport, P. P.; Bundock, A. C.; Burdin, S.; D'Onofrio, M.; Dervan, P.; Gwilliam, C. B.; Jackson, B.; Jackson, J. N.; Jones, T. J.; Klein, U.; Laycock, P.; Maxfield, S. J.; Mehta, A.; Migas, S.; Price, D.; Schnellbach, Y. J.; Sellers, G.; Vossebeld, J. H.; Waller, P.] Univ Liverpool, Oliver Lodge Lab, Liverpool L69 3BX, Merseyside, England. [Cindro, V.; Deliyergiyev, M.; Filipcic, A.; Gorisek, A.; Kersevan, B. P.; Kramberger, G.; Macek, B.; Mandic, I.; Mikuz, M.; Tykhonov, A.] Jozef Stefan Inst, Dept Phys, Ljubljana, Slovenia. [Cindro, V.; Deliyergiyev, M.; Filipuzzi, M.; Gorisek, A.; Kersevan, B. P.; Macek, B.; Mandrysch, R.; Mikuz, M.; Tykhonov, A.] Univ Ljubljana, Ljubljana, Slovenia. [Alpigiani, C.; Bona, M.; Carter, J. R.; Cerrito, L.; Fletcher, G.; Goddard, J. R.; Landon, M. P. J.; Lloyd, S. L.; Piccinini, M.; Rizvi, E.; Salamanna, G.; Snidero, G.; Castanheira, M. Teixeira Dias] Queen Mary Univ London, Sch Phys & Astron, London, England. [Berry, T.; Boisvert, V.; Cantrill, R.; Cooper-Smith, N. J.; Cowan, G.; Duguid, L.; George, S.; Vazquez, J. G. Panduro; Pastore, F.; Rose, A.; Spano, F.; Teixeira-Dias, P.; Thomas-Wilsker, J.] Royal Holloway Univ London, Dept Phys, Surrey, England. [Baker, S.; Bernat, P.; Bieniek, S. P.; Butterworth, J. M.; Campoverde, A.; Casado, M. P.; Chisholm, A. S.; Cooper, B. D.; Davison, A. R.; Davison, P.; Dobson, E.; Fisher, M. J.; Gutschow, C.; Konstantinidis, N.; Korn, A.; Lambourne, L.; Leney, K. J. C.; Martyniuk, A. C.; Mcfayden, J. A.; Pilkington, A. D.; Prabhu, R.; Simmons, B.; Taylor, C.; Wardrope, D. R.; Waugh, A. T.; Wijeratne, P. A.] UCL, Dept Phys & Astron, London, England. [Bernius, C.; Greenwood, Z. D.; Sawyer, C.; Sircar, A.; Subramaniam, R.; Tamsett, M. C.] Louisiana Tech Univ, Ruston, LA 71270 USA. [Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; Davison, A. R.; De Cecco, S.; Demilly, A.; Derue, F.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Marchese, F.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Vannucci, F.; Varouchas, D.] UPMC, Lab Phys Nucl & Hautes Energies, Paris, France. [Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Castro, S.; Demilly, A.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Ocariz, J.; Rangel-Smith, C.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Vannucci, F.; Varouchas, D.] Univ Paris Diderot, Paris, France. [Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Cecco, S.; Demilly, A.; Derue, F.; Krasny, M. W.; Lacour, D.; Laforge, B.; Lefebvre, G.; Nikolics, K.; Ocariz, J.; Ridel, M.; Roos, L.; Tricoli, A.; Vannucci, F.; Varouchas, D.] CNRS, IN2P3, Paris, France. [Akesson, T. P.; Bocchetta, S. S.; Bryngemark, L.; Floderus, A.; Hawkins, A. D.; Hedberg, V.; Jarlskog, G.; Lytken, E.; Meirose, B.; Mjornmark, J. U.; Smirnova, O.; Viazlo, O.] Lund Univ, Inst Fys, Lund, Sweden. [Arnal, V.; Barreiro, F.; Cantero, J.; De la Torre, H.; Del Peso, J.; Glasman, C.; Labarga, L.; Llorente Merino, J.; Terron, J.] Univ Autonoma Madrid, Dept Fis Teor C 15, Madrid, Spain. [Arnaez, O.; Blum, W.; Buehrer, F.; Capua, M.; Ellinghaus, F.; Ertel, E.; Fiedler, F.; Torregrosa, E. Fullana; Goeringer, C.; Heck, T.; Hsu, P. J.; Koenig, A. C.; Masetti, L.; Morel, J.; Moritz, S.; Mueller, F.; Poettgen, R.; Sander, H. G.; Schmitt, C.; Schott, M.; Schuh, N.; Simioni, E.; Tapprogge, S.; Wollstadt, S. J.; Zimmermann, C.] Johannes Gutenberg Univ Mainz, Inst Phys, Mainz, Germany. [Almond, J.; Borri, M.; Cox, B. E.; Da Via, C.; Forti, A.; Ponce, J. M. Iturbe; Joshi, K. D.; Klinger, J. A.; Loebinger, F. K.; Marsden, S. P.; Masik, J.; Neep, T. J.; Tomlinson, L.; Webb, S.; Woudstra, M. J.; Wyatt, T. R.; Yang, U. K.] Univ Manchester, Sch Phys & Astron, Manchester, Lancs, England. [Aad, G.; Alio, L.; Barberis, D.; Clemens, J. C.; Djama, F.; Knoops, E. B. F. G.; Le Guirriec, E.; Li, B.; Monnier, E.; Nagai, K.; Nagai, R.; Pralavorio, P.; Talby, M.; Tannoury, N.; Tiouchichine, E.; Tisserant, S.; Toth, J.; Touchard, F.; Ughetto, M.; Vacavant, L.] Aix Marseille Univ, CPPM, Marseille, France. [Aad, G.; Alio, L.; Barberis, D.; Clemens, J. C.; Djama, F.; Hoffmann, D.; Hubacek, Z.; Le Guirriec, E.; Liberti, B.; Madar, R.; Monnier, E.; Muanza, S.; Nagai, K.; Pralavorio, P.; Rozanov, A.; Serre, T.; Talby, M.; Tiouchichine, E.; Tisserant, S.; Toth, J.; Touchard, F.; Ughetto, M.; Vacavant, L.] CNRS, IN2P3, Marseille, France. [Bellomo, M.; Brau, B.; Colon, G.; Dallapiccola, C.; Meade, A.; Moyse, E. J. W.; Pais, P.; Varol, T.; Ventura, A.; Willocq, S.] Univ Massachusetts, Dept Phys, Amherst, MA 01003 USA. [Belanger-Champagne, C.; Chapleau, B.; Cheatham, S.; Corriveau, F.; Mantifel, R.; Robertson, S. H.; Schramm, S.; Stockton, M. C.; Vachon, B.; Wang, K.; Warburton, A.] McGill Univ, Dept Phys, Montreal, PQ, Canada. [Barberis, D.; Brennan, A. J.; Chitan, A.; Diglio, S.; Hamacher, K.; Limosani, A.; Nuti, F.; Petersen, B. A.; Shao, Q. T.; Taylor, C.; Thong, W. M.; Volpi, M.] Univ Melbourne, Sch Phys, Melbourne, Vic 3010, Australia. [Chelstowska, M. A.; Cheng, H. C.; Dai, T.; Diehl, E. B.; Goldfarb, S.; Harper, D.; Long, J. D.; Mc Kee, S. P.; McCarn, A.; Neal, H. A.; Panikashvili, N.; Qian, J.; Shmeleva, A.; Thun, R. P.; Wilson, J. A.; Yu, J. M.; Zhang, D.; Zhou, B.; Zhu, J.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA. [Abolins, M.; Gonzalez, B. Alvarez; Arabidze, G.; Brock, R.; Bromberg, C.; Caughron, S.; Fisher, M. J.; Halladjian, G.; Hauser, R.; Hayden, D.; Huston, J.; Koll, J.; Linnemann, J. T.; Martin, B.; Pope, B. G.; Schoenrock, B. D.; Schwindling, J.; Ta, D.; Tollefson, K.; True, P.; Zhang, H.] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA. [Alimonti, G.; Andreazza, A.; Besana, M. I.; Carminati, L.; Citterio, M.; Consorti, V.; Costa, G.; Fanti, M.; Giugni, D.; Meloni, F.; Perini, L.; Pizio, C.; Ragusa, F.; Resconi, S.; Simonyan, M.; Troncon, C.; Turra, R.] Ist Nazl Fis Nucl, Sez Milano, I-20133 Milan, Italy. [Andreazza, A.; Carminati, L.; Consonni, S. M.; Fanti, M.; Meloni, F.; Perini, L.; Pizio, C.; Ragusa, F.; Simonyan, M.; Turra, R.] Univ Milan, Dipartimento Fis, Milan, Italy. [Bogouch, A.; Harkusha, S.; Kulchitsky, Y.; Kurochkin, Y. A.; Tsiareshka, P. V.] Natl Acad Sci Belarus, BI Stepanov Phys Inst, Minsk, Byelarus. [Yanush, S.] Natl Sci & Educ Ctr Particle & High Energy Phys, Minsk, Byelarus. [Taylor, F. E.] MIT, Dept Phys, Cambridge, MA 02139 USA. [Arguin, J-F; Asbah, N.; Azuelos, G.; Dallaire, F.; Davies, M.; Gauthier, L.; Leroy, C.; Rezvani, R.; Soueid, P.] Univ Montreal, Grp Particle Phys, Montreal, PQ, Canada. [Akimov, A. V.; Baranov, S. P.; Gavrilenko, I. L.; Komar, A. A.; Mashinistov, R.; Mouraviev, S. V.; Nechaeva, P. Yu; Shmeleva, A.; Snesarev, A. A.; Sulin, V. V.; Tikhomirov, V. O.] Acad Sci, PN Lebedev Phys Inst, Moscow, Russia. [Artamonov, A.; Gorbounov, P. A.; Khovanskiy, V.; Shatalov, P. B.; Tsukerman, I. I.] Inst Theoret & Expt Phys, Moscow 117259, Russia. [Antonaki, A.; Belotskiy, K.; Bulekov, O.; Dolgoshein, B. A.; Kantserov, V. A.; Khodinov, A.; Krasnopevtsev, D.; Romaniouk, A.; Shulga, E.; Smirnova, L. N.; Soldevila, U.; Timoshenko, S.] Moscow Engn & Phys Inst MEPhI, Moscow, Russia. [Adomeit, S.; Becker, S.; Biebel, O.; Calfayan, P.; Chow, B. K. B.; de Graat, J.; Duckeck, G.; Ebke, J.; Elmsheuser, J.; Heller, M.; Hertenberger, R.; Leggett, C.; Lorenz, J.; Mann, A.; Meineck, C.; Mitrevski, J.; Schieck, J.; Vladoiu, D.; Walker, R.; Will, J. Z.; Wittkowski, J.; Zibell, A.] Moscow MV Lomonosov State Univ, DV Skobeltsyn Inst Nucl Phys, Moscow, Russia. [Adomeit, S.; Becker, S.; Biebel, O.; Calfayan, P.; Chow, B. K. B.; de Graat, J.; Duckeck, G.; Ebke, J.; Legger, F.; Lorenz, J.; Mitrevski, J.; Nunnemann, T.; Rauscher, F.; Sander, H. G.; Schaelicke, A.; Schaile, D.; Schmitt, C.; Vladoiu, D.; Wittkowski, J.; Zibell, A.] Univ Munich, Fak Phys, Munich, Germany. [Barillari, T.; Bethke, S.; Bronner, J.; Compostella, G.; Cortiana, G.; Flowerdew, M. J.; Goblirsch-Kolb, M.; Ince, T.; Kiryunin, A. E.; Kluth, S.; Kotov, V. M.; Kroha, H.; Menke, S.; Nagel, M.; Nisius, R.; Pahl, C.; Salihagic, D.; Sandstroem, R.; Schacht, P.; Sforza, F.; Stern, S.; Stonjek, S.; Weigell, P.; Wildauer, A.; Zanzi, D.] Max Planck Inst Phys & Astrophys, Werner Heisenberg Inst, D-80805 Munich, Germany. [Shimojima, M.] Nagasaki Inst Appl Sci, Nagasaki, Japan. [Hasegawa, S.; Morvaj, L.; Ohshima, T.; Takahashi, Y.; Tomoto, M.; Yamauchi, K.] Nagoya Univ, Grad Sch Sci, Nagoya, Aichi 4648601, Japan. [Hasegawa, Y.; Morvaj, L.; Ohshima, T.; Takahashi, Y.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Kobayashi Maskawa Inst, Nagoya, Aichi 4648601, Japan. [Aloisio, A.; Alviggi, M. G.; Canale, V.; Chiefari, G.; Conventi, F.; de Asmundis, R.; Della Pietra, M.; Di Donato, C.; Doria, A.; Giordano, R.; Iengo, P.; Izzo, V.; Merola, L.; Rossi, E.; Sanchez, A.; Sekhniaidze, G.] Ist Nazl Fis Nucl, Sez Napoli, I-80125 Naples, Italy. [Aloisio, A.; Alonso, A.; Alviggi, M. G.; Canale, V.; Chiefari, G.; Di Domenico, A.; Giordani, M. P.; Merola, L.; Patricelli, S.; Rossi, L. P.; Zurzolo, G.] Univ Naples Federico II, Dipartimento Fis, Naples, Italy. [Gorelov, I.; Hoeferkamp, M. R.; Seidel, S. C.; Toms, K.; Wang, R.] Univ New Mexico, Dept Phys & Astron, Albuquerque, NM 87131 USA. [Besjes, G. J.; Caron, S.; Dao, V.; De Groot, N.; Filthaut, F.; Galea, C.; Klok, P. F.; Koenig, A. C.; Salvucci, A.] Radboud Univ Nijmegen Nikhef, Inst Math Astrophys & Particle Phys, Nijmegen, Netherlands. [Aben, R.; Beemster, L. J.; Bentvelsen, S.; Berge, D.; Berglund, E.; Bos, K.; Boterenbrood, H.; Buttinger, W.; Castelli, A.; de Jong, P.; De Nooij, L.; Deigaard, I.; Deluca, C.; Deviveiros, P. O.; Dhaliwal, S.; Ferrari, A.; Gadatsch, S.; Geerts, D. A. A.; Hod, N.; Igonkina, O.; Kluit, P.; Koffeman, E.; Lee, C. A.; Lenzi, B.; Linde, F.; Mahlstedt, J.; Mechnich, J.; Van der Deijl, P. C.; van der Graaf, H.; van der Ster, D.; van Vulpen, I.; Vermeulen, J. C.; Milosavljevic, M. Vranjes; Vreeswijk, M.; Weits, H.] Nikhef Natl Inst Subat Phys, Amsterdam, Netherlands. [Burghgrave, B.; Calkins, R.; Chakraborty, D.; Cole, B.; Suhr, C.; Yurkewicz, A.; Zutshi, V.] Univ Amsterdam, Amsterdam, Netherlands. [Burghgrave, B.; Calkins, R.; Chakraborty, D.; Cole, S.; Suhr, C.; Yurkewicz, A.; Zutshi, V.] Univ Illinois, Dept Phys, De Kalb, IL USA. [Anisenkov, A. V.; Belotskiy, K.; Bobrovnikov, V. S.; Bogdanchikov, A. G.; Kazanin, V. F.; Korol, A. A.; Malyshev, V. M.; Maslennikov, A. L.; Maximov, D. A.; Peleganchuk, S. V.; Skovpen, K. Yu; Soukharev, A. M.; Talyshev, A. A.; Tikhonov, Yu A.] SB RAS, Budker Inst Nucl Phys, Novosibirsk, Russia. [Cranmer, K.; Haas, A.; Heinrich, L.; van Huysduynen, L. Hooft; Kaplan, B.; Konoplich, R.; Kreiss, S.; Lewis, G. H.; Mincer, A. I.; Nemethy, P.; Neves, R. M.; Prokofiev, K.] NYU, Dept Phys, New York, NY 10003 USA. [Fisher, M. J.; Gan, K. K.; Ishmukhametov, R.; Kagan, H.; Kass, R. D.; Merritt, H.; Moss, J.; Nagarkar, A.; Pignotti, D. T.; Yang, Y.] Ohio State Univ, Columbus, OH 43210 USA. [Nakano, I.] Okayama Univ, Fac Sci, Okayama 700, Japan. [Abbott, B.; Gutierrez, P.; Meera-Lebbai, R.; Norberg, S.; Saleem, M.; Severini, H.; Skubic, P.; Strauss, M.] Univ Oklahoma, Homer L Dodge Dept Phys & Astron, Norman, OK 73019 USA. [Abi, B.; Bousson, N.; Khanov, A.; Rizatdinova, F.; Sidorov, D.; Yu, J.] Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USA. [Hrabovsky, M.; Nozka, L.] Palacky Univ, RCPTM, CR-77147 Olomouc, Czech Republic. [Brau, J. E.; Brost, E.; Majewski, S.; Potter, C. T.; Radloff, P.; Reinsch, A.; Shamim, M.; Sinev, N. B.; Strom, D. M.; Torrence, E.; Winklmeier, F.] Univ Oregon, Ctr High Energy Phys, Eugene, OR 97403 USA. [Khalek, S. Abdel; Auge, E.; Bassalat, A.; Binet, S.; Bourdarios, C.; Charfeddine, D.; De la Taille, C.; De Regie, J. B. De Vivie; Duflot, L.; Escalier, M.; Fayard, L.; Fournier, D.; Grivaz, J-F; Guillemin, T.; Correia, A. M. Henriques; Kado, M.; Lounis, A.; Makovec, N.; Poggioli, L.; Puzo, P.; Renaud, A.; Rousseau, D.; Rybkin, G.; Scifo, E.; Serin, L.; Simion, S.; Zerwas, D.; Zhang, Z.] Univ Paris 11, LAL, Orsay, France. [Endo, M.; Hanagaki, K.; Hirose, M.; Lee, J. S. H.; Nomachi, M.; Okamura, W.; Sugaya, Y.] Osaka Univ, Grad Sch Sci, Osaka, Japan. [Bugge, L.; Bugge, M. K.; Cameron, D.; Gjelsten, B. K.; Gramstad, E.; Ould-Saada, F.; Pajchel, K.; Read, A. L.; Smestad, L.; Stapnes, S.; Strandlie, A.] Univ Oslo, Dept Phys, Oslo, Norway. [Apolle, R.; Barr, A. J.; Behr, K.; Boddy, C. R.; Buckingham, R. M.; Cooper-Sarkar, A. M.; Ortuzar, M. Crispin; Dafinca, A.; Davies, E.; Gallas, E. J.; Gupta, S.; Gwenlan, C.; Hall, D.; Lewis, A.; Liang, Z.; Pinder, A.; Robichaud-Veronneau, A.; Ryder, N. C.; Sawyer, C.; Short, D.; Tseng, J. C-L; Viehhauser, G. H. A.; Weidberg, A. R.; Zhong, J.] Univ Oxford, Dept Phys, Oxford, England. [Conta, C.; Dondero, P.; Ferrari, A.; Fraternali, M.; Livan, M.; Negri, A.; Polesello, G.; Rebuzzi, D. M.; Vercesi, V.] Ist Nazl Fis Nucl, Sez Pavia, I-27100 Pavia, Italy. [Conta, C.; Dondero, P.; Fraternali, M.; Livan, M.; Negri, A.; Rebuzzi, D. M.; Rimoldi, A.] Univ Pavia, Dipartimento Fis, I-27100 Pavia, Italy. [Brendlinger, K.; Degenhardt, J.; Heim, S.; Hines, E.; Hong, T. M.; Jackson, B.; Kroll, J.; Olivito, D.; Ospanov, R.; Saxon, J.; Schaelicke, A.; Thompson, A. S.; Tuna, A. N.; Williams, H. H.] Univ Penn, Dept Phys, Philadelphia, PA 19104 USA. [Fedin, O. L.; Gratchev, V.; Grebenyuk, O. G.; Maleev, V. P.; Ryabov, Y. F.; Schegelsky, V. A.; Sedykh, E.; Seliverstov, D. M.; Solovyev, V.] Petersburg Nucl Phys Inst, Gatchina, Russia. [Beccherle, R.; Bertolucci, F.; Cavasinni, V.; Del Prete, T.; Donati, S.; Giannetti, P.; Roda, C.; Scuri, F.; White, S.] Ist Nazl Fis Nucl, Sez Pisa, Pisa, Italy. [Beccherle, R.; Bertolucci, F.; Cavasinni, V.; Del Prete, T.; Donati, S.; Giannetti, P.; Roda, C.; Scuri, F.; White, S.] Univ Pisa, Dipartimento Fis E Fermi, Pisa, Italy. [Bianchi, R. M.; Boudreau, J.; Cleland, W.; Escobar, C.; Kittelmann, T.; Mueller, F.; Prieur, D.; Sapp, K.; Su, J.; Yoosoofmiya, R.] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA. [Aguilar-Saavedra, J. A.; Aloisio, A.; Amor Dos Santos, S. P.; Amorim, A.; Anjos, N.; Castro, N. F.; Conde Muino, P.; Da Cunha Sargedas De Sousa, M. J.; Gomes, A.; Goncalo, R.; Jorge, P. M.; Lopes, L.; Miguens, J. Machado; Maio, A.; Maneira, J.; Marquesa, C. 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Do Valle] Univ Nova Lisboa, CEFITEC, Fac Ciencias & Tecnol, Caparica, Portugal. [Bohm, J.; Chudoba, J.; Harvey, A.; Hejbal, J.; Jakoubek, T.; Kupco, A.; Kus, V.; Lokajicek, M.; Marcisovsky, M.; Mikestikova, M.; Myska, M.; Nemecek, S.; Sicho, P.; Staroba, P.; Svatos, M.; Tasevsky, M.; Vrba, V.] Acad Sci Czech Republic, Inst Phys, Prague, Czech Republic. [Augsten, K.; Gallas, E. J.; Gunther, J.; Jakubek, J.; Kohout, Z.; Kral, V.; Pospisil, S.; Seifert, F.; Slavicek, T.; Smolek, K.; Solar, M.; Solc, J.; Suk, M.; Turecek, D.; Vacek, V.; Vlasak, M.; Vokac, P.; Vykydal, Z.; Zeman, M.] Czech Tech Univ, CR-16635 Prague, Czech Republic. [Balek, P.; Berta, P.; Cerny, K.; Chalupkova, I.; Davidek, T.; Dolezal, Z.; Kodys, P.; Leitner, R.; Rybar, M.; Scheirich, D.; Spousta, M.; Tas, P.; Todorova-Nova, S.; Valkar, S.; Vorobel, V.] Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic. [Ammosov, V. V.; Fakhrutdinov, R. M.; Fenyuk, A. B.; Ivashin, A. V.; Karyukhin, A. N.; Kozhin, A. S.; Myagkov, A. G.; Nikolaenko, V.; Solodkov, A. A.; Starchenko, E. A.; Zaitsev, A. M.; Zenin, O.] State Res Ctr Inst High Energy Phys, Protvino, Russia. [Adye, T.; Apolle, R.; Baines, J. T.; Barnett, B. M.; Burke, S.; Dewhurst, A.; Emeliyanov, D.; Gallop, B. J.; Gee, C. N. P.; Hayward, H. S.; Kirk, J.; Martin-Haugh, S.; Middleton, R. P.; Murray, W. J.; Phillips, P. W.; Sankey, D. P. C.; Scott, W. G.; Wickens, F. J.; Wielers, M.; Wienemann, P.] Rutherford Appleton Lab, Particle Phys Dept, Didcot OX11 0QX, Oxon, England. [Benslama, K.] Univ Regina, Dept Phys, Regina, SK S4S 0A2, Canada. [Tanaka, S.] Ritsumeikan Univ, Kusatsu, Shiga, Japan. [Anulli, F.; Bagiacchi, P.; Bagnaia, P.; Bini, C.; Ciapetti, G.; De Pedis, D.; De Salvo, A.; De Zorzi, G.; Di Domenico, A.; Dionisi, C.; Falciano, S.; Gauzzi, P.; Giagu, S.; Kuna, M.; Lacava, F.; Mirabelli, G.; Petrolo, E.; Pontecorvo, L.; Rescigno, M.; Rosati, S.; Vari, R.; Veneziano, S.] Ist Nazl Fis Nucl, Sez Roma, Rome, Italy. [Bagiacchi, P.; Bagnaia, P.; Bini, C.; Ciapetti, G.; De Zorzi, G.; Di Domenico, A.; Gabrielli, A.; Gauzzi, P.; Giagu, S.; Kuna, M.; Lacava, F.; Monzani, S.; Camillocci, E. Solfaroli; Vanadia, M.; Zanello, L.] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy. [Aielli, G.; Cardarelli, R.; Cattani, G.; Di Ciaccio, A.; Gross, A. Grohsjean E.; Liberti, B.; Salamon, A.] Ist Nazl Fis Nucl, Sez Roma Tor Vergata, Rome, Italy. [Aielli, G.; Cattani, G.; Di Ciaccio, A.; Grossi, G. C.; Marchese, F.; Mazzaferro, L.; Santonico, R.] Univ Roma Tor Vergata, Dipartimento Fis, I-00173 Rome, Italy. [Bacci, C.; Baroncelli, A.; Biglietti, M.; Bortolotto, V.; Ceradini, F.; Di Micco, B.; Farilla, A.; Graziani, E.; Iodice, M.; Orestano, D.; Passeri, A.; Pastore, F.; Petrucci, F.; Stanescu, C.; Trovatelli, M.] Ist Nazl Fis Nucl, Sez Roma Tre, Rome, Italy. [Bacci, C.; Bortolotto, V.; Ceradini, F.; Di Micco, B.; Orestano, D.; Pastore, F.; Petrucci, F.; Trovatelli, M.] Univ Roma Tre, Dipartimento Matemat & Fis, Rome, Italy. [Benchekroun, D.; Chafaq, A.; Gouighri, M.; Hoummada, A.] Univ Hassan 2, Reseau Univ Phys Hautes Energies, Fac Sci Ain Chock, Casablanca, Morocco. [Ghazlane, H.] Ctr Natl Energie Sci Tech Nucl, Rabat, Morocco. [El Kacimi, M.; Goujdami, D.] Univ Cadi Ayyad, LPHEA, Fac Sci Semlalia, Marrakech, Morocco. [Boutouil, S.; Derkaoui, J. E.; Ouchrif, M.; Tayalati, Y.] Univ Mohamed Premier, Fac Sci, Oujda, Morocco. [Boutouil, S.; Derkaoui, J. E.; Ouchrif, M.; Tayalati, Y.] LPTPM, Oujda, Morocco. [El Moursli, R. Cherkaoui; Haddad, N.] Univ Mohammed V Agdal, Fac Sci, Rabat, Morocco. [Grillo, A. A.; Kuhl, A.; Litke, A. M.; Lockman, W. S.; Manning, P. M.; Nielsen, J.; Reece, R.; Sadrozinski, H. F-W; Schumm, B. A.; Seiden, A.] CEA Saclay, DSM IRFU, Inst Rech Lois Fondament Univers, Commissariat Energie Atom & Energies Alternati, F-91191 Gif Sur Yvette, France. [Grillo, A. A.; Kuhl, A.; Litke, A. M.; Lockman, W. S.; Manning, P. M.; Nielsen, J.; Sadrozinski, H. F-W; Schumm, B. A.; Seiden, A.] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA. [Beckingham, M.; Blackburn, D.; Coccaro, A.; Goussiou, A. G.; Harris, O. M.; Hsu, S-C; Lubatti, H. J.; Marx, M.; Rompotis, N.; Rosten, R.; De Bruin, P. H. Sales; Verducci, M.; Watts, G.] Univ Washington, Dept Phys, Seattle, WA 98195 USA. [Anastopoulos, C.; Costanzo, D.; Donszelmann, T. Cuhadar; Dawson, I.; Fletcher, G. T.; Hodgkinson, M. C.; Hodgson, P.; Johansson, P.; Korolkova, E. V.; Paredes, B. Lopez; Paganis, E.; Suruliz, K.; Tovey, D. R.; Tua, A.] Univ Sheffield, Dept Phys & Astron, Sheffield, S Yorkshire, England. [Hasegawa, Y.; Takeshita, T.] Shinshu Univ, Dept Phys, Nagano, Japan. [Atlay, N. B.; Buchholz, P.; Czirr, H.; Fleck, I.; Gaur, B.; Grybel, K.; Ikematsu, K.; Rammes, M.; Rosenthal, O.; Walkowiak, W.; Ziolkowski, M.] Univ Siegen, Fachbereich Phys, D-57068 Siegen, Germany. [Buat, Q.; Dawe, E.; Godfrey, J.; Kvita, J.; O'Neil, D. C.; Petteni, M.; Stelzer, B.; Tanasijczuk, A. J.; Torres, H.; Trottier-McDonald, M.; Van Nieuwkoop, J.; Vetterli, M. C.] Simon Fraser Univ, Dept Phys, Burnaby, BC V5A 1S6, Canada. [Aracena, I.; Mayes, J. Backus; Barklow, T.; Bawa, H. S.; Black, C. W.; Cogan, J. G.; Eifert, T.; Fulsom, B. G.; Gao, Y. S.; Garelli, N.; Kocian, M.; Koi, T.; Lowe, A. J.; Malone, C.; Mount, R.; Nelson, T. K.; Salnikov, A.; Strauss, E.; Su, D.; Swiatlowski, M.; Wittgen, M.; Young, C.] SLAC Natl Accelerator Lab, Stanford, CA USA. [Astalos, R.; Bartos, P.; Batkova, L.; Blazeka, T.; Federic, P.; Stavina, P.; Sykora, I.; Tokar, S.; Zenis, T.] Comenius Univ, Fac Math Phys & Informat, Bratislava, Slovakia. [Antos, J.; Bruncko, D.; Kladiva, E.; Strizenec, P.] Slovak Acad Sci, Inst Expt Phys, Dept Subnucl Phys, Kosice 04353, Slovakia. [Hamilton, A.] Univ Cape Town, Dept Phys, ZA-7925 Cape Town, South Africa. [Aurousseau, M.; Castaneda-Miranda, E.; Connelly, I. A.; Yacoob, S.] Univ Johannesburg, Dept Phys, Johannesburg, South Africa. [Bristow, K.; Carrillo-Montoya, G. D.; Chen, X.; Huang, Y.; Garcia, B. R. Mellado; Ruan, X.; Vickey, T.; Boeriu, O. E. Vickey] Univ Witwatersrand, Sch Phys, Johannesburg, South Africa. [Abulaitia, Y.; Aloisio, A.; Alonso, A.; Asman, B.; Bendtz, K.; Bessidskaia, O.; Bohm, C.; Clement, C.; Eriksson, D.; Gellerstedt, K.; Hellman, S.; Johansson, K. E.; Jon-And, K.; Khandanyan, H.; Kim, H.; Klimek, P.; Lundberg, O.; Moa, T.; Molander, S.; Petridis, A.; Plucinski, P.; Silverstein, S. B.; Sjolin, J.; Tylmad, M.] Stockholm Univ, Dept Phys, S-10691 Stockholm, Sweden. [Abulaitia, Y.; Asman, B.; Bendtz, K.; Bessidskaia, O.; Clement, C.; Gellerstedt, K.; Grosse-Knetter, J.; Jon-And, K.; Khandanyan, H.; Kim, H.; Klimek, P.; Lundberg, O.; Milstead, D. A.; Straessner, A.; Tylmad, M.] Oskar Klein Ctr, Stockholm, Sweden. [Jovicevic, J.; Kuwertz, E. S.; Lund-Jensen, B.; Morley, A. K.; Strandberg, J.] Royal Inst Technol, Dept Phys, S-10044 Stockholm, Sweden. [Bee, C. P.; Campoverde, A.; Chen, K.; Engelmann, R.; Grassi, V.; Hobbs, J.; Jia, J.; Lindquist, B. E.; Mastroberardino, A.; McCarthy, R. L.; Puldon, D.; Radhakrishnan, S. K.; Rijssenbeek, M.; Tsybychev, D.; Zaman, A.] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA. [Bee, C. P.; Campoverde, A.; Chen, C.; Engelmann, R.; Grassi, V.; Hobbs, J.; Jia, J.; Li, H.; Lindquist, B. E.; Mastrandrea, P.; Puldon, D.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.] SUNY Stony Brook, Dept Chem, Stony Brook, NY 11794 USA. [Bartsch, V.; Cerri, A.; Barajas, C. A. Chavez; De Santo, A.; Grout, Z. J.; Potter, C. J.; Rose, A.; Salvucci, A.; Castillo, I. Santoyo; Sutton, M. R.; Vivarelli, I.] Univ Sussex, Dept Phys & Astron, Brighton, E Sussex, England. [Bangert, A.; Black, C. W.; Cuthbert, C.; Finelli, K. D.; Jeng, G-Y; Patel, N. D.; Saavedra, A. F.; Scarcella, M.; Varvell, K. E.; Watson, I. J.; Yabsley, B.] Univ Sydney, Sch Phys, Sydney, NSW 2006, Australia. [Abdallah, J.; Chu, M. L.; Hou, S.; Jamin, D. O.; Lee, C. A.; Lee, S. C.; Lin, S. C.; Liu, B.; Lo Sterzo, F.; Mazini, R.; Ren, Z. L.; Soh, D. A.; Teng, P. K.; Wang, C.; Wang, S. M.; Weng, Z.; Zhang, L.] Acad Sinica, Inst Phys, Taipei, Taiwan. [Di Mattia, A.; Kopeliansky, R.; Musto, E.; Rozen, Y.; Tarem, S.] Technion Israel Inst Technol, Dept Phys, IL-32000 Haifa, Israel. [Abramowicz, H.; Alexander, G.; Amram, N.; Bella, G.; Benary, O.; Benhammou, Y.; Etzion, E.; Gershon, A.; Gueta, O.; Guttman, N.; Oren, Y.; Sadeh, I.; Silver, Y.; Soffer, A.; Taiblum, N.] Tel Aviv Univ, Raymond & Beverly Sackler Sch Phys & Astron, IL-69978 Tel Aviv, Israel. [Bachas, K.; Gkialas, I.; Iliadis, D.; Kordas, K.; Kouskoura, V.; Papageorgiou, K.; Petridou, C.; Sampsonidis, D.] Aristotle Univ Thessaloniki, Dept Phys, GR-54006 Thessaloniki, Greece. [Akimoto, G.; Aloisio, A.; Asai, S.; Azuma, Y.; Doherty, T.; Enari, Y.; Hanawa, K.; Kanaya, N.; Kataoka, Y.; Kawamura, G.; Kazama, S.; Kessoku, K.; Komori, Y.; Mashimo, T.; Ninomiya, Y.; Sakamoto, H.; Sasaki, O.; Tanaka, J.; Ueda, I.; Yamaguchi, H.; Yamaguchi, Y.; Yamamoto, A.; Yamamura, T.; Yamanaka, T.; Yoshihara, K.] Univ Tokyo, Int Ctr Elementary Particle Phys, Tokyo, Japan. [Bratzler, U.; Fukunaga, C.] Univ Tokyo, Dept Phys, Tokyo 113, Japan. [Bratzler, U.; Fukunaga, C.] Tokyo Metropolitan Univ, Grad Sch Sci & Technol, Tokyo 158, Japan. [Ishitsuka, M.; Jinnouchi, O.; Kanno, T.; Kuze, M.; Nagai, R.; Nobe, T.; Petteni, M.] Tokyo Inst Technol, Dept Phys, Tokyo 152, Japan. [AbouZeid, O. S.; Bailey, D. C.; Ilic, N.; Orr, R. S.; Polifka, R.; Rudolph, M. S.; Savard, P.; Schramm, S.; Sinervo, P.; Taenzer, J.; Teuscher, R. J.; Thompson, P. D.; Trischuk, W.; Venturi, N.] Univ Toronto, Dept Phys, Toronto, ON, Canada. [Canepa, A.; Chekulaev, S. V.; Fortin, D.; Koutsman, A.; Losty, M. J.; Codina, E. Perez; Schouten, D.; Seuster, R.; Stelzer-Chilton, O.; Tafirout, R.; Trigger, I. M.] TRIUMF, Vancouver, BC V6T 2A3, Canada. [Garcia, J. A. Benitez; Florez Bustos, A. C.; Ramos, J. A. Manjarres; Palacino, G.; Qureshi, A.; Taylor, W.] York Univ, Dept Phys & Astron, Toronto, ON M3J 2R7, Canada. [Hara, K.; Hayashi, T.; Kim, S. H.; Kiuchi, K.; Ukegawa, F.] Univ Tsukuba, Fac Pure & Appl Sci, Tsukuba, Ibaraki, Japan. [Beauchemin, P. H.; Hamilton, S.; Meoni, E.; Rolli, S.; Sliwa, K.; Wetter, J.] Tufts Univ, Dept Phys & Astron, Medford, MA 02155 USA. [Losada, M.; Mendoza Navas, L.; Navarro, G.; Sandoval, C.] Univ Antonio Narino, Ctr Invest, Bogota, Colombia. [Boscherini, D.; Corso-Radu, A.; Farrell, S.; Gerbaudo, D.; Lankford, A. J.; Mete, A. S.; Rao, K.; Scannicchio, D. A.; Shimmin, C. O.; Taffard, A.; Toggerson, B.; Unel, G.; Whiteson, D.; Zhou, N.] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA USA. [Acharya, B. S.; Alhroob, M.; Brazzale, S. F.; Cobal, M.; De Sanctis, U.; Giordani, M. P.; Pinamonti, M.; Quayle, W. B.; Shaw, K.; Soualah, R.] Ist Nazl Fis Nucl, Grp Collegato Udine, Sez Trieste, Udine, Italy. [Acharya, B. S.; Quayle, W. B.; Shaw, K.] Abdus Salaam Int Ctr Theoret Phys, Trieste, Italy. [Alhroob, M.; Cobal, M.; De Sanctis, U.; Giordani, M. P.; Pinamonti, M.; Soualah, R.] Univ Udine, Dipartimento Chim Fis & Ambiente, I-33100 Udine, Italy. [Atkinson, M.; Basye, A.; Benekos, N.; Cavaliere, V.; Chang, P.; Coggeshall, J.; Errede, D.; Lie, K.; Liss, T. M.; Neubauer, M. S.; Vichou, I.] Univ Illinois, Dept Phys, Urbana, IL 61801 USA. [Brennan, A. J.; Buszello, C. P.; Coniavitis, E.; Ekelof, T.; Ferrari, A.; Isaksson, C.; Madsen, A.; Ohman, H.; Pelikan, D.] Uppsala Univ, Dept Phys & Astron, Uppsala, Sweden. [Cabrera Urban, S.; Castillo Gimenez, V.; Cortes-Gonzalez, A.; Costa, M. J.; Fassi, F.; Ferrer, A.; Garcia, C.; March, L.; Moles-Valls, R.; Damazio, D. Oliveira; Hernandez, D. Paredes; Pedraza Lopez, S.; Codina, E. Perez; Ros, E.; Salt, J.; Sanchez, A.; Sanchez Martinez, V.; Soldevila, U.; Torro Pastor, E.; Valero, A.; Valladolid Gallego, E.; Valls Ferrer, J. A.; Villaplana Perez, M.; Vos, M.] Univ Valencia, Inst Fis Corpuscular, IFIC, Valencia, Spain. [Cabrera Urban, S.; Castillo Gimenez, V.; Costa, G.; Fassi, F.; Ferrer, A.; Fuster, J.; Garcia, C.; Garcia Navarro, J. E.; Gonzalez Parra, G.; Higon-Rodriguez, E.; Irles Quiles, A.; Kaci, M.; Lacasta, C.; March, L.; Perez Garcia-Estan, M. T.; Romeo, G.; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, A.; Sanchez Martinez, V.; Soldevila, U.; Valero, A.; Valladolid Gallego, E.; Valls Ferrer, J. A.; Villaplana Perez, M.; Vos, M.] Univ Valencia, Dept Fis Atom Mol & Nucl, Valencia, Spain. [Cabrera Urban, S.; Castillo Gimenez, V.; Costa, G.; De Sanctis, U.; Fassi, F.; Fiorini, L.; Fuster, J.; Garcia, C.; Gonzalez Parra, G.; Higon-Rodriguez, E.; Irles Quiles, A.; Kaci, M.; King, M.; Lacasta, C.; March, L.; Latour, B. Martin dit; Moles-Valls, R.; Pedraza Lopez, S.; Perez Garcia-Estan, M. T.; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, A.; Soldatov, E. Yu; Valls Ferrer, J. A.; Villaplana Perez, M.; Vos, M.] Univ Valencia, Dept Ingn Elect, Valencia, Spain. [Cabrera Urban, S.; Castillo Gimenez, V.; Costa, M. J.; Fassi, F.; Ferrari, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Garcia Navarro, J. E.; Hernandez Jimenez, Y.; Higon-Rodriguez, E.; Kaci, M.; King, B. T.; King, M.; Lacuesta, V. R.; March, L.; Marchese, F.; Minaenko, A. A.; Mitsou, V. A.; Moles-Valls, R.; Perez Garcia-Estan, M. T.; Ros, E.; Sanchez, A.; Sanchez Martinez, V.; Soldevila, U.; Villaplana Perez, M.; Vos, M.] Univ Valencia, Inst Microelect Barcelona, IMB CNM, Valencia, Spain. [Cabrera Urban, S.; Castillo Gimenez, V.; Costa, G.; De Santo, A.; Ferrari, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Garcia Navarro, J. E.; Hernandez Jimenez, Y.; Kaci, M.; Lacasta, C.; Martinez, H.; Minano Moya, M.; Oliver Garcia, E.; Perez Garcia-Estan, M. T.; Romero Adam, E.; Rose, A.; Salt, J.; Sanchez, J.] CSIC, Valencia, Spain. [Fedorko, W.; Gay, C.; Gecse, Z.; King, B. T.; King, M.; Lister, A.; Loh, C. W.; Swedish, S.; Viel, S.] Univ British Columbia, Dept Phys, Vancouver, BC, Canada. [Albert, J.; Bansal, V.; Berghaus, F.; David, C.; Fincke-Keeler, M.; Keeler, R.; Kowalewski, R.; Lefebvre, G.; Marino, C. P.; McPherson, R. A.; Ouellette, E. A.; Pearce, J.; Sobie, R.] Univ Victoria, Dept Phys & Astron, Victoria, BC, Canada. [Farrington, S. M.; Harrington, R. D.; Janus, M.; Jeske, C.; Jones, G.; Martin, B.; Murray, W. J.; Pianori, E.] Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England. [Iizawa, T.; Kimura, N.; Mitani, T.; Sakurai, Y.; Yorita, K.] Waseda Univ, Tokyo, Japan. [Alon, R.; Barak, L.; Bressler, S.; Citron, Z. H.; Groth-Jensen, J.; Lellouch, D.; Levinson, L. J.; Mikestikova, M.; Milstead, D. A.; Roth, I.; Smakhtin, V.; Vitells, O.; Wotschack, J.] Weizmann Inst Sci, Dept Particle Phys, IL-76100 Rehovot, Israel. [Banerjee, Sw; Castillo, L. R. Flores; Hard, A. S.; Ji, H.; Ju, X.; Kashif, L.; Kruse, A.; Ming, Y.; Dos Santos, D. Roda; Wiedenmann, W.; Wu, S. L.; Yang, H.; Zhang, F.; Zobernig, G.] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA. [Fleischmann, P.; Redelbach, A.; Schreyer, M.; Siragusa, G.; Stroehmer, R.; Trefzger, T.; Weber, S. W.] Univ Wurzburg, Fak Phys & Astron, D-97070 Wurzburg, Germany. [Barisonzi, M.; Becker, K.; Beermann, T. A.; Boek, J.; Boek, T. T.; Braun, H. M.; Cornelissen, T.; Duda, D.; Ernis, G.; Fischer, J.; Flick, T.; Gorisek, A.; Heim, T.; Hirschbuehl, D.; Kersevan, B. P.; Kohlmann, S.; Lenzen, G.; Maettig, P.; Pataraia, S.; Sandhoff, M.; Sartisohn, G.; Wagner, P.; Zeitnitz, C.] Berg Univ Wuppertal, Fachbereich C Phys, Wuppertal, Germany. [Adelman, J.; Baker, O. K.; Bedikian, S.; Cummings, J.; Czyczula, Z.; Demers, S.; Erdmann, J.; Garberson, F.; Golling, T.; Ideal, E.; Lagouri, T.; Lee, L.; Loginov, A.; Tipton, P.; Wall, R.; Walsh, B.; Wang, X.] Yale Univ, Dept Phys, New Haven, CT USA. [Hakobyan, H.; Vardanyan, G.] Yerevan Phys Inst, Yerevan 375036, Armenia. [Rahal, G.] Ctr Calcul Inst Natl Phys Nucl & Phys Particules, IN2P3, Villeurbanne, France. [Acharya, B. S.] Kings Coll London, Dept Phys, London, England. [Bawa, H. S.; Gao, Y. S.; Lowe, A. J.] Calif State Univ Fresno, Dept Phys, Fresno, CA 93740 USA. [Chelkov, G. A.] Tomsk State Univ, Tomsk 634050, Russia. [Della Pietra, M.] Univ Napoli Parthenope, Naples, Italy. [Corriveau, F.; Robertson, S. H.; Sobie, R.; Teuscher, R. J.] Inst Particle Phys, Waterloo, ON, Canada. [Demirkoz, B.] Middle E Tech Univ, Dept Phys, TR-06531 Ankara, Turkey. [Fedin, O. L.] St Petersburg State Polytech Univ, Dept Phys, St Petersburg, Russia. [Fiolhais, M. C. N.] Univ Coimbra, Dept Phys, Coimbra, Portugal. [Castillo, L. R. Flores] Chinese Univ Hong Kong, Hong Kong, Hong Kong, Peoples R China. [Gkialas, I.; Papageorgiou, K.] Univ Aegean, Dept Financial & Management Engn, Chios, Greece. [Grinstein, S.; Juste Rozas, A.; Martinez, M.] ICREA, Inst Catalana Recerca & Estudis Avancats, Barcelona, Spain. [Kono, T.] Ochanomizu Univ, Ochadai Acad Prod, Tokyo 112, Japan. [Konoplich, R.] Manhattan Coll, New York, NY USA. [Liang, Z.; Soh, D. A.; Weng, Z.] Sun Yat Sen Univ, Sch Phys & Engn, Guangzhou 510275, Guangdong, Peoples R China. [Lin, S. C.] Acad Sinica, Inst Phys, Acad Sinica Grid Comp, Taipei, Taiwan. [Mal, P.] Natl Inst Sci Educ & Res, Sch Phys Sci, Bhubaneswar, Orissa, India. [Myagkov, A. G.; Nikolaenko, V.; Zaitsev, A. M.] Moscow Inst Phys & Technol, Dolgoprudnyi, Russia. [Onyisi, P. U. E.] Univ Texas Austin, Dept Phys, Austin, TX 78712 USA. [Pinamonti, M.] SISSA, Int Sch Adv Studies, I-34014 Trieste, Italy. [Purohit, M.] Univ S Carolina, Dept Phys & Astron, Columbia, SC 29208 USA. [Wildt, M. A.] Univ Hamburg, Inst Experimentalphys, Hamburg, Germany. [Yacoob, S.] Univ KwaZulu Natal, Discipline Phys, Durban, South Africa. RP Aad, G (reprint author), Aix Marseille Univ, CPPM, Marseille, France. RI Fassi, Farida/F-3571-2016; Fabbri, Laura/H-3442-2012; Solodkov, Alexander/B-8623-2017; Zaitsev, Alexandre/B-8989-2017; Peleganchuk, Sergey/J-6722-2014; Yang, Haijun/O-1055-2015; Monzani, Simone/D-6328-2017; Grancagnolo, Francesco/K-2857-2015; Korol, Aleksandr/A-6244-2014; Capua, Marcella/A-8549-2015; Tartarelli, Giuseppe Francesco/A-5629-2016; Solfaroli Camillocci, Elena/J-1596-2012; Vanadia, Marco/K-5870-2016; Ippolito, Valerio/L-1435-2016; Mora Herrera, Maria Clemencia/L-3893-2016; Maneira, Jose/D-8486-2011; Prokoshin, Fedor/E-2795-2012; KHODINOV, ALEKSANDR/D-6269-2015; Canelli, Florencia/O-9693-2016; Staroba, Pavel/G-8850-2014; Goncalo, Ricardo/M-3153-2016; Gauzzi, Paolo/D-2615-2009; Mindur, Bartosz/A-2253-2017; Gonzalez de la Hoz, Santiago/E-2494-2016; Guo, Jun/O-5202-2015; Aguilar Saavedra, Juan Antonio/F-1256-2016; Wemans, Andre/A-6738-2012; Leyton, Michael/G-2214-2016; Jones, Roger/H-5578-2011; Vranjes Milosavljevic, Marija/F-9847-2016; Perrino, Roberto/B-4633-2010; SULIN, VLADIMIR/N-2793-2015; Nechaeva, Polina/N-1148-2015; Vykydal, Zdenek/H-6426-2016; Olshevskiy, Alexander/I-1580-2016; Snesarev, Andrey/H-5090-2013; Shmeleva, Alevtina/M-6199-2015; Gavrilenko, Igor/M-8260-2015; Tikhomirov, Vladimir/M-6194-2015; Chekulaev, Sergey/O-1145-2015; Warburton, Andreas/N-8028-2013; Gorelov, Igor/J-9010-2015; Gladilin, Leonid/B-5226-2011; Carvalho, Joao/M-4060-2013; Demirkoz, Bilge/C-8179-2014; Mashinistov, Ruslan/M-8356-2015; Buttar, Craig/D-3706-2011; Cabrera Urban, Susana/H-1376-2015; Mir, Lluisa-Maria/G-7212-2015; Garcia, Jose /H-6339-2015; Marti-Garcia, Salvador/F-3085-2011; Della Pietra, Massimo/J-5008-2012; Cavalli-Sforza, Matteo/H-7102-2015; Petrucci, Fabrizio/G-8348-2012; Negrini, Matteo/C-8906-2014; Ferrer, Antonio/H-2942-2015; Grancagnolo, Sergio/J-3957-2015; Doyle, Anthony/C-5889-2009; spagnolo, stefania/A-6359-2012; Ciubancan, Liviu Mihai/L-2412-2015; Mitsou, Vasiliki/D-1967-2009; Riu, Imma/L-7385-2014; Ventura, Andrea/A-9544-2015; Di Domenico, Antonio/G-6301-2011; Livan, Michele/D-7531-2012; De, Kaushik/N-1953-2013; Moraes, Arthur/F-6478-2010; Smirnova, Oxana/A-4401-2013; Villa, Mauro/C-9883-2009; Brooks, William/C-8636-2013; Bosman, Martine/J-9917-2014; Joergensen, Morten/E-6847-2015 OI Fassi, Farida/0000-0002-6423-7213; Osculati, Bianca Maria/0000-0002-7246-060X; Amorim, Antonio/0000-0003-0638-2321; Coccaro, Andrea/0000-0003-2368-4559; Fabbri, Laura/0000-0002-4002-8353; Solodkov, Alexander/0000-0002-2737-8674; Zaitsev, Alexandre/0000-0002-4961-8368; Peleganchuk, Sergey/0000-0003-0907-7592; Monzani, Simone/0000-0002-0479-2207; Grancagnolo, Francesco/0000-0002-9367-3380; Korol, Aleksandr/0000-0001-8448-218X; Giordani, Mario/0000-0002-0792-6039; Capua, Marcella/0000-0002-2443-6525; Tartarelli, Giuseppe Francesco/0000-0002-4244-502X; Solfaroli Camillocci, Elena/0000-0002-5347-7764; Vanadia, Marco/0000-0003-2684-276X; Ippolito, Valerio/0000-0001-5126-1620; Mora Herrera, Maria Clemencia/0000-0003-3915-3170; Maneira, Jose/0000-0002-3222-2738; Prokoshin, Fedor/0000-0001-6389-5399; KHODINOV, ALEKSANDR/0000-0003-3551-5808; Canelli, Florencia/0000-0001-6361-2117; Goncalo, Ricardo/0000-0002-3826-3442; Gauzzi, Paolo/0000-0003-4841-5822; Mindur, Bartosz/0000-0002-5511-2611; Gonzalez de la Hoz, Santiago/0000-0001-5304-5390; Guo, Jun/0000-0001-8125-9433; Aguilar Saavedra, Juan Antonio/0000-0002-5475-8920; Wemans, Andre/0000-0002-9669-9500; Leyton, Michael/0000-0002-0727-8107; Jones, Roger/0000-0002-6427-3513; Vranjes Milosavljevic, Marija/0000-0003-4477-9733; Perrino, Roberto/0000-0002-5764-7337; SULIN, VLADIMIR/0000-0003-3943-2495; Vykydal, Zdenek/0000-0003-2329-0672; Olshevskiy, Alexander/0000-0002-8902-1793; Tikhomirov, Vladimir/0000-0002-9634-0581; Warburton, Andreas/0000-0002-2298-7315; Gorelov, Igor/0000-0001-5570-0133; Gladilin, Leonid/0000-0001-9422-8636; Carvalho, Joao/0000-0002-3015-7821; Mashinistov, Ruslan/0000-0001-7925-4676; Mir, Lluisa-Maria/0000-0002-4276-715X; Della Pietra, Massimo/0000-0003-4446-3368; Petrucci, Fabrizio/0000-0002-5278-2206; Negrini, Matteo/0000-0003-0101-6963; Ferrer, Antonio/0000-0003-0532-711X; Grancagnolo, Sergio/0000-0001-8490-8304; Doyle, Anthony/0000-0001-6322-6195; spagnolo, stefania/0000-0001-7482-6348; Ciubancan, Liviu Mihai/0000-0003-1837-2841; Mitsou, Vasiliki/0000-0002-1533-8886; Riu, Imma/0000-0002-3742-4582; Ventura, Andrea/0000-0002-3368-3413; Di Domenico, Antonio/0000-0001-8078-2759; Livan, Michele/0000-0002-5877-0062; De, Kaushik/0000-0002-5647-4489; Moraes, Arthur/0000-0002-5157-5686; Smirnova, Oxana/0000-0003-2517-531X; Villa, Mauro/0000-0002-9181-8048; Brooks, William/0000-0001-6161-3570; Bosman, Martine/0000-0002-7290-643X; Joergensen, Morten/0000-0002-6790-9361 FU ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWF, Austria; FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq, Brazil; FAPESP, Brazil; NSERC, Canada; NRC, Canada; CFI, Canada; CERN; CONICYT, Chile; CAS, China; MOST, China; NSFC, China; COLCIENCIAS, Colombia; VSC CR, Czech Republic; MSMT CR, Czech Republic; MPO CR, Czech Republic; DNRF, Denmark; DNSRC, Denmark; Lundbeck Foundation, Denmark; EPLANET; ERC; NSRF; European Union; IN2P3-CNRS, France; CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, Germany; DFG, Germany; HGF, Germany; MPG, Germany; AvH Foundation, Germany; GSRT, Greece; NSRF, Greece; ISF, Israel; MINERVA, Israel; GIF, Israel; I-CORE and Benoziyo Center, Israel; INFN, Italy; MEXT, Japan; JSPS, Japan; CNRST, Morocco; FOM, Netherlands; NWO, Netherlands; BRF, Norway; RCN, Norway; MNiSW, Poland; NCN, Poland; GRICES, Portugal; FCT, Portugal; MNE/IFA, Romania; MES of Russia and ROSATOM; Russian Federation; JINR; MSTD, Serbia; MSSR, Slovakia; ARRS and MIZ Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC, Sweden; Wallenberg Foundation, Sweden; SER, Switzerland; SNSF, Switzerland; Cantons of Bern and Geneva, Switzerland; NSC, Taiwan; TAEK, Turkey; STFC, United Kingdom; Royal Society, United Kingdom; Leverhulme Trust, United Kingdom; DOE, United States of America; NSF, United States of America; TRIUMF (Canada); NDGF (Denmark, Norway, Sweden); KIT/ GridKA (Germany); INFN-CNAF (Italy); NL-Ti (Netherlands); PIC (Spain); ASGC (Taiwan); RAL (UK); BNL (USA); [CC-IN2P3] FX We thank CERN for the very successful operation of the LHC, as well as the support staff from our institutions without whom ATLAS could not be operated efficiently. We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWF and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile; CAS, MOST and NSFC, China; COLCIENCIAS, Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF, DNSRC and Lundbeck Foundation, Denmark; EPLANET, ERC and NSRF, European Union; IN2P3-CNRS, CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, DFG, HGF, MPG and AvH Foundation, Germany; GSRT and NSRF, Greece; ISF, MINERVA, GIF, I-CORE and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; FOM and NWO, Netherlands; BRF and RCN, Norway; MNiSW and NCN, Poland; GRICES and FCT, Portugal; MNE/IFA, Romania; MES of Russia and ROSATOM, Russian Federation; JINR; MSTD, Serbia; MSSR, Slovakia; ARRS and MIZ Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC and Wallenberg Foundation, Sweden; SER, SNSF and Cantons of Bern and Geneva, Switzerland; NSC, Taiwan; TAEK, Turkey; STFC, the Royal Society and Leverhulme Trust, United Kingdom; DOE and NSF, United States of America. The crucial computing support from all WLCG partners is acknowledged gratefully, in particular from CERN and the ATLAS Tier-1 facilities at TRIUMF (Canada), NDGF (Denmark, Norway, Sweden), CC-IN2P3 (France), KIT/ GridKA (Germany), INFN-CNAF (Italy), NL-Ti (Netherlands), PIC (Spain), ASGC (Taiwan), RAL (UK) and BNL (USA) and in the Tier-2 facilities worldwide. NR 45 TC 4 Z9 4 U1 6 U2 78 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 1367-2630 J9 NEW J PHYS JI New J. Phys. PD NOV 4 PY 2014 VL 16 AR 113013 DI 10.1088/1367-2630/16/11/113013 PG 34 WC Physics, Multidisciplinary SC Physics GA AX1MT UT WOS:000346711800007 ER PT J AU Kuo, A Kohler, A Martin, FM Grigoriev, IV AF Kuo, Alan Kohler, Annegret Martin, Francis M. Grigoriev, Igor V. TI Expanding genomics of rnycorrhizal symbiosis SO FRONTIERS IN MICROBIOLOGY LA English DT Review DE mycorrhizae; Laccaria; Tuber; Rhizophagus; Glomus ID FUNGUS LACCARIA-BICOLOR; ARBUSCULAR MYCORRHIZAL FUNGUS; TRUFFLE TUBER-MELANOSPORUM; FREE-LIVING MYCELIUM; GLOMUS-INTRARADICES; GENE FAMILY; CARBOHYDRATE-METABOLISM; PISOLITHUS-TINCTORIUS; STRUCTURAL ANNOTATION; EUCALYPTUS-GLOBULUS AB The mycorrhizal symbiosis between soil fungi and plant roots is a ubiquitous mutualism that plays key roles in plant nutrition, soil health, and carbon cycling. The symbiosis evolved repeatedly and independently as multiple morphotypes [e.g., arbuscular mycorrhizae (AM), ectomycorrhizal (ECM)] in multiple fungal clades (e.g., phyla Glomeromycota, Ascomycota, Basidiomycota). The accessibility and cultivability of many mycorrhizal partners make them ideal models for symbiosis studies. Alongside molecular, physiological, and ecological investigations, sequencing led to the first three mycorrhizal fungal genomes, representing two morphotypes and three phyla. The genome of the ECM basidiomycete Laccaria bicolor showed that the mycorrhizal lifestyle can evolve through loss of plant cell wall-degrading enzymes (PCWDEs) and expansion of lineage-specific gene families such as short secreted protein (SSP) effectors. The genome of the ECM ascomycete Tuber melanosporum showed that the ECM type can evolve without expansion of families as in Laccaria, and thus a different set of symbiosis genes. The genome of the AM glomeromycete Rhizophagus irregularis showed that despite enormous phylogenetic distance and morphological difference from the other two fungi, symbiosis can involve similar solutions as symbiosis-induced SSPs and loss of PCWDEs. The three genomes provide a solid base for addressing fundamental questions about the nature and role of a vital mutualism. C1 [Kuo, Alan; Grigoriev, Igor V.] US DOE, Joint Genome Inst, Walnut Creek, CA USA. [Kohler, Annegret; Martin, Francis M.] Univ Lorraine, INRA, UMR, Lab Excellence Adv Res Biol TRee & Forest Ecosyst, F-54280 Nancy, Champenoux, France. RP Martin, FM (reprint author), Univ Lorraine, INRA, UMR, Lab Excellence Adv Res Biol TRee & Forest Ecosyst, F-54280 Nancy, Champenoux, France. EM fmartin@nancy.inra.fr; ivgrigoriev@lbl.gov FU DOE Office of Science User Facility [DE-AC02-05CH11231]; Laboratory of Excellence ARBRE [ANR-11-LABX-0002-01]; Region Lorraine; Genomic Science Program (project "Plant-Microbe Interactions"), United States Department of Energy, Office of Science, Biological and Environmental Research [DE6 AC05-00OR22725] FX The work conducted by the United States Department of Energy Joint Genome Institute, a DOE Office of Science User Facility, was supported under Contract No DE-AC02-05CH11231. This work was supported by the Laboratory of Excellence ARBRE (ANR-11-LABX-0002-01), the Region Lorraine and the Genomic Science Program (project "Plant-Microbe Interactions"), United States Department of Energy, Office of Science, Biological and Environmental Research under the contract DE6 AC05-00OR22725. NR 76 TC 3 Z9 3 U1 8 U2 68 PU FRONTIERS RESEARCH FOUNDATION PI LAUSANNE PA PO BOX 110, LAUSANNE, 1015, SWITZERLAND SN 1664-302X J9 FRONT MICROBIOL JI Front. Microbiol. PD NOV 4 PY 2014 VL 5 AR 582 DI 10.3389/fmicb.2014.00582 PG 7 WC Microbiology SC Microbiology GA AU5GN UT WOS:000345635200003 PM 25408690 ER PT J AU Trexler, R Solomon, C Brislawn, CJ Wright, JR Rosenberger, A McClure, EE Grube, AM Peterson, MP Keddache, M Mason, OU Hazen, TC Grant, CJ Lamendella, R AF Trexler, Ryan Solomon, Caroline Brislawn, Colin J. Wright, Justin R. Rosenberger, Abigail McClure, Erin E. Grube, Alyssa M. Peterson, Mark P. Keddache, Mehdi Mason, Olivia U. Hazen, Terry C. Grant, Christopher J. Lamendella, Regina TI Assessing impacts of unconventional natural gas extraction on microbial communities in headwater stream ecosystems in Northwestern Pennsylvania SO FRONTIERS IN MICROBIOLOGY LA English DT Article DE marcellus shale; fracking; 16S rRNA gene sequencing; next generation sequencing; methanotrophs; beta diversity; acidophilic ID 16S RIBOSOMAL-RNA; ACID-MINE DRAINAGE; SHALE-GAS; BACTERIAL COMMUNITIES; WATER-QUALITY; MOUNTAIN STREAMS; NATIONAL-PARK; SOIL; NITROGEN; POPULATIONS AB Hydraulic fracturing and horizontal drilling have increased dramatically in Pennsylvania Marcellus shale formations, however the potential for major environmental impacts are still incompletely understood. High-throughput sequencing of the 16S rRNA gene was performed to characterize the microbial community structure of water, sediment, bryophyte, and biofilm samples from 26 headwater stream sites in northwestern Pennsylvania with different histories of fracking activity within Marcellus shale formations. Further, we describe the relationship between microbial community structure and environmental parameters measured. Approximately 3.2 million 16S rRNA gene sequences were retrieved from a total of 58 samples. Microbial community analyses showed significant reductions in species richness as well as evenness in sites with Marcellus shale activity. Beta diversity analyses revealed distinct microbial community structure between sites with and without Marcellus shale activity. For example, operational taxonomic units (OTUs) within the Acetobacteracea, Methylocystaceae, Acidobacteriaceae, and Phenylobacterium were greater than three log-fold more abundant in MSA+ sites as compared to MSA- sites. Further, several of these OTUs were strongly negatively correlated with pH and positively correlated with the number of wellpads in a watershed. It should be noted that many of the OTUs enriched in MSA+ sites are putative acidophilic and/or methanotrophic populations. This study revealed apparent shifts in the autochthonous microbial communities and highlighted potential members that could be responding to changing stream conditions as a result of nascent industrial activity in these aquatic ecosystems. C1 [Trexler, Ryan; Solomon, Caroline; Brislawn, Colin J.; Wright, Justin R.; Rosenberger, Abigail; McClure, Erin E.; Grube, Alyssa M.; Peterson, Mark P.; Grant, Christopher J.; Lamendella, Regina] Juniata Coll, Dept Biol, Huntingdon, PA 16652 USA. [Peterson, Mark P.] Penn State Univ, Dept Biol, University Pk, PA 16802 USA. [Peterson, Mark P.] Penn State Univ, Huck Inst Life Sci, University Pk, PA 16802 USA. [Keddache, Mehdi] Cincinnati Childrens Hosp Med Ctr, DNA Sequencing & Geotyping Facil, Cincinnati, OH 45229 USA. [Mason, Olivia U.] Florida State Univ, Dept Earth Ocean & Atmospher Sci, Tallahassee, FL 32306 USA. [Hazen, Terry C.] Univ Tennessee, Dept Civil & Environm Engn, Knoxville, TN USA. [Hazen, Terry C.] Oak Ridge Natl Lab, Biosci Div, Oak Ridge, TN USA. RP Lamendella, R (reprint author), Juniata Coll, 1700 Moore St, Huntingdon, PA 16652 USA. EM lamendella@juniata.edu RI Hazen, Terry/C-1076-2012; OI Hazen, Terry/0000-0002-2536-9993; Brislawn, Colin/0000-0002-9109-1950; Trexler, Ryan/0000-0002-8321-6127 FU Howard Hughes Medical Institute; National Science Foundation [DBI-1248096]; Colcom Foundation [20013355]; Juniata College; Department of Conservation and Natural Resources; Pennsylvania Game Commission [SFRA-1322]; PA Fish and Boat Commission [604] FX This research was supported by a grant to Juniata College from the Howard Hughes Medical Institute (http://www.hhmi.org) through the Precollege and Undergraduate Science Education Program, the National Science Foundation (www.nsf.gov), NSF Award # DBI-1248096, the Colcom Foundation (http://www.colcomfdn.org), Award #20013355, and startup funds to Regina Lamendella from Juniata College (www.juniata.edu). Stream study sites were all located on public lands, and appropriate permits were acquired through the Department of Conservation and Natural Resources (http://www.dcnr.state.pa.us) and the Pennsylvania Game Commission, SFRA-1322 (http://www.pgc.state.pa.us/portal/server.pt/community/pgc/9106). Permits were acquired through the PA Fish and Boat Commission (Permit #604) to conduct all aquatic research described. All permits are available upon request at Juniata College. We would like to acknowledge Christine Walls and Susan Pierotti for their technical assistance, Kristen Brubaker for the map generation, Krista Leibensperger for help with study site selection, and Nicole Marks, Alex Weimer, and Jacob Oster for help with chemical measurements. NR 82 TC 5 Z9 5 U1 10 U2 109 PU FRONTIERS RESEARCH FOUNDATION PI LAUSANNE PA PO BOX 110, LAUSANNE, 1015, SWITZERLAND SN 1664-302X J9 FRONT MICROBIOL JI Front. Microbiol. PD NOV 4 PY 2014 VL 5 AR 522 DI 10.3389/fmicb.2014.00522 PG 13 WC Microbiology SC Microbiology GA AU5FZ UT WOS:000345633800001 PM 25408683 ER PT J AU Shin, AC Fasshauer, M Filatova, N Grundell, LA Zielinski, E Zhou, JY Scherer, T Lindtner, C White, PJ Lapworth, AL Ilkayeva, O Knippschild, U Wolf, AM Scheja, L Grove, KL Smith, RD Qian, WJ Lynch, CJ Newgard, CB Buettner, C AF Shin, Andrew C. Fasshauer, Martin Filatova, Nika Grundell, Linus A. Zielinski, Elizabeth Zhou, Jian-Ying Scherer, Thomas Lindtner, Claudia White, Phillip J. Lapworth, Amanda L. Ilkayeva, Olga Knippschild, Uwe Wolf, Anna M. Scheja, Ludger Grove, Kevin L. Smith, Richard D. Qian, Wei-Jun Lynch, Christopher J. Newgard, Christopher B. Buettner, Christoph TI Brain Insulin Lowers Circulating BCAA Levels by Inducing Hepatic BCAA Catabolism SO CELL METABOLISM LA English DT Article ID AMINO-ACID-METABOLISM; ADIPOSE-TISSUE LIPOLYSIS; REGULATES FOOD-INTAKE; BRANCHED-CHAIN; GLUCOSE-PRODUCTION; POTENTIAL ROLE; RESISTANCE; LEUCINE; PLASMA; OBESITY AB Circulating branched-chain amino acid (BCAA) levels are elevated in obesity/ diabetes and are a sensitive predictor for type 2 diabetes. Here we show in rats that insulin dose-dependently lowers plasma BCAA levels through induction of hepatic protein expression and activity of branched-chain alpha-keto acid dehydrogenase (BCKDH), the rate-limiting enzyme in the BCAA degradation pathway. Selective induction of hypothalamic insulin signaling in rats and genetic modulation of brain insulin receptors in mice demonstrate that brain insulin signaling is a major regulator of BCAA metabolism by inducing hepatic BCKDH. Short-term overfeeding impairs the ability of brain insulin to lower BCAAs in rats. High-fat feeding in nonhuman primates and obesity and/or diabetes in humans is associated with reduced BCKDH protein in liver. These findings support the concept that decreased hepatic BCKDH is a major cause of increased plasma BCAAs and that hypothalamic insulin resistance may account for impaired BCAA metabolism in obesity and diabetes. C1 [Shin, Andrew C.; Fasshauer, Martin; Filatova, Nika; Grundell, Linus A.; Zielinski, Elizabeth; Scherer, Thomas; Lindtner, Claudia; Buettner, Christoph] Icahn Sch Med Mt Sinai, Dept Med, Diabet Obes & Metab Inst, New York, NY 10029 USA. [Zhou, Jian-Ying; Smith, Richard D.; Qian, Wei-Jun] Pacific NW Natl Lab, Biol Sci Div, Richland, WA 99352 USA. [White, Phillip J.; Lapworth, Amanda L.; Ilkayeva, Olga; Newgard, Christopher B.] Duke Univ, Med Ctr, Sarah W Stedman Nutr & Metab Ctr, Durham, NC 27710 USA. [White, Phillip J.; Lapworth, Amanda L.; Ilkayeva, Olga; Newgard, Christopher B.] Duke Univ, Med Ctr, Duke Mol Physiol Inst, Durham, NC 27710 USA. [Knippschild, Uwe; Wolf, Anna M.] Univ Ulm, Dept Gen & Visceral Surg, D-89081 Ulm, Germany. [Scheja, Ludger] Univ Med Ctr Hamburg Eppendorf, Dept Biochem & Mol Cell Biol, D-20246 Hamburg, Germany. [Grove, Kevin L.] Oregon Natl Primate Res Ctr, Div Diabet Obes & Metab, Beaverton, OR 97006 USA. [Lynch, Christopher J.] Penn State Univ, Coll Med, Hershey, PA 17033 USA. RP Buettner, C (reprint author), Icahn Sch Med Mt Sinai, Dept Med, Diabet Obes & Metab Inst, One Gustave L Levy Pl, New York, NY 10029 USA. EM christoph.buettner@mssm.edu RI Smith, Richard/J-3664-2012; OI Smith, Richard/0000-0002-2381-2349; White, Phillip/0000-0002-0957-425X FU NIH [DK074873, DK083568, DK082724, K01 DK099463, P51 OD011092, P41 GM103493]; Boehringer Ingelheim Foundation; DOE [DE-AC05-76RLO 1830] FX We would like to thank James D. O'Hare, Tiffany Chi, Seta Degann, Brian Closs, Adam Spitz, and Lee Honig for their technical assistance and Dr. Charles V. Mobbs and Elizabeth Schwartz for help with the C. elegans study. This study was supported by NIH grants DK074873, DK083568, DK082724 (C. B.), K01 DK099463 (A. C. S.), P51 OD011092 (K. L. G.), and P41 GM103493 (R. D. S.) and by the Boehringer Ingelheim Foundation (M. F.). Proteomic analysis was performed in the Environmental Molecular Sciences Laboratory (EMSL), a DOE national scientific user facility located at Pacific Northwest National Laboratory, which is operated by Battelle Memorial Institute under contract DE-AC05-76RLO 1830. NR 48 TC 17 Z9 17 U1 3 U2 16 PU CELL PRESS PI CAMBRIDGE PA 600 TECHNOLOGY SQUARE, 5TH FLOOR, CAMBRIDGE, MA 02139 USA SN 1550-4131 EI 1932-7420 J9 CELL METAB JI Cell Metab. PD NOV 4 PY 2014 VL 20 IS 5 BP 898 EP 909 DI 10.1016/j.cmet.2014.09.003 PG 12 WC Cell Biology; Endocrinology & Metabolism SC Cell Biology; Endocrinology & Metabolism GA AT4YF UT WOS:000344947800023 PM 25307860 ER PT J AU Hellmich, J Bommer, M Burkhardt, A Ibrahim, M Kern, J Meents, A Muh, F Dobbek, H Zouni, A AF Hellmich, Julia Bommer, Martin Burkhardt, Anja Ibrahim, Mohamed Kern, Jan Meents, Alke Mueh, Frank Dobbek, Holger Zouni, Athina TI Native-like Photosystem II Superstructure at 2.44 angstrom Resolution through Detergent Extraction from the Protein Crystal SO STRUCTURE LA English DT Article ID MEMBRANE-PROTEIN; MACROMOLECULAR CRYSTALLOGRAPHY; THERMOSYNECHOCOCCUS-ELONGATUS; ROOM-TEMPERATURE; WATER OXIDATION; CRYSTALLIZATION; DIFFRACTION; LIPIDS; CYANOBACTERIAL; ORGANIZATION AB Photosystem II (PSII) catalyzes a key step in photosynthesis, the oxidation of water to oxygen. Excellent structural models exist for the dimeric PSII core complex of cyanobacteria, but higher order physiological assemblies readily dissociate when solubilized from the native thylakoid membrane with detergent. Here, we describe the crystallization of PSII from Thermosynechococcus elongatus with a postcrystallization treatment involving extraction of the detergent C12E8. This resulted in a transition from Type II to Type I-like membrane protein crystals and improved diffraction to 2.44 angstrom resolution. The obtained PSII packing in precise rows, interconnected by specific pairs of galactolipids and a loop in the PsbO subunit specific to cyanobacteria, is superimposable with previous electron microscopy images of the thylakoid membrane. The study provides a detailed model of such a superstructure and its organization of light-harvesting pigments with possible implications for the understanding of their efficient use of solar energy. C1 [Hellmich, Julia; Bommer, Martin; Ibrahim, Mohamed; Dobbek, Holger; Zouni, Athina] Humboldt Univ, Inst Biol, D-10095 Berlin, Germany. [Burkhardt, Anja; Meents, Alke] DESY, D-22607 Hamburg, Germany. [Kern, Jan] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Phys Biosci Div, Berkeley, CA 94720 USA. [Kern, Jan] SLAC Natl Accelerator Lab, Linac Coherence Light Source, Menlo Pk, CA 94025 USA. [Mueh, Frank] Johannes Kepler Univ Linz, Inst Theoret Phys, A-4040 Linz, Austria. RP Bommer, M (reprint author), Humboldt Univ, Inst Biol, Unter den Linden 6, D-10095 Berlin, Germany. EM martin.bommer@hu-berlin.de; athina.zouni@hu-berlin.de RI Kern, Jan/G-2586-2013 OI Kern, Jan/0000-0002-7272-1603 FU Deutsche Forschungsgemeinschaft [SFB 1078]; Cluster of Excellence "Unifying Concepts in Catalysis''; Technische Universitat Berlin [E3/D3]; Human Frontier Science Program Organization (USA); Humboldt Universitat zu Berlin through the Joint Berlin MX-Laboratory FX We are indebted to Professor Egbert Boekema (University of Groningen) for providing electron micrographs. Portions of this research were carried out at beamline P11 at the light source PETRA III at DESY, a member of the Helmholtz Association. HPF experiments were performed at DESY (Hamburg, Germany) and at the Heinrich Pette Institute, Leibniz Institute for Experimental Virology (Hamburg, Germany). We thank the beamline staff of P11 and Martin Warmer, Heinrich Hohenberg, and Rudolph Reimer for assistance in HPF. We thank the beamline staff of the BESSY II electron storage ring (Berlin-Adlershof, Germany) for helpful and competent support. Thanks to Dr. Chris Weise, S. Kussin, and D. DiFiore for technical support; and to Dr. Jae-Hun Jeoung for help in generating geometry restraints for crystallographic refinement of ligands. We thank Professor Wolfram Saenger for critical reading of the manuscript. This work was supported by Deutsche Forschungsgemeinschaft through SFB 1078 (Project A5) and the Cluster of Excellence "Unifying Concepts in Catalysis'' coordinated by the Technische Universitat Berlin (Project E3/D3), the Human Frontier Science Program Organization (USA, grant to A.Z.), as well as the Humboldt Universitat zu Berlin through the Joint Berlin MX-Laboratory. NR 41 TC 17 Z9 17 U1 1 U2 26 PU CELL PRESS PI CAMBRIDGE PA 600 TECHNOLOGY SQUARE, 5TH FLOOR, CAMBRIDGE, MA 02139 USA SN 0969-2126 EI 1878-4186 J9 STRUCTURE JI Structure PD NOV 4 PY 2014 VL 22 IS 11 BP 1607 EP 1615 DI 10.1016/j.str.2014.09.007 PG 9 WC Biochemistry & Molecular Biology; Biophysics; Cell Biology SC Biochemistry & Molecular Biology; Biophysics; Cell Biology GA AT4TG UT WOS:000344934300008 PM 25438669 ER PT J AU Shvartsburg, AA AF Shvartsburg, Alexandre A. TI Ultrahigh-Resolution Differential Ion Mobility Separations of Conformers for Proteins above 10 kDa: Onset of Dipole Alignment? SO ANALYTICAL CHEMISTRY LA English DT Article ID MOLECULAR-DYNAMICS SIMULATIONS; UNSOLVATED CYTOCHROME-C; ESI-FAIMS-MS; GAS-PHASE; MASS-SPECTROMETRY; LIQUID-CHROMATOGRAPHY; CROSS-SECTIONS; HISTONE CODE; IN-VACUO; CONFORMATIONS AB Biomacromolecules tend to assume numerous structures in solution or the gas phase. It has been possible to resolve disparate conformational families but not unique geometries within each, and drastic peak broadening has been the bane of protein analyses by chromatography, electrophoresis, and ion mobility spectrometry (IMS). The new differential or field asymmetric waveform IMS (FAIMS) approach using hydrogen-rich gases was recently found to separate conformers of a small protein ubiquitin with the same peak width and resolving power up to similar to 400 as for peptides. The present work explores the reach of this approach for larger proteins, exemplified by cytochrome c and myoglobin. Resolution similar to that for ubiquitin was largely achieved with longer separations, while the onset of peak broadening and coalescence with shorter separations suggests the limitation of the present technique to proteins under similar to 20 kDa. This capability may enable one to distinguish whole proteins with differing residue sequences or localizations of post-translational modifications. Small features at negative compensation voltages that markedly grow from cytochrome c to myoglobin indicate the dipole alignment of rare conformers in accord with theory, further supporting the concept of pendular macroions in FAIMS. C1 [Shvartsburg, Alexandre A.] Pacific NW Natl Lab, Div Biol Sci, Richland, WA 99352 USA. RP Shvartsburg, AA (reprint author), Wichita State Univ, Dept Chem, 1845 Fairmount, Wichita, KS 67260 USA. EM alexandre.shvartsburg@wichita.edu FU PNNL Technology Commercialization Office and Laboratory-Directed Research & Development program FX We thank Ron Moore for experimental help and Professors David E. Clemmer and Joseph A. Loo for insightful discussions. This work was funded by the PNNL Technology Commercialization Office and Laboratory-Directed Research & Development program and carried out in the Environmental Molecular Sciences Laboratory, a DOE national scientific user facility at PNNL. NR 51 TC 7 Z9 7 U1 3 U2 49 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0003-2700 EI 1520-6882 J9 ANAL CHEM JI Anal. Chem. PD NOV 4 PY 2014 VL 86 IS 21 BP 10608 EP 10615 DI 10.1021/ac502389a PG 8 WC Chemistry, Analytical SC Chemistry GA AS8PK UT WOS:000344510200018 PM 25340280 ER PT J AU Huang, GY Gerlits, OO Blakeley, MP Sankaran, B Kovalevsky, AY Kim, C AF Huang, Gilbert Y. Gerlits, Oksana O. Blakeley, Matthew P. Sankaran, Banumathi Kovalevsky, Andrey Y. Kim, Choel TI Neutron Diffraction Reveals Hydrogen Bonds Critical for cGMP-Selective Activation: Insights for cGMP-Dependent Protein Kinase Agonist Design SO BIOCHEMISTRY LA English DT Article ID REGULATORY SUBUNIT; CRYSTAL-STRUCTURE; CARNEY COMPLEX; BINDING; MUTATIONS; PKA AB High selectivity of cyclic-nucleotide binding (CNB) domains for cAMP and cGMP are required for segregating signaling pathways; however, the mechanism of selectivity remains unclear. To investigate the mechanism of high selectivity in cGMP-dependent protein kinase (PKG), we determined a room-temperature joint X-ray/neutron (XN) structure of PKG I beta CNB-B, a domain 200-fold selective for cGMP over cAMP, bound to cGMP (2.2 angstrom), and a low-temperature X-ray structure of CNB-B with cAMP (1.3 angstrom). The XN structure directly describes the hydrogen bonding interactions that modulate high selectivity for cGMP, while the structure with cAMP reveals that all these contacts are disrupted, explaining its low affinity for cAMP. C1 [Huang, Gilbert Y.; Kim, Choel] Baylor Coll Med, Verna & Mars McClean Dept Biochem & Mol Biol, Houston, TX 77004 USA. [Gerlits, Oksana O.; Kovalevsky, Andrey Y.] Oak Ridge Natl Lab, Biol & Soft Matter Div, Oak Ridge, TN 37831 USA. [Blakeley, Matthew P.] Inst Max Von Laue Paul Langevin, F-38000 Grenoble, France. [Sankaran, Banumathi] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley Ctr Struct Biol, Berkeley, CA 94720 USA. [Kim, Choel] Baylor Coll Med, Dept Pharmacol, Houston, TX 77004 USA. RP Kim, C (reprint author), Baylor Coll Med, Verna & Mars McClean Dept Biochem & Mol Biol, One Baylor Plaza, Houston, TX 77004 USA. EM ckim@bcm.edu RI Blakeley, Matthew/G-7984-2015; OI Blakeley, Matthew/0000-0002-6412-4358; Kovalevsky, Andrey/0000-0003-4459-9142 FU NIH [R01GM090161, T32GM008280]; DOE Office of Basic Sciences; DOE [DE-AC02-05CH11231]; NIGMS; HHMI FX This work was supported by NIH Grants R01GM090161 (to C.K.) and T32GM008280 (to G.Y.H.). O.O.G. and A.Y.K. are supported by the DOE Office of Basic Sciences. The Advanced Light Source is supported by DOE Contract No. DE-AC02-05CH11231, the NIGMS, and the HHMI. NR 19 TC 9 Z9 9 U1 1 U2 12 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0006-2960 J9 BIOCHEMISTRY-US JI Biochemistry PD NOV 4 PY 2014 VL 53 IS 43 BP 6725 EP 6727 DI 10.1021/bi501012v PG 3 WC Biochemistry & Molecular Biology SC Biochemistry & Molecular Biology GA AS8PL UT WOS:000344510300001 PM 25271401 ER PT J AU Alessi, DS Lezama-Pacheco, JS Janot, N Suvorova, EI Cerrato, JM Giammar, DE Davis, JA Fox, PM Williams, KH Long, PE Handley, KM Bernier-Latmani, R Bargar, JR AF Alessi, Daniel S. Lezama-Pacheco, Juan S. Janot, Noemie Suvorova, Elena I. Cerrato, Jose M. Giammar, Daniel E. Davis, James A. Fox, Patricia M. Williams, Kenneth H. Long, Philip E. Handley, Kim M. Bernier-Latmani, Rizlan Bargar, John R. TI Speciation and Reactivity of Uranium Products Formed during in Situ Bioremediation in a Shallow Alluvial Aquifer SO ENVIRONMENTAL SCIENCE & TECHNOLOGY LA English DT Article ID U(VI) REDUCTION; CONTAMINATED GROUNDWATER; MICROBIAL REDUCTION; SP-NOV.; U(IV); SEDIMENTS; URANINITE; IMMOBILIZATION; BIOSTIMULATION; SEPARATION AB In this study, we report the results of in situ U(VI) bioreduction experiments at the Integrated Field Research Challenge site in Rifle, Colorado, USA. Columns filled with sediments were deployed into a groundwater well at the site and, after a period of conditioning with groundwater, were amended with a mixture of groundwater, soluble U(VI), and acetate to stimulate the growth of indigenous microorganisms. Individual reactors were collected as various redox regimes in the column sediments were achieved: (i) during iron reduction, (ii) just after the onset of sulfate reduction, and (iii) later into sulfate reduction. The speciation of U retained in the sediments was studied using X-ray absorption spectroscopy, electron microscopy and chemical extractions. Circa 90% of the total uranium was reduced to U(IV) in each reactor. Noncrystalline U(IV) comprised about two-thirds of the U(IV) pool, across large changes in microbial community structure, redox regime, total uranium accumulation, and reaction time. A significant body of recent research has demonstrated that noncrystalline U(IV) species are more suceptible to remobilization and reoxiation than crystalline U(IV) phases such as uraninite. Our results highlight the importance of considering noncrystalline U(IV) formation across a wide range of aquifer parameters when designing in situ remediation plans. C1 [Alessi, Daniel S.; Suvorova, Elena I.; Bernier-Latmani, Rizlan] Ecole Polytech Fed Lausanne, Environm Microbiol Lab, CH-1015 Lausanne, Switzerland. [Lezama-Pacheco, Juan S.; Janot, Noemie; Bargar, John R.] SLAG Natl Accelerator Lab, Stanford Synchrotron Radiat Lightsource, Chem & Catalysis Div, Menlo Pk, CA 94025 USA. [Cerrato, Jose M.; Giammar, Daniel E.] Washington Univ, Dept Energy Environm & Chem Engn, St Louis, MO 63130 USA. [Davis, James A.; Fox, Patricia M.; Williams, Kenneth H.; Long, Philip E.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Earth Sci, Berkeley, CA 94720 USA. [Handley, Kim M.] Univ Calif Berkeley, Dept Earth & Planetary Sci, Berkeley, CA 94720 USA. RP Bargar, JR (reprint author), SLAG Natl Accelerator Lab, Stanford Synchrotron Radiat Lightsource, Chem & Catalysis Div, Menlo Pk, CA 94025 USA. EM bargar@slac.stanford.edu RI Bernier-Latmani, Rizlan/E-4398-2011; Williams, Kenneth/O-5181-2014; Long, Philip/F-5728-2013; Fox, Patricia/I-2208-2014; Davis, James/G-2788-2015; OI Bernier-Latmani, Rizlan/0000-0001-6547-722X; Alessi, Daniel/0000-0002-8360-8251; Williams, Kenneth/0000-0002-3568-1155; Long, Philip/0000-0003-4152-5682; Fox, Patricia/0000-0002-5264-1876; Handley, Kim/0000-0003-0531-3009 NR 57 TC 16 Z9 16 U1 11 U2 90 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0013-936X EI 1520-5851 J9 ENVIRON SCI TECHNOL JI Environ. Sci. Technol. PD NOV 4 PY 2014 VL 48 IS 21 BP 12842 EP 12850 DI 10.1021/es502701u PG 9 WC Engineering, Environmental; Environmental Sciences SC Engineering; Environmental Sciences & Ecology GA AS7QC UT WOS:000344449100044 PM 25265543 ER PT J AU Dickson, JO Harsh, JB Flury, M Lukens, WW Pierce, EM AF Dickson, Johnbull O. Harsh, James B. Flury, Markus Lukens, Wayne W. Pierce, Eric M. TI Competitive Incorporation of Perrhenate and Nitrate into Sodalite SO ENVIRONMENTAL SCIENCE & TECHNOLOGY LA English DT Article ID CRYSTAL-STRUCTURE; VADOSE ZONE; HYPERALKALINE CONDITIONS; PHASE TRANSFORMATIONS; WASTE; CANCRINITE; SEDIMENTS; PRECIPITATION; DISSOLUTION; ALUMINUM AB Nuclear Waste storage tanks at the Hanford site in southeastern Washington have ,released alkaline solutions, containing radioactive and other contaminants, into subsurface sediments. When this waste reacts with subsurface sediments, feldspathoid minerals (sodalite, cancrinite) can form, sequestering pertechnetate ((TcO4-)-Tc-99) and other ions. This study investigates the potential for incorporation of perrhenate (ReO4-), a chemical surrogate for (TcO4-)-Tc-99, into mixed perrhenate/nitrate (ReO4-/NO3-) sodalite. Mixed-anion sodalites were hydrothermally synthesized in the laboratory from zeolite A in sodium hydroxide, nitrate, and perrhenate solutions at 90 degrees C for 24 h. The resulting solids were characterized by bulk chemical analysis, X-ray diffraction, scanning electron microcopy, and X-ray absorption near edge structure spectroscopy (XANES) to determine the products' chemical composition, structure, morphology, and Re oxidation state. The XANES data indicated that nearly all rhenium (Re) was incorporated as Re(VII)O-4(-). The nonlinear increase of the unit cell parameter with ReO4-/NO3- ratios suggests formation of two separate sodalite phases in lieu of a mixed-anion sodalite. The results reveal that the sodalite cage is highly selective toward NO3- over ReO4-. Calculated enthalpy and Gibbs free energy of formation at 298 K for NO3- and ReO4- sodalite suggest that NO3- incorporation into the cage is favored over the incorporation of the larger ReO4-, due to the smaller ionic radius of NO3-. Based on these results, it is expected that NO3-, which is present at significantly higher concentrations in alkaline waste solutions than (TcO4-)-Tc-99, will be strongly preferred for incorporation into the sodalite cage. C1 [Dickson, Johnbull O.; Harsh, James B.; Flury, Markus] Washington State Univ, Dept Crop & Soil Sci, Pullman, WA 99164 USA. [Lukens, Wayne W.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA. [Pierce, Eric M.] Oak Ridge Natl Lab, Div Environm Sci, Oak Ridge, TN 37831 USA. RP Dickson, JO (reprint author), Washington State Univ, Dept Crop & Soil Sci, POB 646420, Pullman, WA 99164 USA. EM j.dickson@wsu.edu RI Dickson, Johnbull/I-3637-2016; Pierce, Eric/G-1615-2011; Harsh, James/C-7455-2014 OI Dickson, Johnbull/0000-0003-2916-7368; Pierce, Eric/0000-0002-4951-1931; Harsh, James/0000-0002-0177-3342 NR 45 TC 14 Z9 14 U1 7 U2 29 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0013-936X EI 1520-5851 J9 ENVIRON SCI TECHNOL JI Environ. Sci. Technol. PD NOV 4 PY 2014 VL 48 IS 21 BP 12851 EP 12857 DI 10.1021/es503156v PG 7 WC Engineering, Environmental; Environmental Sciences SC Engineering; Environmental Sciences & Ecology GA AS7QC UT WOS:000344449100045 PM 25280127 ER PT J AU Alam, A Khan, SN Smirnov, AV Nicholson, DM Johnson, DD AF Alam, Aftab Khan, Suffian N. Smirnov, A. V. Nicholson, D. M. Johnson, Duane D. TI Green's function multiple-scattering theory with a truncated basis set: An augmented-KKR formalism SO PHYSICAL REVIEW B LA English DT Article ID CONSISTENT ELECTRONIC-STRUCTURE; NI-ZN SYSTEM; RANDOM ALLOYS; TOTAL-ENERGY; AB-INITIO; INCOMMENSURATE; COMMENSURATE; DENSITY; IRON AB The Korringa-Kohn-Rostoker (KKR) Green's function, multiple-scattering theory is an efficient site-centered, electronic-structure technique for addressing an assembly of N scatterers. Wave functions are expanded in a spherical-wave basis on each scattering center and indexed up to a maximum orbital and azimuthal number L-max = (l, m)(max), while scattering matrices, which determine spectral properties, are truncated at L-tr = (l, m) tr where phase shifts delta l> l(tr) are negligible. Historically, L-max is set equal to L-tr, which is correct for large enough L-max but not computationally expedient; a better procedure retains higher-order (free-electron and single-site) contributions for L-max > L-tr with delta(l)> l(tr) set to zero [X.-G. Zhang andW. H. Butler, Phys. Rev. B 46, 7433 (1992)]. We present a numerically efficient and accurate augmented-KKR Green's function formalism that solves the KKR equations by exact matrix inversion [R-3 process with rank N(L-tr + 1) 2] and includes higher-L contributions via linear algebra [R-2 process with rank N(l(max) + 1) 2]. The augmented-KKR approach yields properly normalized wave functions, numerically cheaper basis-set convergence, and a total charge density and electron count that agrees with Lloyd's formula. We apply our formalism to fcc Cu, bcc Fe, and L1(0) CoPt and present the numerical results for accuracy and for the convergence of the total energies, Fermi energies, and magnetic moments versus L-max for a given L-tr C1 [Alam, Aftab] Indian Inst Technol, Dept Phys, Bombay 400076, Maharashtra, India. [Khan, Suffian N.; Smirnov, A. V.; Johnson, Duane D.] Ames Lab, Div Mat Sci Engn, Ames, IA 50011 USA. [Nicholson, D. M.] Oak Ridge Natl Lab, Oak Ridge, TN 37831 USA. [Johnson, Duane D.] Iowa State Univ, Dept Mat Sci & Engn, Ames, IA 50011 USA. RP Alam, A (reprint author), Indian Inst Technol, Dept Phys, Bombay 400076, Maharashtra, India. EM aftab@phy.iitb.ac.in; ddj@ameslab.gov OI Johnson, Duane/0000-0003-0794-7283 FU SEED Grant at IIT Bombay [13IRCCSG020]; U.S. Department of Energy, Office of Science, Basic Energy Sciences, Materials Science and Engineering Division through the Center for Defect Physics, an Energy Frontier Research Center; U.S. Department of Energy, Office of Science, Basic Energy Sciences, Materials Science and Engineering Division through Ames Laboratory [DE-AC02-07CH11358, DE-FG02-03ER46026]; U.S. Department of Energy [DE-AC02-07CH11358] FX A.A. acknowledges support from SEED Grant (sponsored Project No. 13IRCCSG020) at IIT Bombay. Work was supported by the U.S. Department of Energy, Office of Science, Basic Energy Sciences, Materials Science and Engineering Division, partially through the Center for Defect Physics, an Energy Frontier Research Center (A. A., D.M.N., and S.N.K. for Ph.D. thesis), and through Ames Laboratory under Contract No. DE-AC02-07CH11358 for materials discovery (A. S., D.D.J., and S.N.K. for post-doc), and Contract No. DE-FG02-03ER46026 for supplemental code (A. S. and D.D.J.). The research was performed at Ames Laboratory, operated for the U.S. Department of Energy by Iowa State University under Contract No. DE-AC02-07CH11358. NR 49 TC 4 Z9 4 U1 0 U2 7 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 2469-9950 EI 2469-9969 J9 PHYS REV B JI Phys. Rev. B PD NOV 4 PY 2014 VL 90 IS 20 AR 205102 DI 10.1103/PhysRevB.90.205102 PG 7 WC Physics, Condensed Matter SC Physics GA AS8GS UT WOS:000344488500004 ER PT J AU Zhu, S Li, YQ Batista, CD AF Zhu, Shan Li, You-Quan Batista, Cristian D. TI Spin-orbit coupling and electronic charge effects in Mott insulators SO PHYSICAL REVIEW B LA English DT Article ID ANISOTROPIC SUPEREXCHANGE INTERACTION; MULTIFERROIC MATERIAL; WEAK FERROMAGNETISM; POLARIZATION; MAGNETS AB We derive the effective charge-and current-density operators for the strong-coupling limit of a single-band Mott insulator in the presence of spin-orbit coupling and show that the spin-orbit contribution to the effective charge density leads to novel mechanisms for multiferroic behavior. In some sense, these mechanisms are the electronic counterpart of the ionic-based mechanisms, which have been proposed for explaining the electric polarization induced by spiral spin orderings. The new electronic mechanisms are illustrated by considering cycloidal and proper-screwmagnetic orderings on sawtooth and kagome lattices. As for the isotropic case, geometric frustration is crucial for achieving this purely electronic coupling between spin and charge degrees of freedom. C1 [Zhu, Shan; Li, You-Quan] Zhejiang Univ, Zhejiang Inst Modern Phys, Dept Phys, Hangzhou 310027, Zhejiang, Peoples R China. [Batista, Cristian D.] Los Alamos Natl Lab, T4 & CNLS, Div Theoret, Los Alamos, NM 87545 USA. RP Zhu, S (reprint author), Zhejiang Univ, Zhejiang Inst Modern Phys, Dept Phys, Hangzhou 310027, Zhejiang, Peoples R China. EM yqli@zju.edu.cn; cdb@lanl.gov RI Batista, Cristian/J-8008-2016 FU NSFCs [11074216, 11274272]; Fundamental Research Funds for the Central Universities of China; U.S. DOE [DE-AC52-06NA25396]; National Science Foundation [PHYS-1066293] FX We would like to thank Y.-H. Liu, H.-B. Chen, S.-Z. Lin, and Y. Kamiya for helpful discussions. S. Zhu and Y.-Q. Li were supported by NSFCs (Grants No. 11074216 and No. 11274272) and the Fundamental Research Funds for the Central Universities of China. Work at LANL was performed under the auspices of the U.S. DOE Contract No. DE-AC52-06NA25396 through the LDRD program. The work of C. D. B. was supported, in part, by the National Science Foundation under Grant No. PHYS-1066293 and the hospitality of the Aspen Center for Physics. NR 33 TC 2 Z9 2 U1 1 U2 15 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1098-0121 EI 1550-235X J9 PHYS REV B JI Phys. Rev. B PD NOV 4 PY 2014 VL 90 IS 19 AR 195107 DI 10.1103/PhysRevB.90.195107 PG 10 WC Physics, Condensed Matter SC Physics GA AS8GM UT WOS:000344487900005 ER PT J AU Bazavov, A Bhattacharya, T Detar, C Ding, HT Gottlieb, S Gupta, R Hegde, P Heller, UM Karsch, F Laermann, E Levkova, L Mukherjee, S Petreczky, P Schmidt, C Schroeder, C Soltz, RA Soeldner, W Sugar, R Wagner, M Vranas, P AF Bazavov, A. Bhattacharya, Tanmoy DeTar, C. Ding, H. -T. Gottlieb, Steven Gupta, Rajan Hegde, P. Heller, U. M. Karsch, F. Laermann, E. Levkova, L. Mukherjee, Swagato Petreczky, P. Schmidt, C. Schroeder, C. Soltz, R. A. Soeldner, W. Sugar, R. Wagner, M. Vranas, P. TI Equation of state in (2+1)-flavor QCD SO PHYSICAL REVIEW D LA English DT Article ID PHASE-TRANSITION; MONTE-CARLO; LATTICE QCD; FLAVOR QCD; TEMPERATURE; THERMODYNAMICS; SPECTRUM; QUARKS AB We present results for the equation of state in (2 + 1)-flavor QCD using the highly improved staggered quark action and lattices with temporal extent N tau = 6, 8, 10, and 12. We show that these data can be reliably extrapolated to the continuum limit and obtain a number of thermodynamic quantities and the speed of sound in the temperature range 130-400 MeV. We compare our results with previous calculations and provide an analytic parameterization of the pressure, from which other thermodynamic quantities can be calculated, for use in phenomenology. We show that the energy density in the crossover region, 145 MeV <= T <= 163 MeV, defined by the chiral transition, is epsilon(c) = (0.18-0.5) GeV/fm(3), i.e., (1.2-3.1) epsilon(nuclear). At high temperatures, we compare our results with resummed and dimensionally reduced perturbation theory calculations. As a byproduct of our analyses, we obtain the values of the scale parameters r(0) from the static quark potential and w(0) from the gradient flow. C1 [Bazavov, A.] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52240 USA. [Bhattacharya, Tanmoy; Gupta, Rajan] Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA. [DeTar, C.; Levkova, L.] Univ Utah, Dept Phys & Astron, Salt Lake City, UT 84112 USA. [Ding, H. -T.; Hegde, P.] Cent China Normal Univ, Inst Particle Phys, Key Lab Quark Lepton Phys MOE, Wuhan 430079, Peoples R China. [Gottlieb, Steven; Wagner, M.] Indiana Univ, Dept Phys, Bloomington, IN 47405 USA. [Heller, U. M.] Amer Phys Soc, New York, NY 11961 USA. [Karsch, F.; Mukherjee, Swagato; Petreczky, P.] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. [Karsch, F.; Laermann, E.; Schmidt, C.] Univ Bielefeld, Fac Phys, D-33615 Bielefeld, Germany. [Schroeder, C.; Soltz, R. A.; Vranas, P.] Lawrence Livermore Natl Lab, Div Phys, Livermore, CA 94550 USA. [Schroeder, C.] Univ Regensburg, Inst Theoret Phys, D-93040 Regensburg, Germany. [Sugar, R.] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA. RP Bazavov, A (reprint author), Univ Iowa, Dept Phys & Astron, Iowa City, IA 52240 USA. RI Bhattacharya, Tanmoy/J-8956-2013; OI Bhattacharya, Tanmoy/0000-0002-1060-652X; Mukherjee, Swagato/0000-0002-3824-1008; Ding, Heng-Tong/0000-0003-0590-081X; Gupta, Rajan/0000-0003-1784-3058; Schmidt, Christian/0000-0002-9071-4757 FU U.S. Department of Energy [DE-AC02-98CH10886, DE-AC52-07NA27344, DE-FC02-12ER41879, DE-FG02-92ER40699, DE-FG02-91ER-40628, DE-FG02-91ER-40661, DE-FG02-04ER-41298, DE-KA-14-01-02, DE-SC0010120]; NSF [PHY07-03296, PHY07-57333, PHY10-67881, PHY08-57333, PHY-1212389, PHY13-16748]; Bundesministerium fur Bildung und Forschung [06BI9001, 05P12PBCTA]; EU Integrated Infrastructure Initiative Hadron Physics [3]; Lilly Endowment, Inc.; Indiana METACyt Initiative FX This work has been supported in part by Contracts No. DE-AC02-98CH10886, No. DE-AC52-07NA27344, No. DE-FC02-12ER41879, No. DE-FG02-92ER40699, No. DE-FG02-91ER-40628, No. DE-FG02-91ER-40661, No. DE-FG02-04ER-41298, No. DE-KA-14-01-02, and No. DE-SC0010120 with the U.S. Department of Energy; NSF Grants No. PHY07-03296, No. PHY07-57333, No. PHY10-67881, No. PHY08-57333, No. PHY-1212389, and No. PHY13-16748; the Bundesministerium fur Bildung und Forschung under Grants No. 06BI9001 and No. 05P12PBCTA; and the EU Integrated Infrastructure Initiative Hadron Physics 3. The numerical simulations have been performed on BlueGene/L computers GPU cluster (Edge) at Lawrence Livermore National Laboratory (LLNL), the New York Center for Computational Sciences (NYCCS) at Brookhaven National Laboratory; on BlueGene/P and BlueGene/Q computers at Argonne Leadership Computing facility; on BlueGene/P computers at NIC, Juelich, U.S. Teragrid (Texas Advanced Computing Center), at NERSC; on GPU clusters at University of Bielefeld; on the OCuLUS cluster at University of Paderborn; and on clusters of the USQCD collaboration in JLab and FNAL. This research was supported in part by Lilly Endowment, Inc., through its support for the Indiana University Pervasive Technology Institute, and in part by the Indiana METACyt Initiative. The Indiana METACyt Initiative at IU is also supported in part by Lilly Endowment, Inc. We thank Nathan Brown for help with the w0 scale calculations and Michael Strickland for providing us with data from the HTL resummed perturbative calculations. NR 61 TC 150 Z9 150 U1 0 U2 5 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 2470-0010 EI 2470-0029 J9 PHYS REV D JI Phys. Rev. D PD NOV 4 PY 2014 VL 90 IS 9 AR 094503 DI 10.1103/PhysRevD.90.094503 PG 25 WC Astronomy & Astrophysics; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AS8HF UT WOS:000344489700004 ER PT J AU Bernlochner, FU Ligeti, Z Turczyk, S AF Bernlochner, Florian U. Ligeti, Zoltan Turczyk, Sascha TI New ways to search for right-handed current in B -> rho l(nu)over-bar decay SO PHYSICAL REVIEW D LA English DT Article ID FORM-FACTORS; MESON DECAYS; HEAVY; CONSTRAINTS AB An interesting possibility to ease the tension between various determinations of vertical bar V-ub vertical bar is to allow a smallright-handed contribution to the standard model weak current. The present bounds on such a contribution are fairly weak. We propose new ways to search for such a beyond standard model contribution in semileptonic B -> rho l (nu) over bar. Generalized asymmetries in one, two, or three angular variables are introduced as discriminators, which do not require an unbinned analysis of the fully differential distribution, and a detailed study of the corresponding theoretical uncertainties is performed. A discussion on how binned measurements can access all the angular information follows, which may be useful in both B -> rho l (nu) over bar and B -> K*l(+)l(-), and possibly essential in the former decay due to backgrounds. The achievable sensitivity from the available BABAR and Belle data sets is explored, as well as from the anticipated 50 ab(-1) Belle II data. C1 [Bernlochner, Florian U.] Univ Victoria, Victoria, BC V8W 3P, Canada. [Bernlochner, Florian U.] Univ Bonn, Inst Phys, D-53115 Bonn, Germany. [Ligeti, Zoltan] Univ Calif Berkeley, Ernest Orlando Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Turczyk, Sascha] Johannes Gutenberg Univ Mainz, PRISMA Cluster Excellence, D-55099 Mainz, Germany. [Turczyk, Sascha] Johannes Gutenberg Univ Mainz, Mainz Inst Theoret Phys, D-55099 Mainz, Germany. RP Bernlochner, FU (reprint author), Univ Victoria, Victoria, BC V8W 3P, Canada. FU Office of Science, Office of High Energy Physics, of the U.S. Department of Energy [DE-AC02-05CH11231]; Aspen Center for Physics (NSF) [PHY-1066293]; DFG Forschungsstipendium [TU350/1-1]; ERC of the European Research Council [EFT4LHC]; ERC of Cluster of Excellence Precision Physics, Fundamental Interactions and Structure of Matter [PRISMA-EXC 1098] FX We thank Wolfgang Altmannshofer, Danny van Dyk, Jernej Kamenik, Roman Zwicky, and Bob Kowalewski for useful discussions. The work of Z. L. was supported in part by the Office of Science, Office of High Energy Physics, of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. Z. L. thanks the Aspen Center for Physics (NSF Grant No. PHY-1066293), where part of this work was carried out, for the hospitality. S. T. was supported by a DFG Forschungsstipendium under Contract No. TU350/1-1, by the ERC Advanced Grant No. EFT4LHC of the European Research Council and the Cluster of Excellence Precision Physics, Fundamental Interactions and Structure of Matter (PRISMA-EXC 1098). NR 37 TC 11 Z9 11 U1 0 U2 2 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 2470-0010 EI 2470-0029 J9 PHYS REV D JI Phys. Rev. D PD NOV 4 PY 2014 VL 90 IS 9 AR 094003 DI 10.1103/PhysRevD.90.094003 PG 17 WC Astronomy & Astrophysics; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AS8HF UT WOS:000344489700003 ER PT J AU Czarnecki, A Dowling, M Tormo, XGI Marciano, WJ Szafron, R AF Czarnecki, Andrzej Dowling, Matthew Garcia i Tormo, Xavier Marciano, William J. Szafron, Robert TI Michel decay spectrum for a muon bound to a nucleus SO PHYSICAL REVIEW D LA English DT Article ID RADIATIVE-CORRECTIONS; LEPTON SPECTRUM; ELECTRONS AB The spectrum of electrons from muons decaying in an atomic bound state is significantly modified by their interaction with the nucleus. Somewhat unexpectedly, its first measurement, at the Canadian laboratory TRIUMF, differed from basic theory. We show, using a combination of techniques developed in atomic, nuclear, and high-energy physics, that radiative corrections eliminate the discrepancy. In addition to solving that outstanding problem, our more precise predictions are potentially useful for interpreting future high-statistics muon experiments that aim to search for exotic interactions at 10(-16) sensitivity. C1 [Czarnecki, Andrzej; Dowling, Matthew; Garcia i Tormo, Xavier; Szafron, Robert] Univ Alberta, Dept Phys, Edmonton, AB T6G 2G7, Canada. [Marciano, William J.] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. RP Czarnecki, A (reprint author), Univ Alberta, Dept Phys, Edmonton, AB T6G 2G7, Canada. RI Szafron, Robert/I-5242-2016 OI Szafron, Robert/0000-0002-9640-6923 FU Science and Engineering Research Canada (NSERC); United States DOE [DE-ACO2-98CH10886] FX A. C., M. D., X. G. T. and R. S. were supported by Science and Engineering Research Canada (NSERC). W. J. M. was supported by the United States DOE under Grant No. DE-ACO2-98CH10886. NR 31 TC 8 Z9 9 U1 0 U2 4 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 2470-0010 EI 2470-0029 J9 PHYS REV D JI Phys. Rev. D PD NOV 4 PY 2014 VL 90 IS 9 AR 093002 DI 10.1103/PhysRevD.90.093002 PG 6 WC Astronomy & Astrophysics; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AS8HF UT WOS:000344489700001 ER PT J AU Nomura, Y Weinberg, SJ AF Nomura, Yasunori Weinberg, Sean J. TI Entropy of a vacuum: What does the covariant entropy count? SO PHYSICAL REVIEW D LA English DT Article ID BLACK-HOLE EVAPORATION; INFLATIONARY UNIVERSE; PARTICLE CREATION; QUANTUM-GRAVITY; FLUCTUATIONS; INFORMATION; DYNAMICS AB We argue that a unitary description of the formation and evaporation of a black hole implies that the Bekenstein-Hawking entropy is the "entropy of a vacuum": the logarithm of the number of possible independent ways in which quantum field theory on a fixed classical spacetime background can emerge in a full quantum theory of gravity. In many cases, the covariant entropy counts this entropy-the degeneracy of emergent quantum field theories in full quantum gravity-with the entropy of particle excitations in each quantum field theory giving only a tiny perturbation. In the Rindler description of a (black hole) horizon, the relevant vacuum degrees of freedom manifest themselves as an extra hidden quantum number carried by the states representing the second exterior region; this quantum number is invisible in the emergent quantum field theory. In a distant picture, these states arise as exponentially degenerate ground and excited states of the intrinsically quantum gravitational degrees of freedom on the stretched horizon. The formation and evaporation of a black hole involve processes in which the entropy of collapsing matter is transformed into that of a vacuum and then to that of final-state Hawking radiation. In the intermediate stage of this evolution, entanglement between the vacuum and (early) Hawking radiation develops, which is transferred to the entanglement among final-state Hawking quanta through the evaporation process. The horizon is kept smooth throughout the evolution; in particular, no firewall develops. Similar considerations also apply for cosmological horizons, for example for the horizon of a metastable de Sitter space. C1 [Nomura, Yasunori] Univ Calif Berkeley, Dept Phys, Berkeley Ctr Theoret Phys, Berkeley, CA 94720 USA. Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Theoret Phys Grp, Berkeley, CA 94720 USA. RP Nomura, Y (reprint author), Univ Calif Berkeley, Dept Phys, Berkeley Ctr Theoret Phys, Berkeley, CA 94720 USA. OI Nomura, Yasunori/0000-0002-1497-1479 FU Office of Science, Office of High Energy and Nuclear Physics, of the U.S. Department of Energy [DE-AC02-05CH11231]; National Science Foundation [PHY-1214644] FX This work was supported in part by the Director, Office of Science, Office of High Energy and Nuclear Physics, of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231 and in part by the National Science Foundation under Grant No. PHY-1214644. NR 46 TC 6 Z9 6 U1 0 U2 3 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1550-7998 EI 1550-2368 J9 PHYS REV D JI Phys. Rev. D PD NOV 4 PY 2014 VL 90 IS 10 AR 104003 DI 10.1103/PhysRevD.90.104003 PG 17 WC Astronomy & Astrophysics; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AS8HL UT WOS:000344490300002 ER PT J AU Calcavecchia, F Pederiva, F Kalos, MH Kuhne, TD AF Calcavecchia, Francesco Pederiva, Francesco Kalos, Malvin H. Kuehne, Thomas D. TI Sign problem of the fermionic shadow wave function SO PHYSICAL REVIEW E LA English DT Article ID QUANTUM MONTE-CARLO; GROUND-STATE; ZERO-TEMPERATURE; LIQUID-HELIUM; ELECTRON-GAS; HE-3; FORCES AB We present a whole series of methods to alleviate the sign problem of the fermionic shadow wave function in the context of variational Monte Carlo. The effectiveness of our techniques is demonstrated on liquid He-3. We found that although the variance is reduced, the gain in efficiency is restricted by the increased computational cost. Yet, this development not only extends the scope of the fermionic shadow wave function, but also facilitates highly accurate quantum Monte Carlo simulations previously thought not feasible. C1 [Calcavecchia, Francesco] Johannes Gutenberg Univ Mainz, Inst Phys, D-55128 Mainz, Germany. [Calcavecchia, Francesco] Grad Sch Mat Sci Mainz, D-55128 Mainz, Germany. [Pederiva, Francesco] Univ Trento, Dipartimento Fis, I-38050 Trento, Italy. [Pederiva, Francesco] INFN TIFPA, Trento Inst Fundamental Phys & Applicat, Trento, Italy. [Kalos, Malvin H.] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA. [Kuehne, Thomas D.] Johannes Gutenberg Univ Mainz, Inst Phys Chem, D-55128 Mainz, Germany. [Kuehne, Thomas D.] Johannes Gutenberg Univ Mainz, Ctr Computat Sci, D-55128 Mainz, Germany. [Kuehne, Thomas D.] Univ Paderborn, Dept Chem, D-33098 Paderborn, Germany. RP Calcavecchia, F (reprint author), Johannes Gutenberg Univ Mainz, Inst Phys, Staudingerweg 7, D-55128 Mainz, Germany. EM francesco.calcavecchia@gmail.com; tdkuehne@mail.upb.de RI Kuhne, Thomas/B-9508-2008 FU IDEE project of the Carl Zeiss Foundation; Graduate School of Excellence MAINZ; Max-Planck Graduate Center; U.S. Department of Energy by Lawrence Livermore National Laboratory [DE-AC52-07NA27344] FX Financial support from the IDEE project of the Carl Zeiss Foundation is kindly acknowledged. M. K. and F. C. would like to acknowledge the hospitality of the Lawrence Livermore National Laboratory. T. D. K. and F. C. would like to thank the Graduate School of Excellence MAINZ and the Max-Planck Graduate Center for financial support and the Gauss Center form Supercomputing (GCS) for providing computing time through the John von Neumann Institute for Computing (NIC) on the GCS share of the supercomputer JUQUEEN at the Julich Supercomputing Center (JCS). This work was performed in part under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract No. DE-AC52-07NA27344. NR 42 TC 5 Z9 5 U1 0 U2 12 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1539-3755 EI 1550-2376 J9 PHYS REV E JI Phys. Rev. E PD NOV 4 PY 2014 VL 90 IS 5 AR 053304 DI 10.1103/PhysRevE.90.053304 PG 10 WC Physics, Fluids & Plasmas; Physics, Mathematical SC Physics GA AS8IA UT WOS:000344491700010 ER PT J AU Chen, Y Harnik, R Vega-Morales, R AF Chen, Yi Harnik, Roni Vega-Morales, Roberto TI Probing the Higgs Couplings to Photons in h -> 4l at the LHC SO PHYSICAL REVIEW LETTERS LA English DT Article ID STANDARD MODEL; BOSON DECAYS; PHYSICS; SPIN; MASS AB We explore the sensitivity of the Higgs decay to four leptons, the so-called golden channel, to higher dimensional loop-induced couplings of the Higgs boson to ZZ, Z gamma, and gamma gamma pairs, allowing for general CP mixtures. The larger standard model tree level coupling hZ(mu)Z(mu) is the dominant "background" for the loop-induced couplings. However, this large background interferes with the smaller loop-induced couplings, enhancing the sensitivity. We perform a maximum likelihood analysis based on analytic expressions of the fully differential decay width for h -> 4l (4l equivalent to 2e2 mu; 4e; 4 mu), including all interference effects. We find that the spectral shapes induced by Higgs couplings to photons are particularly different than the hZ(mu)Z(mu) background leading to enhanced sensitivity to these couplings. We show that even if the h ->gamma gamma and h -> 4l rates agree with that predicted by the standard model, the golden channel has the potential to probe both the CP nature as well as the overall sign of the Higgs coupling to photons well before the end of a high-luminosity LHC. C1 [Chen, Yi] CALTECH, Lauritsen Lab High Energy Phys, Pasadena, CA 92115 USA. [Harnik, Roni] Fermilab Natl Accelerator Lab, Dept Theoret Phys, Batavia, IL 60510 USA. [Vega-Morales, Roberto] Univ Paris 11, CNRS, Lab Phys Theor Orsay, UMR8627, F-91405 Orsay, France. RP Chen, Y (reprint author), CALTECH, Lauritsen Lab High Energy Phys, Pasadena, CA 92115 USA. EM yichen@caltech.edu; roni@fnal.gov; roberto.vega@th.u-psud.fr FU European Research Council (ERC); United States Department of Energy [DE-AC02-07CH11359]; Weston Havens Foundation; DOE [DE-FG02-92-ER-40701, DE-FG02-91ER40684]; National Science Foundation [OCI-1053575] FX R. V. M. is supported by the European Research Council (ERC) Advanced Grant Higgs@LHC. Fermilab is operated by Fermi Research Alliance, Limited Liability Company (LLC), under Contract No. DE-AC02-07CH11359 with the United States Department of Energy. Y. C. is supported by the Weston Havens Foundation and DOE Grant No. DE-FG02-92-ER-40701. This work is also sponsored in part by the DOE Grant No. DE-FG02-91ER40684. This work used the Extreme Science and Engineering Discovery Environment (XSEDE), which is supported by National Science Foundation Grant No. OCI-1053575. NR 45 TC 18 Z9 18 U1 0 U2 4 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0031-9007 EI 1079-7114 J9 PHYS REV LETT JI Phys. Rev. Lett. PD NOV 4 PY 2014 VL 113 IS 19 AR 191801 DI 10.1103/PhysRevLett.113.191801 PG 5 WC Physics, Multidisciplinary SC Physics GA AS8JZ UT WOS:000344496600004 PM 25415898 ER PT J AU Lynn, JE Carlson, J Epelbaum, E Gandolfi, S Gezerlis, A Schwenk, A AF Lynn, J. E. Carlson, J. Epelbaum, E. Gandolfi, S. Gezerlis, A. Schwenk, A. TI Quantum Monte Carlo Calculations of Light Nuclei Using Chiral Potentials SO PHYSICAL REVIEW LETTERS LA English DT Article ID FORCES AB We present the first Green's function Monte Carlo calculations of light nuclei with nuclear interactions derived from chiral effective field theory up to next-to-next-to-leading order. Up to this order, the interactions can be constructed in a local form and are therefore amenable to quantum Monte Carlo calculations. We demonstrate a systematic improvement with each order for the binding energies of A = 3 and A = 4 systems. We also carry out the first few-body tests to study perturbative expansions of chiral potentials at different orders, finding that higher-order corrections are more perturbative for softer interactions. Our results confirm the necessity of a three-body force for correct reproduction of experimental binding energies and radii, and pave the way for studying few-and many-nucleon systems using quantum Monte Carlo methods with chiral interactions. C1 [Lynn, J. E.; Carlson, J.; Gandolfi, S.] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA. [Epelbaum, E.] Ruhr Univ Bochum, Inst Theoret Phys 2, D-44780 Bochum, Germany. [Gezerlis, A.] Univ Guelph, Dept Phys, Guelph, ON N1G 2W1, Canada. [Schwenk, A.] Tech Univ Darmstadt, Inst Kernphys, D-64289 Darmstadt, Germany. [Schwenk, A.] GSI Helmholtzzentrum Schwerionenforsch GmbH, ExtreMe Matter Inst EMMI, D-64291 Darmstadt, Germany. RP Lynn, JE (reprint author), Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA. EM joel.lynn@gmail.com RI Gezerlis, Alexandros/O-9426-2014; OI Gezerlis, Alexandros/0000-0003-2232-2484; Lynn, Joel/0000-0003-3481-5729; Gandolfi, Stefano/0000-0002-0430-9035 FU U. S. Department of Energy, Office of Nuclear Physics; NUCLEI SciDAC program; LANL LDRD program; Natural Sciences and Engineering Research Council of Canada; ERC [307986 STRONGINT, 259218 NUCLEAREFT]; Helmholtz Alliance Program of the Helmholtz Association [HA216/EMMI]; Office of Science of the U.S. Department of Energy [DE-AC02-05CH11231] FX We thank S. Bacca, P. Navratil, and I. Tews for useful discussions. The work of J. E. L., S. G., and J. C. is supported by the U. S. Department of Energy, Office of Nuclear Physics, and by the NUCLEI SciDAC program. The work of S. G. is also supported by the LANL LDRD program. The work of A. G. is supported by the Natural Sciences and Engineering Research Council of Canada. The work of A. S. is supported in part by ERC Grant No. 307986 STRONGINT, the Helmholtz Alliance Program of the Helmholtz Association Contract No. HA216/EMMI "Extremes of Density and Temperature: Cosmic Matter in the Laboratory," and computing resources at the Julich Supercomputing Center. The work of E. E. is supported in part by ERC Grant No. 259218 NUCLEAREFT. Computational resources have been provided by Los Alamos Open Supercomputing. This research also used resources of the National Energy Research Scientific Computing Center (NERSC), which is supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. NR 35 TC 21 Z9 21 U1 1 U2 7 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0031-9007 EI 1079-7114 J9 PHYS REV LETT JI Phys. Rev. Lett. PD NOV 4 PY 2014 VL 113 IS 19 AR 192501 DI 10.1103/PhysRevLett.113.192501 PG 5 WC Physics, Multidisciplinary SC Physics GA AS8JZ UT WOS:000344496600006 PM 25415900 ER PT J AU Ma, YQ Venugopalan, R AF Ma, Yan-Qing Venugopalan, Raju TI Comprehensive Description of J/psi Production in Proton-Proton Collisions at Collider Energies SO PHYSICAL REVIEW LETTERS LA English DT Article ID COLOR GLASS CONDENSATE; TRANSVERSE-MOMENTUM DISTRIBUTIONS; GLUON DISTRIBUTION-FUNCTIONS; HEAVY FLAVOR PRODUCTION; QUARK PAIR PRODUCTION; PP COLLISIONS; ROOT-S=7 TEV; HADRONIC PRODUCTION; LARGE NUCLEI; J-PSI AB We employ a small x color glass condensate (CGC)+ nonrelativistic QCD (NRQCD) formalism to compute J/psi production at low p(perpendicular to) in proton-proton collisions at collider energies. Very good agreement is obtained for total cross sections, rapidity distributions, and low momentum p(perpendicular to) distributions. Similar agreement is obtained for psi' production. We observe an overlap region in p(perpendicular to) where our results match smoothly to those obtained in a next-to-leading order collinearly factorized NRQCD formalism. The relative contribution of color singlet and color octet contributions can be quantified in the CGC + NRQCD framework, with the former contributing approximately 10% of the total cross section. C1 [Ma, Yan-Qing; Venugopalan, Raju] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. RP Ma, YQ (reprint author), Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. FU U. S. Department of Energy [DE-AC02-98CH10886] FX We thank Adrian Dumitru, Kevin Dusling, and Yasushi Nara for help with their rcBK codes. We thank Zhongbo Kang for his contributions at early stages of this work, and Jean-Philippe Lansberg and Lijuan Ruan for helpful discussions. This work was supported in part by the U. S. Department of Energy under Contract No. DE-AC02-98CH10886. NR 57 TC 23 Z9 23 U1 0 U2 14 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0031-9007 EI 1079-7114 J9 PHYS REV LETT JI Phys. Rev. Lett. PD NOV 4 PY 2014 VL 113 IS 19 AR 192301 DI 10.1103/PhysRevLett.113.192301 PG 5 WC Physics, Multidisciplinary SC Physics GA AS8JZ UT WOS:000344496600005 PM 25415899 ER PT J AU Zhang, W Jungfleisch, MB Jiang, WJ Pearson, JE Hoffmann, A Freimuth, F Mokrousov, Y AF Zhang, Wei Jungfleisch, Matthias B. Jiang, Wanjun Pearson, John E. Hoffmann, Axel Freimuth, Frank Mokrousov, Yuriy TI Spin Hall Effects in Metallic Antiferromagnets SO PHYSICAL REVIEW LETTERS LA English DT Article ID LOCALIZED WANNIER FUNCTIONS; SPINTRONICS; TEMPERATURE; THICKNESS AB We investigate four CuAu-I-type metallic antiferromagnets for their potential as spin current detectors using spin pumping and inverse spin Hall effect. Nontrivial spin Hall effects were observed for FeMn, PdMn, and IrMn while a much higher effect was obtained for PtMn. Using thickness-dependent measurements, we determined the spin diffusion lengths of these materials to be short, on the order of 1 nm. The estimated spin Hall angles of the four materials follow the relationship PtMn > IrMn > PdMn > FeMn, highlighting the correlation between the spin-orbit coupling of nonmagnetic species and the magnitude of the spin Hall effect in their antiferromagnetic alloys. These experiments are compared with first-principles calculations. Engineering the properties of the antiferromagnets as well as their interfaces can pave the way for manipulation of the spin dependent transport properties in antiferromagnet-based spintronics. C1 [Zhang, Wei; Jungfleisch, Matthias B.; Jiang, Wanjun; Pearson, John E.; Hoffmann, Axel] Argonne Natl Lab, Div Mat Sci, Argonne, IL 60439 USA. [Freimuth, Frank; Mokrousov, Yuriy] Forschungszentrum Julich, Peter Grunberg Inst, D-52425 Julich, Germany. [Freimuth, Frank; Mokrousov, Yuriy] Forschungszentrum Julich, Inst Adv Simulat, D-52425 Julich, Germany. [Freimuth, Frank; Mokrousov, Yuriy] JARA, D-52425 Julich, Germany. RP Zhang, W (reprint author), Argonne Natl Lab, Div Mat Sci, 9700 S Cass Ave, Argonne, IL 60439 USA. RI Zhang, Wei/G-1523-2012; Jungfleisch, Matthias Benjamin/G-1069-2015; Jiang, Wanjun/E-6994-2011; Hoffmann, Axel/A-8152-2009; OI Zhang, Wei/0000-0002-5878-3090; Jungfleisch, Matthias Benjamin/0000-0001-8204-3677; Jiang, Wanjun/0000-0003-0918-3862; Hoffmann, Axel/0000-0002-1808-2767; Freimuth, Frank/0000-0001-6193-5991 FU DOE, Office of Science, Basic Energy Science [DE-AC02-06CH11357]; HGF-YIG programme of DFG [VH-NG-513, SPP 1538] FX We thank Ralu Divan for help with the lithography. The experimental work at Argonne was supported by the U.S. Department of Energy, Office of Science, Basic Energy Sciences, Materials Science and Engineering Division. Lithography was carried out at the Center for Nanoscale Materials, which is supported by the DOE, Office of Science, Basic Energy Science under Contract No. DE-AC02-06CH11357. We gratefully acknowledge computing time on the supercomputers JUQUEEN and JUROPA at the Julich Supercomputing Center and the theoretical work at Julich was supported by funding under the HGF-YIG programme VH-NG-513 and SPP 1538 of DFG. NR 44 TC 63 Z9 63 U1 25 U2 135 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0031-9007 EI 1079-7114 J9 PHYS REV LETT JI Phys. Rev. Lett. PD NOV 4 PY 2014 VL 113 IS 19 AR 196602 DI 10.1103/PhysRevLett.113.196602 PG 6 WC Physics, Multidisciplinary SC Physics GA AS8JZ UT WOS:000344496600012 PM 25415914 ER PT J AU Sun, Y Gu, LH Dickinson, RE Norby, RJ Pallardy, SG Hoffman, FM AF Sun, Ying Gu, Lianhong Dickinson, Robert E. Norby, Richard J. Pallardy, Stephen G. Hoffman, Forrest M. TI Impact of mesophyll diffusion on estimated global land CO2 fertilization SO PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA LA English DT Article DE mesophyll conductance; CO2 fertilization; carbon cycle; gross primary production; photosynthetic model ID ATMOSPHERIC CARBON-DIOXIDE; GAS-EXCHANGE MEASUREMENTS; ISOTOPE DISCRIMINATION; TEMPERATURE RESPONSE; CONDUCTANCE; PHOTOSYNTHESIS; CLIMATE; LEAVES; BALANCE; MODELS AB In C-3 plants, CO2 concentrations drop considerably along mesophyll diffusion pathways from substomatal cavities to chloroplasts where CO2 assimilation occurs. Global carbon cycle models have not explicitly represented this internal drawdown and therefore overestimate CO2 available for carboxylation and underestimate photosynthetic responsiveness to atmospheric CO2. An explicit consideration of mesophyll diffusion increases the modeled cumulative CO2 fertilization effect (CFE) for global gross primary production (GPP) from 915 to 1,057 PgC for the period of 1901-2010. This increase represents a 16% correction, which is large enough to explain the persistent overestimation of growth rates of historical atmospheric CO2 by Earth system models. Without this correction, the CFE for global GPP is underestimated by 0.05 PgC/y/ppm. This finding implies that the contemporary terrestrial biosphere is more CO2 limited than previously thought. C1 [Sun, Ying; Dickinson, Robert E.] Univ Texas Austin, Dept Geol Sci, Austin, TX 78712 USA. [Gu, Lianhong; Norby, Richard J.] Oak Ridge Natl Lab, Div Environm Sci, Oak Ridge, TN 37831 USA. [Gu, Lianhong; Norby, Richard J.] Oak Ridge Natl Lab, Climate Change Sci Inst, Oak Ridge, TN 37831 USA. [Pallardy, Stephen G.] Univ Missouri, Dept Forestry, Columbia, MO 65211 USA. [Hoffman, Forrest M.] Oak Ridge Natl Lab, Climate Change Sci Inst, Oak Ridge, TN 37831 USA. [Hoffman, Forrest M.] Oak Ridge Natl Lab, Computat Earth Sci Grp, Oak Ridge, TN 37831 USA. RP Gu, LH (reprint author), Oak Ridge Natl Lab, Div Environm Sci, POB 2008, Oak Ridge, TN 37831 USA. EM lianhong-gu@ornl.gov; robted@jsg.utexas.edu RI Norby, Richard/C-1773-2012; Sun, Ying/G-6611-2016; Hoffman, Forrest/B-8667-2012; Gu, Lianhong/H-8241-2014 OI Norby, Richard/0000-0002-0238-9828; Hoffman, Forrest/0000-0001-5802-4134; Gu, Lianhong/0000-0001-5756-8738 FU US Department of Energy, Office of Science, Biological and Environmental Research Program [DE-FG02-01ER64746]; University of Texas at Austin [DE-AC05-00OR22725]; ORNL's Laboratory Directed Research and Development (LDRD) program FX We thank Drs. Paul Hanson, Stan Wullschleger, Anthony Walker, and David Weston for comments and suggestions. This material is based upon work supported by the US Department of Energy, Office of Science, Biological and Environmental Research Program Grants DE-FG02-01ER64746 to University of Texas at Austin and DE-AC05-00OR22725 to Oak Ridge National Laboratory (ORNL). The ORNL's Laboratory Directed Research and Development (LDRD) program also partially supported the research. ORNL is managed by University of Tennessee-Battelle, LLC. NR 35 TC 25 Z9 25 U1 0 U2 54 PU NATL ACAD SCIENCES PI WASHINGTON PA 2101 CONSTITUTION AVE NW, WASHINGTON, DC 20418 USA SN 0027-8424 J9 P NATL ACAD SCI USA JI Proc. Natl. Acad. Sci. U. S. A. PD NOV 4 PY 2014 VL 111 IS 44 BP 15774 EP 15779 DI 10.1073/pnas.1418075111 PG 6 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AS2CY UT WOS:000344088100046 PM 25313079 ER PT J AU Duanmu, DQ Bachy, C Sudek, S Wong, CH Jimenez, V Rockwell, NC Martin, SS Ngan, CY Reistetter, EN van Baren, MJ Price, DC Wei, CL Reyes-Prieto, A Lagarias, JC Worden, AZ AF Duanmu, Deqiang Bachy, Charles Sudek, Sebastian Wong, Chee-Hong Jimenez, Valeria Rockwell, Nathan C. Martin, Shelley S. Ngan, Chew Yee Reistetter, Emily N. van Baren, Marijke J. Price, Dana C. Wei, Chia-Lin Reyes-Prieto, Adrian Lagarias, J. Clark Worden, Alexandra Z. TI Marine algae and land plants share conserved phytochrome signaling systems SO PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA LA English DT Article DE phytoplankton; light harvesting; transcriptomics; marine ecology; light signaling evolution ID EUKARYOTIC PHYTOCHROMES; LIGHT; EVOLUTION; PROTEIN; RED; PHOTORECEPTORS; TRANSDUCTION; GENE; CYANOBACTERIAL; RESPONSES AB Phytochrome photosensors control a vast gene network in streptophyte plants, acting as master regulators of diverse growth and developmental processes throughout the life cycle. In contrast with their absence in known chlorophyte algal genomes and most sequenced prasinophyte algal genomes, a phytochrome is found in Micromonas pusilla, a widely distributed marine picoprasinophyte (<2 mu m cell diameter). Together with phytochromes identified from other prasinophyte lineages, we establish that prasinophyte and streptophyte phytochromes share core light-input and signaling-output domain architectures except for the loss of C-terminal response regulator receiver domains in the streptophyte phytochrome lineage. Phylogenetic reconstructions robustly support the presence of phytochrome in the common progenitor of green algae and land plants. These analyses reveal a monophyletic clade containing streptophyte, prasinophyte, cryptophyte, and glaucophyte phytochromes implying an origin in the eukaryotic ancestor of the Archaeplastida. Transcriptomic measurements reveal diurnal regulation of phytochrome and bilin chromophore biosynthetic genes in Micromonas. Expression of these genes precedes both light-mediated phytochrome redistribution from the cytoplasm to the nucleus and increased expression of photosynthesis-associated genes. Prasinophyte phytochromes perceive wavelengths of light transmitted farther through seawater than the red/far-red light sensed by land plant phytochromes. Prasinophyte phytochromes also retain light-regulated histidine kinase activity lost in the streptophyte phytochrome lineage. Our studies demonstrate that light-mediated nuclear translocation of phytochrome predates the emergence of land plants and likely represents a widespread signaling mechanism in unicellular algae. C1 [Duanmu, Deqiang; Rockwell, Nathan C.; Martin, Shelley S.; Lagarias, J. Clark] Univ Calif Davis, Dept Mol & Cell Biol, Davis, CA 95616 USA. [Bachy, Charles; Sudek, Sebastian; Jimenez, Valeria; Reistetter, Emily N.; van Baren, Marijke J.; Worden, Alexandra Z.] Monterey Bay Aquarium Res Inst, Moss Landing, CA 95039 USA. [Wong, Chee-Hong; Ngan, Chew Yee; Wei, Chia-Lin] Lawrence Berkeley Natl Lab, Joint Genome Inst, Sequencing Technol Grp, Walnut Creek, CA 94598 USA. [Price, Dana C.] Rutgers State Univ, Inst Marine & Coastal Sci, Dept Ecol Evolut & Nat Resources, New Brunswick, NJ 08903 USA. [Reyes-Prieto, Adrian] Univ New Brunswick, Dept Biol, Fredericton, NB E3B 5A3, Canada. [Reyes-Prieto, Adrian; Worden, Alexandra Z.] Canadian Inst Adv Res, Integrated Microbial Biodivers Program, Toronto, ON M5G 1Z8, Canada. RP Lagarias, JC (reprint author), Univ Calif Davis, Dept Mol & Cell Biol, Davis, CA 95616 USA. EM jclagarias@ucdavis.edu; azworden@mbari.org RI Lagarias, J Clark/L-3139-2013 OI Lagarias, J Clark/0000-0002-2093-0403 FU Gordon and Betty Moore Foundation (GBMF) [GBMF2637]; Technology Development Grant from the US Department of Energy (DOE) Joint Genome Institute, under the Office of Science of the DOE [DE-AC02-05CH11231]; National Science Foundation (NSF) [1004213]; National Institutes of Health [GM068552, NSF-MCB-0843625]; Lucile and David Packard Foundation; GBMF Investigator Award [3788, NSF-IOS0843119, DOE-DE-SC0004765] FX We thank H. Yu, J. Guo, A. J. Limardo, and N. Alvarado for laboratory assistance. Transciptome sequencing was performed by the National Center for Genome Resources supported by a grant from the Gordon and Betty Moore Foundation (GBMF), Grant GBMF2637. CCMP1545 RNA-seq was supported by a Technology Development Grant from the US Department of Energy (DOE) Joint Genome Institute, under the Office of Science of the DOE Contract DE-AC02-05CH11231. D.C.P. was supported by National Science Foundation (NSF) Grant 1004213 (to D. Bhattacharya, Rutgers University). We also acknowledge support from National Institutes of Health GM068552 and NSF-MCB-0843625 in the early stages of this work (both to J.C.L.) and support from the Lucile and David Packard Foundation, a GBMF Investigator Award (3788), NSF-IOS0843119, and DOE-DE-SC0004765 (to A.Z.W.). NR 42 TC 30 Z9 30 U1 4 U2 60 PU NATL ACAD SCIENCES PI WASHINGTON PA 2101 CONSTITUTION AVE NW, WASHINGTON, DC 20418 USA SN 0027-8424 J9 P NATL ACAD SCI USA JI Proc. Natl. Acad. Sci. U. S. A. PD NOV 4 PY 2014 VL 111 IS 44 BP 15827 EP 15832 DI 10.1073/pnas.1416751111 PG 6 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AS2CY UT WOS:000344088100055 PM 25267653 ER PT J AU Tilley, DC Eum, KS Fletcher-Taylor, S Austin, DC Dupre, C Patron, LA Garcia, RL Lam, K Yarov-Yarovoy, V Cohen, BE Sack, JT AF Tilley, Drew C. Eum, Kenneth S. Fletcher-Taylor, Sebastian Austin, Daniel C. Dupre, Christophe Patron, Lilian A. Garcia, Rita L. Lam, Kit Yarov-Yarovoy, Vladimir Cohen, Bruce E. Sack, Jon T. TI Chemoselective tarantula toxins report voltage activation of wild-type ion channels in live cells SO PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA LA English DT Article DE voltage-gated ion channel; potassium channel; gating modifier; fluorescence; allostery ID RECTIFIER K+ CHANNEL; SODIUM-CHANNELS; GATING MODIFIER; POTASSIUM CHANNELS; DEPENDENT INHIBITION; PYRAMIDAL NEURONS; CALCIUM-CHANNELS; SCORPION TOXIN; SPIDER TOXIN; KV CHANNELS AB Electrically excitable cells, such as neurons, exhibit tremendous diversity in their firing patterns, a consequence of the complex collection of ion channels present in any specific cell. Although numerous methods are capable of measuring cellular electrical signals, understanding which types of ion channels give rise to these signals remains a significant challenge. Here, we describe exogenous probes which use a novel mechanism to report activity of voltage-gated channels. We have synthesized chemoselective derivatives of the tarantula toxin guangxitoxin-1E (GxTX), an inhibitory cystine knot peptide that binds selectively to Kv2-type voltage gated potassium channels. We find that voltage activation of Kv2.1 channels triggers GxTX dissociation, and thus GxTX binding dynamically marks Kv2 activation. We identify GxTX residues that can be replaced by thiol-or alkyne-bearing amino acids, without disrupting toxin folding or activity, and chemoselectively ligate fluorophores or affinity probes to these sites. We find that GxTX-fluorophore conjugates colocalize with Kv2.1 clusters in live cells and are released from channels activated by voltage stimuli. Kv2.1 activation can be detected with concentrations of probe that have a trivial impact on cellular currents. Chemoselective GxTX mutants conjugated to dendrimeric beads likewise bind live cells expressing Kv2.1, and the beads are released by channel activation. These optical sensors of conformational change are prototype probes that can indicate when ion channels contribute to electrical signaling. C1 [Tilley, Drew C.; Eum, Kenneth S.; Fletcher-Taylor, Sebastian; Austin, Daniel C.; Yarov-Yarovoy, Vladimir; Sack, Jon T.] Univ Calif Davis, Dept Physiol & Membrane Biol, Davis, CA 95616 USA. [Eum, Kenneth S.; Dupre, Christophe; Patron, Lilian A.; Sack, Jon T.] Marine Biol Lab, Neurobiol Course, Woods Hole, MA 02543 USA. [Garcia, Rita L.; Cohen, Bruce E.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Mol Foundry, Berkeley, CA 94720 USA. [Lam, Kit; Yarov-Yarovoy, Vladimir] Univ Calif Davis, Dept Biochem & Mol Med, Davis, CA 95616 USA. RP Sack, JT (reprint author), Univ Calif Davis, Dept Physiol & Membrane Biol, Davis, CA 95616 USA. EM jsack@ucdavis.edu RI Foundry, Molecular/G-9968-2014; OI Dupre, Christophe/0000-0002-5929-8492 FU US NIH Grants [5P30GM092328-02, R01NS042225-09S1, R25NS063307, T32HL086350]; American Heart Association Grant [10SDG4220047]; Milton L. Shifman Endowed Scholarship for the Neurobiology Course at Woods Hole; Office of Science, Office of Basic Energy Sciences, of the US Department of Energy [DE-AC02-05CH11231] FX We thank Yi Liu of the Molecular Foundry for the BTTAA reagent. We are very grateful to many at the University of California, Davis: Oscar Cerda for his talented culturing of hippocampal neurons; James Trimmer for ion channel plasmids and helpful discussion; Jie Zheng and Peter Cala for feedback on the manuscript; and Sebastian Ayala, Christina Berry, and Yuanpei Li for providing technical assistance. This work was supported by US NIH Grants 5P30GM092328-02, R01NS042225-09S1, R25NS063307, and T32HL086350; American Heart Association Grant 10SDG4220047; and Milton L. Shifman Endowed Scholarship for the Neurobiology Course at Woods Hole. Work at the Molecular Foundry was supported by the Office of Science, Office of Basic Energy Sciences, of the US Department of Energy under Contract DE-AC02-05CH11231. This work is dedicated to the memory of coauthor Kenneth S. Eum (1987-2014). Ken was a talented PhD student, a driven and caring soul who brought joy to the lives of those who knew him. NR 66 TC 8 Z9 8 U1 2 U2 12 PU NATL ACAD SCIENCES PI WASHINGTON PA 2101 CONSTITUTION AVE NW, WASHINGTON, DC 20418 USA SN 0027-8424 J9 P NATL ACAD SCI USA JI Proc. Natl. Acad. Sci. U. S. A. PD NOV 4 PY 2014 VL 111 IS 44 BP E4789 EP E4796 DI 10.1073/pnas.1406876111 PG 8 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AS2CY UT WOS:000344088100011 PM 25331865 ER PT J AU Li, Q Luo, KH Kang, QJ Chen, Q AF Li, Qing Luo, K. H. Kang, Q. J. Chen, Q. TI Contact angles in the pseudopotential lattice Boltzmann modeling of wetting SO PHYSICAL REVIEW E LA English DT Article ID SUPERHYDROPHOBIC SURFACES; DYNAMICS; DROPS; SIMULATION; FLOWS; TRANSITIONS; WETTABILITY; LINE AB In this paper we investigate the implementation of contact angles in the pseudopotential lattice Boltzmann modeling of wetting at a large density ratio rho(L)/rho(V) = 500. The pseudopotential lattice Boltzmann model [X. Shan and H. Chen, Phys. Rev. E 49, 2941 (1994)] is a popular mesoscopic model for simulating multiphase flows and interfacial dynamics. In this model the contact angle is usually realized by a fluid-solid interaction. Two widely used fluid-solid interactions, the density-based interaction and the pseudopotential-based interaction, as well as a modified pseudopotential-based interaction formulated in the present paper are numerically investigated and compared in terms of the achievable contact angles, the maximum and the minimum densities, and the spurious currents. It is found that the pseudopotential-based interaction works well for simulating small static (liquid) contact angles theta < 90 degrees, however, it is unable to reproduce static contact angles close to 180 degrees. Meanwhile, it is found that the proposed modified pseudopotential-based interaction performs better in light of the maximum and the minimum densities and is overall more suitable for simulating large contact angles theta > 90 degrees. as compared with the two other types of fluid-solid interactions. Furthermore, the spurious currents are found to be enlarged when the fluid-solid interaction force is introduced. Increasing the kinematic viscosity ratio between the vapor and liquid phases is shown to be capable of reducing the spurious currents caused by the fluid-solid interactions. C1 [Li, Qing] Cent S Univ, Sch Energy Sci & Engn, Changsha 410083, Hunan, Peoples R China. [Luo, K. H.] UCL, Dept Mech Engn, London WC1E 7JE, England. [Kang, Q. J.] Los Alamos Natl Lab, Div Earth & Environm Sci, Computat Earth Sci Grp, Los Alamos, NM 87545 USA. [Chen, Q.] Nanjing Univ Sci & Technol, Sch Energy & Power Engn, Nanjing 210094, Jiangsu, Peoples R China. RP Luo, KH (reprint author), UCL, Dept Mech Engn, Torrington Pl, London WC1E 7JE, England. EM K.Luo@ucl.uk RI Kang, Qinjun/A-2585-2010 OI Kang, Qinjun/0000-0002-4754-2240 FU Engineering and Physical Sciences Research Council of the United Kingdom [EP/I012605/1, EP/J016381/2]; Los Alamos National Laboratory's Lab Directed Research & Development Program FX The authors gratefully acknowledge support from the Engineering and Physical Sciences Research Council of the United Kingdom under Grants No. EP/I012605/1 and No. EP/J016381/2 and the Los Alamos National Laboratory's Lab Directed Research & Development Program. NR 47 TC 5 Z9 5 U1 6 U2 31 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1539-3755 EI 1550-2376 J9 PHYS REV E JI Phys. Rev. E PD NOV 3 PY 2014 VL 90 IS 5 AR 053301 DI 10.1103/PhysRevE.90.053301 PG 9 WC Physics, Fluids & Plasmas; Physics, Mathematical SC Physics GA AU4PU UT WOS:000345594900011 ER PT J AU Emma, C Wu, J Fang, K Chen, S Serkez, S Pellegrini, C AF Emma, C. Wu, J. Fang, K. Chen, S. Serkez, S. Pellegrini, C. TI Terawatt x-ray free-electron-laser optimization by transverse electron distribution shaping SO PHYSICAL REVIEW SPECIAL TOPICS-ACCELERATORS AND BEAMS LA English DT Article ID SIDE-BAND INSTABILITY; HIGH-GAIN; SIMULATION AB We study the dependence of the peak power of a 1.5 angstrom Terawatt (TW), tapered x-ray free-electron laser (FEL) on the transverse electron density distribution. Multidimensional optimization schemes for TW hard x-ray free-electron lasers are applied to the cases of transversely uniform and parabolic electron beam distributions and compared to a Gaussian distribution. The optimizations are performed for a 200 m undulator and a resonant wavelength of lambda(r) = 1.5 angstrom using the fully three-dimensional FEL particle code GENESIS. The study shows that the flatter transverse electron distributions enhance optical guiding in the tapered section of the undulator and increase the maximum radiation power from a maximum of 1.56 TW for a transversely Gaussian beam to 2.26 TW for the parabolic case and 2.63 TW for the uniform case. Spectral data also shows a 30%-70% reduction in energy deposited in the sidebands for the uniform and parabolic beams compared with a Gaussian. An analysis of the transverse coherence of the radiation shows the coherence area to be much larger than the beam spotsize for all three distributions, making coherent diffraction imaging experiments possible. C1 [Emma, C.; Pellegrini, C.] Univ Calif Los Angeles, Los Angeles, CA 90095 USA. [Wu, J.; Fang, K.; Chen, S.; Pellegrini, C.] Stanford Linear Accelerator Ctr, Menlo Pk, CA 94025 USA. [Serkez, S.] Deutches Elektronen Synchrotron, D-22607 Hamburg, Germany. RP Emma, C (reprint author), Univ Calif Los Angeles, Los Angeles, CA 90095 USA. FU U.S. DOE [DE-SC0009983] FX This work was supported by U.S. DOE under Grant No. DE-SC0009983. NR 20 TC 7 Z9 7 U1 1 U2 6 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1098-4402 J9 PHYS REV SPEC TOP-AC JI Phys. Rev. Spec. Top.-Accel. Beams PD NOV 3 PY 2014 VL 17 IS 11 AR 110701 DI 10.1103/PhysRevSTAB.17.110701 PG 7 WC Physics, Nuclear; Physics, Particles & Fields SC Physics GA AU5KM UT WOS:000345645800001 ER PT J AU Bennett, AB Meehan, TD Gratton, C Isaacs, R AF Bennett, Ashley B. Meehan, Timothy D. Gratton, Claudio Isaacs, Rufus TI Modeling Pollinator Community Response to Contrasting Bioenergy Scenarios SO PLOS ONE LA English DT Article ID EASTERN NORTH-AMERICA; LAND-USE CHANGE; FRUIT-SET; AGRICULTURAL LANDSCAPES; CROP POLLINATION; BEE POLLINATORS; BIOFUEL CROPS; SERVICES; BIODIVERSITY; DIVERSITY AB In the United States, policy initiatives aimed at increasing sources of renewable energy are advancing bioenergy production, especially in the Midwest region, where agricultural landscapes dominate. While policy directives are focused on renewable fuel production, biodiversity and ecosystem services will be impacted by the land-use changes required to meet production targets. Using data from field observations, we developed empirical models for predicting abundance, diversity, and community composition of flower-visiting bees based on land cover. We used these models to explore how bees might respond under two contrasting bioenergy scenarios: annual bioenergy crop production and perennial grassland bioenergy production. In the two scenarios, 600,000 ha of marginal annual crop land or marginal grassland were converted to perennial grassland or annual row crop bioenergy production, respectively. Model projections indicate that expansion of annual bioenergy crop production at this scale will reduce bee abundance by 0 to 71%, and bee diversity by 0 to 28%, depending on location. In contrast, converting annual crops on marginal soil to perennial grasslands could increase bee abundance from 0 to 600% and increase bee diversity between 0 and 53%. Our analysis of bee community composition suggested a similar pattern, with bee communities becoming less diverse under annual bioenergy crop production, whereas bee composition transitioned towards a more diverse community dominated by wild bees under perennial bioenergy crop production. Models, like those employed here, suggest that bioenergy policies have important consequences for pollinator conservation. C1 [Bennett, Ashley B.; Isaacs, Rufus] Michigan State Univ, Dept Entomol, E Lansing, MI 48824 USA. [Bennett, Ashley B.; Isaacs, Rufus] Michigan State Univ, Great Lakes Bioenergy Res Ctr, E Lansing, MI 48824 USA. [Meehan, Timothy D.; Gratton, Claudio] Univ Wisconsin, Dept Entomol, Madison, WI 53706 USA. [Meehan, Timothy D.; Gratton, Claudio] Univ Wisconsin, Great Lakes Bioenergy Res Ctr, Madison, WI USA. RP Isaacs, R (reprint author), Michigan State Univ, Dept Entomol, E Lansing, MI 48824 USA. EM isaacsr@msu.edu FU Department of Energy Great Lakes Bioenergy Research Center (DOE BER Office of Science) [DE-FC02-07ER64494]; DOE OBP Office of Energy and Renewable Energy [DE-AC05-76RL01830]; USDA-NIFA grant [2012-67009-20146] FX This work was funded by the Department of Energy Great Lakes Bioenergy Research Center (DOE BER Office of Science DE-FC02-07ER64494), DOE OBP Office of Energy and Renewable Energy (DE-AC05-76RL01830), and by a USDA-NIFA grant to CG and RI(2012-67009-20146). The funders had no role in the study design, data collection and analysis, decision to publish, or preparation of the manuscript. NR 56 TC 4 Z9 4 U1 3 U2 40 PU PUBLIC LIBRARY SCIENCE PI SAN FRANCISCO PA 1160 BATTERY STREET, STE 100, SAN FRANCISCO, CA 94111 USA SN 1932-6203 J9 PLOS ONE JI PLoS One PD NOV 3 PY 2014 VL 9 IS 11 AR e110676 DI 10.1371/journal.pone.0110676 PG 10 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AU4DB UT WOS:000345558100025 PM 25365559 ER PT J AU Brgoch, J Gaultois, MW Balasubramanian, M Page, K Hong, BC Seshadri, R AF Brgoch, J. Gaultois, M. W. Balasubramanian, M. Page, K. Hong, B. -C. Seshadri, R. TI Local structure and structural rigidity of the green phosphor beta-SiAlON:Eu2+ SO APPLIED PHYSICS LETTERS LA English DT Article ID BETA-SIALON; ELECTRONIC-STRUCTURE; COMBUSTION SYNTHESIS; TEMPERATURE AB Eu2+ inserted in beta-Si3-xAlxOxN4-x is a material that shows exceptional promise as a green-emitting phosphor. Synchrotron X-ray and neutron scattering, in conjunction with first-principles calculations and Eu L-3 X-ray absorption measurements, yield a consistent picture of the composition, and the favorable position for Eu2+ substitution in the crystal structure. The Debye temperature Theta(D), which is a proxy for structural rigidity relating to effectiveness as a phosphor, is very high for the starting beta-Si3N4 framework and is determined to decrease only slightly for the small amounts of Al3+ and O2- co-substitution that are required for charge balance associated with Eu2+ insertion. (C) 2014 AIP Publishing LLC. C1 [Brgoch, J.; Gaultois, M. W.; Seshadri, R.] Univ Calif Santa Barbara, Mitsubishi Chem Ctr Adv Mat, Santa Barbara, CA 93106 USA. [Brgoch, J.; Gaultois, M. W.; Seshadri, R.] Univ Calif Santa Barbara, Mat Res Lab, Santa Barbara, CA 93106 USA. [Balasubramanian, M.] Argonne Natl Lab, Adv Photon Source, Xray Sci Div, Argonne, IL 60439 USA. [Page, K.] Oak Ridge Natl Lab, Spallat Neutron Source, Oak Ridge, TN 37831 USA. [Hong, B. -C.] Mitsubishi Chem Grp Sci & Technol Res Ctr Inc, Aoba Ku, Yokohama, Kanagawa 2278502, Japan. RP Brgoch, J (reprint author), Univ Calif Santa Barbara, Mitsubishi Chem Ctr Adv Mat, Santa Barbara, CA 93106 USA. EM jbrgoch@uh.edu; mgaultois@mrl.ucsb.edu RI Page, Katharine/C-9726-2009; Seshadri, Ram/C-4205-2013; Gaultois, Michael/D-2867-2009 OI Page, Katharine/0000-0002-9071-3383; Seshadri, Ram/0000-0001-5858-4027; Gaultois, Michael/0000-0003-2172-2507 FU Natural Sciences and Engineering Council of Canada through NSERC; U.S. Department of State for an International Fulbright Science & Technology Award; U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-AC02-06CH11357]; neutron scattering at the Lujan Center - DOE Office of Basic Energy Sciences FX M.W.G. thanks the Natural Sciences and Engineering Council of Canada for support through a NSERC Postgraduate Scholarship, and the U.S. Department of State for an International Fulbright Science & Technology Award. The research made use of the shared facilities at the Materials Research Laboratory (MRL) (DMR-1121053). Calculations were conducted at the UCSB Center for Scientific Computing, supported by the California Nanosystems Institute (NSF CNS-0960316), Hewlett-Packard, and the MRL. This work benefited from the use of the Advanced Photon Source at Argonne National Laboratory was supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences (DE-AC02-06CH11357), and neutron scattering at the Lujan Center, funded by DOE Office of Basic Energy Sciences at the time of measurement; LANL is operated by Los Alamos National Security LLC (DE-AC52-06NA25396). NR 29 TC 10 Z9 11 U1 8 U2 72 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0003-6951 EI 1077-3118 J9 APPL PHYS LETT JI Appl. Phys. Lett. PD NOV 3 PY 2014 VL 105 IS 18 AR 181904 DI 10.1063/1.4901104 PG 4 WC Physics, Applied SC Physics GA AT5RQ UT WOS:000345000000028 ER PT J AU Haefner, A Gunter, D Plimley, B Pavlovsky, R Vetter, K AF Haefner, A. Gunter, D. Plimley, B. Pavlovsky, R. Vetter, K. TI Gamma-ray momentum reconstruction from Compton electron trajectories by filtered back-projection SO APPLIED PHYSICS LETTERS LA English DT Article ID DETECTORS; CAMERA AB Gamma-ray imaging utilizing Compton scattering has traditionally relied on measuring coincident gamma-ray interactions to map directional information of the source distribution. This coincidence requirement makes it an inherently inefficient process. We present an approach to gamma-ray reconstruction from Compton scattering that requires only a single electron tracking detector, thus removing the coincidence requirement. From the Compton scattered electron momentum distribution, our algorithm analytically computes the incident photon's correlated direction and energy distributions. Because this method maps the source energy and location, it is useful in applications, where prior information about the source distribution is unknown. We demonstrate this method with electron tracks measured in a scientific Si charge coupled device. While this method was demonstrated with electron tracks in a Si-based detector, it is applicable to any detector that can measure electron direction and energy, or equivalently the electron momentum. For example, it can increase the sensitivity to obtain energy and direction in gas-based systems that suffer from limited efficiency. (C) 2014 Author(s). C1 [Haefner, A.; Plimley, B.; Pavlovsky, R.; Vetter, K.] Univ Calif Berkeley, Dept Nucl Engn, Berkeley, CA 94720 USA. [Gunter, D.; Vetter, K.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. RP Haefner, A (reprint author), Univ Calif Berkeley, Dept Nucl Engn, 4155 Etcheverry Hall,MC 1730, Berkeley, CA 94720 USA. EM ahaefner@berkeley.edu FU DNDO; U.S. Department of Homeland Security [ECCS-1140069] FX The authors would like to thank DNDO for supporting this work. This material was based upon work supported by the U.S. Department of Homeland Security under the Grant Award Number Contract No. ECCS-1140069. Disclaimer: The views and conclusions contained in this document are those of the authors and should not be interpreted as necessarily representing the official policies either expressed or implied, of the U. S. Department of Homeland Security. NR 11 TC 2 Z9 2 U1 1 U2 13 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0003-6951 EI 1077-3118 J9 APPL PHYS LETT JI Appl. Phys. Lett. PD NOV 3 PY 2014 VL 105 IS 18 AR 184101 DI 10.1063/1.4898087 PG 4 WC Physics, Applied SC Physics GA AT5RQ UT WOS:000345000000087 ER PT J AU Heyes, JE Withayachumnankul, W Grady, NK Chowdhury, DR Azad, AK Chen, HT AF Heyes, Jane E. Withayachumnankul, Withawat Grady, Nathaniel K. Chowdhury, Dibakar Roy Azad, Abul K. Chen, Hou-Tong TI Hybrid metasurface for ultra-broadband terahertz modulation SO APPLIED PHYSICS LETTERS LA English DT Article ID METAMATERIAL; GRAPHENE; REFLECTARRAY; ABSORBERS AB We demonstrate an ultra-broadband free-space terahertz modulator based on a semiconductor-integrated metasurface. The modulator is made of a planar array of metal cut-wires on a silicon-on-sapphire substrate, where the silicon layer functions as photoconductive switches. Without external excitation, the cut-wire array exhibits a Lorentzian resonant response with a transmission passband spanning dc up to the fundamental dipole resonance above 2 THz. Under photoexcitation with 1.55 eV near-infrared light, the silicon regions in the cut-wire gaps become highly conductive, causing a transition of the resonant metasurface to a wire grating with a Drude response. In effect, the low-frequency passband below 2 THz evolves into a stopband for the incident terahertz waves. Experimental validations confirm a bandwidth of at least 100%, spanning 0.5-1.5 THz with -10 dB modulation depth. This modulation depth is far superior to -5 dB achievable from a plain silicon-on-sapphire substrate with effectively 25 times higher pumping energy. The proposed concept of ultra-broadband metasurface modulator can be readily extended to electrically controlled terahertz wave modulation. (C) 2014 AIP Publishing LLC. C1 [Heyes, Jane E.; Grady, Nathaniel K.; Chowdhury, Dibakar Roy; Azad, Abul K.; Chen, Hou-Tong] Los Alamos Natl Lab, Ctr Integrated Nanotechnol, Los Alamos, NM 87545 USA. [Withayachumnankul, Withawat] Univ Adelaide, Sch Elect & Elect Engn, Adelaide, SA 5005, Australia. RP Heyes, JE (reprint author), MIT, Elect Res Lab, Cambridge, MA 02139 USA. EM withawat.withayachumnankul@adelaide.edu.au; chenht@lanl.gov RI Chen, Hou-Tong/C-6860-2009; OI Chen, Hou-Tong/0000-0003-2014-7571; Azad, Abul/0000-0002-7784-7432 FU National Nuclear Security Administration of the U.S. Department of Energy [DE-AC52-06NA25396] FX This work was performed, in part, at the Center for Integrated Nanotechnologies, an Office of Science User Facility operated for the U. S. Department of Energy (DOE) Office of Science. Los Alamos National Laboratory, an affirmative action equal opportunity employer, is operated by Los Alamos National Security, LLC, for the National Nuclear Security Administration of the U.S. Department of Energy under Contract No. DE-AC52-06NA25396. NR 33 TC 9 Z9 9 U1 21 U2 135 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0003-6951 EI 1077-3118 J9 APPL PHYS LETT JI Appl. Phys. Lett. PD NOV 3 PY 2014 VL 105 IS 18 AR 181108 DI 10.1063/1.4901050 PG 4 WC Physics, Applied SC Physics GA AT5RQ UT WOS:000345000000008 ER PT J AU Huang, XR Peng, RW Gog, T Siddons, DP Assoufid, L AF Huang, Xian-Rong Peng, Ru-Wen Gog, Thomas Siddons, D. P. Assoufid, Lahsen TI Realizing in-plane surface diffraction by x-ray multiple-beam diffraction with large incidence angle SO APPLIED PHYSICS LETTERS LA English DT Article AB Based on rigorous dynamical-theory calculations, we demonstrate the principle of an x-ray multiple-beam diffraction (MBD) scheme that overcomes the long-lasting difficulties of high-resolution in-plane diffraction from crystal surfaces. This scheme only utilizes symmetric reflection geometry with large incident angles but activates the out-of-plane and in-plane diffraction processes simultaneously and separately in the continuous MBD planes. The in-plane diffraction is realized by detoured MBD, where the intermediate diffracted waves propagate parallel to the surface, which corresponds to an absolute Bragg surface diffraction configuration that is extremely sensitive to surface structures. A series of MBD diffraction and imaging techniques may be developed from this principle to study surface/interface (misfit) strains, lateral nanostructures, and phase transitions of a wide range of (pseudo) cubic crystal structures, including ultrathin epitaxial films and multilayers, quantum dots, strain-engineered semiconductor or (multi)ferroic materials, etc. (C) 2014 AIP Publishing LLC. C1 [Huang, Xian-Rong; Gog, Thomas; Assoufid, Lahsen] Argonne Natl Lab, Adv Photon Source, Argonne, IL 60439 USA. [Peng, Ru-Wen] Nanjing Univ, Natl Lab Solid State Microstruct, Nanjing 210093, Jiangsu, Peoples R China. [Peng, Ru-Wen] Nanjing Univ, Dept Phys, Nanjing 210093, Jiangsu, Peoples R China. [Siddons, D. P.] Brookhaven Natl Lab, Natl Synchrotron Light Source, Upton, NY 11973 USA. RP Huang, XR (reprint author), Argonne Natl Lab, Adv Photon Source, Argonne, IL 60439 USA. EM xiahuang@aps.anl.gov; rwpeng@nju.edu.cn FU U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-AC02-06CH11357, DEAC-02-98CH10886]; MOST of China [2012CB921502, 2010CB630705]; NSFC [11034005, 61475070, 91321312] FX This work was supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract Nos. DE-AC02-06CH11357 and DEAC-02-98CH10886. R.-W.P. was supported by the MOST of China (Grant Nos. 2012CB921502 and 2010CB630705) and the NSFC (Grant Nos. 11034005, 61475070, and 91321312). NR 19 TC 1 Z9 1 U1 2 U2 14 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0003-6951 EI 1077-3118 J9 APPL PHYS LETT JI Appl. Phys. Lett. PD NOV 3 PY 2014 VL 105 IS 18 AR 181903 DI 10.1063/1.4901046 PG 5 WC Physics, Applied SC Physics GA AT5RQ UT WOS:000345000000027 ER PT J AU Lichtenwalner, DJ Cheng, L Dhar, S Agarwal, A Palmour, JW AF Lichtenwalner, Daniel J. Cheng, Lin Dhar, Sarit Agarwal, Anant Palmour, John W. TI High mobility 4H-SiC (0001) transistors using alkali and alkaline earth interface layers SO APPLIED PHYSICS LETTERS LA English DT Article ID CHANNEL MOBILITY; GATE OXIDES; MOSFETS; PASSIVATION; OXIDATION; NITROGEN; CESIUM; SODIUM; TRAP; FACE AB Alkali (Rb and Cs) and alkaline earth (Ca, Sr, and Ba) elements have been investigated as interface passivation materials for metal-oxide-semiconductor field-effect transistors (MOSFETs) on 4H-SiC (0001). While the alkali elements Rb and Cs result in field-effect mobility (mu FE) values > 25 cm(2)/V.s, the alkaline earth elements Sr and Ba resulted in higher lFE values of 40 and 85 cm(2)/V.s, respectively. The Ba-modified MOSFETs show a slight decrease in mobility with heating to 150 degrees C, as expected when mobility is not interface-trap-limited, but phonon-scattering-limited. With a Ba interface layer, the interface state density 0.25 eV below the conduction band is similar to 3 x 10(11) cm(-2) eV(-1), lower than that obtained with nitric oxide passivation. Devices show stable threshold voltage under 2 MV/cm gate bias stress at 175 degrees C, indicating no mobile ions. Secondaryion mass spectrometry shows that the Sr and Ba stay predominantly at the interface after oxidation anneals. (C) 2014 AIP Publishing LLC. C1 [Lichtenwalner, Daniel J.; Cheng, Lin; Palmour, John W.] Cree Inc, Durham, NC 27709 USA. [Dhar, Sarit] Auburn Univ, Dept Phys, Auburn, AL 36849 USA. [Agarwal, Anant] US DOE, Off Energy Efficiency & Renewable Energy, Washington, DC 20585 USA. RP Lichtenwalner, DJ (reprint author), Cree Inc, Durham, NC 27709 USA. RI Lichtenwalner, Daniel/D-4396-2009 FU Army Research Laboratory FX Research was sponsored by the Army Research Laboratory and was accomplished under Cooperative Agreement No. W911NF-12-2-0064. The views and conclusions contained in this document are those of the authors and should not be interpreted as representing the official policies, either expressed or implied, of the Army Research Laboratory or the U.S. Government. The U.S. Government is authorized to reproduce and distribute reprints for Government purposes. NR 23 TC 11 Z9 11 U1 3 U2 21 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0003-6951 EI 1077-3118 J9 APPL PHYS LETT JI Appl. Phys. Lett. PD NOV 3 PY 2014 VL 105 IS 18 AR 182107 DI 10.1063/1.4901259 PG 4 WC Physics, Applied SC Physics GA AT5RQ UT WOS:000345000000041 ER PT J AU Lohn, AJ Mickel, PR Marinella, MJ AF Lohn, Andrew J. Mickel, Patrick R. Marinella, Matthew J. TI Modeling of filamentary resistive memory by concentric cylinders with variable conductivity SO APPLIED PHYSICS LETTERS LA English DT Article ID DRIVEN ION MIGRATION; SPICE MODEL; MEMRISTOR; CIRCUIT; SYSTEMS; DEVICE AB We demonstrate a method for modeling memristors (resistive random access memories) where the filament is composed of a set of nanoscale or sub-nanoscale concentric cylinders, each having its own conductivity. This approach allows for the inclusion of multiple state variables, which, we show experimentally, can be used to control electrical behavior. The simulations accurately reproduce the current-voltage hysteresis loop as well as these more complex experimental behaviors resulting from intricate switching histories. The simulations can be both static and dynamic, and are based upon physical design parameters, so optimized values from simulation can be easily linked to device design. (C) 2014 AIP Publishing LLC. C1 [Lohn, Andrew J.; Mickel, Patrick R.; Marinella, Matthew J.] Sandia Natl Labs, Albuquerque, NM 87185 USA. RP Lohn, AJ (reprint author), Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA. EM ajlohn@sandia.gov FU Sandia's Laboratory Directed Research and Development (LDRD) program; U.S. Department of Energy's National Nuclear Security Administration [DE-AC04-94AL85000] FX The authors would like to thank Jim Stevens and the Sandia MESA Fab for their work in fabricating devices used in this study. This work was funded by Sandia's Laboratory Directed Research and Development (LDRD) program. Sandia National Laboratories is a multi-program laboratory managed and operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the U.S. Department of Energy's National Nuclear Security Administration under contract DE-AC04-94AL85000. NR 28 TC 1 Z9 1 U1 4 U2 17 PU AMER INST PHYSICS PI MELVILLE PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA SN 0003-6951 EI 1077-3118 J9 APPL PHYS LETT JI Appl. Phys. Lett. PD NOV 3 PY 2014 VL 105 IS 18 AR 183511 DI 10.1063/1.4901351 PG 5 WC Physics, Applied SC Physics GA AT5RQ UT WOS:000345000000083 ER PT J AU Lee, JA Mounce, AM Oh, S Zimmerman, AM Halperin, WP AF Lee, Jeongseop A. Mounce, A. M. Oh, Sangwon Zimmerman, A. M. Halperin, W. P. TI Enhanced self-diffusion of adsorbed methanol in silica aerogel SO PHYSICAL REVIEW B LA English DT Article ID SURFACE-DIFFUSION; SUPERFLUID HE-3; ADSORPTION; RELAXATION; WATER; PRESSURE; HYDROGEN; FIELD AB Molecular transport of a two-component system of liquid and vapor in a porous medium can be anomalously increased owing to fast exchange between the two phases [Phys. Rev. Lett. 63, 43 (1989)]. We have investigated this phenomenon measuring the self-diffusion coefficient of methanol adsorbed in a 98% porosity aerogel using nuclear magnetic resonance field gradient techniques. We found enhancement of several orders of magnitude from which we determined the ballistic mean-free path in the vapor phase. We have grown globally uniform anisotropic aerogels and applied the diffusion measurements to characterize the anisotropy. Our results are important for understanding the novel properties of superfluid He-3 confined within an aerogel framework and for application to other physical systems. C1 [Lee, Jeongseop A.; Zimmerman, A. M.; Halperin, W. P.] Northwestern Univ, Dept Phys & Astron, Evanston, IL 60208 USA. [Mounce, A. M.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA. [Oh, Sangwon] Schlumberger Doll Res Ctr, Cambridge, MA 02139 USA. RP Lee, JA (reprint author), Northwestern Univ, Dept Phys & Astron, Evanston, IL 60208 USA. FU US Department of Energy, Office of Basic Energy Sciences, Division of Materials Sciences and Engineering [DE-FG02-05ER46248] FX We are grateful for discussions with J. I. A. (Leo) Li, Charles Collett, and Jim Sauls. Research was supported by the US Department of Energy, Office of Basic Energy Sciences, Division of Materials Sciences and Engineering under Award No. DE-FG02-05ER46248 (Northwestern University). NR 30 TC 1 Z9 1 U1 2 U2 13 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1098-0121 EI 1550-235X J9 PHYS REV B JI Phys. Rev. B PD NOV 3 PY 2014 VL 90 IS 17 AR 174501 DI 10.1103/PhysRevB.90.174501 PG 6 WC Physics, Condensed Matter SC Physics GA AU1ZD UT WOS:000345415100004 ER PT J AU Abelev, B Adam, J Adamova, D Aggarwal, MM Rinella, GA Agnello, M Agostinelli, A Agrawal, N Ahammed, Z Ahmad, N Ahmed, I Ahn, SU Ahn, SA Aimo, I Aiola, S Ajaz, M Akindinov, A Alam, SN Aleksandrov, D Alessandro, B Alexandre, D Alici, A Alkin, A Alme, J Alt, T Altinpinar, S Altsybeev, I Prado, CAG Andrei, C Andronic, A Anguelov, V Anielski, J Anticic, T Antinori, F Antonioli, P Aphecetche, L Appelshauser, H Arcelli, S Armesto, N Arnaldi, R Aronsson, T Arsene, IC Arslandok, M Augustinus, A Averbeck, R Awes, TC Azmi, MD Bach, M Badala, A Baek, YW Bagnasco, S Bailhache, R Bala, R Baldisseri, A Pedrosa, FBD Baral, RC Barbera, R Barile, F Barnafoldi, GG Barnby, LS Barret, V Bartke, J Basile, M Bastid, N Basu, S Bathen, B Batigne, G Camejo, AB Batyunya, B Batzing, PC Baumann, C Bearden, IG Beck, H Bedda, C Behera, NK Belikov, I Bellini, F Bellwied, R Belmont-Moreno, E Belmont, R Belyaev, V Bencedi, G Beole, S Berceanu, I Bercuci, A Berdnikov, Y Berenyi, D Berger, ME Bertens, RA Berzano, D Betev, L Bhasin, A Bhat, IR Bhati, AK Bhattacharjee, B Bhom, J Bianchi, L Bianchi, N Bianchin, C Bielcik, J Bielcikova, J Bilandzic, A Bjelogrlic, S Blanco, F Blau, D Blume, C Bock, F Bogdanov, A Boggild, H Bogolyubsky, M Bohmer, FV Boldizsar, L Bombara, M Book, J Borel, H Borissov, A Bossu, F Botje, M Botta, E Bottger, S Braun-Munzinger, P Bregant, M Breitner, T Broker, TA Browning, TA Broz, M Bruna, E Bruno, GE Budnikov, D Buesching, H Bufalino, S Buncic, P Busch, O Buthelezi, Z Caffarri, D Cai, X Caines, H Diaz, LC Caliva, A Villar, EC Camerini, P Carena, F Carena, W Castellanos, JC Casula, EAR Catanescu, V Cavicchioli, C Sanchez, CC Cepila, J Cerello, P Chang, B Chapeland, S Charvet, JL Chattopadhyay, S Chattopadhyay, S Chelnokov, V Cherney, M Cheshkov, C Cheynis, B Barroso, VC Chinellato, DD Chochula, P Chojnacki, M Choudhury, S Christakoglou, P Christensen, CH Christiansen, P Chujo, T Chung, SU Cicalo, C Cifarelli, L Cindolo, F Cleymans, J Colamaria, F Colella, D Collu, A Colocci, M Balbastre, GC del Valle, ZC Connors, ME Contreras, JG Cormier, TM Morales, YC Cortese, P Maldonado, IC Cosentino, MR Costa, F Crochet, P Albino, RC Cuautle, E Cunqueiro, L Dainese, A Dang, R Danu, A Das, D Das, I Das, K Das, S Dash, A Dash, S De, S Delagrange, H Deloff, A Denes, E D'Erasmo, G De Caro, A de Cataldo, G de Cuveland, J De Falco, A De Gruttola, D De Marco, N De Pasquale, S de Rooij, R Corchero, MAD Dietel, T Dillenseger, P Divia, R Di Bari, D Di Liberto, S Di Mauro, A Di Nezza, P Djuvsland, O Dobrin, A Dobrowolski, T Gimenez, DD Onigus, BD Dordic, O Dorheim, S Dubey, AK Dubla, A Ducroux, L Dupieux, P Majumdar, AKD Hilden, TE Ehlers, RJ Elia, D Engel, H Erazmus, B Erdal, HA Eschweiler, D Espagnon, B Esposito, M Estienne, M Esumi, S Evans, D Evdokimov, S Fabris, D Faivre, J Falchieri, D Fantoni, A Fasel, M Fehlker, D Feldkamp, L Felea, D Feliciello, A Feofilov, G Ferencei, J Tellez, AF Ferreiro, EG Ferretti, A Festanti, A Figiel, J Figueredo, MAS Filchagin, S Finogeev, D Fionda, FM Fiore, EM Floratos, E Floris, M Foertsch, S Foka, P Fokin, S Fragiacomo, E Francescon, A Frankenfeld, U Fuchs, U Furget, C Furs, A Girard, MF Gaardhoje, JJ Gagliardi, M Gago, AM Gallio, M Gangadharan, DR Ganoti, P Garabatos, C Garcia-Solis, E Gargiulo, C Garishvili, I Gerhard, J Germain, M Gheata, A Gheata, M Ghidini, B Ghosh, P Ghosh, SK Gianotti, P Giubellino, P Gladysz-Dziadus, E Glassel, P Ramirez, AG Gonzalez-Zamora, P Gorbunov, S Gorlich, L Gotovac, S Graczykowski, LK Grelli, A Grigoras, A Grigoras, C Grigoriev, V Grigoryan, A Grigoryan, S Grinyov, B Grion, N Grosse-Oetringhaus, JF Grossiord, JY Grosso, R Guber, F Guernane, R Guerzoni, B Guilbaud, M Gulbrandsen, K Gulkanyan, H Gumbo, M Gunji, T Gupta, A Gupta, R Khan, KH Haake, R Haaland, O Hadjidakis, C Haiduc, M Hamagaki, H Hamar, G Hanratty, LD Hansen, A Harris, JW Hartmann, H Harton, A Hatzifotiadou, D Hayashi, S Heckel, ST Heide, M Helstrup, H Herghelegiu, A Corral, GH Hess, BA Hetland, KF Hippolyte, B Hladky, J Hristov, P Huang, M Humanic, TJ Hussain, N Hutter, D Hwang, DS Ilkaev, R Ilkiv, I Inaba, M Innocenti, GM Ionita, C Ippolitov, M Irfan, M Ivanov, M Ivanov, V Jacholkowski, A Jacobs, PM Jahnke, C Jang, HJ Janik, MA Jayarathna, PHSY Jena, C Jena, S Bustamante, RTJ Jones, PG Jung, H Jusko, A Kadyshevskiy, V Kalcher, S Kalinak, P Kalweit, A Kamin, J Kang, JH Kaplin, V Kar, S Uysal, AK Karavichev, O Karavicheva, T Karpechev, E Kebschull, U Keidel, R Keijdener, DLD Svn, MK Khan, MM Khan, P Khan, SA Khanzadeev, A Kharlov, Y Kileng, B Kim, B Kim, DW Kim, DJ Kim, JS Kim, M Kim, M Kim, S Kim, T Kirsch, S Kisel, I Kiselev, S Kisiel, A Kiss, G Klay, JL Klein, J Klein-Bosing, C Kluge, A Knichel, ML Knospe, AG Kobdaj, C Kofarago, M Kohler, MK Kollegger, T Kolojvari, A Kondratiev, V Kondratyeva, N Konevskikh, A Kovalenko, V Kowalski, M Kox, S Meethaleveedu, GK Kral, J Kralik, I Kravcakova, A Krelina, M Kretz, M Krivda, M Krizek, F Kryshen, E Krzewicki, M Kucera, V Kucheriaev, Y Kugathasan, T Kuhn, C Kuijer, PG Kulakov, I Kumar, J Kurashvili, P Kurepin, A Kurepin, AB Kuryakin, A Kushpil, S Kweon, MJ Kwon, Y de Guevara, PL Fernandes, CL Lakomov, I Langoy, R Lara, C Lardeux, A Lattuca, A La Pointe, SL La Rocca, P Lea, R Leardini, L Lee, GR Legrand, I Lehnert, J Lemmon, RC Lenti, V Leogrande, E Leoncino, M Monzon, IL Levai, P Li, S Lien, J Lietava, R Lindal, S Lindenstruth, V Lippmann, C Lisa, MA Ljunggren, HM Lodato, DF Loenne, PI Loggins, VR Loginov, V Lohner, D Loizides, C Lopez, X Torres, EL Lu, XG Luettig, P Lunardon, M Luparello, G Ma, R Maevskaya, A Mager, M Mahapatra, DP Mahmood, SM Maire, A Majka, RD Malaev, M Cervantes, IM Malinina, L Mal'Kevich, D Malzacher, P Mamonov, A Manceau, L Manko, V Manso, F Manzari, V Marchisone, M Mares, J Margagliotti, GV Margotti, A Marin, A Markert, C Marquard, M Martashvili, I Martin, NA Martinengo, P Martinez, MI Garcia, GM Blanco, JM Martynov, Y Mas, A Masciocchi, S Masera, M Masoni, A Massacrier, L Mastroserio, A Matyja, A Mayer, C Mazer, J Mazzoni, MA Meddi, F Menchaca-Rocha, A Meninno, E Perez, JM Meres, M Miake, Y Mikhaylov, K Milano, L Milosevic, J Mischke, A Mishra, AN Miskowiec, D Mitra, J Mitu, CM Mlynarz, J Mohammadi, N Mohanty, B Molnar, L Zetina, LM Montes, E Morando, M De Godoy, DAM Moretto, S Morreale, A Morsch, A Muccifora, V Mudnic, E Muhlheim, D Muhuri, S Mukherjee, M Muller, H Munhoz, MG Murray, S Musa, L Musinsky, J Nandi, BK Nania, R Nappi, E Nattrass, C Nayak, K Nayak, TK Nazarenko, S Nedosekin, A Nicassio, M Niculescu, M Nielsen, BS Nikolaev, S Nikulin, S Nikulin, V Nilsen, BS Noferini, F Nomokonov, P Nooren, G Norman, J Nyanin, A Nystrand, J Oeschler, H Oh, S Oh, SK Okatan, A Olah, L Oleniacz, J Da Silva, ACO Onderwaater, J Oppedisano, C Velasquez, AO Oskarsson, A Otwinowski, J Oyama, K Ozdemir, M Sahoo, P Pachmayer, Y Pachr, M Pagano, P 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P Riegler, W Riggi, F Rivetti, A Rocco, E Cahuantzi, MR Manso, AR Roed, K Rogochaya, E Rohni, S Rohr, D Rohrich, D Romita, R Ronchetti, F Ronflette, L Rosnet, P Rossi, A Roukoutakis, F Roy, A Roy, C Roy, P Montero, AJR Rui, R Russo, R Ryabinkin, E Ryabov, Y Rybicki, A Sadovsky, S Safarik, K Sahlmuller, B Sahoo, R Sahu, PK Saini, J Sakai, S Salgado, CA Salzwedel, J Sambyal, S Samsonov, V Castro, XS Rodriguez, FJS Sandor, L Sandoval, A Sano, M Santagati, G Sarkar, D Scapparone, E Scarlassara, F Scharenberg, RP Schiaua, C Schicker, R Schmidt, C Schmidt, HR Schuchmann, S Schukraft, J Schulc, M Schuster, T Schutz, Y Schwarz, K Schweda, K Scioli, G Scomparin, E Scott, R Segato, G Seger, JE Sekiguchi, Y Selyuzhenkov, I Seo, J Serradilla, E Sevcenco, A Shabetai, A Shabratova, G Shahoyan, R Shangaraev, A Sharma, N Sharma, S Shigaki, K Shtejer, K Sibiriak, Y Siddhanta, S Siemiarczuk, T Silvermyr, D Silvestre, C Simatovic, G Singaraju, R Singh, R Singha, S Singhal, V Sinha, BC Sinha, T Sitar, B 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Timmins, A. R. Toia, A. Trubnikov, V. Trzaska, W. H. Tsuji, T. Tumkin, A. Turrisi, R. Tveter, T. S. Ullaland, K. Uras, A. Usai, G. L. Vajzer, M. Vala, M. Palomo, L. Valencia Vallero, S. Vyvre, P. Vande Van der Maarel, J. Van Hoorne, J. W. van Leeuwen, M. Vargas, A. Vargyas, M. Varma, R. Vasileiou, M. Vasiliev, A. Vechernin, V. Veldhoen, M. Velure, A. Venaruzzo, M. Vercellin, E. Vergara Limon, S. Vernet, R. Verweij, M. Vickovic, L. Viesti, G. Viinikainen, J. Vilakazi, Z. Baillie, O. Villalobos Vinogradov, A. Vinogradov, L. Vinogradov, Y. Virgili, T. Viyogi, Y. P. Vodopyanov, A. Voelkl, M. A. Voloshin, K. Voloshin, S. A. Volpe, G. von Haller, B. Vorobyev, I. Vranic, D. Vrlakova, J. Vulpescu, B. Vyushin, A. Wagner, B. Wagner, J. Wagner, V. Wang, M. Wang, Y. Watanabe, D. Weber, M. Wessels, J. P. Westerhoff, U. Wiechula, J. Wikne, J. Wilde, M. Wilk, G. Wilkinson, J. Williams, M. C. S. Windelband, B. Winn, M. Yaldo, C. G. Yamaguchi, Y. Yang, H. Yang, P. Yang, S. Yano, S. Yasnopolskiy, S. Yi, J. Yin, Z. Yoo, I. -K. Yushmanov, I. Zaccolo, V. Zach, C. Zaman, A. Zampolli, C. Zaporozhets, S. Zarochentsev, A. Zavada, P. Zaviyalov, N. Zbroszczyk, H. Zgura, I. S. Zhalov, M. Zhang, H. Zhang, X. Zhang, Y. Zhao, C. Zhigareva, N. Zhou, D. Zhou, F. Zhou, Y. Zhou, Zhuo Zhu, H. Zhu, J. Zhu, X. Zichichi, A. Zimmermann, A. Zimmermann, M. B. Zinovjev, G. Zoccarato, Y. Zyzak, M. CA ALICE Collaboration TI Multiparticle azimuthal correlations in p-Pb and Pb-Pb collisions at the CERN Large Hadron Collider SO PHYSICAL REVIEW C LA English DT Article ID NUCLEUS-NUCLEUS COLLISIONS; QUARK-GLUON PLASMA; ANGULAR-CORRELATIONS; TRANSVERSE-MOMENTUM; ROOT-S(NN)=5.02 TEV; PPB COLLISIONS; LONG-RANGE; FLOW; DEPENDENCE; ECCENTRICITIES AB Measurements of multiparticle azimuthal correlations (cumulants) for charged particles in p-Pb at root s(NN) = 5.02 TeV and Pb-Pb at root s(NN) = 2.76 TeV collisions are presented. They help address the question of whether there is evidence for global, flowlike, azimuthal correlations in the p-Pb system. Comparisons are made to measurements from the larger Pb-Pb system, where such evidence is established. In particular, the second harmonic two-particle cumulants are found to decrease with multiplicity, characteristic of a dominance of few-particle correlations in p-Pb collisions. However, when a vertical bar Delta eta vertical bar gap is placed to suppress such correlations, the two-particle cumulants begin to rise at high multiplicity, indicating the presence of global azimuthal correlations. The Pb-Pb values are higher than the p-Pb values at similar multiplicities. In both systems, the second harmonic four-particle cumulants exhibit a transition from positive to negative values when the multiplicity increases. The negative values allow for a measurement of v(2){4} to be made, which is found to be higher in Pb-Pb collisions at similar multiplicities. The second harmonic six-particle cumulants are also found to be higher in Pb-Pb collisions. In Pb-Pb collisions, we generally find v(2){4} similar or equal to v(2){6} not equal 0 which is indicative of a Bessel-Gaussian function for the v(2) distribution. For very high-multiplicity Pb-Pb collisions, we observe that the four-and six-particle cumulants become consistent with 0. Finally, third harmonic two-particle cumulants in p-Pb and Pb-Pb are measured. These are found to be similar for overlapping multiplicities, when a vertical bar Delta eta vertical bar > 1.4 gap is placed. C1 [Abelev, B.; Garishvili, I.; Soltz, R.] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA. [Adam, J.; Bielcik, J.; Broz, M.; Cepila, J.; Contreras, J. G.; Krelina, M.; Pachr, M.; Petracek, V.; Petran, M.; Schulc, M.; Spacek, M.; Wagner, V.; Zach, C.] Czech Tech Univ, Fac Nucl Sci & Phys Engn, CR-11519 Prague, Czech Republic. [Adamova, D.; Bielcikova, J.; Ferencei, J.; Krizek, F.; Kucera, V.; Kushpil, S.; Sumbera, M.; Vajzer, M.] Acad Sci Czech Republic, Inst Nucl Phys, CZ-25068 Rez, Czech Republic. [Aggarwal, M. M.; Bhati, A. K.; Parmar, S.; Rathee, D.] Panjab Univ, Dept Phys, Chandigarh 160014, India. [Rinella, G. Aglieri; Augustinus, A.; Pedrosa, F. Baltasar Dos Santos; Betev, L.; Buncic, P.; Caffarri, D.; Carena, F.; Carena, W.; Cavicchioli, C.; Chapeland, S.; Chibante Barroso, V.; Chochula, P.; Costa, F.; Cunqueiro, L.; Divia, R.; Di Mauro, A.; Erazmus, B.; Esposito, M.; Floris, M.; Francescon, A.; Fuchs, U.; Gargiulo, C.; Gheata, A.; Gheata, M.; Giubellino, P.; Grigoras, C.; Grosse-Oetringhaus, J. F.; Grosso, R.; Hristov, P.; Ionita, C.; Kalweit, A.; Svn, M. Keil; Kluge, A.; Kobdaj, C.; Kofarago, M.; Kryshen, E.; Kugathasan, T.; Legrand, I.; Mager, M.; Martinengo, P.; Milano, L.; Morsch, A.; Mueller, H.; Musa, L.; Niculescu, M.; Pinazza, O.; Poghosyan, M. G.; Reidt, F.; Revol, J. -P.; Riedler, P.; Riegler, W.; Rossi, A.; Safarik, K.; Schukraft, J.; Schutz, Y.; Shahoyan, R.; Szczepankiewicz, A.; Martinez, A. Tarazona; Tauro, A.; Van Hoorne, J. W.; Volpe, G.; von Haller, B.; Vranic, D.; Weber, M.; Zimmermann, M. B.] CERN, European Org Nucl Res, CH-1211 Geneva, Switzerland. [Agnello, M.; Aimo, I.; Alessandro, B.; Arnaldi, R.; Bagnasco, S.; Beole, S.; Berzano, D.; Bianchi, L.; Botta, E.; Bruna, E.; Bufalino, S.; Cerello, P.; Morales, Y. Corrales; De Marco, N.; Feliciello, A.; Ferretti, A.; Gagliardi, M.; Gallio, M.; Innocenti, G. M.; Lattuca, A.; La Pointe, S. L.; Leoncino, M.; Marchisone, M.; Masera, M.; Oppedisano, C.; Prino, F.; Rivetti, A.; Russo, R.; Scomparin, E.; Shtejer, K.; Vallero, S.; Vercellin, E.] Sezione Ist Nazl Fis Nucl, Turin, Italy. [Agnello, M.; Aimo, I.; Bedda, C.] Politecn Torino, Turin, Italy. [Agostinelli, A.; Arcelli, S.; Basile, M.; Cifarelli, L.; Colocci, M.; Falchieri, D.; Guerzoni, B.; Scioli, G.; Zichichi, A.] Univ Bologna, Dipartimento Fis & Astron, Bologna, Italy. [Agostinelli, A.; Alici, A.; Antonioli, P.; Arcelli, S.; Basile, M.; Bellini, F.; Cifarelli, L.; Cindolo, F.; Colocci, M.; Falchieri, D.; Guerzoni, B.; Hatzifotiadou, D.; Margotti, A.; Nania, R.; Noferini, F.; Pesci, A.; Pinazza, O.; Preghenella, R.; Scapparone, E.; Scioli, G.; Williams, M. C. S.; Zampolli, C.; Zichichi, A.] Sezione Ist Nazl Fis Nucl, Bologna, Italy. [Agrawal, N.; Behera, N. K.; Dash, S.; Meethaleveedu, G. Koyithatta; Kumar, J.; Nandi, B. K.; Pant, D.; Varma, R.] Indian Inst Technol, Bombay 400076, Maharashtra, India. [Ahammed, Z.; Alam, S. N.; Basu, S.; Chattopadhyay, S.; Choudhury, S.; De, S.; Dubey, A. K.; Ghosh, P.; Kar, S.; Khan, S. A.; Mitra, J.; Mohanty, B.; Muhuri, S.; Mukherjee, M.; Nayak, T. K.; Pal, S. K.; Saini, J.; Sarkar, D.; Singaraju, R.; Singha, S.; Singhal, V.; Sinha, B. C.; Viyogi, Y. P.] Ctr Variable Energy Cyclotron, Kolkata, India. [Ahmad, N.; Azmi, M. D.; Irfan, M.; Khan, M. M.] Aligarh Muslim Univ, Dept Phys, Aligarh 202002, Uttar Pradesh, India. [Ahmed, I.; Ajaz, M.; Khan, K. H.; Rauf, A. W.; Suleymanov, M.; Zaman, A.] COMSATS Inst Informat Technol, Islamabad, Pakistan. [Ahn, S. U.; Ahn, S. A.; Jang, H. J.; Kim, D. W.] Korea Inst Sci & Technol Informat, Taejon, South Korea. [Aiola, S.; Aronsson, T.; Caines, H.; Connors, M. E.; Ehlers, R. J.; Harris, J. W.; Ma, R.; Majka, R. D.; Oh, S.; Reed, R. J.; Schuster, T.; Smirnov, N.] Yale Univ, New Haven, CT USA. [Akindinov, A.; Kiselev, S.; Mal'Kevich, D.; Mikhaylov, K.; Nedosekin, A.; Sultanov, R.; Voloshin, K.; Zhigareva, N.] Inst Theoret & Expt Phys, Moscow 117259, Russia. [Aleksandrov, D.; Blau, D.; Fokin, S.; Ippolitov, M.; Kucheriaev, Y.; Manko, V.; Nikolaev, S.; Nikulin, S.; Nyanin, A.; Peresunko, D.; Ryabinkin, E.; Sibiriak, Y.; Vasiliev, A.; Vinogradov, A.; Yasnopolskiy, S.; Yushmanov, I.] Russian Res Ctr, Kurchatov Inst, Moscow, Russia. [Alexandre, D.; Barnby, L. S.; Evans, D.; Hanratty, L. D.; Jones, P. G.; Jusko, A.; Krivda, M.; Lee, G. R.; Lietava, R.; Baillie, O. Villalobos] Univ Birmingham, Sch Phys & Astron, Birmingham, W Midlands, England. [Alici, A.; Cifarelli, L.; De Caro, A.; De Gruttola, D.; Noferini, F.; Preghenella, R.; Zichichi, A.] Ctr Fermi Museo Stor Fis, Rome, Italy. [Alici, A.; Cifarelli, L.; De Caro, A.; De Gruttola, D.; Noferini, F.; Preghenella, R.; Zichichi, A.] Ctr Studi & Ric Enrico Fermi, Rome, Italy. [Alkin, A.; Chelnokov, V.; Grinyov, B.; Martynov, Y.; Trubnikov, V.; Zinovjev, G.] Bogolyubov Inst Theoret Phys, Kiev, Ukraine. [Alme, J.; Erdal, H. A.; Helstrup, H.; Hetland, K. F.; Kileng, B.] Bergen Univ Coll, Fac Engn, Bergen, Norway. [Alt, T.; Bach, M.; de Cuveland, J.; Eschweiler, D.; Gerhard, J.; Gorbunov, S.; Hartmann, H.; Hutter, D.; Kalcher, S.; Kirsch, S.; Kisel, I.; Kollegger, T.; Kretz, M.; Krzewicki, M.; Lindenstruth, V.; Painke, F.; Rettig, F.; Rohr, D.] Goethe Univ Frankfurt, Frankfurt Inst Adv Studies, D-60054 Frankfurt, Germany. [Altinpinar, S.; Djuvsland, O.; Fehlker, D.; Haaland, O.; Huang, M.; Loenne, P. I.; Nystrand, J.; Rehman, A.; Rohrich, D.; Skjerdal, K.; Ullaland, K.; Velure, A.; Wagner, B.; Yang, S.; Zhou, Zhuo] Univ Bergen, Dept Phys & Technol, Bergen, Norway. [Altsybeev, I.; Feofilov, G.; Kolojvari, A.; Kondratiev, V.; Kovalenko, V.; Vechernin, V.; Vinogradov, L.; Vorobyev, I.; Zarochentsev, A.] St Petersburg State Univ, V Fock Inst Phys, St Petersburg 199034, Russia. [Alves Garcia Prado, C.; Bregant, M.; Cosentino, M. R.; Domenicis Gimenez, D.; Jahnke, C.; Lagana Fernandes, C.; Moreira De Godoy, D. A.; Munhoz, M. G.; Oliveira Da Silva, A. C.; Pereira De Oliveira Filho, E.; Suaide, A. A. P.; Szanto de Toledo, A.] Univ Sao Paulo, Sao Paulo, Brazil. [Andrei, C.; Bercuci, A.; Catanescu, V.; Herghelegiu, A.; Petris, M.; Petrovici, M.; Pop, A.; Schiaua, C.; Tarzila, M. G.] Natl Inst Phys & Nucl Engn, Bucharest, Romania. [Andrei, C.; Berceanu, I.; Catanescu, V.; Herghelegiu, A.; Petris, M.; Petrovici, M.; Pop, A.; Schiaua, C.; Tarzila, M. G.] GSI Helmholtzzentrum Schwerionenforschung, Div Res, Darmstadt, Germany. GSI Helmholtzzentrum Schwerionenforschung, ExtreMe Matter Inst, Darmstadt, Germany. [Andronic, A.; Arsene, I. C.; Averbeck, R.; Braun-Munzinger, P.; Foka, P.; Frankenfeld, U.; Garabatos, C.; Ivanov, M.; Knichel, M. L.; Koehler, M. K.; Krzewicki, M.; Lippmann, C.; Malzacher, P.; Martin, N. A.; Masciocchi, S.; Miskowiec, D.; Nicassio, M.; Onderwaater, J.; Otwinowski, J.; Park, W. J.; Schmidt, C.; Schwarz, K.; Selyuzhenkov, I.; Vranic, D.; Wagner, J.] Heidelberg Univ, Inst Phys, Heidelberg, Germany. [Anguelov, V.; Bock, F.; Busch, O.; Fasel, M.; Glaessel, P.; Klein, J.; Kweon, M. J.; Leardini, L.; Lohner, D.; Lu, X. -G.; Maire, A.; Perez, J. Mercado; Oeschler, H.; Oyama, K.; Pachmayer, Y.; Reidt, F.; Reygers, K.; Schiaua, C.; Stiller, J. H.; Vallero, S.; Voelkl, M. A.; Wang, Y.; Wilkinson, J.; Windelband, B.; Winn, M.; Zimmermann, A.] Univ Munster, Inst Kernphys, D-48149 Munster, Germany. [Anticic, T.; Planinic, M.; Poljak, N.; Susa, T.] Rudjer Boskovic Inst, Zagreb, Croatia. [Antinori, F.; Caffarri, D.; Dainese, A.; Fabris, D.; Festanti, A.; Francescon, A.; Jena, C.; Lunardon, M.; Morando, M.; Moretto, S.; Scarlassara, F.; Segato, G.; Soramel, F.; Toia, A.; Turrisi, R.; Viesti, G.] Sezione Ist Nazl Fis Nucl, Padua, Italy. [Aphecetche, L.; Batigne, G.; Delagrange, H.; Erazmus, B.; Estienne, M.; Germain, M.; Lardeux, A.; Garcia, G. Martinez; Blanco, J. Martin; Mas, A.; Massacrier, L.; Morreale, A.; Pillot, P.; Ronflette, L.; Schutz, Y.; Shabetai, A.; Stocco, D.; Wang, M.] Univ Nantes, Ecole Mines Nantes, SUBATECH, CNRS IN2P3, Nantes, France. [Appelshaeuser, H.; Arslandok, M.; Bailhache, R.; Baumann, C.; Beck, H.; Blume, C.; Book, J.; Broker, T. A.; Buesching, H.; Dillenseger, P.; Heckel, S. T.; Kamin, J.; Kulakov, I.; Lehnert, J.; Luettig, P.; Marquard, M.; Ozdemir, M.; Peskov, V.; Rascanu, B. T.; Reichelt, P.; Renfordt, R.; Sahlmuller, B.; Schuchmann, S.; Peloni, A. Tarantola; Toia, A.; Zyzak, M.] Goethe Univ Frankfurt, Inst Kernphys, Frankfurt, Germany. [Armesto, N.; Ferreiro, E. G.; Pajares, C.; Salgado, C. A.] Univ Santiago de Compostela, Dept Fis Particulas, Santiago De Compostela, Spain. [Armesto, N.; Ferreiro, E. G.; Pajares, C.; Salgado, C. A.] Univ Santiago de Compostela, IGFAE, Santiago De Compostela, Spain. [Arsene, I. C.; Batzing, P. C.; Dordic, O.; Lindal, S.; Mahmood, S. M.; Milosevic, J.; Qvigstad, H.; Richter, M.; Roed, K.; Skaali, T. B.; Tveter, T. S.; Wikne, J.; Zhao, C.] Univ Oslo, Dept Phys, Oslo, Norway. [Awes, T. C.; Cormier, T. M.; Ganoti, P.; Silvermyr, D.] Oak Ridge Natl Lab, Oak Ridge, TN USA. [Azmi, M. D.; Cleymans, J.; Dietel, T.; Gumbo, M.; Murray, S.] Univ Cape Town, Dept Phys, ZA-7925 Cape Town, South Africa. [Badala, A.; Barbera, R.; Jacholkowski, A.; La Rocca, P.; Palmeri, A.; Pappalardo, G. S.; Petta, C.; Riggi, F.; Santagati, G.] Sezione Ist Nazl Fis Nucl, Catania, Italy. [Baek, Y. W.; Jung, H.; Kim, D. W.; Kim, M.; Oh, S. K.] Gangneung Wonju Natl Univ, Kangnung, South Korea. [Baek, Y. W.; Barret, V.; Bastid, N.; Camejo, A. Batista; Crochet, P.; Dupieux, P.; Li, S.; Lopez, X.; Manso, F.; Marchisone, M.; Porteboeuf-Houssais, S.; Rosnet, P.; Palomo, L. Valencia; Vulpescu, B.] Univ Clermont Ferrand, Univ Blaise Pascal, Phys Corpusculaire Lab, CNRS IN2P3, Clermont Ferrand, France. [Bala, R.; Bhasin, A.; Bhat, I. R.; Gupta, A.; Gupta, R.; Potukuchi, B.; Rohni, S.; Sambyal, S.; Sharma, S.; Singh, R.] Univ Jammu, Dept Phys, Jammu 180004, India. [Baldisseri, A.; Castellanos, J. Castillo; Charvet, J. L.; Da Costa, H. Pereira; Rakotozafindrabe, A.] IRFU, Commissariat Energie Atom, Saclay, France. [Baral, R. C.; Mahapatra, D. P.; Sahu, P. K.] Inst Phys, Bhubaneswar 751007, Orissa, India. [Barbera, R.; Jacholkowski, A.; La Rocca, P.; Petta, C.; Santagati, G.] Univ Catania, Dipartimento Fis & Astron, Catania, Italy. [Barile, F.; Bruno, G. E.; Colamaria, F.; Colella, D.; D'Erasmo, G.; Di Bari, D.; Fionda, F. M.; Fiore, E. M.; Ghidini, B.; Mastroserio, A.; Tangaro, M. A.] Dipartimento Interateneo Fis M Merlin, Bari, Italy. [Barile, F.; Bruno, G. E.; Colamaria, F.; Colella, D.; D'Erasmo, G.; de Cataldo, G.; Di Bari, D.; Elia, D.; Fionda, F. M.; Fiore, E. M.; Ghidini, B.; Lenti, V.; Manzari, V.; Mastroserio, A.; Nappi, E.; Paticchio, V.; Tangaro, M. A.] Sezione Ist Nazl Fis Nucl, Bari, Italy. [Bartke, J.; Figiel, J.; Gladysz-Dziadus, E.; Goerlich, L.; Kowalski, M.; Matyja, A.; Mayer, C.; Otwinowski, J.; Rybicki, A.; Sputowska, I.] Hungarian Acad Sci, Wigner Res Ctr Phys, Budapest, Hungary. [Bartke, J.; Figiel, J.; Gladysz-Dziadus, E.; Goerlich, L.; Kowalski, M.; Matyja, A.; Mayer, C.; Otwinowski, J.; Rybicki, A.; Sputowska, I.] Polish Acad Sci, Niewodniczanski Inst Nucl Phys, Krakow, Poland. [Batyunya, B.; Grigoryan, S.; Kadyshevskiy, V.; Malinina, L.; Mikhaylov, K.; Nomokonov, P.; Rogochaya, E.; Shabratova, G.; Vala, M.; Vodopyanov, A.; Zaporozhets, S.] Joint Inst Nucl Res, Dubna, Russia. [Bearden, I. G.; Bilandzic, A.; Boggild, H.; Chojnacki, M.; Gaardhoje, J. J.; Gulbrandsen, K.; Hansen, A.; Nielsen, B. S.; Zaccolo, V.] Univ Copenhagen, Niels Bohr Inst, DK-2100 Copenhagen, Denmark. [Belikov, I.; Hippolyte, B.; Kuhn, C.; Maire, A.; Molnar, L.; Roy, C.; Castro, X. Sanchez] Univ Strasbourg, Inst Pluridisciplinaire Hubert Curien, CNRS, IN2P3, Strasbourg, France. [Bellwied, R.; Chinellato, D. D.; Jayarathna, P. H. S. Y.; Jena, S.; Pinsky, L.; Piyarathna, D. B.; Timmins, A. R.; Weber, M.] Univ Houston, Houston, TX USA. [Belmont-Moreno, E.; Menchaca-Rocha, A.; Sandoval, A.; Serradilla, E.] Univ Nacl Autonoma Mexico, Inst Fis, Mexico City 01000, DF, Mexico. [Belmont, R., III; Borissov, A.; Cormier, T. M.; Loggins, V. R.; Mlynarz, J.; Prasad, S. K.; Pruneau, C. A.; Pujahari, P.; Putschke, J.; Reed, R. J.; Verweij, M.; Voloshin, S. A.; Yaldo, C. G.] Wayne State Univ, Detroit, MI USA. [Belyaev, V.; Bogdanov, A.; Grigoriev, V.; Kaplin, V.; Kondratyeva, N.; Loginov, V.] Moscow Engn Phys Inst, Moscow 115409, Russia. [Beole, S.; Berzano, D.; Bianchi, L.; Botta, E.; Morales, Y. Corrales; Ferretti, A.; Gagliardi, M.; Gallio, M.; Innocenti, G. M.; Lattuca, A.; Leoncino, M.; Marchisone, M.; Masera, M.; Russo, R.; Shtejer, K.; Vallero, S.; Vercellin, E.] Univ Turin, Dipartmento Fis, Turin, Italy. [Beole, S.; Berzano, D.; Bianchi, L.; Botta, E.; Morales, Y. Corrales; Ferretti, A.; Gagliardi, M.; Gallio, M.; Innocenti, G. M.; Lattuca, A.; Leoncino, M.; Marchisone, M.; Masera, M.; Russo, R.; Shtejer, K.; Vallero, S.; Vercellin, E.] Sezione Ist Nazl Fis Nucl, Turin, Italy. [Berdnikov, Y.] St Petersburg State Polytech Univ, St Petersburg, Russia. [Berdnikov, Y.; Ivanov, V.; Khanzadeev, A.; Malaev, M.; Nikulin, V.; Riabov, V.; Ryabov, Y.; Samsonov, V.; Zhalov, M.] Petersburg Nucl Phys Inst, Gatchina, Russia. [Berger, M. E.; Boehmer, F. V.; Dorheim, S.] Tech Univ Munich, Dept Phys, D-80290 Munich, Germany. [Bertens, R. A.; Bianchin, C.; Bjelogrlic, S.; Caliva, A.; de Cataldo, G.; de Rooij, R.; Dubla, A.; Grelli, A.; Keijdener, D. L. D.; La Pointe, S. L.; Leogrande, E.; Lodato, D. F.; Luparello, G.; Mischke, A.; Mohammadi, N.; Nooren, G.; Peitzmann, T.; Reicher, M.; Rocco, E.; Snellings, R. J. M.; Thomas, D.; Van der Maarel, J.; van Leeuwen, M.; Veldhoen, M.; Yang, H.; Zhou, Y.] Univ Utrecht, Inst Subat Phys, Utrecht, Netherlands. [Bhattacharjee, B.; Hussain, N.] Gauhati Univ, Dept Phys, Gauhati, India. [Bhom, J.; Chujo, T.; Esumi, S.; Inaba, M.; Miake, Y.; Sano, M.; Watanabe, D.] Univ Tsukuba, Tsukuba, Ibaraki, Japan. [Bianchi, N.; Diaz, L. Calero; Cunqueiro, L.; Di Nezza, P.; Fantoni, A.; Gianotti, P.; Muccifora, V.; Reolon, A. R.; Ronchetti, F.; Sakai, S.; Spiriti, E.] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy. [Blanco, F.; Diaz Corchero, M. A.; Gonzalez-Zamora, P.; Montes, E.; Rubio Montero, A. J.; Serradilla, E.] CIEMAT, Ctr Invest Energet Medioambientales & Tecnol, E-28040 Madrid, Spain. [Bock, F.; Fasel, M.; Gangadharan, D. R.; Jacobs, P. M.; Loizides, C.; Ploskon, M.; Porter, J.; Symons, T. J. M.; Zhang, X.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Bogolyubsky, M.; Evdokimov, S.; Kharlov, Y.; Patalakha, D. I.; Polichtchouk, B.; Sadovsky, S.; Shangaraev, A.; Stolpovskiy, M.] SSC IHEP NRC Kurchatov Inst, Protvino, Russia. [Bombara, M.; Kravcakova, A.; Vrlakova, J.] Safarik Univ, Fac Nat Sci, Kosice, Slovakia. [Borissov, A.; Chung, S. U.; Seo, J.; Song, J.; Yi, J.; Yoo, I. -K.] Pusan Natl Univ, Pusan 609735, South Korea. [Bossu, F.; Buthelezi, Z.; Foertsch, S.; Steyn, G.; Vilakazi, Z.] Natl Res Fdn, iThemba LABS, Somerset West, South Africa. [Botje, M.; Christakoglou, P.; Kuijer, P. G.; Lara, C. E. Perez; Manso, A. Rodriguez] Natl Inst Subat Phys, Nikhef, Amsterdam, Netherlands. [Boettger, S.; Breitner, T.; Engel, H.; Ramirez, A. Gomez; Kebschull, U.; Lara, C.] Goethe Univ Frankfurt, Inst Phys, Frankfurt, Germany. [Browning, T. A.; Scharenberg, R. P.; Srivastava, B. K.] Purdue Univ, W Lafayette, IN 47907 USA. [Budnikov, D.; Filchagin, S.; Ilkaev, R.; Mamonov, A.; Nazarenko, S.; Punin, V.; Tumkin, A.; Vinogradov, Y.; Vyushin, A.; Zaviyalov, N.] Russian Fed Nucl Ctr VNIIEF, Sarov, Russia. [Caffarri, D.; Festanti, A.; Francescon, A.; Jena, C.; Lunardon, M.; Morando, M.; Moretto, S.; Scarlassara, F.; Segato, G.; Soramel, F.; Viesti, G.] Univ Padua, Dipartimento Fis & Astron, Padua, Italy. [Cai, X.; Dang, R.; Li, S.; Wang, M.; Yang, P.; Yin, Z.; Zhang, H.; Zhang, X.; Zhang, Y.; Zhou, D.; Zhou, F.; Zhu, J.] Cent China Normal Univ, Wuhan, Peoples R China. [Villar, E. Calvo; Gago, A. M.] Pontificia Univ Catolica Peru, Dept Ciencias, Secc Fis, Lima, Peru. [Camerini, P.; Lea, R.; Luparello, G.; Margagliotti, G. V.; Rui, R.; Venaruzzo, M.] Univ Trieste, Dipartmento Fis, I-34127 Trieste, Italy. [Camerini, P.; Gangadharan, D. R.; Humanic, T. J.; Lea, R.; Lisa, M. A.; Luparello, G.; Margagliotti, G. V.; Rui, R.; Salzwedel, J.; Steinpreis, M.; Venaruzzo, M.] Sezione Ist Nazl Fis Nucl, Trieste, Italy. [Casula, E. A. R.; Collu, A.; De Falco, A.; Puddu, G.; Razazi, V.; Terrevoli, C.; Usai, G. L.] Univ Cagliari, Dipartmento Fis, Cagliari, Italy. [Casula, E. A. R.; Collu, A.; De Falco, A.; Puddu, G.; Razazi, V.; Terrevoli, C.; Usai, G. L.] Sezione Ist Nazl Fis Nucl, Cagliari, Italy. [Sanchez, C. Ceballos; Lopez Torres, E.] Ctr Aplicac Tecnol & Desarrollo Nucl CEADEN, Havana, Cuba. [Chang, B.; Kim, D. J.; Kral, J.; Rak, J.; Slupecki, M.; Trzaska, W. H.; Vargyas, M.; Viinikainen, J.] Univ Jyvaskyla, Jyvaskyla, Finland. [Chattopadhyay, S.; Das, D.; Das, K.; Majumdar, A. K. Dutta; Khan, P.; Paul, B.; Roy, P.; Sinha, T.] Saha Inst Nucl Phys, Kolkata, India. [Cherney, M.; Nilsen, B. S.; Poghosyan, M. G.; Seger, J. E.] Creighton Univ, Dept Phys, Omaha, NE 68178 USA. [Cheshkov, C.; Cheynis, B.; Ducroux, L.; Grossiord, J. -Y.; Tieulent, R.; Uras, A.; Zoccarato, Y.] Univ Lyon 1, CNRS, IN2P3, IPN Lyon, F-69622 Villeurbanne, France. [Chinellato, D. D.; Dash, A.; Takahashi, J.] Univ Estadual Campinas, UNICAMP, Campinas, SP, Brazil. [Christiansen, P.; Ljunggren, H. M.; Ortiz Velasquez, A.; Oskarsson, A.; Richert, T.; Sogaard, C.; Stenlund, E.] Lund Univ, Div Expt High Energy Phys, Lund, Sweden. [Balbastre, G. Conesa; Faivre, J.; Furget, C.; Guernane, R.; Kox, S.; Real, J. S.; Silvestre, C.] Univ Grenoble Alpes, CNRS IN2P3, Lab Phys Subatom & Cosmol, Grenoble, France. [del Valle, Z. Conesa; Dash, A.; Espagnon, B.; Hadjidakis, C.; Lakomov, I.; Suire, C.; Takaki, J. D. Tapia] Univ Paris 11, CNRS, IN2P3, Inst Phys Nucl Orsay, F-91405 Orsay, France. [Contreras, J. G.; Cruz Albino, R.; Herrera Corral, G.; Montano Zetina, L.] CINVESTAV, Ctr Invest & Estudios Avanzados, Mexico City 14000, DF, Mexico. [Contreras, J. G.; Cruz Albino, R.; Herrera Corral, G.; Montano Zetina, L.] CINVESTAV, Ctr Invest & Estudios Avanzados, Merida, Mexico. [Cortese, P.; Ramello, L.; Sitta, M.] Univ Piemonte Orientale, Dipartimento Sci & Innovaz Tecnol, Alessandria, Italy. [Cortese, P.; Ramello, L.; Sitta, M.] Ist Nazl Fis Nucl, Grp Collegato, Alessandria, Italy. [Cortes Maldonado, I.; Fernandez Tellez, A.; Martinez, M. I.; Rodriguez Cahuantzi, M.; Tejeda Munoz, G.; Vargas, A.; Vergara Limon, S.] Benemerita Univ Autonoma Puebla, Puebla, Mexico. [Cuautle, E.; Jimenez Bustamante, R. T.; Ladron de Guevara, P.; Maldonado Cervantes, I.; Ortiz Velasquez, A.; Paic, G.] Univ Nacl Autonoma Mexico, Inst Ciencias Nucl, Mexico City 04510, DF, Mexico. [Danu, A.; Felea, D.; Gheata, M.; Haiduc, M.; Mitu, C. M.; Niculescu, M.; Sevcenco, A.; Stan, I.; Zgura, I. S.] Inst Space Sci, Bucharest, Romania. [Das, S.; Ghosh, P.; Prasad, S. K.; Raha, S.] Bose Inst, Dept Phys, Kolkata, India. [Das, S.; Ghosh, S. K.; Prasad, S. K.; Raha, S.] Ctr Astroparticle Phys & Space Sci, Kolkata, India. [Deloff, A.; Dobrowolski, T.; Ilkiv, I.; Kurashvili, P.; Redlich, K.; Siemiarczuk, T.; Stefanek, G.; Wilk, G.] Natl Ctr Nucl Studies, Warsaw, Poland. [De Caro, A.; De Gruttola, D.; De Pasquale, S.; Girard, M. Fusco; Meninno, E.; Pagano, P.; Virgili, T.] Univ Salerno, Dipartimento Fis ER Caianiello, I-84100 Salerno, Italy. [De Caro, A.; De Gruttola, D.; De Pasquale, S.; Girard, M. Fusco; Meninno, E.; Pagano, P.; Virgili, T.] Ist Nazl Fis Nucl, Grp Collegato, Salerno, Italy. [Di Liberto, S.; Mazzoni, M. A.] Sezione Ist Nazl Fis Nucl, Rome, Italy. [Hilden, T. E.; Pohjoisaho, E. H. O.; Rasanen, S. S.] Helsinki Inst Phys, Helsinki, Finland. [Figueredo, M. A. S.; Norman, J.; Romita, R.] Univ Liverpool, Liverpool L69 3BX, Merseyside, England. [Finogeev, D.; Furs, A.; Guber, F.; Karavichev, O.; Karavicheva, T.; Karpechev, E.; Konevskikh, A.; Kurepin, A.; Kurepin, A. B.; Maevskaya, A.; Pshenichnov, I.; Reshetin, A.] Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia. [Floratos, E.; Ganoti, P.; Roukoutakis, F.; Spyropoulou-Stassinaki, M.; Vasileiou, M.] Univ Athens, Dept Phys, Athens, Greece. [Gangadharan, D. R.; Humanic, T. J.; Lisa, M. A.; Salzwedel, J.; Steinpreis, M.] Ohio State Univ, Dept Phys, Columbus, OH 43210 USA. [Garcia-Solis, E.; Harton, A.] Chicago State Univ, Chicago, IL USA. [Gotovac, S.; Mudnic, E.; Vickovic, L.] Tech Univ Split FESB, Split, Croatia. [Grigoryan, A.; Gulkanyan, H.; Papikyan, V.] Warsaw Univ Technol, Warsaw, Poland. [Gunji, T.; Hamagaki, H.; Hayashi, S.; Sekiguchi, Y.; Tsuji, T.; Yamaguchi, Y.] Yerevan Phys Inst, AI Alikhanyan Natl Sci Lab, Yerevan 375036, Armenia. [Hess, B. A.; Schmidt, H. R.; Wiechula, J.] Univ Tokyo, Tokyo, Japan. [Hladky, J.; Mares, J.; Zavada, P.] Univ Tubingen, Tubingen, Germany. [Hladky, J.; Mares, J.; Zavada, P.] Acad Sci Czech Republic, Inst Phys, Prague, Czech Republic. [Hwang, D. S.; Kim, S.] Sejong Univ, Dept Phys, Seoul, South Korea. [Kang, J. H.; Kim, B.; Kim, M.; Kim, T.; Kwon, Y.; Song, M.] Slovak Acad Sci, Inst Expt Phys, Kosice 04353, Slovakia. [Kang, J. H.; Kwon, Y.; Song, M.] Yonsei Univ, Seoul 120749, South Korea. [Uysal, A. Karasu; Okatan, A.] KTO Karatay Univ, Konya, Turkey. [Keidel, R.] Fachhochschule Worms, Zentrum Technologietransfer & Telekommun, Worms, Germany. [Khan, M. M.] Aligarh Muslim Univ, Dept Appl Phys, Aligarh, Uttar Pradesh, India. [Klay, J. L.] Calif Polytech State Univ San Luis Obispo, San Luis Obispo, CA 93407 USA. [Kobdaj, C.] Univ Texas Austin, Dept Phys, Austin, TX 78712 USA. [Kobdaj, C.] Suranaree Univ Technol, Nakhon Ratchasima, Thailand. [Kweon, M. J.] Inha Univ, Inchon, South Korea. [Langoy, R.; Lien, J.] Vestfold Univ Coll, Tonsberg, Norway. [Lemmon, R. C.; Romita, R.] STFC Daresbury Lab, Nucl Phys Grp, Daresbury, England. [Leon Monzon, I.; Podesta-Lerma, P. L. M.; Sanchez Rodriguez, F. J.] Univ Autonoma Sinaloa, Culiacan, Mexico. [Malinina, L.] Moscow MV Lomonosov State Univ, DV Skobeltsyn Inst Nucl Phys, Moscow, Russia. [Martashvili, I.; Mazer, J.; Nattrass, C.; Read, K. F.; Scott, R.; Sharma, N.; Sorensen, S.] Univ Tennessee, Knoxville, TN USA. [Meddi, F.] Univ Roma La Sapienza, Dipartmento Fis, I-00185 Rome, Italy. [Meddi, F.] Sez INFN Rome, Rome, Italy. [Meres, M.; Pikna, M.; Sitar, B.; Strmen, P.; Szabo, A.; Szarka, I.] Comenius Univ, Fac Math Phys & Informat, Bratislava, Slovakia. [Milosevic, J.] Univ Belgrade, Fac Phys, Belgrade 11001, Serbia. [Milosevic, J.] Vinca Inst Nucl Sci, Belgrade, Serbia. [Mishra, A. N.; Sahoo, P.; Pareek, P.; Roy, A.; Sahoo, R.] Indian Inst Technol Indore, Indore, Madhya Pradesh, India. [Mohanty, B.; Nayak, K.; Singha, S.] Natl Inst Sci Educ & Res, Bhubaneswar, Orissa, India. [Oh, S. K.] Konkuk Univ, Seoul, South Korea. [Pestov, Y.] Budker Inst Nucl Phys, Novosibirsk 630090, Russia. [Simatovic, G.] Univ Zagreb, Zagreb 41000, Croatia. [Planinic, M.; Poljak, N.; Raniwala, R.; Raniwala, S.] Univ Rajasthan, Dept Phys, Jaipur 302004, Rajasthan, India. [Redlich, K.] Univ Wroclaw, Inst Theoret Phys, PL-50138 Wroclaw, Poland. [Ricci, R. A.; Venaruzzo, M.] Ist Nazl Fis Nucl, Lab Nazl Legnaro, I-35020 Legnaro, Italy. [Shigaki, K.; Sugitate, T.; Yano, S.] Hiroshima Univ, Hiroshima, Japan. [Takaki, J. D. Tapia] Univ Kansas, Lawrence, KS 66045 USA. [Vernet, R.] Ctr Calcul IN2P3, Villeurbanne, France. RP Abelev, B (reprint author), Lawrence Livermore Natl Lab, Livermore, CA 94550 USA. RI De Pasquale, Salvatore/B-9165-2008; Chinellato, David/D-3092-2012; de Cuveland, Jan/H-6454-2016; Kurepin, Alexey/H-4852-2013; Jena, Deepika/P-2873-2015; Akindinov, Alexander/J-2674-2016; Nattrass, Christine/J-6752-2016; Cosentino, Mauro/L-2418-2014; Suaide, Alexandre/L-6239-2016; Castillo Castellanos, Javier/G-8915-2013; Inst. of Physics, Gleb Wataghin/A-9780-2017; Zarochentsev, Andrey/J-6253-2013; Altsybeev, Igor/K-6687-2013; Vinogradov, Leonid/K-3047-2013; Kondratiev, Valery/J-8574-2013; Vechernin, Vladimir/J-5832-2013; Janik, Malgorzata/O-7520-2015; Graczykowski, Lukasz/O-7522-2015; feofilov, grigory/A-2549-2013; Adamova, Dagmar/G-9789-2014; Christensen, Christian/D-6461-2012; Mitu, Ciprian/E-6733-2011; Sevcenco, Adrian/C-1832-2012; Ahmed, Ijaz/E-9144-2015; Usai, Gianluca/E-9604-2015; Salgado, Carlos A./G-2168-2015; Bregant, Marco/I-7663-2012; Barnby, Lee/G-2135-2010; Barbera, Roberto/G-5805-2012; Bruna, Elena/C-4939-2014; Karasu Uysal, Ayben/K-3981-2015; HAMAGAKI, HIDEKI/G-4899-2014; Pshenichnov, Igor/A-4063-2008; Guber, Fedor/I-4271-2013; Vajzer, Michal/G-8469-2014; Wagner, Vladimir/G-5650-2014; Sumbera, Michal/O-7497-2014; Peitzmann, Thomas/K-2206-2012; Kharlov, Yuri/D-2700-2015; Kovalenko, Vladimir/C-5709-2013; Takahashi, Jun/B-2946-2012; Felea, Daniel/C-1885-2012; Barnafoldi, Gergely Gabor/L-3486-2013; Kucera, Vit/G-8459-2014; Krizek, Filip/G-8967-2014; Bielcikova, Jana/G-9342-2014; Ferreiro, Elena/C-3797-2017; Armesto, Nestor/C-4341-2017; Ferretti, Alessandro/F-4856-2013; Martinez Hernandez, Mario Ivan/F-4083-2010; Vickovic, Linda/F-3517-2017; Fernandez Tellez, Arturo/E-9700-2017; Jena, Satyajit/P-2409-2015; Rui, Rinaldo/L-1926-2015 OI De Pasquale, Salvatore/0000-0001-9236-0748; Chinellato, David/0000-0002-9982-9577; de Cuveland, Jan/0000-0003-0455-1398; Kurepin, Alexey/0000-0002-1851-4136; Jena, Deepika/0000-0003-2112-0311; Akindinov, Alexander/0000-0002-7388-3022; Nattrass, Christine/0000-0002-8768-6468; Cosentino, Mauro/0000-0002-7880-8611; Suaide, Alexandre/0000-0003-2847-6556; Castillo Castellanos, Javier/0000-0002-5187-2779; Zarochentsev, Andrey/0000-0002-3502-8084; Altsybeev, Igor/0000-0002-8079-7026; Vinogradov, Leonid/0000-0001-9247-6230; Kondratiev, Valery/0000-0002-0031-0741; Vechernin, Vladimir/0000-0003-1458-8055; Janik, Malgorzata/0000-0002-3356-3438; feofilov, grigory/0000-0003-3700-8623; Christensen, Christian/0000-0002-1850-0121; Sevcenco, Adrian/0000-0002-4151-1056; Usai, Gianluca/0000-0002-8659-8378; Salgado, Carlos A./0000-0003-4586-2758; Barnby, Lee/0000-0001-7357-9904; Barbera, Roberto/0000-0001-5971-6415; Bruna, Elena/0000-0001-5427-1461; Karasu Uysal, Ayben/0000-0001-6297-2532; Pshenichnov, Igor/0000-0003-1752-4524; Guber, Fedor/0000-0001-8790-3218; Sumbera, Michal/0000-0002-0639-7323; Peitzmann, Thomas/0000-0002-7116-899X; Kovalenko, Vladimir/0000-0001-6012-6615; Takahashi, Jun/0000-0002-4091-1779; Felea, Daniel/0000-0002-3734-9439; Zhou, You/0000-0002-7868-6706; D'Erasmo, Ginevra/0000-0003-3407-6962; Beole', Stefania/0000-0003-4673-8038; Di Bari, Domenico/0000-0002-5559-8906; Murray, Sean/0000-0003-0548-588X; Fernandez Tellez, Arturo/0000-0001-5092-9748; Riggi, Francesco/0000-0002-0030-8377; Dainese, Andrea/0000-0002-2166-1874; Paticchio, Vincenzo/0000-0002-2916-1671; Scarlassara, Fernando/0000-0002-4663-8216; Turrisi, Rosario/0000-0002-5272-337X; Scomparin, Enrico/0000-0001-9015-9610; Virgili, Tiziano/0000-0003-0471-7052; Guerzoni, Barbara/0000-0003-3187-7051; Christiansen, Peter/0000-0001-7066-3473; Lemmon, Roy/0000-0002-1259-979X; Read, Kenneth/0000-0002-3358-7667; Ferreiro, Elena/0000-0002-4449-2356; Armesto, Nestor/0000-0003-0940-0783; Ferretti, Alessandro/0000-0001-9084-5784; Martinez Hernandez, Mario Ivan/0000-0002-8503-3009; Vickovic, Linda/0000-0002-9820-7960; Fernandez Tellez, Arturo/0000-0003-0152-4220; Gaardhoje, Jens-Jorgen/0000-0001-6122-4698; Feliciello, Alessandro/0000-0001-5823-9733; Fiore, Enrichetta Maria/0000-0002-3548-2690; Jena, Satyajit/0000-0002-6220-6982; Rui, Rinaldo/0000-0002-6993-0332 FU Grid centres; Worldwide LHC Computing Grid (WLCG); State Committee of Science; World Federation of Scientists (WFS); Swiss Fonds Kidagan, Armenia; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq); Financiadora de Estudos e Projetos (FINEP); Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP); National Natural Science Foundation of China (NSFC); Chinese Ministry of Education (CMOE); Ministry of Science and Technology of China (MSTC); Ministry of Education and Youth of the Czech Republic; Danish Natural Science Research Council; Carlsberg Foundation; Danish National Research Foundation; European Research Council under the European Community; Helsinki Institute of Physics and the Academy of Finland; French CNRS-IN2P3; 'Region Pays de Loire'; 'Region Alsace'; 'Region Auvergne'; CEA, France; German BMBF; Helmholtz Association; General Secretariat for Research and Technology, Ministry of Development, Greece; Hungarian OTKA; National Office for Research and Technology (NKTH); Department of Atomic Energy and Department of Science and Technology of the Government of India; Istituto Nazionale di Fisica Nucleare (INFN); Centro Fermi - Museo Storico della Fisica e Centro Studi e Ricerche "Enrico Fermi", Italy; MEXT, Japan; Joint Institute for Nuclear Research, Dubna; National Research Foundation of Korea (NRF); CONACYT; DGAPA, Mexico; ALFA-EC; EPLANET Program (European Particle Physics Latin American Network); Stichting voor Fundamenteel Onderzoek der Materie (FOM); Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Netherlands; Research Council of Norway (NFR); Polish Ministry of Science and Higher Education; National Science Centre, Poland; Ministry of National Education/Institute for Atomic Physics; CNCS-UEFISCDI - Romania; Ministry of Education and Science of Russian Federation; Russian Academy of Sciences; Russian Federal Agency of Atomic Energy; Russian Federal Agency for Science and Innovations; Russian Foundation for Basic Research; Ministry of Education of Slovakia; Department of Science and Technology, South Africa; CIEMAT; EELA; Ministerio de Economia y Competitividad (MINECO) of Spain; Xunta de Galicia (Conselleria de Educacion); CEADEN, Cubaenergia, Cuba; IAEA (International Atomic Energy Agency); Swedish Research Council (VR); Knut & Alice Wallenberg Foundation (KAW); Ukraine Ministry of Education and Science; United Kingdom Science and Technology Facilities Council (STFC); United States Department of Energy; United States National Science Foundation FX The ALICE Collaboration would like to thank all its engineers and technicians for their invaluable contributions to the construction of the experiment and the CERN accelerator teams for the outstanding performance of the LHC complex. The ALICE Collaboration gratefully acknowledges the resources and support provided by all Grid centres and the Worldwide LHC Computing Grid (WLCG) collaboration. The ALICE Collaboration would like to thank the authors of the theoretical calculations for providing their results. The ALICE Collaboration acknowledges the following funding agencies for their support in building and running the ALICE detector: State Committee of Science, World Federation of Scientists (WFS) and Swiss Fonds Kidagan, Armenia; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP); National Natural Science Foundation of China (NSFC), the Chinese Ministry of Education (CMOE) and the Ministry of Science and Technology of China (MSTC); Ministry of Education and Youth of the Czech Republic; Danish Natural Science Research Council, the Carlsberg Foundation and the Danish National Research Foundation; The European Research Council under the European Community's Seventh Framework Programme; Helsinki Institute of Physics and the Academy of Finland; French CNRS-IN2P3, the 'Region Pays de Loire', 'Region Alsace', 'Region Auvergne' and CEA, France; German BMBF and the Helmholtz Association; General Secretariat for Research and Technology, Ministry of Development, Greece; Hungarian OTKA and National Office for Research and Technology (NKTH); Department of Atomic Energy and Department of Science and Technology of the Government of India; Istituto Nazionale di Fisica Nucleare (INFN) and Centro Fermi - Museo Storico della Fisica e Centro Studi e Ricerche "Enrico Fermi", Italy; MEXT Grant-in-Aid for Specially Promoted Research, Japan; Joint Institute for Nuclear Research, Dubna; National Research Foundation of Korea (NRF); CONACYT, DGAPA, Mexico, ALFA-EC and the EPLANET Program (European Particle Physics Latin American Network); Stichting voor Fundamenteel Onderzoek der Materie (FOM) and the Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Netherlands; Research Council of Norway (NFR); Polish Ministry of Science and Higher Education; National Science Centre, Poland; Ministry of National Education/Institute for Atomic Physics and CNCS-UEFISCDI - Romania; Ministry of Education and Science of Russian Federation, Russian Academy of Sciences, Russian Federal Agency of Atomic Energy, Russian Federal Agency for Science and Innovations and The Russian Foundation for Basic Research; Ministry of Education of Slovakia; Department of Science and Technology, South Africa; CIEMAT, EELA, Ministerio de Economia y Competitividad (MINECO) of Spain, Xunta de Galicia (Conselleria de Educacion), CEADEN, Cubaenergia, Cuba, and IAEA (International Atomic Energy Agency); Swedish Research Council (VR) and Knut & Alice Wallenberg Foundation (KAW); Ukraine Ministry of Education and Science; United Kingdom Science and Technology Facilities Council (STFC); The United States Department of Energy, the United States National Science Foundation, the State of Texas, and the State of Ohio. NR 41 TC 40 Z9 40 U1 1 U2 60 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0556-2813 EI 1089-490X J9 PHYS REV C JI Phys. Rev. C PD NOV 3 PY 2014 VL 90 IS 5 AR UNSP 054901 DI 10.1103/PhysRevC.90.054901 PG 16 WC Physics, Nuclear SC Physics GA AU2CN UT WOS:000345423700001 ER PT J AU Zhao, YX Wang, Y Allada, K Aniol, K Annand, JRM Averett, T Benmokhtar, F Bertozzi, W Bradshaw, PC Bosted, P Camsonne, A Canan, M Cates, GD Chen, C Chen, JP Chen, W Chirapatpimol, K Chudakov, E Cisbani, E Cornejo, JC Cusanno, F Dalton, MM Deconinck, W de Jager, CW De Leo, R Deng, X Deur, A Ding, H Dolph, PAM Dutta, C Dutta, D El Fassi, L Frullani, S Gao, H Garibaldi, F Gaskell, D Gilad, S Gilman, R Glamazdin, O Golge, S Guo, L Hamilton, D Hansen, O Higinbotham, DW Holmstrom, T Huang, J Huang, M Ibrahim, HF Iodice, M Jiang, X Jin, G Jones, MK Katich, J Kelleher, A Kim, W Kolarkar, A Korsch, W LeRose, JJ Li, X Li, Y Lindgren, R Liyanage, N Long, E Lu, HJ Margaziotis, DJ Markowitz, P Marrone, S McNulty, D Meziani, ZE Michaels, R Moffit, B Camacho, CM Nanda, S Narayan, A Nelyubin, V Norum, B Oh, Y Osipenko, M Parno, D Peng, JC Phillips, SK Posik, M Puckett, AJR Qian, X Qiang, Y Rakhman, A Ransome, R Riordan, S Saha, A Sawatzky, B Schulte, E Shahinyan, A Shabestari, MH Sirca, S Stepanyan, S Subedi, R Sulkosky, V Tang, LG Tobias, A Urciuoli, GM Vilardi, I Wang, K Wojtsekhowski, B Yan, X Yao, H Ye, Y Ye, Z Yuan, L Zhan, X Zhang, Y Zhang, YW Zhao, B Zheng, X Zhu, L Zhu, X Zong, X AF Zhao, Y. X. Wang, Y. Allada, K. Aniol, K. Annand, J. R. M. Averett, T. Benmokhtar, F. Bertozzi, W. Bradshaw, P. C. Bosted, P. Camsonne, A. Canan, M. Cates, G. D. Chen, C. Chen, J. -P. Chen, W. Chirapatpimol, K. Chudakov, E. Cisbani, E. Cornejo, J. C. Cusanno, F. Dalton, M. M. Deconinck, W. de Jager, C. W. De Leo, R. Deng, X. Deur, A. Ding, H. Dolph, P. A. M. Dutta, C. Dutta, D. El Fassi, L. Frullani, S. Gao, H. Garibaldi, F. Gaskell, D. Gilad, S. Gilman, R. Glamazdin, O. Golge, S. Guo, L. Hamilton, D. Hansen, O. Higinbotham, D. W. Holmstrom, T. Huang, J. Huang, M. Ibrahim, H. F. Iodice, M. Jiang, X. Jin, G. Jones, M. K. Katich, J. Kelleher, A. Kim, W. Kolarkar, A. Korsch, W. LeRose, J. J. Li, X. Li, Y. Lindgren, R. Liyanage, N. Long, E. Lu, H. -J. Margaziotis, D. J. Markowitz, P. Marrone, S. McNulty, D. Meziani, Z. -E. Michaels, R. Moffit, B. Camacho, C. Munoz Nanda, S. Narayan, A. Nelyubin, V. Norum, B. Oh, Y. Osipenko, M. Parno, D. Peng, J. -C. Phillips, S. K. Posik, M. Puckett, A. J. R. Qian, X. Qiang, Y. Rakhman, A. Ransome, R. Riordan, S. Saha, A. Sawatzky, B. Schulte, E. Shahinyan, A. Shabestari, M. H. Sirca, S. Stepanyan, S. Subedi, R. Sulkosky, V. Tang, L. -G. Tobias, A. Urciuoli, G. M. Vilardi, I. Wang, K. Wojtsekhowski, B. Yan, X. Yao, H. Ye, Y. Ye, Z. Yuan, L. Zhan, X. Zhang, Y. Zhang, Y. -W. Zhao, B. Zheng, X. Zhu, L. Zhu, X. Zong, X. CA Jefferson Lab Hall A Collaboration TI Single spin asymmetries in charged kaon production from semi-inclusive deep inelastic scattering on a transversely polarized He-3 target SO PHYSICAL REVIEW C LA English DT Article ID STATE INTERACTIONS; DRELL-YAN; LEPTOPRODUCTION; PROTON AB We report the first measurement of target single spin asymmetries of charged kaons produced in semi-inclusive deep inelastic scattering of electrons off a transversely polarized He-3 target. Both the Collins and Sivers moments, which are related to the nucleon transversity and Sivers distributions, respectively, are extracted over the kinematic range of 0.1 < x(bj) < 0.4 for K+ and K- production. While the Collins and Sivers moments for K+ are consistent with zero within the experimental uncertainties, both moments for K- favor negative values. The Sivers moments are compared to the theoretical prediction from a phenomenological fit to the world data. While the K+ Sivers moments are consistent with the prediction, the K- results differ from the prediction at the 2-sigma level. C1 [Zhao, Y. X.; Lu, H. -J.; Yan, X.; Ye, Y.] Univ Sci & Technol China, Hefei 230026, Peoples R China. [Wang, Y.; Peng, J. -C.; Zhu, L.] Univ Illinois, Urbana, IL 61801 USA. [Allada, K.; Bertozzi, W.; Deconinck, W.; Gilad, S.; Huang, J.; Moffit, B.; Puckett, A. J. R.; Sulkosky, V.; Zhan, X.] MIT, Cambridge, MA 02139 USA. [Allada, K.; Bosted, P.; Camsonne, A.; Chen, J. -P.; Chudakov, E.; de Jager, C. W.; Deur, A.; Gaskell, D.; Gilman, R.; Hansen, O.; Higinbotham, D. W.; Jones, M. K.; LeRose, J. J.; Michaels, R.; Moffit, B.; Nanda, S.; Qiang, Y.; Saha, A.; Sawatzky, B.; Sulkosky, V.; Wojtsekhowski, B.] Thomas Jefferson Natl Accelerator Facil, Newport News, VA 23606 USA. [Aniol, K.; Cornejo, J. C.; Margaziotis, D. J.] Calif State Univ Los Angeles, Los Angeles, CA 90032 USA. [Annand, J. R. M.; Hamilton, D.] Univ Glasgow, Glasgow G12 8QQ, Lanark, Scotland. [Averett, T.; Bradshaw, P. C.; Katich, J.; Kelleher, A.; Zhao, B.] Coll William & Mary, Williamsburg, VA 23187 USA. [Benmokhtar, F.] Duquesne Univ, Pittsburgh, PA 15282 USA. [Canan, M.; Golge, S.] Old Dominion Univ, Norfolk, VA 23529 USA. [Cates, G. D.; Chirapatpimol, K.; Dalton, M. M.; Deng, X.; Ding, H.; Dolph, P. A. M.; Jin, G.; Lindgren, R.; Liyanage, N.; Nelyubin, V.; Norum, B.; Riordan, S.; Shabestari, M. H.; Subedi, R.; Tobias, A.; Wang, K.; Zheng, X.] Univ Virginia, Charlottesville, VA 22904 USA. [Chen, C.; Tang, L. -G.; Ye, Z.; Yuan, L.; Zhu, L.] Hampton Univ, Williamsburg, VA 23187 USA. [Chen, W.; Gao, H.; Huang, M.; Qian, X.; Qiang, Y.; Zhu, X.; Zong, X.] Duke Univ, Durham, NC 27708 USA. [Cisbani, E.; Urciuoli, G. M.] Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy. [Cisbani, E.; Frullani, S.; Garibaldi, F.] Ist Super Sanita, I-00161 Rome, Italy. [Cusanno, F.; Frullani, S.; Garibaldi, F.] Ist Nazl Fis Nucl, Sez Roma, I-00161 Rome, Italy. [De Leo, R.; Marrone, S.; Vilardi, I.] Ist Nazl Fis Nucl, Sez Bari, I-70126 Bari, Italy. [De Leo, R.; Marrone, S.; Vilardi, I.] Univ Bari, I-70126 Bari, Italy. [Dutta, C.; Kolarkar, A.; Korsch, W.] Univ Kentucky, Lexington, KY 40506 USA. [Dutta, D.; Narayan, A.] Mississippi State Univ, Mississippi State, MS 39762 USA. [El Fassi, L.; Gilman, R.; Jiang, X.; Ransome, R.; Schulte, E.] Rutgers State Univ, Piscataway, NJ 08855 USA. [Glamazdin, O.] Kharkov Phys & Technol Inst, UA-61108 Kharkov, Ukraine. [Guo, L.; Huang, J.; Jiang, X.; Puckett, A. J. R.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA. [Holmstrom, T.] Longwood Univ, Farmville, VA 23909 USA. [Huang, J.; Qian, X.] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. [Ibrahim, H. F.] Cairo Univ, Giza 12613, Egypt. [Iodice, M.] Ist Nazl Fis Nucl, Sez Roma Tre, I-00146 Rome, Italy. [Kim, W.] Kyungpook Natl Univ, Taegu 702701, South Korea. [Li, X.; Li, Y.] China Inst Atom Energy, Beijing, Peoples R China. [Long, E.] Kent State Univ, Kent, OH 44242 USA. [Long, E.; Phillips, S. K.] Univ New Hampshire, Durham, NH 03824 USA. [Markowitz, P.] Florida Int Univ, Miami, FL 33199 USA. [McNulty, D.] Univ Massachusetts, Amherst, MA 01003 USA. [Meziani, Z. -E.; Posik, M.; Sawatzky, B.; Yao, H.] Temple Univ, Philadelphia, PA 19122 USA. [Camacho, C. Munoz] Univ Clermont Ferrand, IN2P3, F-63177 Aubiere, France. [Oh, Y.] Seoul Natl Univ, Seoul, South Korea. [Osipenko, M.] Ist Nazl Fis Nucl, Sez Genova, I-16146 Genoa, Italy. [Parno, D.] Carnegie Mellon Univ, Pittsburgh, PA 15213 USA. [Qian, X.] CALTECH, Kellogg Radiat Lab, Pasadena, CA 91125 USA. [Rakhman, A.] Syracuse Univ, Syracuse, NY 13244 USA. [Shahinyan, A.] Yerevan Phys Inst, Yerevan 375036, Armenia. [Sirca, S.] Univ Ljubljana, SI-1000 Ljubljana, Slovenia. [Stepanyan, S.] Kyungpook Natl Univ, Taegu 702701, South Korea. [Zhang, Y.; Zhang, Y. -W.] Lanzhou Univ, Lanzhou 730000, Gansu, Peoples R China. RP Zhao, YX (reprint author), Univ Sci & Technol China, Hefei 230026, Peoples R China. EM yxzhao@jlab.org RI Cisbani, Evaristo/C-9249-2011; Rakhman, Adurahim/K-8146-2012; Osipenko, Mikhail/N-8292-2015; Dalton, Mark/B-5380-2016; Narayan, Amrendra/Q-3243-2016; Parno, Diana/B-7546-2017; Ye, Zhihong/E-6651-2017 OI Cisbani, Evaristo/0000-0002-6774-8473; Qian, Xin/0000-0002-7903-7935; Rakhman, Adurahim/0000-0002-9880-6074; Osipenko, Mikhail/0000-0001-9618-3013; Dalton, Mark/0000-0001-9204-7559; Narayan, Amrendra/0000-0003-3814-9559; Parno, Diana/0000-0002-9363-0401; Ye, Zhihong/0000-0002-1873-2344 FU U.S. National Science Foundation; DOE [DE-AC05-06OR23177]; National Natural Science Foundation of China [11135002, 11120101004] FX We acknowledge the outstanding support of the JLab Hall A technical staff and the Accelerator Division in accomplishing this experiment. We also thank Alexei Prokudin for helpful discussions. This work was supported in part by the U.S. National Science Foundation, and by DOE Contract No. DE-AC05-06OR23177, under which the Jefferson Science Associates (JSA) operates the Thomas Jefferson National Accelerator Facility. This work was also supported by the National Natural Science Foundation of China under Grants No. 11135002 and No. 11120101004. NR 36 TC 10 Z9 10 U1 2 U2 10 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 0556-2813 EI 1089-490X J9 PHYS REV C JI Phys. Rev. C PD NOV 3 PY 2014 VL 90 IS 5 AR 055201 DI 10.1103/PhysRevC.90.055201 PG 6 WC Physics, Nuclear SC Physics GA AU2CN UT WOS:000345423700002 ER PT J AU Hattab, H Jnawali, G Horn-von Hoegen, M AF Hattab, H. Jnawali, G. Horn-von Hoegen, M. TI In-situ high-resolution low energy electron diffraction study of strain relaxation in heteroepitaxy of Bi(111) on Si(001): Interplay of strain state, misfit dislocation array and lattice parameter SO THIN SOLID FILMS LA English DT Article DE Bismuth; Heteroepitaxy; Strain state; Low-energy electron diffraction; Dislocation network ID SURFACTANT-MEDIATED GROWTH; SCANNING-TUNNELING-MICROSCOPY; THERMAL-EXPANSION; EPITAXIAL-GROWTH; HIGH-MOBILITY; GE; RELIEF; FILMS; SILICON; SI(111) AB The relief of lattice mismatch-induced strain in Bi(111) on Si(001) heteroepitaxial system was investigated in real time as the Bi film relaxes, by means of high resolution low-energy electron diffraction (LEED). The inherent lattice mismatch of 2.5% at room temperature is accommodated through the formation of an ordered misfit dislocation array confined to the interface. The strain fields of the dislocations cause a periodic height undulation of the surface in the sub-Angstrom regime, which is observed through spot splitting in LEED. From a simulations measurement of the position of the first-order LEED spots, which corresponds to the lattice parameter of the film, and of the separation of satellite spots, which corresponds to the ordering of the dislocation array, the evolution of the strain state during annealing of a 6 nm Bi film was determined. The strain is solely relaxed by full edge-type dislocations arranged in the ordered array at the interface. From the remaining strain of epsilon = 0.6% the critical thickness for generation of misfit dislocations under equilibrium conditions can be derived. (C) 2014 Published by Elsevier B.V. C1 Univ Duisburg Essen, Dept Phys, D-47057 Duisburg, Germany. Univ Duisburg Essen, Ctr Nanointegrat CENIDE, D-47057 Duisburg, Germany. RP Hattab, H (reprint author), Iowa State Univ, Ames Lab, US DOE, Ames, IA 50011 USA. FU Deutsche Forschungsgemeinschaft [SFB 616] FX Financial support from the Deutsche Forschungsgemeinschaft through SFB 616 "Energy Dissipation at Surfaces" is gratefully acknowledged. NR 38 TC 0 Z9 0 U1 2 U2 15 PU ELSEVIER SCIENCE SA PI LAUSANNE PA PO BOX 564, 1001 LAUSANNE, SWITZERLAND SN 0040-6090 J9 THIN SOLID FILMS JI Thin Solid Films PD NOV 3 PY 2014 VL 570 BP 159 EP 163 DI 10.1016/j.tsf.2014.08.013 PN A PG 5 WC Materials Science, Multidisciplinary; Materials Science, Coatings & Films; Physics, Applied; Physics, Condensed Matter SC Materials Science; Physics GA AT9EL UT WOS:000345230700026 ER PT J AU Jamison, RD Shen, YL AF Jamison, R. D. Shen, Y. -L. TI Indentation behavior of multilayered thin films: Effects of layer undulation SO THIN SOLID FILMS LA English DT Article; Proceedings Paper CT 3rd Biennial TACT International Thin Films Conference (TACT) CY OCT 05-09, 2013 CL Taipei, TAIWAN SP Taiwan Assoc Coatings & Thin Films Technol DE Nanoindentation; Multilayers; Finite element analysis; Layer undulation ID MECHANICAL-PROPERTIES; NANOINDENTATION; COMPOSITES; MICROSTRUCTURES; HARDNESS AB The behavior of aluminum/silicon carbide multilayered thin films in response to nanoindentation loading is studied. The effect of undulating layer geometry on indentation derived hardness and modulus, and stress/strain field development, is investigated using the finite element method. Two regular waveforms that are 180 degrees out-of-phase are used to represent the undulating features of the SiC layers. The derived hardness and modulus are shown to be sensitive to the undulating layers and the phase of the waveform used to describe these layers. Undulating layers create bands of tensile and compressive axial stress that is significantly different from the flat layers. The amount of equivalent plastic strain in the Al layers is increased. Lastly, the unloading-induced plasticity in the Al layers is amplified with the presence of undulating layers. c 2014 Elsevier B. V. All rights reserved. C1 [Jamison, R. D.] Sandia Natl Labs, Albuquerque, NM 87175 USA. [Shen, Y. -L.] Univ New Mexico, Dept Mech Engn, Albuquerque, NM 87131 USA. RP Shen, YL (reprint author), Univ New Mexico, Dept Mech Engn, Albuquerque, NM 87131 USA. EM rdjamis@sandia.gov; shenyl@unm.edu RI Shen, Yu-Lin/C-1942-2008 NR 23 TC 4 Z9 4 U1 1 U2 11 PU ELSEVIER SCIENCE SA PI LAUSANNE PA PO BOX 564, 1001 LAUSANNE, SWITZERLAND SN 0040-6090 J9 THIN SOLID FILMS JI Thin Solid Films PD NOV 3 PY 2014 VL 570 BP 235 EP 242 DI 10.1016/j.tsf.2014.04.023 PN B PG 8 WC Materials Science, Multidisciplinary; Materials Science, Coatings & Films; Physics, Applied; Physics, Condensed Matter SC Materials Science; Physics GA AT9EN UT WOS:000345230900014 ER PT J AU Tanabe, KK Ferrandon, MS Siladke, NA Kraft, SJ Zhang, GH Niklas, J Poluektov, OG Lopykinski, SJ Bunel, EE Krause, TR Miller, JT Hock, AS Nguyen, ST AF Tanabe, Kristine K. Ferrandon, Magali S. Siladke, Nathan A. Kraft, Steven J. Zhang, Guanghui Niklas, Jens Poluektov, Oleg G. Lopykinski, Susan J. Bunel, Emilio E. Krause, Theodore R. Miller, Jeffrey T. Hock, Adam S. Nguyen, SonBinh T. TI Discovery of Highly Selective Alkyne Semihydrogenation Catalysts Based on First-Row Transition-Metallated Porous Organic Polymers SO ANGEWANDTE CHEMIE-INTERNATIONAL EDITION LA English DT Article DE heterogeneous catalysis; high-throughput screening; hydrogenation; polymers; transition metals ID RAY-ABSORPTION SPECTROSCOPY; ALKENE HYDROGENATION; HOMOGENEOUS CATALYSTS; SURFACE-AREA; COMPLEXES; CHROMIUM; LIGANDS; PRECURSORS; FRAMEWORKS; STABILITY AB Five different first-row transition metal precursors (V-III, Cr-III, Mn-II, Co-II, Ni-II) were successfully incorporated into a catechol porous organic polymer (POP) and characterized using ATR-IR and XAS analysis. The resulting metallated POPs were then evaluated for catalytic alkyne hydrogenation using high-throughput screening techniques. All POPs were unexpectedly found to be active and selective catalysts for alkyne semihydrogenation. Three of the metallated POPs (V, Cr, Mn) are the first of their kind to be active single-site hydrogenation catalysts. These results highlight the advantages of using a POP platform to develop new catalysts which are otherwise difficult to achieve through traditional heterogeneous and homogeneous routes. C1 [Tanabe, Kristine K.; Ferrandon, Magali S.; Siladke, Nathan A.; Kraft, Steven J.; Zhang, Guanghui; Niklas, Jens; Poluektov, Oleg G.; Lopykinski, Susan J.; Bunel, Emilio E.; Krause, Theodore R.; Miller, Jeffrey T.; Hock, Adam S.; Nguyen, SonBinh T.] Argonne Natl Lab, Chem Sci & Engn Div, Lemont, IL 60439 USA. [Hock, Adam S.] IIT, Dept Biol & Chem Sci, Chicago, IL 60616 USA. [Nguyen, SonBinh T.] Northwestern Univ, Dept Chem, Evanston, IL 60208 USA. [Nguyen, SonBinh T.] Northwestern Univ, Int Inst Nanotechnol, Evanston, IL 60208 USA. RP Miller, JT (reprint author), Argonne Natl Lab, Chem Sci & Engn Div, 9700 S Cass Ave, Lemont, IL 60439 USA. EM millerjt@anl.gov; hock@anl.gov; stn@anl.gov RI Zhang, Guanghui/C-4747-2008; Nguyen, SonBinh/C-1682-2014; ID, MRCAT/G-7586-2011; BM, MRCAT/G-7576-2011; Niklas, Jens/I-8598-2016; Hock, Adam/D-7660-2012 OI Zhang, Guanghui/0000-0002-5854-6909; Nguyen, SonBinh/0000-0002-6977-3445; Niklas, Jens/0000-0002-6462-2680; Hock, Adam/0000-0003-1440-1473 FU U.S. Department of Energy, Office of Basic Energy Sciences, Division of Chemical Sciences, Geosciences, and Biosciences [DE-AC02-06CH11357]; U.S. DOE [DE-AC02-06CH11357]; Department of Energy; MRCAT FX The authors thank Dr. Jeffrey Camacho-Bunquin and Dr. Marc J. A. Johnson for helpful discussions, Bo Hu for help with precursor synthesis, and Dr. Andrew "Bean" Getsoian, Dr. James Gallagher, and Dr. Elizabeth A. Mader for assistance with XAS experiments. This work was supported by the U.S. Department of Energy, Office of Basic Energy Sciences, Division of Chemical Sciences, Geosciences, and Biosciences, under Contract DE-AC02-06CH11357. Use of the Advanced Photon Source, an Office of Science User Facility operated for the U. S. Department of Energy (DOE) Office of Science by Argonne National Laboratory, was supported by the U.S. DOE under Contract No. DE-AC02-06CH11357. Materials Research Collaborative Access Team (MRCAT, Sector 10-BM) operations are supported by the Department of Energy and the MRCAT member institutions. NR 44 TC 16 Z9 16 U1 13 U2 98 PU WILEY-V C H VERLAG GMBH PI WEINHEIM PA BOSCHSTRASSE 12, D-69469 WEINHEIM, GERMANY SN 1433-7851 EI 1521-3773 J9 ANGEW CHEM INT EDIT JI Angew. Chem.-Int. Edit. PD NOV 3 PY 2014 VL 53 IS 45 BP 12055 EP 12058 DI 10.1002/anie.201405080 PG 4 WC Chemistry, Multidisciplinary SC Chemistry GA AS1PG UT WOS:000344052000006 PM 25219329 ER PT J AU Burgo, TAL Erdemir, A AF Burgo, Thiago A. L. Erdemir, Ali TI Bipolar Tribocharging Signal During Friction Force Fluctuations at Metal-Insulator Interfaces SO ANGEWANDTE CHEMIE-INTERNATIONAL EDITION LA English DT Article DE charge transfer; contact electrification; electrostatic interactions; friction; surface chemistry ID STICK-SLIP FRICTION; CONTACT ELECTRIFICATION; ENERGY-DISSIPATION; POLYMER SURFACES; IONIC ELECTRETS; CHARGE-TRANSFER; ADHESION; TRIBOELECTRIFICATION; TRIBOEMISSION; POLYETHYLENE AB Friction and triboelectrification of materials show a strong correlation during sliding contacts. Friction force fluctuations are always accompanied by two tribocharging events at metal-insulator [e. g., polytetrafluoroethylene (PTFE)] interfaces: injection of charged species from the metal into PTFE followed by the flow of charges from PTFE to the metal surface. Adhesion maps that were obtained by atomic force microscopy (AFM) show that the region of contact increases the pull-off force from 10 to 150 nN, reflecting on a resilient electrostatic adhesion between PTFE and the metallic surface. The reported results suggest that friction and triboelectrification have a common origin that must be associated with the occurrence of strong electrostatic interactions at the interface. C1 [Burgo, Thiago A. L.; Erdemir, Ali] Argonne Natl Lab, Div Energy Syst, Tribol Sect, Argonne, IL 60439 USA. RP Burgo, TAL (reprint author), Argonne Natl Lab, Div Energy Syst, Tribol Sect, 9700 S Cass Ave, Argonne, IL 60439 USA. EM tburgo@iqm.unicamp.br RI Burgo, Thiago Augusto Lima/G-2080-2012 OI Burgo, Thiago Augusto Lima/0000-0003-2521-3574 FU U. S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-AC02-06CH11357] FX Work at the Argonne National Laboratory and use of the Center for Nanoscale Materials was supported by the U. S. Department of Energy, Office of Science, Office of Basic Energy Sciences (DE-AC02-06CH11357). We also thank Dr. Osman Levent Eryilmaz for assistance with photography. NR 65 TC 3 Z9 3 U1 19 U2 53 PU WILEY-V C H VERLAG GMBH PI WEINHEIM PA BOSCHSTRASSE 12, D-69469 WEINHEIM, GERMANY SN 1433-7851 EI 1521-3773 J9 ANGEW CHEM INT EDIT JI Angew. Chem.-Int. Edit. PD NOV 3 PY 2014 VL 53 IS 45 BP 12101 EP 12105 DI 10.1002/anie.201406541 PG 5 WC Chemistry, Multidisciplinary SC Chemistry GA AS1PG UT WOS:000344052000016 PM 25168573 ER PT J AU Zhang, HB Gu, XK Canlas, C Kropf, AJ Aich, P Greeley, JP Elam, JW Meyers, RJ Dumesic, JA Stair, PC Marshall, CL AF Zhang, Hongbo Gu, Xiang-Kui Canlas, Christian Kropf, A. Jeremy Aich, Payoli Greeley, Jeffrey P. Elam, Jeffrey W. Meyers, Randall J. Dumesic, James A. Stair, Peter C. Marshall, Christopher L. TI Atomic Layer Deposition Overcoating: Tuning Catalyst Selectivity for Biomass Conversion SO ANGEWANDTE CHEMIE-INTERNATIONAL EDITION LA English DT Article DE atomic layer deposition; biomass; catalyst selectivity; hydrogenation; palladium ID SINGLE-CRYSTAL SURFACES; STRUCTURE SENSITIVITY; METAL NANOCRYSTALS; OXYGEN REDUCTION; SHAPE; HYDROGENATION; OXIDATION; ACID AB The terraces, edges, and facets of nanoparticles are all active sites for heterogeneous catalysis. These different active sites may cause the formation of various products during the catalytic reaction. Here we report that the step sites of Pd nanoparticles (NPs) can be covered precisely by the atomic layer deposition (ALD) method, whereas the terrace sites remain as active component for the hydrogenation of furfural. Increasing the thickness of the ALD-generated overcoats restricts the adsorption of furfural onto the step sites of Pd NPs and increases the selectivity to furan. Furan selectivities and furfural conversions are linearly correlated for samples with or without an overcoating, though the slopes differ. The ALD technique can tune the selectivity of furfural hydrogenation over Pd NPs and has improved our understanding of the reaction mechanism. The above conclusions are further supported by density functional theory (DFT) calculations. C1 [Zhang, Hongbo; Kropf, A. Jeremy; Stair, Peter C.; Marshall, Christopher L.] Argonne Natl Lab, Chem Sci & Engn Div, Lemont, IL 60439 USA. [Gu, Xiang-Kui; Greeley, Jeffrey P.] Purdue Univ, Sch Chem Engn, W Lafayette, IN 47907 USA. [Canlas, Christian; Elam, Jeffrey W.] Argonne Natl Lab, Div Energy Syst, Lemont, IL 60439 USA. [Aich, Payoli; Meyers, Randall J.] Univ Illinois, Dept Chem Engn, Chicago, IL 60607 USA. [Dumesic, James A.] Univ Wisconsin, Dept Chem & Biol Engn, Madison, WI 53706 USA. [Stair, Peter C.] Northwestern Univ, Dept Chem, Evanston, IL 60208 USA. RP Marshall, CL (reprint author), Argonne Natl Lab, Chem Sci & Engn Div, 9700 South Cass Ave, Lemont, IL 60439 USA. EM Marshall@anl.gov RI Gu, Xiangkui/H-3706-2014; Marshall, Christopher/D-1493-2015 OI Marshall, Christopher/0000-0002-1285-7648 FU Institute for Atom-Efficient Chemical Transformations (IACT); U.S. Department of Energy, Office of Science and Office of Basic Energy Sciences; U.S. Department of Energy, Office of Science, and Office of Basic Energy Sciences [DE-AC02-06CH11357]; Department of Energy; MRCAT FX This material is based upon work supported as part of the Institute for Atom-Efficient Chemical Transformations (IACT), an Energy Frontier Research Center funded by the U.S. Department of Energy, Office of Science and Office of Basic Energy Sciences. Use of the Advanced Photon Source is supported by the U.S. Department of Energy, Office of Science, and Office of Basic Energy Sciences, under Contract DE-AC02-06CH11357. MRCAT operations are supported by the Department of Energy and the MRCAT member institutions. We thank Dr. HengShou for helpful discussions. We thank Dr. Neil M. Schweitzer for the FTIR experiment. NR 24 TC 21 Z9 21 U1 27 U2 217 PU WILEY-V C H VERLAG GMBH PI WEINHEIM PA BOSCHSTRASSE 12, D-69469 WEINHEIM, GERMANY SN 1433-7851 EI 1521-3773 J9 ANGEW CHEM INT EDIT JI Angew. Chem.-Int. Edit. PD NOV 3 PY 2014 VL 53 IS 45 BP 12132 EP 12136 DI 10.1002/anie.201407236 PG 5 WC Chemistry, Multidisciplinary SC Chemistry GA AS1PG UT WOS:000344052000022 PM 25251418 ER PT J AU Xu, C Rao, LF AF Xu, Chao Rao, Linfeng TI Interactions of Bis(2,4,4-trimethylpentyl)dithiophosphinate with Nd-III and Cm-III in a Homogeneous Medium: A Comparative Study of Thermodynamics and Coordination Modes SO CHEMISTRY-A EUROPEAN JOURNAL LA English DT Article DE coordination modes; dithiophosphinate; lanthanide; actinides separation; thermodynamics ID DENSITY-FUNCTIONAL THEORY; PURIFIED CYANEX 301; DITHIOPHOSPHINIC ACIDS; SELECTIVE EXTRACTION; TRIVALENT ACTINIDES; CURIUM COMPLEXATION; LANTHANIDE CATIONS; DONOR LIGANDS; SEPARATION; COVALENCY AB Complexation of Nd-III and Cm-III with purified Cyanex301 (ammonium bis(2,4,4-trimethylpentyl)dithiophosphinate, denoted as HL) was studied in 1% v/v water/ethanol under identical conditions by spectrophotometry and microcalorimetry. For Nd-III, three successive complexes, NdL2+, NdL2+, and NdL3, formed in the solution. In contrast, four complexes, CmL2+, CmL2+, CmL3, and CmL4- formed during the titration with Cm. Fluorescence lifetime measurements provided additional insight into the complexation of Cm-III with Cyanex301. The stepwise stability constants for the CmLj(3-j)+ (j=1-3) complexes are about one order of magnitude higher than the corresponding NdLj(3-j)+ complexes. The enthalpies of complexation are endothermic for both Nd-III and Cm-III, suggesting that the energy required for desolvation exceeds the energy gained from the cation/ligand combination. Specifically, the enthalpy of complexation for CmL2+ is 3.5kJmol(-1) less endothermic than that of NdL2+, implying stronger covalent interaction in CmL2+ than NdL2+. However, the enthalpies of complexation for CmL2+ and NdL2+ are nearly identical, and the enthalpy of complexation for CmL3(aq) becomes more endothermic than that for NdL3(aq). The observations suggest that, in the ethanol/water media, the overall energetics of the Cm-III/Nd-III complexation with Cyanex301 could depend on a number of factors, including the extent of covalency, the degree of desolvation, and the coordination modes. C1 [Xu, Chao; Rao, Linfeng] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA. [Xu, Chao] Tsinghua Univ, Inst Nucl & New Energy Technol, Beijing 100084, Peoples R China. RP Rao, LF (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Chem Sci, 1 Cyclotron Rd, Berkeley, CA 94720 USA. EM LRao@lbl.gov RI XU, CHAO/S-4253-2016 OI XU, CHAO/0000-0001-5539-4754 FU Office of Science, Office of Basic Energy Science of the U. S. Department of Energy (DOE) at Lawrence Berkeley National Laboratory [DE-AC02-05CH11231]; China Scholarship Council; National Natural Science Foundation of China [21201107] FX This work was supported by the Director, Office of Science, Office of Basic Energy Science of the U. S. Department of Energy (DOE), under Contract No. DE-AC02-05CH11231 at Lawrence Berkeley National Laboratory. Dr. Chao Xu acknowledges the partial financial support from China Scholarship Council and National Natural Science Foundation of China (Grant No. 21201107). NR 48 TC 4 Z9 4 U1 3 U2 36 PU WILEY-V C H VERLAG GMBH PI WEINHEIM PA BOSCHSTRASSE 12, D-69469 WEINHEIM, GERMANY SN 0947-6539 EI 1521-3765 J9 CHEM-EUR J JI Chem.-Eur. J. PD NOV 3 PY 2014 VL 20 IS 45 BP 14807 EP 14815 DI 10.1002/chem.201402987 PG 9 WC Chemistry, Multidisciplinary SC Chemistry GA AS6FC UT WOS:000344358900035 PM 25213623 ER PT J AU King, AE Nippe, M Atanasov, M Chantarojsiri, T Wray, CA Bill, E Neese, F Long, JR Chang, CJ AF King, Amanda E. Nippe, Michael Atanasov, Mihail Chantarojsiri, Teera Wray, Curtis A. Bill, Eckhard Neese, Frank Long, Jeffrey R. Chang, Christopher J. TI A Well-Defined Terminal Vanadium(III) Oxo Complex SO INORGANIC CHEMISTRY LA English DT Article ID STATE PERTURBATION-THEORY; O BOND-CLEAVAGE; X-RAY-STRUCTURE; AEROBIC OXIDATION; STRUCTURAL-CHARACTERIZATION; PROPARGYLIC ALCOHOLS; ELECTRONIC-STRUCTURE; GENERATING HYDROGEN; CATALYZED OXIDATION; OXOPEROXO COMPLEXES AB The ubiquity of vanadium oxo complexes in the V+ and IV+ oxidation states has contributed to a comprehensive understanding of their electronic structure and reactivity. However, despite being predicted to be stable by ligand-field theory, the isolation and characterization of a well-defined terminal mononuclear vanadium(III) oxo complex has remained elusive. We present the synthesis and characterization of a unique terminal mononuclear vanadium(III) oxo species supported by the pentadentate polypyridyl ligand 2,6-bis[1,1-bis(2-pyridyl)ethyl]pyridine (PY5Me(2)). Exposure of [V(II)(NCCH3)(PY5Me(2))](2+) (1) to either dioxygen or selected O-atom-transfer reagents yields [V(IV)(O)(PY5Me(2))](2+) (2). The metal-centered one-electron reduction of this vanadium(IV) oxo complex furnishes a stable, diamagnetic [V(III)(O)(PY5Me(2))](+) (3) species. The vanadium(III) oxo species is unreactive toward H- and O-atom transfer but readily reacts with protons to form a putative vanadium hydroxo complex. Computational results predict that further one-electron reduction of the vanadium(III) oxo species will result in ligand-based reduction, even though pyridine is generally considered to be a poor p-accepting ligand. These results have implications for future efforts toward low-valent vanadyl chemistry, particularly with regard to the isolation and study of formal vanadium(II) oxo species. C1 [King, Amanda E.; Nippe, Michael; Chantarojsiri, Teera; Wray, Curtis A.; Long, Jeffrey R.; Chang, Christopher J.] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA. [King, Amanda E.; Nippe, Michael; Chang, Christopher J.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA. [Long, Jeffrey R.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA. [Chang, Christopher J.] Univ Calif Berkeley, Dept Mol & Cell Biol, Berkeley, CA 94720 USA. [Chang, Christopher J.] Univ Calif Berkeley, Howard Hughes Med Inst, Berkeley, CA 94720 USA. [Atanasov, Mihail; Bill, Eckhard; Neese, Frank] Max Planck Inst Chem Energiekonvers, D-45470 Mulheim, Germany. [Atanasov, Mihail] Bulgarian Acad Sci, Inst Gen & Inorgan Chem, BU-1113 Sofia, Bulgaria. RP Atanasov, M (reprint author), Max Planck Inst Chem Energiekonvers, D-45470 Mulheim, Germany. EM mihail.atanasov@cec.mpg.de; frank.neese@cec.mpg.de; jrlong@berkeley.edu; chrischang@berkeley.edu RI Nippe, Michael/A-6222-2015; Neese, Frank/J-4959-2014 OI Nippe, Michael/0000-0003-1091-4677; Neese, Frank/0000-0003-4691-0547 FU DOE/LBNL [403801]; NSF [CHE-1111900] FX The synthesis, characterization, and reactivity studies described were supported by DOE/LBNL Grant 403801 (to C.J.C.). The contributions of J.R.L. were supported by NSF Grant CHE-1111900. C.J.C. is an Investigator with the Howard Hughes Medical Institute. The authors thank Prof. Karl Wieghardt and Dr. Thomas Weihermuller (Max-Planck Institute fur Chemische Energiekonversion, Mulheim an der Ruhr, Germany) for helpful discussions. NR 83 TC 11 Z9 11 U1 4 U2 46 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0020-1669 EI 1520-510X J9 INORG CHEM JI Inorg. Chem. PD NOV 3 PY 2014 VL 53 IS 21 BP 11388 EP 11395 DI 10.1021/ic5010177 PG 8 WC Chemistry, Inorganic & Nuclear SC Chemistry GA AS5JM UT WOS:000344307400008 PM 25097094 ER PT J AU Pemmaraju, CD Copping, R Wang, S Janousch, M Teat, SJ Tyliszcak, T Canning, A Shuh, DK Prendergast, D AF Pemmaraju, C. D. Copping, Roy Wang, Shuao Janousch, Markus Teat, Simon. J. Tyliszcak, Tolek Canning, Andrew Shuh, David K. Prendergast, David TI Bonding and Charge Transfer in Nitrogen-Donor Uranyl Complexes: Insights from NEXAFS Spectra SO INORGANIC CHEMISTRY LA English DT Article ID X-RAY-ABSORPTION; TRIPLE-HELICAL COMPLEXES; TRIDENTATE AROMATIC LIGANDS; ELECTRONIC-STRUCTURE; ACTINYL IONS; LANTHANIDES; SPECTROSCOPY; COVALENCY; ACTINIDES; SYSTEMS AB We investigate the electronic structure of three newly synthesized nitrogen-donor uranyl complexes [(UO2)(H(2)bbp)Cl-2], [(UO)(2)(Hbbp)(Py)Cl], and [(UO2)(bbp)(Py)(2)] using a combination of near-edge X-ray absorption fine structure (NEXAFS) spectroscopy experiments and simulations. The complexes studied feature derivatives of the tunable tridentate N-donor ligand 2,6-bis(2-benzimidazyl)pyridine (bbp) and exhibit discrete chemical differences in uranyl coordination. The sensitivity of the N K-edge X-ray absorption spectrum to local bonding and charge transfer is exploited to systematically investigate the evolution of structural as well as electronic properties across the three complexes. A thorough interpretation of the measured experimental spectra is achieved via ab initio NEXAFS simulations based on the eXcited electron and Core-Hole (XCH) approach and enables the assignment of spectral features to electronic transitions on specific absorbing sites. We find that ligand-uranyl bonding leads to a signature blue shift in the N K-edge absorption onset, resulting from charge displacement toward the uranyl, while changes in the equatorial coordination shell of the uranyl lead to more subtle modulations in the spectral features. Theoretical simulations show that the flexible local chemistry at the nonbinding imidazole-N sites of the bbp ligand is also reflected in the NEXAFS spectra and highlights potential synthesis strategies to improve selectivity. In particular, we find that interactions of the bbp ligand with solvent molecules can lead to changes in ligand-uranyl binding geometry while also modulating the K-edge absorption. Our results suggest that NEXAFS spectroscopy combined with first-principles interpretation can offer insights into the coordination chemistry of analogous functionalized conjugated ligands. C1 [Pemmaraju, C. D.; Prendergast, David] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Mol Foundry, Berkeley, CA 94720 USA. [Pemmaraju, C. D.; Copping, Roy; Wang, Shuao; Janousch, Markus; Shuh, David K.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Chem Sci, Glenn T Seaborg Ctr, Berkeley, CA 94720 USA. [Canning, Andrew] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Computat Res Div, Berkeley, CA 94720 USA. [Teat, Simon. J.; Tyliszcak, Tolek] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94720 USA. [Canning, Andrew] Univ Calif Davis, Dept Chem Engn & Mat Sci, Davis, CA 95616 USA. [Janousch, Markus] Paul Scherrer Inst, Lab Synchrotron Radiat, CH-5232 Villigen, Switzerland. RP Pemmaraju, CD (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Mol Foundry, Berkeley, CA 94720 USA. EM scpemmaraju@lbl.gov RI Janousch, Markus/B-3285-2010; PEMMARAJU, DAS/O-8153-2014; Foundry, Molecular/G-9968-2014 OI PEMMARAJU, DAS/0000-0002-9016-7044; FU Laboratory Directed Research and Development Program at LBNL; Office of Science of the U.S. Department of Energy [DE-AC02-05CH11231]; U.S. Department of Energy at LBNL [DE-AC02-05CH11231] FX Theoretical and computational work by C.D.P. and D.P. was supported by the Laboratory Directed Research and Development Program of Lawrence Berkeley National Laboratory (LBNL) and as a User Project at the Molecular Foundry, LBNL. D.K.S, R.C., and S.W. were also supported by the Laboratory Directed Research and Development Program at LBNL. Calculations were performed on Hopper, at the National Energy Research Scientific Computing Center, LBNL and Molecular Foundry computing resources, Nano and Vulcan, managed by the High Performance Computing Services Group, LBNL. All LBNL work is supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. The Advanced Light Source is supported by the Director, Office of Science, Office of Basic Energy Sciences; and the MES Beamline by the aforementioned office, Division of Chemical Sciences, Geosciences, and Biosciences; both of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231 at LBNL. NR 57 TC 1 Z9 1 U1 7 U2 39 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0020-1669 EI 1520-510X J9 INORG CHEM JI Inorg. Chem. PD NOV 3 PY 2014 VL 53 IS 21 BP 11415 EP 11425 DI 10.1021/ic501107a PG 11 WC Chemistry, Inorganic & Nuclear SC Chemistry GA AS5JM UT WOS:000344307400011 PM 25330350 ER PT J AU Overgaard, J Walsh, JPS Hathwar, VR Lorgensen, MRV Hoffinan, C Platts, JA Piltz, R Winpenny, REP AF Overgaard, Jacob Walsh, James P. S. Hathwar, Venkatesha R. Lorgensen, Mads R. V. Hoffinan, Christina Platts, Jamie A. Piltz, Ross Winpenny, Richard E. P. TI Relationships between Electron Density and Magnetic Properties in Water-Bridged Dimetal Complexes SO INORGANIC CHEMISTRY LA English DT Article ID POLARIZED NEUTRON-DIFFRACTION; EXPERIMENTAL CHARGE-DENSITY; X-RAY; PHOTOSYSTEM-II; CARBOXYLATE COMPLEXES; SUBATOMIC RESOLUTION; METAL-COMPLEXES; ACTIVE-SITES; SPIN-DENSITY; MODEL AB The electron densities in two analogous dimetallic transition metal compounds, namely, [M-2(mu-OH2)-(BuCOO)(4)((BuCOOH)-Bu-t)(2)(C5H5N)(2)] (M = Co((1)), Ni(2)), were determined from combined X-ray and neutron single-crystal diffraction at 100 K. Excellent correspondence between the thermal parameters from X- and N-derived atomic displacement parameters is found, indicating high-quality X-ray data and a successful separation of thermal and electronic effects. Topological analysis of electron densities derived from high-resolution X-ray diffraction, as well as density functional theory calculations, shows no direct metal-metal bonding in either compound, while the total energy density at the bond critical points suggests stronger metal-oxygen interactions for the Ni system, in correspondence with its shorter bond distances. The analysis also allows for estimation of the relative strength of binding of terminal and bridging ligands to the metals, showing that the bridging water molecule is more strongly bound than terminal carboxylic acid, but less so than bridging carboxylates. Recently, modeling of magnetic and spectroscopic data in both of these systems has shown weak ferromagnetic interactions between the metal atoms. Factors related to large zero-field splitting effects complicate the magnetic analysis in both compounds, albeit to a much greater degree in 1. The current results support the conclusion drawn from previous magnetic and spectroscopic measurements that there is no appreciable direct communication between metal centers. C1 [Overgaard, Jacob; Hathwar, Venkatesha R.; Lorgensen, Mads R. V.] Aarhus Univ, Dept Chem, Ctr Mat Crystallog, DK-8000 Aarhus C, Denmark. [Lorgensen, Mads R. V.; Hoffinan, Christina] Oak Ridge Natl Lab, Chem & Engn Mat Div, Oak Ridge, TN 37831 USA. [Platts, Jamie A.] Cardiff Univ, Sch Chem, Cardiff CF10 3AT, S Glam, Wales. [Piltz, Ross] ANSTO, Bragg Inst, Kirrawee Dc, NSW 2232, Australia. [Walsh, James P. S.; Winpenny, Richard E. P.] Univ Manchester, Sch Chem, Manchester M13 9PL, Lancs, England. [Walsh, James P. S.; Winpenny, Richard E. P.] Univ Manchester, Photon Sci Inst, Manchester M13 9PL, Lancs, England. RP Overgaard, J (reprint author), Aarhus Univ, Dept Chem, Ctr Mat Crystallog, DK-8000 Aarhus C, Denmark. EM jacobo@chem.au.dk RI Jorgensen, Mads Ry Vogel/C-6109-2017; Walsh, James Paul Slater/M-6527-2014; Platts, Jamie/A-2310-2011; OI Jorgensen, Mads Ry Vogel/0000-0001-5507-9615; Walsh, James Paul Slater/0000-0003-3454-3428; Platts, Jamie/0000-0002-1008-6595; Overgaard, Jacob/0000-0001-6492-7962 FU Scientific User Facilities Division, Office of Basic Energy Sciences, US Department of Energy; North West Nanoscience DTC; Danish National Research Foundation [DNRF93]; Danish Council for Nature and Universe (DanScatt) FX We acknowledge the support of the Bragg Institute, Australian Nuclear Science and Technology Organisation, in accepting proposal 2749 for beam time on KOALA. Research conducted at ORNL's Spallation Neutron Source was sponsored by the Scientific User Facilities Division, Office of Basic Energy Sciences, US Department of Energy. J.P.S.W. acknowledges the North West Nanoscience DTC for a Ph.D. studentship. This work was supported by the Danish National Research Foundation (DNRF93) and the Danish Council for Nature and Universe (DanScatt). NR 68 TC 1 Z9 1 U1 1 U2 21 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0020-1669 EI 1520-510X J9 INORG CHEM JI Inorg. Chem. PD NOV 3 PY 2014 VL 53 IS 21 BP 11531 EP 11539 DI 10.1021/ic501411w PG 9 WC Chemistry, Inorganic & Nuclear SC Chemistry GA AS5JM UT WOS:000344307400022 PM 25330274 ER PT J AU Hunter, SC Smith, BA Hoffmann, CM Wang, XP Chen, YS McIntyre, GJ Xue, ZL AF Hunter, Seth C. Smith, Brenda A. Hoffmann, Christina M. Wang, Xiaoping Chen, Yu-Sheng McIntyre, Garry J. Xue, Zi-Ling TI Intermolecular Interactions in Solid-State Metalloporphyrins and Their Impacts on Crystal and Molecular Structures SO INORGANIC CHEMISTRY LA English DT Article ID SOLUBLE GUANYLATE-CYCLASE; FERROUS HEME-NITROSYLS; NITRIC-OXIDE; ELECTRONIC-STRUCTURE; PLATELET-AGGREGATION; MAGNETIC-RESONANCE; BIOLOGICAL-SYSTEMS; STEREOCHEMISTRY; PORPHYRINS; SPECTROSCOPY AB A variable-temperature (VT) crystal structure study of [Fe(TPP)Cl] (TPP2- = meso-tetraphenylporphyrinate) and Hirshfeld surface analyses of its structures and previously reported structures of [M(TPP)(NO)] (M = Fe, Co) reveal that intermolecular interactions are a significant factor in structure disorder in the three metalloporphyrins and phase changes in the nitrosyl complexes. These interactions cause, for example, an 8-fold disorder in the crystal structures of [M(TPP)(NO)] at room temperature that obscures the M-NO binding. Hirshfeld analyses of the structure of [Co(TPP)(NO)] indicate that the phase change from I4/m to P1(_) leads to an increase in void-volume percentage, permitting additional structural compression through tilting of the phenyl rings to offset the close-packing interactions at the interlayer positions in the crystal structures with temperature decrease. X-ray and neutron structure studies of [Fe(TPP)Cl] at 293, 143, and 20 K reveal a tilting of the phenyl groups away from being perpendicular to the porphyrin ring as a result of intermolecular interactions. Structural similarities and differences among the three complexes are identified and described by Hirshfeld surface and void-volume calculations. C1 [Hunter, Seth C.; Smith, Brenda A.; Xue, Zi-Ling] Univ Tennessee, Dept Chem, Knoxville, TN 37996 USA. [Hoffmann, Christina M.; Wang, Xiaoping] Oak Ridge Natl Lab, Chem & Engn Mat Div, Oak Ridge, TN 37830 USA. [Chen, Yu-Sheng] Univ Chicago, Ctr Adv Radiat Sources, ChemMatCARS, Argonne, IL 60439 USA. [McIntyre, Garry J.] Inst Max Von Laue Paul Langevin, F-38042 Grenoble 9, France. RP Hoffmann, CM (reprint author), Oak Ridge Natl Lab, Chem & Engn Mat Div, Oak Ridge, TN 37830 USA. EM choffmann@ornl.gov; wangx@ornl.gov; xue@utk.edu RI Wang, Xiaoping/E-8050-2012; hoffmann, christina/D-2292-2016 OI Wang, Xiaoping/0000-0001-7143-8112; hoffmann, christina/0000-0002-7222-5845 FU Joint Institute for Neutron Sciences (JINS) fellowship program; U.S. National Science Foundation [CHE-0516928, CHE-1012173, CHE-1362548]; American Chemical Society Petroleum Research Fund; National Science Foundation/Department of Energy [CHE-1346572]; The University of Chicago at Argonne, LLC [DE-AC02-06CH11357]; U.S. Department of Energy [DE-AC05-000R22725] FX We thank the Joint Institute for Neutron Sciences (JINS) fellowship program (S.C.H. and BA.S.) and the U.S. National Science Foundation (CHE-0516928, CHE-1012173, and CHE-1362548 to Z.X.) for funding, ANL's Advanced Photon Source on beamline 15ID-C for X-ray data at 20 K, and the Institut Laue-Langevin for the allocation of neutron beam time on D9. Acknowledgment is also made to the donors of the American Chemical Society Petroleum Research Fund for partial support of this research. Beamline 15ID-C is principally supported by the National Science Foundation/Department of Energy under Grant CHE-1346572. ANL is a U.S. Department of Energy laboratory operated by The University of Chicago at Argonne, LLC, under Contract DE-AC02-06CH11357. ORNL/SNS is managed by UT-Battelle, LLC, for the U.S. Department of Energy under contract DE-AC05-000R22725. NR 62 TC 4 Z9 4 U1 3 U2 30 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0020-1669 EI 1520-510X J9 INORG CHEM JI Inorg. Chem. PD NOV 3 PY 2014 VL 53 IS 21 BP 11552 EP 11562 DI 10.1021/ic5015835 PG 11 WC Chemistry, Inorganic & Nuclear SC Chemistry GA AS5JM UT WOS:000344307400024 PM 25338536 ER PT J AU Xu, JG Kuang, XJ Veron, E Allix, M Suchomel, MR Porcher, F Liang, CL Pan, FJ Wu, MM AF Xu, Jungu Kuang, Xiaojun Veron, Emmanuel Allix, Mathieu Suchomel, Matthew R. Porcher, Florence Liang, Chaolun Pan, Fengjuan Wu, Mingmei TI Localization of Oxygen Interstitials in CeSrGa3O7+delta Melilite SO INORGANIC CHEMISTRY LA English DT Article ID OXIDE-ION CONDUCTIVITY; MAGNESIUM-DOPED LAGAO3; CRYSTAL-STRUCTURE; MIXED CONDUCTIVITY; ELECTROLYTES; STRONTIUM; TEMPERATURES; DIFFRACTION; CERAMICS; XPS AB The solubility of Ce in the La1-xCexSrGa3O7+delta and La1.54-xCexSr0.46Ga3O7.27+delta melilites was investigated, along with the thermal redox stability in air of these melilites and the conductivity variation associated with oxidization of Ce3+ into Ce4+. Under CO reducing atmosphere, the La in LaSrGa3O7 may be completely substituted by Ce to form the La1-xCexSrGa3O7+delta solid solution, which is stable in air to similar to 600 degrees C when x = 0.6. On the other side, the La1.54-xCexSr0.46Ga3O7.27+delta compositions displayed much lower Ce solubility (x = 0.1), irrespective of the synthesis atmosphere. In the as-made La1-xCexSrGa3O7+delta, the conductivity increased with the cerium content, due to the enhanced electronic conduction arising from the 4f electrons in Ce3+ cations. At 600 degrees C, CeSrGa3O7+delta showed a conductivity of similar to 10(-4) S/cm in air, nearly 4 orders of magnitude higher than that of LaSrGa3O7. The oxidation of Ce3+ into Ce4+ in CeSrGa3O7+delta slightly reduced the conductivity, and the oxygen excess did not result in apparent increase of oxide ion conduction in CeSrGa3O7+delta. The Ce doping in air also reduced the interstitial oxide ion conductivity of La1.54Sr0.46Ga3O7.27. Neutron powder diffraction study on CeSrGa3O7.39 composition revealed that the extra oxygen is incorporated in the four-linked GaO4 polyhedral environment, leading to distorted GaO5 trigonal bipyramid. The stabilization and low mobility of interstitial oxygen atoms in CeSrGa3O7+d, in contrast with those in La1+xSr1-xGa3O7+0.5x, may be correlated with the cationic size contraction from the oxidation of Ce3+ to Ce4+. These results provide a new comprehensive understanding of the accommodation and conduction mechanism of the oxygen interstitials in the melilite structure. C1 [Xu, Jungu; Kuang, Xiaojun; Pan, Fengjuan; Wu, Mingmei] Sun Yat Sen Univ, Sch Chem & Chem Engn, State Key Lab Optoelect Mat & Technol, MOE Key Lab Bioinorgan & Synthet Chem, Guangzhou 510275, Guangdong, Peoples R China. [Xu, Jungu; Kuang, Xiaojun] Guilin Univ Technol, State Key Lab Proc Nonferrous Met & Featured Mat, MOE Key Lab New Proc Technol Nonferrous Met & Mat, Guangxi Minist Prov Jointly Constructed Cultivat, Guilin 541004, Peoples R China. [Veron, Emmanuel; Allix, Mathieu] CEMHTI, UPR3079, F-45071 Orleans 2, France. [Veron, Emmanuel; Allix, Mathieu] Univ Orleans, Fac Sci, F-45067 Orleans 2, France. [Suchomel, Matthew R.] Argonne Natl Lab, Adv Photon Source, Lemont, IL 60439 USA. [Porcher, Florence] CEA Saclay, Lab Leon Brillouin, F-91191 Gif Sur Yvette, France. [Liang, Chaolun] Sun Yat Sen Univ, Instrumental Anal & Res Ctr, Guangzhou 510275, Guangdong, Peoples R China. RP Kuang, XJ (reprint author), Sun Yat Sen Univ, Sch Chem & Chem Engn, State Key Lab Optoelect Mat & Technol, MOE Key Lab Bioinorgan & Synthet Chem, Guangzhou 510275, Guangdong, Peoples R China. EM kuangxj@glut.edu.cn; ceswmm@mail.sysu.edu.cn RI Suchomel, Matthew/C-5491-2015; VERON, Emmanuel/C-1825-2008; Allix, Mathieu/C-1679-2008; Kuang, Xiaojun/K-4129-2013; OI Allix, Mathieu/0000-0001-9317-1316; SUCHOMEL, Matthew/0000-0002-9500-5079 FU National Science Foundation of China [21101174]; Chinese Ministry of Education, Program for New Century Excellent Talents in University [213030A, NCET-13-0752]; Guangdong Province Research Project for industrial applications [2012B09000026, 2011A090200083]; U.S. Department of Energy [DE-AC02-06CH11357]; Guilin University of Technology; Chinese Ministry of Education Scientific Research Foundation FX This work is funded by National Science Foundation of China (No. 21101174), the Research Project (No. 213030A) of Chinese Ministry of Education, Program for New Century Excellent Talents in University (No. NCET-13-0752), and the Guangdong Province Research Project for industrial applications (Nos. 2012B09000026 and 2011A090200083). Use of the Advanced Photon Source (beamline 11-BM) at Argonne National Laboratory was supported by the U.S. Department of Energy under Contract No. DE-AC02-06CH11357. The authors acknowledge the support of the Laboratoire Leon Brillouin at CEA/Saclay (beamline 3T2) for the neutron beamtirne. X.K. also thanks Guilin University of Technology and Chinese Ministry of Education Scientific Research Foundation for Returned Scholars for the Start-up Funds. We thank Prof. C.-Y. Su for access to TGA instrument and Ms. H.J. Yu for helping with the TGA measurement. NR 39 TC 3 Z9 3 U1 4 U2 49 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 0020-1669 EI 1520-510X J9 INORG CHEM JI Inorg. Chem. PD NOV 3 PY 2014 VL 53 IS 21 BP 11589 EP 11597 DI 10.1021/ic501662p PG 9 WC Chemistry, Inorganic & Nuclear SC Chemistry GA AS5JM UT WOS:000344307400028 PM 25303629 ER PT J AU Guggenmos, A Radunz, S Rauhut, R Hofstetter, M Venkatesan, S Wochnik, A Gullikson, EM Fischer, S Nickel, B Scheu, C Kleineberg, U AF Guggenmos, Alexander Raduenz, Stefan Rauhut, Roman Hofstetter, Michael Venkatesan, Sriram Wochnik, Angela Gullikson, Eric M. Fischer, Stefan Nickel, Bert Scheu, Christina Kleineberg, Ulf TI Ion polished Cr/Sc attosecond multilayer mirrors for high water window reflectivity SO OPTICS EXPRESS LA English DT Article ID SOFT-X-RAY; PULSES; MICROSCOPY; STABILITY; NM AB Recent advances in the development of attosecond soft X-ray sources ranging into the water window spectral range, between the 1s states of carbon and oxygen (284 eV-543 eV), are also driving the development of suited broadband multilayer optics for steering and shaping attosecond pulses. The relatively low intensity of current High Harmonic Generation (HHG) soft X-ray sources calls for an efficient use of photons, thus the development of low-loss multilayer optics is of uttermost importance. Here, we report about the realization of broadband Cr/Sc attosecond multilayer mirrors with nearly atomically smooth interfaces by an optimized ion beam deposition and assisted interface polishing process. This yields to our knowledge highest multilayer mirror reflectivity at 300 eV near normal incidence. The results are verified by transmission electron microscopy (TEM) and soft/hard X-ray reflectometry. (C) 2014 Optical Society of America C1 [Guggenmos, Alexander; Raduenz, Stefan; Rauhut, Roman; Hofstetter, Michael; Fischer, Stefan; Nickel, Bert; Kleineberg, Ulf] Univ Munich, Fak Phys, D-85748 Garching, Germany. [Guggenmos, Alexander; Raduenz, Stefan; Rauhut, Roman; Hofstetter, Michael; Kleineberg, Ulf] Max Planck Inst Quantum Opt, D-85748 Garching, Germany. [Venkatesan, Sriram; Wochnik, Angela; Scheu, Christina] Univ Munich, Dept Chem, D-81377 Munich, Germany. [Gullikson, Eric M.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Ctr Xray Opt, Berkeley, CA 94720 USA. [Fischer, Stefan; Nickel, Bert] Univ Munich, Ctr NanoSci, D-80799 Munich, Germany. RP Guggenmos, A (reprint author), Univ Munich, Fak Phys, Coulombwall 1, D-85748 Garching, Germany. EM alexander.guggenmos@physik.uni-muenchen.de RI Venkatesan, Sriram/B-1899-2009; Nickel, Bert/A-2095-2009 OI Venkatesan, Sriram/0000-0003-2389-2761; Nickel, Bert/0000-0002-0254-8841 FU DFG via the Excellence Cluster Munich-Centre for Advanced Photonics (MAP) [EXC 158] FX We thankfully acknowledge scientific support and valuable discussions by Ferenc Krausz (MPQ, LMU) and Philip Bohm (LMU) for supporting the hard X-ray measurements. This work was financially supported by the DFG via the Excellence Cluster Munich-Centre for Advanced Photonics (MAP, EXC 158). NR 42 TC 4 Z9 4 U1 0 U2 10 PU OPTICAL SOC AMER PI WASHINGTON PA 2010 MASSACHUSETTS AVE NW, WASHINGTON, DC 20036 USA SN 1094-4087 J9 OPT EXPRESS JI Opt. Express PD NOV 3 PY 2014 VL 22 IS 22 BP 26526 EP 26536 DI 10.1364/OE.22.026526 PG 11 WC Optics SC Optics GA AS0ZI UT WOS:000344004900009 PM 25401804 ER PT J AU Souhan, B Grote, RR Chen, CP Huang, HC Driscoll, JB Lu, M Stein, A Bakhru, H Bergman, K Green, WMJ Osgood, RM AF Souhan, Brian Grote, Richard R. Chen, Christine P. Huang, Hsu-Cheng Driscoll, Jeffrey B. Lu, Ming Stein, Aaron Bakhru, Hassaram Bergman, Keren Green, William M. J. Osgood, Richard M., Jr. TI Si+-implanted Si-wire waveguide photodetectors for the mid-infrared SO OPTICS EXPRESS LA English DT Article ID ERROR-FREE OPERATION; ALL-SILICON; INFRARED PHOTODIODES; IRRADIATED SILICON; C-BAND; MU-M; SENSITIVITY; MODULATION; DETECTORS; GERMANIUM AB CMOS-compatible Si+-implanted Si-waveguide p-i-n photodetectors operating at room temperature and at mid-infrared wavelengths from 2.2 to 2.3 mu m are demonstrated. Responsivities of 9.9 +/- 2.0 mA/W are measured at a 5 V reverse bias with an estimated internal quantum efficiency of 2.7 - 4.5%. The dark current is found to vary from a few microamps down to less than a nanoamp after a post-implantation annealing of 350 degrees C. The measured photocurrent dependence on input power shows a linear correspondence over more than three decades, and the frequency response of a 250 mu m-length p-i-n device is measured to be similar to 1.7 GHz for a wavelength of lambda = 2.2 mu m, thus potentially opening up new communication bands for photonic integrated circuits. (C) 2014 Optical Society of America C1 [Souhan, Brian; Grote, Richard R.; Huang, Hsu-Cheng; Driscoll, Jeffrey B.; Osgood, Richard M., Jr.] Columbia Univ, Microelect Sci Labs, New York, NY 10027 USA. [Chen, Christine P.; Bergman, Keren] Columbia Univ, Dept Elect Engn, New York, NY 10027 USA. [Lu, Ming; Stein, Aaron] Brookhaven Natl Lab, Ctr Funct Nanomat, Upton, NY 11973 USA. [Bakhru, Hassaram] SUNY Albany, Coll Nanoscale Sci & Engn, Albany, NY 12222 USA. [Green, William M. J.] IBM Corp, TJ Watson Res Ctr, Yorktown Hts, NY 10598 USA. RP Souhan, B (reprint author), Columbia Univ, Microelect Sci Labs, 500 W 120th St, New York, NY 10027 USA. EM brian.souhan@gmail.com FU Center for Functional Nanomaterials, Brookhaven National Laboratory; U. S. Department of Energy, Office of Basic Energy Sciences [DE-AC02-98CH10886]; Semiconductor Research Corporation Master's Scholarship; Columbia Optics and Quantum Electronics IGERT under NSF [DGE-1069420] FX Research carried out in part at the Center for Functional Nanomaterials, Brookhaven National Laboratory, which is supported by the U. S. Department of Energy, Office of Basic Energy Sciences, under Contract No. DE-AC02-98CH10886. The authors also acknowledge support from the Semiconductor Research Corporation Master's Scholarship and the Columbia Optics and Quantum Electronics IGERT under NSF grant DGE-1069420. The authors would also like to acknowledge Michael W. Geis and Steven J. Spector for device fabrication and design. NR 28 TC 5 Z9 5 U1 5 U2 24 PU OPTICAL SOC AMER PI WASHINGTON PA 2010 MASSACHUSETTS AVE NW, WASHINGTON, DC 20036 USA SN 1094-4087 J9 OPT EXPRESS JI Opt. Express PD NOV 3 PY 2014 VL 22 IS 22 BP 27415 EP 27424 DI 10.1364/OE.22.027415 PG 10 WC Optics SC Optics GA AS0ZI UT WOS:000344004900094 PM 25401890 ER PT J AU Frey, SE Destaillats, H Cohn, S Ahrentzen, S Fraser, MP AF Frey, Sarah E. Destaillats, Hugo Cohn, Sebastian Ahrentzen, Sherry Fraser, Matthew P. TI Characterization of indoor air quality and resident health in an Arizona senior housing apartment building SO JOURNAL OF THE AIR & WASTE MANAGEMENT ASSOCIATION LA English DT Article ID SECONDARY POLLUTANTS; VENTILATION FILTERS; PARTICULATE MATTER; FINE PARTICLES; UNITED-STATES; FORMALDEHYDE; EMISSIONS; POLLUTION; ASTHMA; OZONE AB A survey of key indoor air quality (IAQ) parameters and resident health was carried out in 72 apartments within a single low-income senior housing building in Phoenix, Arizona. Air sampling was carried out simultaneously with a questionnaire on personal habits and general health of residents. Mean PM10 concentrations are 66 +/- 16, 58 +/- 13, and 24 +/- 3 mu g/m(3) and mean PM2.5 concentrations are 62 +/- 16, 53 +/- 13, and 20 +/- 2 mu g/m(3) for the living room, kitchen, and outdoor balcony, respectively. Median PM10 concentrations are 17, 18 and 17 mu g/m(3) and median PM2.5 concentrations are 13, 14, and 13 mu g/m(3), respectively. The initial results indicate that increased indoor particle concentrations coincide with residents who report smoking cigarettes. Indoor formaldehyde concentrations revealed median levels of 36.9, 38.8, and 4.3 ppb in the living room, kitchen, and balcony, respectively. Results show that 36% of living room samples and 44% of kitchen samples exceeded the Health Canada REL for chronic exposure to formaldehyde (40 ppb). Associations between occupants' behavior, self-reported health conditions, and IAQ are evaluated. [GRAPHICS] C1 [Frey, Sarah E.] Arizona State Univ, Dept Chem & Biochem, Tempe, AZ 85287 USA. [Destaillats, Hugo; Cohn, Sebastian] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Environm Energy Technol Div, Indoor Environm Grp, Berkeley, CA 94720 USA. [Ahrentzen, Sherry] Univ Florida, Rinker Sch Construct Management, Gainesville, FL USA. [Fraser, Matthew P.] Arizona State Univ, Sch Sustainable Engn & Built Environm, Tempe, AZ 85287 USA. RP Fraser, MP (reprint author), Arizona State Univ, Sch Sustainable Engn & Built Environm, POB 875306, Tempe, AZ 85287 USA. EM Matthew.Fraser@asu.edu FU U.S. Department of Housing and Urban Development FX Funding was provided by the U.S. Department of Housing and Urban Development. NR 34 TC 2 Z9 2 U1 2 U2 31 PU TAYLOR & FRANCIS INC PI PHILADELPHIA PA 530 WALNUT STREET, STE 850, PHILADELPHIA, PA 19106 USA SN 1096-2247 EI 2162-2906 J9 J AIR WASTE MANAGE JI J. Air Waste Manage. Assoc. PD NOV 2 PY 2014 VL 64 IS 11 BP 1251 EP 1259 DI 10.1080/10962247.2014.937513 PG 9 WC Engineering, Environmental; Environmental Sciences; Meteorology & Atmospheric Sciences SC Engineering; Environmental Sciences & Ecology; Meteorology & Atmospheric Sciences GA AR1BE UT WOS:000343313500005 PM 25509546 ER PT J AU Edwards, PG Gaines, KF Bryan, AL Novak, JM Blas, SA AF Edwards, Paul G. Gaines, Karen F. Bryan, A. Lawrence, Jr. Novak, James M. Blas, Susan A. TI Are U, Ni, and Hg an Environmental Risk within a RCRA/CERCLA Unit on the US Department of Energy's Savannah River Site? SO HUMAN AND ECOLOGICAL RISK ASSESSMENT LA English DT Article DE hazard quotient; mercury; nickel; RCRA; CERCLA; transfer factors; uranium ID RANA-PEREZI-SEOANE; WATER CHEMISTRY; METHYL MERCURY; URANIUM; METHYLMERCURY; EXPOSURE; WETLAND; POND; TRANSPORT; SEDIMENTS AB The U.S. Department of Energy's Savannah River Site (SRS) is a former nuclear weapon production facility. From 1954-1985, releases of Al, Cu, Cr, Hg, Ni, Pb, U, and Zn were discharged into the Tims Branch-Steed Pond water system. This study investigates whether metal concentrations in Tims Branch's sediment, biofilm, and other biota exceed screening level risk calculations to determine if remedial actions should be pursued for the Contaminants of Potential Concern (U, Ni, Hg). Transfer factors (TFs) were calculated to determine metal concentration changes throughout lower trophic levels and results were compared with sediment benchmarks to create hazard quotients (HQs) to assess risk and a scientific-management decision point. Most TFs for Ni and U from lower to higher trophic level biota were <1, suggesting no biomagnifications; however HQs > 1 and cumulative distributions showed the majority of the samples exceeded action levels. Elevated TFs and HQs > 1 in the upper trophic levels for Hg indicated a high degree of bioavailability and biomagnification. Monte Carlo resampling analyses supported these empirical results. This system should continue to be closely monitored to ensure that contamination does not move off the SRS. C1 [Edwards, Paul G.; Gaines, Karen F.; Novak, James M.] Eastern Illinois Univ, Dept Biol Sci, Charleston, IL 61920 USA. [Bryan, A. Lawrence, Jr.] Univ Georgia, Savannah River Ecol Lab, Aiken, SC USA. [Blas, Susan A.] Savannah River Nucl Solut, Savannah, SC USA. RP Gaines, KF (reprint author), Eastern Illinois Univ, Dept Biol Sci, Life Sci Bldg 2056, Charleston, IL 61920 USA. EM kfgaines@eiu.edu FU Area Completions Project (ACP) of SRNS through DOE [DE-FC09-07SR22506] FX This project was funded by the Area Completions Project (ACP) of SRNS through DOE Award Number DE-FC09-07SR22506 to the University of Georgia Research Foundation and was used in partial fulfillment of a Master's of Science degree in the Department of Biological Sciences at Eastern Illinois University. NR 66 TC 1 Z9 1 U1 2 U2 91 PU TAYLOR & FRANCIS INC PI PHILADELPHIA PA 530 WALNUT STREET, STE 850, PHILADELPHIA, PA 19106 USA SN 1080-7039 EI 1549-7860 J9 HUM ECOL RISK ASSESS JI Hum. Ecol. Risk Assess. PD NOV 2 PY 2014 VL 20 IS 6 BP 1565 EP 1589 DI 10.1080/10807039.2013.862107 PG 25 WC Biodiversity Conservation; Environmental Sciences SC Biodiversity & Conservation; Environmental Sciences & Ecology GA AE8QO UT WOS:000334266600010 ER PT J AU Campbell, MD Chiao, YA Gaffrey, MJ Djukovic, D Gu, H Szeto, HS Raftery, D Rabinovitch, P Qian, WJ Marcinek, DJ AF Campbell, Matthew David Chiao, Ying Ann Gaffrey, Matthew J. Djukovic, Danijel Gu, Haiwei Szeto, Hazel S. Raftery, Daniel Rabinovitch, Peter Qian, Wei-Jun Marcinek, David J. TI Targeting Mitochondrial Oxidative Stress to Improve Aged Skeletal Muscle Function SO FREE RADICAL BIOLOGY AND MEDICINE LA English DT Meeting Abstract C1 [Campbell, Matthew David; Chiao, Ying Ann; Djukovic, Danijel; Gu, Haiwei; Raftery, Daniel; Rabinovitch, Peter; Marcinek, David J.] Univ Washington, Seattle, WA 98195 USA. [Gaffrey, Matthew J.; Qian, Wei-Jun] Pacific NW Natl Lab, Richland, WA 99352 USA. [Szeto, Hazel S.] Weill Cornell Med Coll, New York, NY USA. NR 0 TC 0 Z9 0 U1 0 U2 2 PU ELSEVIER SCIENCE INC PI NEW YORK PA 360 PARK AVE SOUTH, NEW YORK, NY 10010-1710 USA SN 0891-5849 EI 1873-4596 J9 FREE RADICAL BIO MED JI Free Radic. Biol. Med. PD NOV PY 2014 VL 76 SU 1 MA 41 BP S29 EP S29 DI 10.1016/j.freeradbiomed.2014.10.436 PG 1 WC Biochemistry & Molecular Biology; Endocrinology & Metabolism SC Biochemistry & Molecular Biology; Endocrinology & Metabolism GA CO9WA UT WOS:000359525800061 ER PT J AU Duan, JC Kodali, VK Gaffrey, MJ Chu, RK Moore, RJ Smith, RD Thrall, BD Qian, WJ AF Duan, Jicheng Kodali, Vamsi K. Gaffrey, Matthew J. Chu, Rosalie K. Moore, Ronald J. Smith, Richard D. Thrall, Brian D. Qian, Weijun TI Quantitative Site-Specific Profiling of S-Glutathionylation in Macrophages in Response to Oxidative Stress Induced by Engineered Nanoparticles SO FREE RADICAL BIOLOGY AND MEDICINE LA English DT Meeting Abstract C1 [Duan, Jicheng; Kodali, Vamsi K.; Gaffrey, Matthew J.; Chu, Rosalie K.; Moore, Ronald J.; Smith, Richard D.; Thrall, Brian D.; Qian, Weijun] Pacific NW Natl Lab, Richland, WA 99352 USA. RI Smith, Richard/J-3664-2012; OI Smith, Richard/0000-0002-2381-2349; Kodali, Vamsi/0000-0001-6177-0568 NR 0 TC 0 Z9 0 U1 0 U2 2 PU ELSEVIER SCIENCE INC PI NEW YORK PA 360 PARK AVE SOUTH, NEW YORK, NY 10010-1710 USA SN 0891-5849 EI 1873-4596 J9 FREE RADICAL BIO MED JI Free Radic. Biol. Med. PD NOV PY 2014 VL 76 SU 1 MA 249 BP S106 EP S107 DI 10.1016/j.freeradbiomed.2014.10.263 PG 2 WC Biochemistry & Molecular Biology; Endocrinology & Metabolism SC Biochemistry & Molecular Biology; Endocrinology & Metabolism GA CO9WA UT WOS:000359525800269 ER PT J AU Yao, Y Graziano, D Riddle, M Cresko, J Masanet, E AF Yao, Yuan Graziano, Diane Riddle, Matthew Cresko, Joe Masanet, Eric TI Greener pathways for energy-intensive commodity chemicals: opportunities and challenges SO CURRENT OPINION IN CHEMICAL ENGINEERING LA English DT Article ID LIFE-CYCLE ASSESSMENT; OXIDATIVE DEHYDROGENATION; STRUCTURED PACKINGS; DIRECT CONVERSION; STEAM CRACKING; HOLLOW FIBERS; METHANE; CHEMISTRY; BIOREFINERY; SEPARATION AB The chemical industry is poised for significant growth and investment, which presents an opportunity for adoption of greener chemical technologies. This article reviews available and emerging technologies for reducing the fossil fuel demand associated with the ammonia, ethylene, methanol, propylene, and benzene, toluene, and xylenes (BTX) industries. These few energy-intensive commodity chemicals (EICCs) account for around half of the energy use and greenhouse gas (GHG) emissions of the global chemical industry. Available data are harmonized to characterize potential energy use and GHG emissions savings, while technical and economic barriers to adoption are discussed. This information sheds light on the status of future technological options for reducing the impacts of the chemicals industry, and provides quantitative data to industry analysts and policy makers seeking a greater understanding of such options for EICCs. C1 [Yao, Yuan; Masanet, Eric] Northwestern Univ, Dept Chem & Biol Engn, Evanston, IL 60201 USA. [Graziano, Diane] Argonne Natl Lab, Global Secur Sci Div, Argonne, IL 60439 USA. [Riddle, Matthew] Argonne Natl Lab, Div Energy Syst, Argonne, IL 60439 USA. [Cresko, Joe] US DOE, Adv Mfg Off, Washington, DC 20585 USA. [Masanet, Eric] Northwestern Univ, Dept Mech Engn, Evanston, IL 60201 USA. RP Masanet, E (reprint author), Northwestern Univ, Dept Chem & Biol Engn, 2145 Sheridan Rd, Evanston, IL 60201 USA. EM eric.masanet@northwestern.edu RI Yao, Yuan/A-9150-2017 OI Yao, Yuan/0000-0001-9359-2030 FU DOE [DE-AC02-06CH11357] FX This work was supported by DOE under contract number DE-AC02-06CH11357. The data and views expressed in this paper are those of the authors and are not endorsed by the U.S. Department of Energy or the United States government. NR 79 TC 3 Z9 3 U1 4 U2 20 PU ELSEVIER SCI LTD PI OXFORD PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, OXON, ENGLAND SN 2211-3398 J9 CURR OPIN CHEM ENG JI Curr. Opin. Chem. Eng. PD NOV PY 2014 VL 6 BP 90 EP 98 DI 10.1016/j.coche.2014.10.005 PG 9 WC Biotechnology & Applied Microbiology; Engineering, Chemical SC Biotechnology & Applied Microbiology; Engineering GA CM4QS UT WOS:000357670400014 ER PT J AU Gilioli, E Ehm, L AF Gilioli, Edmondo Ehm, Lars TI High pressure and multiferroics materials: a happy marriage SO IUCRJ LA English DT Article DE high pressure; multiferroics; materials science ID THIN-FILMS; METASTABLE BIMNO3; PHASE-TRANSITIONS; CRYSTAL-STRUCTURE; TEMPERATURE POLYMORPHISM; STRUCTURAL-PROPERTIES; DIELECTRIC-PROPERTIES; PEROVSKITE; BIFEO3; FERROELECTRICITY AB The community of material scientists is strongly committed to the research area of multiferroic materials, both for the understanding of the complex mechanisms supporting the multiferroism and for the fabrication of new compounds, potentially suitable for technological applications. The use of high pressure is a powerful tool in synthesizing new multiferroic, in particular magneto-electric phases, where the pressure stabilization of otherwise unstable perovskite-based structural distortions may lead to promising novel metastable compounds. The in situ investigation of the high-pressure behavior of multiferroic materials has provided insight into the complex interplay between magnetic and electronic properties and the coupling to structural instabilities. C1 [Gilioli, Edmondo] IMEM CNR, I-43124 Parma, Italy. [Ehm, Lars] SUNY Stony Brook, Inst Mineral Phys, Stony Brook, NY 11794 USA. [Ehm, Lars] Brookhaven Natl Lab, Photon Sci Directorate, Upton, NY 11973 USA. RP Gilioli, E (reprint author), IMEM CNR, Area Sci 37-A, I-43124 Parma, Italy. EM edi@imem.cnr.it; lars.ehm@stonybrook.edu OI GILIOLI, Edmondo/0000-0001-6973-2179 FU National Science Foundation [GEO-11-07155] FX EG thanks Francesco Mezzadri, Gianluca Calestani and Davide Delmonte for material synthesis and fruitful discussions. LE acknowledges the support by the National Science Foundation through grant GEO-11-07155. Melissa Sims is acknowledged for her help with editing of the article and the references. We would like to thank the anonymous reviewer for the comments that helped to improve the manuscript. NR 161 TC 12 Z9 12 U1 12 U2 45 PU INT UNION CRYSTALLOGRAPHY PI CHESTER PA 2 ABBEY SQ, CHESTER, CH1 2HU, ENGLAND SN 2052-2525 J9 IUCRJ JI IUCrJ PD NOV PY 2014 VL 1 BP 590 EP 603 DI 10.1107/S2052252514020569 PN 6 PG 14 WC Chemistry, Multidisciplinary; Crystallography; Materials Science, Multidisciplinary SC Chemistry; Crystallography; Materials Science GA CL3QO UT WOS:000356865600022 PM 25485138 ER PT J AU Jones, CG Cappillino, PJ Stavila, V Robinson, DB AF Jones, Christopher G. Cappillino, Patrick J. Stavila, Vitalie Robinson, David B. TI Control of both particle and pore size in nanoporous palladium alloy powders SO POWDER TECHNOLOGY LA English DT Article DE Mesoporous; Monodisperse; Uniform; Hydride; Microspheres; Copper ID LIQUID-CRYSTALLINE PHASES; THERMAL-STABILITY; HYDROGEN; FILMS; ARCHITECTURES; ELECTRODES; DEPOSITION; NANOWIRES; BATTERIES; TRANSPORT AB Energy storage materials often involve chemical reactions with bulk solids. Porosity within the solids can enhance reaction rates. The porosity can be either within or between individual particles of the material. Greater control of the size and uniformity of both types of pore should lead to enhancements of charging and discharging rates in energy storage systems. To control both particle and pore size in nanoporous palladium (Pd)-based hydrogen storage materials, we have first created uniformly sized copper particles of about 1 mu m diameter by the reduction of copper sulfate with ascorbic acid. In turn, these were used as reducing agents for tetrachloropalladate in the presence of a block copolymer surfactant. The copper reductant particles are geometrically self-limiting, so the resulting Pd particles are of similar size. The surfactant induces formation of 10 nm-scale pores within the particles. Some residual copper is alloyed with the Pd, reducing hydrogen storage capacity; use of a more reactive Pd salt can mitigate this. The reaction is conveniently performed in gram-scale batches. (C) 2014 Elsevier B.V. All rights reserved. C1 [Jones, Christopher G.; Cappillino, Patrick J.; Robinson, David B.] Sandia Natl Labs, Energy Nanomat Dept, Livermore, CA 94551 USA. RP Robinson, DB (reprint author), Sandia Natl Labs, Energy Nanomat Dept, POB 969 MS 9291, Livermore, CA 94551 USA. EM drobins@sandia.gov FU Lockheed Martin Corporation; U.S. Department of Energy's National Nuclear Security Administration [DE-AC04-94AL85000] FX The authors thank Jeffrey Chames and Charles Steinhaus for assistance with SEM. Sandia National Laboratories is a multi-program laboratory managed and operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the U.S. Department of Energy's National Nuclear Security Administration under contract DE-AC04-94AL85000. NR 30 TC 1 Z9 1 U1 4 U2 10 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0032-5910 EI 1873-328X J9 POWDER TECHNOL JI Powder Technol. PD NOV PY 2014 VL 267 BP 95 EP 102 DI 10.1016/j.powtec.2014.07.008 PG 8 WC Engineering, Chemical SC Engineering GA CG3MS UT WOS:000353184900012 ER PT J AU Ade, PAR Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Bartlett, JG Bartolo, N Battaner, E Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bonaldi, A Bond, JR Borrill, J Bouchet, FR Bridges, M Bucher, M Burigana, C Butler, RC Calabrese, E Cardoso, JF Catalano, A Challinor, A Chamballu, A Chiang, HC Chiang, LY Christensen, PR Church, S Clements, DL Colombi, S Colombo, LPL Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Danese, L Davies, RD Davis, RJ de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Delouis, JM Desert, FX Dickinson, C Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Dunkley, J Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Finelli, F Forni, O Frailis, M Franceschi, E Galeotta, S Ganga, K Gauthier, C Giard, M Giardino, G Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Hamann, J Hansen, FK Hanson, D Harrison, D Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Jaffe, AH Jaffe, TR Jones, WC Juvela, M Keihanen, E Keskitalo, R Kisner, TS Kneissl, R Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lahteenmaki, A Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Leach, S Leahy, JP Leonardi, R Lesgourgues, J Lewis, A Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maffei, B Maino, D Mandolesi, N Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Mazzotta, P Meinhold, PR Melchiorri, A Mendes, L Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, MA Moneti, A Montier, L Morgante, G Mortlock, D Moss, A Munshi, D Murphy, JA Naselsky, P Nati, F Natoli, P Netterfield, CB Norgaard-Nielsen, HU Noviello, F Novikov, D Novikov, I O'Dwyer, IJ Osborne, S Oxborrow, CA Paci, F Pagano, L Pajot, F Paladini, R Pandolfi, S Paoletti, D Partridge, B Pasian, F Patanchon, G Peiris, HV Perdereau, O Perotto, L Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Rebolo, R Reinecke, M Remazeilles, M Renault, C Ricciardi, S Riller, T Ristorcelli, I Rocha, G Rosset, C Roudier, G Rowan-Robinson, M Rubino-Martin, JA Rusholme, B Sandri, M Santos, D Savelainen, M Savini, G Scott, D Seiffert, MD Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sunyaev, R Sureau, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Treguer-Goudineau, J Tristram, M Tucci, M Tuovinen, J Valenziano, L Valiviita, J Van Tent, B Varis, J Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD White, M Wilkinson, A Yvon, D Zacchei, A Zibin, JP Zonca, A AF Ade, P. A. R. Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Bartlett, J. G. Bartolo, N. Battaner, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J.-P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bonaldi, A. Bond, J. R. Borrill, J. Bouchet, F. R. Bridges, M. Bucher, M. Burigana, C. Butler, R. C. Calabrese, E. Cardoso, J.-F. Catalano, A. Challinor, A. Chamballu, A. Chiang, H. C. Chiang, L.-Y. Christensen, P. R. Church, S. Clements, D. L. Colombi, S. Colombo, L. P. L. Couchot, F. Coulais, A. Crill, B. P. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. Davis, R. J. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Delouis, J.-M. Desert, F.-X. Dickinson, C. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dunkley, J. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Finelli, F. Forni, O. Frailis, M. Franceschi, E. Galeotta, S. Ganga, K. Gauthier, C. Giard, M. Giardino, G. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Hamann, J. Hansen, F. K. Hanson, D. Harrison, D. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Jaffe, A. H. Jaffe, T. R. Jones, W. C. Juvela, M. Keihaenen, E. Keskitalo, R. Kisner, T. S. Kneissl, R. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Laehteenmaeki, A. Lamarre, J.-M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leach, S. Leahy, J. P. Leonardi, R. Lesgourgues, J. Lewis, A. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maffei, B. Maino, D. Mandolesi, N. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. Meinhold, P. R. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Miville-Deschenes, M.-A. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Moss, A. Munshi, D. Murphy, J. A. Naselsky, P. Nati, F. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novikov, I. O'Dwyer, I. J. Osborne, S. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paladini, R. Pandolfi, S. Paoletti, D. Partridge, B. Pasian, F. Patanchon, G. Peiris, H. V. Perdereau, O. Perotto, L. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J.-L. Rachen, J. P. Rebolo, R. Reinecke, M. Remazeilles, M. Renault, C. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Rosset, C. Roudier, G. Rowan-Robinson, M. Rubino-Martin, J. A. Rusholme, B. Sandri, M. Santos, D. Savelainen, M. Savini, G. Scott, D. Seiffert, M. D. Shellard, E. P. S. Spencer, L. D. Starck, J.-L. Stolyarov, V. Stompor, R. Sudiwala, R. Sunyaev, R. Sureau, F. Sutton, D. Suur-Uski, A.-S. Sygnet, J.-F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Treguer-Goudineau, J. Tristram, M. Tucci, M. Tuovinen, J. Valenziano, L. Valiviita, J. Van Tent, B. Varis, J. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. White, M. Wilkinson, A. Yvon, D. Zacchei, A. Zibin, J. P. Zonca, A. CA Planck Collaboration TI Planck 2013 results. XXII. Constraints on inflation SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE cosmic background radiation; inflation; early Universe ID PROBE WMAP OBSERVATIONS; BARYON ACOUSTIC-OSCILLATIONS; ISOTHERMAL DENSITY PERTURBATIONS; MICROWAVE BACKGROUND ANISOTROPY; PRIMORDIAL POWER SPECTRUM; OBSERVATIONS COSMOLOGICAL INTERPRETATION; AXION-DOMINATED UNIVERSE; PARTICLE PHYSICS MODELS; HUBBLE-SPACE-TELESCOPE; LARGE-SCALE STRUCTURE AB We analyse the implications of the Planck data for cosmic inflation. The Planck nominal mission temperature anisotropy measurements, combined with the WMAP large-angle polarization, constrain the scalar spectral index to be n(s) = 0.9603 +/- 0:0073, ruling out exact scale invariance at over 5 sigma Planck establishes an upper bound on the tensor-to-scalar ratio of r < 0.11 (95% CL). The Planck data thus shrink the space of allowed standard inflationary models preferring potentials with V '' < 0. Exponential potential models, the simplest hybrid inflationary models, and monomial potential models of degree n >= 2 do not provide a good fit to the data. Planck does not find statistically significant running of the scalar spectral index, obtaining dn(s)/dln k = -0.0134 +/- 0.0090. We verify these conclusions through a numerical analysis, which makes no slowroll approximation, and carry out a Bayesian parameter estimation and model-selection analysis for a number of inflationary models including monomial, natural, and hilltop potentials. For each model, we present the Planck constraints on the parameters of the potential and explore several possibilities for the post-inflationary entropy generation epoch, thus obtaining nontrivial data-driven constraints. We also present a direct reconstruction of the observable range of the inflaton potential. Unless a quartic term is allowed in the potential, we find results consistent with second-order slow-roll predictions. We also investigate whether the primordial power spectrum contains any features. We find that models with a parameterized oscillatory feature improve the fit by delta 2 10; however, Bayesian evidence does not prefer these models. We constrain several single-field inflation models with generalized Lagrangians by combining power spectrum data with Planck bounds on fNL. Planck constrains with unprecedented accuracy the amplitude and possible correlation (with the adiabatic mode) of non-decaying isocurvature fluctuations. The fractional primordial contributions of cold dark matter (CDM) isocurvature modes of the types expected in the curvaton and axion scenarios have upper bounds of 0.25% and 3.9% (95% CL), respectively. In models with arbitrarily correlated CDM or neutrino isocurvature modes, an anticorrelated isocurvature component can improve the 2 by approximately 4 as a result of slightly lowering the theoretical prediction for the 40 multipoles relative to the higher multipoles. Nonetheless, the data are consistent with adiabatic initial conditions. C1 [Bartlett, J. G.; Bucher, M.; Cardoso, J.-F.; Delabrouille, J.; Ganga, K.; Gauthier, C.; Giraud-Heraud, Y.; Patanchon, G.; Piat, M.; Poutanen, T.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.; Treguer-Goudineau, J.] Univ Paris Diderot, Observ Paris, Sorbonne Paris Cite, CNRS IN2P3,CEA lrfu,APC, F-75205 Paris 13, France. [Laehteenmaeki, A.] Aalto Univ, Metsahovi Radio Observ, Kylmala 02540, Finland. [Kunz, M.] African Inst Math Sci, ZA-7701 Cape Town, South Africa. [Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana, Sci Data Ctr, I-00133 Rome, Italy. [Mandolesi, N.] Agenzia Spaziale Italiana, I-00198 Rome, Italy. [Ashdown, M.; Bridges, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 0HE, England. [Chiang, H. C.] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, ZA-4000 Durban, South Africa. [Kneissl, R.] ALMA Santiago Cent Off, Vitacura 7630355, Casilla, Chile. [Bond, J. R.; Hanson, D.; Martin, P. G.; Miville-Deschenes, M.-A.] Univ Toronto, CITA, Toronto, ON M5S 3H8, Canada. [Banday, A. J.; Bernard, J.-P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] CNRS, IRAP, F-31028 Toulouse 4, France. [Bock, J. J.; Dore, O.; Hildebrandt, S. R.; Prezeau, G.; Rocha, G.; Seiffert, M. D.] CALTECH, Pasadena, CA 91125 USA. [Challinor, A.; Shellard, E. P. S.] Univ Cambridge, DAMTP, Ctr Theoret Cosmol, Cambridge CB3 0WA, England. [Hernandez-Monteagudo, C.] Ctr Estudios Fis Cosmos Aragon, Teruel 44001, Spain. [Borrill, J.; Keskitalo, R.] Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 94720 USA. CSIC, Madrid 28006, Spain. [Chamballu, A.; Rebolo, R.; Yvon, D.] CEA Saclay, DSM Irfu SPP, F-91191 Gif Sur Yvette, France. [Hornstrup, A.; Linden-Vornle, M.; Norgaard-Nielsen, H. U.; Oxborrow, C. A.] Tech Univ Denmark, Natl Space Inst, DTU Space, Lyngby 2800, Denmark. [Kunz, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, CH-1211 Geneva 4, Switzerland. [Atrio-Barandela, F.] Univ Salamanca, Fac Ciencias, Dept Fis Fundamental, Salamanca 37008, Spain. [Toffolatti, L.] Univ Oviedo, Dept Fis, Oviedo 33007, Spain. [Netterfield, C. B.] Univ Toronto, Dept Astron & Astrophys, Toronto, ON, Canada. [Rachen, J. P.] Radboud Univ Nijmegen, Dept Astrophys, IMAPP, NL-6500 GL Nijmegen, Netherlands. [Keskitalo, R.] Univ Calif Berkeley, Dept Elect Engn & Comp Sci, Berkeley, CA 94720 USA. [Scott, D.; Zibin, J. P.] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V5Z 1M9, Canada. [Colombo, L. P. L.; Pierpaoli, E.] Univ So Calif, Dept Phys & Astron, Dana & David Dornsife Coll Letter Arts & Sci, Los Angeles, CA 90089 USA. [Benoit-Levy, A.; Peiris, H. V.] UCL, Dept Phys & Astron, London WC1E 6BT, England. [Lewis, A.] Univ Sussex, Dept Phys & Astron, Brighton BN1 9QH, E Sussex, England. [Huffenberger, K. M.] Florida State Univ, Dept Phys, Tallahassee, FL USA. [Juvela, M.; Keihaenen, E.; Kurki-Suonio, H.; Poutanen, T.; Savelainen, M.; Suur-Uski, A.-S.; Valiviita, J.] Univ Helsinki, Dept Phys, FIN-00014 Helsinki, Finland. [Chiang, H. C.; Jones, W. C.] Princeton Univ, Dept Phys, Princeton, NJ USA. [White, M.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA. [Knox, L.] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA. [Lubin, P. M.; Meinhold, P. 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R.; Munshi, D.; Spencer, L. D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales. [Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England. [Sunyaev, R.] Russian Acad Sci, Special Astrophys Observ IKI, Moscow 117997, Russia. [Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA. [Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Karachai Cherkessian Rep, Russia. [Church, S.; Osborne, S.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA. [Armitage-Caplan, C.; Calabrese, E.; Dunkley, J.] Univ Oxford, Sub Dept Astrophys, Oxford OX1 3RH, England. [Hamann, J.; Lesgourgues, J.] CERN, Div Theory, PH TH, CH-1211 Geneva 23, Switzerland. [Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Colombi, S.; Delouis, J.-M.; Hivon, E.; Prunet, S.; Wandelt, B. D.] Univ Paris 06, UMR 7095, F-75014 Paris, France. [Banday, A. J.; Bernard, J.-P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, TRAP, F-31028 Toulouse 4, France. [Battaner, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, E-18071 Granada, Spain. [Gorski, K. M.] Univ Warsaw Observ, PL-00478 Warsaw, Poland. RP Bucher, M (reprint author), Univ Paris Diderot, Observ Paris, Sorbonne Paris Cite, CNRS IN2P3,CEA lrfu,APC, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France. EM bucher@apc.univ-paris7.fr RI Tomasi, Maurizio/I-1234-2016; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; White, Martin/I-3880-2015; Valiviita, Jussi/A-9058-2016; Kurki-Suonio, Hannu/B-8502-2016; Lahteenmaki, Anne/L-5987-2013; Toffolatti, Luigi/K-5070-2014; Martinez-Gonzalez, Enrique/E-9534-2015; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Mazzotta, Pasquale/B-1225-2016; Butler, Reginald/N-4647-2015; Barreiro, Rita Belen/N-5442-2014; Vielva, Patricio/F-6745-2014; bonavera, laura/E-9368-2017; Remazeilles, Mathieu/N-1793-2015; Yvon, Dominique/D-2280-2015; OI Tomasi, Maurizio/0000-0002-1448-6131; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; White, Martin/0000-0001-9912-5070; Valiviita, Jussi/0000-0001-6225-3693; Kurki-Suonio, Hannu/0000-0002-4618-3063; Toffolatti, Luigi/0000-0003-2645-7386; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Gruppuso, Alessandro/0000-0001-9272-5292; Mazzotta, Pasquale/0000-0002-5411-1748; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Galeotta, Samuele/0000-0002-3748-5115; Ricciardi, Sara/0000-0002-3807-4043; Zacchei, Andrea/0000-0003-0396-1192; Scott, Douglas/0000-0002-6878-9840; Villa, Fabrizio/0000-0003-1798-861X; Franceschi, Enrico/0000-0002-0585-6591; Mitra, Sanjit/0000-0002-0800-4626; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; Lopez-Caniego, Marcos/0000-0003-1016-9283; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Butler, Reginald/0000-0003-4366-5996; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Maris, Michele/0000-0001-9442-2754; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Frailis, Marco/0000-0002-7400-2135; Vielva, Patricio/0000-0003-0051-272X; bonavera, laura/0000-0001-8039-3876; Rubino-Martin, Jose Alberto/0000-0001-5289-3021; De Zotti, Gianfranco/0000-0003-2868-2595; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Savini, Giorgio/0000-0003-4449-9416; Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834 FU ESA; CNES; CNRS/INSU-IN2P3-INP (France); ASI; CNR; INAF (Italy); NASA; DoE (USA); STFC; UKSA (UK); CSIC; MICINN; JA; RES (Spain); Tekes; AoF; CSC (Finland); DLR; MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); PRACE (EU) FX The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.sciops.esa.int/index.php? project=planck&page=Planck_Collaboration. We gratefully acknowledge CINECA (http://www.cineca.it/) under the agreement LFI/CINECA and IN2P3 Computer Center (http://cc.in2p3.fr) for providing a significant amount of the computing resources and services needed for this work. NR 332 TC 1126 Z9 1126 U1 21 U2 89 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A22 DI 10.1051/0004-6361/201321569 PG 42 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600105 ER PT J AU Kaur, M Qiang, Y Jiang, WL Pearce, C McCloy, JS AF Kaur, Maninder Qiang, You Jiang, Weilin Pearce, Carolyn McCloy, John S. TI Magnetization Measurements and XMCD Studies on Ion Irradiated Iron Oxide and Core-Shell Iron/Iron-Oxide Nanomaterials SO IEEE TRANSACTIONS ON MAGNETICS LA English DT Article; Proceedings Paper CT IEEE International Magnetics Conference (Intermag) CY MAY 04-08, 2014 CL Dresden, GERMANY SP IEEE DE Core-shell; irradiation; magnetite; X-ray magnetic circular dichroism (XMCD) ID 2P ABSORPTION-SPECTRA; DICHROISM; NANOPARTICLES; DAMAGE AB Magnetite (Fe3O4) and core-shell iron/iron-oxide (Fe/FexOy) nanomaterials prepared by a cluster deposition system were irradiated with 5.5 MeV Si2+ ions and the structures determined by X-ray diffraction as consisting of 100% magnetite and 36/64 wt% Fe/FeO, respectively. However, X-ray magnetic circular dichroism (XMCD) indicates similar surfaces in the two samples, slightly oxidized and so having more Fe3+ than the expected magnetite structure, with XMCD intensity much lower for the irradiated core-shell samples indicating weaker magnetism. X-ray absorption spectroscopy (XAS) data lack a strong signature for FeO, but the irradiated core-shell system consists of Fe-cores with similar to 13 nm of separating oxide crystallite, so it is likely that most FeO (octahedral Fe2+) exists deeper than the probe depth of the XAS (similar to 5 nm). Exchange bias (H-ex) for both samples becomes increasingly negative as temperature is lowered, but the irradiated Fe3O4 sample shows greater sensitivity of cooling field on H-ex. Loop asymmetries and H-ex sensitivities of the irradiated Fe3O4 sample are due to interfaces and interactions between grains, which were not present in samples before irradiation, as well as surface oxidation. Asymmetries in the hysteresis curves of the irradiated core/shell sample are related to the reversal mechanism of the antiferromagnetic FeO and possibly some near surface oxidation. C1 [Kaur, Maninder; Qiang, You] Univ Idaho, Dept Phys, Moscow, ID 83844 USA. [Jiang, Weilin] Pacific NW Natl Lab, Richland, WA 99352 USA. [Pearce, Carolyn] Univ Manchester, Sch Chem, Manchester M13 9PL, Lancs, England. [McCloy, John S.] Washington State Univ, Sch Mech & Mat Engn, Pullman, WA 98163 USA. [McCloy, John S.] Washington State Univ, Mat Sci & Engn Program, Pullman, WA 98163 USA. RP McCloy, JS (reprint author), Washington State Univ, Sch Mech & Mat Engn, Pullman, WA 98163 USA. EM john.mccloy@wsu.edu OI Jiang, Weilin/0000-0001-8302-8313; McCloy, John/0000-0001-7476-7771 FU Laboratory Directed Research and Development, Idaho National Laboratory, Idaho Falls, ID, USA; National Science Foundation [DMR-1008791]; U.S. Department of Energy (DOE), Battelle, Benton, WA, USA through Pacific Northwest National Laboratory (PNNL), Richland, WA, USA [DE-AC05-76RL01830]; DOE Office of Science, Office of Basic Energy Sciences through Advance Light Source [DE-AC02-05CH11231]; DOE's Office of Biological and Environmental Research at PNNL FX This work was supported in part by the Laboratory Directed Research and Development, Idaho National Laboratory, Idaho Falls, ID, USA, in part by the National Science Foundation under Grant DMR-1008791, in part by the U.S. Department of Energy (DOE), Battelle, Benton, WA, USA, through the Pacific Northwest National Laboratory (PNNL), Richland, WA, USA, under Contract DE-AC05-76RL01830, and in part by the DOE Office of Science, Office of Basic Energy Sciences, through the Advance Light Source, under Contract DE-AC02-05CH11231. The authors would like to thank E. Arenholz for the assistance. Ion irradiation was performed using the Environmental Molecular Sciences Laboratory (EMSL), a national scientific user facility sponsored by the DOE's Office of Biological and Environmental Research and located at PNNL. NR 22 TC 2 Z9 2 U1 2 U2 20 PU IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC PI PISCATAWAY PA 445 HOES LANE, PISCATAWAY, NJ 08855-4141 USA SN 0018-9464 EI 1941-0069 J9 IEEE T MAGN JI IEEE Trans. Magn. PD NOV PY 2014 VL 50 IS 11 AR 4800305 DI 10.1109/TMAG.2014.2332347 PG 5 WC Engineering, Electrical & Electronic; Physics, Applied SC Engineering; Physics GA CB2NZ UT WOS:000349465900296 ER PT J AU Bonilla, CM Paudyal, D Herrero-Albillos, J Pecharsky, VK Gschneidner, KA Garcia, LM Bartolome, F AF Marcela Bonilla, Claudia Paudyal, Durga Herrero-Albillos, Julia Pecharsky, Vitalij K. Gschneidner, Karl A., Jr. Miguel Garcia, Luis Bartolome, Fernando TI Formation of Co Moment in the Paramagnetic Phase of RCo2 SO IEEE TRANSACTIONS ON MAGNETICS LA English DT Article; Proceedings Paper CT IEEE International Magnetics Conference (Intermag) CY MAY 04-08, 2014 CL Dresden, GERMANY SP IEEE DE First principles calculations; magnetic materials; rare-earth metals ID POINT-DEFECTS; ALLOYS AB The formation of Co magnetic moment in the paramagnetic phase of GdCo2 has been studied by means of first principles calculations. The introduction of impurities in the transition metal-rare-earth Laves phases leads to changes in the density of states of the transition metal 3d band. In this paper, we calculate the electronic structure of GdCo2 system (a C15 unit cell) with an interstitial impurity (Ti). Calculations show that local disorder introduced by the impurity shifts the Fermi level in such a way that Co 3d up and down states split. This result suggests that local disorder may be responsible for the formation of Co moment in this system. To deepen this phenomenon, we have considered the antisite substitution of a Gd atom by a Co within the unit cell, which is the most common defect in the Laves phases. Calculations show the formation of magnetic moment in the Co atom at the substituted site as well as in their nearest Co atoms, similarly to the observed in the systems with the interstitial impurity. Our results are compatible with the reported x-ray magnetic circular dichroism measurements performed in the RCo2 family of compounds. C1 [Marcela Bonilla, Claudia; Herrero-Albillos, Julia; Miguel Garcia, Luis; Bartolome, Fernando] Univ Zaragoza, Consejo Super Invest Cient, Inst Ciencia Mat Aragon, E-50009 Zaragoza, Spain. [Marcela Bonilla, Claudia; Miguel Garcia, Luis; Bartolome, Fernando] Dept Fis Mat Condensada, E-50009 Zaragoza, Spain. [Paudyal, Durga; Pecharsky, Vitalij K.; Gschneidner, Karl A., Jr.] Iowa Sate Univ, Ames Lab, Ames, IA 50011 USA. [Herrero-Albillos, Julia] Fdn ARAID, Zaragoza 50004, Spain. [Herrero-Albillos, Julia] Ctr Univ Def, Zaragoza 50090, Spain. [Pecharsky, Vitalij K.; Gschneidner, Karl A., Jr.] Iowa State Univ, Dept Mat Sci & Engn, Ames, IA 50011 USA. RP Bonilla, CM (reprint author), Univ Zaragoza, Consejo Super Invest Cient, Inst Ciencia Mat Aragon, E-50009 Zaragoza, Spain. EM mbonilla@unizar.es RI Herrero-Albillos, Julia/I-5462-2012; Herrero-Albillos, Julia/B-9837-2009; Bartolome, Fernando/K-1700-2014 OI Herrero-Albillos, Julia/0000-0002-0901-8341; Herrero-Albillos, Julia/0000-0002-0901-8341; Bartolome, Fernando/0000-0002-0047-1772 FU Ministry of Economy and Competitiveness, Government of Spain [MAT2011-23791]; European Social Fund through Diputacion General de Aragon; U. S. Department of Energy [DE-AC02-07-CH11358] FX This work was supported in part by the Ministry of Economy and Competitiveness, Government of Spain, under Grant MAT2011-23791, and in part by the European Social Fund through Diputacion General de Aragon. The work of D. Paudyal, V. K. Pecharsky, and K. A. Gschneidner, Jr., was supported by the U. S. Department of Energy under Contract DE-AC02-07-CH11358. NR 15 TC 1 Z9 1 U1 1 U2 13 PU IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC PI PISCATAWAY PA 445 HOES LANE, PISCATAWAY, NJ 08855-4141 USA SN 0018-9464 EI 1941-0069 J9 IEEE T MAGN JI IEEE Trans. Magn. PD NOV PY 2014 VL 50 IS 11 AR 1700204 DI 10.1109/TMAG.2014.2330815 PG 4 WC Engineering, Electrical & Electronic; Physics, Applied SC Engineering; Physics GA CB2NZ UT WOS:000349465900030 ER PT J AU Poudel, N Lorenz, B Liang, KC Wang, YQ Sun, YY Ye, F Fernandez-Baca, JA Chu, CW AF Poudel, Narayan Lorenz, Bernd Liang, Kao-Chen Wang, Ya-Qi Sun, Yan Yi Ye, Feng Fernandez-Baca, Jaime A. Chu, Ching-Wu TI Spontaneous Polarization Reversal in Multiferroic Mn0.85Co0.15WO4 Induced by an External Magnetic Field SO IEEE TRANSACTIONS ON MAGNETICS LA English DT Article; Proceedings Paper CT IEEE International Magnetics Conference (Intermag) CY MAY 04-08, 2014 CL Dresden, GERMANY SP IEEE DE Magnetic domains; multiferroics; polarization switching AB The multiferroic properties of Mn0.85Co0.15WO4 are studied in magnetic fields oriented along the monoclinic c-axis. A spontaneous sign reversal of the ferroelectric polarization is observed upon decreasing temperature if cooled in a constant magnetic field. This unusual phenomenon is explained by the coexistence of different multiferroic phases with conical and spiral spin structures. These phases form domains which contribute to the electrical polarization in different temperature ranges. The sign reversal of the polarization is explained by an analysis of the contributions from the different domains to the net value of the polarization. It is concluded that the spiral and conical magnetic orders in neighboring domains are strongly coupled leading to the preservation of the spin chirality across the domain walls. C1 [Poudel, Narayan; Lorenz, Bernd; Liang, Kao-Chen; Wang, Ya-Qi; Sun, Yan Yi; Chu, Ching-Wu] Univ Houston, Texas Ctr Superconduct, Houston, TX 77204 USA. [Poudel, Narayan; Lorenz, Bernd; Liang, Kao-Chen; Wang, Ya-Qi; Sun, Yan Yi; Chu, Ching-Wu] Univ Houston, Dept Phys, Houston, TX 77204 USA. [Ye, Feng; Fernandez-Baca, Jaime A.] Oak Ridge Natl Lab, Quantum Condensed Matter Div, Oak Ridge, TN 37831 USA. [Fernandez-Baca, Jaime A.] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA. [Chu, Ching-Wu] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. RP Lorenz, B (reprint author), Univ Houston, Texas Ctr Superconduct, Houston, TX 77204 USA. EM blorenz@uh.edu RI Ye, Feng/B-3210-2010; Fernandez-Baca, Jaime/C-3984-2014 OI Ye, Feng/0000-0001-7477-4648; Fernandez-Baca, Jaime/0000-0001-9080-5096 FU U.S. Air Force Office of Scientific Research [FA9550-09-0656]; T.L.L. Temple Foundation; John J. and Rebecca Moores Endowment; State of Texas through the Texas Center for Superconductivity, University of Houston; DOE BES Office of Scientific User Facilities at the Oak Ridge National Laboratory, Oak Ridge, TN, USA FX This work was supported in part by the U.S. Air Force Office of Scientific Research under Grant FA9550-09-0656, in part by the T.L.L. Temple Foundation, in part by the John J. and Rebecca Moores Endowment, in part by the State of Texas through the Texas Center for Superconductivity, University of Houston, and in part by the DOE BES Office of Scientific User Facilities at the Oak Ridge National Laboratory, Oak Ridge, TN, USA. NR 16 TC 0 Z9 0 U1 0 U2 5 PU IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC PI PISCATAWAY PA 445 HOES LANE, PISCATAWAY, NJ 08855-4141 USA SN 0018-9464 EI 1941-0069 J9 IEEE T MAGN JI IEEE Trans. Magn. PD NOV PY 2014 VL 50 IS 11 AR 2503904 DI 10.1109/TMAG.2014.2320192 PG 4 WC Engineering, Electrical & Electronic; Physics, Applied SC Engineering; Physics GA CB2NZ UT WOS:000349465900121 ER PT J AU Rahman, BMF Divan, R Stan, L Rosenmann, D Ocola, LE Wang, GA AF Rahman, B. M. Farid Divan, Ralu Stan, Liliana Rosenmann, Daniel Ocola, Leonidas E. Wang, Guoan TI Tunable Transmission Line With Nanopatterned Thin Films for Smart RF Applications SO IEEE TRANSACTIONS ON MAGNETICS LA English DT Article; Proceedings Paper CT IEEE International Magnetics Conference (Intermag) CY MAY 04-08, 2014 CL Dresden, GERMANY SP IEEE DE Ferroelectric film; ferromagnetic film; impedance matching network; nanopatterns; transmission line (TL); tunable delay line ID FILTER AB A concept of tunable transmission line (TL) enabled with nanopatterned ferromagnetic permalloy (Py) and ferroelectric lead zirconium titanate (PZT) thin films is presented. The permittivity (epsilon(r)) of PZT is electrical tunable with dc voltage, and the permeability (mu(r)) of Py is electrical tunable with dc current, thus simultaneous electric tunable capacitance and inductance capability are provided for the proposed TL. The proposed TL has been fabricated and compared with a regular line without nanofilm patterns. Py is patterned with the dimensions of 10 mu m x 150 nm and thickness of 100 nm for high built-in anisotropy field. The ferromagnetic resonant frequency is measured to be 6.3 GHz. Compared with the regular TL, the implemented TL has only generated 0.05 dB additional insertion loss at 4 GHz. The electrical tunability of both the capacitance and the inductance has been demonstrated for the first time. By applying the varied dc current (0-150 mA) and the dc voltage (0-20 V), measured results have shown that the proposed line can provide 90 degrees phase shift from 3.75 to 4 GHz with the fixed characteristic impedance. The continuous tuning of the characteristics impedance from 59 to 61 Omega under suitable bias conditions shows its promise as an impedance matching network. Tunable range of both the phase shifter and the impedance matching network can be further increased with thicker and multilayer films. C1 [Rahman, B. M. Farid; Wang, Guoan] Univ S Carolina, Dept Elect Engn, Microwave Applicat Grp, Columbia, SC 29208 USA. [Divan, Ralu; Stan, Liliana; Rosenmann, Daniel; Ocola, Leonidas E.] Argonne Natl Lab, Ctr Nanoscale Mat, Lemont, IL 60439 USA. RP Wang, GA (reprint author), Univ S Carolina, Dept Elect Engn, Microwave Applicat Grp, Columbia, SC 29208 USA. EM gwang@cec.sc.edu OI Ocola, Leonidas/0000-0003-4990-1064 FU NSF [1253929]; U. S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-AC02- 06CH11357] FX This work was supported in part by the NSF under Award 1253929, and in part by the U. S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract DE-AC02- 06CH11357 for fabrication of the device using the Center for Nanoscale Materials, Argonne National Laboratory. The authors would like to thank ANSYS for software support. NR 20 TC 2 Z9 2 U1 1 U2 13 PU IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC PI PISCATAWAY PA 445 HOES LANE, PISCATAWAY, NJ 08855-4141 USA SN 0018-9464 EI 1941-0069 J9 IEEE T MAGN JI IEEE Trans. Magn. PD NOV PY 2014 VL 50 IS 11 AR 2801604 DI 10.1109/TMAG.2014.2329793 PG 4 WC Engineering, Electrical & Electronic; Physics, Applied SC Engineering; Physics GA CB2NZ UT WOS:000349465900159 ER PT J AU Kota, KP Soloveva, V Wanner, LM Gomba, G Kiris, E Panchal, RG Kane, CD Bavari, S AF Kota, Krishna P. Soloveva, Veronica Wanner, Laura M. Gomba, Glenn Kiris, Erkan Panchal, Rekha G. Kane, Christopher D. Bavari, Sina TI A High Content Imaging Assay for Identification of Botulinum Neurotoxin Inhibitors SO JOVE-JOURNAL OF VISUALIZED EXPERIMENTS LA English DT Article DE Neuroscience; Issue 93; neuroscience; neurobiology; Botulinum neurotoxin; Clostridium botulinum; high content imaging system; neurotoxicity ID SEROTYPE AB Synaptosomal-associated protein-25 (SNAP-25) is a component of the soluble NSF attachment protein receptor (SNARE) complex that is essential for synaptic neurotransmitter release. Botulinum neurotoxin serotype A (BoNT/A) is a zinc metalloprotease that blocks exocytosis of neurotransmitter by cleaving the SNAP-25 component of the SNARE complex. Currently there are no licensed medicines to treat BoNT/A poisoning after internalization of the toxin by motor neurons. The development of effective therapeutic measures to counter BoNT/A intoxication has been limited, due in part to the lack of robust high-throughput assays for screening small molecule libraries. Here we describe a high content imaging (HCI) assay with utility for identification of BoNT/A inhibitors. Initial optimization efforts focused on improving the reproducibility of inter-plate results across multiple, independent experiments. Automation of immunostaining, image acquisition, and image analysis were found to increase assay consistency and minimize variability while enabling the multiparameter evaluation of experimental compounds in a murine motor neuron system. C1 [Kota, Krishna P.] Perkin Elmer Inc, Waltham, MA 02451 USA. [Soloveva, Veronica; Kane, Christopher D.] Henry M Jackson Fdn, Bethesda, MD USA. [Wanner, Laura M.; Kiris, Erkan] Geneva Fdn, Tacoma, WA USA. [Gomba, Glenn] ORISE, Oak Ridge, TN USA. [Kiris, Erkan] Frederick Natl Lab Canc Res, Frederick, MD USA. [Kota, Krishna P.; Soloveva, Veronica; Wanner, Laura M.; Gomba, Glenn; Kiris, Erkan; Panchal, Rekha G.; Kane, Christopher D.; Bavari, Sina] US Army Med Res Inst Infect Dis, Div Mol & Translat Sci, Frederick, MD USA. [Soloveva, Veronica; Kane, Christopher D.] USAMRMC, TATRC, DoD Biotechnol High Performance Comp Software App, Frederick, MD USA. RP Kota, KP (reprint author), Perkin Elmer Inc, Waltham, MA 02451 USA. EM krishna.p.kota.ctr@mail.mil FU Joint Science and Technology Office - Chemical Biological Defense (JSTO-CBD) Defense Threat Reduction Agency (DTRA) [CB3675]; National Institutes of Health [1 R21 AI101387-01, 5 U01AI082051-05] FX Funding was provided by the Joint Science and Technology Office - Chemical Biological Defense (JSTO-CBD) Defense Threat Reduction Agency (DTRA) under sponsor project number CCAR# CB3675 and National Institutes of Health (1 R21 AI101387-01 and 5 U01AI082051-05). NR 14 TC 2 Z9 2 U1 1 U2 3 PU JOURNAL OF VISUALIZED EXPERIMENTS PI CAMBRIDGE PA 1 ALEWIFE CENTER, STE 200, CAMBRIDGE, MA 02140 USA SN 1940-087X J9 JOVE-J VIS EXP JI J. Vis. Exp. PD NOV PY 2014 IS 93 AR e51915 DI 10.3791/51915 PG 10 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA CB0JH UT WOS:000349311400022 PM 25489815 ER PT J AU Adamska, L Nayyar, I Chen, H Swan, AK Oldani, N Fernandez-Alberti, S Golder, MR Jasti, R Doorn, SK Tretiak, S AF Adamska, Lyudmyla Nayyar, Iffat Chen, Hang Swan, Anna K. Oldani, Nicolas Fernandez-Alberti, Sebastian Golder, Matthew R. Jasti, Ramesh Doorn, Stephen K. Tretiak, Sergei TI Self-Trapping of Excitons, Violation of Condon Approximation, and Efficient Fluorescence in Conjugated Cycloparaphenylenes SO NANO LETTERS LA English DT Article DE Time-dependent density functional theory; nonadiabatic excited state molecular dynamics; exciton-vibrational coupling; photoluminescence spectra ID DENSITY-FUNCTIONAL THEORY; CARBON NANORINGS; OPTOELECTRONIC PROPERTIES; OPTICAL-PROPERTIES; DYNAMICS; DEPENDENCE; SCATTERING; MOLECULES; SPECTRA; N=8-13 AB Cycloparaphenylenes, the simplest structural unit of armchair carbon nanotubes, have unique optoelectronic properties counterintuitive in the class of conjugated organic materials. Our time-dependent density functional theory study and excited state dynamics simulations of cycloparaphenylene chromophores provide a simple and conceptually appealing physical picture explaining experimentally observed trends in optical properties in this family of molecules. Fully delocalized degenerate second and third excitonic states define linear absorption spectra. Self-trapping of the lowest excitonic state due to electron-phonon coupling leads to the formation of spatially localized excitation in large cycloparaphenylenes within 100 fs. This invalidates the commonly used Condon approximation and breaks optical selection rules, making these materials superior fluorophores. This process does not occur in the small molecules, which remain inefficient emitters. A complex interplay of symmetry, p-conjugation, conformational distortion and bending strain controls all photophysics of cycloparaphenylenes. C1 [Adamska, Lyudmyla; Nayyar, Iffat; Doorn, Stephen K.; Tretiak, Sergei] Los Alamos Natl Lab, Ctr Nonlinear Studies, Theoret Div, Los Alamos, NM 87545 USA. [Adamska, Lyudmyla; Nayyar, Iffat; Doorn, Stephen K.; Tretiak, Sergei] Los Alamos Natl Lab, Ctr Integrated Nanotechnol CINT, Los Alamos, NM 87545 USA. [Nayyar, Iffat; Chen, Hang] Boston Univ, Dept Elect & Comp Engn, Boston, MA 02215 USA. [Chen, Hang; Swan, Anna K.] Boston Univ, Photon Ctr, Boston, MA 02215 USA. [Oldani, Nicolas; Fernandez-Alberti, Sebastian] Univ Nacl Quilmes, Bernal, Argentina. [Golder, Matthew R.; Jasti, Ramesh] Univ Oregon, Dept Chem & Biochem, Eugene, OR 97403 USA. [Golder, Matthew R.; Jasti, Ramesh] Univ Oregon, Mat Sci Inst 1253, Eugene, OR 97403 USA. RP Tretiak, S (reprint author), Los Alamos Natl Lab, Ctr Nonlinear Studies, Theoret Div, Los Alamos, NM 87545 USA. EM serg@lanl.gov RI Tretiak, Sergei/B-5556-2009; Nayyar, Iffat/B-4925-2016 OI Tretiak, Sergei/0000-0001-5547-3647; Nayyar, Iffat/0000-0002-0896-5259 FU U.S. Department of Energy; Los Alamos LDRD funds; CONICET; UNQ; ANPCyT [PICT-2010-2375]; National Nuclear Security Administration of the U.S. Department of Energy [DE-AC5206NA25396]; Center for Integrated Nanotechnologies (CINT); Center for Nonlinear Studies (CNLS) at LANL FX L.A. acknowledges Professor A. Zhugayevych for his help with data processing. This work was supported by the U.S. Department of Energy and Los Alamos LDRD funds. This work was also partially supported by CONICET, UNQ, ANPCyT (PICT-2010-2375). Los Alamos National Laboratory is operated by Los Alamos National Security, LLC, for the National Nuclear Security Administration of the U.S. Department of Energy under contract DE-AC5206NA25396. We acknowledge support from the Center for Integrated Nanotechnologies (CINT) and the Center for Nonlinear Studies (CNLS) at LANL. NR 47 TC 35 Z9 35 U1 2 U2 32 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1530-6984 EI 1530-6992 J9 NANO LETT JI Nano Lett. PD NOV PY 2014 VL 14 IS 11 BP 6539 EP 6546 DI 10.1021/nl503133e PG 8 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied; Physics, Condensed Matter SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AU6PE UT WOS:000345723800081 PM 25310514 ER PT J AU Biegalski, MD Takamura, Y Mehta, A Gai, Z Kalinin, SV Ambaye, H Lauter, V Fong, D Pantelides, ST Kim, YM He, J Borisevich, A Siemons, W Christen, HM AF Biegalski, Michael. D. Takamura, Yayoi Mehta, Apurva Gai, Zhang Kalinin, Sergei V. Ambaye, Haile Lauter, Valieria Fong, Dillon Pantelides, Sokrates T. Kim, Young. M. He, Jun. Borisevich, Albina Siemons, Wolter Christen, Hans M. TI Interrelation between Structure - Magnetic Properties in La0.5Sr0.5CoO3 SO ADVANCED MATERIALS INTERFACES LA English DT Article ID PEROVSKITES; LEVEL C1 [Biegalski, Michael. D.; Gai, Zhang; Kalinin, Sergei V.; Christen, Hans M.] Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37830 USA. [Takamura, Yayoi] Univ Calif Davis, Dept Chem Engn & Mat Sci, Davis, CA 95616 USA. [Mehta, Apurva] Stanford Synchrotron Radiat Lightsource, Menlo Pk, CA 94025 USA. [Ambaye, Haile; Lauter, Valieria] Oak Ridge Natl Lab, Neutron Scattering Sci Div, Oak Ridge, TN 37830 USA. [Fong, Dillon] Argonne Natl Lab, Div Mat Sci, Argonne, IL 60439 USA. [Pantelides, Sokrates T.] Vanderbilt Univ, Dept Phys & Astron, Nashville, TN 37235 USA. [Kim, Young. M.] Korea Basic Sci Inst, Taejon 305806, South Korea. [Kim, Young. M.; He, Jun.; Borisevich, Albina; Siemons, Wolter] Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37830 USA. RP Biegalski, MD (reprint author), Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37830 USA. EM biegalskim@ornl.gov RI Borisevich, Albina/B-1624-2009; Kalinin, Sergei/I-9096-2012; Christen, Hans/H-6551-2013; Ambaye, Haile/D-1503-2016; Kim, Young-Min/B-7338-2012; Gai, Zheng/B-5327-2012 OI Borisevich, Albina/0000-0002-3953-8460; Kalinin, Sergei/0000-0001-5354-6152; Christen, Hans/0000-0001-8187-7469; Ambaye, Haile/0000-0002-8122-9952; Kim, Young-Min/0000-0003-3220-9004; Gai, Zheng/0000-0002-6099-4559 FU Office of Basic Energy Sciences (BES), U.S. Department of Energy (DOE); Division of Materials Sciences, DOE-BES FX Research performed at the Center for Nanophase Materials Sciences, the Spallation Neutron Source (both at Oak Ridge National Laboratory), and the Stanford Synchrotron Radiation Lightsource (SLAC National Accelerator Laboratory), which are sponsored by the Office of Basic Energy Sciences (BES), U.S. Department of Energy (DOE). S.V.K, Y.M.K, A.B., and W.S. were supported by the Division of Materials Sciences, DOE-BES. YT acknowledges the National Science Foundation (DMR 0747896). NR 28 TC 7 Z9 7 U1 2 U2 38 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 2196-7350 J9 ADV MATER INTERFACES JI Adv. Mater. Interfaces PD NOV PY 2014 VL 1 IS 8 AR 1400203 DI 10.1002/admi.201400203 PG 7 WC Chemistry, Multidisciplinary; Materials Science, Multidisciplinary SC Chemistry; Materials Science GA AZ5UJ UT WOS:000348285900014 ER PT J AU Wagner, M Seiler, S Meyer, B Boatner, LA Schmid, M Diebold, U AF Wagner, Margareta Seiler, Steffen Meyer, Bernd Boatner, Lynn A. Schmid, Michael Diebold, Ulrike TI Reducing the In2O3 (111) Surface Results in Ordered Indium Adatoms SO ADVANCED MATERIALS INTERFACES LA English DT Article ID GAS SENSOR; FILMS; RECONSTRUCTION; TIO2(110); CHEMISTRY; STM C1 [Wagner, Margareta; Schmid, Michael; Diebold, Ulrike] Vienna Univ Technol, Inst Appl Phys, A-1040 Vienna, Austria. [Seiler, Steffen; Meyer, Bernd] Univ Erlangen Nurnberg, Interdisciplinary Ctr Mol Mat, D-91052 Erlangen, Germany. [Seiler, Steffen; Meyer, Bernd] Univ Erlangen Nurnberg, Comp Chem Ctr, D-91052 Erlangen, Germany. [Boatner, Lynn A.] Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA. RP Wagner, M (reprint author), Vienna Univ Technol, Inst Appl Phys, Wiedner Hauptstr 8-10-134, A-1040 Vienna, Austria. EM wagner@iap.tuwien.ac.at RI Wagner, Margareta/F-3835-2015; OI Schmid, Michael/0000-0003-3373-9357 FU European Research Council; Fonds der Chemischen Industrie (FCI); U.S. Department of Energy, Basic Energy Sciences, Materials Sciences and Engineering Division FX This work was supported by the European Research Council Advanced Grant "OxideSurfaces". S. S. thanks the Fonds der Chemischen Industrie (FCI) for a Chemiefonds Fellowship. Research at the Oak Ridge National Laboratory for one author (L. A. B.) was sponsored by the U.S. Department of Energy, Basic Energy Sciences, Materials Sciences and Engineering Division. NR 35 TC 3 Z9 3 U1 3 U2 25 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 2196-7350 J9 ADV MATER INTERFACES JI Adv. Mater. Interfaces PD NOV PY 2014 VL 1 IS 8 AR UNSP 1400289 DI 10.1002/admi.201400289 PG 6 WC Chemistry, Multidisciplinary; Materials Science, Multidisciplinary SC Chemistry; Materials Science GA AZ5UJ UT WOS:000348285900017 ER PT J AU Zherebetskyy, D Wang, LW AF Zherebetskyy, Danylo Wang, Lin-Wang TI In-Gap States in Electronic Structure of Nonpolar Surfaces of Insulating Metal Oxides SO ADVANCED MATERIALS INTERFACES LA English DT Article ID TOTAL-ENERGY CALCULATIONS; AUGMENTED-WAVE METHOD; SEMICONDUCTOR SURFACES; HYBRID DFT; BASIS-SET; 1ST-PRINCIPLES; SRTIO3; PEROVSKITE; DENSITY; BATIO3 C1 [Zherebetskyy, Danylo; Wang, Lin-Wang] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA. RP Wang, LW (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Mat Sci, 1 Cyclotron Rd Mail Stop 066, Berkeley, CA 94720 USA. EM lwwang@lbl.gov FU Office of Science (SC), Basic Energy Science (BES)/Materials Science and Engineering Division (MSED) of the U.S. Department of Energy (DOE) [DE-AC02-05CH11231]; Office of Science of the U.S. Department of Energy FX This work was supported by the Director, Office of Science (SC), Basic Energy Science (BES)/Materials Science and Engineering Division (MSED) of the U.S. Department of Energy (DOE) under the contract No. DE-AC02-05CH11231. It used resources of the National Energy Research Scientific Computing Center (NERSC) and Oak Ridge Leadership Computing Facility (OLCF) that are supported by the Office of Science of the U.S. Department of Energy, with the computational time allocated by the Innovative and Novel Computational Impact on Theory and Experiment (INCITE) project. NR 69 TC 8 Z9 8 U1 3 U2 10 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 2196-7350 J9 ADV MATER INTERFACES JI Adv. Mater. Interfaces PD NOV PY 2014 VL 1 IS 8 AR 1300131 DI 10.1002/admi.201300131 PG 6 WC Chemistry, Multidisciplinary; Materials Science, Multidisciplinary SC Chemistry; Materials Science GA AZ5UJ UT WOS:000348285900001 ER PT J AU Abergel, A Ade, PAR Aghanim, N Alves, MIR Aniano, G Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Bartlett, JG Battaner, E Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bonaldi, A Bond, JR Borrill, J Bouchet, FR Boulanger, F Bridges, M Bucher, M Burigana, C Butler, RC Cardoso, JF Catalano, A Chamballu, A Chary, RR Chiang, HC Chiang, LY Christensen, PR Church, S Clemens, M Clements, DL Colombi, S Colombo, LPL Combet, C Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Danese, L Davies, RD Davis, RJ de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Delouis, JM Desert, FX Dickinson, C Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Draine, BT Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Falgarone, E Finelli, F Forni, O Frailis, M Fraisse, AA Franceschi, E Galeotta, S Ganga, K Ghosh, T Giard, M Giardino, G Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Grenier, IA Gruppuso, A Guillet, V Hansen, FK Hanson, D Harrison, DL Helou, G Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Jaffe, AH Jaffe, TR Jewell, J Joncas, G Jones, WC Juvela, M Keihanen, E Keskitalo, R Kisner, TS Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lahteenmaki, A Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Leonardi, R Leon-Tavares, J Lesgourgues, J Levrier, F Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maffei, B Maino, D Mandolesi, N Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Mazzotta, P McGehee, P Melchiorri, A Mendes, L Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, MA Moneti, A Montier, L Morgante, G Mortlock, D Munshi, D Murphy, JA Naselsky, P Nati, F Natoli, P Netterfield, CB Norgaard-Nielsen, HU Noviello, F Novikov, D Novikov, I Osborne, S Oxborrow, CA Paci, F Pagano, L Pajot, F Paladini, R Paoletti, D Pasian, F Patanchon, G Perdereau, O Perotto, L Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Reach, WT Rebolo, R Reinecke, M Remazeilles, M Renault, C Ricciardi, S Riller, T Ristorcelli, I Rocha, G Rosset, C Roudier, G Rowan-Robinson, M Rubino-Martin, JA Rusholme, B Sandri, M Santos, D Savini, G Scott, D Seiffert, MD Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sunyaev, R Sureau, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Tuovinen, J Turler, M Umana, G Valenziano, L Valiviita, J Van Tent, B Verstraete, L Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD Welikala, N Ysard, N Yvon, D Zacchei, A Zonca, A AF Abergel, A. Ade, P. A. R. Aghanim, N. Alves, M. I. R. Aniano, G. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Bartlett, J. G. Battaner, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bonaldi, A. Bond, J. R. Borrill, J. Bouchet, F. R. Boulanger, F. Bridges, M. Bucher, M. Burigana, C. Butler, R. C. Cardoso, J. -F. Catalano, A. Chamballu, A. Chary, R. -R. Chiang, H. C. Chiang, L. -Y Christensen, P. R. Church, S. Clemens, M. Clements, D. L. Colombi, S. Colombo, L. P. L. Combet, C. Couchot, F. Coulais, A. Crill, B. P. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. Davis, R. J. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Delouis, J. -M. Desert, F. -X. Dickinson, C. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Draine, B. T. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Falgarone, E. Finelli, F. Forni, O. Frailis, M. Fraisse, A. A. Franceschi, E. Galeotta, S. Ganga, K. Ghosh, T. Giard, M. Giardino, G. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Grenier, I. A. Gruppuso, A. Guillet, V. Hansen, F. K. Hanson, D. Harrison, D. L. Helou, G. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Jaffe, A. H. Jaffe, T. R. Jewell, J. Joncas, G. Jones, W. C. Juvela, M. Keihaenen, E. Keskitalo, R. Kisner, T. S. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Laehteenmaeki, A. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leonardi, R. Leon-Tavares, J. Lesgourgues, J. Levrier, F. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maffei, B. Maino, D. Mandolesi, N. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. McGehee, P. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Miville-Deschenes, M. -A. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Munshi, D. Murphy, J. A. Naselsky, P. Nati, F. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novikov, I. Osborne, S. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paladini, R. Paoletti, D. Pasian, F. Patanchon, G. Perdereau, O. Perotto, L. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Reach, W. T. Rebolo, R. Reinecke, M. Remazeilles, M. Renault, C. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Rosset, C. Roudier, G. Rowan-Robinson, M. Rubino-Martin, J. A. Rusholme, B. Sandri, M. Santos, D. Savini, G. Scott, D. Seiffert, M. D. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sunyaev, R. Sureau, F. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Tuovinen, J. Tuerler, M. Umana, G. Valenziano, L. Valiviita, J. Van Tent, B. Verstraete, L. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. Welikala, N. Ysard, N. Yvon, D. Zacchei, A. Zonca, A. TI Planck 2013 results. XI. All-sky model of thermal dust emission SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE methods: data analysis; ISM: general; dust, extinction; infrared: ISM; submillimeter: ISM; opacity ID INTERSTELLAR MOLECULAR-HYDROGEN; SPECTRAL ENERGY-DISTRIBUTIONS; HIGH GALACTIC LATITUDES; 7TH DATA RELEASE; INFRARED-EMISSION; ULTRAVIOLET EXTINCTION; CIRRUS CLOUDS; H-I; PROTOPLANETARY DISKS; SOLAR NEIGHBORHOOD AB This paper presents an all-sky model of dust emission from the Planck 353, 545, and 857 GHz, and IRAS 100 mu m data. Using a modified blackbody fit to the data we present all-sky maps of the dust optical depth, temperature, and spectral index over the 353-3000 GHz range. This model is a good representation of the IRAS and Planck data at 5 0 between 353 and 3000 GHz (850 and 100 mu m). It shows variations of the order of 30% compared with the widely-used model of Finkbeiner, Davis, and Schlegel. The Planck data allow us to estimate the dust temperature uniformly over the whole sky, down to an angular resolution of 5 0, providing an improved estimate of the dust optical depth compared to previous all-sky dust model, especially in high-contrast molecular regions where the dust temperature varies strongly at small scales in response to dust evolution, extinction, and/or local production of heating photons. An increase of the dust opacity at 353 GHz, tau(353)/N-H, from the diffuse to the denser interstellar medium (ISM) is reported. It is associated with a decrease in the observed dust temperature, T-obs, that could be due at least in part to the increased dust opacity. We also report an excess of dust emission at HI column densities lower than 10(20) cm(-2) that could be the signature of dust in the warm ionized medium. In the diffuse ISM at high Galactic latitude, we report an anticorrelation between tau(353)/N-H and T-obs while the dust specific luminosity, i.e., the total dust emission integrated over frequency (the radiance) per hydrogen atom, stays about constant, confirming one of the Planck Early Results obtained on selected fields. This e ff ect is compatible with the view that, in the diffuse ISM, Tobs responds to spatial variations of the dust opacity, due to variations of dust properties, in addition to (small) variations of the radiation field strength. The implication is that in the di ff use high-latitude ISM tau(353) is not as reliable a tracer of dust column density as we conclude it is in molecular clouds where the correlation of tau(353) with dust extinction estimated using colour excess measurements on stars is strong. To estimate Galactic E(B-V) in extragalactic fields at high latitude we develop a new method based on the thermal dust radiance, instead of the dust optical depth, calibrated to E(B-V) using reddening measurements of quasars deduced from Sloan Digital Sky Survey data. C1 [Bartlett, J. G.; Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Gorski, K. M.; Patanchon, G.; Piat, M.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.; Welikala, N.] Univ Paris Diderot, CNRS IN2P3, Observ Paris, Sorbonne Paris Cite,CEA Irfu,APC, F-75205 Paris 13, France. [Laehteenmaeki, A.; Leon-Tavares, J.; Poutanen, T.] Aalto Univ, Metsahovi Radio Observ, Aalto 00076, Finland. 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T.] Univ Space Res Assoc, Stratospher Observ Infrared Astron, Moffett Field, CA 94035 USA. [Battaner, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, Granada, Spain. [Gorski, K. M.] Univ Warsaw Observ, PL-00478 Warsaw, Poland. RP Miville-Deschenes, MA (reprint author), Univ Paris 11, CNRS, Inst Astrophys Spatiale, UMR8617, Batiment 121, F-91405 Orsay, France. EM mamd@ias.u-psud.fr RI Barreiro, Rita Belen/N-5442-2014; Butler, Reginald/N-4647-2015; Remazeilles, Mathieu/N-1793-2015; Ghosh, Tuhin/E-6899-2016; Tomasi, Maurizio/I-1234-2016; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; Lahteenmaki, Anne/L-5987-2013; Novikov, Dmitry/P-1807-2015; Valiviita, Jussi/A-9058-2016; Mazzotta, Pasquale/B-1225-2016; Kurki-Suonio, Hannu/B-8502-2016; Toffolatti, Luigi/K-5070-2014; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Martinez-Gonzalez, Enrique/E-9534-2015; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Gruppuso, Alessandro/N-5592-2015 OI Juvela, Mika/0000-0002-5809-4834; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Savini, Giorgio/0000-0003-4449-9416; Pierpaoli, Elena/0000-0002-7957-8993; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; Reach, William/0000-0001-8362-4094; Zacchei, Andrea/0000-0003-0396-1192; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Ricciardi, Sara/0000-0002-3807-4043; Villa, Fabrizio/0000-0003-1798-861X; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Lopez-Caniego, Marcos/0000-0003-1016-9283; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Butler, Reginald/0000-0003-4366-5996; Umana, Grazia/0000-0002-6972-8388; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Galeotta, Samuele/0000-0002-3748-5115; Tomasi, Maurizio/0000-0002-1448-6131; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; Rubino-Martin, Jose Alberto/0000-0001-5289-3021; De Zotti, Gianfranco/0000-0003-2868-2595; Matarrese, Sabino/0000-0002-2573-1243; Valiviita, Jussi/0000-0001-6225-3693; Mazzotta, Pasquale/0000-0002-5411-1748; Kurki-Suonio, Hannu/0000-0002-4618-3063; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Gruppuso, Alessandro/0000-0001-9272-5292 FU ESA; CNES FX The development of Planck has been supported by: ESA; CNES and CNRS /INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER /SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT /MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.sciops.esa.int/index.php?project=planck&page=Planck_Collabora tion. The research leading to these results has received funding from the European Research Council under the European Union's Seventh Framework Programme (FP7 /2007-2013) /ERC grant agreement No. 267934. Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the US Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbuk agakusho, the Max Planck Society, and the Higher Education Funding Council for England. The SDSS web site is http://www.sdss.org/. The SDSS is managed by the Astrophysical Research Consortium for the Participating Institutions. The Participating Institutions are the American Museum of Natural History, Astrophysical Institute Potsdam, University of Basel, University of Cambridge, Case Western Reserve University, University of Chicago, Drexel University, Fermilab, the Institute for Advanced Study, the Japan Participation Group, Johns Hopkins University, the Joint Institute for Nuclear Astrophysics, the Kavli Institute for Particle Astrophysics and Cosmology, the Korean Scientist Group, the Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory, the Max-PlanckInstitute for Astronomy (MPIA), the Max-Planck-Institute for Astrophysics (MPA), New Mexico State University, Ohio State University, University of Pittsburgh, University of Portsmouth, Princeton University, the United States Naval Observatory, and the University of Washington. Some of the results in this paper have been derived using the HEALPix package. NR 142 TC 126 Z9 124 U1 4 U2 23 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A11 DI 10.1051/0004-6361/201323195 PG 37 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600034 ER PT J AU Ade, PAR Arnaud, M Ashdown, M Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Battaner, E Benabed, K Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bond, JR Borrill, J Bouchet, FR Burigana, C Cardoso, JF Catalano, A Challinor, A Chamballu, A Chiang, HC Christensen, PR Clements, DL Colombi, S Colombo, LPL Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Danese, L Davies, RD Davis, RJ de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Desert, FX Dickinson, C Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Dupac, X Ensslin, TA Eriksen, HK Finelli, F Forni, O Frailis, M Fraisse, AA Franceschi, E Galeotta, S Ganga, K Giard, M Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Gudmundsson, JE Hansen, FK Hanson, D Harrison, DL Henrot-Versille, S Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Jaffe, AH Jaffe, TR Jones, WC Keihanen, E Keskitalo, R Knoche, J Kunz, M Kurki-Suonio, H Lagache, G Lahteenmaki, A Lamarre, JM Lasenby, A Lawrence, CR Leonardi, R Leon-Tavares, J Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maino, D Mandolesi, N Maris, M Martin, PG Martinez-Gonzalez, E Masi, S Matarrese, S Mazzotta, P Meinhold, PR Melchiorri, A Mendes, L Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, MA Moneti, A Montier, L Morgante, G Mortlock, D Moss, A Munshi, D Murphy, JA Naselsky, P Nati, F Natoli, P Norgaard-Nielsen, HU Noviello, F Novikov, D Novikov, I Oxborrow, CA Pagano, L Pajot, F Paoletti, D Partridge, B Pasian, F Patanchon, G Pearson, D Pearson, TJ Perdereau, O Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Popa, L Pratt, GW Prunet, S Puget, JL Rachen, JP Reinecke, M Remazeilles, M Renault, C Ricciardi, S Ristorcelli, I Rocha, G Roudier, G Rubino-Martin, JA Rusholme, B Sandri, M Scott, D Stolyarov, V Sudiwala, R Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Valenziano, L Valiviita, J Van Tent, B Vielva, P Villa, F Wade, LA Wandelt, BD Wehus, IK White, SDM Yvon, D Zacchei, A Zonca, A AF Ade, P. A. R. Arnaud, M. Ashdown, M. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Battaner, E. Benabed, K. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bond, J. R. Borrill, J. Bouchet, F. R. Burigana, C. Cardoso, J. -F. Catalano, A. Challinor, A. Chamballu, A. Chiang, H. C. Christensen, P. R. Clements, D. L. Colombi, S. Colombo, L. P. L. Couchot, F. Coulais, A. Crill, B. P. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. Davis, R. J. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Desert, F. -X. Dickinson, C. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dupac, X. Ensslin, T. A. Eriksen, H. K. Finelli, F. Forni, O. Frailis, M. Fraisse, A. A. Franceschi, E. Galeotta, S. Ganga, K. Giard, M. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Gudmundsson, J. E. Hansen, F. K. Hanson, D. Harrison, D. L. Henrot-Versille, S. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Jaffe, A. H. Jaffe, T. R. Jones, W. C. Keihaenen, E. Keskitalo, R. Knoche, J. Kunz, M. Kurki-Suonio, H. Lagache, G. Lahteenmaki, A. Lamarre, J. -M. Lasenby, A. Lawrence, C. R. Leonardi, R. Leon-Tavares, J. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maino, D. Mandolesi, N. Maris, M. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Matarrese, S. Mazzotta, P. Meinhold, P. R. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Miville-Deschenes, M. -A. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Moss, A. Munshi, D. Murphy, J. A. Naselsky, P. Nati, F. Natoli, P. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novikov, I. Oxborrow, C. A. Pagano, L. Pajot, F. Paoletti, D. Partridge, B. Pasian, F. Patanchon, G. Pearson, D. Pearson, T. J. Perdereau, O. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Pratt, G. W. Prunet, S. Puget, J. -L. Rachen, J. P. Reinecke, M. Remazeilles, M. Renault, C. Ricciardi, S. Ristorcelli, I. Rocha, G. Roudier, G. Rubino-Martin, J. A. Rusholme, B. Sandri, M. Scott, D. Stolyarov, V. Sudiwala, R. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Valenziano, L. Valiviita, J. Van Tent, B. Vielva, P. Villa, F. Wade, L. A. Wandelt, B. D. Wehus, I. K. White, S. D. M. Yvon, D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. XXXI. Consistency of the Planck data SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE cosmology: observations; cosmic background radiation; instrumentation: detectors ID MICROWAVE; MAPS AB The Planck design and scanning strategy provide many levels of redundancy that can be exploited to provide tests of internal consistency. One of the most important is the comparison of the 70 GHz (amplifier) and 100 GHz (bolometer) channels. Based on different instrument technologies, with feeds located differently in the focal plane, analysed independently by different teams using different software, and near the minimum of diffuse foreground emission, these channels are in effect two different experiments. The 143 GHz channel has the lowest noise level on Planck, and is near the minimum of unresolved foreground emission. In this paper, we analyse the level of consistency achieved in the 2013 Planck data. We concentrate on comparisons between the 70, 100, and 143 GHz channel maps and power spectra, particularly over the angular scales of the first and second acoustic peaks, on maps masked for diffuse Galactic emission and for strong unresolved sources. Difference maps covering angular scales from 8 degrees to 15 ' are consistent with noise, and show no evidence of cosmic microwave background structure. Including small but important corrections for unresolved-source residuals, we demonstrate agreement (measured by deviation of the ratio from unity) between 70 and 100 GHz power spectra averaged over 70 <= l <= 390 at the 0.8% level, and agreement between 143 and 100 GHz power spectra of 0.4% over the same l range. These values are within and consistent with the overall uncertainties in calibration given in the Planck 2013 results. We also present results based on the 2013 likelihood analysis showing consistency at the 0.35% between the 100, 143, and 217 GHz power spectra. We analyse calibration procedures and beams to determine what fraction of these differences can be accounted for by known approximations or systematic errors that could be controlled even better in the future, reducing uncertainties still further. Several possible small improvements are described. Subsequent analysis of the beams quantifies the importance of asymmetry in the near sidelobes, which was not fully accounted for initially, affecting the 70/100 ratio. Correcting for this, the 70, 100, and 143 GHz power spectra agree to 0.4% over the first two acoustic peaks. The likelihood analysis that produced the 2013 cosmological parameters incorporated uncertainties larger than this. We show explicitly that correction of the missing near sidelobe power in the HFI channels would result in shifts in the posterior distributions of parameters of less than 0.3 sigma except for As, the amplitude of the primordial curvature perturbations at 0.05 Mpc(-1), which changes by about 1 sigma. We extend these comparisons to include the sky maps from the complete nine-year mission of the Wilkinson Microwave Anisotropy Probe (WMAP), and find a roughly 2% difference between the Planck and WMAP power spectra in the region of the first acoustic peak. 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F.; Renault, C.] Univ Grenoble 1, Inst Natl Polytech Grenoble, CNRS IN2P3, Lab Phys Subatom & Cosmol, F-38026 Grenoble, France. [Van Tent, B.] Univ Paris 11, Lab Phys Theor, CNRS, F-91405 Orsay, France. [Ensslin, T. A.; Hovest, W.; Knoche, J.; Rachen, J. P.; Reinecke, M.; White, S. D. M.] Max Planck Inst Astrophys, D-85741 Garching, Germany. [Hanson, D.] McGill Univ, McGill Phys, Montreal, PQ H3A 2T8, Canada. [Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Co Kildare, Ireland. [Christensen, P. R.; Naselsky, P.; Novikov, I.] Niels Bohr Inst, DK-2100 Copenhagen, Denmark. [Crill, B. P.] CALTECH, Observ Cosmol, Pasadena, CA 91125 USA. [Lesgourgues, J.] Ecole Polytech Fed Lausanne, SB ITP LPPC, CH-1015 Lausanne, Switzerland. [Baccigalupi, C.; Bielewicz, P.; Danese, L.; de Zotti, G.; Gonzalez-Nuevo, J.; Perrotta, F.] SISSA, Astrophys Sector, I-34136 Trieste, Italy. [Ade, P. A. R.; Munshi, D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, The Parade, Cardiff CF24 3AA, S Glam, Wales. [Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England. [Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA. [Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Karachai Cherkessian Rep 369167, Russia. [Lesgourgues, J.] CERN, PH TH, Div Theory, CH-1211 Geneva 23, Switzerland. [Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Colombi, S.; Hivon, E.; Prunet, S.; Wandelt, B. D.] Univ Paris 06, UMR7095, F-75014 Paris, France. [Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France. [Battaner, E.] Univ Granada, Dept Fis Teor & Cosmos, Fac Ciencias, E-18071 Granada, Spain. [Battaner, E.] Univ Granada, Inst Carlos Fis Teor & Computac I, E-18071 Granada, Spain. [Gorski, K. M.] Univ Warsaw Observ, PL-00478 Warsaw, Poland. RP Lawrence, CR (reprint author), CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91125 USA. EM charles.lawrence@jpl.nasa.gov RI Remazeilles, Mathieu/N-1793-2015; Kurki-Suonio, Hannu/B-8502-2016; Tomasi, Maurizio/I-1234-2016; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Stolyarov, Vladislav/C-5656-2017; Lahteenmaki, Anne/L-5987-2013; Toffolatti, Luigi/K-5070-2014; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Martinez-Gonzalez, Enrique/E-9534-2015; Mazzotta, Pasquale/B-1225-2016; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Pearson, Timothy/N-2376-2015; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Valiviita, Jussi/A-9058-2016; Barreiro, Rita Belen/N-5442-2014; OI de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Kurki-Suonio, Hannu/0000-0002-4618-3063; Tomasi, Maurizio/0000-0002-1448-6131; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Stolyarov, Vladislav/0000-0001-8151-828X; Rubino-Martin, Jose Alberto/0000-0001-5289-3021; Matarrese, Sabino/0000-0002-2573-1243; De Zotti, Gianfranco/0000-0003-2868-2595; Lopez-Caniego, Marcos/0000-0003-1016-9283; Masi, Silvia/0000-0001-5105-1439; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Mazzotta, Pasquale/0000-0002-5411-1748; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Pearson, Timothy/0000-0001-5213-6231; Gruppuso, Alessandro/0000-0001-9272-5292; Valiviita, Jussi/0000-0001-6225-3693; Pierpaoli, Elena/0000-0002-7957-8993; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Ricciardi, Sara/0000-0002-3807-4043; Villa, Fabrizio/0000-0003-1798-861X; TERENZI, LUCA/0000-0001-9915-6379; Galeotta, Samuele/0000-0002-3748-5115; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017 FU ESA; CNES (France) [CNRS/INSU-IN2P3-INP]; ASI (Italy); CNR (Italy); INAF (Italy); NASA and DoE (USA); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); DEISA (EU); STFC and UKSA (UK); CSIC, MICINN and JA (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany) FX The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN and JA (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and DEISA (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.rssd.esa.int/Planck. Some of the results in this paper have been derived using the HEALPix package. We acknowledge the use of the Legacy Archive for Microwave Background Data Analysis ( LAMBDA), part of the High Energy Astrophysics Science Archive Center (HEASARC); HEASARC/LAMBDA is a service of the Astrophysics Science Division at the NASA Goddard Space Flight Center. NR 35 TC 40 Z9 39 U1 3 U2 15 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A31 DI 10.1051/0004-6361/201423743 PG 25 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600045 ER PT J AU Ade, PAR Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Bartlett, JG Battaner, E Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bethermin, M Bielewicz, P Blagrave, K Bobin, J Bock, JJ Bonaldi, A Bond, JR Borrill, J Bouchet, FR Boulanger, F Bridges, M Bucher, M Burigana, C Butler, RC Cardoso, JF Catalano, A Challinor, A Chamballu, A Chen, X Chiang, HC Chiang, LY Christensen, PR Church, S Clements, DL Colombi, S Colombo, LPL Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Danese, L Davies, RD Davis, RJ de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Delouis, JM Desert, FX Dickinson, C Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Finelli, F Forni, O Frailis, M Franceschi, E Galeotta, S Ganga, K Ghosh, T Giard, M Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Hansen, FK Hanson, D Harrison, D Helou, G Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Jaffe, AH Jaffe, TR Jones, WC Juvela, M Kalberla, P Keihanen, E Kerp, J Keskitalo, R Kisner, TS Kneissl, R Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lacasa, F Lagache, G Lahteenmaki, A Lamarre, JM Langer, M Lasenby, A Laureijs, RJ Lawrence, CR Leonardi, R Leon-Tavares, J Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maffei, B Maino, D Mandolesi, N Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Mazzotta, P Melchiorri, A Mendes, L Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, MA Moneti, A Montier, L Morgante, G Mortlock, D Munshi, D Murphy, JA Naselsky, P Nati, F Natoli, P Netterfield, CB Norgaard-Nielsen, HU Noviello, F Novikov, D Novikov, I Osborne, S Oxborrow, CA Paci, F Pagano, L Pajot, F Paladini, R Paoletti, D Partridge, B Pasian, F Patanchon, G Perdereau, O Perotto, L Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Reach, WT Rebolo, R Reinecke, M Remazeilles, M Renault, C Ricciardi, S Riller, T Ristorcelli, I Rocha, G Rosset, C Roudier, G Rowan-Robinson, M Rubino-Martin, JA Rusholme, B Sandri, M Santos, D Savini, G Scott, D Seiffert, MD Serra, P Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sunyaev, R Sureau, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Tuovinen, J Turler, M Valenziano, L Valiviita, J Van Tent, B Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD Welikala, N White, M White, SDM Winkel, B Yvon, D Zacchei, A Zonca, A AF Ade, P. A. R. Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Bartlett, J. G. Battaner, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bethermin, M. Bielewicz, P. Blagrave, K. Bobin, J. Bock, J. J. Bonaldi, A. Bond, J. R. Borrill, J. Bouchet, F. R. Boulanger, F. Bridges, M. Bucher, M. Burigana, C. Butler, R. C. Cardoso, J. -F. Catalano, A. Challinor, A. Chamballu, A. Chen, X. Chiang, H. C. Chiang, L. -Y Christensen, P. R. Church, S. Clements, D. L. Colombi, S. Colombo, L. P. L. Couchot, F. Coulais, A. Crill, B. P. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. Davis, R. J. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Delouis, J. -M. Desert, F. -X. Dickinson, C. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Finelli, F. Forni, O. Frailis, M. Franceschi, E. Galeotta, S. Ganga, K. Ghosh, T. Giard, M. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Hansen, F. K. Hanson, D. Harrison, D. Helou, G. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Jaffe, A. H. Jaffe, T. R. Jones, W. C. Juvela, M. Kalberla, P. Keihanen, E. Kerp, J. Keskitalo, R. Kisner, T. S. Kneissl, R. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lacasa, F. Lagache, G. Lahteenmaki, A. Lamarre, J. -M. Langer, M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leonardi, R. Leon-Tavares, J. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maffei, B. Maino, D. Mandolesi, N. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Miville-Deschenes, M. -A. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Munshi, D. Murphy, J. A. Naselsky, P. Nati, F. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novikov, I. Osborne, S. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paladini, R. Paoletti, D. Partridge, B. Pasian, F. Patanchon, G. Perdereau, O. Perotto, L. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Reach, W. T. Rebolo, R. Reinecke, M. Remazeilles, M. Renault, C. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Rosset, C. Roudier, G. Rowan-Robinson, M. Rubino-Martin, J. A. Rusholme, B. Sandri, M. Santos, D. Savini, G. Scott, D. Seiffert, M. D. Serra, P. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sunyaev, R. Sureau, F. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Tuovinen, J. Tuerler, M. Valenziano, L. Valiviita, J. Van Tent, B. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. Welikala, N. White, M. White, S. D. M. Winkel, B. Yvon, D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE cosmology: observations; large-scale structure of Universe; galaxies: star formation; infrared: diffuse background ID FORMATION RATE DENSITY; SOUTH-POLE TELESCOPE; DARK-MATTER HALOES; CONDITIONAL LUMINOSITY FUNCTION; SPECTRAL ENERGY-DISTRIBUTIONS; ANGULAR POWER SPECTRA; SIMILAR-TO 2; 100 MU-M; SUBMILLIMETER GALAXIES; FORMING GALAXIES AB We present new measurements of cosmic infrared background (CIB) anisotropies using Planck. Combining HFI data with IRAS, the angular auto-and cross-frequency power spectrum is measured from 143 to 3000 GHz, and the auto-bispectrum from 217 to 545 GHz. The total areas used to compute the CIB power spectrum and bispectrum are about 2240 and 4400 deg(2), respectively. After careful removal of the contaminants (cosmic microwave background anisotropies, Galactic dust, and Sunyaev-Zeldovich emission), and a complete study of systematics, the CIB power spectrum is measured with unprecedented signal to noise ratio from angular multipoles l similar to 150 to 2500. The bispectrum due to the clustering of dusty, star-forming galaxies is measured from l similar to 130 to 1100, with a total signal to noise ratio of around 6, 19, and 29 at 217, 353, and 545 GHz, respectively. Two approaches are developed for modelling CIB power spectrum anisotropies. The first approach takes advantage of the unique measurements by Planck at large angular scales, and models only the linear part of the power spectrum, with a mean bias of dark matter haloes hosting dusty galaxies at a given redshift weighted by their contribution to the emissivities. The second approach is based on a model that associates star-forming galaxies with dark matter haloes and their subhaloes, using a parametrized relation between the dust-processed infrared luminosity and (sub-) halo mass. The two approaches simultaneously fit all auto-and cross-power spectra very well. We find that the star formation history is well constrained up to redshifts around 2, and agrees with recent estimates of the obscured star-formation density using Spitzer and Herschel. However, at higher redshift, the accuracy of the star formation history measurement is strongly degraded by the uncertainty in the spectral energy distribution of CIB galaxies. We also find that the mean halo mass which is most efficient at hosting star formation is log (M-eff/ M-circle dot) = 12.6 and that CIB galaxies have warmer temperatures as redshift increases. The CIB bispectrum is steeper than that expected from the power spectrum, although well fitted by a power law; this gives some information about the contribution of massive haloes to the CIB bispectrum. Finally, we show that the same halo occupation distribution can fit all power spectra simultaneously. The precise measurements enabled by Planck pose new challenges for the modelling of CIB anisotropies, indicating the power of using CIB anisotropies to understand the process of galaxy formation. C1 [Bartlett, J. G.; Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Piat, M.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.; Welikala, N.] Univ Paris Diderot, Sorbonne Paris Cite, APC, CNRS IN2P3,CEA Lrfu,Observ Paris, F-75205 Paris 13, France. [Lahteenmaki, A.; Leon-Tavares, J.; Poutanen, T.] Aalto Univ, Metsahovi Radio Observ, Kylmala 02540, Finland. [Kunz, M.] African Inst Math Sci, ZA-7945 Cape Town, South Africa. [Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana Sci Data Ctr, I-00133 Rome, Italy. [Mandolesi, N.] Agenzia Spaziale Italiana, Rome, Italy. [Kalberla, P.; Kerp, J.; Winkel, B.] Univ Bonn, Argelander Inst Astron, D-53121 Bonn, Germany. [Ashdown, M.; Bridges, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 0HE, England. [Chiang, H. C.] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, ZA-4000 Durban, South Africa. [Kneissl, R.] ALMA Santiago Cent Off, Atacama Large Millimeter Submillimeter Array, Santiago 0355, Chile. [Blagrave, K.; Bond, J. R.; Hanson, D.; Martin, P. G.; Miville-Deschenes, M. -A.] Univ Toronto, CITA, Toronto, ON M5S 3H8, Canada. [Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] CNRS, IRAP, F-31028 Toulouse 4, France. [Bock, J. J.; Dore, O.; Helou, G.; Hildebrandt, S. R.; Prezeau, G.; Rocha, G.; Seiffert, M. D.] CALTECH, Pasadena, CA 91125 USA. [Challinor, A.; Shellard, E. P. S.] Univ Cambridge, DAMTP, Ctr Theoret Cosmol, Cambridge CB3 0WA, England. [Hernandez-Monteagudo, C.] CEFCA, Teruel 44001, Spain. [Borrill, J.; Keskitalo, R.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 94720 USA. CSIC, Madrid 28049, Spain. [Chamballu, A.; Yvon, D.] CEA Saclay, DSM Irfu SPP, F-91191 Gif Sur Yvette, France. [Hornstrup, A.; Linden-Vornle, M.; Norgaard-Nielsen, H. U.; Oxborrow, C. A.] Tech Univ Denmark, Natl Space Inst, DTU Space, DK-2800 Lyngby, Denmark. [Kunz, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, CH-1211 Geneva 4, Switzerland. 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EM guilaine.lagache@ias.u-psud.fr RI Butler, Reginald/N-4647-2015; Barreiro, Rita Belen/N-5442-2014; SERRA, PAOLO/G-9678-2014; Remazeilles, Mathieu/N-1793-2015; Mazzotta, Pasquale/B-1225-2016; Kurki-Suonio, Hannu/B-8502-2016; Ghosh, Tuhin/E-6899-2016; Tomasi, Maurizio/I-1234-2016; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Valiviita, Jussi/A-9058-2016; Lahteenmaki, Anne/L-5987-2013; Toffolatti, Luigi/K-5070-2014; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Langer, Mathieu/C-5100-2013; Martinez-Gonzalez, Enrique/E-9534-2015; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; White, Martin/I-3880-2015 OI Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Savini, Giorgio/0000-0003-4449-9416; Bethermin, Matthieu/0000-0002-3915-2015; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; Reach, William/0000-0001-8362-4094; Butler, Reginald/0000-0003-4366-5996; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Ricciardi, Sara/0000-0002-3807-4043; Villa, Fabrizio/0000-0003-1798-861X; Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834; Galeotta, Samuele/0000-0002-3748-5115; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; SERRA, PAOLO/0000-0002-7609-3931; Lopez-Caniego, Marcos/0000-0003-1016-9283; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Mazzotta, Pasquale/0000-0002-5411-1748; Kurki-Suonio, Hannu/0000-0002-4618-3063; Tomasi, Maurizio/0000-0002-1448-6131; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; Rubino-Martin, Jose Alberto/0000-0001-5289-3021; De Zotti, Gianfranco/0000-0003-2868-2595; Gruppuso, Alessandro/0000-0001-9272-5292; Valiviita, Jussi/0000-0001-6225-3693; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; Langer, Mathieu/0000-0002-9088-2718; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; White, Martin/0000-0001-9912-5070 FU ESA; CNES FX The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP-PNCG (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN and JA (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members with the technical or scientific activities they have been involved into, can be found at http://www.rssd.esa.int/index.php?project=PLANCK&page=PlanckCollaboratio n. The Parkes radio telescope is part of the Australia Telescope National Facility which is funded by the Commonwealth of Australia for operation as a National Facility managed by CSIRO. Some Hi data used in this paper are based on observations with the 100 m telescope of the MPIfR (Max-Planck-Institut fur Radioastronomie) at Effelsberg. NR 162 TC 74 Z9 73 U1 3 U2 14 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A30 DI 10.1051/0004-6361/201322093 PG 39 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600030 ER PT J AU Ade, PAR Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Bartlett, JG Battaner, E Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bonaldi, A Bonavera, L Bond, JR Borrill, J Bouchet, FR Boulanger, F Bridges, M Bucher, M Burigana, C Butler, RC Cardoso, JF Castex, G Catalano, A Challinor, A Chamballu, A Chary, RR Chen, X Chiang, HC Chiang, LY Christensen, PR Church, S Clements, DL Colombi, S Colombo, LPL Couchot, F Coulais, A Crill, BP Cruz, M Curto, A Cuttaia, F Danese, L Davies, RD Davis, RJ de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Delouis, JM Desert, FX Dickinson, C Diego, JM Dobler, G Dole, H Donzelli, S Dore, O Douspis, M Dunkley, J Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Falgarone, E Finelli, F Forni, O Frailis, M Fraisse, AA Franceschi, E Galeotta, S Ganga, K Giard, M Giardino, G Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Hansen, FK Hanson, D Harrison, DL Helou, G Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huey, G Huffenberger, KM Jaffe, AH Jaffe, TR Jewell, J Jones, WC Juvela, M Keihanen, E Keskitalo, R Kisner, TS Kneissl, R Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lahteenmaki, A Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Le Jeune, M Leach, S Leahy, JP Leonardi, R Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maffei, B Maino, D Mandolesi, N Marcos-Caballero, A Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Mazzotta, P Meinhold, PR Melchiorri, A Mendes, L Mennella, A Migliaccio, M Mikkelsen, K Mitra, S Miville-Deschenes, MA Molinari, D Moneti, A Montier, L Morgante, G Mortlock, D Moss, A Munshi, D Murphy, JA Naselsky, P Nati, F Natoli, P Netterfield, CB Norgaard-Nielsen, HU Noviello, F Novikov, D Novikov, I O'Dwyer, IJ Osborne, S Oxborrow, CA Paci, F Pagano, L Pajot, F Paladini, R Paoletti, D Partridge, B Pasian, F Patanchon, G Pearson, TJ Perdereau, O Perotto, L Perrotta, F Pettorino, V Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Platania, P Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Reach, WT Rebolo, R Reinecke, M Remazeilles, M Renault, C Renzi, A Ricciardi, S Riller, T Ristorcelli, I Rocha, G Roman, M Rosset, C Roudier, G Rowan-Robinson, M Rubino-Martin, JA Rusholme, B Salerno, E Sandri, M Santos, D Savini, G Schiavon, F Scott, D Seiffert, MD Shellard, EPS Spencer, LD Starck, JL Stompor, R Sudiwala, R Sunyaev, R Sureau, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Tuovinen, J Turler, M Umana, G Valenziano, L Valiviita, J Van Tent, B Varis, J Viel, M Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD Wehus, IK Wilkinson, A Xia, JQ Yvon, D Zacchei, A Zonca, A AF Ade, P. 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A. Franceschi, E. Galeotta, S. Ganga, K. Giard, M. Giardino, G. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Hansen, F. K. Hanson, D. Harrison, D. L. Helou, G. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huey, G. Huffenberger, K. M. Jaffe, A. H. Jaffe, T. R. Jewell, J. Jones, W. C. Juvela, M. Keihanen, E. Keskitalo, R. Kisner, T. S. Kneissl, R. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Lahteenmaki, A. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Le Jeune, M. Leach, S. Leahy, J. P. Leonardi, R. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maffei, B. Maino, D. Mandolesi, N. Marcos-Caballero, A. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. Meinhold, P. R. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Mikkelsen, K. Mitra, S. Miville-Deschenes, M. -A. Molinari, D. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Moss, A. Munshi, D. Murphy, J. A. Naselsky, P. Nati, F. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novikov, I. O'Dwyer, I. J. Osborne, S. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paladini, R. Paoletti, D. Partridge, B. Pasian, F. Patanchon, G. Pearson, T. J. Perdereau, O. Perotto, L. Perrotta, F. Pettorino, V. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Platania, P. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Reach, W. T. Rebolo, R. Reinecke, M. Remazeilles, M. Renault, C. Renzi, A. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Roman, M. Rosset, C. Roudier, G. Rowan-Robinson, M. Rubino-Martin, J. A. Rusholme, B. Salerno, E. Sandri, M. Santos, D. Savini, G. Schiavon, F. Scott, D. Seiffert, M. D. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stompor, R. Sudiwala, R. Sunyaev, R. Sureau, F. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Tuovinen, J. Tuerler, M. Umana, G. Valenziano, L. Valiviita, J. Van Tent, B. Varis, J. Viel, M. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. Wehus, I. K. Wilkinson, A. Xia, J. -Q. Yvon, D. Zacchei, A. Zonca, A. TI Planck 2013 results. XII. Diffuse component separation SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE cosmic background radiation ID MICROWAVE-ANISOTROPY-PROBE; INTERSTELLAR-MEDIUM EMISSION; TEMPERATURE POWER SPECTRUM; SPINNING DUST; FOREGROUND EMISSION; FULL-SKY; GALACTIC EMISSION; WMAP OBSERVATIONS; POLARIZATION DATA; LIKELIHOOD AB Planck has produced detailed all-sky observations over nine frequency bands between 30 and 857 GHz. These observations allow robust reconstruction of the primordial cosmic microwave background (CMB) temperature fluctuations over nearly the full sky, as well as new constraints on Galactic foregrounds, including thermal dust and line emission from molecular carbon monoxide (CO). This paper describes the component separation framework adopted by Planck for many cosmological analyses, including CMB power spectrum determination and likelihood construction on large angular scales, studies of primordial non-Gaussianity and statistical isotropy, the integrated Sachs-Wolfe effect, gravitational lensing, and searches for topological defects. We test four foreground-cleaned CMB maps derived using qualitatively different component separation algorithms. The quality of our reconstructions is evaluated through detailed simulations and internal comparisons, and shown through various tests to be internally consistent and robust for CMB power spectrum and cosmological parameter estimation up to l = 2000. The parameter constraints on ACDM cosmologies derived from these maps are consistent with those presented in the cross-spectrum based Planck likelihood analysis. We choose two of the CMB maps for specific scientific goals. We also present maps and frequency spectra of the Galactic low-frequency, CO, and thermal dust emission. The component maps are found to provide a faithful representation of the sky, as evaluated by simulations, with the largest bias seen in the CO component at 3%. For the low-frequency component, the spectral index varies widely over the sky, ranging from about beta = 4 to -2. Considering both morphology and prior knowledge of the low frequency components, the index map allows us to associate a steep spectral index (beta < -3.2) with strong anomalous microwave emission, corresponding to a spinning dust spectrum peaking below 20 GHz, a flat index of beta > -2.3 with strong free-free emission, and intermediate values with synchrotron emission. C1 [Bartlett, J. G.; Bucher, M.; Cardoso, J. -F.; Castex, G.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Le Jeune, M.; Patanchon, G.; Piat, M.; Remazeilles, M.; Roman, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, Univ Paris 04, APC, CNRS IN2P3,CEA Lrfu,Observ Paris, F-75205 Paris 13, France. [Lahteenmaki, A.; Poutanen, T.] Aalto Univ, Metsahovi Radio Observ, Aalto 00076, Finland. [Lahteenmaki, A.; Poutanen, T.] Aalto Univ, Dept Radio Sci & Engn, Aalto 00076, Finland. [Kunz, M.] African Inst Math Sci, ZA-7945 Cape Town, South Africa. 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EM maja1@mrao.cam.ac.uk RI Renzi, Alessandro/K-4114-2015; Barreiro, Rita Belen/N-5442-2014; Remazeilles, Mathieu/N-1793-2015; Valiviita, Jussi/A-9058-2016; Mazzotta, Pasquale/B-1225-2016; Kurki-Suonio, Hannu/B-8502-2016; Tomasi, Maurizio/I-1234-2016; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; bonavera, laura/E-9368-2017; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Lahteenmaki, Anne/L-5987-2013; Toffolatti, Luigi/K-5070-2014; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Cruz, Marcos/N-3429-2014; Martinez-Gonzalez, Enrique/E-9534-2015; Salerno, Emanuele/A-2137-2010; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Pearson, Timothy/N-2376-2015; Butler, Reginald/N-4647-2015; OI Renzi, Alessandro/0000-0001-9856-1970; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Viel, Matteo/0000-0002-2642-5707; Galeotta, Samuele/0000-0002-3748-5115; Ricciardi, Sara/0000-0002-3807-4043; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Rubino-Martin, Jose Alberto/0000-0001-5289-3021; De Zotti, Gianfranco/0000-0003-2868-2595; Lopez-Caniego, Marcos/0000-0003-1016-9283; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Maris, Michele/0000-0001-9442-2754; Valiviita, Jussi/0000-0001-6225-3693; Mazzotta, Pasquale/0000-0002-5411-1748; Kurki-Suonio, Hannu/0000-0002-4618-3063; Tomasi, Maurizio/0000-0002-1448-6131; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; bonavera, laura/0000-0001-8039-3876; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Savini, Giorgio/0000-0003-4449-9416; Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; Reach, William/0000-0001-8362-4094; Molinari, Diego/0000-0002-7799-3915; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Gruppuso, Alessandro/0000-0001-9272-5292; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; Cruz, Marcos/0000-0002-4767-530X; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Salerno, Emanuele/0000-0002-3433-3634; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Pearson, Timothy/0000-0001-5213-6231; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Villa, Fabrizio/0000-0003-1798-861X; Umana, Grazia/0000-0002-6972-8388; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Butler, Reginald/0000-0003-4366-5996; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099 FU ESA; CNES; CNRS/INSU-IN2P3-INP (France); ASI; CNR; INAF (Italy); NASA; DoE (USA); STFC; UKSA (UK); CSIC; MICINN; JA; RES (Spain); Tekes; AoF; CSC (Finland); DLR; MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); PRACE (EU); Advanced Computing and e-Science team at IFCA FX The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.sciops.esa.int/index.php? project=planck&page=Planck_Collaboration. The authors acknowledge the support provided by the Advanced Computing and e-Science team at IFCA. This work made use of the COSMOS supercomputer, part of the STFC DiRAC HPC Facility. Some of the results in this paper have been derived using the HEALPix package. NR 90 TC 136 Z9 136 U1 9 U2 24 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A12 DI 10.1051/0004-6361/201321580 PG 31 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600026 ER PT J AU Ade, PAR Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Battaner, E Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bond, JR Borrill, J Bouchet, FR Bridges, M Bucher, M Burigana, C Cardoso, JF Catalano, A Challinor, A Chamballu, A Chiang, HC Chiang, LY Christensen, PR Church, S Clements, DL Colombi, S Colombo, LPL Couchot, F Coulais, A Crill, P Curto, A Cuttaia, F Danese, L Davies, RD de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Delouis, JM Desert, FX Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Finelli, F Forni, O Frailis, M Franceschi, E Galeotta, S Gana, K Giard, M Girard, D Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Hansen, FK Hanson, D Harrison, D Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Jaffe, AH Jaffe, TR Jones, WC Juvela, M Keihanen, E Keskitalo, R Kisner, TS Kneissl, R Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Leonardi, R Leroy, C Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Mandolesi, N Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Mazzotta, P McGehee, P Melchiorri, A Mendes, L Mennella, A Migliaccio, M Miniussi, A Mitra, A Miville-Deschenes, MA Moneti, A Montier, L Morgante, G Mortlock, D Mottet, S Munshi, D Murphy, JA Naselsky, P Nati, F Natoli, P Netterfield, CB Norgaard-Nielsen, HU Noviello, F Novikov, D Novikov, I Osborne, S Oxborrow, CA Paci, F Pagano, L Pajot, F Paoletti, D Pasian, F Patanchon, G Perdereau, O Perotto, L Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Racine, B Reinecke, M Remazeilles, M Renault, C Ricciardi, S Riller, T Ristorcelli, I Rocha, G Rosset, C Roudier, G Rusholme, B Sanselme, L Santos, D Sauve, A Savini, G Scott, D Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sureau, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Umana, G Valenziano, L Valiviita, J Van Tent, B Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD Yvon, D Zacchei, A Zonca, A AF Ade, P. A. R. Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Battaner, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bond, J. R. Borrill, J. Bouchet, F. R. Bridges, M. Bucher, M. Burigana, C. Cardoso, J. -F. Catalano, A. Challinor, A. Chamballu, A. Chiang, H. C. Chiang, L. -Y. Christensen, P. R. Church, S. Clements, D. L. Colombi, S. Colombo, L. P. L. Couchot, F. Coulais, A. Crill, P. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Delouis, J. -M. Desert, F. -X. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Finelli, F. Forni, O. Frailis, M. Franceschi, E. Galeotta, S. Gana, K. Giard, M. Girard, D. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Hansen, F. K. Hanson, D. Harrison, D. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Jaffe, A. H. Jaffe, T. R. Jones, W. C. Juvela, M. Keihanen, E. Keskitalo, R. Kisner, T. S. Kneissl, R. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leonardi, R. Leroy, C. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Mandolesi, N. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. McGehee, P. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Miniussi, A. Mitra, A. Miville-Deschenes, M. -A. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Mottet, S. Munshi, D. Murphy, J. A. Naselsky, P. Nati, F. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novikov, I. Osborne, S. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paoletti, D. Pasian, F. Patanchon, G. Perdereau, O. Perotto, L. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Racine, B. Reinecke, M. Remazeilles, M. Renault, C. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Rosset, C. Roudier, G. Rusholme, B. Sanselme, L. Santos, D. Sauve, A. Savini, G. Scott, D. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sureau, F. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Umana, G. Valenziano, L. Valiviita, J. Van Tent, B. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. Yvon, D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. X. HFI energetic particle effects: characterization, removal, and simulation SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE cosmic background radiation; cosmology: observations; instrumentation: detectors; space vehicles: instruments; methods: data analysis ID INSTRUMENT; ANISOTROPY; BOOMERANG; FLIGHT AB We describe the detection, interpretation, and removal of the signal resulting from interactions of high energy particles with the Planck High Frequency Instrument (HFI). There are two types of interactions: heating of the 0.1 K bolometer plate; and glitches in each detector time stream. The transient responses to detector glitch shapes are not simple single- pole exponential decays and fall into three families. The glitch shape for each family has been characterized empirically in flight data and these shapes have been used to remove glitches from the detector time streams. The spectrum of the count rate per unit energy is computed for each family and a correspondence is made to the location on the detector of the particle hit. Most of the detected glitches are from Galactic protons incident on the die frame supporting the micro- machined bolometric detectors. In the Planck orbit at L2, the particle flux is around 5 cm 2 s 1 and is dominated by protons incident on the spacecraft with energy > 39 MeV, at a rate of typically one event per second per detector. Di ff erent categories of glitches have di ff erent signatures in the time stream. Two of the glitch types have a low amplitude component that decays over nearly 1 s. This component produces excess noise if not properly removed from the time- ordered data. We have used a glitch detection and subtraction method based on the joint fit of population templates. The application of this novel glitch subtraction method removes excess noise from the time streams. 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[McGehee, P.; Rusholme, B.] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA. [Benoit, A.] Univ Grenoble 1, CNRS, Inst Neel, F-38042 Grenoble, France. [Dole, H.] Inst Univ France, F-75005 Paris, France. [Aghanim, N.; Aumont, J.; Chamballu, A.; Dole, H.; Douspis, M.; Kunz, M.; Lagache, G.; Leroy, C.; Miniussi, A.; Miville-Deschenes, M. -A.; Pajot, F.; Ponthieu, N.; Puget, J. -L.; Remazeilles, M.] Univ Paris 11, CNRS, Inst Astrophys Spatiale, UMR 8617, F-91405 Orsay, France. [Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Cardoso, J. -F.; Colombi, S.; Delouis, J. -M.; Hivon, E.; Moneti, A.; Mottet, S.; Prunet, S.; Sygnet, J. -F.; Wandelt, B. D.] CNRS, Inst Astrophys Paris, UMR 7095, F-75014 Paris, France. [Popa, L.] Inst Space Sci, Bucharest 077125, Romania. [Chiang, L. -Y.] Acad Sinica, Inst Astron & Astrophys, Taipei 10617, Taiwan. [Bridges, M.; Challinor, A.; Efstathiou, G.; Gratton, S.; Harrison, D.; Migliaccio, M.; Sutton, D.] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England. [Eriksen, H. K.; Hansen, F. K.; Lilje, P. B.; Valiviita, J.] Univ Oslo, Inst Theoret Astrophys, N-0315 Oslo, Norway. [Barreiro, R. B.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Toffolatti, L.; Vielva, P.] Univ Cantabria, CSIC, Inst Fis Cantabria, Santander 39005, Spain. [Bock, J. J.; Colombo, L. P. L.; Crill, P.; Dore, O.; Gorski, K. M.; Hanson, D.; Holmes, W. A.; Lawrence, C. R.; Mitra, A.; Pietrobon, D.; Prezeau, G.; Rocha, G.; Roudier, G.; Wade, L. A.] CALTECH, Jet Prop Lab, Pasadena, CA USA. [Davies, R. D.; Noviello, F.; Remazeilles, M.] Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Manchester M13 9PL, Lancs, England. [Ashdown, M.; Bridges, M.; Challinor, A.; Gratton, S.; Harrison, D.; Lasenby, A.; Migliaccio, M.; Stolyarov, V.; Sutton, D.] Cosmol Cambridge, Kavli Inst, Cambridge CB3 0HA, England. [Couchot, F.; Henrot-Versille, S.; Perdereau, O.; Plaszczynski, S.; Tristram, M.; Tucci, M.] Univ Paris 11, CNRS, IN2P3, LAL, Orsay, France. [Catalano, A.; Coulais, A.; Lamarre, J. -M.; Roudier, G.] Observ Paris, CNRS, LERMA, F-75014 Paris, France. [Arnaud, M.; Bobin, J.; Chamballu, A.; Marshall, D. J.; Pratt, G. W.; Starck, J. -L.; Sureau, F.] Univ Paris Diderot, CEA Saclay, CNRS, CEA DSM,IRFU,Serv Astrophys,Lab AIM, F-91191 Gif Sur Yvette, France. [Cardoso, J. -F.] CNRS, Lab Traitement & Commun Informat, UMR 5141, F-75634 Paris 13, France. [Cardoso, J. -F.] Telecom Paris Tech, F-75634 Paris 13, France. [Catalano, A.; Girard, D.; Macias-Perez, J. F.; Perotto, L.; Renault, C.; Sanselme, L.; Santos, D.] Univ Grenoble 1, CNRS, IN2P3, Inst Natl Polytech Grenoble,Lab Phys Subatom & Co, F-38026 Grenoble, France. [Van Tent, B.] Univ Paris 11, CNRS, Phys Theor Lab, F-91405 Orsay, France. [Kisner, T. S.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Ensslin, T. A.; Hernandez-Monteagudo, C.; Hovest, W.; Knoche, J.; Matthai, F.; Reinecke, M.; Riller, T.] Max Planck Inst Astrophys, D-85741 Garching, Germany. [Hanson, D.] McGill Univ, McGill Phys, Montreal, PQ H3A 2T8, Canada. [Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Co Kildare, Ireland. [Christensen, P. R.; Naselsky, P.; Novikov, I.] Niels Bohr Inst, DK-2100 Copenhagen, Denmark. [Crill, P.] CALTECH, Pasadena, CA 91125 USA. [Savini, G.] UCL, Opt Sci Lab, London, England. [Lesgourgues, J.] Ecole Polytech Fed Lausanne, SB ITP LPPC, CH-1015 Lausanne, Switzerland. [Baccigalupi, C.; Bielewicz, P.; Danese, L.; de Zotti, G.; Gonzalez-Nuevo, J.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sect, I-34136 Trieste, Italy. [Ade, P. A. R.; Munshi, D.; Spencer, L. D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales. [Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA. [Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Karachai Cherkessian Rep 369167, Zelenchukskiy R, Russia. [Church, S.; Osborne, S.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA. [Armitage-Caplan, C.] Univ Oxford, Sub Dept Astrophys, Oxford OX1 3RH, England. [Lesgourgues, J.] CERN, PH TH, Div Theory, CH-1211 Geneva, Switzerland. [Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Colombi, S.; Delouis, J. -M.; Hivon, E.; Prunet, S.; Wandelt, B. D.] Univ Paris 06, UMR 7095, F-75014 Paris, France. [Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Leroy, C.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.; Sauve, A.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France. [Battaner, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, Granada, Spain. [Gorski, K. M.] Univ Warsaw Observ, PL-00478 Warsaw, Poland. RP Patanchon, G (reprint author), Univ Paris Diderot, Sorbonne Paris Cite, CNRS, IN2P3,CEA Irfu,Observ Paris,APC, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France. EM patanchon@apc.univ-paris-Diderot.fr RI Barreiro, Rita Belen/N-5442-2014; Remazeilles, Mathieu/N-1793-2015; Tomasi, Maurizio/I-1234-2016; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; Martinez-Gonzalez, Enrique/E-9534-2015; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Valiviita, Jussi/A-9058-2016; Mazzotta, Pasquale/B-1225-2016; Kurki-Suonio, Hannu/B-8502-2016; Toffolatti, Luigi/K-5070-2014; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; OI Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Umana, Grazia/0000-0002-6972-8388; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Lopez-Caniego, Marcos/0000-0003-1016-9283; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Remazeilles, Mathieu/0000-0001-9126-6266; Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Galeotta, Samuele/0000-0002-3748-5115; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Tomasi, Maurizio/0000-0002-1448-6131; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; De Zotti, Gianfranco/0000-0003-2868-2595; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Gruppuso, Alessandro/0000-0001-9272-5292; Valiviita, Jussi/0000-0001-6225-3693; Mazzotta, Pasquale/0000-0002-5411-1748; Kurki-Suonio, Hannu/0000-0002-4618-3063; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; Pierpaoli, Elena/0000-0002-7957-8993; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Savini, Giorgio/0000-0003-4449-9416; Bouchet, Francois/0000-0002-8051-2924; Ricciardi, Sara/0000-0002-3807-4043; Villa, Fabrizio/0000-0003-1798-861X; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794 FU ESA FX Planck is a project of the European Space Agency ESA -with instruments provided by two scientific Consortia funded by ESA member states (in particular the lead countries: France and Italy) with contributions from NASA (USA), and telescope reflectors provided in a collaboration between ESA and a scientific Consortium led and funded by Denmark. The development of Planck has been supported by: ESA; CNES and CNRS / INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER / SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT / MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at h t t p : / / w w w. s c i o p s. e s a. i n t / i n d e x. p h p ? p r o j e c t = p l a n c k & p a g e = P l a n c k _ C o l l a b o r a t i o n NR 54 TC 40 Z9 39 U1 3 U2 12 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A10 DI 10.1051/0004-6361/201321577 PG 23 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600025 ER PT J AU Ade, PAR Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Battaner, E Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bond, JR Borrill, J Bouchet, FR Boulanger, F Bowyer, JW Bridges, M Bucher, M Burigana, C Cardoso, JF Catalano, A Chamballu, A Chary, RR Chen, X Chiang, HC Chiang, LY Christensen, PR Church, S Clements, DL Colombi, S Colombo, LPL Combet, C Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Danese, L Davies, RD Davis, RJ de Bernardis, P de Rose, A de Zotti, G Delabrouille, J Delouis, JM Desert, FX Dickinson, C Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Dunkley, J Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Finelli, F Forni, O Frailis, M Fraisse, AA Franceschi, E Galeotta, S Ganga, K Giard, M Giardino, G Girard, D Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Gudmundsson, JE Hansen, FK Hanson, D Harrison, D Helou, G Henrot-Versille, S Herent, O Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hou, Z Hovest, W Huffenberger, KM Hurier, G Jaffe, AH Jaffe, TR Jones, WC Juvela, M Keihanen, E Keskitalo, R Kisner, TS Kneissl, R Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Le Jaune, M Leonardi, R Leroy, C Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF MacTavish, CJ Maffei, B Mandolesi, N Maris, M Marleau, F Marshall, J Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Mazzotta, P McGehee, P Meinhold, PR Melchiorri, A Melot, F Mendes, L Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, MA Moneti, A Montier, L Morgante, G Mortlock, D Mottet, S Munshi, D Murphy, JA Naselsky, P Nati, F Natoli, P Netterfield, CB Norgaard-Nielsen, HU North, C Noviello, F Novikov, D Novikov, I Orieux, F Osborne, S Oxborrow, CA Paci, F Pagano, L Pajot, F Paladini, R Paoletti, D Pasian, F Patanchon, G Perdereaun, O Perotto, L Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Racine, B Reach, WT Rebolo, R Reinecke, M Remazeilles, M Renault, C Ricciardi, S Riller, T Ristorcelli, I Rocha, G Rosset, C Roudier, G Rowan-Robinson, M Rusholme, B Sanselme, L Santos, D Sauve, A Savini, G Scott, D Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sureae, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Techene, S Terenzi, L Tomasi, M Tristram, M Tucci, M Umana, G Valenziano, L Valiviita, J Van Tent, B Vibert, L Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD White, SDM Yvon, D Zacchei, A Zonca, A AF Ade, P. A. R. Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Battaner, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bond, J. R. Borrill, J. Bouchet, F. R. Boulanger, F. Bowyer, J. W. Bridges, M. Bucher, M. Burigana, C. Cardoso, J. -F. Catalano, A. Chamballu, A. Chary, R. -R. Chen, X. Chiang, H. C. Chiang, L. -Y Christensen, P. R. Church, S. Clements, D. L. Colombi, S. Colombo, L. P. L. Combet, C. Couchot, F. Coulais, A. Crill, B. P. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. Davis, R. J. de Bernardis, P. de Rose, A. de Zotti, G. Delabrouille, J. Delouis, J. -M. Desert, F. -X. Dickinson, C. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dunkley, J. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Finelli, F. Forni, O. Frailis, M. Fraisse, A. A. Franceschi, E. Galeotta, S. Ganga, K. Giard, M. Giardino, G. Girard, D. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Gudmundsson, J. E. Hansen, F. K. Hanson, D. Harrison, D. Helou, G. Henrot-Versille, S. Herent, O. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hou, Z. Hovest, W. Huffenberger, K. M. Hurier, G. Jaffe, A. H. Jaffe, T. R. Jones, W. C. Juvela, M. Keihanen, E. Keskitalo, R. Kisner, T. S. Kneissl, R. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Le Jaune, M. Leonardi, R. Leroy, C. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. MacTavish, C. J. Maffei, B. Mandolesi, N. Maris, M. Marleau, F. Marshall, J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. McGehee, P. Meinhold, P. R. Melchiorri, A. Melot, F. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Miville-Deschenes, M. -A. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Mottet, S. Munshi, D. Murphy, J. A. Naselsky, P. Nati, F. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. North, C. Noviello, F. Novikov, D. Novikov, I. Orieux, F. Osborne, S. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paladini, R. Paoletti, D. Pasian, F. Patanchon, G. Perdereaun, O. Perotto, L. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Racine, B. Reach, W. T. Rebolo, R. Reinecke, M. Remazeilles, M. Renault, C. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Rosset, C. Roudier, G. Rowan-Robinson, M. Rusholme, B. Sanselme, L. Santos, D. Sauve, A. Savini, G. Scott, D. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sureae, F. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Techene, S. Terenzi, L. Tomasi, M. Tristram, M. Tucci, M. Umana, G. Valenziano, L. Valiviita, J. Van Tent, B. Vibert, L. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. White, S. D. M. Yvon, D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. VI. High Frequency Instrument data processing SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE methods: data analysis; cosmic background radiation; cosmology: observations; surveys ID PRE-LAUNCH STATUS; MODEL; CALIBRATION; BEAMS AB We describe the processing of the 531 billion raw data samples from the High Frequency Instrument (HFI), which we performed to produce six temperature maps from the first 473 days of Planck-HFI survey data. These maps provide an accurate rendition of the sky emission at 100, 143, 217, 353, 545, and 857 GHz with an angular resolution ranging from 9. 0 7 to 4. 0 6. The detector noise per (effective) beam solid angle is respectively, 10, 6, 12, and 39 K in the four lowest HFI frequency channels (100-353 GHz) and 13 and 14 kJy sr 1 in the 545 and 857 GHz channels. Relative to the 143 GHz channel, these two high frequency channels are calibrated to within 5% and the 353 GHz channel to the percent level. The 100 and 217 GHz channels, which together with the 143 GHz channel determine the high-multipole part of the CMB power spectrum (50 < l < 2500), are calibrated relative to 143 GHz to better than 0.2%. C1 [Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Le Jaune, M.; Patanchon, G.; Piat, M.; Racine, B.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, APC, CNRS IN2P3, CEA Irfu,Observ Paris,Sorbonne Paris Cite, F-75205 Paris 13, France. [Poutanen, T.] Aalto Univ, Metsahovi Radio Observ, Kylmala 02540, Finland. [Kunz, M.] African Inst Math Sci, ZA-7945 Cape Town, South Africa. [Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana Sci Data Ctr, I-00133 Rome, Italy. [Mandolesi, N.] Agenzia Spaziale Italiana, Rome, Italy. [Ashdown, M.; Bridges, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 OHE, England. [Chiang, H. C.] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, ZA-4000 Durban, South Africa. [Kneissl, R.] ALMA, Santiago Cent Off, Santiago 7630355, Chile. [Bond, J. R.; Hanson, D.; Martin, P. G.; Miville-Deschenes, M. -A.] Univ Toronto, CITA, Toronto, ON M5S 3H8, Canada. [Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Leroy, C.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.; Sauve, A.] CNRS, IRAP, F-31028 Toulouse 4, France. [Bock, J. J.; Dore, O.; Helou, G.; Hildebrandt, S. R.; Prezeau, G.; Rocha, G.] CALTECH, Pasadena, CA 91125 USA. [Shellard, E. P. S.] Univ Cambridge, DAMTP, Ctr Theoret Cosmol, Cambridge CB3 0WA, England. [Hernandez-Monteagudo, C.] CEFCA, Teruel 44001, Spain. [Borrill, J.; Keskitalo, R.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 94720 USA. [Rebolo, R.] CSIC, E-28006 Madrid, Spain. [Chamballu, A.; Yvon, D.] CEA Saclay, DSM Irfu SPP, F-91191 Gif Sur Yvette, France. [Hornstrup, A.; Linden-Vornle, M.; Norgaard-Nielsen, H. U.; Oxborrow, C. A.] Tech Univ Denmark, Natl Space Inst, DTU Space, DK-2800 Lyngby, Denmark. [Kunz, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, CH-1211 Geneva 4, Switzerland. [Atrio-Barandela, F.] Univ Salamanca, Fac Ciencias, Dept Fis Fundamental, E-37008 Salamanca, Spain. [Netterfield, C. B.] Univ Toronto, Dept Astron & Astrophys, Toronto, ON, Canada. [Rachen, J. P.] Radboud Univ Nijmegen, IMAPP, Dept Astrophys, NL-6500 GL Nijmegen, Netherlands. [Keskitalo, R.] Univ Calif Berkeley, Dept Elect Engn & Comp Sci, Berkeley, CA 94720 USA. [Scott, D.] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V5Z 1M9, Canada. [Colombo, L. P. L.; Pierpaoli, E.] Univ So Calif, Dana & David Dornsife Coll Letter Arts & Sci, Dept Phys & Astron, Los Angeles, CA 90089 USA. [Benoit-Levy, A.] UCL, Dept Phys & Astron, London WC1E 6BT, England. [Huffenberger, K. M.] Florida State Univ, Dept Phys, Tallahassee, FL 32306 USA. [Juvela, M.; Keihanen, E.; Kurki-Suonio, H.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Dept Phys, FIN-00014 Helsinki, Finland. [Chiang, H. C.; Fraisse, A. A.; Gudmundsson, J. E.; Jones, W. C.] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA. [Hou, Z.; Knox, L.] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA. [Lubin, P. M.; Meinhold, P. R.; Zonca, A.] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA. [Wandelt, B. D.] Univ Illinois, Dept Phys, Urbana, IL USA. [Liguori, M.; Matarrese, S.] Univ Padua, Dipartimento Fis & Astron G Galilei, I-35131 Padua, Italy. [Burigana, C.; Mandolesi, N.; Natoli, P.] Univ Ferrara, Dipartimento Fis & Sci Terra, I-44122 Ferrara, Italy. [de Bernardis, P.; Masi, S.; Melchiorri, A.; Nati, F.; Pagano, L.; Piacentini, F.] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy. [Bersanelli, M.; Mennella, A.] Univ Milan, Dipartimento Fis, I-20133 Milan, Italy. [Gregorio, A.; Tavagnacco, D.] Univ Trieste, Dipartimento Fis, I-34127 Trieste, Italy. [Mazzotta, P.; Vittorio, N.] Univ Roma Tor Vergata, Dipartimento Fis, I-00133 Rome, Italy. [Christensen, P. R.; Naselsky, P.] Niels Bohr Inst, Discovery Ctr, DK-2100 Copenhagen, Denmark. [Rebolo, R.] Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain. [Kneissl, R.] ESO Vitacura, European So Observ, Santiago 19001, Chile. [Dupac, X.; Leonardi, R.; Mendes, L.] European Space Agcy, ESAC, Planck Sci Off, Madrid 28692, Spain. [Frailis, M.; Giardino, G.; Laureijs, R. J.; Tauber, J. A.] Estec, European Space Agcy, NL-2201 AZ Noordwijk, Netherlands. [Kurki-Suonio, H.; Poutanen, T.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Helsinki Inst Phys, FIN-00014 Helsinki, Finland. [Umana, G.] INAF Osservatorio Astrofis Catania, Catania, Italy. [de Zotti, G.] INAF Osservatorio Astron Padova, I-35122 Padua, Italy. [Polenta, G.] INAF Osservatorio Astron Roma, I-00040 Monte Porzio Catone, Italy. [Galeotta, S.; Gregorio, A.; Maris, M.; Pasian, F.; Tavagnacco, D.; Zacchei, A.] INAF Osservatorio Astron Trieste, Trieste, Italy. [Massardi, M.] INAF Ist Radioastron, I-40129 Bologna, Italy. [Burigana, C.; Cuttaia, F.; de Rose, A.; Finelli, F.; Franceschi, E.; Gruppuso, A.; Mandolesi, N.; Morgante, G.; Natoli, P.; Paoletti, D.; Ricciardi, S.; Terenzi, L.; Valenziano, L.; Villa, F.] INAF IASF Bologna, I-40129 Bologna, Italy. [Bersanelli, M.; Donzelli, S.; Mennella, A.; Tomasi, M.] INAF IASF Milano, I-20133 Milan, Italy. [Finelli, F.; Paoletti, D.] Ist Nazl Fis Nucl, Sez Bologna, I-40126 Bologna, Italy. [Melchiorri, A.; Pagano, L.] Univ Roma La Sapienza, Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy. Univ Joseph Fourier Grenoble 1, CNRS INSU, IPAG, UMR 5274, F-38041 Grenoble, France. [Mitra, S.] IUCAA, Pune 411007, Maharashtra, India. [Bowyer, J. W.; Clements, D. L.; Jaffe, A. H.; Mortlock, D.; Novikov, D.; Rowan-Robinson, M.] Univ London Imperial Coll Sci Technol & Med, Astrophys Grp, Blackett Lab, London SW7 2AZ, England. [Chary, R. -R.; Chen, X.; Desert, F. -X.; McGehee, P.; Paladini, R.; Rusholme, B.] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA. [Benoit, A.] Univ Joseph Fourier Grenoble I, CNRS, Inst Neel, F-38042 Grenoble, France. [Dole, H.] Inst Univ France, F-75005 Paris, France. [Aghanim, N.; Aumont, J.; Boulanger, F.; Chamballu, A.; Dole, H.; Douspis, M.; Hurier, G.; Kunz, M.; Lagache, G.; Leroy, C.; Miville-Deschenes, M. -A.; Pajot, F.; Ponthieu, N.; Puget, J. -L.; Remazeilles, M.; Vibert, L.] Univ Paris 11, CNRS, Inst Astrophys Spatiale, UMR8617, F-91405 Orsay, France. [Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Cardoso, J. -F.; Colombi, S.; Delouis, J. -M.; Herent, O.; Hivon, E.; Moneti, A.; Mottet, S.; Orieux, F.; Prunet, S.; Sygnet, J. -F.; Techene, S.; Wandelt, B. D.] CNRS, Inst Astrophys Paris, UMR7095, F-75014 Paris, France. [Popa, L.] Inst Space Sci, Bucharest, Romania. [Marleau, F.] Univ Innsbruck, Inst Astro & Particle Phys, A-6020 Innsbruck, Austria. [Chiang, L. -Y] Acad Sinica, Inst Astron & Astrophys, Taipei 10617, Taiwan. [Bridges, M.; Efstathiou, G.; Gratton, S.; Harrison, D.; Migliaccio, M.; Sutton, D.] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England. [Eriksen, H. K.; Hansen, F. K.; Lilje, P. B.; Valiviita, J.] Univ Oslo, Inst Theoret Astrophys, Oslo, Norway. [Rebolo, R.] Inst Astrofis Canarias, Tenerife, Spain. [Barreiro, R. B.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Vielva, P.] Univ Cantabria, CSIC, Inst Fis Cantabria, E-39005 Santander, Spain. [Bock, J. J.; Colombo, L. P. L.; Crill, B. P.; Dore, O.; Gorski, K. M.; Hanson, D.; Holmes, W. A.; Lawrence, C. R.; Mitra, S.; Pietrobon, D.; Prezeau, G.; Rocha, G.; Roudier, G.; Wade, L. A.] CALTECH, Jet Prop Lab, Pasadena, CA USA. [Davies, R. D.; Davis, R. J.; Dickinson, C.; Maffei, B.; Noviello, F.; Remazeilles, M.] Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Manchester M13 9PL, Lancs, England. [Ashdown, M.; Bridges, M.; Gratton, S.; Harrison, D.; Lasenby, A.; MacTavish, C. J.; Migliaccio, M.; Stolyarov, V.; Sutton, D.] Kavli Inst Cosmol Cambridge, Cambridge CB3 0HA, England. [Couchot, F.; Henrot-Versille, S.; Perdereaun, O.; Plaszczynski, S.; Tristram, M.; Tucci, M.] Univ Paris 11, CNRS IN2P3, LAL, F-91405 Orsay, France. [Catalano, A.; Coulais, A.; Lamarre, J. -M.; Roudier, G.] Observ Paris, CNRS, LERMA, F-75014 Paris, France. [Arnaud, M.; Bobin, J.; Chamballu, A.; Marshall, J.; Pratt, G. W.; Starck, J. -L.; Sureae, F.] Univ Paris Diderot, CEA Saclay, CEA DSM CNRS, Lab AIM,IRFU,Serv Astrophys, F-91191 Gif Sur Yvette, France. [Cardoso, J. -F.] CNRS, UMR 5141, Lab Traitement & Commun Informat, F-75634 Paris 13, France. [Cardoso, J. -F.] Telecom Paris Tech, F-75634 Paris 13, France. [Catalano, A.; Combet, C.; Girard, D.; Hurier, G.; Macias-Perez, J. F.; Melot, F.; Perotto, L.; Renault, C.; Sanselme, L.; Santos, D.] Univ Joseph Fourier Grenoble I, CNRS IN2P3, Inst Natl Polytech Grenoble, Lab Phys Subatom & Cosmol, F-38026 Grenoble, France. [Van Tent, B.] Univ Paris 11, Phys Theor Lab, F-91405 Orsay, France. [Van Tent, B.] CNRS, F-91405 Orsay, France. [Kisner, T. S.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Ensslin, T. A.; Hernandez-Monteagudo, C.; Hovest, W.; Knoche, J.; Matthai, F.; Rachen, J. P.; Reinecke, M.; Riller, T.; White, S. D. M.] Max Planck Inst Astrophys, D-85741 Garching, Germany. [Hanson, D.] McGill Univ, McGill Phys, Montreal, PQ H3A 2T8, Canada. [Murphy, J. A.] Natl Univ Ireland, Maynooth, Kildare, Ireland. [Christensen, P. R.; Naselsky, P.; Novikov, I.] Niels Bohr Inst, DK-2100 Copenhagen, Denmark. [Crill, B. P.] CALTECH, Observ Cosmol, Pasadena, CA 91125 USA. [Savini, G.] UCL, Opt Sci Lab, London, England. [Lesgourgues, J.] Ecole Polytech Fed Lausanne, SB ITP LPPC, CH-1015 Lausanne, Switzerland. [Baccigalupi, C.; Bielewicz, P.; Danese, L.; de Zotti, G.; Gonzalez-Nuevo, J.; North, C.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sector, I-34136 Trieste, Italy. [Ade, P. A. R.; Munshi, D.; Spencer, L. D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales. [Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA. [Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz 369167, Zelenchukskiy R, Russia. [Church, S.; Osborne, S.] Stanford Univ, Dept Phys, Stanford, CA USA. [Armitage-Caplan, C.; Dunkley, J.] Univ Oxford, Sub Dept Astrophys, Oxford OX1 3RH, England. [Lesgourgues, J.] CERN, PH TH, Div Theory, CH-1211 Geneva 23, Switzerland. [Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Colombi, S.; Delouis, J. -M.; Hivon, E.; Prunet, S.; Wandelt, B. D.] Univ Paris 06, UMR7095, Paris, France. [Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Leroy, C.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.; Sauve, A.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France. [Reach, W. T.] Univ Space Res Assoc, Stratospher Observ Infrared Astron, Moffett Field, CA 94035 USA. [Battaner, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, E-18071 Granada, Spain. [Gorski, K. M.] Univ Warsaw Observ, PL-00478 Warsaw, Poland. RP Bouchet, FR (reprint author), CNRS, Inst Astrophys Paris, UMR7095, 98bis Blvd Arago, F-75014 Paris, France. EM bouchet@iap.fr RI Barreiro, Rita Belen/N-5442-2014; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; Remazeilles, Mathieu/N-1793-2015; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Valiviita, Jussi/A-9058-2016; Mazzotta, Pasquale/B-1225-2016; Kurki-Suonio, Hannu/B-8502-2016; Tomasi, Maurizio/I-1234-2016; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Martinez-Gonzalez, Enrique/E-9534-2015; OI Finelli, Fabio/0000-0002-6694-3269; Umana, Grazia/0000-0002-6972-8388; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Lopez-Caniego, Marcos/0000-0003-1016-9283; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Galeotta, Samuele/0000-0002-3748-5115; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; De Zotti, Gianfranco/0000-0003-2868-2595; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Savini, Giorgio/0000-0003-4449-9416; Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Gruppuso, Alessandro/0000-0001-9272-5292; Valiviita, Jussi/0000-0001-6225-3693; Mazzotta, Pasquale/0000-0002-5411-1748; Kurki-Suonio, Hannu/0000-0002-4618-3063; Tomasi, Maurizio/0000-0002-1448-6131; Vielva, Patricio/0000-0003-0051-272X; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Reach, William/0000-0001-8362-4094; Hurier, Guillaume/0000-0002-1215-0706; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Ricciardi, Sara/0000-0002-3807-4043; Villa, Fabrizio/0000-0003-1798-861X; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794 FU ESA FX The development of Planck has been supported by: ESA; CNES and CNRS / INSU- IN2P3- INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER / SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT / MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at h t t p : / / w w w. s c i o p s. e s a. i n t / i n d e x. p h p ? p r o j e c t = p l a n c k & p a g e = P l a n c k _ C o l l a b o r a t i o n. NR 57 TC 66 Z9 65 U1 3 U2 16 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A6 DI 10.1051/0004-6361/201321570 PG 44 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600022 ER PT J AU Ade, PAR Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Bartlett, JG Battaner, E Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bonaldi, A Bond, JR Borrill, J Bouchet, FR Boulanger, F Bridges, M Bucher, M Burigana, C Butler, RC Cardoso, JF Catalano, A Chamballu, A Chary, RR Chen, X Chiang, HC Chiang, LY Christensen, PR Church, S Clements, DL Colley, JM Colombi, S Colombo, LPL Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Danese, L Davies, RD de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Delouis, JM Desert, FX Dickinson, C Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Finelli, F Forni, O Frailis, M Fraisse, AA Franceschi, E Galeotta, S Ganga, K Giard, M Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Hansen, FK Hanson, D Harrison, D Helou, G Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Jaffe, AH Jaffe, TR Jones, WC Juvela, M Keihanen, E Keskitalo, R Kisner, TS Kneissl, R Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lahteenmaki, A Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Leonardi, R Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maffei, B Maino, D Mandolesi, N Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Mazzotta, P Meinhold, PR Melchiorri, A Mendes, L Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, MA Moneti, A Montier, L Morgante, G Mortlock, D Mottet, S Munshi, D Murphy, JA Naselsky, P Nati, F Natoli, P Netterfield, CB Norgaard-Nielsen, HU Noviello, F Novikov, D Novikov, I Osborne, S O'Sullivan, C Oxborrow, CA Paci, F Pagano, L Pajot, F Paladini, R Paoletti, D Pasian, F Patanchon, G Perdereau, O Perotto, L Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polegre, AM Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Reach, WT Rebolo, R Reinecke, M Remazeilles, M Renault, C Ricciardi, S Riller, T Ristorcelli, I Rocha, G Rosset, C Roudier, G Rowan-Robinson, M Rusholme, B Sandri, M Santos, D Savini, G Scott, D Seiffert, MD Shellard, EPS Smoot, GF Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sureau, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Tuovinen, J Umana, G Valenziano, L Valiviita, J Van Tent, B Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD Yvon, D Zacchei, A Zonca, A AF Ade, P. A. R. Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Bartlett, J. G. Battaner, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bonaldi, A. Bond, J. R. Borrill, J. Bouchet, F. R. Boulanger, F. Bridges, M. Bucher, M. Burigana, C. Butler, R. C. Cardoso, J. -F. Catalano, A. Chamballu, A. Chary, R. -R. Chen, X. Chiang, H. C. Chiang, L. -Y Christensen, P. R. Church, S. Clements, D. L. Colley, J. -M. Colombi, S. Colombo, L. P. L. Couchot, F. Coulais, A. Crill, B. P. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Delouis, J. -M. Desert, F. -X. Dickinson, C. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Finelli, F. Forni, O. Frailis, M. Fraisse, A. A. Franceschi, E. Galeotta, S. Ganga, K. Giard, M. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Hansen, F. K. Hanson, D. Harrison, D. Helou, G. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Jaffe, A. H. Jaffe, T. R. Jones, W. C. Juvela, M. Keihanen, E. Keskitalo, R. Kisner, T. S. Kneissl, R. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Lahteenmaki, A. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leonardi, R. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maffei, B. Maino, D. Mandolesi, N. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. Meinhold, P. R. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Miville-Deschenes, M. -A. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Mottet, S. Munshi, D. Murphy, J. A. Naselsky, P. Nati, F. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novikov, I. Osborne, S. O'Sullivan, C. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paladini, R. Paoletti, D. Pasian, F. Patanchon, G. Perdereau, O. Perotto, L. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polegre, A. M. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Reach, W. T. Rebolo, R. Reinecke, M. Remazeilles, M. Renault, C. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Rosset, C. Roudier, G. Rowan-Robinson, M. Rusholme, B. Sandri, M. Santos, D. Savini, G. Scott, D. Seiffert, M. D. Shellard, E. P. S. Smoot, G. F. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sureau, F. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Tuovinen, J. Umana, G. Valenziano, L. Valiviita, J. Van Tent, B. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. Yvon, D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. XIV. Zodiacal emission SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE zodiacal dust; interplanetary medium; cosmic background radiation ID SYSTEM DUST BANDS; SOLAR-SYSTEM; INFRARED-EMISSION; IRAS OBSERVATIONS; ORIGIN; CLOUD; COBE; MODEL; COMETARY; SPECTRUM AB The Planck satellite provides a set of all-sky maps at nine frequencies from 30 GHz to 857 GHz. Planets, minor bodies, and di ff use interplanetary dust emission (IPD) are all observed. The IPD can be separated from Galactic and other emissions because Planck views a given point on the celestial sphere multiple times, through di ff erent columns of IPD. We use the Planck data to investigate the behaviour of zodiacal emission over the whole sky at sub-millimetre and millimetre wavelengths. We fit the Planck data to find the emissivities of the various components of the COBE zodiacal model -a di ff use cloud, three asteroidal dust bands, a circumsolar ring, and an Earth-trailing feature. The emissivity of the diffuse cloud decreases with increasing wavelength, as expected from earlier analyses. The emissivities of the dust bands, however, decrease less rapidly, indicating that the properties of the grains in the bands are di ff erent from those in the di ff use cloud. We fit the small amount of Galactic emission seen through the telescope's far sidelobes, and place limits on possible contamination of the cosmic microwave background (CMB) results from both zodiacal and far-sidelobe emission. When necessary, the results are used in the Planck pipeline to make maps with zodiacal emission and far sidelobes removed. We show that the zodiacal correction to the CMB maps is small compared to the Planck CMB temperature power spectrum and give a list of flux densities for small solar system bodies. C1 [Bartlett, J. G.; Bucher, M.; Cardoso, J. -F.; Colley, J. -M.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Piat, M.; Remazeilles, M.; Rosset, C.; Roudier, G.; Smoot, G. F.; Stompor, R.] Univ Paris Diderot, Observ Paris, Sorbonne Paris Cite, CNRS IN2P3 CEA Irfu,APC, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France. [Lahteenmaki, A.; Poutanen, T.] Aalto Univ, Metsahovi Radio Observ, Kylmala 02540, Finland. [Kunz, M.] African Inst Math Sci, ZA-7945 Cape Town, South Africa. [Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana, Sci Data Ctr, I-00133 Rome, Italy. [Mandolesi, N.] Agenzia Spaziale Italiana, I-00198 Rome, Italy. [Ashdown, M.; Bridges, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 0HE, England. 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EM ganga@apc.univ-paris-diderot.fr RI Butler, Reginald/N-4647-2015; Barreiro, Rita Belen/N-5442-2014; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; Remazeilles, Mathieu/N-1793-2015; Martinez-Gonzalez, Enrique/E-9534-2015; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Mazzotta, Pasquale/B-1225-2016; Kurki-Suonio, Hannu/B-8502-2016; Tomasi, Maurizio/I-1234-2016; Novikov, Igor/N-5098-2015; Lahteenmaki, Anne/L-5987-2013; Toffolatti, Luigi/K-5070-2014; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; OI Umana, Grazia/0000-0002-6972-8388; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Lopez-Caniego, Marcos/0000-0003-1016-9283; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Butler, Reginald/0000-0003-4366-5996; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Galeotta, Samuele/0000-0002-3748-5115; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; De Zotti, Gianfranco/0000-0003-2868-2595; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Gruppuso, Alessandro/0000-0001-9272-5292; Mazzotta, Pasquale/0000-0002-5411-1748; Kurki-Suonio, Hannu/0000-0002-4618-3063; Tomasi, Maurizio/0000-0002-1448-6131; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; Paoletti, Daniela/0000-0003-4761-6147; Savini, Giorgio/0000-0003-4449-9416; Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834; Reach, William/0000-0001-8362-4094; Valiviita, Jussi/0000-0001-6225-3693; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Bouchet, Francois/0000-0002-8051-2924; Ricciardi, Sara/0000-0002-3807-4043; Villa, Fabrizio/0000-0003-1798-861X; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794 FU NASA FX This paper benefited from exchanges with Dale Fixsen, Tom Kelsall and Janet Weiland. We acknowledge the IN2P3 Computer Center ( h t t p : / / c c. i n 2 p 3. f r) for providing a significant amount of the computing resources and services needed for this work. We acknowledge the use of the Legacy Archive for Microwave Background Data Analysis ( LAMBDA). Support for LAMBDA is provided by the NASA O ffi ce of Space Science. The development of Planck has been supported by: ESA; CNES and CNRS / INSUIN2P3- INP ( France); ASI, CNR, and INAF ( Italy); NASA and DoE ( USA); STFC and UKSA ( UK); CSIC, MICINN, JA and RES ( Spain); Tekes, AoF and CSC ( Finland); DLR and MPG ( Germany); CSA ( Canada); DTU Space ( Denmark); SER / SSO ( Switzerland); RCN ( Norway); SFI ( Ireland); FCT / MCTES ( Portugal); and PRACE ( EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at h t t p : / / w w w. s c i o p s. e s a. i n t / i n d e x. p h p ? p r o j e c t = p l a n c k & p a g e = P l a n c k _ C o l l a b o r a t i o n NR 75 TC 49 Z9 48 U1 3 U2 15 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A14 DI 10.1051/0004-6361/201321562 PG 25 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600020 ER PT J AU Ade, PAR Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Bartlett, JG Battaner, E Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bonaldi, A Bonavera, L Bond, JR Borrill, J Bouchet, FR Bridges, M Bucher, M Burigana, C Butler, RC Cardoso, JF Catalano, A Challinor, A Chamballu, A Chiang, HC Chiang, LY Christensen, PR Church, S Clements, DL Colombi, S Colombo, LPL Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Danese, L Davies, RD Davis, RJ de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Delouis, JM Desert, FX Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Fabre, O Finelli, F Forni, O Frailis, M Franceschi, E Galeotta, S Ganga, K Giard, M Giardino, G Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Hansen, FK Hanson, D Harrison, DL Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Jaffe, AH Jaffe, TR Jones, WC Juvela, M Keihanen, E Keskitalo, R Kisner, TS Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lahteenmaki, A Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Leahy, JP Leonardi, R Leroy, C Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maffei, B Maino, D Mandolesi, N Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Mazzotta, P McEwen, JD Melchiorri, A Mendes, L Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, MA Moneti, A Montier, L Morgante, G Mortlock, D Moss, A Munshi, D Murphy, JA Naselsky, P Nati, F Natoli, P Netterfield, CB Norgaard-Nielsen, HU Noviello, F Novikov, D Novikov, I Osborne, S Oxborrow, CA Paci, F Pagano, L Pajot, F Paoletti, D Pasian, F Patanchon, G Peiris, HV Perdereau, O Perotto, L Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pogosyan, D Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Rebolo, R Reinecke, M Remazeilles, M Renault, C Riazuelo, A Ricciardi, S Riller, T Ristorcelli, I Rocha, G Rosset, C Roudier, G Rowan-Robinson, M Rusholme, B Sandri, M Santos, D Savini, G Scott, D Seiffert, MD Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sureau, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Tuovinen, J Valenziano, L Valiviita, J Van Tent, B Varis, J Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD Yvon, D Zacchei, A Zonca, A AF Ade, P. A. R. Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Bartlett, J. G. Battaner, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bonaldi, A. Bonavera, L. Bond, J. R. Borrill, J. Bouchet, F. R. Bridges, M. Bucher, M. Burigana, C. Butler, R. C. Cardoso, J. -F. Catalano, A. Challinor, A. Chamballu, A. Chiang, H. C. Chiang, L. -Y. Christensen, P. R. Church, S. Clements, D. L. Colombi, S. Colombo, L. P. L. Couchot, F. Coulais, A. Crill, B. P. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. Davis, R. J. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Delouis, J. -M. Desert, F. -X. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Fabre, O. Finelli, F. Forni, O. Frailis, M. Franceschi, E. Galeotta, S. Ganga, K. Giard, M. Giardino, G. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Hansen, F. K. Hanson, D. Harrison, D. L. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Jaffe, A. H. Jaffe, T. R. Jones, W. C. Juvela, M. Keihanen, E. Keskitalo, R. Kisner, T. S. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Lahteenmaki, A. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leahy, J. P. Leonardi, R. Leroy, C. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maffei, B. Maino, D. Mandolesi, N. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. McEwen, J. D. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Miville-Deschenes, M. -A. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Moss, A. Munshi, D. Murphy, J. A. Naselsky, P. Nati, F. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novikov, I. Osborne, S. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paoletti, D. Pasian, F. Patanchon, G. Peiris, H. V. Perdereau, O. Perotto, L. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pogosyan, D. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Rebolo, R. Reinecke, M. Remazeilles, M. Renault, C. Riazuelo, A. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Rosset, C. Roudier, G. Rowan-Robinson, M. Rusholme, B. Sandri, M. Santos, D. Savini, G. Scott, D. Seiffert, M. D. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sureau, F. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Tuovinen, J. Valenziano, L. Valiviita, J. Van Tent, B. Varis, J. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. Yvon, D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. XXVI. Background geometry and topology of the Universe SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE cosmology: observations; cosmic background radiation; cosmological parameters; gravitation; methods: data analysis; methods: statistical ID MICROWAVE-ANISOTROPY-PROBE; DODECAHEDRAL SPACE TOPOLOGY; BIANCHI-VIIH MODELS; WMAP OBSERVATIONS; COBE-DMR; SKY MAPS; COSMIC CRYSTALLOGRAPHY; PARAMETER-ESTIMATION; COSMOLOGICAL MODELS; SPHERICAL WAVELETS AB The new cosmic microwave background (CMB) temperature maps from Planck provide the highest-quality full-sky view of the surface of last scattering available to date. This allows us to detect possible departures from the standard model of a globally homogeneous and isotropic cosmology on the largest scales. We search for correlations induced by a possible non-trivial topology with a fundamental domain intersecting, or nearly intersecting, the last scattering surface (at comoving distance chi(rec)), both via a direct search for matched circular patterns at the intersections and by an optimal likelihood search for specific topologies. For the latter we consider flat spaces with cubic toroidal (T3), equal-sided chimney (T2) and slab (T1) topologies, three multi-connected spaces of constant positive curvature (dodecahedral, truncated cube and octahedral) and two compact negative-curvature spaces. These searches yield no detection of the compact topology with the scale below the diameter of the last scattering surface. For most compact topologies studied the likelihood maximized over the orientation of the space relative to the observed map shows some preference for multi-connected models just larger than the diameter of the last scattering surface. Since this effect is also present in simulated realizations of isotropic maps, we interpret it as the inevitable alignment of mild anisotropic correlations with chance features in a single sky realization; such a feature can also be present, in milder form, when the likelihood is marginalized over orientations. Thus marginalized, the limits on the radius R-i of the largest sphere inscribed in topological domain (at log-likelihood-ratio Delta ln L > -5 relative to a simply-connected flat Planck best-fit model) are: in a flat Universe, R-i > 0.92 chi(rec) for the T3 cubic torus; R-i > 0.71 chi(rec) for the T2 chimney; R-i > 0.50 chi(rec) for the T1 slab; and in a positively curved Universe, R-i > 1.03 chi(rec) for the dodecahedral space; R-i > 1.0 chi(rec) for the truncated cube; and R-i > 0.89 chi(rec) for the octahedral space. The limit for a wider class of topologies, i. e., those predicting matching pairs of back-to-back circles, among them tori and the three spherical cases listed above, coming from the matched-circles search, is R-i > 0.94 chi(rec) at 99% confidence level. Similar limits apply to a wide, although not exhaustive, range of topologies. We also perform a Bayesian search for an anisotropic global Bianchi VIIh geometry. In the non-physical setting where the Bianchi cosmology is decoupled from the standard cosmology, Planck data favour the inclusion of a Bianchi component with a Bayes factor of at least 1.5 units of log-evidence. Indeed, the Bianchi pattern is quite efficient at accounting for some of the large-scale anomalies found in Planck data. However, the cosmological parameters that generate this pattern are in strong disagreement with those found from CMB anisotropy data alone. In the physically motivated setting where the Bianchi parameters are coupled and fitted simultaneously with the standard cosmological parameters, we find no evidence for a Bianchi VIIh cosmology and constrain the vorticity of such models to (omega/H)(0) < 8.1 x 10(-10) (95% confidence level). C1 [Bartlett, J. G.; Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Piat, M.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, Sorbonne Paris Cite, Observ Paris, CNRS,IN2P3,CEA,Irfu,APC, F-75205 Paris 13, France. [Lahteenmaki, A.; Poutanen, T.] Aalto Univ Metsahovi Radio Observ, Aalto 00076, Finland. [Lahteenmaki, A.; Poutanen, T.] Dept Radio Sci & Engn, Aalto 00076, Finland. [Kunz, M.] African Inst Math Sci, ZA-7945 Cape Town, South Africa. [Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana Sci Data Ctr, I-00133 Rome, Italy. [Mandolesi, N.] Agenzia Spaziale Italiana, Rome, Italy. 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[Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Zelenchukskiy Region 369167, Karachai Cherke, Russia. [Church, S.; Osborne, S.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA. [Armitage-Caplan, C.] Univ Oxford, Sub Dept Astrophys, Oxford OX1 3RH, England. [Lesgourgues, J.] CERN, Div Theory, PH TH, CH-1211 Geneva 23, Switzerland. [Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Colombi, S.; Delouis, J. -M.; Hivon, E.; Prunet, S.; Riazuelo, A.; Wandelt, B. D.] Univ Paris 06, UMR 7095, F-75014 Paris, France. [Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Leroy, C.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France. [Battaner, E.] Univ Granada, Dept Fis Teor & Cosmos, Fac Ciencias, E-18071 Granada, Spain. [Gorski, K. M.] Univ Warsaw Observ, PL-00478 Warsaw, Poland. RP Jaffe, AH (reprint author), Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Astrophys Grp, Prince Consort Rd, London SW7 2AZ, England. EM a.jaffe@imperial.ac.uk RI Remazeilles, Mathieu/N-1793-2015; Tomasi, Maurizio/I-1234-2016; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; bonavera, laura/E-9368-2017; Kurki-Suonio, Hannu/B-8502-2016; Toffolatti, Luigi/K-5070-2014; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Martinez-Gonzalez, Enrique/E-9534-2015; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Valiviita, Jussi/A-9058-2016; Mazzotta, Pasquale/B-1225-2016; Lahteenmaki, Anne/L-5987-2013; Barreiro, Rita Belen/N-5442-2014; Butler, Reginald/N-4647-2015; OI Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Galeotta, Samuele/0000-0002-3748-5115; Ricciardi, Sara/0000-0002-3807-4043; Pasian, Fabio/0000-0002-4869-3227; Tomasi, Maurizio/0000-0002-1448-6131; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; bonavera, laura/0000-0001-8039-3876; De Zotti, Gianfranco/0000-0003-2868-2595; Lopez-Caniego, Marcos/0000-0003-1016-9283; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Kurki-Suonio, Hannu/0000-0002-4618-3063; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Gruppuso, Alessandro/0000-0001-9272-5292; Valiviita, Jussi/0000-0001-6225-3693; Mazzotta, Pasquale/0000-0002-5411-1748; Savini, Giorgio/0000-0003-4449-9416; Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Villa, Fabrizio/0000-0003-1798-861X; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Butler, Reginald/0000-0003-4366-5996; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017 FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR (Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC (Spain); MICINN (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF (Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); PRACE (EU); Canada Foundation for Innovation under the auspices of Compute Canada; Government of Ontario; Ontario Research Fund - Research Excellence; University of Toronto FX The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.sciops.esa.int/index.php?project=planck&page=Planck_Collabora tion. The authors thank the anonymous referee for helpful comments and acknowledge the use of the UCL Legion High Performance Computing Facility (Legion@UCL), and associated support services, in the completion of this work. Part of the computations were performed on the Andromeda cluster of the University of Geneve, the Hopper Cray XE6 at NERSC and on the GPC supercomputer at the SciNet HPC Consortium. SciNet is funded by: the Canada Foundation for Innovation under the auspices of Compute Canada; the Government of Ontario; Ontario Research Fund - Research Excellence; and the University of Toronto. NR 124 TC 82 Z9 81 U1 3 U2 13 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A26 DI 10.1051/0004-6361/201321546 PG 23 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600015 ER PT J AU Ade, PAR Aghanim, N Alves, MIR Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Bartlett, JG Battaner, E Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bonaldi, A Bond, JR Borrill, J Bouchet, FR Boulanger, F Bridges, M Bucher, M Burigana, C Butler, RC Cardos, JF Catalano, A Chamballu, A Chary, RR Chen, X Chiang, HC Chiang, LY Christensen, PR Church, S Clements, DL Colombi, S Colombo, LPL Combet, C Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Danese, L Davies, RD de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Delouis, JM Dempsey, JT Desert, FX Dickinson, C Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Falgarone, E Finelli, F Forni, O Frailis, M Franceschi, E Fukui, Y Galeotta, S Ganga, K Giard, M Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Handa, T Hansen, FK Hanson, D Harrison, D Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hily-Blant, P Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Hurier, G Jaffe, AH Jaffe, TR Jewell, J Jones, WC Juvela, M Keihanen, E Keskitalo, R Kisner, TS Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lahteenmaki, A Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Leonardi, R Leon-Tavares, J Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maffein, B Mandolesi, N Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Mazzotta, P McGehee, P Melchiorri, A Mendes, L Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, MA Moneti, A Montier, L Moore, TJT Morgante, G Morino, J Mortlock, D Munshi, D Murphy, JA Nakajima, T Naselsky, P Nati, F Natoli, P Netterfield, CB Norgaard-Nielsen, HU Noviellon, F Novikov, D Novikov, I Okuda, T Osborne, S Oxborrow, CA Paci, F Pagano, L Pajot, F Paladini, R Paoletti, D Pasian, F Patanchon, G Perdereau, O Perotto, L Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Reach, WT Rebolo, R Reinecke, M Remazeilles, M Renault, C Ricciardi, S Riller, T Ristorcelli, I Rocha, G Rosset, C Roudier, G Rowan-Robinson, M Rubino-Martin, JA Rusholme, B Sandri, M Santos, D Savini, G Scott, D Seiffert, MD Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sunyaev, R Sureau, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Thomas, HS Toffolatti, L Tomasi, M Torii, K Tristram, M Tucci, M Tuovinen, J Umana, G Valenziano, L Valiviita, J Van Tent, B Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD Wehus, IK Yamamoto, H Yoda, T Yvon, D Zacchei, A Zonca, A AF Ade, P. A. R. Aghanim, N. Alves, M. I. R. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Bartlett, J. G. Battaner, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bonaldi, A. Bond, J. R. Borrill, J. Bouchet, F. R. Boulanger, F. Bridges, M. Bucher, M. Burigana, C. Butler, R. C. Cardos, J. -F. Catalano, A. Chamballu, A. Chary, R. -R. Chen, X. Chiang, H. C. Chiang, L. -Y. Christensen, P. R. Church, S. Clements, D. L. Colombi, S. Colombo, L. P. L. Combet, C. Couchot, F. Coulais, A. Crill, B. P. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Delouis, J. -M. Dempsey, J. T. Desert, F. -X. Dickinson, C. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Falgarone, E. Finelli, F. Forni, O. Frailis, M. Franceschi, E. Fukui, Y. Galeotta, S. Ganga, K. Giard, M. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Handa, T. Hansen, F. K. Hanson, D. Harrison, D. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hily-Blant, P. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Hurier, G. Jaffe, A. H. Jaffe, T. R. Jewell, J. Jones, W. C. Juvela, M. Keihanen, E. Keskitalo, R. Kisner, T. S. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Lahteenmaki, A. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leonardi, R. Leon-Tavares, J. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maffein, B. Mandolesi, N. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. McGehee, P. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Miville-Deschenes, M. -A. Moneti, A. Montier, L. Moore, T. J. T. Morgante, G. Morino, J. Mortlock, D. Munshi, D. Murphy, J. A. Nakajima, T. Naselsky, P. Nati, F. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Noviellon, F. Novikov, D. Novikov, I. Okuda, T. Osborne, S. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paladini, R. Paoletti, D. Pasian, F. Patanchon, G. Perdereau, O. Perotto, L. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Reach, W. T. Rebolo, R. Reinecke, M. Remazeilles, M. Renault, C. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Rosset, C. Roudier, G. Rowan-Robinson, M. Rubino-Martin, J. A. Rusholme, B. Sandri, M. Santos, D. Savini, G. Scott, D. Seiffert, M. D. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sunyaev, R. Sureau, F. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Thomas, H. S. Toffolatti, L. Tomasi, M. Torii, K. Tristram, M. Tucci, M. Tuovinen, J. Umana, G. Valenziano, L. Valiviita, J. Van Tent, B. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. Wehus, I. K. Yamamoto, H. Yoda, T. Yvon, D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. XIII. Galactic CO emission SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE ISM: molecules ID LATITUDE MOLECULAR GAS; (CO)-C-13 J=2-1; CARBON-MONOXIDE; MAPPING SURVEY; MILKY-WAY; CLOUDS; REGION; GALAXY; ORION; HEMISPHERE AB Rotational transition lines of CO play a major role in molecular radio astronomy as a mass tracer and in particular in the study of star formation and Galactic structure. Although a wealth of data exists for the Galactic plane and some well-known molecular clouds, there is no available high sensitivity all-sky survey of CO emission to date. Such all-sky surveys can be constructed using the Planck HFI data because the three lowest CO rotational transition lines at 115, 230 and 345 GHz significantly contribute to the signal of the 100, 217 and 353 GHz HFI channels, respectively. Two different component separation methods are used to extract the CO maps from Planck HFI data. The maps obtained are then compared to one another and to existing external CO surveys. From these quality checks the best CO maps, in terms of signal to noise ratio and/or residual contamination by other emission, are selected. Three different sets of velocity-integrated CO emission maps are produced with different trade-offs between signal-to-noise, angular resolution, and reliability. Maps for the CO J = 1 -> 0, J = 2 -> 1, and J = 3 -> 2 rotational transitions are presented and described in detail. They are shown to be fully compatible with previous surveys of parts of the Galactic plane as well as with undersampled surveys of the high latitude sky. The Planck HFI velocity-integrated CO maps for the J = 1 -> 0, J = 2 -> 1, and J = 3 -> 2 rotational transitions provide an unprecedented all-sky CO view of the Galaxy. These maps are also of great interest to monitor potential CO contamination of the Planck studies of the cosmological microwave background. C1 [Bartlett, J. G.; Bucher, M.; Cardos, J. -F.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Piat, M.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, Observ Paris, Sorbonne Paris Cite, CNRS IN2P3,CEA Irfu,APC, F-75205 Paris 13, France. [Lahteenmaki, A.; Leon-Tavares, J.; Poutanen, T.] Aalto Univ, Metsahovi Radio Observ, Kylmala 02540, Finland. [Kunz, M.] African Inst Math Sci, ZA-7701 Rondebosch, South Africa. [Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana, Sci Data Ctr, I-00133 Rome, Italy. [Mandolesi, N.] Agenzia Spaziale Italiana, Rome, Italy. 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[Borrill, J.; Keskitalo, R.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 94720 USA. [Rebolo, R.] CSIC, Madrid, Spain. [Chamballu, A.; Yvon, D.] CEA Saclay, DSM Irfu SPP, F-91191 Gif Sur Yvette, France. [Hornstrup, A.; Linden-Vornle, M.; Norgaard-Nielsen, H. U.; Oxborrow, C. A.] Tech Univ Denmark, Natl Space Inst, DTU Space, DK-2800 Lyngby, Denmark. [Kunz, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, CH-1211 Geneva 4, Switzerland. [Atrio-Barandela, F.] Univ Salamanca, Fac Ciencias, Dept Fis Fundamental, E-37008 Salamanca, Spain. [Toffolatti, L.] Univ Oviedo, Dept Fis, E-33007 Oviedo, Spain. [Netterfield, C. B.] Univ Toronto, Dept Astron & Astrophys, Toronto, ON, Canada. [Rachen, J. P.] Radboud Univ Nijmegen, Dept Astrophys, IMAPP, NL-6500 GL Nijmegen, Netherlands. [Keskitalo, R.] Univ Calif Berkeley, Dept Elect Engn & Comp Sci, Berkeley, CA 94720 USA. [Scott, D.] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V5Z 1M9, Canada. 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[Bersanelli, M.; Donzelli, S.; Mennella, A.; Tomasi, M.] INAF IASF Milano, I-20133 Milan, Italy. [Finelli, F.; Paoletti, D.] Ist Nazl Fis Nucl, Sez Bologna, I-40126 Bologna, Italy. [Melchiorri, A.; Pagano, L.] Univ Roma La Sapienza, Ist Nazl Fis Nucl, Sez Roma 1, I-00185 Rome, Italy. [Desert, F. -X.; Hily-Blant, P.; Ponthieu, N.] Univ Grenoble 1, CNRS INSU, Inst Planetol & Astrophys Grenoble, UMR 5274, F-38041 Grenoble, France. [Mitra, S.] IUCAA, Pune 411007, Maharashtra, India. [Clements, D. L.; Jaffe, A. H.; Mortlock, D.; Novikov, D.; Rowan-Robinson, M.] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Astrophys Grp, London SW7 2AZ, England. [Chary, R. -R.; Chen, X.; McGehee, P.; Paladini, R.; Rusholme, B.] CALTECH, Ctr Infrared Proc & Anal, Pasadena, CA 91125 USA. [Benoit, A.] Univ Grenoble 1, CNRS, Inst Neel, F-38042 Grenoble, France. [Dole, H.] Inst Univ France, F-75005 Paris, France. [Aghanim, N.; Alves, M. I. R.; Aumont, J.; Boulanger, F.; Chamballu, A.; Dole, H.; Douspis, M.; Hurier, G.; Kunz, M.; Lagache, G.; Miville-Deschenes, M. -A.; Pajot, F.; Ponthieu, N.; Puget, J. -L.; Remazeilles, M.] Univ Paris 11, CNRS, Inst Astrophys Spatiale, UMR 8617, F-91405 Orsay, France. [Benabed, K.; Benoit-Levy, A.; Boulanger, F.; Cardos, J. -F.; Colombi, S.; Delouis, J. -M.; Hivon, E.; Moneti, A.; Prunet, S.; Sygnet, J. -F.; Wandelt, B. D.] CNRS, Inst Astrophys Paris, UMR 7095, F-75014 Paris, France. [Popa, L.] Inst Space Sci, Bucharest 077125, Romania. [Chiang, L. -Y.] Acad Sinica, Inst Astron & Astrophys, Taipei 115, Taiwan. [Bridges, M.; Efstathiou, G.; Gratton, S.; Harrison, D.; Migliaccio, M.; Sutton, D.] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England. [Yoda, T.] Univ Tokyo, Inst Astron, Mitaka, Tokyo 181, Japan. [Eriksen, H. K.; Hansen, F. K.; Lilje, P. B.; Valiviita, J.] Univ Oslo, Inst Theoret Astrophys, N-0315 Oslo, Norway. [Rebolo, R.; Rubino-Martin, J. A.] Inst Astrofis Canarias, Tenerife 38200, Spain. [Barreiro, R. B.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Toffolatti, L.; Vielva, P.] Univ Cantabria, CSIC, Inst Fis Cantabria, E-39005 Santander, Spain. [Bartlett, J. G.; Bock, J. J.; Colombo, L. P. L.; Crill, B. P.; Dore, O.; Gorski, K. M.; Holmes, W. A.; Jewell, J.; Lawrence, C. R.; Mitra, S.; Pietrobon, D.; Prezeau, G.; Rocha, G.; Roudier, G.; Seiffert, M. D.; Wade, L. A.; Wehus, I. K.] CALTECH, Jet Prop Lab, Pasadena, CA USA. [Bonaldi, A.; Davies, R. D.; Maffein, B.; Noviellon, F.; Remazeilles, M.] Univ Manchester, Jodrell Bank Ctr Astrophys, Sch Phys & Astron, Manchester M13 9PL, Lancs, England. [Dempsey, J. T.; Thomas, H. S.] Joint Astron Ctr, Hilo, HI 96720 USA. [Couchot, F.; Henrot-Versille, S.; Perdereau, O.; Plaszczynski, S.; Tristram, M.; Tucci, M.] Kavli Inst Cosmol Cambridge, Cambridge, England. [Catalano, A.; Coulais, A.; Falgarone, E.; Lamarre, J. -M.; Roudier, G.] Univ Paris 11, CNRS, IN2P3, LAL, F-91898 Orsay, France. [Arnaud, M.; Bobin, J.; Chamballu, A.; Marshall, D. J.; Pratt, G. W.; Starck, J. -L.; Sureau, F.] CNRS, Observ Paris, LERMA, F-75014 Paris, France. [Cardos, J. -F.] Univ Paris Diderot, CNRS, CEA DSM, Lab AIM,IRFU Serv Astrophys, F-91191 Gif Sur Yvette, France. [Cardos, J. -F.] CNRS, Lab Traitement & Commun Informat, UMR 5141, F-75634 Paris 13, France. [Cardos, J. -F.] Telecom Paris Tech, F-75634 Paris 13, France. [Catalano, A.; Combet, C.; Hurier, G.; Macias-Perez, J. F.; Perotto, L.; Renault, C.; Santos, D.] Univ Grenoble 1, Inst Natl Polytech Grenoble, CNRS IN2P3, Lab Phys Subatom & Cosmol, F-38026 St Martin Dheres, France. [Van Tent, B.] Univ Paris 11, Phys Theor Lab, F-91405 Orsay, France. [Kisner, T. S.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Ensslin, T. A.; Hernandez-Monteagudo, C.; Hovest, W.; Knoche, J.; Matthai, F.; Rachen, J. P.; Reinecke, M.; Riller, T.; Sunyaev, R.] Max Planck Inst Astrophys, D-85741 Garching, Germany. [Hanson, D.] McGill Univ, McGill Phys, Montreal H3A 2T8, PQ, Canada. [Tuovinen, J.] VTT Tech Res Ctr Finland, MilliLab, Espoo 02044, Finland. [Morino, J.] Natl Astron Observ Japan, Tokyo 1818588, Japan. [Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Kildare, Ireland. [Christensen, P. R.; Naselsky, P.; Novikov, I.] Niels Bohr Inst, DK-2100 Copenhagen, Denmark. [Nakajima, T.] Natl Astron Observ Japan, Nobeyama Radio Observ, Minamisa Ku, Minamimaki, Nagano 3841305, Japan. [Crill, B. P.] CALTECH, Observat Cosmol, Pasadena, CA 91125 USA. [Savini, G.] UCL, Opt Sci Lab, London, England. [Lesgourgues, J.] Ecole Polytech Fed Lausanne, SB ITP LPPC, CH-1015 Lausanne, Switzerland. [Baccigalupi, C.; Danese, L.; de Zotti, G.; Gonzalez-Nuevo, J.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sect, I-34136 Trieste, Italy. [Ade, P. A. R.; Munshi, D.; Spencer, L. D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales. [Sunyaev, R.] Russian Acad Sci, Space Res Inst IKI, Moscow 117997, Russia. [Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA. [Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Karachai Cherkessian 369167, Russia. [Church, S.; Osborne, S.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA. [Armitage-Caplan, C.] Univ Oxford, Sub Dept Astrophys, Oxford OX1 3RH, England. [Lesgourgues, J.] CERN, Div Theory, PH TH, CH-1211 Geneva 23, Switzerland. [Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Colombi, S.; Delouis, J. -M.; Prunet, S.; Wandelt, B. D.] Univ Paris 06, UMR 7095, F-75014 Paris, France. [Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France. [Reach, W. T.] Univ Space Res Assoc, Observ Infrared Astron, Moffett Field, CA 94035 USA. [Battaner, E.] Univ Granada, Dept Fis Teor & Cosmos, Fac Ciencias, E-18071 Granada, Spain. [Gorski, K. M.] Univ Warsaw Observ, PL-00478 Warsaw, Poland. RP Macias-Perez, JF (reprint author), Univ Grenoble 1, Inst Natl Polytech Grenoble, CNRS IN2P3, Lab Phys Subatom & Cosmol, 53 Rue Martyrs, F-38026 St Martin Dheres, France. EM macias@lpsc.in2p3.fr RI Barreiro, Rita Belen/N-5442-2014; Remazeilles, Mathieu/N-1793-2015; Kurki-Suonio, Hannu/B-8502-2016; Tomasi, Maurizio/I-1234-2016; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; Martinez-Gonzalez, Enrique/E-9534-2015; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Butler, Reginald/N-4647-2015; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Valiviita, Jussi/A-9058-2016; Mazzotta, Pasquale/B-1225-2016; Lahteenmaki, Anne/L-5987-2013; Toffolatti, Luigi/K-5070-2014; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; OI Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Umana, Grazia/0000-0002-6972-8388; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Lopez-Caniego, Marcos/0000-0003-1016-9283; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Galeotta, Samuele/0000-0002-3748-5115; Ricciardi, Sara/0000-0002-3807-4043; Juvela, Mika/0000-0002-5809-4834; Kurki-Suonio, Hannu/0000-0002-4618-3063; Tomasi, Maurizio/0000-0002-1448-6131; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; Rubino-Martin, Jose Alberto/0000-0001-5289-3021; De Zotti, Gianfranco/0000-0003-2868-2595; Masi, Silvia/0000-0001-5105-1439; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Savini, Giorgio/0000-0003-4449-9416; Pierpaoli, Elena/0000-0002-7957-8993; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Butler, Reginald/0000-0003-4366-5996; Gruppuso, Alessandro/0000-0001-9272-5292; Valiviita, Jussi/0000-0001-6225-3693; Mazzotta, Pasquale/0000-0002-5411-1748; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; Reach, William/0000-0001-8362-4094; Hurier, Guillaume/0000-0002-1215-0706; Zacchei, Andrea/0000-0003-0396-1192; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Villa, Fabrizio/0000-0003-1798-861X FU ESA FX The development of Planck has been supported by: ESA; CNES and CNRS /INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER /SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT /MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at h t t p : //w w w. s c i o p s. e s a. i n t /i n d e x. p h p ? p r o j e c t = P l a n c k \ & p a g e = P l a n c k _ C o l l a b o r a t i o n. We acknowledge the use of the H E A L P i x software. NR 77 TC 77 Z9 76 U1 3 U2 19 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A13 DI 10.1051/0004-6361/201321553 PG 22 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600017 ER PT J AU Ade, PAR Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Bartlett, JG Basak, S Battaner, E Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bethermin, M Bielewicz, P Bobin, J Bock, JJ Bonaldi, A Bond, JR Borrill, J Bouchet, FR Boulanger, F Bridges, M Bucher, M Burigana, C Butler, RC Cardoso, JF Catalano, A Challinor, A Chamballu, A Chiang, HC Chiang, LY Christensen, PR Church, S Clements, DL Colombi, S Colombo, LPL Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Danese, L Davies, RD de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Delouis, JM Desert, FX Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Finelli, F Forni, O Frailis, M Franceschi, E Galeotta, S Ganga, K Giard, M Giardino, G Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Gudmundsson, JE Hansen, FK Hanson, D Harrison, D Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Jaffe, AH Jaffe, TR Jones, WC Juvela, M Keihanen, E Keskitalo, R Kisner, TS Kneissl, R Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lacasa, F Lagache, G Lahteenmaki, A Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Leonardi, R Leon-Tavares, J Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maffei, B Maino, D Mandolesi, N Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Mazzotta, P Melchiorri, A Mendes, L Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, MA Moneti, A Montier, L Morgante, G Mortlock, D Munshi, D Naselsky, P Nati, F Natoli, P Netterfield, CB Norgaard-Nielsen, HU Noviello, F Novikov, D Novikov, I Osborne, S Oxborrow, CA Paci, F Pagano, L Pajot, F Paoletti, D Pasian, F Patanchon, G Perdereau, O Perotto, L Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Rebolo, R Reinecke, M Remazeilles, M Renault, C Ricciardi, S Riller, T Ristorcelli, I Rocha, G Rosset, C Roudier, G Rowan-Robinson, M Rusholme, B Sandri, M Santos, D Savini, G Scott, D Seiffert, MD Serra, P Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sunyaev, R Sureau, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Tuovinen, J Valenziano, L Valiviita, J Van Tent, B Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD White, SDM Yvon, D Zacchei, A Zonca, A AF Ade, P. A. R. Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Bartlett, J. G. Basak, S. Battaner, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bethermin, M. Bielewicz, P. Bobin, J. Bock, J. J. Bonaldi, A. Bond, J. R. Borrill, J. Bouchet, F. R. Boulanger, F. Bridges, M. Bucher, M. Burigana, C. Butler, R. C. Cardoso, J. -F. Catalano, A. Challinor, A. Chamballu, A. Chiang, H. C. Chiang, L. -Y Christensen, P. R. Church, S. Clements, D. L. Colombi, S. Colombo, L. P. L. Couchot, F. Coulais, A. Crill, B. P. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Delouis, J. -M. Desert, F. -X. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Finelli, F. Forni, O. Frailis, M. Franceschi, E. Galeotta, S. Ganga, K. Giard, M. Giardino, G. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Gudmundsson, J. E. Hansen, F. K. Hanson, D. Harrison, D. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Jaffe, A. H. Jaffe, T. R. Jones, W. C. Juvela, M. Keihanen, E. Keskitalo, R. Kisner, T. S. Kneissl, R. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lacasa, F. Lagache, G. Lahteenmaki, A. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leonardi, R. Leon-Tavares, J. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maffei, B. Maino, D. Mandolesi, N. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Miville-Deschenes, M. -A. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Munshi, D. Naselsky, P. Nati, F. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novikov, I. Osborne, S. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paoletti, D. Pasian, F. Patanchon, G. Perdereau, O. Perotto, L. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Rebolo, R. Reinecke, M. Remazeilles, M. Renault, C. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Rosset, C. Roudier, G. Rowan-Robinson, M. Rusholme, B. Sandri, M. Santos, D. Savini, G. Scott, D. Seiffert, M. D. Serra, P. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sunyaev, R. Sureau, F. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Tuovinen, J. Valenziano, L. Valiviita, J. Van Tent, B. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. White, S. D. M. Yvon, D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. XVIII. The gravitational lensing-infrared background correlation SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE gravitational lensing: weak; cosmic background radiation; large-scale structure of Universe; dark matter; galaxies: star formation ID STAR-FORMING GALAXIES; SOUTH-POLE TELESCOPE; PRE-LAUNCH STATUS; ANISOTROPY POWER SPECTRUM; SENSITIVITY HI SURVEY; DARK-MATTER HALOES; FINAL DATA RELEASE; DUST EMISSION; FORMATION HISTORY; DISTANT GALAXIES AB The multi-frequency capability of the Planck satellite provides information both on the integrated history of star formation (via the cosmic infrared background, or CIB) and on the distribution of dark matter (via the lensing effect on the cosmic microwave background, or CMB). The conjunction of these two unique probes allows us to measure directly the connection between dark and luminous matter in the high redshift (1 <= z <= 3) Universe. We use a three-point statistic optimized to detect the correlation between these two tracers, using lens reconstructions at 100, 143, and 217 GHz, together with CIB measurements at 100-857 GHz. Following a thorough discussion of possible contaminants and a suite of consistency tests, we report the first detection of the correlation between the CIB and CMB lensing. The well matched redshift distribution of these two signals leads to a detection significance with a peak value of 42/19 sigma (statistical/statistical + systematics) at 545 GHz and a correlation as high as 80% across these two tracers. Our full set of multi-frequency measurements (both CIB auto-and CIB-lensing cross-spectra) are consistent with a simple halo-based model, with a characteristic mass scale for the halos hosting CIB sources of log(10)(M/M-circle dot) = 10.5 +/- 0.6. Leveraging the frequency dependence of our signal, we isolate the high redshift contribution to the CIB, and constrain the star formation rate (SFR) density at z >= 1. We measure directly the SFR density with around 2 sigma significance for three redshift bins between z = 1 and 7, thus opening a new window into the study of the formation of stars at early times. C1 [Ade, P. A. R.; Bartlett, J. G.; Bucher, M.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Piat, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, Sorbonne Paris Cite, Observ Paris, CNRS,IN2P3,CEA,lrfu,APC, F-75205 Paris 13, France. [Aghanim, N.; Lahteenmaki, A.] Aalto Univ Metsahovi Radio Observ, Kylmala 02540, Finland. [Armitage-Caplan, C.] African Inst Math Sci, ZA-7701 Muizenberg, Rondebosch Cape, South Africa. [Armitage-Caplan, C.; Polenta, G.] Agenzia Spaziale Italiana Sci Data Ctr, I-00133 Rome, Italy. [Arnaud, M.] Agenzia Spaziale Italiana, I-00198 Rome, Italy. [Ashdown, M.; Atrio-Barandela, F.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 0HE, England. [Aumont, J.] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, ZA-4000 Durban, South Africa. [Baccigalupi, C.] Atacama Large Millimeter submillimeter Array, ALMA Santiago Cent Off, Santiago 7630355, Chile. [Arnaud, M.; Banday, A. J.; Bond, J. R.; Martin, P. G.] Univ Toronto, CITA, Toronto, ON M5S 3H8, Canada. [Barreiro, R. B.; Bartlett, J. G.; Basak, S.; Battaner, E.; Benabed, K.; Benoit, A.; Benoit-Levy, A.; Bernard, J. -P.; Bersanelli, M.] CNRS, IRAP, F-31028 Toulouse 4, France. [Bethermin, M.; Bielewicz, P.; Bobin, J.; Bock, J. J.; Hildebrandt, S. 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EM olivier.p.dore@jpl.nasa.gov RI Barreiro, Rita Belen/N-5442-2014; Butler, Reginald/N-4647-2015; Remazeilles, Mathieu/N-1793-2015; Tomasi, Maurizio/I-1234-2016; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Valiviita, Jussi/A-9058-2016; Mazzotta, Pasquale/B-1225-2016; Kurki-Suonio, Hannu/B-8502-2016; Lahteenmaki, Anne/L-5987-2013; Toffolatti, Luigi/K-5070-2014; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Martinez-Gonzalez, Enrique/E-9534-2015; OI Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Butler, Reginald/0000-0003-4366-5996; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Galeotta, Samuele/0000-0002-3748-5115; Tomasi, Maurizio/0000-0002-1448-6131; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; De Zotti, Gianfranco/0000-0003-2868-2595; Lopez-Caniego, Marcos/0000-0003-1016-9283; Masi, Silvia/0000-0001-5105-1439; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Gruppuso, Alessandro/0000-0001-9272-5292; Valiviita, Jussi/0000-0001-6225-3693; Mazzotta, Pasquale/0000-0002-5411-1748; Kurki-Suonio, Hannu/0000-0002-4618-3063; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Paoletti, Daniela/0000-0003-4761-6147; Savini, Giorgio/0000-0003-4449-9416; Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834; Starck, Jean-Luc/0000-0003-2177-7794; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Ricciardi, Sara/0000-0002-3807-4043; Villa, Fabrizio/0000-0003-1798-861X; Bethermin, Matthieu/0000-0002-3915-2015; TERENZI, LUCA/0000-0001-9915-6379 FU ESA; CNES (France); CNRS/INSU-IN2P3INP (France); ASI (Italy); CNR (Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC (Spain); MICINN (Spain); JA (Spain); Tekes (Finland); AoF (Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); PRACE (EU); ESA Member State, NASA; ESA Member State, Canada FX Based on observations obtained with Planck (http://www.esa.int/Planck), an ESA science mission with instruments and contributions directly funded by ESA Member States, NASA, and Canada. The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN and JA (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http : //www.sciops.esa.int/index.php?project=planck&page=Planck_Collaboration. We acknowledge the use of the HEALPix package, and the LAMBDA archive (http://lambda.gsfc.nasa.gov). NR 113 TC 65 Z9 64 U1 3 U2 9 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A18 DI 10.1051/0004-6361/201321540 PG 24 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600012 ER PT J AU Ade, PAR Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Battaner, E Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bertincourt, B Bielewicz, P Bobin, J Bock, JJ Bond, JR Borrill, J Bouchet, FR Boulanger, F Bridges, M Bucher, M Burigana, C Cardoso, JF Catalano, A Challinor, A Chamballu, A Chary, RR Chen, X Chiang, HC Chiang, LY Christensen, PR Church, S Clements, DL Colombi, S Colombo, LPL Combet, C Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Danese, L Davies, RD de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Delouis, JM Desert, FX Dickinson, C Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Filliard, C Finelli, F Forni, O Frailis, M Franceschi, E Galeotta, S Ganga, K Giard, M Giardino, G Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Hansen, FK Hanson, D Harrison, D Helou, G Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Jaffe, AH Jaffe, TR Jones, WC Juvela, M Keihanen, E Keskitalo, R Kisner, TS Kneissl, R Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Le Jeune, M Lellouch, E Leonardi, R Leroy, C Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maffei, B Mandolesi, N Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Maurin, L Mazzotta, P McGehee, P Meinhold, PR Melchiorri, A Mendes, L Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, MA Moneti, A Montier, L Moreno, R Morgante, G Mortlock, D Munshi, D Murphy, JA Naselsky, P Nati, F Natoli, P Netterfield, CB Norgaard-Nielsen, HU Noviello, F Novikov, D Novikov, I Osborne, S Oxborrow, CA Paci, F Pagano, L Pajot, F Paladini, R Paoletti, D Partridge, B Pasian, F Patanchon, G Pearson, TJ Perdereau, O Perotto, L Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Reinecke, M Remazeilles, M Renault, C Ricciardi, S Riller, T Ristorcelli, I Rocha, G Rosset, C Roudier, G Rusholme, B Santos, D Savini, G Scott, D Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sunyaev, R Sureau, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Techene, S Terenzi, L Tomasi, M Tristram, M Tucci, M Umana, G Valenziano, L Valiviita, J Van Tent, B Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD Yvon, D Zacchei, A Zonca, A AF Ade, P. A. R. Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Battaner, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bertincourt, B. Bielewicz, P. Bobin, J. Bock, J. J. Bond, J. R. Borrill, J. Bouchet, F. R. Boulanger, F. Bridges, M. Bucher, M. Burigana, C. Cardoso, J. -F. Catalano, A. Challinor, A. Chamballu, A. Chary, R. -R. Chen, X. Chiang, H. C. Chiang, L. -Y Christensen, P. R. Church, S. Clements, D. L. Colombi, S. Colombo, L. P. L. Combet, C. Couchot, F. Coulais, A. Crill, B. P. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Delouis, J. -M. Desert, F. -X. Dickinson, C. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Filliard, C. Finelli, F. Forni, O. Frailis, M. Franceschi, E. Galeotta, S. Ganga, K. Giard, M. Giardino, G. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Hansen, F. K. Hanson, D. Harrison, D. Helou, G. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Jaffe, A. H. Jaffe, T. R. Jones, W. C. Juvela, M. Keihanen, E. Keskitalo, R. Kisner, T. S. Kneissl, R. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Le Jeune, M. Lellouch, E. Leonardi, R. Leroy, C. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maffei, B. Mandolesi, N. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Maurin, L. Mazzotta, P. McGehee, P. Meinhold, P. R. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Miville-Deschenes, M. -A. Moneti, A. Montier, L. Moreno, R. Morgante, G. Mortlock, D. Munshi, D. Murphy, J. A. Naselsky, P. Nati, F. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novikov, I. Osborne, S. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paladini, R. Paoletti, D. Partridge, B. Pasian, F. Patanchon, G. Pearson, T. J. Perdereau, O. Perotto, L. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Reinecke, M. Remazeilles, M. Renault, C. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Rosset, C. Roudier, G. Rusholme, B. Santos, D. Savini, G. Scott, D. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sunyaev, R. Sureau, F. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Techene, S. Terenzi, L. Tomasi, M. Tristram, M. Tucci, M. Umana, G. Valenziano, L. Valiviita, J. Van Tent, B. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. Yvon, D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. VIII. HFI photometric calibration and mapmaking SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE cosmic background radiation; cosmology: observations; surveys; methods: data analysis ID IN-FLIGHT PERFORMANCE; PRE-LAUNCH STATUS; DUST EMISSION; 1ST DETECTION; COBE FIRAS; ATMOSPHERE; ANISOTROPY; SPECTRUM; DESIGN; DIRBE AB This paper describes the methods used to produce photometrically calibrated maps from the Planck High Frequency Instrument (HFI) cleaned, time-ordered information. HFI observes the sky over a broad range of frequencies, from 100 to 857 GHz. To obtain the best calibration accuracy over such a large range, two different photometric calibration schemes have to be used. The 545 and 857 GHz data are calibrated by comparing flux-density measurements of Uranus and Neptune with models of their atmospheric emission. The lower frequencies (below 353 GHz) are calibrated using the solar dipole. A component of this anisotropy is time-variable, owing to the orbital motion of the satellite in the solar system. Photometric calibration is thus tightly linked to mapmaking, which also addresses low-frequency noise removal. By comparing observations taken more than one year apart in the same configuration, we have identified apparent gain variations with time. These variations are induced by non-linearities in the read-out electronics chain. We have developed an effective correction to limit their effect on calibration. We present several methods to estimate the precision of the photometric calibration. We distinguish relative uncertainties (between detectors, or between frequencies) and absolute uncertainties. Absolute uncertainties lie in the range from 0.54% to 10% from 100 to 857 GHz. We describe the pipeline used to produce the maps from the HFI timelines, based on the photometric calibration parameters, and the scheme used to set the zero level of the maps a posteriori. We also discuss the cross-calibration between HFI and the SPIRE instrument on board Herschel. Finally we summarize the basic characteristics of the set of HFI maps included in the 2013 Planck data release. C1 [Ade, P. A. R.; Bucher, M.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Le Jeune, M.; Maurin, L.; Patanchon, G.; Piat, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, APC, Sorbonne Paris Cite, CNRS,IN2P3,CEA,Irfu,Observ Paris, F-75205 Paris 13, France. [Aghanim, N.] Aalto Univ, Metsahovi Radio Observ, Aalto 00076, Finland. [Aghanim, N.] Dept Radio Sci & Engn, Aalto 00076, Finland. [Armitage-Caplan, C.] African Inst Math Sci, ZA-7701 Cape Town, Rondebosh, South Africa. [Aghanim, N.; Polenta, G.] Agenzia Spaziale Italiana Sci Data Ctr, I-00133 Rome, Italy. 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[Bertincourt, B.; Frailis, M.; Franceschi, E.; Galeotta, S.; Ganga, K.; Giard, M.; Giardino, G.; Giraud-Heraud, Y.] Univ Paris 06, UMR7095, F-75014 Paris, France. [Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Gonzalez-Nuevo, J.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France. [Battaner, E.] Univ Granada, Dept Fis Teer & Cosmos, E-18071 Granada, Spain. [Gorski, K. M.] Univ Warsaw Observ, PL-00478 Warsaw, Poland. RP Perdereau, O (reprint author), Univ Paris 11, CNRS, IN2P3, LAL, Bat 425, F-91898 Orsay, France. EM guilaine.lagache@ias.u-psud.fr; perdereau@lal.in2p3.fr RI Remazeilles, Mathieu/N-1793-2015; Tomasi, Maurizio/I-1234-2016; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; Valiviita, Jussi/A-9058-2016; Mazzotta, Pasquale/B-1225-2016; Kurki-Suonio, Hannu/B-8502-2016; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Martinez-Gonzalez, Enrique/E-9534-2015; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Pearson, Timothy/N-2376-2015; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Barreiro, Rita Belen/N-5442-2014; OI de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Galeotta, Samuele/0000-0002-3748-5115; Pasian, Fabio/0000-0002-4869-3227; Tomasi, Maurizio/0000-0002-1448-6131; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; De Zotti, Gianfranco/0000-0003-2868-2595; Lopez-Caniego, Marcos/0000-0003-1016-9283; Masi, Silvia/0000-0001-5105-1439; Valiviita, Jussi/0000-0001-6225-3693; Mazzotta, Pasquale/0000-0002-5411-1748; Kurki-Suonio, Hannu/0000-0002-4618-3063; Vielva, Patricio/0000-0003-0051-272X; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Pearson, Timothy/0000-0001-5213-6231; Gruppuso, Alessandro/0000-0001-9272-5292; Savini, Giorgio/0000-0003-4449-9416; Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Ricciardi, Sara/0000-0002-3807-4043; Villa, Fabrizio/0000-0003-1798-861X; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Umana, Grazia/0000-0002-6972-8388; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099 FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR (Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC (Spain); MICINN (Spain); JA (Spain); Tekes (Finland); AoF (Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); PRACE (EU) FX The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN and JA (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members with the technical or scientific activities they have been involved into, can be found at http://www.rssd.esa.int/index.php?project=PLANCK&page=PlanckCollaboratio n NR 67 TC 70 Z9 69 U1 5 U2 14 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A8 DI 10.1051/0004-6361/201321538 PG 25 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600011 ER PT J AU Ade, PAR Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, E Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Battaner, E Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bond, JR Borrill, J Bouchet, FR Bowyer, JW Bridges, M Bucher, M Burigana, C Cardoso, JE Catalano, A Challinor, A Chamballu, A Chary, RR Chiang, HC Chiang, LY Christensen, PR Church, S Clements, DL Colombi, S Colombo, LPL Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, E Danese, L Davies, RD de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Delouis, JM Desert, FX Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Dunkley, J Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Finelli, F Forni, O Frailis, M Fraisse, AA Franceschi, E Galeotta, S Ganga, K Giard, M Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Gudmundsson, JE Haissinski, J Hansen, FK Hanson, D Harrison, D Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hou, Z Hovest, W Huffenberger, KM Jaffe, AH Jaffe, TR Jones, WC Juvela, M Keihanen, E Keskitalo, R Kisner, TS Kneiss, R Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Leonardi, R Leroy, C Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF MacTavish, CJ Maffei, B Mandolesi, N Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matsumura, T Matthai, E Mazzotta, P McGehee, P Melchiorri, A Mendes, L Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, MA Moneti, A Montier, L Morgante, G Mortlock, D Munshi, D Murphy, JA Naselsky, P Nati, E Natoli, P Netterfield, CB Norgaard-Nielsen, HU Noviello, F Novikov, D Novikov, I Osborne, S Oxborrow, CA Paci, F Pagano, L Pajot, F Paoletti, D Pasian, F Patanchon, G Perdereau, O Perotto, L Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polegre, AM Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Reinecke, M Remazeilles, M Renault, C Ricciardi, S Riller, T Ristorcelli, I Rocha, G Rosset, C Roudier, G Rowan-Robinson, M Rusholme, B Sandri, M Santos, D Sauve, A Savini, G Scott, D Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sureau, E Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Tomasi, M Tristram, M Tucci, M Umana, G Valenziano, L Valiviita, J Van Tent, B Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD Yvon, D Zacchei, A Zonca, A AF Ade, P. A. R. Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, E. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Battaner, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bond, J. R. Borrill, J. Bouchet, F. R. Bowyer, J. W. Bridges, M. Bucher, M. Burigana, C. Cardoso, J. -E Catalano, A. Challinor, A. Chamballu, A. Chary, R. -R. Chiang, H. C. Chiang, L. -Y Christensen, P. R. Church, S. Clements, D. L. Colombi, S. Colombo, L. P. L. Couchot, F. Coulais, A. Crill, B. P. Curto, A. Cuttaia, E. Danese, L. Davies, R. D. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Delouis, J. -M. Desert, F. -X. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dunkley, J. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Finelli, F. Forni, O. Frailis, M. Fraisse, A. A. Franceschi, E. Galeotta, S. Ganga, K. Giard, M. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Gudmundsson, J. E. Haissinski, J. Hansen, F. K. Hanson, D. Harrison, D. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hou, Z. Hovest, W. Huffenberger, K. M. Jaffe, A. H. Jaffe, T. R. Jones, W. C. Juvela, M. Keihanen, E. Keskitalo, R. Kisner, T. S. Kneiss, R. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leonardi, R. Leroy, C. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. MacTavish, C. J. Maffei, B. Mandolesi, N. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matsumura, T. Matthai, E. Mazzotta, P. McGehee, P. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Miville-Deschenes, M. -A. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Munshi, D. Murphy, J. A. Naselsky, P. Nati, E. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novikov, I. Osborne, S. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paoletti, D. Pasian, F. Patanchon, G. Perdereau, O. Perotto, L. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polegre, A. M. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Reinecke, M. Remazeilles, M. Renault, C. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Rosset, C. Roudier, G. Rowan-Robinson, M. Rusholme, B. Sandri, M. Santos, D. Sauve, A. Savini, G. Scott, D. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sureau, E. Sutton, D. Suur-Uski, A-S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Tomasi, M. Tristram, M. Tucci, M. Umana, G. Valenziano, L. Valiviita, J. Van Tent, B. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. Yvon, D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. VII. HFI time response and beams SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE cosmic background radiation; cosmology: observations; instrumentation: detectors; surveys ID PRE-LAUNCH STATUS; POWER SPECTRUM; MAP-MAKING; MICROWAVE; CALIBRATION; PLANETS; CMB AB This paper characterizes the effective beams, the effective beam window functions and the associated errors for the Planck High Frequency Instrument (HFI) detectors. The effective beam is the angular response including the effect of the optics, detectors, data processing and the scan strategy. The window function is the representation of this beam in the harmonic domain which is required to recover an unbiased measurement of the cosmic microwave background angular power spectrum. The HFI is a scanning instrument and its effective beams are the convolution of: a) the optical response of the telescope and feeds; b) the processing of the time-ordered data and deconvolution of the bolometric and electronic transfer function; and c) the merging of several surveys to produce maps. The time response transfer functions are measured using observations of Jupiter and Saturn and by minimizing survey difference residuals. The scanning beam is the post-deconvolution angular response of the instrument, and is characterized with observations of Mars. The main beam solid angles are determined to better than 0.5% at each HFI frequency band. Observations of Jupiter and Saturn limit near sidelobes (within 5 degrees) to about 0.1% of the total solid angle. Time response residuals remain as long tails in the scanning beams, but contribute less than 0.1% of the total solid angle. The bias and uncertainty in the beam products are estimated using ensembles of simulated planet observations that include the impact of instrumental noise and known systematic effects. The correlation structure of these ensembles is well-described by five errors eigenmodes that are sub-dominant to sample variance and instrumental noise in the harmonic domain. A suite of consistency tests provide confidence that the error model represents a sufficient description of the data. The total error in the effective beam window functions is below 1% at 100 GHz up to multiple l similar to 1500, below 0.5% at 143 and 217 GHz up to l similar to 2000. C1 [Bucher, M.; Cardoso, J. -E; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Piat, M.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, Observ Paris, Sorbonne Paris Cite, CNRS IN2P3,CEA lrfu,APC, F-75205 Paris 13, France. [Poutanen, T.] Aalto Univ, Metsahovi Radio Observ, Kylmala 02540, Finland. [Kunz, M.] African Inst Math Sci, Cape Town, South Africa. [Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana, Sci Data Ctr, I-00133 Rome, Italy. [Mandolesi, N.] Agenzia Spaziale Italiana, I-00198 Rome, Italy. [Ashdown, M.; Bridges, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 0HE, England. [Chiang, H. C.] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, ZA-4000 Durban, South Africa. [Kneiss, R.] ALMA Santiago Cent Off, Santiago 0355, Chile. [Bond, J. R.; Hanson, D.; Martin, P. G.; Miville-Deschenes, M. -A.] Univ Toronto, CITA, Toronto, ON M5S 3H8, Canada. [Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Leroy, C.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.; Sauve, A.] CNRS, TRAP, F-31028 Toulouse 4, France. [Bock, J. J.; Dore, O.; Hildebrandt, S. R.; Matsumura, T.; Prezeau, G.; Rocha, G.] CALTECH, Pasadena, CA 91125 USA. [Challinor, A.; Shellard, E. 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[Scott, D.] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V5Z 1M9, Canada. [Colombo, L. P. L.; Pierpaoli, E.] Univ So Calif, Dept Phys & Astron, Dana & David Dornsife Coll Letter Arts & Sci, Los Angeles, CA 90089 USA. [Benoit-Levy, A.] UCL, Dept Phys & Astron, London WC1E 6BT, England. [Huffenberger, K. M.] Florida State Univ, Dept Phys, Tallahassee, FL 32306 USA. [Juvela, M.; Keihanen, E.; Kurki-Suonio, H.; Poutanen, T.; Suur-Uski, A-S.; Valiviita, J.] Univ Helsinki, Dept Phys, FIN-00014 Helsinki, Finland. [Chiang, H. C.; Fraisse, A. A.; Gudmundsson, J. E.; Jones, W. C.] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA. [Hou, Z.; Knox, L.] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA. [Lubin, P. M.; Zonca, A.] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA. [Wandelt, B. D.] Univ Illinois UrbanaChampaign, Dept Phys, Urbana, IL USA. [Liguori, M.; Matarrese, S.] Univ Padua, Dipartimento Fis & Astron G Galilei, I-35131 Padua, Italy. 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[Melchiorri, A.; Pagano, L.] Univ Roma La Sapienza, Ist Nazl Fis Nucl, Sez Roma 1, I-00185 Rome, Italy. [Desert, F. -X.; Ponthieu, N.] Univ Grenoble 1, CNRS INSU, UMR 5274, Inst Planetol & Astrophys Grenoble, F-38041 Grenoble, France. [Mitra, S.] IUCAA, Pune 411007, Maharashtra, India. [Bowyer, J. W.; Clements, D. L.; Jaffe, A. H.; Mortlock, D.; Novikov, D.; Rowan-Robinson, M.] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, London SW7 2AZ, England. [Chary, R. -R.; McGehee, P.; Rusholme, B.] CALTECH, Ctr Infrared Proc & Anal, Pasadena, CA 91125 USA. [Benoit, A.] Univ Grenoble 1, CNRS, Inst Neel, F-38042 Grenoble, France. [Dole, H.] Inst Univ France, F-75005 Paris, France. [Aghanim, N.; Aumont, J.; Chamballu, A.; Dole, H.; Douspis, M.; Kunz, M.; Lagache, G.; Leroy, C.; Miville-Deschenes, M. -A.; Pajot, F.; Ponthieu, N.; Puget, J. -L.; Remazeilles, M.] Univ Paris 11, CNRS, Inst Astrophys Spatiale, UMR 8617, F-91405 Orsay, France. [Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Cardoso, J. -E; Delouis, J. -M.; Hivon, E.; Moneti, A.; Prunet, S.; Sygnet, J. -F.; Wandelt, B. D.] CNRS, Inst Astrophys Paris, UMR 7095, F-75014 Paris, France. [Popa, L.] Inst Space Sci, Bucharest 077125, Romania. [Chiang, L. -Y] Acad Sinica, Inst Astron & Astrophys, Taipei 10617, Taiwan. [Bridges, M.; Challinor, A.; Efstathiou, G.; Gratton, S.; Harrison, D.; Migliaccio, M.; Sutton, D.] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England. [Eriksen, H. K.; Hansen, F. K.; Lilje, P. B.; Valiviita, J.] Univ Oslo, Inst Theoret Astrophys, N-0315 Oslo, Norway. [Barreiro, R. B.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Vielva, P.] Univ Cantabria, CSIC, Inst Fis Cantabria, E-39005 Santander, Spain. [Bock, J. J.; Colombo, L. P. L.; Crill, B. P.; Dore, O.; Gorski, K. M.; Hanson, D.; Holmes, W. A.; Lawrence, C. R.; Mitra, S.; Pietrobon, D.; Prezeau, G.; Rocha, G.; Roudier, G.; Wade, L. A.] CALTECH, Jet Prop Lab, Pasadena, CA 91125 USA. [Davies, R. D.; Maffei, B.; Noviello, F.; Remazeilles, M.] Univ Manchester, Jodrell Bank, Ctr Astrophys, Sch Phys & Astron, Manchester M13 9PL, Lancs, England. [Ashdown, M.; Bridges, M.; Challinor, A.; Gratton, S.; Harrison, D.; Lasenby, A.; MacTavish, C. J.; Migliaccio, M.; Stolyarov, V.; Sutton, D.] Kavli Inst Cosmol Cambridge, Cambridge CB3 0HA, England. [Couchot, F.; Haissinski, J.; Henrot-Versille, S.; Perdereau, O.; Plaszczynski, S.; Tristram, M.; Tucci, M.] Univ Paris 11, CNRS, IN2P3, LAL, F-91898 Orsay, France. [Catalano, A.; Coulais, A.; Lamarre, J. -M.; Roudier, G.] CNRS, Observ Paris, LERMA, F-75014 Paris, France. [Arnaud, M.; Bobin, J.; Chamballu, A.; Marshall, D. J.; Pratt, G. W.; Starck, J. -L.; Sureau, E.] Univ Paris Diderot, CNRS, CEA DSM, Lab AIM,IRFU Serv Astrophys, F-91191 Gif Sur Yvette, France. [Cardoso, J. -E] CNRS, Lab Traitement & Commun Informat, UMR 5141, F-75634 Paris 13, France. [Cardoso, J. -E] Telecom Paris Tech, F-75634 Paris 13, France. [Catalano, A.; Macias-Perez, J. F.; Perotto, L.; Renault, C.; Santos, D.] Univ Grenoble 1, Inst Natl Polytech Grenoble, Lab Phys Subatom & Cosmol, CNRS IN2P3, F-38026 Grenoble, France. [Van Tent, B.] Univ Paris 11, Phys Theor Lab, F-91405 Orsay, France. [Van Tent, B.] CNRS, F-91405 Orsay, France. [Kisner, T. S.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Ensslin, T. A.; Hernandez-Monteagudo, C.; Hovest, W.; Knoche, J.; Matthai, E.; Rachen, J. P.; Reinecke, M.; Riller, T.] Max Planck Inst Astrophys, D-85741 Garching, Germany. [Hanson, D.] McGill Univ, McGill Phys, Montreal, PQ H3A 2T8, Canada. [Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Kildare, Ireland. [Christensen, P. R.; Naselsky, P.; Novikov, I.] Niels Bohr Inst, DK-2100 Copenhagen, Denmark. [Crill, B. P.] CALTECH, Observat Cosmol, Pasadena, CA 91125 USA. [Savini, G.] UCL, Opt Sci Lab, London, England. [Lesgourgues, J.] Ecole Polytech Fed Lausanne, SB ITP LPPC, CH-1015 Lausanne, Switzerland. [Baccigalupi, C.; Bielewicz, P.; Danese, L.; de Zotti, G.; Gonzalez-Nuevo, J.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sect, I-34136 Trieste, Italy. [Ade, P. A. R.; Munshi, D.; Spencer, L. D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales. [Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA. [Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Karachai Cherkessian 369167, Russia. [Church, S.; Osborne, S.] Stanford Univ, Dept Phys, Stanford, CA USA. [Armitage-Caplan, C.; Dunkley, J.] Univ Oxford, Sub Dept Astrophys, Oxford OX1 3RH, England. [Lesgourgues, J.] CERN, Div Theory, PH TH, CH-1211 Geneva 23, Switzerland. [Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Delouis, J. -M.; Hivon, E.; Prunet, S.; Wandelt, B. D.] Univ Paris 06, UMR7095, F-75014 Paris, France. [Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Leroy, C.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.; Sauve, A.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France. [Battaner, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, E-18071 Granada, Spain. [Gorski, K. M.] Univ Warsaw Observ, PL-00478 Warsaw, Poland. RP Crill, BP (reprint author), CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91125 USA. EM bcrill@jpl.nasa.gov RI Barreiro, Rita Belen/N-5442-2014; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; Remazeilles, Mathieu/N-1793-2015; Mazzotta, Pasquale/B-1225-2016; Kurki-Suonio, Hannu/B-8502-2016; Tomasi, Maurizio/I-1234-2016; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Martinez-Gonzalez, Enrique/E-9534-2015; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Valiviita, Jussi/A-9058-2016; OI Finelli, Fabio/0000-0002-6694-3269; Umana, Grazia/0000-0002-6972-8388; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Lopez-Caniego, Marcos/0000-0003-1016-9283; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Galeotta, Samuele/0000-0002-3748-5115; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; De Zotti, Gianfranco/0000-0003-2868-2595; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Mazzotta, Pasquale/0000-0002-5411-1748; Kurki-Suonio, Hannu/0000-0002-4618-3063; Tomasi, Maurizio/0000-0002-1448-6131; Vielva, Patricio/0000-0003-0051-272X; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Gruppuso, Alessandro/0000-0001-9272-5292; Valiviita, Jussi/0000-0001-6225-3693; Savini, Giorgio/0000-0003-4449-9416; Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Bouchet, Francois/0000-0002-8051-2924; Ricciardi, Sara/0000-0002-3807-4043; Villa, Fabrizio/0000-0003-1798-861X; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794 FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR (Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC (Spain); MICINN (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF (Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); PRACE (EU) FX The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.sciops.esa.int/index.php?project=planck&page=Planck-Collabora tion. NR 68 TC 57 Z9 56 U1 2 U2 11 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A7 DI 10.1051/0004-6361/201321535 PG 31 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600010 ER PT J AU Ade, PAR Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, E Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Bartlett, JG Basak, S Battaner, E Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bonaldi, A Bonavera, L Bond, JR Borrill, J Bouchet, FR Bridges, M Bucher, M Burigana, C Butler, RC Cardoso, JF Catalano, A Challinor, A Chamballu, A Chiang, HC Chiang, LY Christensen, PR Church, S Clements, DL Colombi, S Colombo, LPL Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Danese, L Davies, RD Davis, RJ de Bernardis, P de Rosa, A de Zotti, G Dechelette, T Delabrouille, J Delouis, JM Desert, FX Dickinson, C Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Dunkley, J Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Finelli, F Forni, O Frailis, M Franceschi, E Galeotta, S Ganga, K Giard, M Giardino, G Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Gudmundsson, JE Hansen, EK Hanson, D Harrison, D Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Ho, S Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Jaffe, AH Jaffe, TR Jones, WC Juvela, M Keihanen, E Keskitalo, R Kisner, TS Kneissl, R Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lahteenmaki, A Lamarre, JM Lasenby, A Laureijs, RJ Lavabre, A Lawrence, CR Leahy, JP Leonardi, R Leon-Tavares, J Lesgourgues, J Lewis, A Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maffei, B Maino, D Mandolesi, N Mangilli, A Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, E Mazzotta, P Melchiorri, A Mendes, L Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, MA Moneti, A Montier, L Morgante, G Mortlock, D Moss, A Munshi, D Murphy, JA Naselsky, P Nati, F Natoli, P Netterfield, CB Norgaard-Nielsen, HU Noviello, F Novikov, D Novikov, I Osborne, S Oxborrow, CA Paci, F Pagano, L Pajot, F Paoletti, D Partridge, B Pasian, F Patanchon, G Perdereau, O Perotto, L Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeaul, G Prunet, S Puget, JL Pullen, AR Rachen, JP Rebolo, R Reinecke, M Remazeilles, M Renault, C Ricciardi, S Riller, T Ristorcelli, I Rocha, G Rosset, C Roudier, G Rowan-Robinson, M Rubino-Martin, JA Rusholme, B Sandri, M Santos, D Savini, G Scott, D Seiffert, MD Shellard, EPS Smith, K Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sunyaev, R Sureau, E Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Tuovinen, J Umana, G Valenziano, L Valiviita, J Van Tent, B Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD White, M White, SDM Yvon, D Zacchei, A Zonca, A AF Ade, P. A. R. Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, E. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Bartlett, J. G. Basak, S. Battaner, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bonaldi, A. Bonavera, L. Bond, J. R. Borrill, J. Bouchet, F. R. Bridges, M. Bucher, M. Burigana, C. Butler, R. C. Cardoso, J. -F. Catalano, A. Challinor, A. Chamballu, A. Chiang, H. C. Chiang, L. -Y Christensen, P. R. Church, S. Clements, D. L. Colombi, S. Colombo, L. P. L. Couchot, F. Coulais, A. Crill, B. P. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. Davis, R. J. de Bernardis, P. de Rosa, A. de Zotti, G. Dechelette, T. Delabrouille, J. Delouis, J. -M. Desert, F. -X. Dickinson, C. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dunkley, J. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Finelli, F. Forni, O. Frailis, M. Franceschi, E. Galeotta, S. Ganga, K. Giard, M. Giardino, G. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Gudmundsson, J. E. Hansen, F. K. Hanson, D. Harrison, D. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Ho, S. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Jaffe, A. H. Jaffe, T. R. Jones, W. C. Juvela, M. Keihanen, E. Keskitalo, R. Kisner, T. S. Kneissl, R. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Lahteenmaki, A. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lavabre, A. Lawrence, C. R. Leahy, J. P. Leonardi, R. Leon-Tavares, J. Lesgourgues, J. Lewis, A. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maffei, B. Maino, D. Mandolesi, N. Mangilli, A. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Miville-Deschenes, M. -A. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Moss, A. Munshi, D. Murphy, J. A. Naselsky, P. Nati, F. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novikov, I. Osborne, S. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paoletti, D. Partridge, B. Pasian, F. Patanchon, G. Perdereau, O. Perotto, L. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeaul, G. Prunet, S. Puget, J. -L. Pullen, A. R. Rachen, J. P. Rebolo, R. Reinecke, M. Remazeilles, M. Renault, C. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Rosset, C. Roudier, G. Rowan-Robinson, M. Rubino-Martin, J. A. Rusholme, B. Sandri, M. Santos, D. Savini, G. Scott, D. Seiffert, M. D. Shellard, E. P. S. Smith, K. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sunyaev, R. Sureau, E. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Tuovinen, J. Umana, G. Valenziano, L. Valiviita, J. Van Tent, B. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. White, M. White, S. D. M. Yvon, D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. XVII. Gravitational lensing by large-scale structure SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE gravitational lensing: weak; methods: data analysis; cosmic background radiation; large-scale structure of Universe ID MICROWAVE BACKGROUND ANISOTROPIES; SOUTH-POLE TELESCOPE; PROBE WMAP OBSERVATIONS; DIGITAL SKY SURVEY; POWER SPECTRUM; CROSS-CORRELATION; GALAXY CLUSTERS; NON-GAUSSIANITY; DAMPING TAIL; MAPS AB On the arcminute angular scales probed by Planck, the cosmic microwave background (CMB) anisotropies are gently perturbed by gravitational lensing. Here we present a detailed study of this effect, detecting lensing independently in the 100, 143, and 217 GHz frequency bands with an overall significance of greater than 25 sigma. We use the temperature-gradient correlations induced by lensing to reconstruct a (noisy) map of the CMB lensing potential, which provides an integrated measure of the mass distribution back to the CMB last-scattering surface. Our lensing potential map is significantly correlated with other tracers of mass, a fact which we demonstrate using several representative tracers of large-scale structure. We estimate the power spectrum of the lensing potential, finding generally good agreement with expectations from the best-fitting ACDM model for the Planck temperature power spectrum, showing that this measurement at z = 1100 correctly predicts the properties of the lower-redshift, later-time structures which source the lensing potential. When combined with the temperature power spectrum, our measurement provides degeneracy-breaking power for parameter constraints; it improves CMB-alone constraints on curvature by a factor of two and also partly breaks the degeneracy between the amplitude of the primordial perturbation power spectrum and the optical depth to reionization, allowing a measurement of the optical depth to reionization which is independent of large-scale polarization data. Discarding scale information, our measurement corresponds to a 4% constraint on the amplitude of the lensing potential power spectrum, or a 2% constraint on the root-mean-squared amplitude of matter fluctuations at z similar to 2. C1 [Bartlett, J. G.; Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Piat, M.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, Observ Paris, Sorbonne Paris Cite, CNRS,IN2P3,CEA,lrfu,APC, F-75205 Paris 13, France. [Lahteenmaki, A.; Leon-Tavares, J.; Poutanen, T.] Aalto Univ Metsahovi Radio Observ, Kylmala 02540, Finland. [Kunz, M.] African Inst Math Sci, Cape Town, South Africa. [Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana Sci Data Ctr, I-00133 Rome, Italy. [Mandolesi, N.] Agenzia Spaziale Italiana, Rome, Italy. [Ashdown, M.; Bridges, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 0HE, England. [Chiang, H. C.] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, ZA-4000 Durban, South Africa. [Kneissl, R.] Atacama Large Millimeter Submillimeter Array, ALMA Santiago Cent Off, Santiago 7630355, Chile. [Bond, J. R.; Hanson, D.; Martin, P. G.; Miville-Deschenes, M. -A.] Univ Toronto, CITA, Toronto, ON M5S 3H8, Canada. [Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] CNRS, IRAP, F-31028 Toulouse 4, France. [Bock, J. J.; Dore, O.; Hildebrandt, S. R.; Prezeaul, G.; Rocha, G.; Seiffert, M. D.] CALTECH, Pasadena, CA 91125 USA. [Challinor, A.; Shellard, E. P. S.] Univ Cambridge, Ctr Theoret Cosmol, DAMTP, Cambridge CB3 0WA, England. [Hernandez-Monteagudo, C.] Ctr Estudios Fis Cosmos Aragon, Teruel 44001, Spain. [Borrill, J.; Keskitalo, R.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 94720 USA. [Rebolo, R.] CSIC, Madrid, Spain. [Chamballu, A.; Yvon, D.] CEA Saclay, DMS, SPP, Irfu, F-91191 Gif Sur Yvette, France. [Hornstrup, A.; Linden-Vornle, M.; Norgaard-Nielsen, H. U.; Oxborrow, C. A.] Tech Univ Denmark, Natl Space Inst, DTU Space, DK-2800 Lyngby, Denmark. [Kunz, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, CH-1211 Geneva 4, Switzerland. [Atrio-Barandela, E.] Univ Salamanca, Dept Fis Fundamental, Fac Ciencias, E-37008 Salamanca, Spain. [Toffolatti, L.] Univ Oviedo, Dept Fis, E-33007 Oviedo, Spain. [Netterfield, C. B.] Univ Toronto, Dept Astron & Astrophys, Toronto, ON, Canada. [Rachen, J. P.] Radboud Univ Nijmegen, Dept Astrophys, IMAPP, NL-6500 GL Nijmegen, Netherlands. [Keskitalo, R.] Univ Calif Berkeley, Dept Elect Engn & Comp Sci, Berkeley, CA 94720 USA. [Scott, D.] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V5Z 1M9, Canada. [Colombo, L. P. L.; Pierpaoli, E.] Univ So Calif, Dept Phys & Astron, Dana & David Dornsife Coll Letter Arts & Sci, Los Angeles, CA 90089 USA. [Benoit-Levy, A.] UCL, Dept Phys & Astron, London WC1E 6BT, England. [Lewis, A.] Univ Sussex, Dept Phys & Astron, Brighton BN1 9QH, E Sussex, England. [Ho, S.] Carnegie Mellon Univ, Dept Phys, Pittsburgh, PA 15213 USA. [Huffenberger, K. M.] Florida State Univ, Dept Phys, Tallahassee, FL 32306 USA. [Juvela, M.; Keihanen, E.; Kurki-Suonio, H.; Poutanen, T.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Dept Phys, Helsinki, Finland. [Chiang, H. C.; Gudmundsson, J. E.; Jones, W. 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EM benabed@iap.fr; dhanson@physics.mcgill.ca RI Butler, Reginald/N-4647-2015; Remazeilles, Mathieu/N-1793-2015; Mazzotta, Pasquale/B-1225-2016; Kurki-Suonio, Hannu/B-8502-2016; Tomasi, Maurizio/I-1234-2016; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; bonavera, laura/E-9368-2017; Pullen, Anthony/I-7007-2015; White, Martin/I-3880-2015; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Valiviita, Jussi/A-9058-2016; Lahteenmaki, Anne/L-5987-2013; Toffolatti, Luigi/K-5070-2014; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Martinez-Gonzalez, Enrique/E-9534-2015; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Barreiro, Rita Belen/N-5442-2014; OI Galeotta, Samuele/0000-0002-3748-5115; Frailis, Marco/0000-0002-7400-2135; De Zotti, Gianfranco/0000-0003-2868-2595; Polenta, Gianluca/0000-0003-4067-9196; Butler, Reginald/0000-0003-4366-5996; Lopez-Caniego, Marcos/0000-0003-1016-9283; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Maris, Michele/0000-0001-9442-2754; Mazzotta, Pasquale/0000-0002-5411-1748; Kurki-Suonio, Hannu/0000-0002-4618-3063; Tomasi, Maurizio/0000-0002-1448-6131; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; bonavera, laura/0000-0001-8039-3876; Rubino-Martin, Jose Alberto/0000-0001-5289-3021; Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834; Pullen, Anthony/0000-0002-2091-8738; White, Martin/0000-0001-9912-5070; Gruppuso, Alessandro/0000-0001-9272-5292; Valiviita, Jussi/0000-0001-6225-3693; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Savini, Giorgio/0000-0003-4449-9416; Villa, Fabrizio/0000-0003-1798-861X; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; Zacchei, Andrea/0000-0003-0396-1192; Gregorio, Anna/0000-0003-4028-8785; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Ricciardi, Sara/0000-0002-3807-4043; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Umana, Grazia/0000-0002-6972-8388; Scott, Douglas/0000-0002-6878-9840 FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); INAF (Italy); CNR (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC (Spain); MICINN (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF (Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); PRACE (EU); Office of Science of the US Department of Energy [DE-AC02-05CH11231]; IN2P3 Computer Center; CNES; Science and Technology Facilities Council [ST/I000976/1] FX The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.soirees.esa.int/index.php?project=planck&pagess-Planck_Collab oration. Some of the results in this paper have been derived using the HEALPix package (Gorski et al. 2005). This research used resources of the National Energy Research Scientific Computing Center, which is supported by the Office of Science of the US Department of Energy under Contract No. DE-AC02-05CH11231, as well as of the IN2P3 Computer Center (http://cc.in2p3.fr) and the Planck-HFI data processing center infrastructures hosted at the Institut d'Astrophysique de Paris (France) and financially supported by CNES. We acknowledge support from the Science and Technology Facilities Council [grant number ST/I000976/1]. NR 120 TC 198 Z9 197 U1 3 U2 20 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A17 DI 10.1051/0004-6361/201321543 PG 39 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600013 ER PT J AU Ade, PAR Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandelals, E Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Bartlett, JG Bartlett, JG Bartolo, N Battaner, E Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bonaldi, A Bonavera, L Bond, JR Borrill, J Bouchet, FR Bridges, M Bucher, M Burigana, C Butler, RC Cardoso, JF Catalano, A Challinor, A Chamballu, A Chiang, HC Chiang, LY Christensen, PR Church, S Clements, DL Colombi, S Colombo, LPL Couchot, E Coulais, A Crill, BP Curto, A Cuttaia, E Danese, L Davies, RD Davis, RJ de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Delouis, JM Desert, FX Dickinson, C Diego, JM Dolag, K Dole, H Donzelli, S Dore, O Douspis, M Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Fergusson, J Finelli, F Fomi, O Fosalba, P Frailis, M Franceschi, E Frommert, M Galeotta, S Ganga, K Genova-Santos, RT Giard, M Giardino, G Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Hansen, EK Hanson, D Harrison, D Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Ho, S Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Ilic, S Jaffe, AH Jaffe, TR Jasche, J Jones, WC Juvela, M Keihanen, E Keskitalo, R Kisner, TS Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lahteenmaki, A Lamarre, JM Langer, M Lasenby, A Laureijs, RJ Lawrence, CR Leahy, JP Leonardi, R Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maffei, B Maino, D Mandolesi, N Mangilli, A Marcos-Caballero, A Maris, M Marshall, DJ Martins, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthais, E Mazzotta, P Meinhold, PR Melchiorri, A Mendes, L Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, MA Moneti, A Montier, L Morgante, G Mortlock, D Moss, A Munshi, D Naselsky, P Nati, F Natoli, P Netterfield, CB Norgaard-Nielsen, HU Noviello, F Novikov, D Novikov, I Osborne, S Oxborrow, CA Paci, E Pagano, L Pajot, F Paoletti, D Partridge, B Pasian, F Patanchon, G Perdereau, O Perotto, L Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Racine, B Rebolo, R Reinecke, M Remazeilles, M Renault, C Renzi, A Ricciardi, S Riller, T Ristorcelli, I Rocha, G Rosset, C Roudier, G Rowan-Robinson, M Rubino-Martin, JA Rusholme, B Sandri, M Santos, D Savini, G Schaefer, BM Schiavon, F Scott, D Seiffert, MD Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sunyaev, R Sureau, F Sutter, P Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Tuovinen, J Umana, G Valenziano, L Valiviita, J Van Tent, B Varis, J Viel, M Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD White, M Xia, JQ Yvon, D Zacchei, A Zonca, A AF Ade, P. A. R. Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandelals, E. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Bartlett, J. G. Bartlett, J. G. Bartolo, N. Battaner, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bonaldi, A. Bonavera, L. Bond, J. R. Borrill, J. Bouchet, F. R. Bridges, M. Bucher, M. Burigana, C. Butler, R. C. Cardoso, J. -F. Catalano, A. Challinor, A. Chamballu, A. Chiang, H. C. Chiang, L. -Y. Christensen, P. R. Church, S. Clements, D. L. Colombi, S. Colombo, L. P. L. Couchot, E. Coulais, A. Crill, B. P. Curto, A. Cuttaia, E. Danese, L. Davies, R. D. Davis, R. J. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Delouis, J. -M. Desert, F. -X. Dickinson, C. Diego, J. M. Dolag, K. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Fergusson, J. Finelli, F. Fomi, O. Fosalba, P. Frailis, M. Franceschi, E. Frommert, M. Galeotta, S. Ganga, K. Genova-Santos, R. T. Giard, M. Giardino, G. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Hansen, E. K. Hanson, D. Harrison, D. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Ho, S. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Ilic, S. Jaffe, A. H. Jaffe, T. R. Jasche, J. Jones, W. C. Juvela, M. Keihanen, E. Keskitalo, R. Kisner, T. S. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Laehteenmaeki, A. Lamarre, J. -M. Langer, M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leahy, J. P. Leonardi, R. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maffei, B. Maino, D. Mandolesi, N. Mangilli, A. Marcos-Caballero, A. Maris, M. Marshall, D. J. Martins, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthais, E. Mazzotta, P. Meinhold, P. R. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Miville-Deschenes, M. -A. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Moss, A. Munshi, D. Naselsky, P. Nati, F. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novikov, I. Osborne, S. Oxborrow, C. A. Paci, E. Pagano, L. Pajot, F. Paoletti, D. Partridge, B. Pasian, F. Patanchon, G. Perdereau, O. Perotto, L. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Racine, B. Rebolo, R. Reinecke, M. Remazeilles, M. Renault, C. Renzi, A. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Rosset, C. Roudier, G. Rowan-Robinson, M. Rubino-Martin, J. A. Rusholme, B. Sandri, M. Santos, D. Savini, G. Schaefer, B. M. Schiavon, F. Scott, D. Seiffert, M. D. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sunyaev, R. Sureau, F. Sutter, P. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Tuovinen, J. Umana, G. Valenziano, L. Valiviita, J. Van Tent, B. Varis, J. Viel, M. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. White, M. Xia, J. -Q. Yvon, D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. XIX. The integrated Sachs-Wolfe effect SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE cosmic background radiation; large-scale structure of Universe; dark energy; galaxies: clusters: general; methods: data analysis ID DIGITAL SKY SURVEY; PRIMORDIAL NON-GAUSSIANITY; DARK ENERGY CONSTRAINTS; PROBE WMAP OBSERVATIONS; ANGULAR POWER SPECTRUM; CROSS-CORRELATION; RADIO-SOURCES; SPHERICAL WAVELETS; GALAXY SURVEY; DATA RELEASE AB Based on cosmic microwave background (CMB) maps from the 2013 Planck Mission data release, this paper presents the detection of the integrated Sachs-Wolfe (ISW) effect, that is, the correlation between the CMB and large-scale evolving gravitational potentials. The significance of detection ranges from 2 to 4 sigma, depending on which method is used. We investigated three separate approaches, which essentially cover all previous studies, and also break new ground. (i) We correlated the CMB with the Planck reconstructed gravitational lensing potential (for the first time). This detection was made using the lensing-induced bispectrum between the low-l and high-l temperature anisotropies; the correlation between lensing and the ISW effect has a significance close to 2.5 sigma. (ii) We cross-correlated with tracers of large-scale structure, which yielded a significance of about 3 sigma, based on a combination of radio (NVSS) and optical (SDSS) data. (iii) We used aperture photometry on stacked CMB fields at the locations of known large-scale structures, which yielded and confirms a 4 sigma signal, over a broader spectral range, when using a previously explored catalogue, but shows strong discrepancies in amplitude and scale when compared with expectations. More recent catalogues give more moderate results that range from negligible to 2.5 sigma at most, but have a more consistent scale and amplitude, the latter being still slightly higher than what is expected from numerical simulations within Lambda CMD. Where they can be compared, these measurements are compatible with previous work using data from WMAP, where these scales have been mapped to the limits of cosmic variance. Planck's broader frequency coverage allows for better foreground cleaning and confirms that the signal is achromatic, which makes it preferable for ISW detection. As a final step we used tracers of large-scale structure to filter the CMB data, from which we present maps of the ISW temperature perturbation. These results provide complementary and independent evidence for the existence of a dark energy component that governs the currently accelerated expansion of the Universe. C1 [Bartlett, J. 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[Schaefer, B. M.] Heidelberg Univ, Inst Theoret Astrophys, D-69120 Heidelberg, Germany. [Barreiro, R. B.; Bernard, J. -P.; Bielewicz, P.; Fomi, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse, France. [Dolag, K.] Univ Munich, Univ Observ, D-81679 Munich, Germany. [Battaner, E.] Univ Granada, Dept Fis Teor & Cosmos, Granada 18071, Spain. [Gorski, K. M.] Univ Warsaw Observ, PL-00478 Warsaw, Poland. RP Vielva, P (reprint author), Univ Cantabria, CSIC, Inst Fis Cantabria, E-39005 Santander, Spain. EM vielva@ifca.unican.es RI Remazeilles, Mathieu/N-1793-2015; Renzi, Alessandro/K-4114-2015; Mazzotta, Pasquale/B-1225-2016; Kurki-Suonio, Hannu/B-8502-2016; Tomasi, Maurizio/I-1234-2016; Fosalba Vela, Pablo/I-5515-2016; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; bonavera, laura/E-9368-2017; Novikov, Dmitry/P-1807-2015; Valiviita, Jussi/A-9058-2016; Lahteenmaki, Anne/L-5987-2013; Toffolatti, Luigi/K-5070-2014; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Langer, Mathieu/C-5100-2013; Martinez-Gonzalez, Enrique/E-9534-2015; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; White, Martin/I-3880-2015; Gruppuso, Alessandro/N-5592-2015; Butler, Reginald/N-4647-2015; Barreiro, Rita Belen/N-5442-2014; OI Masi, Silvia/0000-0001-5105-1439; Rubino-Martin, Jose Alberto/0000-0001-5289-3021; De Zotti, Gianfranco/0000-0003-2868-2595; Lopez-Caniego, Marcos/0000-0003-1016-9283; Scott, Douglas/0000-0002-6878-9840; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Maris, Michele/0000-0001-9442-2754; Renzi, Alessandro/0000-0001-9856-1970; Franceschi, Enrico/0000-0002-0585-6591; Mazzotta, Pasquale/0000-0002-5411-1748; Kurki-Suonio, Hannu/0000-0002-4618-3063; Tomasi, Maurizio/0000-0002-1448-6131; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; bonavera, laura/0000-0001-8039-3876; de Bernardis, Paolo/0000-0001-6547-6446; Valiviita, Jussi/0000-0001-6225-3693; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; Langer, Mathieu/0000-0002-9088-2718; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; White, Martin/0000-0001-9912-5070; Gruppuso, Alessandro/0000-0001-9272-5292; Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Savini, Giorgio/0000-0003-4449-9416; Ricciardi, Sara/0000-0002-3807-4043; Villa, Fabrizio/0000-0003-1798-861X; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Butler, Reginald/0000-0003-4366-5996; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Viel, Matteo/0000-0002-2642-5707; Galeotta, Samuele/0000-0002-3748-5115; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Umana, Grazia/0000-0002-6972-8388; Frailis, Marco/0000-0002-7400-2135 FU ESA; CNES (France); CNRS/INSU- IN2P3-INP (France); ASI (Italy); CNR (Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC (Spain); MICINN (Spain); J.A. (Spain); RES (Spain); Tekes (Finland); AoF (Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); PRACE (EU); Advanced Computing and e-Sciance team at IFCA FX The development of Planck has been supported by: ESA; CNES and CNRS/INSU- IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, J.A. and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found athttp://www.sciops.esa.int/index.php?project=planck&page=Planck_Collabo ration. The modal and KSW bispectrum estimator analysis was performed on the COSMOS supercomputer, part of the STFC DiRAC HPC Facility. We acknowledge the computer resources, technical expertise and assistance provided by the Spanish Supercomputing Network (RES) node at Universidad de Cantarbria, and the support provided by the Advanced Computing and e-Sciance team at IFCA. NR 133 TC 105 Z9 104 U1 4 U2 13 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A19 DI 10.1051/0004-6361/201321526 PG 23 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600005 ER PT J AU Ade, PAR Aghanim, N Argueso, F Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Bartlett, JG Battaner, E Beelen, A Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bonaldi, A Bonavera, L Bond, JR Borrill, J Bouchet, FR Bridges, M Bucher, M Burigana, C Butler, RC Cardoso, JF Carvalho, P Catalano, A Challinor, A Chamballu, A Chen, X Chiang, HC Chiang, LY Christensen, PR Church, S Clemens, M Clements, DL Colombi, S Colombo, LPL Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Danese, L Davies, RD Davis, RJ de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Delouis, JM Desert, FX Dickinson, C Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Finelli, F Forni, O Frailis, M Franceschi, E Galeotta, S Ganga, K Giard, M Giardino, G Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Hansen, FK Hanson, D Harrison, DL Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Jaffe, AH Jaffe, TR Jones, WC Juvela, M Keihanen, E Keskitalo, R Kisner, TS Kneissl, R Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lahteenmaki, A Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Leahy, JP Leonardi, R Leon-Tavares, J Leroy, C Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maffei, B Maino, D Mandolesi, N Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Mazzotta, P McGehee, P Meinhold, PR Melchiorri, A Mendes, L Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, MA Moneti, A Montier, L Morgante, G Mortlock, D Munshi, D Murphy, JA Naselsky, P Nati, F Natoli, P Negrello, M Netterfield, CB Norgaard-Nielsen, HU Noviello, F Novikov, D Novikov, I O'Dwyer, IJ Osborne, S Oxborrow, CA Paci, F Pagano, L Pajot, F Paladini, R Paoletti, D Partridge, B Pasian, F Patanchon, G Pearson, TJ Perdereau, O Perotto, L Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Reach, WT Rebolo, R Reinecke, M Remazeilles, M Renault, C Ricciardi, S Riller, T Ristorcelli, I Rocha, G Rosset, C Roudier, G Rowan-Robinson, M Rubino-Martin, JA Rusholme, B Sandri, M Santos, D Savini, G Scott, D Seiffert, MD Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sunyaev, R Sureau, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Tuovinen, J Turler, M Umana, G Valenziano, L Valiviita, J Van Tent, B Varis, J Vielva, P Villa, F Vittorio, N Wade, LA Walter, B Wandelt, BD Yvon, D Zacchei, A Zonca, A AF Ade, P. A. R. Aghanim, N. Argueeso, F. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Bartlett, J. G. Battaner, E. Beelen, A. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bonaldi, A. Bonavera, L. Bond, J. R. Borrill, J. Bouchet, F. R. Bridges, M. Bucher, M. Burigana, C. Butler, R. C. Cardoso, J. -F. Carvalho, P. Catalano, A. Challinor, A. Chamballu, A. Chen, X. Chiang, H. C. Chiang, L. -Y Christensen, P. R. Church, S. Clemens, M. Clements, D. L. Colombi, S. Colombo, L. P. L. Couchot, F. Coulais, A. Crill, B. P. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. Davis, R. J. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Delouis, J. -M. Desert, F. -X. Dickinson, C. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Finelli, F. Forni, O. Frailis, M. Franceschi, E. Galeotta, S. Ganga, K. Giard, M. Giardino, G. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Hansen, F. K. Hanson, D. Harrison, D. L. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Jaffe, A. H. Jaffe, T. R. Jones, W. C. Juvela, M. Keihanen, E. Keskitalo, R. Kisner, T. S. Kneissl, R. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Lahteenmaki, A. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leahy, J. P. Leonardi, R. Leon-Tavares, J. Leroy, C. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maffei, B. Maino, D. Mandolesi, N. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. McGehee, P. Meinhold, P. R. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Miville-Deschenes, M. -A. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Munshi, D. Murphy, J. A. Naselsky, P. Nati, F. Natoli, P. Negrello, M. Netterfield, C. B. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novikov, I. O'Dwyer, I. J. Osborne, S. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paladini, R. Paoletti, D. Partridge, B. Pasian, F. Patanchon, G. Pearson, T. J. Perdereau, O. Perotto, L. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Reach, W. T. Rebolo, R. Reinecke, M. Remazeilles, M. Renault, C. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Rosset, C. Roudier, G. Rowan-Robinson, M. Rubino-Martin, J. A. Rusholme, B. Sandri, M. Santos, D. Savini, G. Scott, D. Seiffert, M. D. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sunyaev, R. Sureau, F. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. . Tucci, M. Tuovinen, J. Tuerler, M. Umana, G. Valenziano, L. Valiviita, J. Van Tent, B. Varis, J. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Walter, B. Wandelt, B. D. Yvon, D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. XXVIII. The Planck Catalogue of Compact Sources SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE cosmology: observations; radio continuum: general; submillimeter: general ID COEVAL OBSERVATIONS PROJECT; EXTRAGALACTIC POINT SOURCES; MICROWAVE BACKGROUND MAPS; STAR-FORMING GALAXIES; HERSCHEL-ATLAS; RADIO-SOURCES; NEARBY GALAXIES; NUMBER COUNTS; SAMPLE; RELEASE AB The Planck Catalogue of Compact Sources (PCCS) is the catalogue of sources detected in the first 15 months of Planck operations, the "nominal" mission. It consists of nine single-frequency catalogues of compact sources, both Galactic and extragalactic, detected over the entire sky. The PCCS covers the frequency range 30-857 GHz with higher sensitivity (it is 90% complete at 180 mJy in the best channel) and better angular resolution (from 32.88' to 4.33') than previous all-sky surveys in this frequency band. By construction its reliability is >80% and more than 65% of the sources have been detected in at least two contiguous Planck channels. In this paper we present the construction and validation of the PCCS, its contents and its statistical characterization. C1 [Bartlett, J. G.; Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Piat, M.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.] Sorbonne Paris Cite, Univ Paris Diderot, Observ Paris, CNRS IN2P3 CEA lrfu,APC, F-75205 Paris 13, France. [Lahteenmaki, A.; Leon-Tavares, J.; Poutanen, T.] Aalto Univ, Metsahovi Radio Observ, Aalto 00076, Finland. [Lahteenmaki, A.; Leon-Tavares, J.; Poutanen, T.] Dept Radio Sci & Engn, Aalto 00076, Finland. 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[Kisner, T. S.] CNRS, F-91405 Orsay, France. [Ensslin, T. A.; Hernandez-Monteagudo, C.; Hovest, W.; Knoche, J.; Matthai, F.; Rachen, J. P.; Reinecke, M.; Riller, T.; Sunyaev, R.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Hanson, D.] Max Planck Inst Astrophys, D-85741 Garching, Germany. [Tuovinen, J.; Varis, J.] McGill Univ, Montreal, PQ H3A 2T8, Canada. [Tuovinen, J.; Varis, J.] VTT Tech Res Ctr Finland, Milli Lab, Espoo 02044, Finland. [Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Kildare, Ireland. [Christensen, P. R.; Naselsky, P.; Novikov, I.] Niels Bohr Inst, DK-2100 Copenhagen, Denmark. [Crill, B. P.] CALTECH, Observ Cosmol, Pasadena, CA 91125 USA. [Savini, G.] UCL, Opt Sci Lab, London, England. [Lesgourgues, J.] Ecole Polytech Fed Lausanne, SB ITP LPPC, CH-1015 Lausanne, Switzerland. [Baccigalupi, C.; Bobin, J.; Danese, L.; de Zotti, G.; Gonzalez-Nuevo, J.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sect, I-34136 Trieste, Italy. [Ade, P. A. R.; Munshi, D.; Spencer, L. D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales. [Sunyaev, R.] Russian Acad Sci, Space Res Inst IKI, Moscow 117997, Russia. [Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA. [Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz 369167, Russia. [Church, S.; Osborne, S.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA. [Armitage-Caplan, C.] Univ Oxford, Sub Dept Astrophys, Oxford OX1 3RH, England. [Lesgourgues, J.] CERN, PH TH, Div Theory, CH-1211 Geneva 23, Switzerland. [Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Colombi, S.; Delouis, J. -M.; Hivon, E.; Prunet, S.; Wandelt, B. D.] Univ Paris 06, UMR7095, F-75014 Paris, France. [Banday, A. J.; Beelen, A.; Bernard, J. -P.; Bobin, J.; Forni, O.; Giard, M.; Jaffe, T. R.; Leroy, C.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France. [Reach, W. T.] Univ Space Res Assoc, Stratospher Observ Infrared Astron, Moffett Field, CA 94035 USA. [Battaner, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, E-18071 Granada, Spain. [Gorski, K. M.] Univ Warsaw Observ, PL-00478 Warsaw, Poland. RP Gonzalez-Nuevo, J (reprint author), Univ Cantabria, CSIC, Inst Fis Cantabria, Avda Castros S-N, E-39005 Santander, Spain. EM gnuevo@ifca.unican.es RI Barreiro, Rita Belen/N-5442-2014; Remazeilles, Mathieu/N-1793-2015; Kurki-Suonio, Hannu/B-8502-2016; Tomasi, Maurizio/I-1234-2016; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; bonavera, laura/E-9368-2017; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Pearson, Timothy/N-2376-2015; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Valiviita, Jussi/A-9058-2016; Mazzotta, Pasquale/B-1225-2016; Lahteenmaki, Anne/L-5987-2013; Toffolatti, Luigi/K-5070-2014; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Martinez-Gonzalez, Enrique/E-9534-2015; Butler, Reginald/N-4647-2015; OI Matarrese, Sabino/0000-0002-2573-1243; Galeotta, Samuele/0000-0002-3748-5115; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Umana, Grazia/0000-0002-6972-8388; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Lopez-Caniego, Marcos/0000-0003-1016-9283; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834; Kurki-Suonio, Hannu/0000-0002-4618-3063; Tomasi, Maurizio/0000-0002-1448-6131; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; bonavera, laura/0000-0001-8039-3876; Rubino-Martin, Jose Alberto/0000-0001-5289-3021; De Zotti, Gianfranco/0000-0003-2868-2595; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Pearson, Timothy/0000-0001-5213-6231; Gruppuso, Alessandro/0000-0001-9272-5292; Valiviita, Jussi/0000-0001-6225-3693; Mazzotta, Pasquale/0000-0002-5411-1748; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Savini, Giorgio/0000-0003-4449-9416; Villa, Fabrizio/0000-0003-1798-861X; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; Reach, William/0000-0001-8362-4094; Butler, Reginald/0000-0003-4366-5996; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Ricciardi, Sara/0000-0002-3807-4043 FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR (Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC (Spain); MICINN (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF (Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); PRACE (EU) FX The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.sciops.esa.int/index.php?project=planck&page=Planck_Collabora tion. This research has made use of Aladin. We are deeply grateful to Rick Perley and the U.S. National Radio Astronomy Observatory for participating in the joint Planck-VLA observations. We also thank Steve Eales and the H-ATLAS team (Eales et al, 2010 PASP 122 499E) for sharing their SPIRE catalogs prior to publication, allowing a comparison of flux densities between HFI and SPIRE. NR 91 TC 77 Z9 76 U1 2 U2 9 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A28 DI 10.1051/0004-6361/201321524 PG 22 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600004 ER PT J AU Ade, PAR Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Battaner, E Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bond, JR Bonrrill, J Bouchet, FR Boulanger, F Bridges, M Bucher, M Burigana, C Cardoso, JF Catalano, A Challinor, A Chamballu, A Chary, RR Chen, X Chiang, HC Chiang, LY Christensen, PR Church, S Clements, DL Colombi, S Colombo, LPL Combet, C Comis, B Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Danese, L Davies, RD de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Delouis, JM Desert, FX Dickinson, C Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Falgarone, E Finelli, F Forni, O Frailis, M Franceschi, E Galeotta, S Ganga, K Ciard, M Giraud-Heraud, Y Gonzadlez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Hansen, FK Hanson, D Harrison, D Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Hurier, G Jaffe, AH Jaffe, TR Jones, WC Juvela, M Keihanen, E Keskitalo, R Kisner, TS Kneiss, R Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Leahy, JP Leonardi, R Leroy, C Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maffei, B Mandolesi, N Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Mazzotta, P McGehee, P Melchiorri, A Mendes, L Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, MA Moneti, A Montier, L Morgante, G Mortlock, D Munshi, D Murphy, JA Naselsky, P Nati, F Natoli, P Netterfield, CB Norgaard-Nielsen, HU North, C Noviello, F Novikov, D Novikov, I Osborne, S Oxborrow, CA Paci, F Pagano, L Pajot, F Paoletti, D Pasian, F Patanchon, G Perdereau, O Perotto, L Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Reinecke, M Remazeilles, M Renault, C Ricciardi, S Riller, T Ristorcelli, I Rocha, G Rosset, C Roudier, G Rusholme, B Santos, D Savini, G Scott, D Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sureau, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Tomasi, M Tristram, M Tucci, M Umana, G Valenziano, L Valiviita, J Van Tent, B Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD Yvon, D Zacchei, A Zonca, A AF Ade, P. A. R. Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Battaner, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bond, J. R. Borrill, J. Bouchet, F. R. Boulanger, F. Bridges, M. Bucher, M. Burigana, C. Cardoso, J. -F. Catalano, A. Challinor, A. Chamballu, A. Chary, R. -R. Chen, X. Chiang, H. C. Chiang, L. -Y Christensen, P. R. Church, S. Clements, D. L. Colombi, S. Colombo, L. P. L. Combet, C. Comis, B. Couchot, F. Coulais, A. Crill, B. P. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Delouis, J. -M. Desert, F. -X. Dickinson, C. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Falgarone, E. Finelli, F. Forni, O. Frailis, M. Franceschi, E. Galeotta, S. Ganga, K. Ciard, M. Giraud-Heraud, Y. Gonzadlez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Hansen, F. K. Hanson, D. Harrison, D. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Hurier, G. Jaffe, A. H. Jaffe, T. R. Jones, W. C. Juvela, M. Keihanen, E. Keskitalo, R. Kisner, T. S. Kneiss, R. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leahy, J. P. Leonardi, R. Leroy, C. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maffei, B. Mandolesi, N. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. McGehee, P. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Miville-Deschenes, M. -A. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Munshi, D. Murphy, J. A. Naselsky, P. Nati, F. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. North, C. Noviello, F. Novikov, D. Novikov, I. Osborne, S. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paoletti, D. Pasian, F. Patanchon, G. Perdereau, O. Perotto, L. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Reinecke, M. Remazeilles, M. Renault, C. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Rosset, C. Roudier, G. Rusholme, B. Santos, D. Savini, G. Scott, D. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sureau, F. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Tomasi, M. Tristram, M. Tucci, M. Umana, G. Valenziano, L. Valiviita, J. Van Tent, B. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. Yvon, D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. IX. HFI spectral response SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE instrumentation: detectors; instrumentation: photometers; space vehicles: instruments; cosmology: observations; cosmic background radiation ID HIGH-FREQUENCY INSTRUMENT; COBE FIRAS INSTRUMENT; MOLECULAR CLOUDS; MICROWAVE; SPECTROSCOPY; CALIBRATION AB The Planck High Frequency Instrument (HFI) spectral response was determined through a series of ground based tests conducted with the HFI focal plane in a cryogenic environment prior to launch. The main goal of the spectral transmission tests was to measure the relative spectral response (including the level of out-of-band signal rejection) of all HFI detectors to a known source of electromagnetic radiation individually. This was determined by measuring the interferometric output of a continuously scanned Fourier transform spectrometer with all HFI detectors. As there is no on-board spectrometer within HFI, the ground-based spectral response experiments provide the definitive data set for the relative spectral calibration of the HFI. Knowledge of the relative variations in the spectral response between HFI detectors allows for a more thorough analysis of the HFI data. The spectral response of the HFI is used in Planck data analysis and component separation, this includes extraction of CO emission observed within Planck bands, dust emission, Sunyaev-Zeldovich sources, and intensity to polarization leakage. The HFI spectral response data have also been used to provide unit conversion and colour correction analysis tools. While previous papers describe the pre-flight experiments conducted on the Planck HFI, this paper focusses on the analysis of the pre-flight spectral response measurements and the derivation of data products, e.g. band-average spectra, unit conversion coefficients, and colour correction coefficients, all with related uncertainties. Verifications of the HFI spectral response data are provided through comparisons with photometric HFI flight data. This validation includes use of HFI zodiacal emission observations to demonstrate out-of-band spectral signal rejection better than 10(8). The accuracy of the HFI relative spectral response data is verified through comparison with complementary flight-data based unit conversion coefficients and colour correction coefficients. These coefficients include those based upon HFI observations of CO, dust, and Sunyaev-Zeldovich emission. General agreement is observed between the ground-based spectral characterization of HFI and corresponding in-flight observations, within the quoted uncertainty of each; explanations are provided for any discrepancies. C1 [Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Piat, M.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, Observ Paris, Sorbonne Paris Cite, CNRS IN2P3,CEA lrfu,APC, F-75205 Paris 13, France. [Poutanen, T.] Aalto Univ, Metsahovi Radio Observ, Kylmala 02540, Finland. [Kunz, M.] African Inst Math Sci, ZA-7701 Cape Town, South Africa. [Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana Sci, Ctr Data, I-00133 Rome, Italy. [Mandolesi, N.] Agenzia Spaziale Italiana, Rome, Italy. [Ashdown, M.; Bridges, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 OHE, England. [Chiang, H. 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[Battaner, E.] Univ Toulouse, UPS OMP, TRAP, F-31028 Toulouse 4, France. [Battaner, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, E-18071 Granada, Spain. [Gorski, K. M.] Univ Warsaw Observ, Warsaw, Poland. RP Spencer, LD (reprint author), Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, S Glam, Wales. EM Locke.Spencer@astro.cf.ac.uk RI Barreiro, Rita Belen/N-5442-2014; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; Remazeilles, Mathieu/N-1793-2015; Valiviita, Jussi/A-9058-2016; Mazzotta, Pasquale/B-1225-2016; Kurki-Suonio, Hannu/B-8502-2016; Tomasi, Maurizio/I-1234-2016; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Martinez-Gonzalez, Enrique/E-9534-2015; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; OI Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Galeotta, Samuele/0000-0002-3748-5115; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; De Zotti, Gianfranco/0000-0003-2868-2595; Lopez-Caniego, Marcos/0000-0003-1016-9283; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Valiviita, Jussi/0000-0001-6225-3693; Mazzotta, Pasquale/0000-0002-5411-1748; Kurki-Suonio, Hannu/0000-0002-4618-3063; Tomasi, Maurizio/0000-0002-1448-6131; Vielva, Patricio/0000-0003-0051-272X; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Gruppuso, Alessandro/0000-0001-9272-5292; Savini, Giorgio/0000-0003-4449-9416; Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834; Hurier, Guillaume/0000-0002-1215-0706; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Ricciardi, Sara/0000-0002-3807-4043; Villa, Fabrizio/0000-0003-1798-861X; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; Finelli, Fabio/0000-0002-6694-3269; Umana, Grazia/0000-0002-6972-8388; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924 FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR (Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC (Spain); MICINN (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF (Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); PRACE (EU); NSERC (Canada) FX The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.sciops.esa.int/index.php?project=planck&page=Planck_Collabora tion. The authors thank Emmanuel Lellouch, Raphael Moreno, and Matt Griffin for the provision of the planet model spectra used to generate HFI planet colour correction coefficients. L. Spencer acknowledges support from NSERC (Canada) and STFC (UK). NR 70 TC 60 Z9 59 U1 2 U2 11 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A9 DI 10.1051/0004-6361/201321531 PG 27 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600008 ER PT J AU Ade, PAR Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Aussel, H Baccigalupi, C Banday, AJ Barreiro, RB Barrena, R Bartelinann, M Bartlett, JG Battaner, E Benabed, K Benoit, A Benoit-Ley, A Bernard, J Bersanelli, M Bielewicz, P Bikmaev, I Bobin, J Bock, JJ Bohringer, H Bonaldi, A Bond, JR Borrill, J Bouchet, FR Bridges, M Bucher, M Burenin, R Burigana, C Butier, RC Cardoso, JF Carvalho, P Catalano, A Challinor, A Chamballu, A Chary, RR Chen, X Chiang, HC Chiang, LY Chon, G Christensen, PR Churazov, E Church, S Clements, DL Colombi, S Colombo, LPL Comis, B Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Da Silva, A Dahle, H Danese, L Davies, RD Davis, RJ de Bernardis, P de Rosa, A de Zotti, G Delabrouilie, J Delouis, JM Democles, J Desert, FX Dickinson, C Diego, IM Dolag, K Dole, H Donzelli, S Dore, O Douspis, M Dupac, X Efstathiou, G Eisenhardt, PRM Ensslin, TA Eriksen, HK Feroz, F Finelli, F Flores-Cacho, I Forni, O Frailis, M Franceschi, E Fromenteau, S Galeotta, S Ganga, K Genova-Santos, RT Giard, M Giardino, G Gilfanov, M Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Grainge, KJB Gratton, S Gregorio, A Groeneboom, NE Gruppuso, A Hansen, FK Hanson, D Harrison, D Hempel, A Elenrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Homstrup, A Hovest, W Huffenberger, KM Hurier, G Hurley-Walker, N Jaffe, AH Jaffe, TR Jones, WC Juvela, M Keihanen, E Keskitalo, R Khamitov, I Kisner, TS Kneissl, R Knoche, J Knox, L Kunz, M Kurki-Suonio, H Laeache, G Lahteenmaki, A Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Leahy, JP Leonardi, R Leon-Tavares, J Lesgourgues, J Li, C Liddle, A Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF MacTavish, CJ Maffei, B Maino, D Mandolesi, N Maris, M Marshal, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Mazzotta, P Mei, S Meinhold, PR Meichiorri, A Melin, JB Mendes, L Mennelia, A Migliaccio, M Mikkeisen, K Mitra, S Miville-Deschenes, MA Moneti, A Montier, L Morgante, G Mortlock, D Munshi, D Murphy, JA Naselsky, P Nati, F Natoli, P Nesvadba, NPH Netterfield, CB Norgaard-Nielsen, HU Noviello, F Novikov, D Novilov, I O'Dwyer, IJ Olamaie, M Osborne, S Oxborrow, CA Paci, F Pagano, L Pajot, F Paoletti, D Pasian, F Patanchon, G Pearson, TJ Perdereau, O Perotto, L Perrott, YC Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pletrobon, D Plaszczynski, S Pointecouteau, E Polenta, O Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Reach, WT Rebolo, R Reinecke, M Remazeilles, M Renault, C Ricciardi, S Riller, T Ristorcelli, I Rocha, G Rosset, C Roudier, G Rowan-Robinson, M Rubino-Martin, JA Rumsey, C Rusholme, B Sandri, M Santos, D Saunders, RDE Savini, G Schammel, MP Scott, D Seiffert, MD Shellard, EPS Shimwell, TW Spencer, LD Stanford, SA Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sunyaev, R Sureau, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Tuovinen, J Turler, M Umana, G Valenziano, L Valiviita, J Van Tent, B Vibert, L Vielva, P Vilia, F Vittorio, N Wade, LA Wandelt, BD White, M White, SDM Yvon, D Zacchei, A Zonca, A AF Ade, P. A. R. Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Aussel, H. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Barrena, R. Bartelinann, M. Bartlett, J. G. Battaner, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. . Bersanelli, M. Bielewicz, P. Bikmaev, I. Bobin, J. Bock, J. J. Boehringer, H. Bonaldi, A. Bond, J. R. Borrill, J. Bouchet, F. R. Bridges, M. Bucher, M. Burenin, R. Burigana, C. Butier, R. C. Cardoso, J. -F. Carvalho, P. Catalano, A. Challinor, A. Chamballu, A. Chary, R. -R. Chen, X. Chiang, H. C. Chiang, L. -Y. Chon, G. Christensen, P. R. Churazov, E. Church, S. Clements, D. L. Colombi, S. Colombo, L. P. L. Comis, B. Couchot, F. Coulais, A. Crill, B. P. Curto, A. Cuttaia, F. Da Silva, A. Dahle, H. Danese, L. Davies, R. D. Davis, R. J. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouilie, J. Delouis, J. -M. Democles, J. Desert, F. -X. Dickinson, C. Diego, I. M. Dolag, K. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dupac, X. Efstathiou, G. Eisenhardt, P. R. M. Ensslin, T. A. Eriksen, H. K. Feroz, F. Finelli, F. Flores-Cacho, I. Forni, O. Frailis, M. Franceschi, E. Fromenteau, S. Galeotta, S. Ganga, K. Genova-Santos, R. T. Giard, M. Giardino, G. Gilfanov, M. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Grainge, K. J. B. Gratton, S. Gregorio, A. Groeneboom, N. E. Gruppuso, A. Hansen, F. K. Hanson, D. Harrison, D. Hempel, A. Elenrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Homstrup, A. Hovest, W. Huffenberger, K. M. Hurier, G. Hurley-Walker, N. Jaffe, A. H. Jaffe, T. R. Jones, W. C. Juvela, M. Keihanen, E. Keskitalo, R. Khamitov, I. Kisner, T. S. Kneissl, R. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Laeache, G. Lahteenmaki, A. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leahy, J. P. Leonardi, R. Leon-Tavares, J. Lesgourgues, J. Li, C. Liddle, A. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. MacTavish, C. J. Maffei, B. Maino, D. Mandolesi, N. Maris, M. Marshal, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. Mei, S. Meinhold, P. R. Meichiorri, A. Melin, J. -B. Mendes, L. Mennelia, A. Migliaccio, M. Mikkeisen, K. Mitra, S. Miville-Deschenes, M. -A. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Munshi, D. Murphy, J. A. Naselsky, P. Nati, F. Natoli, P. Nesvadba, N. P. H. Netterfield, C. B. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novilov, I. O'Dwyer, I. J. Olamaie, M. Osborne, S. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paoletti, D. Pasian, F. Patanchon, G. Pearson, T. J. Perdereau, O. Perotto, L. Perrott, Y. C. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pletrobon, D. Plaszczynski, S. Pointecouteau, E. Polenta, O. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Reach, W. T. Rebolo, R. Reinecke, M. Remazeilles, M. Renault, C. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Rosset, C. Roudier, G. Rowan-Robinson, M. Rubino-Martin, J. A. Rumsey, C. Rusholme, B. Sandri, M. Santos, D. Saunders, R. D. E. Savini, G. Schammel, M. P. Scott, D. Seiffert, M. D. Shellard, E. P. S. Shimwell, T. W. Spencer, L. D. Stanford, S. A. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sunyaev, R. Sureau, F. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Tuovinen, J. Tuerler, M. Umana, G. Valenziano, L. Valiviita, J. Van Tent, B. Vibert, L. Vielva, P. Vilia, F. Vittorio, N. Wade, L. A. Wandelt, B. D. White, M. White, S. D. M. Yvon, D. Zacchei, A. Zonca, A. TI Planck 2013 results. XXIX. The Planck catalogue of Sunyaev-Zeldovich sources SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE large-scale structure of Universe; galaxies: clusters: general; catalogs ID GALAXY CLUSTER SURVEY; SOUTH-POLE TELESCOPE; DIGITAL SKY SURVEY; X-RAY-PROPERTIES; LUMINOSITY-TEMPERATURE RELATION; MICROWAVE BACKGROUND-RADIATION; ARCMINUTE MICROKELVIN IMAGER; DISCRETE OBJECT DETECTION; ADAPTIVE MATCHED-FILTER; ASTRONOMICAL DATA SETS AB We describe the all-sky Planck catalogue of clusters and cluster candidates derived from Sunyaev-Zeldovich (SZ) effect detections using the first 15.5 months of Planck satellite observations. The catalogue contains 1227 entries, making it over six times the size of the Planck Early SZ (ESZ) sample and the largest SZ-selected catalogue to date. It contains 861 confirmed clusters, of which 178 have been confirmed as clusters, mostly through follow-up observations, and a further 683 are previously-known clusters. The remaining 366 have the status of cluster candidates, and we divide them into three classes according to the quality of evidence that they are likely to be true clusters. The Planck SZ catalogue is the deepest all-sky cluster catalogue, with redshifts up to about one, and spans the broadest cluster mass range from (0.1 to 1.6) x 10(15) M-circle dot. Confirmation of cluster candidates through comparison with existing surveys or cluster catalogues is extensively described, as is the statistical characterization of the catalogue in terms of completeness and statistical reliability. The outputs of the validation process are provided as additional information. This gives, in particular, an ensemble of 813 cluster redshifts, and for all these Planck clusters we also include a mass estimated from a newly-proposed SZ-mass proxy. 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EM nabila.aghanim@ias.u-psud.fr RI Barreiro, Rita Belen/N-5442-2014; Remazeilles, Mathieu/N-1793-2015; Valiviita, Jussi/A-9058-2016; Mazzotta, Pasquale/B-1225-2016; Kurki-Suonio, Hannu/B-8502-2016; Tomasi, Maurizio/I-1234-2016; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; Martinez-Gonzalez, Enrique/E-9534-2015; Churazov, Eugene/A-7783-2013; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; White, Martin/I-3880-2015; Pearson, Timothy/N-2376-2015; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Hurley-Walker, Natasha/B-9520-2013; Lahteenmaki, Anne/L-5987-2013; Toffolatti, Luigi/K-5070-2014; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Butler, Reginald/N-4647-2015; OI Matarrese, Sabino/0000-0002-2573-1243; Galeotta, Samuele/0000-0002-3748-5115; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Umana, Grazia/0000-0002-6972-8388; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Lopez-Caniego, Marcos/0000-0003-1016-9283; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834; Valiviita, Jussi/0000-0001-6225-3693; Mazzotta, Pasquale/0000-0002-5411-1748; Kurki-Suonio, Hannu/0000-0002-4618-3063; Tomasi, Maurizio/0000-0002-1448-6131; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; Rubino-Martin, Jose Alberto/0000-0001-5289-3021; De Zotti, Gianfranco/0000-0003-2868-2595; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; White, Martin/0000-0001-9912-5070; Pearson, Timothy/0000-0001-5213-6231; Gruppuso, Alessandro/0000-0001-9272-5292; Hurley-Walker, Natasha/0000-0002-5119-4808; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Savini, Giorgio/0000-0003-4449-9416; Villa, Fabrizio/0000-0003-1798-861X; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; Reach, William/0000-0001-8362-4094; Hurier, Guillaume/0000-0002-1215-0706; Butler, Reginald/0000-0003-4366-5996; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Ricciardi, Sara/0000-0002-3807-4043 FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR (Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC (Spain); MICINN (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF (Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); PRACE (EU); BTA 6-m telescope Time Allocation Committee (TAC); CCI International Time Programme; Alfred P. Sloan Foundation; Participating Institutions; National Science Foundation; DoE; NASA; CNES; CNRS FX The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.sciops.esa.int/index.php?project=planck&page=Planck_Collabora tion. The authors thank N. Schartel, ESA XMM-Newton project scientist, for granting the Director Discretionary Time used for confirmation of SZ Planck candidates. The authors thank TUBITAK, IKI, KFU and AST for support in using RTT150 (Russian-Turkish 1.5-m telescope, Bakyrlytepe, Turkey); in particular we thank KFU and IKI for providing significant amount of their observing time at RTT150. We also thank BTA 6-m telescope Time Allocation Committee (TAC) for support of optical follow-up project. The authors acknowledge the use of the INT and WHT telescopes operated on the island of La Palma by the Isaac Newton Group of Telescopes at the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias (IAC); the Nordic Optical Telescope, operated on La Palma jointly by Denmark, Finland, Iceland, Norway, and Sweden, at the Spanish Observatorio del Roque de los Muchachos of the IAC; the TNG telescope, operated on La Palma by the Fundacion Galileo Galilei of the INAF at the Spanish Observatorio del Roque de los Muchachos of the IAC; the GTC telescope, operated on La Palma by the IAC at the Spanish Observatorio del Roque de los Muchachos of the IAC; and the IAC80 telescope operated on the island of Tenerife by the IAC at the Spanish Observatorio del Teide of the IAC. Part of this research has been carried out with telescope time awarded by the CCI International Time Programme. The authors thank the TAC of the MPG/ESO-2.2m telescope for support of optical follow-up with WFI under Max Planck time. Observations were also conducted with ESO NTT at the La Silla Paranal Observatory. This research has made use of SDSS-III data. Funding for SDSS-III http://www.sdss3.org/ has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and DoE. SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration. This research has made use of the following databases: the NED and IRSA databases, operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the NASA; SIMBAD, operated at CDS, Strasbourg, France; SZ cluster database operated by Integrated Data and Operation Center (IDOC) operated by IAS under contract with CNES and CNRS. The authors acknowledge the use of software provided by the US National Virtual Observatory. NR 160 TC 179 Z9 178 U1 3 U2 24 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A29 DI 10.1051/0004-6361/201321523 PG 41 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600003 ER PT J AU Ade, PAR Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, B Bartlett, JG Battanerioo, E Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bonaldi, A Bond, JR Borrill, J Bouchet, FR Bridges, M Bucher, M Burigana, C Butler, RC Cardoso, JF Carvalho, P Catalano, A Challinor, A Chamballu, A Chiang, HC Chiang, LY Christensen, PR Church, S Clements, DL Colombi, S Colombo, LPL Comis, B Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Da Silva, A Danese, L Davies, RD Davis, RJ de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Delouis, JM Desert, FX Dickinson, C Diego, JM Dolag, K Dole, H Donzelli, S Dore, A Douspis, M Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Finelli, F Flores-Cacho, I Forni, O Frailis, M Franceschi, E Galeotta, S Ganga, K Genova-Santos, RT Giard, M Giardino, G Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Hansen, FK Hanson, D Harrison, D Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Hurier, G Jaffe, AH Jaffe, TR Jones, WC Juvela, M Keihanen, E Keskitalo, R Kisner, TS Kneissl, R Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lacasa, F Lagache, G Lahteenmaki, A Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Leahy, JP Leonardi, R Loen-Tavares, J Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maffei, B Maino, D Mandolesi, N Marcos-Caballero, A Maris, M Marshall, DJ Martin, G Macinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Mazzotta, P Melchiorri, A Melin, JB Mendes, L Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, MA Moneti, A Montier, L Morgante, G Mortlock, D Moss, A Munshi, D Naselsky, P Nati, F Natoli, P Netterfield, CB Norgaard-Nielsen, HU Noviello, F Novikov, D Novikov, I Osborne, S Oxborrow, CA Paci, F Pagano, L Pajot, F Paoletti, D Partridge, B Pasian, F Patanchonl, G Perdereau, . Perotto, L Perrotta, F Piacentini, F Mae, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Rebolo, R Reinecke, M Remazeilles, M Renault, C Ricciardi, S Riller, T Ristorcelli, I Rocha, G Rossetl, C Rossetti, M Roudier, G Rubino-Martin, JA Rusholme, B Sandri, M Santos, D Savini, G Scott, D Seiffert, MD Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sunyaev, R Sureau, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Tuovinen, J Umana, G Valenziano, L Valiviita, J Van Tent, B Varis, J Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD White, SDM Yvon, D Zacchei, A Zonca, A AF Ade, P. A. R. Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, B. Bartlett, J. G. Battanerioo, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bonaldi, A. Bond, J. R. Borrill, J. Bouchet, F. R. Bridges, M. Bucher, M. Burigana, C. Butler, R. C. Cardoso, J. -F. Carvalho, P. Catalano, A. Challinor, A. Chamballu, A. Chiang, H. C. Chiang, L. -Y Christensen, P. R. Church, S. Clements, D. L. Colombi, S. Colombo, L. P. L. Comis, B. Couchot, F. Coulais, A. Crill, B. P. Curto, A. Cuttaia, F. Da Silva, A. Danese, L. Davies, R. D. Davis, R. J. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Delouis, J. -M. Desert, F. -X. Dickinson, C. Diego, J. M. Dolag, K. Dole, H. Donzelli, S. Dore, A. Douspis, M. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Finelli, F. Flores-Cacho, I. Forni, O. Frailis, M. Franceschi, E. Galeotta, S. Ganga, K. Genova-Santos, R. T. Giard, M. Giardino, G. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Hansen, F. K. Hanson, D. Harrison, D. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Hurier, G. Jaffe, A. H. Jaffe, T. R. Jones, W. C. Juvela, M. Keihanen, E. Keskitalo, R. Kisner, T. S. Kneissl, R. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lacasa, F. Lagache, G. Lahteenmaki, A. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leahy, J. P. Leonardi, R. Loen-Tavares, J. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maffei, B. Maino, D. Mandolesi, N. Marcos-Caballero, A. Maris, M. Marshall, D. J. Martin, G. Macinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. Melchiorri, A. Melin, J. -B. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Miville-Deschenes, M. -A. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Moss, A. Munshi, D. Naselsky, P. Nati, F. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novikov, I. Osborne, S. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paoletti, D. Partridge, B. Pasian, F. Patanchonl, G. Perdereau, . Perotto, L. Perrotta, F. Piacentini, F. Mae, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Rebolo, R. Reinecke, M. Remazeilles, M. Renault, C. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Rossetl, C. Rossetti, M. Roudier, G. Rubino-Martin, J. A. Rusholme, B. Sandri, M. Santos, D. Savini, G. Scott, D. Seiffert, M. D. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sunyaev, R. Sureau, F. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Tuovinen, J. Umana, G. Valenziano, L. Valiviita, J. Van Tent, B. Varis, J. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. White, S. D. M. Yvon, D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. XXI. Power spectrum and high-order statistics of the Planck all-sky Compton parameter map SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE cosmological parameters; large-scale structure of Universe; galaxies: clusters: general ID SUNYAEV-ZELDOVICH CLUSTERS; MICROWAVE BACKGROUND MAPS; POLE TELESCOPE SURVEY; POINT SOURCES; COSMOLOGICAL PARAMETERS; DATA SETS; COUNTS; CMB; EXTRACTION; GALAXIES AB We have constructed the first all-sky map of the thermal Sunyaev-Zeldovich (tSZ) effect by applying specifically tailored component separation algorithms to the 100 to 857 GHz frequency channel maps from the Planck survey. This map shows an obvious galaxy cluster tSZ signal that is well matched with blindly detected clusters in the Planck SZ catalogue. To characterize the signal in the tSZ map we have computed its angular power spectrum. At large angular scales (l < 60), the major foreground contaminant is the diffuse thermal dust emission. At small angular scales (l > 500) the clustered cosmic infrared background and residual point sources are the major contaminants. These foregrounds are carefully modelled and subtracted. We thus measure the tSZ power spectrum over angular scales 0.17 degrees less than or similar to theta less than or similar to 3.0 degrees that were previously unexplored. The measured tSZ power spectrum is consistent with that expected from the Planck catalogue of SZ sources, with clear evidence of additional signal from unresolved clusters and, potentially, diffuse warm baryons. Marginalized band-powers of the Planck tSZ power spectrum and the best-fit model are given. The non-Gaussianity of the Compton parameter map is further characterized by computing its 1D probability distribution function and its bispectrum. The measured tSZ power spectrum and high order statistics are used to place constraints on sigma(8). C1 [Bartlett, J. G.; Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchonl, G.; Mae, M.; Remazeilles, M.; Rossetl, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, Sorbonne Paris Cite, CNRS, IN2P3,CEA Irfu,Observ Paris,APC, F-75205 Paris 13, France. [Lahteenmaki, A.; Loen-Tavares, J.; Poutanen, T.] Aalto Univ Metsahovi Radio Observ, Kylmala 02540, Finland. [Kunz, M.] African Inst Math Sci, Cape Town, South Africa. [Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana, Sci Data Ctr, I-00133 Rome, Italy. [Mandolesi, N.] Agenzia Spaziale Italiana, Rome, Italy. [Ashdown, M.; Bridges, M.; Carvalho, P.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 0HE, England. [Chiang, H. C.] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, ZA-4000 Durban, South Africa. [Kneissl, R.] ALMA Santiago Cent Offices, Santiago 0355, Chile. [Bond, J. R.; Hanson, D.; Martin, G.; Miville-Deschenes, M. -A.] Univ Toronto, CITA, Toronto, ON M5S 3H8, Canada. [Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Flores-Cacho, I.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] CNRS, IRAP, F-31028 Toulouse 4, France. [Bock, J. J.; Dore, A.; Hildebrandt, S. R.; Prezeau, G.; Rocha, G.; Seiffert, M. D.] CALTECH, Pasadena, CA USA. [Challinor, A.; Shellard, E. P. S.] Univ Cambridge, Ctr Theoret Cosmol, DAMTP, Cambridge CB3 0WA, England. [Da Silva, A.] Univ Porto, Ctr Astrofis, P-4150762 Oporto, Portugal. [Hernandez-Monteagudo, C.] CEFCA, Teruel 44001, Spain. [Borrill, J.; Keskitalo, R.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 94720 USA. CSIC, Madrid, Spain. [Chamballu, A.; Melin, J. -B.; Yvon, D.] CEA Saclay, DSM Irfu SPP, F-91191 Gif Sur Yvette, France. Tech Univ Denmark, Natl Space Inst, DTU Space, DK-2800 Lyngby, Denmark. [Kunz, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, CH-1211 Geneva 4, Switzerland. [Atrio-Barandela, F.] Univ Salamanca, Fac Ciencias, Dept Fis Fundamental, E-37008 Salamanca, Spain. [Toffolatti, L.] Univ Oviedo, Dept Fis, E-33007 Oviedo, Spain. [Netterfield, C. B.] Univ Toronto, Dept Astron & Astrophys, Toronto, ON, Canada. [Rachen, J. P.] Radboud Univ Nijmegen, IMAPP, Dept Astrophys, NL-6500 GL Nijmegen, Netherlands. [Keskitalo, R.] Univ Calif Berkeley, Dept Elect Engn & Comp Sci, Berkeley, CA 94720 USA. [Scott, D.] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V5Z 1M9, Canada. [Colombo, L. P. L.; Pierpaoli, E.] Univ So Calif, Dana & David Dornsife Coll Letter Arts & Sci, Dept Phys & Astron, Los Angeles, CA 90089 USA. [Benoit-Levy, A.] UCL, Dept Phys & Astron, London WC1E 6BT, England. [Huffenberger, K. M.] Florida State Univ, Dept Phys, Tallahassee, FL USA. [Juvela, M.; Keihanen, E.; Kurki-Suonio, H.; Poutanen, T.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Dept Phys, FIN-00014 Helsinki, Finland. [Chiang, H. C.; Jones, W. C.] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA. [Knox, L.] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA. [Lubin, P. M.; Zonca, A.] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA. [Wandelt, B. D.] Univ Illinois, Dept Phys, Urbana, IL USA. [Liguori, M.; Matarrese, S.] Univ Padua, Dipartimento Fis Astron G Galilei, I-35131 Padua, Italy. [Burigana, C.; Mandolesi, N.; Natoli, P.] Univ Ferrara, Dipartimento Fis & Sci Terra, I-44122 Ferrara, Italy. [de Bernardis, P.; Melchiorri, A.; Nati, F.; Pagano, L.; Piacentini, F.] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy. [Bersanelli, M.; Maino, D.; Mennella, A.; Rossetti, M.] Univ Milan, Dipartimento Fis, I-20133 Milan, Italy. [Gregorio, A.; Tavagnacco, D.] Univ Trieste, Dipartimento Fis, I-34127 Trieste, Italy. [Mazzotta, P.; Vittorio, N.] Univ Roma Tor Vergata, Dipartimento Fis, I-00133 Rome, Italy. [Christensen, P. R.; Naselsky, P.] Niels Bohr Inst, Discovery Ctr, DK-2100 Copenhagen, Denmark. [Rebolo, R.; Rubino-Martin, J. A.] Univ La Laguna, Dpto Astrofis, E-38206 Tenerife, Spain. [Kneissl, R.] ESO Vitacura, Santiago, Chile. [Dupac, X.; Leonardi, R.; Mendes, L.] European Space Agcy, ESAC, Planck Sci Off, Madrid, Spain. [Giardino, G.; Laureijs, R. J.; Tauber, J. A.] Estec, European Space Agcy, NL-2201 AZ Noordwijk, Netherlands. [Loen-Tavares, J.] Univ Turku, Finnish Ctr Astron ESO FINCA, Piikkio 21500, Finland. [Partridge, B.] Haverford Coll, Dept Astron, Haverford, PA 19041 USA. [Kurki-Suonio, H.; Lahteenmaki, A.; Poutanen, T.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Helsinki Inst Phys, FIN-00014 Helsinki, Finland. [Umana, G.] Osserv Astrofis Catania, INAF, I-95123 Catania, Italy. [de Zotti, G.; Villa, F.] Osserv Astron Padova, INAF, I-35122 Padua, Italy. 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[Clements, D. L.; Jaffe, A. H.; Mortlock, D.; Novikov, D.] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Astrophys Grp, London SW7 2AZ, England. [Rusholme, B.] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA. [Benoit, A.] Univ Grenoble 1, CNRS, Inst Neel, F-38042 Grenoble, France. [Dole, H.] Inst Univ France, F-75005 Paris, France. [Aghanim, N.; Aumont, J.; Chamballu, A.; Dole, H.; Douspis, M.; Hurier, G.; Kunz, M.; Lacasa, F.; Lagache, G.; Masi, S.; Miville-Deschenes, M. -A.; Pajot, F.; Ponthieu, N.; Puget, J. -L.; Remazeilles, M.] Univ Paris 11, CNRS, Inst Astrophys Spatiale, UMR 8617, F-91405 Orsay, France. [Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Cardoso, J. -F.; Colombi, S.; Delouis, J. -M.; Hivon, E.; Moneti, A.; Prunet, S.; Sygnet, J. -F.; Wandelt, B. D.] CNRS, Inst Astrophys Paris, UMR 7095, Paris, France. [Popa, L.] Inst Space Sci, Bucharest 077125, Romania. [Chiang, L. -Y] Acad Sinica, Inst Astron & Astrophys, Taipei 106, Taiwan. [Bridges, M.; Challinor, A.; Efstathiou, G.; Gratton, S.; Harrison, D.; Migliaccio, M.; Sutton, D.] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England. [Eriksen, H. K.; Hansen, F. K.; Lilje, P. B.; Valiviita, J.] Univ Oslo, Inst Theoret Astrophys, N-0315 Oslo, Norway. [Genova-Santos, R. T.; Rebolo, R.; Rubino-Martin, J. A.] Inst Astrofis Canarias, Tenerife 38205, Spain. [Barreiro, B.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Marcos-Caballero, A.; Macinez-Gonzalez, E.; Toffolatti, L.; Vielva, P.] Univ Cantabria, CSIC, Inst Fis Cantabria, E-39005 Santander, Spain. [Bartlett, J. G.; Bock, J. J.; Colombo, L. P. L.; Crill, B. P.; Dore, A.; Gorski, K. M.; Hanson, D.; Holmes, W. A.; Lawrence, C. R.; Mitra, S.; Pietrobon, D.; Prezeau, G.; Rocha, G.; Roudier, G.; Seiffert, M. D.; Wade, L. A.] CALTECH, Jet Prop Lab, Pasadena, CA 91125 USA. [Bonaldi, A.; Davies, R. D.; Davis, R. J.; Dickinson, C.; Leahy, J. P.; Maffei, B.; Noviello, F.; Remazeilles, M.] Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Manchester M13 9PL, Lancs, England. [Ashdown, M.; Bridges, M.; Challinor, A.; Gratton, S.; Harrison, D.; Lasenby, A.; Migliaccio, M.; Stolyarov, V.; Sutton, D.] Kavli Inst Cosmol Cambridge, Cambridge CB3 0HA, England. [Couchot, F.; Dore, A.; Henrot-Versille, S.; Perdereau, .; Plaszczynski, S.; Tristram, M.; Tucci, M.] Univ Paris 11, CNRS, IN2P3, LAL, F-91898 Orsay, France. [Catalano, A.; Coulais, A.; Lamarre, J. -M.; Roudier, G.] CNRS, Observ Paris, LERMA, F-75014 Paris, France. [Arnaud, M.; Bobin, J.; Chamballu, A.; Marshall, D. J.; Pratt, G. W.; Starck, J. -L.; Sureau, F.] Univ Paris Diderot, CEA Saclay, CNRS, CEA CSM,IRFU,Serv Astrophys,Lab AIM, F-91191 Gif Sur Yvette, France. [Cardoso, J. -F.] CNRS, Lab Traitement & Commun Informat, UMR 51541, F-75634 Paris 13, France. [Catalano, A.; Comis, B.; Hurier, G.; Macias-Perez, J. F.; Perotto, L.; Renault, C.; Santos, D.] Univ Grenoble 1, CNRS, IN2P3, Inst Natl Polytech Grenoble,Lab Phys Subatom & Co, F-38026 Grenoble 13, France. [Van Tent, B.] Univ Paris 11, Phys Theor Lab, F-91405 Orsay, France. [Van Tent, B.] CNRS, F-91405 Orsay, France. [Kisner, T. S.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Dolag, K.; Ensslin, T. A.; Hernandez-Monteagudo, C.; Hovest, W.; Knoche, J.; Matthai, F.; Rachen, J. P.; Reinecke, M.; Riller, T.; Sunyaev, R.; White, S. D. M.] Max Planck Inst Astrophys, D-85741 Garching, Germany. [Hanson, D.] McGill Univ, Montreal, PQ H3A 2T8, Canada. [Tuovinen, J.; Varis, J.] VTT Tech Res Ctr Finland, Milli Lab, Espoo 02044, Finland. [Christensen, P. R.; Naselsky, P.; Novikov, I.] Niels Bohr Inst, DK-2100 Copenhagen, Denmark. [Crill, B. P.] CALTECH, Observ Cosmol, Pasadena, CA 91125 USA. [Savini, G.] UCL, Opt Sci Lab, London, England. [Lesgourgues, J.] Ecole Polytech Fed Lausanne, SB ITP LPPC, CH-1015 Lausanne, Switzerland. [Baccigalupi, C.; Danese, L.; de Zotti, G.; Gonzalez-Nuevo, J.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sector, I-34136 Trieste, Italy. [Ade, P. A. R.; Munshi, D.; Spencer, L. D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales. [Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England. [Sunyaev, R.] Russian Acad Sci, Space Res Inst IKI, Moscow 117997, Russia. [Borrill, J.; Stolyarov, V.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA. [Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Karachai Cherkessian Rep 369167, Zelenchukskiy R, Russia. [Church, S.; Osborne, S.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA. [Armitage-Caplan, C.] Univ Oxford, Sub Dept Astrophys, Oxford OX1 3RH, England. [Lesgourgues, J.] CERN, PH TH, Div Theory, CH-1211 Geneva 23, Switzerland. [Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Colombi, S.; Delouis, J. -M.; Hivon, E.; Prunet, S.; Wandelt, B. D.] Univ Paris 06, UMR7095, F-75014 Paris, France. [Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Flores-Cacho, I.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France. [Dolag, K.] Univ Munich, Univ Observ, D-81679 Munich, Germany. [Battanerioo, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, E-18071 Granada, Spain. [Gorski, K. M.] Univ Warsaw Observ, PL-00478 Warsaw, Poland. RP Macias-Perez, JF (reprint author), Univ Grenoble 1, CNRS, IN2P3, Inst Natl Polytech Grenoble,Lab Phys Subatom & Co, 53 Rue Martyrs, F-38026 Grenoble 13, France. EM macias@lpsc.in2p3.fr RI Remazeilles, Mathieu/N-1793-2015; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; Mazzotta, Pasquale/B-1225-2016; Kurki-Suonio, Hannu/B-8502-2016; Tomasi, Maurizio/I-1234-2016; Lahteenmaki, Anne/L-5987-2013; Toffolatti, Luigi/K-5070-2014; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Valiviita, Jussi/A-9058-2016; Barreiro, Rita Belen/N-5442-2014; Butler, Reginald/N-4647-2015; OI Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Galeotta, Samuele/0000-0002-3748-5115; Ricciardi, Sara/0000-0002-3807-4043; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; WANDELT, Benjamin/0000-0002-5854-8269; Rubino-Martin, Jose Alberto/0000-0001-5289-3021; De Zotti, Gianfranco/0000-0003-2868-2595; Lopez-Caniego, Marcos/0000-0003-1016-9283; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Mazzotta, Pasquale/0000-0002-5411-1748; Kurki-Suonio, Hannu/0000-0002-4618-3063; Tomasi, Maurizio/0000-0002-1448-6131; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Gruppuso, Alessandro/0000-0001-9272-5292; Valiviita, Jussi/0000-0001-6225-3693; Paoletti, Daniela/0000-0003-4761-6147; Savini, Giorgio/0000-0003-4449-9416; Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834; Hurier, Guillaume/0000-0002-1215-0706; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Villa, Fabrizio/0000-0003-1798-861X; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; Pasian, Fabio/0000-0002-4869-3227; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Umana, Grazia/0000-0002-6972-8388; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Butler, Reginald/0000-0003-4366-5996; Sandri, Maura/0000-0003-4806-5375 FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR (Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC (Spain); MICINN (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF (Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); PRACE (EU) FX The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.sciops.esa.int/index.php?project=Planck&page=Planck_Collabora tion. We acknowledge the use of the HEALPix software. NR 87 TC 77 Z9 76 U1 2 U2 12 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A21 DI 10.1051/0004-6361/201321522 PG 18 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600002 ER PT J AU Ade, PAR Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Barrena, R Bartlett, JG Battaner, E Battye, R Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bikmaev, I Blanchard, A Bobin, J Bock, JJ Bohringer, H Bonaldi, A Bond, JR Borrill, J Bouchet, FR Bourdin, H Bridges, M Brown, ML Bucher, M Burenin, R Burigana, C Butler, RC Cardoso, JF Carvalho, P Catalano, A Challinor, A Chamballu, A Chary, RR Chiang, LY Chiang, HC Chon, G Christensen, PR Church, S Clements, DL Colombi, S Colombo, LPL Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Da Silva, A Dahle, H Danese, L Davies, RD Davis, RJ de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Delouis, JM Democles, J Desert, FX Dickinson, C Diego, JM Dolag, K Dole, H Donzelli, S Dore, O Douspis, M Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Finelli, F Flores-Cacho, I Forni, O Frailis, M Franceschi, E Fromenteau, S Galeotta, S Ganga, K Genova-Santos, RT Giard, M Giardino, G Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Hansen, FK Hanson, D Harrison, D Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Hurier, G Jaffe, TR Jaffe, AH Jones, WC Juvela, M Keihanen, E Keskitalo, R Khamitov, I Kisner, TS Kneissl, R Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lahteenmaki, A Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Leahy, JP Leonardi, R Leon-Tavares, J Lesgourgues, J Liddle, A Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maffei, B Maino, D Mandolesi, N Marcos-Caballero, A Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Matarrese, S Matthai, F Mazzotta, P Meinhold, PR Melchiorri, A Melin, JB Mendes, L Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, MA Moneti, A Montier, L Morgante, G Mortlock, D Moss, A Munshi, D Naselsky, P Nati, F Natoli, P Netterfield, CB Norgaard-Nielsen, HU Noviello, F Novikov, D Novikov, I Osborne, S Oxborrow, CA Paci, F Pagano, L Pajot, F Paoletti, D Partridge, B Pasian, F Patanchon, G Perdereau, O Perotto, L Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Rebolo, R Reinecke, M Remazeilles, M Renault, C Ricciardi, S Riller, T Ristorcelli, I Rocha, G Roman, M Rosset, C Roudier, G Rowan-Robinson, M Rubino-Martin, A Rusholme, B Sandri, M Santos, D Savini, G Scott, D Seiffert, MD Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sunyaev, R Sureau, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Tuovinen, J Turler, M Umana, G Valenziano, L Valiviita, J Van Tent, B Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD Weller, J White, M White, SDM Yvon, D Zacchei, A Zonca, A AF Ade, P. A. R. Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Barrena, R. Bartlett, J. G. Battaner, E. Battye, R. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bikmaev, I. Blanchard, A. Bobin, J. Bock, J. J. Boehringer, H. Bonaldi, A. Bond, J. R. Borrill, J. Bouchet, F. R. Bourdin, H. Bridges, M. Brown, M. L. Bucher, M. Burenin, R. Burigana, C. Butler, R. C. Cardoso, J. -F. Carvalho, P. Catalano, A. Challinor, A. Chamballu, A. Chary, R. -R. Chiang, L. -Y Chiang, H. C. Chon, G. Christensen, P. R. Church, S. Clements, D. L. Colombi, S. Colombo, L. P. L. Couchot, F. Coulais, A. Crill, B. P. Curto, A. Cuttaia, F. Da Silva, A. Dahle, H. Danese, L. Davies, R. D. Davis, R. J. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Delouis, J. -M. Democles, J. Desert, F. -X. Dickinson, C. Diego, J. M. Dolag, K. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Finelli, F. Flores-Cacho, I. Forni, O. Frailis, M. Franceschi, E. Fromenteau, S. Galeotta, S. Ganga, K. Genova-Santos, R. T. Giard, M. Giardino, G. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Hansen, F. K. Hanson, D. Harrison, D. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Hurier, G. Jaffe, T. R. Jaffe, A. H. Jones, W. C. Juvela, M. Keihanen, E. Keskitalo, R. Khamitov, I. Kisner, T. S. Kneissl, R. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Lahteenmaki, A. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leahy, J. P. Leonardi, R. Leon-Tavares, J. Lesgourgues, J. Liddle, A. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maffei, B. Maino, D. Mandolesi, N. Marcos-Caballero, A. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Matarrese, S. Matthai, F. Mazzotta, P. Meinhold, P. R. Melchiorri, A. Melin, J. -B. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Miville-Deschenes, M. -A. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Moss, A. Munshi, D. Naselsky, P. Nati, F. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novikov, I. Osborne, S. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paoletti, D. Partridge, B. Pasian, F. Patanchon, G. Perdereau, O. Perotto, L. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Rebolo, R. Reinecke, M. Remazeilles, M. Renault, C. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Roman, M. Rosset, C. Roudier, G. Rowan-Robinson, M. Rubino-Martin, A. Rusholme, B. Sandri, M. Santos, D. Savini, G. Scott, D. Seiffert, M. D. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sunyaev, R. Sureau, F. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Tuovinen, J. Tuerler, M. Umana, G. Valenziano, L. Valiviita, J. Van Tent, B. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. Weller, J. White, M. White, S. D. M. Yvon, D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE cosmological parameters; large-scale structure of Universe; galaxies: clusters: general ID BARYON ACOUSTIC-OSCILLATIONS; SOUTH-POLE TELESCOPE; MASSIVE GALAXY CLUSTERS; LARGE-SCALE STRUCTURE; DIGITAL SKY SURVEY; X-RAY-PROPERTIES; SPT-SZ SURVEY; XMM-NEWTON; HYDRODYNAMIC SIMULATIONS; NONTHERMAL PRESSURE AB We present constraints on cosmological parameters using number counts as a function of redshift for a sub-sample of 189 galaxy clusters from the Planck SZ (PSZ) catalogue. The PSZ is selected through the signature of the Sunyaev-Zeldovich (SZ) effect, and the sub-sample used here has a signal-to-noise threshold of seven, with each object confirmed as a cluster and all but one with a redshift estimate. We discuss the completeness of the sample and our construction of a likelihood analysis. Using a relation between mass M and SZ signal Y calibrated to X-ray measurements, we derive constraints on the power spectrum amplitude sigma(8) and matter density parameter Omega(m) in a flat Lambda CDM model. We test the robustness of our estimates and find that possible biases in the Y-M relation and the halo mass function are larger than the statistical uncertainties from the cluster sample. Assuming the X-ray determined mass to be biased low relative to the true mass by between zero and 30%, motivated by comparison of the observed mass scaling relations to those from a set of numerical simulations, we find that sigma(8) = 0.75 +/- 0.03, Omega(m) = 0.29 +/- 0.02, and sigma(8)(Omega(m)/0.27)(0.3) = 0.764 +/- 0.025. The value of sigma(8) is degenerate with the mass bias; if the latter is fixed to a value of 20% (the central value from numerical simulations) we find sigma(8)(Omega(m)/0.27)(0.3) = 0.78 +/- 0.01 and a tighter one-dimensional range sigma(8) = 0.77 +/- 0.02. We find that the larger values of sigma(8) and Omega(m) preferred by Planck's measurements of the primary CMB anisotropies can be accommodated by a mass bias of about 40%. Alternatively, consistency with the primary CMB constraints can be achieved by inclusion of processes that suppress power on small scales relative to the Lambda CDM model, such as a component of massive neutrinos. We place our results in the context of other determinations of cosmological parameters, and discuss issues that need to be resolved in order to make further progress in this field. C1 [Bartlett, J. G.; Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Fromenteau, S.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Piat, M.; Remazeilles, M.; Roman, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, Sorbonne Paris Cite, Observ Paris, CEA lrfu,APC,CNRS IN2P3, F-75205 Paris 13, France. [Lahteenmaki, A.; Leon-Tavares, J.; Poutanen, T.] Aalto Univ, Metsahovi Radio Observ, Kylmala 02540, Finland. 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EM marian.douspis@ias.u-psud.fr RI Kurki-Suonio, Hannu/B-8502-2016; Tomasi, Maurizio/I-1234-2016; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Lopez-Caniego, Marcos/M-4695-2013; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; Lahteenmaki, Anne/L-5987-2013; Toffolatti, Luigi/K-5070-2014; Novikov, Dmitry/P-1807-2015; Yvon, Dominique/D-2280-2015; Valiviita, Jussi/A-9058-2016; Mazzotta, Pasquale/B-1225-2016; Vielva, Patricio/F-6745-2014; Martinez-Gonzalez, Enrique/E-9534-2015; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; White, Martin/I-3880-2015; Gruppuso, Alessandro/N-5592-2015; Butler, Reginald/N-4647-2015; Barreiro, Rita Belen/N-5442-2014; da Silva, Antonio/A-2693-2010; Remazeilles, Mathieu/N-1793-2015; OI Kurki-Suonio, Hannu/0000-0002-4618-3063; Tomasi, Maurizio/0000-0002-1448-6131; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; Rubino-Martin, Jose Alberto/0000-0001-5289-3021; De Zotti, Gianfranco/0000-0003-2868-2595; Lopez-Caniego, Marcos/0000-0003-1016-9283; Toffolatti, Luigi/0000-0003-2645-7386; Valiviita, Jussi/0000-0001-6225-3693; Mazzotta, Pasquale/0000-0002-5411-1748; Vielva, Patricio/0000-0003-0051-272X; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; White, Martin/0000-0001-9912-5070; Gruppuso, Alessandro/0000-0001-9272-5292; Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Savini, Giorgio/0000-0003-4449-9416; Villa, Fabrizio/0000-0003-1798-861X; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; Hurier, Guillaume/0000-0002-1215-0706; Polenta, Gianluca/0000-0003-4067-9196; Butler, Reginald/0000-0003-4366-5996; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Ricciardi, Sara/0000-0002-3807-4043; Galeotta, Samuele/0000-0002-3748-5115; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; da Silva, Antonio/0000-0002-6385-1609; Finelli, Fabio/0000-0002-6694-3269; Umana, Grazia/0000-0002-6972-8388; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Weller, Jochen/0000-0002-8282-2010; Gregorio, Anna/0000-0003-4028-8785; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243 NR 126 TC 252 Z9 251 U1 5 U2 29 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A20 DI 10.1051/0004-6361/201321521 PG 20 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600001 ER PT J AU Ade, PAR Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Bartlett, JG Battaner, E Benabed, K Benoit, A Benoit-Levy, A Bemard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bonaldi, A Bonavera, L Bond, JR Borrill, J Bouchet, FR Boulanger, F Bridges, M Bucher, M Burigana, C Butler, RC Calabrese, E Cardoso, JF Catalano, A Challinor, A Chamballu, A Chiang, HC Chiang, LY Christensen, PR Church, S Clements, DL Colombi, S Colombo, LPL Combet, C Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Danese, L Davies, RD Davis, RJ de Bemardis, P de Rosa, A de Zotti, G Delabrouille, J Delouis, JM Desert, FX Dickinson, C Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Dunkley, J Dupac, X Efstathiou, G Elsner, F Ensslin, TA Eriksen, HK Finelli, F Forni, O Frailis, M Fraisse, AA Franceschi, E Gaier, TC Galeotta, S Galli, S Ganga, K Giard, M Giardino, G Giraud-Heraud, Y Gjerlow, E Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Gudmundsson, JE Hansen, FK Hanson, D Harrison, D Helou, G Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Homtrup, A Hovest, W Huffenberger, KM Hurier, G Jaffe, AH Jaffe, TR Jewell, J Jones, WC Juvela, M Keihanen, E Kesldtalo, R Kiiveri, K Kisner, TS Krieiss, R Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lahteenmaki, A Lamarre, JM Lasenby, A Lattanzi, M Laureijs, RJ Lawrence, CR Le Jeune, M Leach, S Leahy, JP Leonardi, R Leon-Tavares, J Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lindholm, V Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maffei, B Maino, D Mandolesi, N Marinucci, D Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Mazzotta, P Meinhold, PR Melchiorri, A Mendes, L Menegoni, E Mennella, A Migliaccio, M Millea, M Mitra, S Miville-Deschenes, MA Molinari, D Moneti, A Montier, L Morgante, G Mortlock, D Moss, A Munshi, D Murphy, JA Naselsky, P Nati, F Natoli, P Netterfield, CB Norgaard-Nielsen, HU Noviello, F Novikov, D Novikov, I O'Dwyer, IJ Orieux, F Osborne, S Oxborrow, CA Paci, F Pagano, L Pajot, F Paladini, R Paoletti, D Partridge, B Pasian, F Patanchon, G Paykari, P Perdereaun, O Perotto, L Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Rahlin, A Rebolo, R Reinecke, M Remazeilles, M Renault, C Ricciardi, S Riller, T Ringeval, C Ristorcelli, I Rocha, G Rosset, C Roudier, G Rowan-Robinson, M Rubino-Martin, JA Rusholme, B Sandri, M Sanselme, L Santos, D Savini, G Scott, D Seiffert, MD Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sureau, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Tuovinen, J Turler, M Valenziano, L Valiviita, J Van Tent, B Varis, J Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD Wehus, IK White, M White, SDM Yvon, D Zacchei, A Zonca, A AF Ade, P. A. R. Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Bartlett, J. G. Battaner, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bemard, J. -P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bonaldi, A. Bonavera, L. Bond, J. R. Borrill, J. Bouchet, F. R. Boulanger, F. Bridges, M. Bucher, M. Burigana, C. Butler, R. C. Calabrese, E. Cardoso, J. -F. Catalano, A. Challinor, A. Chamballu, A. Chiang, H. C. Chiang, L. -Y Christensen, P. R. Church, S. Clements, D. L. Colombi, S. Colombo, L. P. L. Combet, C. Couchot, F. Coulais, A. Crill, B. P. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. Davis, R. J. de Bemardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Delouis, J. -M. Desert, F. -X. Dickinson, C. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dunkley, J. Dupac, X. Efstathiou, G. Elsner, F. Ensslin, T. A. Eriksen, H. K. Finelli, F. Forni, O. Frailis, M. Fraisse, A. A. Franceschi, E. Gaier, T. C. Galeotta, S. Galli, S. Ganga, K. Giard, M. Giardino, G. Giraud-Heraud, Y. Gjerlow, E. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Gudmundsson, J. E. Hansen, F. K. Hanson, D. Harrison, D. Helou, G. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Homtrup, A. Hovest, W. Huffenberger, K. M. Hurier, G. Jaffe, A. H. Jaffe, T. R. Jewell, J. Jones, W. C. Juvela, M. Keihanen, E. Kesldtalo, R. Kiiveri, K. Kisner, T. S. krieiss, R. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Lahteenmaki, A. Lamarre, J. -M. Lasenby, A. Lattanzi, M. Laureijs, R. J. Lawrence, C. R. Le Jeune, M. Leach, S. Leahy, J. P. Leonardi, R. Leon-Tavares, J. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lindholm, V. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maffei, B. Maino, D. Mandolesi, N. Marinucci, D. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. Meinhold, P. R. Melchiorri, A. Mendes, L. Menegoni, E. Mennella, A. Migliaccio, M. Millea, M. Mitra, S. Miville-Deschenes, M. -A. Molinari, D. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Moss, A. Munshi, D. Murphy, J. A. Naselsky, P. Nati, F. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novikov, I. O'Dwyer, I. J. Orieux, F. Osborne, S. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paladini, R. Paoletti, D. Partridge, B. Pasian, F. Patanchon, G. Paykari, P. Perdereaun, O. Perotto, L. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Rahlin, A. Rebolo, R. Reinecke, M. Remazeilles, M. Renault, C. Ricciardi, S. Riller, T. Ringeval, C. Ristorcelli, I. Rocha, G. Rosset, C. Roudier, G. Rowan-Robinson, M. Rubino-Martin, J. A. Rusholme, B. Sandri, M. Sanselme, L. Santos, D. Savini, G. Scott, D. Seiffert, M. D. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sureau, F. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Tuovinen, J. Tuerler, M. Valenziano, L. Valiviita, J. Van Tent, B. Varis, J. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. Wehus, I. K. White, M. White, S. D. M. Yvon, D. Zacchei, A. Zonca, A. TI Planck 2013 results. XV. CMB power spectra and likelihood SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE cosmic background radiation; cosmological parameters; cosmology: observations; methods: data analysis ID PROBE WMAP OBSERVATIONS; SOUTH-POLE TELESCOPE; ATACAMA COSMOLOGY TELESCOPE; STAR-FORMING GALAXIES; MICROWAVE BACKGROUND ANISOTROPY; SUPERNOVA LEGACY SURVEY; LOW-RESOLUTION DATA; SUNYAEV-ZELDOVICH; EXTRAGALACTIC SOURCES; COMPONENT SEPARATION AB This paper presents the Planck 2013 likelihood, a complete statistical description of the two-point correlation function of the CMB temperature fluctuations that accounts for all known relevant uncertainties, both instrumental and astrophysical in nature. We use this likelihood to derive our best estimate of the CMB angular power spectrum from Planck over three decades in multipole moment, t, covering 2 2500. The main source of uncertainty at S 1500 is cosmic variance. Uncertainties in small-scale foreground modelling and instrumental noise dominate the error budget at higher Es. For < 50, our likelihood exploits all Planck frequency channels from 30 to 353 GHz, separating the cosmological CMB signal from diffuse Galactic foregrounds through a physically motivated Bayesian component separation technique. At 50, we employ a correlated Gaussian likelihood approximation based on a fine-grained set of angular cross-spectra derived from multiple detector combinations between the 100, 143, and 217 GHz frequency channels, marginalising over power spectrum foreground templates. We validate our likelihood through an extensive suite of consistency tests, and assess the impact of residual foreground and instrumental uncertainties on the final cosmological parameters. We find good internal agreement among the high- cross-spectra with residuals below a few fiK2 at S 1000, in agreement with estimated calibration uncertainties. We compare our results with foreground-cleaned CMB maps derived from all Planck frequencies, as well as with cross-spectra derived from the 70 GHz Planck map, and find broad agreement in terms of spectrum residuals and cosmological parameters. We further show that the best-fit ACDM cosmology is in excellent agreement with preliminary Planck EE and T E polarisation spectra. We find that the standard ACDM cosmology is well constrained by Planck from the measurements at C 1500. One specific example is the spectral index of scalar perturbations, for which we report a 5.4o- deviation from scale invariance, ns = 1. Increasing the multipole range beyond = 1500 does not increase our accuracy for the ACDM parameters, but instead allows us to study extensions beyond the standard model. We find no indication of significant departures from the ACDM framework. Finally, we report a tension between the Planck best-fit ACDM model and the low- spectrum in the form of a power deficit of 5-10% at 40, with a statistical significance of 2.5-3o-. Without a theoretically motivated model for this power deficit, we do not elaborate further on its cosmological implications, but note that this is our most puzzling finding in an otherwise remarkably consistent data set. C1 [Bartlett, J. G.; Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Le Jeune, M.; Patanchon, G.; Piat, M.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, APC, CNRS IN2P3, CEA lrfu,Observ Paris,Sorbonne Paris Cite, F-75205 Paris 13, France. [Lahteenmaki, A.; Leon-Tavares, J.; Poutanen, T.] Aalto Univ, Metsahovi Radio Observ, Kylmala 02540, Finland. [Kunz, M.] African Inst Math Sci, ZA-7945 Cape Town, South Africa. [Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana Sci Data Ctr, I-00133 Rome, Italy. 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[Chiang, L. -Y] Acad Sinica, Inst Astron & Astrophys, Taipei 10617, Taiwan. [Challinor, A.; Efstathiou, G.; Gratton, S.; Harrison, D.; Migliaccio, M.; Sutton, D.] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England. [Ringeval, C.] Univ Louvain, Ctr Cosmol Particle Phys & Phenomenol, Inst Math & Phys, B-1348 Louvain, Belgium. [Eriksen, H. K.; Gjerlow, E.; Hansen, F. K.; Lilje, P. B.; Valiviita, J.] Univ Oslo, Inst Theoret Astrophys, N-0315 Oslo, Norway. [Rebolo, R.; Rubino-Martin, J. A.] Inst Astrofis Canarias, Tenerife 38205, Spain. [Barreiro, R. B.; Bonavera, L.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Toffolatti, L.; Vielva, P.] Univ Cantabria, CSIC, Inst Fis Cantabria, E-39005 Santander, Spain. [Bartlett, J. G.; Bock, J. J.; Colombo, L. P. L.; Crill, B. P.; Dore, O.; Gaier, T. C.; Gorski, K. M.; Hanson, D.; Holmes, W. A.; Jewell, J.; Lawrence, C. R.; Mitra, S.; O'Dwyer, I. J.; Pietrobon, D.; Prezeau, G.; Rocha, G.; Roudier, G.; Seiffert, M. D.; Wade, L. A.; Wehus, I. K.] CALTECH, Jet Prop Lab, Pasadena, CA USA. [Bonaldi, A.; Davies, R. D.; Davis, R. J.; Dickinson, C.; Leahy, J. P.; Maffei, B.; Noviello, F.; Remazeilles, M.] Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Manchester M13 9PL, Lancs, England. [Ashdown, M.; Bridges, M.; Challinor, A.; Gratton, S.; Harrison, D.; Lasenby, A.; Migliaccio, M.; Stolyarov, V.; Sutton, D.] Kavli Inst Cosmol Cambridge, Cambridge CB3 0HA, England. [Couchot, F.; Henrot-Versille, S.; Perdereaun, O.; Plaszczynski, S.; Tristram, M.; Tucci, M.] Univ Paris 11, CNRS IN2P3, LAL, F-91898 Orsay, France. [Catalano, A.; Coulais, A.; Lamarre, J. -M.; Roudier, G.] CNRS, LERMA, Observ Paris, F-75014 Paris, France. [Arnaud, M.; Bobin, J.; Chamballu, A.; Marshall, D. J.; Paykari, P.; Pratt, G. W.; Starck, J. -L.; Sureau, F.] Univ Paris Diderot, CEA Saclay, CNRS, IRFU Serv Astrophys CEA DSM,Lab AIM, F-91191 Gif Sur Yvette, France. [Cardoso, J. -F.] CNRS, Lab Traitement & Commun Informat, UMR 5141, F-75634 Paris 13, France. [Cardoso, J. -F.] Telecom ParisTech, F-75634 Paris 13, France. [Catalano, A.; Combet, C.; Hurier, G.; Macias-Perez, J. F.; Perotto, L.; Renault, C.; Sanselme, L.; Santos, D.] Univ Joseph Fourier Grenoble I, CNRS IN2P3, Inst Natl Polytech Grenoble, F-38026 Grenoble, France. [Van Tent, B.] Univ Paris 11, Phys Theor Lab, F-91405 Orsay, France. [Van Tent, B.] CNRS, F-91405 Orsay, France. [Kisner, T. S.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Ensslin, T. A.; Hernandez-Monteagudo, C.; Hovest, W.; Knoche, J.; Matthai, F.; Rachen, J. P.; Reinecke, M.; Riller, T.; White, S. D. M.] Max Planck Inst Astrophys, D-85741 Garching, Germany. [Hanson, D.] McGill Univ, Montreal H3A 2T8, PQ, Canada. [Tuovinen, J.; Varis, J.] VTT Tech Res Ctr Finland, MilliLab, Espoo 02044, Finland. [Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Co Kildare, Ireland. [Christensen, P. R.; Naselsky, P.; Novikov, I.] Niels Bohr Inst, DK-2100 Copenhagen, Denmark. [Crill, B. P.] CALTECH, Observ Cosmol, Pasadena, CA 91125 USA. [Savini, G.] UCL, Opt Sci Lab, London, England. [Lesgourgues, J.] Ecole Polytech Fed Lausanne, SB ITP LPPC, CH-1015 Lausanne, Switzerland. [Baccigalupi, C.; Bielewicz, P.; Danese, L.; de Zotti, G.; Gonzalez-Nuevo, J.; Leach, S.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sect, I-34136 Trieste, Italy. [Ade, P. A. R.; Munshi, D.; Spencer, L. D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales. [Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England. [Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA. [Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz 369167, Zelenchukskiy R, Russia. [Church, S.; Osborne, S.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA. [Armitage-Caplan, C.; Calabrese, E.; Dunkley, J.] Univ Oxford, Subdept Astrophys, Oxford OX1 3RH, England. [Lesgourgues, J.] CERN, PH TH, Div Theory, CH-1211 Geneva 23, Switzerland. [Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Colombi, S.; Delouis, J. -M.; Elsner, F.; Hivon, E.; Prunet, S.; Ringeval, C.; Wandelt, B. D.] Univ Paris 06, UMR7095, F-75014 Paris, France. [Banday, A. J.; Bemard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, IRAP, UPS OMP, F-31028 Toulouse 4, France. [Battaner, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, E-18071 Granada, Spain. [Gorski, K. M.] Univ Warsaw Observ, PL-00478 Warsaw, Poland. RP Bouchet, FR (reprint author), CNRS, Inst Astrophys Paris, UMR 7095, 98bis Bd Arago, F-75014 Paris, France. EM bouchet@iap.fr RI Butler, Reginald/N-4647-2015; Barreiro, Rita Belen/N-5442-2014; Remazeilles, Mathieu/N-1793-2015; Kurki-Suonio, Hannu/B-8502-2016; Tomasi, Maurizio/I-1234-2016; Lattanzi, Massimiliano/D-8120-2011; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; bonavera, laura/E-9368-2017; Lahteenmaki, Anne/L-5987-2013; Valiviita, Jussi/A-9058-2016; Mazzotta, Pasquale/B-1225-2016; Toffolatti, Luigi/K-5070-2014; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Martinez-Gonzalez, Enrique/E-9534-2015; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; White, Martin/I-3880-2015; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015 OI Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Savini, Giorgio/0000-0003-4449-9416; Villa, Fabrizio/0000-0003-1798-861X; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; Hurier, Guillaume/0000-0002-1215-0706; Molinari, Diego/0000-0002-7799-3915; Butler, Reginald/0000-0003-4366-5996; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Ricciardi, Sara/0000-0002-3807-4043; Maris, Michele/0000-0001-9442-2754; Matarrese, Sabino/0000-0002-2573-1243; Galeotta, Samuele/0000-0002-3748-5115; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Lopez-Caniego, Marcos/0000-0003-1016-9283; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Finelli, Fabio/0000-0002-6694-3269; De Zotti, Gianfranco/0000-0003-2868-2595; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Kurki-Suonio, Hannu/0000-0002-4618-3063; Tomasi, Maurizio/0000-0002-1448-6131; Lattanzi, Massimiliano/0000-0003-1059-2532; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; bonavera, laura/0000-0001-8039-3876; Rubino-Martin, Jose Alberto/0000-0001-5289-3021; Valiviita, Jussi/0000-0001-6225-3693; Mazzotta, Pasquale/0000-0002-5411-1748; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; White, Martin/0000-0001-9912-5070; Gruppuso, Alessandro/0000-0001-9272-5292; FU ESA FX The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members with the technical or scientific activities they have been involved into, can be found at http: //www. set ups. esa. int/index. phprproj net= planck&page=Planck_Collaboration. We acknowledge the use of the CLASS Boltzmann code (Lesgourgues 201D and the Monte Python package (Audren et al, 2013) in earlier stages of this work. The likelihood code and some of the validation work was built on the library pmclib from the CosmoPMC package (Kilhinger et al. 2011). This research used resources of the IN2P3 Computer Center (http //cc.in2p3.fr) as well as of the Planck-HFI data processing centre infrastructures hosted at the Institut d'Astrophysique de Paris (France) and financially supported by CNES. NR 124 TC 399 Z9 398 U1 18 U2 63 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A15 DI 10.1051/0004-6361/201321573 PG 60 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600023 ER PT J AU Ade, PAR Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Bartlett, JG Bartolo, N Battaner, E Battye, R Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bonaldi, A Bonavera, L Bond, JR Borrill, J Bouchet, FR Bridges, M Bucher, M Burigana, C Butler, RC Cardoso, JF Catalano, A Challinor, A Chamballu, A Chiang, LY Chiang, HC Christensen, PR Church, S Clements, DL Colombi, S Colombo, LPL Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Danese, L Davies, RD Davis, RJ de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Delouis, JM Desert, FX Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Ducout, A Dunkley, J Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Fergusson, J Finelli, F Forni, O Frailis, M Franceschi, E Galeotta, S Ganga, K Giard, M Giardino, G Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Hansen, FK Hanson, D Harrison, D Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Jaffe, TR Jaffe, AH Jones, WC Juvela, M Keihanen, E Keskitalo, R Kisner, TS Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lahteenmaki, A Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Leahy, JP Leonardi, R Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maffei, B Maino, D Mandolesi, N Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Matarrese, S Matthai, F Mazzotta, P McEwen, JD Melchiorri, A Mendes, L Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, MA Moneti, A Montier, L Morgante, G Mortlock, D Moss, A Munshi, D Naselsky, P Natoli, P Netterfield, CB Norgaard-Nielsen, HU Noviello, F Novikov, D Novikov, I Osborne, S Oxborrow, CA Paci, F Pagano, L Pajot, F Paoletti, D Pasian, F Patanchon, G Peiris, HV Perdereau, O Perotto, L Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Rath, C Rebolo, R Remazeilles, M Renault, C Ricciardi, S Riller, T Ringeval, C Ristorcelli, I Rocha, G Rosset, C Roudier, G Rowan-Robinson, M Rusholme, B Sandri, M Santos, D Savini, G Scott, D Seiffert, MD Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sureau, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Tuovinen, J Valenziano, L Valiviita, J Van Tent, B Varis, J Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD Yvon, D Zacchei, A Zonca, A AF Ade, P. A. R. Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Bartlett, J. G. Bartolo, N. Battaner, E. Battye, R. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bonaldi, A. Bonavera, L. Bond, J. R. Borrill, J. Bouchet, F. R. Bridges, M. Bucher, M. Burigana, C. Butler, R. C. Cardoso, J. -F. Catalano, A. Challinor, A. Chamballu, A. Chiang, L. -Y Chiang, H. C. Christensen, P. R. Church, S. Clements, D. L. Colombi, S. Colombo, L. P. L. Couchot, F. Coulais, A. Crill, B. P. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. Davis, R. J. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Delouis, J. -M. Desert, F. -X. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Ducout, A. Dunkley, J. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Fergusson, J. Finelli, F. Forni, O. Frailis, M. Franceschi, E. Galeotta, S. Ganga, K. Giard, M. Giardino, G. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Hansen, F. K. Hanson, D. Harrison, D. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Jaffe, T. R. Jaffe, A. H. Jones, W. C. Juvela, M. Keihanen, E. Keskitalo, R. Kisner, T. S. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Lahteenmaki, A. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leahy, J. P. Leonardi, R. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maffei, B. Maino, D. Mandolesi, N. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Matarrese, S. Matthai, F. Mazzotta, P. McEwen, J. D. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Miville-Deschenes, M. -A. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Moss, A. Munshi, D. Naselsky, P. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novikov, I. Osborne, S. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paoletti, D. Pasian, F. Patanchon, G. Peiris, H. V. Perdereau, O. Perotto, L. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Raeth, C. Rebolo, R. Remazeilles, M. Renault, C. Ricciardi, S. Riller, T. Ringeval, C. Ristorcelli, I. Rocha, G. Rosset, C. Roudier, G. Rowan-Robinson, M. Rusholme, B. Sandri, M. Santos, D. Savini, G. Scott, D. Seiffert, M. D. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sureau, F. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Tuovinen, J. Valenziano, L. Valiviita, J. Van Tent, B. Varis, J. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. Yvon, D. Zacchei, A. Zonca, A. TI Planck 2013 results. XXV. Searches for cosmic strings and other topological defects SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE cosmic background radiation; cosmological parameters; early Universe; large-scale structure of Universe; cosmology: theory; cosmology: observations ID MICROWAVE BACKGROUND FLUCTUATIONS; NON-GAUSSIANITY; HIGHER CRITICISM; VACUUM STRINGS; POWER SPECTRUM; WMAP DATA; EVOLUTION; ANISOTROPY; NETWORKS; WAVELETS AB Planck data have been used to provide stringent new constraints on cosmic strings and other defects. We describe forecasts of the CMB power spectrum induced by cosmic strings, calculating these from network models and simulations using line-of-sight Boltzmann solvers. We have studied Nambu-Goto cosmic strings, as well as field theory strings for which radiative effects are important, thus spanning the range of theoretical uncertainty in the underlying strings models. We have added the angular power spectrum from strings to that for a simple adiabatic model, with the extra fraction defined as f(10) at multipole l = 10. This parameter has been added to the standard six parameter fit using CO S M OM C with flat priors. For the Nambu-Goto string model, we have obtained a constraint on the string tension of G mu/c(2) < 1.5 x 10(-7) and f(10) < 0.015 at 95% confidence that can be improved to G mu/c(2) < 1.3 x 10(-7) and f(10) < 0.010 on inclusion of high-l CMB data. For the Abelian-Higgs field theory model we find, G mu(AH)/c2 < 3.2x10(-7) and f(10) < 0.028. The marginalised likelihoods for f(10) and in the f(10)-Omega(b)h(2) plane are also presented. We have additionally obtained comparable constraints on f(10) for models with semilocal strings and global textures. In terms of the effective defect energy scale these are somewhat weaker at G mu/c(2) < 1.1 x 10(-6). We have made complementarity searches for the specific non-Gaussian signatures of cosmic strings, calibrating with all-sky Planck resolution CMB maps generated from networks of post-recombination strings. We have validated our non-Gaussian searches using these simulated maps in a Planck-realistic context, estimating sensitivities of up to Delta G mu/c(2) approximate to 4 x 10(-7). We have obtained upper limits on the string tension at 95% confidence of G mu/c(2) < 9.0 x 10(-7) with modal bispectrum estimation and G mu/c(2) < 7.8 x 10(-7) for real space searches with Minkowski functionals. These are conservative upper bounds because only post-recombination string contributions have been included in the non-Gaussian analysis. C1 [Bartlett, J. G.; Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Piat, M.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, Sorbonne Paris Cite, APC, CNRS IN2P3,CEA Lrfu,Observ Paris, F-75205 Paris 13, France. [Lahteenmaki, A.; Poutanen, T.] Aalto Univ, Metsahovi Radio Observ, Kylmala 02540, Finland. [Kunz, M.] African Inst Math Sci, ZA-7701 Rondebosch Cape Town, South Africa. [Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana Sci Data Ctr, I-00044 Frascati, Italy. [Mandolesi, N.] Agenzia Spaziale Italiana, I-00198 Rome, Italy. [Ashdown, M.; Bridges, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 0HE, England. [Chiang, H. C.] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, ZA-4000 Durban, South Africa. [Bond, J. R.; Hanson, D.; Martin, P. G.; Miville-Deschenes, M. -A.] Univ Toronto, CITA, Toronto, ON M5S 3H8, Canada. [Banday, A. 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[Ashdown, M.; Bridges, M.; Challinor, A.; Gratton, S.; Harrison, D.; Lasenby, A.; Migliaccio, M.; Stolyarov, V.; Sutton, D.] Kavli Inst Cosmol Cambridge, Cambridge CB3 0HA, England. [Couchot, F.; Henrot-Versille, S.; Perdereau, O.; Plaszczynski, S.; Tristram, M.; Tucci, M.] Univ Paris 11, LAL, CNRS, IN2P3, F-91898 Orsay, France. [Catalano, A.; Coulais, A.; Lamarre, J. -M.; Roudier, G.] Observ Paris, CNRS, LERMA, F-75014 Paris, France. [Arnaud, M.; Bobin, J.; Chamballu, A.; Marshall, D. J.; Pratt, G. W.; Starck, J. -L.; Sureau, F.] Univ Paris Diderot, CEA Saclay, Lab AIM, IRFU Serv Astrophys CEA DSM CNRS, F-91191 Gif Sur Yvette, France. [Cardoso, J. -F.] CNRS, UMR 5141, Lab Traitement & Commun Informat, F-75634 Paris 13, France. [Cardoso, J. -F.] Telecom ParisTech, F-75634 Paris 13, France. [Catalano, A.; Macias-Perez, J. F.; Perotto, L.; Renault, C.; Santos, D.] Univ Grenoble 1, Lab Phys Subatom & Cosmol, Inst Natl Polytech Grenoble, CNRS IN2P3, F-38026 Grenoble, France. 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J.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France. [Battaner, E.] Univ Granada, Dept Fis Teor & Cosmos, Fac Ciencias, Granada 1807, Spain. [Huffenberger, K. M.] Univ Miami, Coral Gables, FL 33124 USA. [Gorski, K. M.] Univ Warsaw Observ, PL-00478 Warsaw, Poland. RP Moss, A (reprint author), Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England. EM adam.moss@nottingham.ac.uk RI Barreiro, Rita Belen/N-5442-2014; Butler, Reginald/N-4647-2015; Lahteenmaki, Anne/L-5987-2013; Mazzotta, Pasquale/B-1225-2016; Toffolatti, Luigi/K-5070-2014; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Kurki-Suonio, Hannu/B-8502-2016; Martinez-Gonzalez, Enrique/E-9534-2015; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Valiviita, Jussi/A-9058-2016; Tomasi, Maurizio/I-1234-2016; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; bonavera, laura/E-9368-2017; Remazeilles, Mathieu/N-1793-2015; OI Savini, Giorgio/0000-0003-4449-9416; Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Ricciardi, Sara/0000-0002-3807-4043; Villa, Fabrizio/0000-0003-1798-861X; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Lopez-Caniego, Marcos/0000-0003-1016-9283; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Butler, Reginald/0000-0003-4366-5996; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Mazzotta, Pasquale/0000-0002-5411-1748; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; Kurki-Suonio, Hannu/0000-0002-4618-3063; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Gruppuso, Alessandro/0000-0001-9272-5292; Valiviita, Jussi/0000-0001-6225-3693; Tomasi, Maurizio/0000-0002-1448-6131; Colombo, Loris/0000-0003-4572-7732; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; bonavera, laura/0000-0001-8039-3876; De Zotti, Gianfranco/0000-0003-2868-2595; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Galeotta, Samuele/0000-0002-3748-5115; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269 FU ESA; CNES FX The development of Planck has been supported by: ESA; CNES and CNRS /INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER /SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT /MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.sciops.esa.int/index.php?project=planck&page=Planck_Collabora tion. We also wish to acknowledge the use of the COSMOS supercomputer, part of the DiRAC HPC Facility funded by STFC and the UK Large Facilities Capital Fund, use of the Andromeda cluster of the University of Geneva, and resources of the National Energy Research Scientific Computing Center. NR 120 TC 150 Z9 149 U1 3 U2 22 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A25 DI 10.1051/0004-6361/201321621 PG 21 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600028 ER PT J AU Ade, PAR Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Bartlett, JG Bartolo, N Battaner, E Battye, R Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bonaldi, A Bonavera, L Bond, JR Borrill, J Bouchet, FR Bridges, M Bucher, M Burigana, C Butler, RC Cardoso, JF Catalano, A Challinor, A Chamballu, A Chary, RR Chiang, HC Chiang, LY Christensen, PR Church, S Clements, DL Colombi, S Colombo, LPL Couchot, F Coulais, A Crill, BP Cruz, M Curto, A Cuttaia, F Danese, L Davies, RD Davis, RJ de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Delouis, JM Desert, FX Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Ducout, A Dupac, X Efstathiou, G Elsner, F Ensslin, TA Eriksen, HK Fantaye, Y Fergusson, J Finelli, F Forni, O Frailis, M Franceschi, E Frommert, M Galeotta, S Ganga, K Giard, M Giardino, G Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Hansen, FK Hansen, M Hanson, D Harrison, DL Helou, G Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Jaffe, AH Jaffe, TR Jones, WC Juvela, M Keihanen, E Keskitalo, R Kim, J Kisner, TS Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lahteenmaki, A Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Leahy, JP Leonardi, R Leroy, C Lesgourgues, J Liguori, M Lille, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maffei, B Maino, D Mandolesi, N Mangilli, A Marinucci, D Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Mazzotta, P McEwen, JD Meinhold, PR Melchiorri, A Mendes, L Mennella, A Migliaccio, M Mikkelsen, K Mitra, S Miville-Deschenes, MA Molinari, D Moneti, A Montier, L Morgante, G Mortlock, D Moss, A Munshi, D Murphy, JA Naselsky, P Nati, F Natoli, P Netterfield, CB Norgaard-Nielsen, HU Noviello, F Novikov, D Novikov, I Osborne, S Oxborrowl, CA Paci, F Pagano, L Pajot, F Paoletti, D Pasian, F Patanchon, G Peiris, HV Perdereau, O Perotto, L Perrotta, F Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Pogosyan, D Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Racine, B Rath, C Rebolo, R Reinecke, M Remazeilles, M Renault, C Renzi, A Ricciardi, S Riller, T Ristorcelli, I Rocha, G Rosset, C Rotti, A Roudier, G Rubino-Martin, JA Ruiz-Granadosioi, B Rusholme, B Sandri, M Santos, D Savini, G Scott, D Seiffert, MD Shellard, EPS Souradeep, T Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sureau, F Sutter, P Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Tuovinen, J Turler, M Valenziano, L Valiviita, J Van Tent, B Varis, J Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD Wehus, IK White, M Wilkinson, A Yvon, D Zacchei, A Zonca, A AF Ade, P. A. R. Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Bartlett, J. G. Bartolo, N. Battaner, E. Battye, R. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bonaldi, A. Bonavera, L. Bond, J. R. Borrill, J. Bouchet, F. R. Bridges, M. Bucher, M. Burigana, C. Butler, R. C. Cardoso, J. -F. Catalano, A. Challinor, A. Chamballu, A. Chary, R. -R. Chiang, H. C. Chiang, L. -Y Christensen, P. R. Church, S. Clements, D. L. Colombi, S. Colombo, L. P. L. Couchot, F. Coulais, A. Crill, B. P. Cruz, M. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. Davis, R. J. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Delouis, J. -M. Desert, F. -X. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Ducout, A. Dupac, X. Efstathiou, G. Elsner, F. Ensslin, T. A. Eriksen, H. K. Fantaye, Y. Fergusson, J. Finelli, F. Forni, O. Frailis, M. Franceschi, E. Frommert, M. Galeotta, S. Ganga, K. Giard, M. Giardino, G. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Hansen, F. K. Hansen, M. Hanson, D. Harrison, D. L. Helou, G. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Jaffe, A. H. Jaffe, T. R. Jones, W. C. Juvela, M. Keihanen, E. Keskitalo, R. Kim, J. Kisner, T. S. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Lahteenmaki, A. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leahy, J. P. Leonardi, R. Leroy, C. Lesgourgues, J. Liguori, M. Lille, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maffei, B. Maino, D. Mandolesi, N. Mangilli, A. Marinucci, D. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. McEwen, J. D. Meinhold, P. R. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Mikkelsen, K. Mitra, S. Miville-Deschenes, M. -A. Molinari, D. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Moss, A. Munshi, D. Murphy, J. A. Naselsky, P. Nati, F. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novikov, I. Osborne, S. Oxborrowl, C. A. Paci, F. Pagano, L. Pajot, F. Paoletti, D. Pasian, F. Patanchon, G. Peiris, H. V. Perdereau, O. Perotto, L. Perrotta, F. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pogosyan, D. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Racine, B. Raeth, C. Rebolo, R. Reinecke, M. Remazeilles, M. Renault, C. Renzi, A. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Rosset, C. Rotti, A. Roudier, G. Rubino-Martin, J. A. Ruiz-Granadosioi, B. Rusholme, B. Sandri, M. Santos, D. Savini, G. Scott, D. Seiffert, M. D. Shellard, E. P. S. Souradeep, T. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sureau, F. Sutter, P. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Tuovinen, J. Tuerler, M. Valenziano, L. Valiviita, J. Van Tent, B. Varis, J. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. Wehus, I. K. White, M. Wilkinson, A. Yvon, D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. XXIII. Isotropy and statistics of the CMB SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE cosmic background radiation; cosmology: observations; cosmology: miscellaneous ID MICROWAVE-ANISOTROPY-PROBE; PRIMORDIAL NON-GAUSSIANITY; DIRECTIONAL SPHERICAL WAVELETS; HEMISPHERICAL POWER ASYMMETRY; DEPENDENT NON-GAUSSIANITIES; POINT CORRELATION-FUNCTIONS; WMAP DATA; BACKGROUND ANISOTROPY; MINKOWSKI FUNCTIONALS; COLD SPOT AB The two fundamental assumptions of the standard cosmological model - that the initial fluctuations are statistically isotropic and Gaussian - are rigorously tested using maps of the cosmic microwave background (CMB) anisotropy from the Planck satellite. The detailed results are based on studies of four independent estimates of the CMB that are compared to simulations using a fiducial Lambda CDM model and incorporating essential aspects of the Planck measurement process. Deviations from isotropy have been found and demonstrated to be robust against component separation algorithm, mask choice, and frequency dependence. Many of these anomalies were previously observed in the WMAP data, and are now confirmed at similar levels of significance (about 3 sigma). However, we find little evidence of non-Gaussianity, with the exception of a few statistical signatures that seem to be associated with specific anomalies. In particular, we find that the quadrupole-octopole alignment is also connected to a low observed variance in the CMB signal. A power asymmetry is now found to persist on scales corresponding to about l = 600 and can be described in the low-l regime by a phenomenological dipole modulation model. However, any primordial power asymmetry is strongly scale-dependent and does not extend to arbitrarily small angular scales. Finally, it is plausible that some of these features may be reflected in the angular power spectrum of the data, which shows a deficit of power on similar scales. Indeed, when the power spectra of two hemispheres defined by a preferred direction are considered separately, one shows evidence of a deficit in power, while its opposite contains oscillations between odd and even modes that may be related to the parity violation and phase correlations also detected in the data. Although these analyses represent a step forward in building an understanding of the anomalies, a satisfactory explanation based on physically motivated models is still lacking. C1 [Bartlett, J. G.; Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Piat, M.; Racine, B.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, Observ Paris, Sorbonne Paris Cite, CNRS IN2P3,CEA lrfu,APC, F-75205 Paris 13, France. 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EM martinez@ifca.unican.es RI Lahteenmaki, Anne/L-5987-2013; Valiviita, Jussi/A-9058-2016; Toffolatti, Luigi/K-5070-2014; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Cruz, Marcos/N-3429-2014; Martinez-Gonzalez, Enrique/E-9534-2015; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; White, Martin/I-3880-2015; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Mazzotta, Pasquale/B-1225-2016; Kurki-Suonio, Hannu/B-8502-2016; Tomasi, Maurizio/I-1234-2016; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; bonavera, laura/E-9368-2017; Remazeilles, Mathieu/N-1793-2015; Renzi, Alessandro/K-4114-2015; Barreiro, Rita Belen/N-5442-2014; Butler, Reginald/N-4647-2015; OI Valiviita, Jussi/0000-0001-6225-3693; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; Cruz, Marcos/0000-0002-4767-530X; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; White, Martin/0000-0001-9912-5070; Gruppuso, Alessandro/0000-0001-9272-5292; Mazzotta, Pasquale/0000-0002-5411-1748; Kurki-Suonio, Hannu/0000-0002-4618-3063; Tomasi, Maurizio/0000-0002-1448-6131; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; bonavera, laura/0000-0001-8039-3876; Rubino-Martin, Jose Alberto/0000-0001-5289-3021; De Zotti, Gianfranco/0000-0003-2868-2595; Lopez-Caniego, Marcos/0000-0003-1016-9283; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Maris, Michele/0000-0001-9442-2754; Renzi, Alessandro/0000-0001-9856-1970; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Galeotta, Samuele/0000-0002-3748-5115; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Butler, Reginald/0000-0003-4366-5996; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Ricciardi, Sara/0000-0002-3807-4043; Villa, Fabrizio/0000-0003-1798-861X; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; Molinari, Diego/0000-0002-7799-3915; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Savini, Giorgio/0000-0003-4449-9416; Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834 FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR (Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC (Spain); MICINN (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF (Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); PRACE (EU) FX The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.sciops.esa.int/index.php?project=planck&page=Planck_Collabora tion. We acknowledge the use of resources from the Norewegian national super computing facilities NOTUR. The modal and KSW bispectrum estimator analysis was performed on the COSMOS supercomputer, part of the STFC DiRAC HPC Facility. We further acknowledge the computer resources and technical assistance provided by the Spanish Supercomputing Network nodes at Universidad de Cantabria and Universidad Politecnica de Madrid as well as by the Advanced Computing and e-Science team at IFCA. Some of the results in this paper have been derived using the HEALPix package. NR 150 TC 293 Z9 293 U1 8 U2 35 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A23 DI 10.1051/0004-6361/201321534 PG 48 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600009 ER PT J AU Ade, PAR Aghanim, N Alves, MIR Armitage-CaplanI, C Amaud, M Ashdown, M Atrio-Barandela, F Aumont, J Ausse, H Baccigalupi, C Banday, AJ Barreiro, RB Barrenass, R Bartelmann, M Bartlett, JG Bartolo, N Basak, S Battaner, E Battye, R Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bertincourt, B Bethermin, M Bielewicz, P Bikmaev, I Blanchard, A Bobin, J Bock, JJ Bohringer, H Bonaldi, A Bonavera, L Bond, JR Borrill, J Bouchet, FR Boulanger, F Bourdin, H Bowyer, JW Bridges, M Brown, ML Bucher, M Burenin, R Burigana, C Butler, RC Calabrese, E Cappellini, B Cardoso, JF Carr, R Carvalho, P Casale, M Castexl, G Catalano, A Challinor, A Chamballu, A Chary, RR Chen, X Chiang, HC Chiang, LY Chon, G Christensen, PR Churazov, E Church, S Clemens, M Clements, DL Colombi, S Colombo, LPL Combet, C Comis, B Couchot, E Coulais, A Crill, BP Cruz, M Curto, A Cuttaia, F Da Silva, A Dahle, H Danese, L Davies, RD Davis, RJ de Bernardis, P de Rosa, A de Zotti, G Dechelette, T Delabrouille, J Delouis, JM Democles, J Desert, FX Dick, J Dickinson, C Diego, JM Dolag, K Dole, H Donzelli, S Dore, O Douspis, M Ducout, A Dunkley, J Dupac, X Efstathiou, G Elsner, F Ensslin, TA Eriksen, HK Fabre, O Falgarone, E Falvella, MC Fantaye, Y FergussonI, J Filliard, C Finelli, F Flores-Cacho, I Foley, S Forni, O Fosalba, P Frailis, M Fraisse, AA Franceschi, E Freschi, M Fromenteau, S Frommert, M Gaier, TC Galeotta, S Gallegos, J Galli, S Gandolfo, B Ganga, K Gauthier, C Genova-Santos, RT Ghosh, T Giard, M Giardino, G Gilfanov, M Girard, D Giraud-Heraud, Y Gjerlow, E Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Gudmundsson, JE Haissinski, J Hamann, J Hansen, FK Hansen, M Hanson, D Harrison, DL Heavens, A Helou, G Hempel, A Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Ho, S Hobson, M Holmes, WA Hornstrup, A Hou, Z Hovest, W Huey, G Huffenberger, KM Hurier, G Ilic, S Jaffe, AH Jaffe, TR Jasches, J Jewell, J Jones, WC Juvela, M Kalberla, P Kangaslahti, P Keihanen, E Kerp, J Keskitalo, R Khamitov, I Kiiveri, K Kim, J Kisnerl, TS Kneissl, R Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lacasa, E Lagache, G Lahteenmaki, A Lamarre, JM Langer, M Lasenby, A Lattanzi, M Laureijs, RJ Lavabre, A Lawrence, CR Le Jeune, M Leach, S Leahy, JP Leonardi, R Leon-Tavares, J Leroy, C Lesgourgues, J Lewis, A Li, C Liddle, A Liguori, M Lilie, PB Linden-Vornle, M Lindholm, V Lopez-Caniego, M Lowe, S Lubin, PM Macias-Perez, JF MacTavish, CJ Maffei, B Maggio, G Maino, D Mandolesi, N Mangilli, A Marcos-Caballero, A Marinucci, D Maris, M Marleau, F Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matsumura, T Matthai, E Maurin, L Mazzotta, P McDonald, A McEwen, JD McGehee, P Mei, S Meinhold, PR Melchiorri, A Melin, JB Mendes, L Menegoni, E Mennella, A Migliaccio, M Mikkelsen, K Millea, M Miniscalco, R Mitra, S Miville-Deschenes, MA Molinari, D Moneti, A Montier, L Morgante, G Morisset, N Mortlock, D Moss, A Munshi, D Murphy, JA Naselsky, P Nati, E Natoli, P Negrello, M Nesvadba, NPH Netterfield, CB Norgaard-Nielsen, HU North, C Noviello, F Novikov, D Novikov, I O'Dwyer, IJ Orieux, F Osborne, S O'Sullivan, C Oxborrow, CA Paci, F Pagano, L Pajot, F Paladini, R Pandolfi, S Paoletti, D Partridge, B Pasian, F Patanchon, G Paykari, P Pearson, D Pearson, TJ Peel, M Peiris, HV Perdereau, O Perotto, L Perrotta, F Pettorino, V Piacentini, F Piat, M Pierpaoli, E Pietrobon, D Plaszczynski, S Platania, P Pogosyan, D Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Pullen, AR Rachen, JP Racine, B Rahlin, A Rath, C Reach, WT Rebolo, R Reinecke, M Remazeilles, M Renault, C Renzi, A Riazuelo, A Ricciardi, S Rillerl, T Ringeval, C Ristorcelli, I Robbers, G Rocha, G Roman, M Rosset, C Rossetti, M Roudier, G Rowan-Robinson, M Rubino-Martin, JA Ruiz-Granados, B Rusholme, B Salerno, E Sandri, M Sanselme, L Santos, D Savelainen, M Savini, G Schaefer, BM Schiavon, F Scott, D Seiffert, MD Serra, P Shellard, EPS Smith, K Smoot, GE Souradeep, T Spencer, LD Starck, JL Stolyarov, V Stompor, R Sudiwala, R Sunyaev, R Sureau, F Sutteer, P Sutton, D Suur-Uski, AS Sygnet, JE Tauber, JA Tavagnacco, D Taylor, D Terenzi, L Texier, D Toffolatti, L Tomasi, M Torre, JP Tristram, M Tucci, M Tuovinen, J Turler, M Tuttlebee, M Umana, G Valenziano, L Valiviita, J Van Tent, B Varisi, J Vibert, L Viel, M Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD Watson, C Watson, R Wehus, IK Welikala, N Weller, J White, M White, SDM Wilkinson, A Winkel, B Xia, JQ Yvon, D Zacchei, A Zibin, JP Zonca, A AF Ade, P. A. R. Aghanim, N. Alves, M. I. R. Armitage-Caplan, C., I Amaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Ausse, H. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Barrenass, R. Bartelmann, M. Bartlett, J. G. Bartolo, N. Basak, S. Battaner, E. Battye, R. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bertincourt, B. Bethermin, M. Bielewicz, P. Bikmaev, I. Blanchard, A. Bobin, J. Bock, J. J. Boehringer, H. Bonaldi, A. Bonavera, L. Bond, J. R. Borrill, J. Bouchet, F. R. Boulanger, F. Bourdin, H. Bowyer, J. W. Bridges, M. Brown, M. L. Bucher, M. Burenin, R. Burigana, C. Butler, R. C. Calabrese, E. Cappellini, B. Cardoso, J. -F. Carr, R. Carvalho, P. Casale, M. Castexl, G. Catalano, A. Challinor, A. Chamballu, A. Chary, R. -R. Chen, X. Chiang, H. C. Chiang, L. -Y Chon, G. Christensen, P. R. Churazov, E. Church, S. Clemens, M. Clements, D. L. Colombi, S. Colombo, L. P. L. Combet, C. Comis, B. Couchot, E. Coulais, A. Crill, B. P. Cruz, M. Curto, A. Cuttaia, F. Da Silva, A. Dahle, H. Danese, L. Davies, R. D. Davis, R. J. de Bernardis, P. de Rosa, A. de Zotti, G. Dechelette, T. Delabrouille, J. Delouis, J. -M. Democles, J. Desert, F. -X. Dick, J. Dickinson, C. Diego, J. M. Dolag, K. Dole, H. Donzelli, S. Dore, O. Douspis, M. Ducout, A. Dunkley, J. Dupac, X. Efstathiou, G. Elsner, F. Ensslin, T. A. Eriksen, H. K. Fabre, O. Falgarone, E. Falvella, M. C. Fantaye, Y. Fergusson, J., I Filliard, C. Finelli, F. Flores-Cacho, I. Foley, S. Forni, O. Fosalba, P. Frailis, M. Fraisse, A. A. Franceschi, E. Freschi, M. Fromenteau, S. Frommert, M. Gaier, T. C. Galeotta, S. Gallegos, J. Galli, S. Gandolfo, B. Ganga, K. Gauthier, C. Genova-Santos, R. T. Ghosh, T. Giard, M. Giardino, G. Gilfanov, M. Girard, D. Giraud-Heraud, Y. Gjerlow, E. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Gudmundsson, J. E. Haissinski, J. Hamann, J. Hansen, F. K. Hansen, M. Hanson, D. Harrison, D. L. Heavens, A. Helou, G. Hempel, A. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Ho, S. Hobson, M. Holmes, W. A. Hornstrup, A. Hou, Z. Hovest, W. Huey, G. Huffenberger, K. M. Hurier, G. Ilic, S. Jaffe, A. H. Jaffe, T. R. Jasches, J. Jewell, J. Jones, W. C. Juvela, M. Kalberla, P. Kangaslahti, P. Keihanen, E. Kerp, J. Keskitalo, R. Khamitov, I. Kiiveri, K. Kim, J. Kisnerl, T. S. Kneissl, R. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lacasa, E. Lagache, G. Lahteenmaki, A. Lamarre, J. -M. Langer, M. Lasenby, A. Lattanzi, M. Laureijs, R. J. Lavabre, A. Lawrence, C. R. Le Jeune, M. Leach, S. Leahy, J. P. Leonardi, R. Leon-Tavares, J. Leroy, C. Lesgourgues, J. Lewis, A. Li, C. Liddle, A. Liguori, M. Lilie, P. B. Linden-Vornle, M. Lindholm, V. Lopez-Caniego, M. Lowe, S. Lubin, P. M. Macias-Perez, J. F. MacTavish, C. J. Maffei, B. Maggio, G. Maino, D. Mandolesi, N. Mangilli, A. Marcos-Caballero, A. Marinucci, D. Maris, M. Marleau, F. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matsumura, T. Matthai, E. Maurin, L. Mazzotta, P. McDonald, A. McEwen, J. D. McGehee, P. Mei, S. Meinhold, P. R. Melchiorri, A. Melin, J. -B. Mendes, L. Menegoni, E. Mennella, A. Migliaccio, M. Mikkelsen, K. Millea, M. Miniscalco, R. Mitra, S. Miville-Deschenes, M. -A. Molinari, D. Moneti, A. Montier, L. Morgante, G. Morisset, N. Mortlock, D. Moss, A. Munshi, D. Murphy, J. A. Naselsky, P. Nati, E. Natoli, P. Negrello, M. Nesvadba, N. P. H. Netterfield, C. B. Norgaard-Nielsen, H. U. North, C. Noviello, F. Novikov, D. Novikov, I. O'Dwyer, I. J. Orieux, F. Osborne, S. O'Sullivan, C. Oxborrow, C. A. Paci, F. Pagano, L. Pajot, F. Paladini, R. Pandolfi, S. Paoletti, D. Partridge, B. Pasian, F. Patanchon, G. Paykari, P. Pearson, D. Pearson, T. J. Peel, M. Peiris, H. V. Perdereau, O. Perotto, L. Perrotta, F. Pettorino, V. Piacentini, F. Piat, M. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Platania, P. Pogosyan, D. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Pullen, A. R. Rachen, J. P. Racine, B. Rahlin, A. Raeth, C. Reach, W. T. Rebolo, R. Reinecke, M. Remazeilles, M. Renault, C. Renzi, A. Riazuelo, A. Ricciardi, S. Rillerl, T. Ringeval, C. Ristorcelli, I. Robbers, G. Rocha, G. Roman, M. Rosset, C. Rossetti, M. Roudier, G. Rowan-Robinson, M. Rubino-Martin, J. A. Ruiz-Granados, B. Rusholme, B. Salerno, E. Sandri, M. Sanselme, L. Santos, D. Savelainen, M. Savini, G. Schaefer, B. M. Schiavon, F. Scott, D. Seiffert, M. D. Serra, P. Shellard, E. P. S. Smith, K. Smoot, G. E. Souradeep, T. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sudiwala, R. Sunyaev, R. Sureau, F. Sutteer, P. Sutton, D. Suur-Uski, A-S. Sygnet, J. -E Tauber, J. A. Tavagnacco, D. Taylor, D. Terenzi, L. Texier, D. Toffolatti, L. Tomasi, M. Torre, J. -P. Tristram, M. Tucci, M. Tuovinen, J. Tuerler, M. Tuttlebee, M. Umana, G. Valenziano, L. Valiviita, J. Van Tent, B. Varisi, J. Vibert, L. Viel, M. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. Watson, C. Watson, R. Wehus, I. K. Welikala, N. Weller, J. White, M. White, S. D. M. Wilkinson, A. Winkel, B. Xia, J. -Q. Yvon, D. Zacchei, A. Zibin, J. P. Zonca, A. CA Planck Collaboration TI Planck 2013 results. I. Overview of products and scientific results SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE cosmology: observations; cosmic background radiation; space vehicles: instruments; instrumentation: detectors ID PROBE WMAP OBSERVATIONS; SOUTH-POLE TELESCOPE; GALAXY CLUSTER SURVEY; ATACAMA COSMOLOGY TELESCOPE; EXTRAGALACTIC POINT SOURCES; MICROWAVE BACKGROUND MAPS; HUBBLE-SPACE-TELESCOPE; IN-FLIGHT PERFORMANCE; PRE-LAUNCH STATUS; COMPONENT SEPARATION AB The European Space Agency's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14 May 2009 and has been scanning the microwave and submillimetre sky continuously since 12 August 2009. In March 2013, ESA and the Planck Collaboration released the initial cosmology products based on the first 15.5 months of Planck data, along with a set of scientific and technical papers and a web-based explanatory supplement. This paper gives an overview of the mission and its performance, the processing, analysis, and characteristics of the data, the scientific results, and the science data products and papers in the release. The science products include maps of the cosmic microwave background (CMB) and diffuse extragalactic foregrounds, a catalogue of compact Galactic and extragalactic sources, and a list of sources detected through the Sunyaev-Zeldovich effect. The likelihood code used to assess cosmological models against the Planck data and a lensing likelihood are described. Scientific results include robust support for the standard six-parameter Lambda CDM model of cosmology and improved measurements of its parameters, including a highly significant deviation from scale invariance of the primordial power spectrum. The Planck values for these parameters and others derived from them are significantly different from those previously determined. Several large-scale anomalies in the temperature distribution of the CMB, first detected by WMAP, are confirmed with higher confidence. Planck sets new limits on the number and mass of neutrinos, and has measured gravitational lensing of CMB anisotropies at greater than 25 sigma. Planck finds no evidence for non-Gaussianity in the CMB. Planck's results agree well with results from the measurements of baryon acoustic oscillations. Planck finds a lower Hubble constant than found in some more local measures. Some tension is also present between the amplitude of matter fluctuations (sigma(8)) derived from CMB data and that derived from Sunyaev-Zeldovich data. The Planck and WMAP power spectra are off set from each other by an average level of about 2% around the first acoustic peak. Analysis of Planck polarization data is not yet mature, therefore polarization results are not released, although the robust detection of E-mode polarization around CMB hot and cold spots is shown graphically. C1 [Bartlett, J. G.; Bucher, M.; Cardoso, J. -F.; Castexl, G.; Delabrouille, J.; Fromenteau, S.; Ganga, K.; Gauthier, C.; Giraud-Heraud, Y.; Le Jeune, M.; Maurin, L.; Patanchon, G.; Piat, M.; Racine, B.; Remazeilles, M.; Roman, M.; Rosset, C.; Roudier, G.; Smoot, G. E.; Stompor, R.; Welikala, N.] Univ Paris Diderot, Observ Paris, Sorbonne Paris Cite, CNRS IN2P3,CEA lrfu,APC, F-75205 Paris 13, France. 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EM jtauber@cosmos.esa.int RI Butler, Reginald/N-4647-2015; Barreiro, Rita Belen/N-5442-2014; Remazeilles, Mathieu/N-1793-2015; Renzi, Alessandro/K-4114-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; bonavera, laura/E-9368-2017; SERRA, PAOLO/G-9678-2014; White, Martin/I-3880-2015; Pearson, Timothy/N-2376-2015; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Valiviita, Jussi/A-9058-2016; Mazzotta, Pasquale/B-1225-2016; Kurki-Suonio, Hannu/B-8502-2016; Ghosh, Tuhin/E-6899-2016; Tomasi, Maurizio/I-1234-2016; Lattanzi, Massimiliano/D-8120-2011; Fosalba Vela, Pablo/I-5515-2016; Novikov, Igor/N-5098-2015; Lahteenmaki, Anne/L-5987-2013; Salerno, Emanuele/A-2137-2010; Churazov, Eugene/A-7783-2013; Herranz, Diego/K-9143-2014; Toffolatti, Luigi/K-5070-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Pullen, Anthony/I-7007-2015; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Ruiz-Granados, Beatriz/K-2798-2014; Cruz, Marcos/N-3429-2014; Langer, Mathieu/C-5100-2013; Martinez-Gonzalez, Enrique/E-9534-2015; OI Reach, William/0000-0001-8362-4094; Hurier, Guillaume/0000-0002-1215-0706; Molinari, Diego/0000-0002-7799-3915; Zacchei, Andrea/0000-0003-0396-1192; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Butler, Reginald/0000-0003-4366-5996; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Matarrese, Sabino/0000-0002-2573-1243; Viel, Matteo/0000-0002-2642-5707; Galeotta, Samuele/0000-0002-3748-5115; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Umana, Grazia/0000-0002-6972-8388; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Weller, Jochen/0000-0002-8282-2010; Lopez-Caniego, Marcos/0000-0003-1016-9283; Peel, Mike/0000-0003-3412-2586; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Maris, Michele/0000-0001-9442-2754; Renzi, Alessandro/0000-0001-9856-1970; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Pierpaoli, Elena/0000-0002-7957-8993; Watson, Robert/0000-0002-5873-0124; Juvela, Mika/0000-0002-5809-4834; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; bonavera, laura/0000-0001-8039-3876; SERRA, PAOLO/0000-0002-7609-3931; Rubino-Martin, Jose Alberto/0000-0001-5289-3021; De Zotti, Gianfranco/0000-0003-2868-2595; Masi, Silvia/0000-0001-5105-1439; White, Martin/0000-0001-9912-5070; Pearson, Timothy/0000-0001-5213-6231; Gruppuso, Alessandro/0000-0001-9272-5292; Valiviita, Jussi/0000-0001-6225-3693; Mazzotta, Pasquale/0000-0002-5411-1748; Kurki-Suonio, Hannu/0000-0002-4618-3063; Tomasi, Maurizio/0000-0002-1448-6131; Lattanzi, Massimiliano/0000-0003-1059-2532; Salerno, Emanuele/0000-0002-3433-3634; Herranz, Diego/0000-0003-4540-1417; Toffolatti, Luigi/0000-0003-2645-7386; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Pullen, Anthony/0000-0002-2091-8738; Vielva, Patricio/0000-0003-0051-272X; Cruz, Marcos/0000-0002-4767-530X; Langer, Mathieu/0000-0002-9088-2718; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Ricciardi, Sara/0000-0002-3807-4043; Villa, Fabrizio/0000-0003-1798-861X; Bethermin, Matthieu/0000-0002-3915-2015; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Savini, Giorgio/0000-0003-4449-9416 FU CNES; CNRS/INSU-IN2P3; ASI; Danish Natural Research Council; ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR (Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC (Spain); MICINN (Spain); JA (Spain); Tekes (Finland); AoF (Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); PRADE (EU) FX Planck is too large a project to allow full acknowledge of all contributions by individuals, institutions, industries, and funding agencies. The main entities involved in the mission operations are as follows. The European Space Agency operates the satellite via its Mission Operations Centre located at ESOC (Darmstadt, Germany) and coordinates scientific operations via the Planck Science Office located at ESAC (Madrid, Spain). Two Consortia, comprising around 100 scientific institutes within Europe, the USA, and Canada, and funded by agencies from the participating countries, developed the scientific instruments LFI and HFI, and continue to operate them via instrument Operations Teams located in Trieste (Italy) and Orsay (France). The Consortia are also responsible for scientific processing of the acquired data. The Consortia are led by the Principal Investigators: J.-L. Puget in France for HFI (funded principally by CNES and CNRS/INSU-IN2P3) and N. Mandolesi in Italy for LFI (funded principally via ASI). NASA's UK Planck Project, based at JPL and involving scientists at many UK institutions, contributes significantly to the efforts of these two Consortia. A third Consortium, led by H. U. Norgaard and Nielsen and supported by the Danish Natural Research Council, contributed to the reflector programme. The author list for this paper has been selected by the Planck Science Team from the Planck Collaboration, and is composed of individuals from all of the above entities who have made multi-year contributions to the development of the mission. It does not pretend to be inclusive of all contributions to Planck. A description of the Planck Collaboration and a list of its members indicating which technical or scientific activities they have been involved in, can be found at (http://www.rssd.esa.int/index.php?project=PLANCK&page=Planck_Collaborat ion). The Planck Collaboration acknowledges the support of: ESA; CNES, and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, and JA (Spain); Tekes, AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRADE (EU). NR 134 TC 4000 Z9 4005 U1 36 U2 116 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A1 DI 10.1051/0004-6361/201321529 PG 48 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600007 ER PT J AU Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Battaner, E Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bonaldi, A Bonavera, L Bond, JR Borrill, J Bouchet, FR Bridges, M Bucher, M Burigana, C Butler, RC Cardoso, JF Catalano, A Chamballu, A Chiang, LY Cristensen, PR Church, S Olombi, SC Colombo, LPL Crill, BP Cruz, M Curto, A Cuttaia, F Danese, L Davies, RD Davis, RJ de Bernardis, P de Rose, A de Zotti, G Delabrouillei, J Dick, J Dickinson, C Diego, JM Dole, H Donzeli, S Dore, O Douspis, M Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Finelli, F Forni, O Frailis, M Franceschi, E Gaier, TC Galeotta, S Ganga, K Giard, M Giraud-Heraud, Y Gjerlow, E Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Hansen, FK Hanson, D Harrison, D Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Jaffe, AH Jaffe, TR Jewell, J Jones, WC Juvela, M Kaneaslahti, P Keihanen, E Keskitalo, R Kuveri, K Kisner, TS Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lahteenmaki, A Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Leahy, JP Leonardi, R Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lindholm, V Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maino, D Mandolesi, N Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Mazzotta, P Meinhold, PR Melchiorri, A Mendes, L Mennella, A Mieliaccio, M Mitra, S Moneti, A Montier, L Morgante, G Mortlock, D Moss, A Munshi, D Naselsky, P Natoli, P Netterfield, CB Norgaard-Nielsen, HU Novikov, D Novikov, I O'Dwyer, IJ Osborne, S Paci, F Pagano, L Paladini, R Paoletti, D Partridge, B Pasian, F Patanchon, G Pearson, D Peel, M Perdereau, O Perotto, L Perrotta, F Pierpaoli, E Pietrobon, D Plaszczynski, S Platania, P Pointecouteau, E Polenta, G Ponthieu, N Popa, I Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Rebolo, R Reinecke, M Remazeilles, M Ricciardi, S Riller, T Rocha, G Rosset, C Rossetti, M Roudier, G Rubino-Martin, JA Rusholme, B Sandri, M Salltos, D Scott, A Seitiert, MA Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Stueau, F Sutton, D Sum-Uski, AS Sygnet, JF Tauber, JA Tavaenacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Tuovinen, J Turler, M Umana, G Valenziano, L Vaiiviita, J Van Tent, B Varis, J Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD Watson, R Wilkinson, A Yvon, D Zacchei, A Zonca, A AF Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Battaner, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bonaldi, A. Bonavera, L. Bond, J. R. Borrill, J. Bouchet, F. R. Bridges, M. Bucher, M. Burigana, C. Butler, R. C. Cardoso, J. -F. Catalano, A. Chamballu, A. Chiang, L. -Y Cristensen, P. R. Church, S. Olombi, S. C. Colombo, L. P. L. Crill, B. P. Cruz, M. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. Davis, R. J. de Bernardis, P. de Rose, A. de Zotti, G. Delabrouillei, J. Dick, J. Dickinson, C. Diego, J. M. Dole, H. Donzeli, S. Dore, O. Douspis, M. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Finelli, F. Forni, O. Frailis, M. Franceschi, E. Gaier, T. C. Galeotta, S. Ganga, K. Giard, M. Giraud-Heraud, Y. Gjerlow, E. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Hansen, F. K. Hanson, D. Harrison, D. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Jaffe, A. H. Jaffe, T. R. Jewell, J. Jones, W. C. Juvela, M. Kaneaslahti, P. Keihanen, E. Keskitalo, R. Kuveri, K. Kisner, T. S. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Lahteenmaki, A. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leahy, J. P. Leonardi, R. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lindholm, V. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maino, D. Mandolesi, N. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. Meinhold, P. R. Melchiorri, A. Mendes, L. Mennella, A. Mieliaccio, M. Mitra, S. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Moss, A. Munshi, D. Naselsky, P. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Novikov, D. Novikov, I. O'Dwyer, I. J. Osborne, S. Paci, F. Pagano, L. Paladini, R. Paoletti, D. Partridge, B. Pasian, F. Patanchon, G. Pearson, D. Peel, M. Perdereau, O. Perotto, L. Perrotta, F. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Platania, P. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, I. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Rebolo, R. Reinecke, M. Remazeilles, M. Ricciardi, S. Riller, T. Rocha, G. Rosset, C. Rossetti, M. Roudier, G. Rubino-Martin, J. A. Rusholme, B. Sandri, M. Salltos, D. Scott, D. Seitiert, M. A. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Stueau, F. Sutton, D. Sum-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavaenacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Tuovinen, J. Turler, M. Umana, G. Valenziano, L. Vaiiviita, J. Van Tent, B. Varis, J. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. Watson, R. Wilkinson, A. Yvon, D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. III. LFI systematic uncertainties SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE cosmic background radiation; cosmology: observations; methods: data analysis ID PERFORMANCE; RADIOMETERS; MAPS; SKY AB We present the current estimate of instrumental and systematic effect uncertainties for the Planck-Low Frequency Instrument relevant to the first release of the Planck cosmological results. We give an overview of the main effects and of the tools and methods applied to assess residuals in maps and power spectra. We also present an overall budget of known systematic effect uncertainties, which are dominated by sidelobe straylight pick-up and imperfect calibration. However, even these two effects are at least two orders of magnitude weaker than the cosmic microwave background fluctuations as measured in terms of the angular temperature power spectrum. A residual signal above the noise level is present in the multipole range l < 20, most notably at 30GHz, and is probably caused by residual Galactic straylight contamination. Current analysis aims to further reduce the level of spurious signals in the data and to improve the systematic effects modelling, in particular with respect to straylight and calibration uncertainties. C1 [Bucher, M.; Cardoso, J. -F.; Delabrouillei, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, Sorbonne Paris Cite, CNRS, IN2P3,CEA Irfu,Observ Paris,APC, F-75205 Paris 13, France. [Lahteenmaki, A.; Poutanen, T.] Aalto Univ Metsahovi Radio Observ, Kylmala 02540, Finland. [Kunz, M.] African Inst Math Sci, ZA-7701 Rondebosch Cape Town, South Africa. [Natoli, P.; Polenta, G.] Aeenzia Spaziale Italiana, Sci Data Ctr, I-00133 Rome, Italy. [Mandolesi, N.] Agenzia Spaziale ilaliana, I-00198 Rome, Italy. [Ashdown, M.; Bridges, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 0HE, England. [Bond, J. R.; Hanson, D.; Martin, P. G.] Univ Toronto, CITA, Toronto, ON M5S 3H8, Canada. [Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.] CNRS, IRAP, F-4 Toulouse 4, France. [Bock, J. J.; Dore, O.; Hildebrandt, S. R.; Prezeau, G.; Rocha, G.; Seitiert, M. A.] CALTECH, Pasadena, CA 91125 USA. [Shellard, E. P. S.] Univ Cambridge, Ctr Theoret Cosmol, DAMTP, Cambridge CB3 0WA, England. [Hernandez-Monteagudo, C.] CEFCA, Teruel 44001, Spain. [Borrill, J.; Keskitalo, R.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 94720 USA. [Rebolo, R.] CSIC, E-28006 Madrid, Spain. [Chamballu, A.; Yvon, D.] CEA Saclay, DSM Irfu SPP, F-91191 Gif Sur Yvette, France. [Hornstrup, A.; Linden-Vornle, M.; Norgaard-Nielsen, H. U.] Tech Univ Denmark, Natl Space Inst, DTU Space, DK-2800 Lyngby, Denmark. [Kunz, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, CH-1211 Geneva 4, Switzerland. [Atrio-Barandela, F.] Univ Salamanca, Fac Ciencias, Dept Fis Fundamental, E-37008 Salamanca, Spain. [Toffolatti, L.] Univ Oviedo, Dept Fis, Oviedo 33007, Spain. [Cruz, M.] Univ Cantabria, Dept Matemat Estadist & Computac, E-39005 Santander, Spain. [Netterfield, C. B.] Univ Toronto, Dept Astron & Astrophys, Toronto, ON, Canada. [Rachen, J. P.] Radboud Univ Nijmegen, IMAPP, Dept Astrophys, NL-6500 GL Nijmegen, Netherlands. [Keskitalo, R.] Univ Calif Berkeley, Dept Elect Engn & Comp Sci, Berkeley, CA 94720 USA. [Scott, D.] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V5Z 1M9, Canada. [Colombo, L. P. L.; Pierpaoli, E.] Univ So Calif, Dana & David Dornsife Coll Letter Arts & Sci, Dept Phys & Astron, Los Angeles, CA 90089 USA. [Benoit-Levy, A.] UCL, Dept Phys & Astron, London WC1E 6BT, England. [Huffenberger, K. M.] Florida State Univ, Dept Phys, Tallahassee, FL USA. [Juvela, M.; Keihanen, E.; Kuveri, K.; Kurki-Suonio, H.; Lindholm, V.; Poutanen, T.; Sum-Uski, A. -S.; Vaiiviita, J.] Univ Helsinki, Dept Phys, FIN-00014 Helsinki, Finland. [Jones, W. C.] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA. [Knox, L.] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA. [Lubin, P. M.; Meinhold, P. R.; Zonca, A.] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA. [Wandelt, B. D.] Univ Illinois, Dept Phys, Urbana, IL USA. [Liguori, M.; Matarrese, S.] Univ Padua, Dipartimento Fis & Astron G Galilei, I-35131 Padua, Italy. [Burigana, C.; Mandolesi, N.; Natoli, P.] Univ Ferrara, Dipartimento Fis & Sci Terra, I-44122 Ferrara, Italy. [de Bernardis, P.; Masi, S.; Melchiorri, A.; Pagano, L.] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy. [Benoit, A.; Bersanelli, M.; Maino, D.; Mennella, A.; Rossetti, M.] Univ Milan, Dipartimento Fis, I-20133 Milan, Italy. [Gregorio, A.; Tavaenacco, D.] Univ Trieste, Dipartmento Fis, I-34127 Trieste, Italy. [Mazzotta, P.; Vittorio, N.] Univ Roma Tor Vergata, Dipartimento Fis, I-00133 Rome, Italy. [Cristensen, P. R.; Naselsky, P.] Niels Bohr Inst, Discovery Ctr, DK-2100 Copenhagen, Denmark. [Rebolo, R.; Rubino-Martin, J. A.] Univ La Laguna, Dpto Astrofis, E-38206 Tenerife, Spain. [Dupac, X.; Leonardi, R.; Mendes, L.] European Space Agcy, ESAC, Planck Sci Off, Madrid, Spain. [Laureijs, R. J.; Tauber, J. A.] European Space Agcy, Estec, NL-2201 AZ Noordwijk, Netherlands. [Partridge, B.] Haverford Coll, Dept Astron, Haverford, PA 19041 USA. [Kuveri, K.; Kurki-Suonio, H.; Lahteenmaki, A.; Lindholm, V.; Poutanen, T.; Sum-Uski, A. -S.; Vaiiviita, J.] Univ Helsinki, Helsinki Inst Phys, FIN-00014 Helsinki, Finland. [Umana, G.] Osserv Astrofis Catania, INAF, I-95123 Catania, Italy. [Benoit, A.; de Zotti, G.] Osserv Astron Padova, INAF, I-35122 Padua, Italy. [Polenta, G.] Osserv Astron Roma, INAF, I-00040 Monte Porzio Catone, Italy. [Frailis, M.; Galeotta, S.; Gregorio, A.; Maris, M.; Pasian, F.; Tavaenacco, D.; Zacchei, A.] Osserv Astron Trieste, INAF, I-34131 Trieste, Italy. [Massardi, M.] Ist Radioastron, INAF, I-40129 Bologna, Italy. [Burigana, C.; Butler, R. C.; Cuttaia, F.; de Rose, A.; Finelli, F.; Franceschi, E.; Gruppuso, A.; Mandolesi, N.; Morgante, G.; Natoli, P.; Paoletti, D.; Ricciardi, S.; Sandri, M.; Terenzi, L.; Valenziano, L.; Villa, F.] IASF Bologna, INAF, I-40129 Bologna, Italy. [Bersanelli, M.; Donzeli, S.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] IASF Bologna, INAF, I-40129 Milan, Italy. [Finelli, F.; Paoletti, D.] Ist Nazl Fis Nucl, Sez Bologna, I-40126 Bologna, Italy. [Melchiorri, A.; Pagano, L.] Univ Roma La Sapienza, Ist Nazl Fis Nucl, Sez Roma 1, I-00185 Rome, Italy. [Ponthieu, N.] Univ Grenoble 1, CNRS, INSU, IPAG,UMR 5274, F-38041 Grenoble, France. 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[Cardoso, J. -F.] CNRS, Lab Traitement & Commun Informat, UMR 5141, F-75634 Paris 13, France. [Cardoso, J. -F.] Telecom ParisTech, F-75634 Paris 13, France. [Catalano, A.; Macias-Perez, J. F.; Perotto, L.; Salltos, D.] Univ Grenoble 1, CNRS, IN2P3, Inst Natl Polytech Grenoble,Lab Phys Subatom & Co, F-38026 Grenoble, France. [Van Tent, B.] Univ Paris 11, Phys Theor Lab, F-91405 Orsay, France. [Van Tent, B.] CNRS, F-91405 Orsay, France. [Kisner, T. S.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Ensslin, T. A.; Hernandez-Monteagudo, C.; Hovest, W.; Knoche, J.; Matthai, F.; Rachen, J. P.; Reinecke, M.; Riller, T.] Max Planck Inst Astrophys, D-85741 Garching, Germany. [Hanson, D.] McGill Univ, McGill Phys, Montreal, PQ H3A 2T8, Canada. [Tuovinen, J.; Varis, J.] VTT Tech Res Ctr Finland, MilliLab, 02044 Espoo, Finland. [Cristensen, P. R.; Naselsky, P.; Novikov, I.] Niels Bohr Inst, DK-2100 Copenhagen, Denmark. [Crill, B. P.] CALTECH, Pasadena, CA 91125 USA. [Lesgourgues, J.] Ecole Polytech Fed Lausanne, SB ITP LPPC, CH-1015 Lausanne, Switzerland. [Baccigalupi, C.; Bielewicz, P.; Danese, L.; de Zotti, G.; Dick, J.; Gonzalez-Nuevo, J.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sect, I-34136 Trieste, Italy. [Munshi, D.; Spencer, L. D.] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales. [Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England. [Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA. [Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Karachai Cherkessian Rep 369167, Zelenchukskiy R, Russia. [Church, S.; Osborne, S.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA. [Armitage-Caplan, C.] Univ Oxford, Sub Dept Astrophys, Oxford OX1 3RH, England. [Lesgourgues, J.] CERN, PH TH, Div Theory, CH-1211 Geneva 23, Switzerland. [Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Olombi, S. C.; Hivon, E.; Prunet, S.; Wandelt, B. D.] Univ Paris 06, UMR7095, F-75014 Paris, France. [Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.] Univ Toulouse, UPS, OMP, IRAP, F-31028 Toulouse 4, France. [Battaner, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, E-18071 Granada, Spain. [Gorski, K. M.] Univ Warsaw Observ, PL-00478 Warsaw, Poland. RP Mennella, A (reprint author), Univ Milan, Dipartimento Fis, Via Celoria 16, I-20133 Milan, Italy. EM aniello.mennella@fisica.unimi.it RI Butler, Reginald/N-4647-2015; Barreiro, Rita Belen/N-5442-2014; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; bonavera, laura/E-9368-2017; Remazeilles, Mathieu/N-1793-2015; Kurki-Suonio, Hannu/B-8502-2016; Tomasi, Maurizio/I-1234-2016; Lahteenmaki, Anne/L-5987-2013; Toffolatti, Luigi/K-5070-2014; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Cruz, Marcos/N-3429-2014; Martinez-Gonzalez, Enrique/E-9534-2015; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Mazzotta, Pasquale/B-1225-2016; OI Umana, Grazia/0000-0002-6972-8388; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Lopez-Caniego, Marcos/0000-0003-1016-9283; Peel, Mike/0000-0003-3412-2586; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Butler, Reginald/0000-0003-4366-5996; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Galeotta, Samuele/0000-0002-3748-5115; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Colombo, Loris/0000-0003-4572-7732; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; bonavera, laura/0000-0001-8039-3876; Rubino-Martin, Jose Alberto/0000-0001-5289-3021; De Zotti, Gianfranco/0000-0003-2868-2595; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Paoletti, Daniela/0000-0003-4761-6147; Pierpaoli, Elena/0000-0002-7957-8993; Watson, Robert/0000-0002-5873-0124; Juvela, Mika/0000-0002-5809-4834; Kurki-Suonio, Hannu/0000-0002-4618-3063; Tomasi, Maurizio/0000-0002-1448-6131; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; Cruz, Marcos/0000-0002-4767-530X; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Gruppuso, Alessandro/0000-0001-9272-5292; Mazzotta, Pasquale/0000-0002-5411-1748; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; Valiviita, Jussi/0000-0001-6225-3693; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Ricciardi, Sara/0000-0002-3807-4043; Villa, Fabrizio/0000-0003-1798-861X NR 56 TC 35 Z9 34 U1 2 U2 4 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A3 DI 10.1051/0004-6361/201321574 PG 23 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600024 ER PT J AU Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Bartlett, JG Benabed, K Benoit-Ley, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bond, JR Borrill, J Bouchet, FR Bridges, M Burigana, C Butler, RC Cardoso, JF Catalano, A Challinor, A Chamballu, A Chiang, HC Chiang, LY Christensen, PR Clements, DL Colombo, LPL Couchot, F Crill, BP Curto, A Cuttaia, F Danese, L Davies, RD Davis, RJ de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Diego, JM Donzelli, S Dore, O Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Finelli, F Forni, O Frailis, M Franceschi, E Galeotta, S Ganga, K Giard, M Giardino, G Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Hansen, FK Hanson, D Harrison, DL Helou, G Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hovest, W Huffenberger, KM Jones, WC Juvela, M Keihanen, E Keskitalo, R Kisner, TS Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lahteenmaki, A Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Leonardi, R Lewis, A Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Mandolesi, N Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Mazzotta, P Meinhold, PR Melchiorri, A Mendes, L Migliaccio, M Mitra, S Moneti, A Montier, L Morgante, G Mortlock, D Moss, A Munshi, D Naselsky, P Nati, F Natoli, P Norgaard-Nielsen, HU Noviello, F Novikov, D Novikov, I Osborne, S Oxborrow, CA Pagano, L Pajot, F Paoletti, D Pasian, F Patanchon, G Perdereau, O Perrotta, F Piacentini, F Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Popa, L Pratt, GW Prezeau, G Puget, JL Rachen, JP Reach, WT Reinecke, M Ricciardi, S Riller, T Ristorcelli, I Rocha, G Rosset, C Rubino-Martin, JA Rusholme, B Santos, D Savini, G Scott, D Seiffert, MD Shellard, EPS Spencer, LD Sunyaev, R Sureau, F Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Turler, M Valenziano, L Valiviita, J Van Tent, B Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD White, M Yvon, D Zacchei, A Zibin, JP Zonca, A AF Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Bartlett, J. G. Benabed, K. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bond, J. R. Borrill, J. Bouchet, F. R. Bridges, M. Burigana, C. Butler, R. C. Cardoso, J. -F. Catalano, A. Challinor, A. Chamballu, A. Chiang, H. C. Chiang, L. -Y Christensen, P. R. Clements, D. L. Colombo, L. P. L. Couchot, F. Crill, B. P. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. Davis, R. J. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Diego, J. M. Donzelli, S. Dore, O. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Finelli, F. Forni, O. Frailis, M. Franceschi, E. Galeotta, S. Ganga, K. Giard, M. Giardino, G. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Hansen, F. K. Hanson, D. Harrison, D. L. Helou, G. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hovest, W. Huffenberger, K. M. Jones, W. C. Juvela, M. Keihanen, E. Keskitalo, R. Kisner, T. S. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lahteenmaki, A. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leonardi, R. Lewis, A. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Mandolesi, N. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Mazzotta, P. Meinhold, P. R. Melchiorri, A. Mendes, L. Migliaccio, M. Mitra, S. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Moss, A. Munshi, D. Naselsky, P. Nati, F. Natoli, P. Norgaard-Nielsen, H. U. Noviello, F. Novikov, D. Novikov, I. Osborne, S. Oxborrow, C. A. Pagano, L. Pajot, F. Paoletti, D. Pasian, F. Patanchon, G. Perdereau, O. Perrotta, F. Piacentini, F. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Pratt, G. W. Prezeau, G. Puget, J. -L. Rachen, J. P. Reach, W. T. Reinecke, M. Ricciardi, S. Riller, T. Ristorcelli, I. Rocha, G. Rosset, C. Rubino-Martin, J. A. Rusholme, B. Santos, D. Savini, G. Scott, D. Seiffert, M. D. Shellard, E. P. S. Spencer, L. D. Sunyaev, R. Sureau, F. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Tuerler, M. Valenziano, L. Valiviita, J. Van Tent, B. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. White, M. Yvon, D. Zacchei, A. Zibin, J. P. Zonca, A. CA Planck Collaboration TI Planck 2013 results. XXVII. Doppler boosting of the CMB: Eppur si muove SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE cosmology: observations; cosmic background radiation; reference systems; relativistic processes ID SKY MAPS; MICROWAVE; ABERRATION; DIPOLE; ANISOTROPY AB Our velocity relative to the rest frame of the cosmic microwave background (CMB) generates a dipole temperature anisotropy on the sky which has been well measured for more than 30 years, and has an accepted amplitude of v/c = 1 x 23(-10), or v = 369 km s(-1). In addition to this signal generated by Doppler boosting of the CMB monopole, our motion also modulates and aberrates the CMB temperature fluctuations (as well as every other source of radiation at cosmological distances). This is an order 10 3 e ff ect applied to fluctuations which are already one part in roughly 105, so it is quite small. Nevertheless, it becomes detectable with the all- sky coverage, high angular resolution, and low noise levels of the Planck satellite. Here we report a first measurement of this velocity signature using the aberration and modulation e ff ects on the CMB temperature anisotropies, finding a component in the known dipole direction, (l; b) = (264 ffi; 48 ffi), of 384 km s 1 +/- 78 km s 1 (stat :) +/- 115 km s 1 (syst :). This is a significant confirmation of the expected velocity. C1 [Bartlett, J. G.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Patanchon, G.; Rosset, C.] Univ Paris Diderot, Observ Paris, Sorbonne Paris Cite, CNRS IN2P3,CEA Irfu,APC, F-75205 Paris 13, France. [Lahteenmaki, A.] Aalto Univ, Metsahovi Radio Observ, Aalto 00076, Finland. [Lahteenmaki, A.] Dept Radio Sci & Engn, Aalto 00076, Finland. [Kunz, M.] African Inst Math Sci, ZA-7945 Cape Town, South Africa. [Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana, Sci Data Ctr, I-00133 Rome, Italy. [Mandolesi, N.] Agenzia Spaziale Italiana, I-00198 Rome, Italy. [Ashdown, M.; Bridges, M.; Curto, A.; Hobson, M.; Lasenby, A.] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 0HE, England. [Chiang, H. C.] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, ZA-4000 Durban, South Africa. [Bond, J. R.; Hanson, D.; Martin, P. G.] Univ Toronto, CITA, University Toronto, ON M5S 3H8, Canada. [Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] CNRS, IRAP, F-31028 Toulouse 4, France. [Bock, J. J.; Helou, G.; Hildebrandt, S. R.; Prezeau, G.; Rocha, G.; Seiffert, M. D.] CALTECH, Pasadena, CA 91125 USA. [Challinor, A.; Shellard, E. P. S.] Univ Cambridge, DAMTP, Ctr Theoret Cosmol, Cambridge CB3 0WA, England. [Borrill, J.; Keskitalo, R.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 94720 USA. [Chamballu, A.; Yvon, D.] CEA Saclay, DSM Irfu SPP, F-91191 Gif Sur Yvette, France. [Linden-Vornle, M.; Norgaard-Nielsen, H. U.; Oxborrow, C. A.] Tech Univ Denmark, Natl Space Inst, DTU Space, DK-2800 Lyngby, Denmark. [Kunz, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, CH-1211 Geneva 4, Switzerland. [Atrio-Barandela, F.] Univ Salamanca, Fac Ciencias, Dept Fis Fundamental, E-37008 Salamanca, Spain. [Toffolatti, L.] Univ Oviedo, Dept Fis, E-33007 Oviedo, Spain. [Rachen, J. P.] Radboud Univ Nijmegen, Dept Astrophys, IMAPP, NL-6500 GL Nijmegen, Netherlands. [Keskitalo, R.] Univ Calif Berkeley, Dept Elect Engn & Comp Sci, Berkeley, CA 94720 USA. [Scott, D.; Zibin, J. P.] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V5Z 1M9, Canada. [Colombo, L. P. L.; Pierpaoli, E.] Univ So Calif, Dept Phys & Astron, Dana & David Dornsife Coll Letter Arts & Sci, Los Angeles, CA 90089 USA. [Benoit-Levy, A.] UCL, Dept Phys & Astron, London WC1E 6BT, England. [Lewis, A.] Univ Sussex, Dept Phys & Astron, Brighton BN1 9QH, E Sussex, England. [Huffenberger, K. M.] Florida State Univ, Dept Phys, Tallahassee, FL 32306 USA. [Juvela, M.; Keihanen, E.; Kurki-Suonio, H.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Dept Phys, FIN-00014 Helsinki, Finland. [Chiang, H. C.; Jones, W. C.] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA. [White, M.] Univ Calif Berkeley, Dept Phys, Berkeley, CA USA. [Knox, L.] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA. [Lubin, P. M.; Meinhold, P. R.; Zonca, A.] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA. [Wandelt, B. D.] Univ Illinois, Dept Phys, Urbana, IL USA. [Liguori, M.; Matarrese, S.] Univ Padua, Dipartimento Fis & Astron G Galilei, I-35131 Padua, Italy. [Burigana, C.; Mandolesi, N.; Natoli, P.] Univ Ferrara, Dipartimento Fis & Sci Terra, I-44122 Ferrara, Italy. [de Bernardis, P.; Masi, S.; Melchiorri, A.; Nati, F.; Pagano, L.; Piacentini, F.] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy. [Bersanelli, M.; Tomasi, M.] Univ Milan, Dipartimento Fis, I-20133 Milan, Italy. [Gregorio, A.; Tavagnacco, D.] Univ Trieste, Dipartmento Fis, I-34127 Trieste, Italy. [Mazzotta, P.; Vittorio, N.] Univ Roma Tor Vergata, Dipartmento Fis, I-00133 Rome, Italy. [Christensen, P. R.; Naselsky, P.] Niels Bohr Inst, Discovery Ctr, DK-2100 Copenhagen, Denmark. [Rubino-Martin, J. A.] Univ La Laguna, Dept Astrofis, Tenerife 38206, Spain. [Dupac, X.; Leonardi, R.; Mendes, L.] European Space Agcy, ESAC, Planck Sci Off, Madrid 28692, Spain. [Giardino, G.; Laureijs, R. J.; Tauber, J. A.] European Space Agcy, Estec, NL-2201 AZ Noordwijk, Netherlands. [Kurki-Suonio, H.; Lahteenmaki, A.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Helsinki Inst Phys, FIN-00014 Helsinki, Finland. [de Zotti, G.] Osserv Astron Padova, INAF, I-35122 Padua, Italy. [Polenta, G.] Osserv Astron Roma, INAF, I-00040 Monte Porzio Catone, Italy. [Frailis, M.; Galeotta, S.; Gregorio, A.; Maris, M.; Pasian, F.; Tavagnacco, D.; Zacchei, A.] Osserv Astron Trieste, INAF, I-34143 Trieste, Italy. [Massardi, M.] INAF Ist Radioastron, I-40129 Bologna, Italy. [Burigana, C.; Butler, R. C.; Cuttaia, F.; de Rosa, A.; Finelli, F.; Franceschi, E.; Gruppuso, A.; Mandolesi, N.; Morgante, G.; Natoli, P.; Paoletti, D.; Ricciardi, S.; Terenzi, L.; Valenziano, L.; Villa, F.] INAF IASF Bologna, I-20133 Bologna, Italy. [Bersanelli, M.; Donzelli, S.; Tomasi, M.] INAF IASF Milano, Milan, Italy. [Finelli, F.; Paoletti, D.] Ist Nazl Fis Nucl, Sez Bologna, I-40126 Bologna, Italy. [Melchiorri, A.; Pagano, L.] Univ Roma La Sapienza, Sez Roma 1, Ist Nazl Fis Nucl, I-00185 Rome, Italy. [Gregorio, A.] Ist Nazl Fis Nucl, I-34127 Trieste, Italy. [Ponthieu, N.] Univ Grenoble 1, CNRS INSU, Inst Planetol & Astrophys Grenoble, UMR 5274, F-38041 Grenoble, France. [Tuerler, M.] Univ Geneva, ISDC Data Ctr Astrophys, CH-1290 Sauverny, Switzerland. [Mitra, S.] IUCAA, Pune 411007, Maharashtra, India. [Clements, D. L.; Mortlock, D.; Novikov, D.] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Astrophys Grp, London SW7 2AZ, England. [Rusholme, B.] CALTECH, Ctr Infrared Proc & Anal, Pasadena, CA 91125 USA. [Aghanim, N.; Aumont, J.; Chamballu, A.; Kunz, M.; Pajot, F.; Ponthieu, N.; Puget, J. -L.] Univ Paris 11, Inst Astrophys Spatiale, CNRS, UMR 8617, F-91405 Orsay, France. [Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Cardoso, J. -F.; Hivon, E.; Moneti, A.; Sygnet, J. -F.; Wandelt, B. D.] CNRS, Inst Astrophys Paris, UMR 7095, F-75014 Paris, France. [Popa, L.] Inst Space Sci, Bucharest 077125, Romania. [Chiang, L. -Y] Acad Sinica, Inst Astron & Astrophys, Taipei 10617, Taiwan. [Bridges, M.; Challinor, A.; Efstathiou, G.; Gratton, S.; Harrison, D. L.; Migliaccio, M.] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England. [Eriksen, H. K.; Hansen, F. K.; Lilje, P. B.; Valiviita, J.] Univ Oslo, Inst Theoret Astrophys, N-0315 Oslo, Norway. [Rubino-Martin, J. A.] Inst Astrofis Canarias, Tenerife 38205, Spain. [Barreiro, R. B.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Toffolatti, L.; Vielva, P.] Univ Cantabria, CSIC, Inst Fis Cantabria, Santander 39065, Spain. [Bartlett, J. G.; Bock, J. J.; Colombo, L. P. L.; Crill, B. P.; Dore, O.; Gorski, K. M.; Holmes, W. A.; Lawrence, C. R.; Mitra, S.; Pietrobon, D.; Prezeau, G.; Rocha, G.; Seiffert, M. D.; Wade, L. A.] CALTECH, Jet Prop Lab, Pasadena, CA USA. [Davies, R. D.; Davis, R. J.; Noviello, F.] Univ Manchester, Jodrell Bank, Ctr Astrophys, Sch Phys & Astron, Manchester M13 9PL, Lancs, England. [Ashdown, M.; Bridges, M.; Challinor, A.; Gratton, S.; Harrison, D. L.; Lasenby, A.; Migliaccio, M.] Kavli Inst Cosmol Cambridge, Cambridge CB3 0HA, England. [Couchot, F.; Perdereau, O.; Plaszczynski, S.; Tristram, M.; Tucci, M.] Univ Paris 11, CNRS, IN2P3, LAL, F-91405 Orsay, France. [Catalano, A.; Lamarre, J. -M.] CNRS, Observ Paris, LERMA, F-75014 Paris, France. [Arnaud, M.; Bobin, J.; Chamballu, A.; Marshall, D. J.; Pratt, G. W.; Sureau, F.] Univ Paris Diderot, CNRS, CEA DSM, Lab AIM,IRFU Serv Astrophys, F-91191 Gif Sur Yvette, France. [Cardoso, J. -F.] CNRS, Lab Traitement & Commun Informat, UMR 5141, F-75634 Paris 13, France. [Cardoso, J. -F.] Telecom ParisTech, F-75634 Paris 13, France. [Catalano, A.; Macias-Perez, J. F.; Santos, D.] Univ Grenoble 1, Inst Natl Polytech Grenoble, CNRS IN2P3, Lab Phys Subatom & Cosmol, F-38026 Grenoble, France. [Van Tent, B.] Univ Paris 11, Phys Theor Lab, F-91405 Orsay, France. [Van Tent, B.] CNRS, F-91405 Orsay, France. [Kisner, T. S.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Ensslin, T. A.; Hovest, W.; Knoche, J.; Rachen, J. P.; Reinecke, M.; Riller, T.; Sunyaev, R.] Max Planck Inst Astrophys, D-85741 Garching, Germany. [Hanson, D.] McGill Univ, McGill Phys, Montreal, PQ H3A 2T8, Canada. [Christensen, P. R.; Naselsky, P.; Novikov, I.] Niels Bohr Inst, DK-2100 Copenhagen, Denmark. [Crill, B. P.] CALTECH, Observat Cosmol, Pasadena, CA 91125 USA. [Savini, G.] UCL, Opt Sci Lab, London, England. [Baccigalupi, C.; Bielewicz, P.; Danese, L.; de Zotti, G.; Gonzalez-Nuevo, J.; Perrotta, F.] SISSA, Astrophys Sect, I-34136 Trieste, Italy. [Munshi, D.; Spencer, L. D.] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales. [Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England. [Sunyaev, R.] Russian Acad Sci, Space Res Inst IKI, Moscow 117997, Russia. [Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA. [Osborne, S.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA. [Armitage-Caplan, C.] Univ Oxford, Sub Dept Astrophys, Oxford OX1 3RH, England. [Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Hivon, E.; Wandelt, B. D.] Univ Paris 06, UMR7095, F-75014 Paris, France. [Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France. [Reach, W. T.] Univ Space Res Assoc, Stratospher Observ Infrared Astron, Moffett Field, CA 94035 USA. [Gorski, K. M.] Univ Warsaw Observ, PL-00478 Warsaw, Poland. RP Scott, D (reprint author), Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC V5Z 1M9, Canada. EM dscott@phas.ubc.ca RI Barreiro, Rita Belen/N-5442-2014; Butler, Reginald/N-4647-2015; Tomasi, Maurizio/I-1234-2016; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; Nati, Federico/I-4469-2016; popa, lucia/B-4718-2012; Piacentini, Francesco/E-7234-2010; Atrio-Barandela, Fernando/A-7379-2017; White, Martin/I-3880-2015; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Valiviita, Jussi/A-9058-2016; Mazzotta, Pasquale/B-1225-2016; Kurki-Suonio, Hannu/B-8502-2016; Lahteenmaki, Anne/L-5987-2013; Toffolatti, Luigi/K-5070-2014; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Martinez-Gonzalez, Enrique/E-9534-2015; Gonzalez-Nuevo, Joaquin/I-3562-2014; OI Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Lopez-Caniego, Marcos/0000-0003-1016-9283; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Butler, Reginald/0000-0003-4366-5996; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Galeotta, Samuele/0000-0002-3748-5115; Ricciardi, Sara/0000-0002-3807-4043; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Tomasi, Maurizio/0000-0002-1448-6131; Colombo, Loris/0000-0003-4572-7732; Nati, Federico/0000-0002-8307-5088; Piacentini, Francesco/0000-0002-5444-9327; Atrio-Barandela, Fernando/0000-0002-2130-2513; Rubino-Martin, Jose Alberto/0000-0001-5289-3021; De Zotti, Gianfranco/0000-0003-2868-2595; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; White, Martin/0000-0001-9912-5070; Gruppuso, Alessandro/0000-0001-9272-5292; Valiviita, Jussi/0000-0001-6225-3693; Mazzotta, Pasquale/0000-0002-5411-1748; Kurki-Suonio, Hannu/0000-0002-4618-3063; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Pierpaoli, Elena/0000-0002-7957-8993; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Savini, Giorgio/0000-0003-4449-9416; Bouchet, Francois/0000-0002-8051-2924; Villa, Fabrizio/0000-0003-1798-861X; TERENZI, LUCA/0000-0001-9915-6379; Reach, William/0000-0001-8362-4094 FU ESA FX The development of Planck has been supported by: ESA; CNES and CNRS / INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA, and RES (Spain); Tekes, AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER / SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT / MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at h t t p : / / w w w. s c i o p s. e s a. i n t / i n d e x. p h p ? p r o j e c t = p l a n c k & p a g e = P l a n c k _ C o l l a b o r a t i o n. Some of the results in this paper have been derived using the H E A L P i x package. This research used resources of the National Energy Research Scientific Computing Center, which is supported by the O ffi ce of Science of the US Department of Energy under Contract No. DE-AC02-05CH11231. We acknowledge support from the Science and Technology Facilities Council [ grant number ST / I000976 / 1]. NR 66 TC 80 Z9 79 U1 3 U2 10 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A27 DI 10.1051/0004-6361/201321556 PG 11 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600019 ER PT J AU Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Battaner, E Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bonaldi, A Bonavera, L Bond, JR Borrill, J Bouchet, FR Bridges, M Bucher, M Burigana, C Butler, RC Cappellini, B Cardoso, JF Catalano, A Chamballu, A Chen, X Chiang, LY Christensen, PR Church, S Colombi, S Colombo, LPL Crill, BP Cruz, M Curto, A Cattaia, F Danese, L Davies, RD Davis, RJ de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Dickinson, C Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Falvella, MC Finelli, F Forni, O Frailis, M Franceschi, E Gaier, TC Galeotta, S Ganga, K Giard, M Giardino, G Giraud-Heraud, Y Gjerlow, E Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Hansen, FK Hanson, D Harrison, D Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Jaffe, AH Jaffe, TR Jewel, J Jones, WC Juvela, M Kangaslahti, P Keihanen, E Keskitalo, R Kiiveri, K Kisner, TS Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lahteenmaki, A Lamarre, JM Lasenby, A Lattanzi, M Laureijs, RJ Lawrence, CR Leach, S Leahy, JP Leonardi, R Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lindholm, V Lopez-Caniego, M Lubin, PM Macias-Perez, JE Maggio, G Maino, D Mandolesi, N Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Mazzotta, P Meinhold, PR Melchiorri, A Mendes, L Mennella, A Migliaccio, M Mitra, S Moneti, A Montier, L Morgantes, G Morisset, N Mortlock, D Moss, A Munshi, D Naseisky, P Natoli, P Netterfield, CB Norgaard-Nielsen, HU Novikov, D Novikov, I O'Dwyer, IJ Osborne, S Paci, F Pagano, L Paladini, R Paoletti, D Partridge, B Pasian, F Patanchon, G Peel, M Perdereau, O Perotto, L Perrotta, F Pierpaoli, E Pietrobon, D Plaszczynski, S Platania, P Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Reach, WT Rebolo, R Reinecke, M Remazeilles, M Ricciardi, S Riller, T Robbers, G Rocha, G Rosset, C Rossetti, M Roudier, G Rubino-Martin, JA Rusholme, B Salerno, E Sandri, M Santos, D Scott, D Seiffert, MD Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Sureau, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Tuovinen, J Turler, M Umana, G Valenziano, L Valiviita, J Van Tent, B Varis, J Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD Watson, R Wehus, IK White, SDM Wilkson, A Yvon, D Zacchei, A Zonca, A AF Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Battaner, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bonaldi, A. Bonavera, L. Bond, J. R. Borrill, J. Bouchet, F. R. Bridges, M. Bucher, M. Burigana, C. Butler, R. C. Cappellini, B. Cardoso, J. -F. Catalano, A. Chamballu, A. Chen, X. Chiang, L. -Y Christensen, P. R. Church, S. Colombi, S. Colombo, L. P. L. Crill, B. P. Cruz, M. Curto, A. Cattaia, F. Danese, L. Davies, R. D. Davis, R. J. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Dickinson, C. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Falvella, M. C. Finelli, F. Forni, O. Frailis, M. Franceschi, E. Gaier, T. C. Galeotta, S. Ganga, K. Giard, M. Giardino, G. Giraud-Heraud, Y. Gjerlow, E. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Hansen, F. K. Hanson, D. Harrison, D. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Jaffe, A. H. Jaffe, T. R. Jewel, J. Jones, W. C. Juvela, M. Kangaslahti, P. Keihanen, E. Keskitalo, R. Kiiveri, K. Kisner, T. S. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Lahteenmaki, A. Lamarre, J. -M. Lasenby, A. Lattanzi, M. Laureijs, R. J. Lawrence, C. R. Leach, S. Leahy, J. P. Leonardi, R. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lindholm, V. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. E. Maggio, G. Maino, D. Mandolesi, N. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. Meinhold, P. R. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Moneti, A. Montier, L. Morgantes, G. Morisset, N. Mortlock, D. Moss, A. Munshi, D. Naseisky, P. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Novikov, D. Novikov, I. O'Dwyer, I. J. Osborne, S. Paci, F. Pagano, L. Paladini, R. Paoletti, D. Partridge, B. Pasian, F. Patanchon, G. Peel, M. Perdereau, O. Perotto, L. Perrotta, F. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Platania, P. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Reach, W. T. Rebolo, R. Reinecke, M. Remazeilles, M. Ricciardi, S. Riller, T. Robbers, G. Rocha, G. Rosset, C. Rossetti, M. Roudier, G. Rubino-Martin, J. A. Rusholme, B. Salerno, E. Sandri, M. Santos, D. Scott, D. Seiffert, M. D. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sureau, F. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Tuovinen, J. Tuerler, M. Umana, G. Valenziano, L. Valiviita, J. Van Tent, B. Varis, J. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. Watson, R. Wehus, I. K. White, S. D. M. Wilkson, A. Yvon, D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. II. Low Frequency Instrument data processing SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE cosmic background radiation; methods: data analysis; cosmology: observations; surveys ID MAP-MAKING ALGORITHM; PRE-LAUNCH STATUS; DATA SETS; RADIOMETERS; NOISE AB We describe the data processing pipeline of the Planck Low Frequency Instrument (LFI) data processing centre (DPC) to create and characterize full-sky maps based on the first 15.5 months of operations at 30, 44, and 70 GHz. In particular, we discuss the various steps involved in reducing the data, from telemetry packets through to the production of cleaned, calibrated timelines and calibrated frequency maps. Data are continuously calibrated using the modulation induced on the mean temperature of the cosmic microwave background radiation by the proper motion of the spacecraft. Sky signals other than the dipole are removed by an iterative procedure based on simultaneous fitting of calibration parameters and sky maps. Noise properties are estimated from time-ordered data after the sky signal has been removed, using a generalized least squares map-making algorithm. A destriping code (Madam) is employed to combine radiometric data and pointing information into sky maps, minimizing the variance of correlated noise. Noise covariance matrices, required to compute statistical uncertainties on LFI and Planck products, are also produced. Main beams are estimated down to the approximate to-20 dB level using Jupiter transits, which are also used for the geometrical calibration of the focal plane. C1 [Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, Observ Paris, Sorbonne Paris Cite, CNRS IN2P3,CEA lrfu,APC, F-75205 Paris 13, France. [Lahteenmaki, A.; Poutanen, T.] Aalto Univ, Metsahovi Radio Observ, Kylmala 02540, Finland. [Kunz, M.] African Inst Math Sci, ZA-7945 Cape Town, South Africa. [Natoli, P.; Polenta, G.] Aeenzia Spaziale Italiana, Sci Data Ctr, I-00133 Rome, Italy. [Falvella, M. C.; Mandolesi, N.] Agenzia Spaziale Ilaliana, Rome, Italy. [Ashdown, M.; Bridges, M.; Curto, A.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 0HE, England. [Bond, J. R.; Hanson, D.; Martin, P. G.] Univ Toronto, CITA, Toronto, ON M5S 3H8, Canada. [Salerno, E.] CNR, ISTI, I-56100 Pisa, Italy. [Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.] CNRS, IRAP, F-31028 Toulouse 4, France. [Bock, J. J.; Dore, O.; Hildebrandt, S. R.; Prezeau, G.; Rocha, G.; Seiffert, M. D.] CALTECH, Pasadena, CA 91125 USA. [Shellard, E. P. S.] Univ Cambridge, Ctr Theoret Cosmol, DAMTP, Cambridge CB3 0WA, England. 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EM zacchei@oats.inaf.it RI Barreiro, Rita Belen/N-5442-2014; Remazeilles, Mathieu/N-1793-2015; Mazzotta, Pasquale/B-1225-2016; Kurki-Suonio, Hannu/B-8502-2016; Tomasi, Maurizio/I-1234-2016; Lattanzi, Massimiliano/D-8120-2011; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; popa, lucia/B-4718-2012; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; bonavera, laura/E-9368-2017; Martinez-Gonzalez, Enrique/E-9534-2015; Salerno, Emanuele/A-2137-2010; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Valiviita, Jussi/A-9058-2016; Lahteenmaki, Anne/L-5987-2013; Toffolatti, Luigi/K-5070-2014; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Cruz, Marcos/N-3429-2014; Butler, Reginald/N-4647-2015; OI Matarrese, Sabino/0000-0002-2573-1243; Galeotta, Samuele/0000-0002-3748-5115; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Umana, Grazia/0000-0002-6972-8388; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Lopez-Caniego, Marcos/0000-0003-1016-9283; Peel, Mike/0000-0003-3412-2586; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Mazzotta, Pasquale/0000-0002-5411-1748; Kurki-Suonio, Hannu/0000-0002-4618-3063; Tomasi, Maurizio/0000-0002-1448-6131; Lattanzi, Massimiliano/0000-0003-1059-2532; Colombo, Loris/0000-0003-4572-7732; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; bonavera, laura/0000-0001-8039-3876; Rubino-Martin, Jose Alberto/0000-0001-5289-3021; De Zotti, Gianfranco/0000-0003-2868-2595; Pierpaoli, Elena/0000-0002-7957-8993; Watson, Robert/0000-0002-5873-0124; Juvela, Mika/0000-0002-5809-4834; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Salerno, Emanuele/0000-0002-3433-3634; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Gruppuso, Alessandro/0000-0001-9272-5292; Valiviita, Jussi/0000-0001-6225-3693; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; Cruz, Marcos/0000-0002-4767-530X; Ricciardi, Sara/0000-0002-3807-4043; Villa, Fabrizio/0000-0003-1798-861X; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; Reach, William/0000-0001-8362-4094; Butler, Reginald/0000-0003-4366-5996; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924 NR 54 TC 48 Z9 47 U1 2 U2 14 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A2 DI 10.1051/0004-6361/201321550 PG 25 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600016 ER PT J AU Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Battaner, E Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bonaldi, A Bond, JR Borrill, J Bouchet, FR Bridges, M Bucher, M Burigana, C Butler, RC Cardoso, JF Catalano, A Chamballu, A Chiang, LY Christensen, PR Church, S Colombi, S Colombo, LPL Crill, BP Curto, A Cuttaia, F Danese, L Davies, RD Davis, RJ de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Dickinson, C Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Finelli, F Forni, O Frailis, M Franceschi, E Gaier, TC Galeotta, S Ganga, K Giard, M Giraud-Heraud, Y Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Hansen, FK Hanson, D Harrison, D Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Jaffe, AH Jaffe, TR Jewell, J Jones, WC Juvela, M Kangaslahti, P Keihanen, E Keskitalo, R Kiiveri, K Kisner, TS Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lahteenmaki, A Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Leahy, JP Leonardi, R Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lindholm, V Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maino, D Mandolesi, N Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Mazzotta, P Meinhold, PR Melchiorri, A Mendes, L Mennella, A Migliaccio, M Mitra, S Moneti, A Montier, L Morgante, G Mortlock, D Moss, A Munshi, D Naselsky, P Natoli, P Netterfield, CB Norgaard-Nielsen, HU Novikov, D Novikov, I O'Dwyer, IJ Osborne, S Paci, F Pagano, L Paoletti, D Partridge, B Pasian, F Patanchon, G Perdereau, O Perotto, L Perrotta, F Pierpaoli, E Pietrobon, D Plaszczynski, S Platania, P Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Rebolo, R Reinecke, M Remazeilles, M Ricciardi, S Riller, T Rocha, G Rosset, C Roudier, G Rubino-Martin, JA Rusholme, B Sandri, M Santos, D Scott, D Seiffert, MD Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Sureau, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Tuovinen, J Turler, M Umana, G Valenziano, L Valiviita, J Van Tent, B Varis, J Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD Zacchei, A Zonca, A AF Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Battaner, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bonaldi, A. Bond, J. R. Borrill, J. Bouchet, F. R. Bridges, M. Bucher, M. Burigana, C. Butler, R. C. Cardoso, J. -F. Catalano, A. Chamballu, A. Chiang, L. -Y Christensen, P. R. Church, S. Colombi, S. Colombo, L. P. L. Crill, B. P. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. Davis, R. J. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Dickinson, C. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Finelli, F. Forni, O. Frailis, M. Franceschi, E. Gaier, T. C. Galeotta, S. Ganga, K. Giard, M. Giraud-Heraud, Y. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Hansen, F. K. Hanson, D. Harrison, D. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Jaffe, A. H. Jaffe, T. R. Jewell, J. Jones, W. C. Juvela, M. Kangaslahti, P. Keihanen, E. Keskitalo, R. Kiiveri, K. Kisner, T. S. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Lahteenmaki, A. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leahy, J. P. Leonardi, R. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lindholm, V. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maino, D. Mandolesi, N. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. Meinhold, P. R. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Moss, A. Munshi, D. Naselsky, P. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Novikov, D. Novikov, I. O'Dwyer, I. J. Osborne, S. Paci, F. Pagano, L. Paoletti, D. Partridge, B. Pasian, F. Patanchon, G. Perdereau, O. Perotto, L. Perrotta, F. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Platania, P. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Rebolo, R. Reinecke, M. Remazeilles, M. Ricciardi, S. Riller, T. Rocha, G. Rosset, C. Roudier, G. Rubino-Martin, J. A. Rusholme, B. Sandri, M. Santos, D. Scott, D. Seiffert, M. D. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sureau, F. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Tuovinen, J. Tuerler, M. Umana, G. Valenziano, L. Valiviita, J. Van Tent, B. Varis, J. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. IV. Low Frequency Instrument beams and window functions SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE methods: data analysis; cosmic background radiation; telescopes ID PROBE WMAP OBSERVATIONS; PRE-LAUNCH STATUS; POWER SPECTRUM; MICROWAVE; MAPS; ERRORS AB This paper presents the characterization of the in-flight beams, the beam window functions, and the associated uncertainties for the Planck Low Frequency Instrument (LFI). Knowledge of the beam profiles is necessary for determining the transfer function to go from the observed to the actual sky anisotropy power spectrum. The main beam distortions affect the beam window function, complicating the reconstruction of the anisotropy power spectrum at high multipoles, whereas the sidelobes affect the low and intermediate multipoles. The in-flight assessment of the LFI main beams relies on the measurements performed during Jupiter observations. By stacking the data from multiple Jupiter transits, the main beam profiles are measured down to -20 dB at 30 and 44 GHz, and down to -25 dB at 70 GHz. The main beam solid angles are determined to better than 0.2% at each LFI frequency band. The Planck pre-launch optical model is conveniently tuned to characterize the main beams independently of any noise effects. This approach provides an optical model whose beams fully reproduce the measurements in the main beam region, but also allows a description of the beams at power levels lower than can be achieved by the Jupiter measurements themselves. The agreement between the simulated beams and the measured beams is better than 1% at each LFI frequency band. The simulated beams are used for the computation of the window functions for the effective beams. The error budget for the window functions is estimated from both main beam and sidelobe contributions, and accounts for the radiometer bandshapes. 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EM sandri@iasfbo.inaf.it RI Barreiro, Rita Belen/N-5442-2014; Tomasi, Maurizio/I-1234-2016; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; popa, lucia/B-4718-2012; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; Remazeilles, Mathieu/N-1793-2015; Mazzotta, Pasquale/B-1225-2016; Kurki-Suonio, Hannu/B-8502-2016; Lahteenmaki, Anne/L-5987-2013; Toffolatti, Luigi/K-5070-2014; Vielva, Patricio/F-6745-2014; Martinez-Gonzalez, Enrique/E-9534-2015; Herranz, Diego/K-9143-2014; Gonzalez-Nuevo, Joaquin/I-3562-2014; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Valiviita, Jussi/A-9058-2016; Butler, Reginald/N-4647-2015; OI Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Galeotta, Samuele/0000-0002-3748-5115; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Tomasi, Maurizio/0000-0002-1448-6131; Colombo, Loris/0000-0003-4572-7732; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; Rubino-Martin, Jose Alberto/0000-0001-5289-3021; De Zotti, Gianfranco/0000-0003-2868-2595; Lopez-Caniego, Marcos/0000-0003-1016-9283; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Mazzotta, Pasquale/0000-0002-5411-1748; Kurki-Suonio, Hannu/0000-0002-4618-3063; Toffolatti, Luigi/0000-0003-2645-7386; Vielva, Patricio/0000-0003-0051-272X; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Herranz, Diego/0000-0003-4540-1417; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Gruppuso, Alessandro/0000-0001-9272-5292; Valiviita, Jussi/0000-0001-6225-3693; Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Ricciardi, Sara/0000-0002-3807-4043; Villa, Fabrizio/0000-0003-1798-861X; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; Umana, Grazia/0000-0002-6972-8388; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Butler, Reginald/0000-0003-4366-5996; Sandri, Maura/0000-0003-4806-5375; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099 FU CNES; CNRS/INSU-IN2P3-INP; ASI; Italian Space Agency (ASI); INAF; Academy of Finland [253204, 256265, 257989]; European Community [RI-283493]; Spanish Ministerio de Ciencia e Innovacion through the Plan Nacional del Espacio y Plan Nacional de Astronomia y Astrofisica; Space Agency of the German Aerospace Center (DLR) [50OP0901]; Max Planck Society; National Energy Research Scientific Computing Center - Office of Science of the US Department of Energy [DE-AC02-05CH11231]; ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR (Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC (Spain); MICINN (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF (Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); PRACE (EU) FX Planck is too large a project to allow full acknowledgement of all contributions by individuals, institutions, industries, and funding agencies. The main entities involved in the mission operations are as follows. The European Space Agency (ESA) operates the satellite via its Mission Operations Centre located at ESOC (Darmstadt, Germany) and coordinates scientific operations via the Planck Science Office located at ESAC (Madrid, Spain). Two Consortia, comprising around 50 scientific institutes within Europe, the USA, and Canada, and funded by agencies from the participating countries, developed the scientific instruments LFI and HFI, and continue to operate them via Instrument Operations Teams located in Trieste (Italy) and Orsay (France). The Consortia are also responsible for scientific processing of the acquired data. The Consortia are led by the Principal Investigators: J. L. Puget in France for HFI (funded principally by CNES and CNRS/INSU-IN2P3-INP) and N. Mandolesi in Italy for LFI (funded principally via ASI). NASA US Planck Project, based at JPL and involving scientists at many US institutions, contributes significantly to the efforts of these two Consortia. The author list for this paper has been selected by the Planck Science Team, and is composed of individuals from all of the above entities who have made multi-year contributions to the development of the mission. It does not pretend to be inclusive of all contributions. The Planck-LFI project is developed by an International Consortium lead by Italy and involving Canada, Finland, Germany, Norway, Spain, Switzerland, UK, USA. The Italian contribution to Planck is supported by the Italian Space Agency (ASI) and INAF. This work was supported by the Academy of Finland grants 253204, 256265, and 257989. This work was granted access to the HPC resources of CSC made available within the Distributed European Computing Initiative by the PRACE-2IP, receiving funding from the European Community's Seventh Framework Programme (FP7/2007-2013) under grant agreement RI-283493. We thank CSC-IT Center for Science Ltd (Finland) for computational resources. We acknowledge financial support provided by the Spanish Ministerio de Ciencia e Innovacion through the Plan Nacional del Espacio y Plan Nacional de Astronomia y Astrofisica. We acknowledge the Max Planck Institute for Astrophysics Planck Analysis Centre (MPAC), funded by the Space Agency of the German Aerospace Center (DLR) under grant 50OP0901 with resources of the German Federal Ministry of Economics and Technology, and by the Max Planck Society. This work has made use of the Planck satellite simulation package (Level-S), which is assembled by the Max Planck Institute for Astrophysics Planck Analysis Centre (MPAC) Reinecke et al. (2006). We acknowledge financial support provided by the National Energy Research Scientific Computing Center, which is supported by the Office of Science of the US Department of Energy under Contract No. DE-AC02-05CH11231. Some of the results in this paper have been derived using the HEALPix package Gorski et al. (2005). The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU).; A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.sciops.esa.int/index.php?project=planck&page=Planck_Collabora tion NR 59 TC 41 Z9 40 U1 2 U2 11 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A4 DI 10.1051/0004-6361/201321544 PG 22 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600014 ER PT J AU Aghanim, N Armitage-Caplan, C Arnaud, M Ashdown, M Atrio-Barandela, F Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Battaner, E Benabed, K Benoit, A Benoit-Levy, A Bernard, JP Bersanelli, M Bielewicz, P Bobin, J Bock, JJ Bonaldi, A Bonavera, L Bond, JR Borrill, J Bouchet, FR Bridges, M Bucher, M Burigana, C Butler, RC Cappellini, B Cardoso, JF Catalano, A Chamballu, A Chen, X Chiang, LY Christensen, PR Church, S Colombi, S Colombo, LPL Crill, BP Curto, A Cuttaia, F Danese, L Davies, RD Davis, RJ de Bernardis, P de Rosa, A de Zotti, G Delabrouille, J Dickinson, C Diego, JM Dole, H Donzelli, S Dore, O Douspis, M Dupac, X Efstathiou, G Ensslin, TA Eriksen, HK Finelli, F Forni, O Frailis, M Franceschi, E Gaier, TC Galeotta, S Ganga, K Giard, M Giardino, G Giraud-Heraud, Y Gjerlow, E Gonzalez-Nuevo, J Gorski, KM Gratton, S Gregorio, A Gruppuso, A Hansen, FK Hanson, D Harrison, D Henrot-Versille, S Hernandez-Monteagudo, C Herranz, D Hildebrandt, SR Hivon, E Hobson, M Holmes, WA Hornstrup, A Hovest, W Huffenberger, KM Jaffe, AH Jaffe, TR Jewell, J Jones, WC Juvela, M Kangaslahti, P Keihanen, E Keskitalo, R Kisner, TS Knoche, J Knox, L Kunz, M Kurki-Suonio, H Lagache, G Lahteenmaki, A Lamarre, JM Lasenby, A Laureijs, RJ Lawrence, CR Leach, S Leahy, JP Leonard, R Lesgourgues, J Liguori, M Lilje, PB Linden-Vornle, M Lopez-Caniego, M Lubin, PM Macias-Perez, JF Maino, D Mandolesi, N Maris, M Marshall, DJ Martin, PG Martinez-Gonzalez, E Masi, S Massardi, M Matarrese, S Matthai, F Mazzotta, P Meinhold, PR Melchiorri, A Mendes, L Mennella, A Migliaccio, M Mitra, S Moneti, A Montier, L Morgante, G Mortlock, D Moss, A Munshi, D Naselsky, P Natoli, P Netterfield, CB Norgaard-Nielsen, HU Novikov, D Novikov, I O'Dwyer, IJ Osborne, S Paci, F Pagano, L Paladini, R Paoletti, D Partridge, B Pasian, F Patanchon, G Pearson, D Peel, M Perdereau, O Perotto, L Perrotta, F Pierpaoli, E Pietrobon, D Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Popa, L Poutanen, T Pratt, GW Prezeau, G Prunet, S Puget, JL Rachen, JP Rebolo, R Reinecke, M Remazeilles, M Ricciardi, S Riller, T Rocha, G Rosset, C Rossetti, M Roudier, G Rubino-Martin, JA Rusholme, B Sandri, M Santos, D Scott, D Seiffert, MD Shellard, EPS Spencer, LD Starck, JL Stolyarov, V Stompor, R Sureau, F Sutton, D Suur-Uski, AS Sygnet, JF Tauber, JA Tavagnacco, D Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Tuovinen, J Turler, M Umana, G Valenziano, L Valiviita, J Van Tent, B Varis, J Vielva, P Villa, F Vittorio, N Wade, LA Wandelt, BD Watson, R Wilkinson, A Yvon, D Zacchei, A Zonca, A AF Aghanim, N. Armitage-Caplan, C. Arnaud, M. Ashdown, M. Atrio-Barandela, F. Aumont, J. Baccigalupi, C. Banday, A. J. Barreiro, R. B. Battaner, E. Benabed, K. Benoit, A. Benoit-Levy, A. Bernard, J. -P. Bersanelli, M. Bielewicz, P. Bobin, J. Bock, J. J. Bonaldi, A. Bonavera, L. Bond, J. R. Borrill, J. Bouchet, F. R. Bridges, M. Bucher, M. Burigana, C. Butler, R. C. Cappellini, B. Cardoso, J. -F. Catalano, A. Chamballu, A. Chen, X. Chiang, L. -Y Christensen, P. R. Church, S. Colombi, S. Colombo, L. P. L. Crill, B. P. Curto, A. Cuttaia, F. Danese, L. Davies, R. D. Davis, R. J. de Bernardis, P. de Rosa, A. de Zotti, G. Delabrouille, J. Dickinson, C. Diego, J. M. Dole, H. Donzelli, S. Dore, O. Douspis, M. Dupac, X. Efstathiou, G. Ensslin, T. A. Eriksen, H. K. Finelli, F. Forni, O. Frailis, M. Franceschi, E. Gaier, T. C. Galeotta, S. Ganga, K. Giard, M. Giardino, G. Giraud-Heraud, Y. Gjerlow, E. Gonzalez-Nuevo, J. Gorski, K. M. Gratton, S. Gregorio, A. Gruppuso, A. Hansen, F. K. Hanson, D. Harrison, D. Henrot-Versille, S. Hernandez-Monteagudo, C. Herranz, D. Hildebrandt, S. R. Hivon, E. Hobson, M. Holmes, W. A. Hornstrup, A. Hovest, W. Huffenberger, K. M. Jaffe, A. H. Jaffe, T. R. Jewell, J. Jones, W. C. Juvela, M. Kangaslahti, P. Keihanen, E. Keskitalo, R. Kisner, T. S. Knoche, J. Knox, L. Kunz, M. Kurki-Suonio, H. Lagache, G. Lahteenmaki, A. Lamarre, J. -M. Lasenby, A. Laureijs, R. J. Lawrence, C. R. Leach, S. Leahy, J. P. Leonard, R. Lesgourgues, J. Liguori, M. Lilje, P. B. Linden-Vornle, M. Lopez-Caniego, M. Lubin, P. M. Macias-Perez, J. F. Maino, D. Mandolesi, N. Maris, M. Marshall, D. J. Martin, P. G. Martinez-Gonzalez, E. Masi, S. Massardi, M. Matarrese, S. Matthai, F. Mazzotta, P. Meinhold, P. R. Melchiorri, A. Mendes, L. Mennella, A. Migliaccio, M. Mitra, S. Moneti, A. Montier, L. Morgante, G. Mortlock, D. Moss, A. Munshi, D. Naselsky, P. Natoli, P. Netterfield, C. B. Norgaard-Nielsen, H. U. Novikov, D. Novikov, I. O'Dwyer, I. J. Osborne, S. Paci, F. Pagano, L. Paladini, R. Paoletti, D. Partridge, B. Pasian, F. Patanchon, G. Pearson, D. Peel, M. Perdereau, O. Perotto, L. Perrotta, F. Pierpaoli, E. Pietrobon, D. Plaszczynski, S. Pointecouteau, E. Polenta, G. Ponthieu, N. Popa, L. Poutanen, T. Pratt, G. W. Prezeau, G. Prunet, S. Puget, J. -L. Rachen, J. P. Rebolo, R. Reinecke, M. Remazeilles, M. Ricciardi, S. Riller, T. Rocha, G. Rosset, C. Rossetti, M. Roudier, G. Rubino-Martin, J. A. Rusholme, B. Sandri, M. Santos, D. Scott, D. Seiffert, M. D. Shellard, E. P. S. Spencer, L. D. Starck, J. -L. Stolyarov, V. Stompor, R. Sureau, F. Sutton, D. Suur-Uski, A. -S. Sygnet, J. -F. Tauber, J. A. Tavagnacco, D. Terenzi, L. Toffolatti, L. Tomasi, M. Tristram, M. Tucci, M. Tuovinen, J. Tuerler, M. Umana, G. Valenziano, L. Valiviita, J. Van Tent, B. Varis, J. Vielva, P. Villa, F. Vittorio, N. Wade, L. A. Wandelt, B. D. Watson, R. Wilkinson, A. Yvon, D. Zacchei, A. Zonca, A. CA Planck Collaboration TI Planck 2013 results. V. LFI calibration SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE cosmic background radiation; instrumentation: polarimeters; methods: data analysis ID MICROWAVE-ANISOTROPY-PROBE; PRE-LAUNCH STATUS; WMAP OBSERVATIONS; SKY MAPS; GHZ AB We discuss the methods employed to photometrically calibrate the data acquired by the Low Frequency Instrument on Planck. Our calibration is based on a combination of the orbital dipole plus the solar dipole, caused respectively by the motion of the Planck spacecraft with respect to the Sun and by motion of the solar system with respect to the cosmic microwave background (CMB) rest frame. The latter provides a signal of a few mK with the same spectrum as the CMB anisotropies and is visible throughout the mission. In this data release we rely on the characterization of the solar dipole as measured by WMAP. We also present preliminary results (at 44 GHz only) on the study of the Orbital Dipole, which agree with the WMAP value of the solar system speed within our uncertainties. We compute the calibration constant for each radiometer roughly once per hour; in order to keep track of changes in the detectors' gain. Since non-idealities in the optical response of the beams proved to be important, we implemented a fast convolution algorithm which considers the full beam response in estimating the signal generated by the dipole. Moreover, in order to further reduce the impact of residual systematics due to sidelobes, we estimated time variations in the calibration constant of the 30 GHz radiometers (the ones with the largest sidelobes) using the signal of an internal reference load at 4 K instead of the CMB dipole. We have estimated the accuracy of the LFI calibration following two strategies: (1) we have run a set of simulations to assess the impact of statistical errors and systematic effects in the instrument and in the calibration procedure; and (2) we have performed a number of internal consistency checks on the data and on the brightness temperature of Jupiter. Errors in the calibration of this Planck/LFI data release are expected to be about 0.6% at 44 and 70 GHz, and 0.8% at 30 GHz. Both these preliminary results at low and high l are consistent with WMAP results within uncertainties and comparison of power spectra indicates good consistency in the absolute calibration with HFI (0.3%) and a 1.4 sigma discrepancy with WMAP (0.9%). C1 [Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, Observ Paris, Sorbonne Paris Cite, APC,CNRS IN2P3,CEA lrfu, F-75205 Paris 13, France. 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[Tuovinen, J.; Varis, J.] VTT Tech Res Ctr Finland, MilliLab, Espoo, Finland. [Christensen, P. R.; Naselsky, P.; Novikov, I.] Niels Bohr Inst, DK-2100 Copenhagen, Denmark. [Crill, B. P.] CALTECH, Obser Cosmol, Pasadena, CA 91125 USA. [Lesgourgues, J.] Ecole Polytech Fed Lausanne, SB ITP LPPC, CH-1015 Lausanne, Switzerland. [Baccigalupi, C.; Bielewicz, P.; Danese, L.; de Zotti, G.; Gonzalez-Nuevo, J.; Leach, S.; Paci, F.] SISSA, Astrophys Sect, I-34136 Trieste, Italy. [Munshi, D.; Spencer, L. D.] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales. [Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England. [Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA. [Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz 369167, Zelenchukskiy R, Russia. [Church, S.; Osborne, S.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA. [Armitage-Caplan, C.] Univ Oxford, Sub Dept Astrophys, Oxford OX1 3RH, England. [Lesgourgues, J.] CERN, PH TH, Div Theory, CH-1211 Geneva 23, Switzerland. [Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Colombi, S.; Hivon, E.; Prunet, S.; Wandelt, B. D.] Univ Paris 06, UMR7095, F-75014 Paris, France. [Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France. [Battaner, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, Granada, Spain. [Gorski, K. M.] Univ Warsaw Observ, PL-00478 Warsaw, Poland. RP Tomasi, M (reprint author), Univ Milan, Dipartimento Fis, Via Celoria 16, Milan, Italy. EM maurizio.tomasi@unimi.it RI Remazeilles, Mathieu/N-1793-2015; Tomasi, Maurizio/I-1234-2016; Novikov, Igor/N-5098-2015; Colombo, Loris/J-2415-2016; popa, lucia/B-4718-2012; Atrio-Barandela, Fernando/A-7379-2017; Stolyarov, Vladislav/C-5656-2017; bonavera, laura/E-9368-2017; Lahteenmaki, Anne/L-5987-2013; Gonzalez-Nuevo, Joaquin/I-3562-2014; Gruppuso, Alessandro/N-5592-2015; Novikov, Dmitry/P-1807-2015; Toffolatti, Luigi/K-5070-2014; Valiviita, Jussi/A-9058-2016; Mazzotta, Pasquale/B-1225-2016; Kurki-Suonio, Hannu/B-8502-2016; Yvon, Dominique/D-2280-2015; Vielva, Patricio/F-6745-2014; Martinez-Gonzalez, Enrique/E-9534-2015; Herranz, Diego/K-9143-2014; Barreiro, Rita Belen/N-5442-2014; Butler, Reginald/N-4647-2015; OI Morgante, Gianluca/0000-0001-9234-7412; Remazeilles, Mathieu/0000-0001-9126-6266; Maris, Michele/0000-0001-9442-2754; Franceschi, Enrico/0000-0002-0585-6591; Valenziano, Luca/0000-0002-1170-0104; Matarrese, Sabino/0000-0002-2573-1243; Galeotta, Samuele/0000-0002-3748-5115; Pasian, Fabio/0000-0002-4869-3227; WANDELT, Benjamin/0000-0002-5854-8269; Tomasi, Maurizio/0000-0002-1448-6131; Colombo, Loris/0000-0003-4572-7732; Atrio-Barandela, Fernando/0000-0002-2130-2513; Stolyarov, Vladislav/0000-0001-8151-828X; bonavera, laura/0000-0001-8039-3876; Rubino-Martin, Jose Alberto/0000-0001-5289-3021; De Zotti, Gianfranco/0000-0003-2868-2595; Lopez-Caniego, Marcos/0000-0003-1016-9283; Peel, Mike/0000-0003-3412-2586; Masi, Silvia/0000-0001-5105-1439; de Bernardis, Paolo/0000-0001-6547-6446; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Gruppuso, Alessandro/0000-0001-9272-5292; Toffolatti, Luigi/0000-0003-2645-7386; Valiviita, Jussi/0000-0001-6225-3693; Mazzotta, Pasquale/0000-0002-5411-1748; Kurki-Suonio, Hannu/0000-0002-4618-3063; Vielva, Patricio/0000-0003-0051-272X; Martinez-Gonzalez, Enrique/0000-0002-0179-8590; Herranz, Diego/0000-0003-4540-1417; Paoletti, Daniela/0000-0003-4761-6147; Pierpaoli, Elena/0000-0002-7957-8993; Watson, Robert/0000-0002-5873-0124; Juvela, Mika/0000-0002-5809-4834; TERENZI, LUCA/0000-0001-9915-6379; Starck, Jean-Luc/0000-0003-2177-7794; Zacchei, Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Lilje, Per/0000-0003-4324-7794; Cuttaia, Francesco/0000-0001-6608-5017; Huffenberger, Kevin/0000-0001-7109-0099; Burigana, Carlo/0000-0002-3005-5796; Bouchet, Francois/0000-0002-8051-2924; Ricciardi, Sara/0000-0002-3807-4043; Villa, Fabrizio/0000-0003-1798-861X; Barreiro, Rita Belen/0000-0002-6139-4272; Finelli, Fabio/0000-0002-6694-3269; Umana, Grazia/0000-0002-6972-8388; Scott, Douglas/0000-0002-6878-9840; Frailis, Marco/0000-0002-7400-2135; Gregorio, Anna/0000-0003-4028-8785; Polenta, Gianluca/0000-0003-4067-9196; Butler, Reginald/0000-0003-4366-5996; Sandri, Maura/0000-0003-4806-5375 FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR (Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC (Spain); MICINN (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF (Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); PRACE (EU) FX The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.sciops.esa.int/index.php?project=planck&page=Planck_Collabora tion. NR 69 TC 47 Z9 46 U1 2 U2 11 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD NOV PY 2014 VL 571 AR A5 DI 10.1051/0004-6361/201321527 PG 29 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AT9ZK UT WOS:000345282600006 ER PT J AU Garbe, JC Vrba, L Sputova, K Fuchs, L Novak, P Brothman, AR Jackson, M Chin, K LaBarge, MA Watts, G Futscher, BW Stampfer, MR AF Garbe, James C. Vrba, Lukas Sputova, Klara Fuchs, Laura Novak, Petr Brothman, Arthur R. Jackson, Mark Chin, Koei LaBarge, Mark A. Watts, George Futscher, Bernard W. Stampfer, Martha R. TI Immortalization of normal human mammary epithelial cells in two steps by direct targeting of senescence barriers does not require gross genomic alterations SO CELL CYCLE LA English DT Article DE carcinogenesis; c-Myc; genomic instability; human mammary epithelial cells; immortalization; p16INK4a; senescence; telomerase ID HUMAN BREAST-CANCER; TELOMERASE ACTIVITY; DNA METHYLATION; IN-SITU; MALIGNANT-TRANSFORMATION; P16 INACTIVATION; GROWTH ARREST; P53 FUNCTION; LIFE-SPAN; INSTABILITY AB Telomerase reactivation and immortalization are critical for human carcinoma progression. However, little is known about the mechanisms controlling this crucial step, due in part to the paucity of experimentally tractable model systems that can examine human epithelial cell immortalization as it might occur in vivo. We achieved efficient non-clonal immortalization of normal human mammary epithelial cells (HMEC) by directly targeting the 2 main senescence barriers encountered by cultured HMEC. The stress-associated stasis barrier was bypassed using shRNA to p16(INK4); replicative senescence due to critically shortened telomeres was bypassed in post-stasis HMEC by c-MYC transduction. Thus, 2 pathologically relevant oncogenic agents are sufficient to immortally transform normal HMEC. The resultant non-clonal immortalized lines exhibited normal karyotypes. Most human carcinomas contain genomically unstable cells, with widespread instability first observed in vivo in pre-malignant stages; in vitro, instability is seen as finite cells with critically shortened telomeres approach replicative senescence. Our results support our hypotheses that: (1) telomere-dysfunction induced genomic instability in pre-malignant finite cells may generate the errors required for telomerase reactivation and immortalization, as well as many additional passenger errors carried forward into resulting carcinomas; (2) genomic instability during cancer progression is needed to generate errors that overcome tumor suppressive barriers, but not required per se; bypassing the senescence barriers by direct targeting eliminated a need for genomic errors to generate immortalization. Achieving efficient HMEC immortalization, in the absence of passenger genomic errors, should facilitate examination of telomerase regulation during human carcinoma progression, and exploration of agents that could prevent immortalization. C1 [Garbe, James C.; Sputova, Klara; LaBarge, Mark A.; Stampfer, Martha R.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Life Sci, Berkeley, CA 94720 USA. [Vrba, Lukas; Novak, Petr; Watts, George; Futscher, Bernard W.; Stampfer, Martha R.] Univ Arizona, Arizona Canc Ctr, Tucson, AZ USA. [Vrba, Lukas; Futscher, Bernard W.] Univ Arizona, Coll Pharm, Dept Pharmacol & Toxicol, Tucson, AZ 85721 USA. [Vrba, Lukas; Novak, Petr] Acad Sci Czech Republic, Inst Plant Mol Biol, Ctr Biol, Vvi, CR-37005 Ceske Budejovice, Czech Republic. [Fuchs, Laura; Brothman, Arthur R.] Univ Arizona, Coll Med, Dept Pathol, Tucson, AZ 85721 USA. [Jackson, Mark] Case Western Reserve Univ, Case Comprehens Canc Ctr, Cleveland, OH 44106 USA. [Chin, Koei] Univ Calif San Francisco, San Francisco, CA 94143 USA. RP Stampfer, MR (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Life Sci, Berkeley, CA 94720 USA. EM JCGarbe@lbl.gov; mrstampfer@lbl.gov RI Vrba, Lukas/J-9268-2015; Novak, Petr/A-3059-2013 OI Vrba, Lukas/0000-0003-3042-6275; Novak, Petr/0000-0002-5068-9681 FU DOD [BCRP BC060444]; NIH [CA24844, CA23074]; NIH NIA [R00AG033176, R01AG040081]; SWEHSC NIEHS [ES06694]; Margaret E. and Fenton L. Maynard Endowment for Breast Cancer Research; University of Arizona Cytogenomics Laboratory; ACS RSG CCG [122517]; Office of Energy Research, Office of Health and Biological Research, US. Department of Energy [DE-AC02-05CH11231]; [RVO:60077344] FX This work was supported by DOD BCRP BC060444 (JCG, MRS), NIH CA24844 (JCG, MRS), NIH NIA R00AG033176 and R01AG040081 (JCG, KS, MAL), SWEHSC NIEHS ES06694 and NIH CA23074 (LV, PN, GW, BWF), Margaret E. and Fenton L. Maynard Endowment for Breast Cancer Research (BWF), RVO:60077344 (PN), University of Arizona Cytogenomics Laboratory (LF, AB), ACS RSG CCG 122517 (MJ), and the Office of Energy Research, Office of Health and Biological Research, US. Department of Energy under Contract No. DE-AC02-05CH11231. (JCG, KS, MAL, MRS). NR 68 TC 10 Z9 10 U1 2 U2 12 PU LANDES BIOSCIENCE PI AUSTIN PA 1806 RIO GRANDE ST, AUSTIN, TX 78702 USA SN 1538-4101 EI 1551-4005 J9 CELL CYCLE JI Cell Cycle PD NOV 1 PY 2014 VL 13 IS 21 BP 3423 EP 3435 DI 10.4161/15384101.2014.954456 PG 13 WC Cell Biology SC Cell Biology GA AZ6FA UT WOS:000348313100015 PM 25485586 ER PT J AU Gearhart, J Brown, N Jones, D Nozick, L Romero, N Xu, NX AF Gearhart, Jared Brown, Nathanael Jones, Dean Nozick, Linda Romero, Natalia Xu, Ningxiong TI Optimization-Based Probabilistic Consequence Scenario Construction for Lifeline Systems SO EARTHQUAKE SPECTRA LA English DT Article AB The construction of a suite of consequence scenarios that is consistent with the joint distribution of damage to a lifeline system is critical to properly estimating regional loss after an earthquake. This paper describes an optimization method that identifies a suite of consequence scenarios that can be used in regional loss estimation for lifeline systems when computational demands are of concern, and it is important to capture the spatial correlation associated with individual events. This method is applied to a realistic case study focused on the highway network in Memphis, Tennessee, within the New Madrid Seismic Zone. This case study illustrates that significantly fewer consequence scenarios are needed with this method than would be required using Monte Carlo simulation. C1 [Gearhart, Jared; Brown, Nathanael; Jones, Dean] Sandia Natl Labs, Albuquerque, NM 87185 USA. [Nozick, Linda; Romero, Natalia; Xu, Ningxiong] Cornell Univ, Sch Civil & Environm Engn, Ithaca, NY 14853 USA. RP Gearhart, J (reprint author), Sandia Natl Labs, POB 5800,Mail Stop 1138, Albuquerque, NM 87185 USA. NR 23 TC 1 Z9 1 U1 1 U2 2 PU EARTHQUAKE ENGINEERING RESEARCH INST PI OAKLAND PA 499 14TH ST, STE 320, OAKLAND, CA 94612-1934 USA SN 8755-2930 EI 1944-8201 J9 EARTHQ SPECTRA JI Earthq. Spectra PD NOV PY 2014 VL 30 IS 4 BP 1531 EP 1551 DI 10.1193/092711EQS237M PG 21 WC Engineering, Civil; Engineering, Geological SC Engineering GA AZ1MB UT WOS:000348002000009 ER PT J AU Engelsen, A Wnup-Lipinska, K Tiron, C Pelissier, F Jokela, T Haaland, G Gausdal, G Sandal, T Frink, R Liang, X Hinz, S Ahmed, L Hellesoy, M Mickelm, D Minna, J LaBarge, M Brekken, R Lorens, J AF Engelsen, A. Wnup-Lipinska, K. Tiron, C. Pelissier, F. Jokela, T. Haaland, G. Gausdal, G. Sandal, T. Frink, R. Liang, X. Hinz, S. Ahmed, L. Hellesoy, M. Mickelm, D. Minna, J. LaBarge, M. Brekken, R. Lorens, J. TI Phenotypic plasticity in epithelial progenitors and mesenchymal carcinoma is regulated by Axl signaling SO EUROPEAN JOURNAL OF CANCER LA English DT Meeting Abstract CT 26th EORTC-NCI-AACR Symposium on Molecular Targets and Cancer Therapeutics CY NOV 18-21, 2014 CL European Org Res & Treatment Canc, Barcelona, SPAIN SP Natl Canc Inst, Amer Assoc Canc Res HO European Org Res & Treatment Canc C1 [Engelsen, A.; Wnup-Lipinska, K.; Tiron, C.; Pelissier, F.; Jokela, T.; Haaland, G.; Lorens, J.] Univ Bergen, Bergen, Norway. [Gausdal, G.; Sandal, T.; Liang, X.; Ahmed, L.; Hellesoy, M.; Mickelm, D.] BerGenBio, Biomed, Bergen, Norway. [Frink, R.; Hinz, S.; Minna, J.; Brekken, R.] UT Southwestern, Harmon Canc Ctr, Dallas, TX USA. [LaBarge, M.] LBNL, Berkeley, CA USA. RI Lorens, James/B-9737-2017 OI Lorens, James/0000-0002-6782-3349 NR 0 TC 0 Z9 0 U1 1 U2 4 PU ELSEVIER SCI LTD PI OXFORD PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, OXON, ENGLAND SN 0959-8049 EI 1879-0852 J9 EUR J CANCER JI Eur. J. Cancer PD NOV PY 2014 VL 50 SU 6 MA 362 BP 117 EP 117 PG 1 WC Oncology SC Oncology GA AY7RC UT WOS:000347755700363 ER PT J AU Harrington, GA Gardner, WP Munday, TJ AF Harrington, Glenn A. Gardner, W. Payton Munday, Tim J. TI Tracking Groundwater Discharge to a Large River using Tracers and Geophysics SO GROUNDWATER LA English DT Article ID RESISTIVITY DATA; RN-222; INVERSION; CATCHMENT; STREAMS; RADON AB Few studies have investigated large reaches of rivers in which multiple sources of groundwater are responsible for maintaining baseflow. This paper builds upon previous work undertaken along the Fitzroy River, one of the largest perennial river systems in north-western Australia. Synoptic regional-scale sampling of both river water and groundwater for a suite of environmental tracers (He-4, Sr-87/Sr-86, Rn-222 and major ions), and subsequent modeling of tracer behavior in the river, has enabled definition and quantification of groundwater input from at least three different sources. We show unambiguous evidence of both shallow "local'' groundwater, possibly recharged to alluvial aquifers beneath the adjacent floodplain during recent high-flow events, and old "regional'' groundwater introduced via artesian flow from deep confined aquifers. We also invoke hyporheic exchange and either bank return flow or parafluvial flow to account for background 222Rn activities and anomalous chloride trends along river reaches where there is no evidence of the local or regional groundwater inputs. Vertical conductivity sections acquired through an airborne electromagnetic (AEM) survey provide insights to the architecture of the aquifers associated with these sources and general groundwater quality characteristics. These data indicate fresh groundwater from about 300 m below ground preferentially discharging to the river, at locations consistent with those inferred from tracer data. The results demonstrate how sampling rivers for multiple environmental tracers of different types-including stable and radioactive isotopes, dissolved gases and major ions-can significantly improve conceptualization of groundwater-surface water interaction processes, particularly when coupled with geophysical techniques in complex hydrogeological settings. C1 [Harrington, Glenn A.] Innovat Groundwater Solut, Blackwood, SA 5051, Australia. [Harrington, Glenn A.; Gardner, W. Payton; Munday, Tim J.] Commonwealth Sci & Ind Res Org, Water Healthy Country Natl Res Flagship, Adelaide, SA 5064, Australia. [Gardner, W. Payton] Sandia Natl Labs, Albuquerque, NM 87123 USA. RP Harrington, GA (reprint author), Innovat Groundwater Solut, POB 79, Blackwood, SA 5051, Australia. EM glenn@innovativegroundwater.com.au FU Tropical Rivers and Coastal Knowledge (TRaCK) research alliance through Australian Government National Water Commission's Raising National Water Standards program; CSIRO Water for a Healthy Country National Research Flagship FX We wish to acknowledge the Aboriginal traditional owners of the lower Fitzroy Valley, who supported this research and granted access to sample river water and groundwater wells on their land. We are also thankful for the field and logistic support provided by the Western Australia Department of Water, and specifically the collaboration and assistance of Louise Stelfox and Duncan Palmer. New interpretation of basement geology extents were kindly provided by Arthur Mory of the Western Australia Department of Mines and Petroleum. We are very grateful for the assistance in processing the geophysical data provided by Andrew Fitzpatrick, and spatial analysis and mapping support provided by Phil Davies and Tania Abdat of CSIRO. This work was funded in part through the Tropical Rivers and Coastal Knowledge (TRaCK) research alliance, in part through the Australian Government National Water Commission's Raising National Water Standards program, and in part by CSIRO Water for a Healthy Country National Research Flagship. Finally, we are grateful for the comments provided by two anonymous reviewers on an earlier version of this manuscript. NR 40 TC 6 Z9 6 U1 3 U2 33 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0017-467X EI 1745-6584 J9 GROUNDWATER JI Groundwater PD NOV-DEC PY 2014 VL 52 IS 6 BP 837 EP 852 DI 10.1111/gwat.12124 PG 16 WC Geosciences, Multidisciplinary; Water Resources SC Geology; Water Resources GA AZ1DM UT WOS:000347980500009 PM 24124692 ER PT J AU Peisert, S Margulies, J AF Peisert, Sean Margulies, Jonathan TI Closing the Gap on Securing Energy Sector Control Systems Introduction SO IEEE SECURITY & PRIVACY LA English DT Editorial Material C1 [Peisert, Sean] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Peisert, Sean] Univ Calif Davis, Davis, CA 95616 USA. [Margulies, Jonathan] Qmulos, Chantilly, VA 20151 USA. RP Margulies, J (reprint author), Qmulos, Chantilly, VA 20151 USA. EM jonathan@qmulos.com NR 0 TC 0 Z9 0 U1 0 U2 1 PU IEEE COMPUTER SOC PI LOS ALAMITOS PA 10662 LOS VAQUEROS CIRCLE, PO BOX 3014, LOS ALAMITOS, CA 90720-1314 USA SN 1540-7993 EI 1558-4046 J9 IEEE SECUR PRIV JI IEEE Secur. Priv. PD NOV-DEC PY 2014 VL 12 IS 6 BP 13 EP 14 PG 2 WC Computer Science, Information Systems; Computer Science, Software Engineering SC Computer Science GA AZ2JC UT WOS:000348059000003 ER PT J AU Schwartz, M Mulder, J Chavez, AR Allan, BA AF Schwartz, Moses Mulder, John Chavez, Adrian R. Allan, Benjamin A. TI Emerging Techniques for Field Device Security SO IEEE SECURITY & PRIVACY LA English DT Article AB Industrial control systems (ICSs) rely on embedded devices to control essential processes. State-of-the-art security solutions can't detect attacks on these devices at the hardware or firmware level. To improve ICS cybersecurity, defensive measures should focus on inspectability, trustworthiness, and diversity. C1 [Schwartz, Moses] Bechtel Corp, Comp Incident Response Team, San Francisco, CA 94105 USA. [Mulder, John; Chavez, Adrian R.; Allan, Benjamin A.] Sandia Natl Labs, Livermore, CA 94550 USA. RP Schwartz, M (reprint author), Bechtel Corp, Comp Incident Response Team, San Francisco, CA 94105 USA. EM moses.schwartz@gmail.com; jmulder@sandia.gov; adrchav@sandia.gov; baallan@sandia.gov NR 22 TC 0 Z9 0 U1 2 U2 4 PU IEEE COMPUTER SOC PI LOS ALAMITOS PA 10662 LOS VAQUEROS CIRCLE, PO BOX 3014, LOS ALAMITOS, CA 90720-1314 USA SN 1540-7993 EI 1558-4046 J9 IEEE SECUR PRIV JI IEEE Secur. Priv. PD NOV-DEC PY 2014 VL 12 IS 6 BP 24 EP 31 PG 8 WC Computer Science, Information Systems; Computer Science, Software Engineering SC Computer Science GA AZ2JC UT WOS:000348059000005 ER PT J AU McParland, C Peisert, S Scaglione, A AF McParland, Chuck Peisert, Sean Scaglione, Anna TI Monitoring Security of Networked Control Systems: It's the Physics SO IEEE SECURITY & PRIVACY LA English DT Article AB Physical systems must be operated safely and correctly. One way of enhancing operational safety is by leveraging specifi cation-based intrusion detection to monitor for physical constraint violations. This additional security layer enhances protection from both outsider attacks and insider mistakes. C1 [McParland, Chuck; Peisert, Sean] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Peisert, Sean; Scaglione, Anna] Univ Calif Davis, Davis, CA 95616 USA. RP McParland, C (reprint author), Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. EM cpmcparland@lbl.gov; sppeisert@lbl.gov; ascaglione@ucdavis.edu FU Office of Computational and Technology Research, Division of Mathematical, Information, and Computational Sciences of the US Department of Energy [DE-AC02-05CH11231]; National Science Foundation [CCF-1018871] FX This research was supported in part by the Director, Office of Computational and Technology Research, Division of Mathematical, Information, and Computational Sciences of the US Department of Energy, under contract DE-AC02-05CH11231. It was also supported in part by the National Science Foundation under grant CCF-1018871. Any opinions, findings, conclusions, or recommendations expressed in this article are those of the authors and do not necessarily reflect those of any of the employers or sponsors of this work. NR 17 TC 3 Z9 3 U1 0 U2 4 PU IEEE COMPUTER SOC PI LOS ALAMITOS PA 10662 LOS VAQUEROS CIRCLE, PO BOX 3014, LOS ALAMITOS, CA 90720-1314 USA SN 1540-7993 EI 1558-4046 J9 IEEE SECUR PRIV JI IEEE Secur. Priv. PD NOV-DEC PY 2014 VL 12 IS 6 BP 32 EP 39 PG 8 WC Computer Science, Information Systems; Computer Science, Software Engineering SC Computer Science GA AZ2JC UT WOS:000348059000006 ER PT J AU Peisert, S Margulies, J Byres, E Dorey, P Peterson, D Tudor, Z AF Peisert, Sean Margulies, Jonathan Byres, Eric Dorey, Paul Peterson, Dale Tudor, Zach TI Control Systems Security from the Front Lines SO IEEE SECURITY & PRIVACY LA English DT Editorial Material C1 [Peisert, Sean] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Peisert, Sean] Univ Calif Davis, Davis, CA 95616 USA. RP Peisert, S (reprint author), Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. EM sppeisert@lbl.gov; jonathan@qmulos.com; eric.byres@belden.com; paul.dorey@csoconfidential.com; peterson@digitalbond.com; zachary.tudor@sri.com NR 0 TC 0 Z9 0 U1 0 U2 1 PU IEEE COMPUTER SOC PI LOS ALAMITOS PA 10662 LOS VAQUEROS CIRCLE, PO BOX 3014, LOS ALAMITOS, CA 90720-1314 USA SN 1540-7993 EI 1558-4046 J9 IEEE SECUR PRIV JI IEEE Secur. Priv. PD NOV-DEC PY 2014 VL 12 IS 6 BP 55 EP 58 PG 4 WC Computer Science, Information Systems; Computer Science, Software Engineering SC Computer Science GA AZ2JC UT WOS:000348059000009 ER PT J AU Bauer, T Hamlet, J AF Bauer, Todd Hamlet, Jason TI Physical Unclonable Functions: A Primer SO IEEE SECURITY & PRIVACY LA English DT Article C1 [Bauer, Todd; Hamlet, Jason] Sandia Natl Labs, Livermore, CA 94550 USA. RP Bauer, T (reprint author), Sandia Natl Labs, Livermore, CA 94550 USA. EM tmbaue@sandia.gov; jrhamle@sandia.gov FU US Department of Energy's National Nuclear Security Administration [DE-AC04-94AL85000] FX Sandia National Laboratories is a multiprogram laboratory managed and operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the US Department of Energy's National Nuclear Security Administration under contract DE-AC04-94AL85000. SAND2014-19298 J. NR 26 TC 0 Z9 0 U1 1 U2 6 PU IEEE COMPUTER SOC PI LOS ALAMITOS PA 10662 LOS VAQUEROS CIRCLE, PO BOX 3014, LOS ALAMITOS, CA 90720-1314 USA SN 1540-7993 EI 1558-4046 J9 IEEE SECUR PRIV JI IEEE Secur. Priv. PD NOV-DEC PY 2014 VL 12 IS 6 BP 97 EP 101 PG 5 WC Computer Science, Information Systems; Computer Science, Software Engineering SC Computer Science GA AZ2JC UT WOS:000348059000017 ER PT J AU Mante, OD Amidon, TE Stipanovic, A Babu, SP AF Mante, Ofei D. Amidon, Thomas E. Stipanovic, Arthur Babu, Suresh P. TI Integration of biomass pretreatment with fast pyrolysis: An evaluation of electron beam (EB) irradiation and hot-water extraction (HWE) SO JOURNAL OF ANALYTICAL AND APPLIED PYROLYSIS LA English DT Article DE Biomass pretreatment; Fast pyrolysis; Hot-water extraction; Electron-beam irradiation; Bio-oil; HZSM-5; Catalytic fast pyrolysis ID BIO-OIL; PRODUCT DISTRIBUTION; LIGNOCELLULOSIC BIOMASS; THERMAL-DECOMPOSITION; ENZYMATIC-HYDROLYSIS; CRYSTALLITE SIZE; WOODY BIOMASS; TORREFACTION; CELLULOSE; TECHNOLOGIES AB Integration of biomass pretreatment with pyrolysis offers an opportunity to improve end-product quality and conversion efficiency. In this study, sugar maple (Acer saccharum) was subjected to both hot-water extraction (HWE) at 160 C (at residence times of 0.5 h, 1.0 h, and 2.0 h) and electron beam (EB) irradiation at a dose of 1000 kGy. Pyrolysis studies were then conducted on all the treated samples at 550 degrees C using a bench scale pyroprobe-gas chromatography-mass spectrometry (Py-GC/MS). The HWE samples were selected for further evaluation in catalytic pyrolysis using HZSM-5 catalysts for the production of aromatic hydrocarbons. Analysis of the hot-water treated sample at 160 degrees C for 2 h showed that HWE increased the volatile mater and decreased the fixed carbon and ash contents; also the glucan content increased by 24% and the xylan decreased by 54%. Derivative thermogravimetry (DTG) analysis indicated that EB irradiation reduced the crystallinity of the sugar based polymers while HWE solubilized the hemicellulose fraction. The pyrolysis results showed that EB irradiation increased the formation of furanic aldehydes (furfural and 5-hydroxymethylfurfural (5-HMF)) and decreased hydroxyacetaldehyde (HAA) and levoglucosan (LG). By contrast, HWE increased the yield of LG, HM, 5-HMF and furfural; but, decreased the yields of acetic acid (HAc), hydroxyacetone, and other ketones. For the HWE-2 h sample, LG formation increased from 4.45 wt.% to 11.57 wt.% and HAc decreased from 4.87 wt.% to 2.40 wt.%. Catalytic pyrolysis of HWE samples with HZSM-5 zeolite showed that the carbon yields of monoaromatic hydrocarbons increased. HWE treatment at 160 degrees C for 2 h increased the yield of benzene by 46%, toluene by 35% and xylene by 26%. Pyrolysis-TGA also indicated that HWE decreased the formation of char/coke. Overall, the reduction in the formation of acids and ketones caused by HWE suggest that it could be used to improve bio-oil quality in non-catalytic pyrolysis whilst the increase in the yield of monoaromatic hydrocarbons indicate that HWE could be used to enhance the carbon efficiency in catalytic pyrolysis. (C) 2014 Elsevier B.V. All rights reserved. C1 [Mante, Ofei D.; Babu, Suresh P.] Brookhaven Natl Lab, Dept Sustainable Energy Technol, Upton, NY 11973 USA. [Amidon, Thomas E.] SUNY Coll Environm Sci & Forestry, Dept Paper & Bioproc Engn, Syracuse, NY 13210 USA. [Stipanovic, Arthur] SUNY Coll Environm Sci & Forestry, Dept Chem, Syracuse, NY 13210 USA. RP Mante, OD (reprint author), Brookhaven Natl Lab, Dept Sustainable Energy Technol, Upton, NY 11973 USA. EM nmante@bnl.gov RI Mante, Ofei/E-8513-2014 OI Mante, Ofei/0000-0002-0960-2943 FU BNL Laboratory-Directed Research and Development Program, LDRD [12-024]; USDA [2007-35504-18341] FX The authors acknowledge funding support from the BNL Laboratory-Directed Research and Development Program, LDRD Project #12-024. Mr. Christopher Wood (SUNY-ESF) is acknowledged for performing the HWE experiments. The EB treated maple samples were prepared as part of USDA Grant number 2007-35504-18341. We thank Professor Agblevor of Utah State University for providing the catalyst used in this work. NR 37 TC 2 Z9 2 U1 7 U2 27 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0165-2370 EI 1873-250X J9 J ANAL APPL PYROL JI J. Anal. Appl. Pyrolysis PD NOV PY 2014 VL 110 BP 44 EP 54 DI 10.1016/j.jaap.2014.08.004 PG 11 WC Chemistry, Analytical; Spectroscopy SC Chemistry; Spectroscopy GA AY3QC UT WOS:000347496800006 ER PT J AU Carreras-Sospedra, M Lunden, MM Brouwer, J Singer, BC Dabdub, D AF Carreras-Sospedra, Marc Lunden, Melissa M. Brouwer, Jack Singer, Brett C. Dabdub, Donald TI Air quality impacts of liquefied natural gas in the South Coast Air Basin of California SO JOURNAL OF NATURAL GAS SCIENCE AND ENGINEERING LA English DT Article DE Air pollution; Emissions; Ozone; Aerosols; NOx; Modeling ID SECONDARY ORGANIC AEROSOL; MECHANISM; EQUILIBRIUM; MODEL AB The effects of liquefied natural gas (LNG) on pollutant emission inventories and air quality in the South Coast Air Basin (SoCAB) of California are evaluated using recent appliance emissions measurements by Lawrence Berkeley National Laboratory and the Southern California Gas Company (SoCalGas), and use of a state-of-the-art air quality model. Pollutant emissions can be impacted by LNG operation because of differences in composition and physical properties including the Wobbe index, a measure of energy delivery rate. Various LNG distribution scenarios are evaluated to determine the potential impacts of LNG. Projected penetration of LNG in the SoCalGas pipeline network in SoCAB is expected to be limited, which could cause increases in overall (area-wide) emissions of nitrogen oxides that are smaller than 0.05%. Based on the photochemical state of the South Coast Air Basin of California, any increase in NOx is expected to cause an increase in the highest local ozone concentrations, which is observed in model results. However, the magnitude of NOx emissions increases due to LNG use is determined to be within the uncertainty range of natural gas combustion sources and would not be discernible with the existing monitoring network. (C) 2014 Elsevier B.V. All rights reserved. C1 [Carreras-Sospedra, Marc; Brouwer, Jack; Dabdub, Donald] Univ Calif Irvine, Mech & Aerosp Engn Dept, Irvine, CA 92697 USA. [Lunden, Melissa M.; Singer, Brett C.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Environm Energy Technol Div, Berkeley, CA 94720 USA. RP Dabdub, D (reprint author), Univ Calif Irvine, 4226 Engn Gateway, Irvine, CA 92697 USA. EM ddabdub@uci.edu FU California Energy Commission [500-05-026] FX Direct funding of this research was provided by the California Energy Commission through Contract 500-05-026. The authors acknowledge with appreciation the following contributors to this work: Les Bamburg from Sempra LNG, Adriano Pangelian from Shell NA LNG, LLC and Kevin Shea and colleagues from Southern California Gas Company for their assistance with the liquefied natural gas delivery scenarios; members of the Project Advisory Committee (PAC) who contributed their time, knowledge, and suggestions that improved this work include Al Baez (SCAQMD), Steve Moore (San Diego APCD), and Linda Lee (ARB). NR 30 TC 1 Z9 1 U1 1 U2 8 PU ELSEVIER SCI LTD PI OXFORD PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, OXON, ENGLAND SN 1875-5100 EI 2212-3865 J9 J NAT GAS SCI ENG JI J. Nat. Gas Sci. Eng. PD NOV PY 2014 VL 21 BP 680 EP 690 DI 10.1016/j.jngse.2014.09.025 PG 11 WC Energy & Fuels; Engineering, Chemical SC Energy & Fuels; Engineering GA AY7MC UT WOS:000347743200070 ER PT J AU Davidovich, RL Tkachev, VV Logvinova, VB Stavila, V AF Davidovich, R. L. Tkachev, V. V. Logvinova, V. B. Stavila, V. TI New structure types of polymeric chain anions in the crystal structures of complex zirconium fluorides SO JOURNAL OF STRUCTURAL CHEMISTRY LA English DT Article DE complex zirconium fluoride; 4-amino-1,2,4-triazol; hydroxonium; tetraethylammonium; crystal structure; polymeric chain; pentagonal bipyramid; tetranuclear fragment ID X-RAY; PENTAFLUOROZIRCONATE; STEREOCHEMISTRY; HAFNIUM; TRANSITION AB The crystal structures of complex zirconium fluorides (C2H5N4)(2)Zr2F10 center dot H2O and (H3O)(3)(NEt4)(2)Zr4F21 center dot 3H(2)O synthesized for the first time are determined. The formation of new structure types of polymeric chain complex anions is found in them. Two crystallographically independent zigzag-like polymeric chains (a)(ZrF5)(-) composed of pentagonal bipyramidal polyhedra of Zr atoms sharing F-F edges form a polymeric chain complex anion in the (C2H5N4)(2)Zr2F10 center dot H2O structure. The polymeric chain complex anion in the (H3O)(3)(NEt4)(2)Zr4F21 center dot 3H(2)O structure is formed of tetranuclear -Zr(1)F-7-Zr(2)F-8-Zr(3)F-8-Zr(4)F-7- moieties in which Zr(2)F-8 and Zr(3)F-8 polyhedra are linked by a common thiangular face and Zr(1)F-7 and Zr(4)F-7 polyhedra are bonded to Zr(2)F-8 and Zr(3)F-8 polyhedra by common edges. In the polymeric chain of the complex [Zr4F21](5-) anion the tetranuclear fragments share edges. The structural fragments of the compounds are combined in three-dimensional units by a branched system of N-Ha <-O, N-Ha <-F, and O-Ha <-F hydrogen bonds. C1 [Davidovich, R. L.; Logvinova, V. B.] Russian Acad Sci, Inst Chem, Far Eastern Branch, Vladivostok 690022, Russia. [Tkachev, V. V.] Russian Acad Sci, Inst Problems Chem Phys, Chernogolovka 142432, Moscow Oblast, Russia. [Stavila, V.] Sandia Natl Labs, Livermore, CA USA. RP Davidovich, RL (reprint author), Russian Acad Sci, Inst Chem, Far Eastern Branch, Vladivostok 690022, Russia. EM davidovich@ich.dvo.ru NR 17 TC 3 Z9 5 U1 0 U2 2 PU MAIK NAUKA/INTERPERIODICA/SPRINGER PI NEW YORK PA 233 SPRING ST, NEW YORK, NY 10013-1578 USA SN 0022-4766 EI 1573-8779 J9 J STRUCT CHEM+ JI J. Struct. Chem. PD NOV PY 2014 VL 55 IS 6 BP 1083 EP 1090 DI 10.1134/S0022476614060110 PG 8 WC Chemistry, Inorganic & Nuclear; Chemistry, Physical SC Chemistry GA AZ7LT UT WOS:000348401200011 ER PT J AU Xu, N AF Xu, Nu CA STAR Collaboration TI An overview of STAR experimental results SO NUCLEAR PHYSICS A LA English DT Article DE Quark-gluon plasma; QCD; Energy loss; Phase transition; Critical point ID HEAVY-ION COLLISIONS; NUCLEUS-NUCLEUS COLLISIONS; QUARK-GLUON PLASMA; QUANTUM CHROMODYNAMICS; MODEL; COLLABORATION; SUPPRESSION; MATTER AB With large acceptance and excellent particle identification, STAR is one of the best mid-rapidity collider experiments for studying high-energy nuclear collisions. The STAR experiment provides full information on initial conditions, properties of the hot and dense medium as well as the properties at freeze-out. In Au+Au collisions at,root s(NN) = 200 GeV, STAR's focus is on the nature of the sQGP produced at RHIC. In order to explore the properties of the QCD phase diagram, since 2010, the experiment has collected sizable data sets of Au+Au collisions at the lower collision energy region where the net-baryon density is large. At the 2014 Quark Matter Conference, the STAR experiment made 16 presentations that cover physics topics including collective dynamics, electromagnetic probes, heavy-flavor, initial state physics, jets, QCD phase diagram, thermodynamics and hadron chemistry, and future experimental facilities, upgrades, and instrumentation [1]. In this overview we will highlight a few results from the STAR experiment, especially those from the recent measurements of the RHIC beam energy scan program. At the end, instead of a summary, we will discuss STAR's near future physics programs at RHIC. (C) 2014 Elsevier B.V. All rights reserved. C1 [Xu, Nu] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Nucl Sci, Berkeley, CA 94720 USA. [Xu, Nu] Cent China Normal Univ, Key Lab Quarks & Lepton Phys, MOE, Wuhan 430079, Peoples R China. [Xu, Nu] Cent China Normal Univ, Inst Particle Phys, Wuhan 430079, Peoples R China. RP Xu, N (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Nucl Sci, 1 Cyclotron Rd, Berkeley, CA 94720 USA. FU Office of Science, U.S. Department of Energy [DE-AC03-76SF00098]; Ministry of Science and Technology of the People's Republic of China of China 973-Project [2015CB856900]; National Natural Science Foundation of China [11221504] FX I would like to thank the STAR experiment for the opportunity to present the talk at the QM2014 conference. This work was supported in part by the Office of Science, U.S. Department of Energy under Contract No. DE-AC03-76SF00098, the Ministry of Science and Technology of the People's Republic of China of China 973-Project No. 2015CB856900 and National Natural Science Foundation of China No. 11221504. NR 69 TC 13 Z9 13 U1 3 U2 37 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 1 EP 12 DI 10.1016/j.nuclphysa.2014.10.022 PG 12 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500001 ER PT J AU Sickles, AM AF Sickles, Anne M. TI Experimental results on p(d) plus A collisions at RHIC and the LHC SO NUCLEAR PHYSICS A LA English DT Article DE Heavy-ion; p plus A ID P-PB COLLISIONS; RANGE ANGULAR-CORRELATIONS; LONG-RANGE; TRANSVERSE-MOMENTUM; ROOT-S(NN)=5.02 TEV; FLOW; HADRONS; PROTON; SIDE; KAON AB Recent experimental results at both the LHC and RHIC show evidence for hydrodynamic behavior in proton nucleus and deuteron nucleus collisions (p + A). This unexpected finding has prompted new measurements in p + A collisions in order to understand whether matter with similar properties is created in A + A and p + A collisions or whether another explanation is needed. In this proceedings, we will discuss the new experimental data and its interpretation within the context of heavy-ion collisions. (C) 2014 Elsevier B.V. All rights reserved. C1 [Sickles, Anne M.] Univ Illinois, Dept Phys, Urbana, IL 61801 USA. [Sickles, Anne M.] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. RP Sickles, AM (reprint author), Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. FU DOE [DE-AC02-98CH10886] FX I thank the organizers for providing such an enjoyable and stimulating conference. I would also like to thank all those who discussed their work with me in preparation for this talk. I would like to thank the ALICE, ATLAS, CMS, PHENIX and STAR collaborations for providing me with the material necessary to put this talk together in a timely manner. This work was supported by the DOE under contract number: DE-AC02-98CH10886. NR 44 TC 2 Z9 2 U1 2 U2 15 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 63 EP 72 DI 10.1016/j.nuclphysa.2014.09.084 PG 10 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500007 ER PT J AU Schmah, A AF Schmah, Alexander TI New physics opportunities at high baryon densities SO NUCLEAR PHYSICS A LA English DT Article DE Beam energy scan; QCD phase transition; Critical point AB Beam energy scan programs are carried out at RHIC and SPS with the goals of finding signatures for the disappearance of the QGP, a QCD phase transition, and for a critical point. In this paper an overview of various observables studied by STAR, PHENIX, and NA60 to identify those structures in the QCD phase diagram are discussed. Furthermore, an outlook on the Beam Energy Scan phase II program at RHIC, which is anticipated for the years 2018-2019, is given. (C) 2014 Elsevier B.V. All rights reserved. C1 Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. RP Schmah, A (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, 1 Cyclotron Rd,MS70-319, Berkeley, CA 94720 USA. NR 23 TC 0 Z9 0 U1 2 U2 13 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 125 EP 134 DI 10.1016/j.nuclphysa.2014.08.023 PG 10 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500013 ER PT J AU Ruan, LJ AF Ruan, Lijuan TI The low and intermediate mass dilepton and photon results SO NUCLEAR PHYSICS A LA English DT Article DE Vector meson in-medium modification; Chiral symmetry restoration; Quark-Gluon Plasma thermal radiation; Dileptons; Thermal photons ID AU COLLISIONS; STAR; RESTORATION; PROTOTYPE; PROBES; PHENIX; MATTER AB I summarize and discuss some of the experimental results on the low and intermediate mass dileptons and direct photons presented at Quark Matter 2014. (C) 2014 Elsevier B.V. All rights reserved. C1 Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. RP Ruan, LJ (reprint author), Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. EM ruanlj@rcf.rhic.bnl.gov FU U.S. Department of Energy [DE-AC02-98CH10886, 2013-BNL-PO143] FX The work of L.R. is supported in part by the U.S. Department of Energy under Contract No. DE-AC02-98CH10886 and under Early Career Research Program Funding Award No. FWP#2013-BNL-PO143. NR 48 TC 7 Z9 7 U1 3 U2 26 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 185 EP 193 DI 10.1016/j.nuclphysa.2014.10.040 PG 9 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500019 ER PT J AU Jia, JY AF Jia, Jiangyong TI Collective phenomena in high-energy nuclear collisions SO NUCLEAR PHYSICS A LA English DT Article DE Heavy-ion collisions; Fluctuations; Correlations; Collective flow; Ridge ID RANGE ANGULAR-CORRELATIONS; P-PB COLLISIONS; LONG-RANGE; ROOT-S(NN)=5.02 TEV; SIDE; PPB AB I review experimental studies of collective phenomena in p + A and A + A collisions presented in the Quark Matter 2014 conference. (C) 2014 Elsevier B.V. All rights reserved. C1 [Jia, Jiangyong] SUNY Stony Brook, Dept Chem, Stony Brook, NY 11794 USA. [Jia, Jiangyong] Brookhaven Natl Lab, Dept Phys, Upton, NY 11796 USA. RP Jia, JY (reprint author), SUNY Stony Brook, Dept Chem, Stony Brook, NY 11794 USA. FU NSF [PHY-1305037]; DOE through BNL [DE-AC02-98CH10886] FX This research is supported by NSF under grant number PHY-1305037 and by DOE through BNL under grant number DE-AC02-98CH10886. NR 49 TC 0 Z9 0 U1 1 U2 12 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 216 EP 226 DI 10.1016/j.nuclphysa.2014.08.045 PG 11 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500022 ER PT J AU Venugopalan, R AF Venugopalan, Raju TI The ridge through colored glass SO NUCLEAR PHYSICS A LA English DT Article DE Color glass condensate; Glasma; Quark-gluon plasma ID COLLISIONS AB We briefly outline the role of gluon saturation, and the interplay between initial and final state effects, in generating the ridge observed in high multiplicity proton proton and proton nucleus collisions. (C) 2014 Published by Elsevier B.V. C1 Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. RP Venugopalan, R (reprint author), Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. FU DOE [DE-AC02-98CH10886] FX This research was supported by DOE Contract No. DE-AC02-98CH10886. I thank Kevin Dusling and Bjoern Schenke for their collaboration on the topics discussed here. NR 23 TC 1 Z9 1 U1 3 U2 4 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 277 EP 282 DI 10.1016/j.nuclphysa.2014.08.071 PG 6 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500028 ER PT J AU Dusling, K Venugopalan, R AF Dusling, Kevin Venugopalan, Raju TI Azimuthal anisotropy from Color Glass Condensates in proton-nucleus collisions SO NUCLEAR PHYSICS A LA English DT Article DE Color Glass Condensate; Proton nucleus; Ridge AB We explore the detailed structure of the ridge in the Color-Glass-Condensate (CGC) effective field theory of QCD. In particular, we study multiple scattering corrections to both the jet and Glasma contributions in a self-consistent framework of dilute dense collisions. (C) 2014 Elsevier B.V. All rights reserved. C1 [Dusling, Kevin] Amer Phys Soc, Phys Review Letters, Ridge, NY 11961 USA. [Dusling, Kevin; Venugopalan, Raju] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. RP Dusling, K (reprint author), Amer Phys Soc, Phys Review Letters, 1 Res Rd, Ridge, NY 11961 USA. OI Dusling, Kevin/0000-0001-9598-0416 NR 26 TC 9 Z9 9 U1 0 U2 1 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 283 EP 287 DI 10.1016/j.nuclphysa.2014.09.024 PG 5 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500029 ER PT J AU Schenke, B Tribedy, P Venugopalan, R AF Schenke, Bjoern Tribedy, Prithwish Venugopalan, Raju TI Initial state geometry and fluctuations in deformed and asymmetric nuclear collisions in the IP-Glasma framework SO NUCLEAR PHYSICS A LA English DT Article DE Heavy ion collisions; Deformed nuclei; Particle production ID DENSITY AB The IP-Glasma model of initial conditions based on the ab initio color glass condensate framework successfully explains most of the bulk features of the global data for various systems like pd+p, p+A and A-I-A over a wide range of energies. We employ this framework to study deformed U+U collisions, asymmetric Cu+Au collisions and the effect of deformation in Au+Au collisions at RHIC. A combined study of these heavy ion systems with varying initial geometries can provide a unique opportunity to determine the origin of different sources of fluctuations that affect global observables like multiplicity and flow. We study the sensitivity of multiplicity, eccentricity and their event-by-event distributions to the details of initial state geometry. Results are compared to a two-component MC-Glauber model implementation that includes Negative-Binomial multiplicity fluctuations. We argue that the measurements of global observables for these systems at RHIC can constrain the mechanism of multi-particle production. (C) 2014 Elsevier B.V. All rights reserved. C1 [Schenke, Bjoern; Venugopalan, Raju] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. [Tribedy, Prithwish] Ctr Variable Energy Cyclotron, Kolkata 700064, India. RP Schenke, B (reprint author), Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. FU Office of Science of the US DOE [DE-AC02-05CH11231]; DOE [DE-AC02-98CH10886] FX This research used resources of NERSC, which is supported by the Office of Science of the US DOE under Contract No. DE-AC02-05CH11231, the DRONA and PRAFULLA cluster of Computer Division and the LHC grid computing centre at the Variable Energy Cyclotron Centre, supported by the Department of Atomic Energy, Government of India. B.P.S. and R.V. are supported under DOE Contract No. DE-AC02-98CH10886. NR 11 TC 0 Z9 0 U1 2 U2 3 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 288 EP 292 DI 10.1016/j.nuclphysa.2014.08.039 PG 5 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500030 ER PT J AU Wang, H AF Wang, H. CA STAR Collaboration TI Flow measurements and selection of body-body and tip tip enhanced samples in U plus U collisions at STAR SO NUCLEAR PHYSICS A LA English DT Article DE QGP; Flow AB The azimuthal anisotropy of particle production is commonly used in high-energy nuclear collisions to study the early evolution of the expanding system. The prolate shape of uranium nuclei provides the possibility to study how the initial geometry of the nuclei affects the azimuthal distributions. In this paper, the two- and four-particle cumulants, v(2){2} and v(2){4}, from U + U collisions at root s(NN) = 193 GeV and Au + Au collisions at root s(NN) = 200 GeV for inclusive charged hadrons will be presented. The STAR Zero Degree Calorimeter is used to subdivide the 0-1% centrality bin into even finer centralities. Differences were observed between the multiplicity dependence of v(2){2} for most central Au + Au and U + U collisions. It has also been demonstrated that ZDC and multiplicity in combination provide a way to select body body or tip tip enhanced samples of central U + U collisions. Comparisons to models show that an IP-Glasma model based on gluon saturation for the initial state better describes the slope of v(2){2} vs. multiplicity than the Glauber model with a standard two-component model for multiplicity. (C) 2014 Elsevier B.V. All rights reserved. C1 [Wang, H.; STAR Collaboration] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. RP Wang, H (reprint author), Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. NR 11 TC 4 Z9 4 U1 0 U2 0 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 293 EP 297 DI 10.1016/j.nuclphysa.2014.08.086 PG 5 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500031 ER PT J AU Berges, J Schenke, B Schlichting, S Venugopalan, R AF Berges, Juergen Schenke, Bjoern Schlichting, Soeren Venugopalan, Raju TI Turbulent thermalization process in high-energy heavy-ion collisions SO NUCLEAR PHYSICS A LA English DT Article DE Pre-equilibrium dynamics; Thermalization process; Wave turbulence ID NUCLEAR COLLISIONS; GLUON PRODUCTION; GLASMA; PLASMA AB We discuss the onset of the thermalization process in high-energy heavy-ion collisions from a weak-coupling perspective, using classical statistical real-time lattice simulations as a first principles tool to study the pre-equilibrium dynamics. Most remarkably, we find that the thermalization process is governed by a universal attractor, where the space time evolution of the plasma becomes independent of the initial conditions and exhibits the self-similar dynamics characteristic of wave turbulence [1]. We discuss the consequences of our weak-coupling results for the thermalization process in heavy-ion experiments and briefly comment on the use of weak-coupling techniques at larger values of the coupling. (C) 2014 Elsevier B.V. All rights reserved. C1 [Berges, Juergen] Heidelberg Univ, Inst Theoret Phys, D-69120 Heidelberg, Germany. [Berges, Juergen] GSI Helmholtzzentrum, ExtreMe Matter Inst EMMI, D-64291 Darmstadt, Germany. [Schenke, Bjoern; Schlichting, Soeren; Venugopalan, Raju] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. RP Schlichting, S (reprint author), Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. FU Office of Science of the U.S. Department of Energy [DE-ACO2-05CH11231]; German Research Foundation (DFG); DOE [DE-ACO2-98CH10886]; Brookhaven Science Associates; DOE Office of Science Early Career Award FX This research used resources of the National Energy Research Scientific Computing Center, which is supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-ACO2-05CH11231. This work was supported in part by the German Research Foundation (DFG). BPS, SS and RV are supported under DOE Contract No. DE-ACO2-98CH10886. SS gratefully acknowledges a Goldhaber Distinguished Fellowship from Brookhaven Science Associates. BPS is supported by a DOE Office of Science Early Career Award. NR 29 TC 12 Z9 12 U1 0 U2 0 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 348 EP 353 DI 10.1016/j.nuclphysa.2014.08.103 PG 6 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500041 ER PT J AU Blaizot, JP Liao, JF McLerran, L AF Blaizot, Jean-Paul Liao, Jinfeng McLerran, Larry TI Gluon transport equation in the small angle approximation and the onset of Bose-Einstein SO NUCLEAR PHYSICS A LA English DT Article DE Heavy ion collision; Quark-gluon plasma; Glasma; Thermalization; Bose-Einstein condensation ID HEAVY-ION COLLISION; THERMALIZATION; CONDENSATION AB To understand the evolution of a dense system of gluons, such as those produced in the early stages of ultra-relativistic heavy ion collisions, is an important and challenging problem. We describe the approach to thermal equilibrium using the small angle approximation for gluon scattering in a Boltzmann equation that includes the effects of Bose statistics. The role of Bose statistical factors in amplifying the rapid growth of the population of the soft modes is essential. With these factors properly taken into account, one finds that elastic scattering alone provides an efficient mechanism for populating soft modes, and in fact leads to rapid infrared local thermalization. Furthermore, recent developments suggest that high initial overpopulation plays a key role and may lead to dynamical Bose Einstein condensation. The kinetics of condensation is an interesting problem in itself. By solving the transport equation for initial conditions with a large enough initial phase-space density the equilibrium state contains a Bose condensate, and we present numerical evidence that such over-occupied systems reach the onset of Bose Einstein condensation in a finite time. It is also found that the approach to condensation is characterized by a scaling behavior. Finally we discuss a number of extensions of the present study. (C) 2014 Elsevier B.V. All rights reserved. C1 [Blaizot, Jean-Paul] CEA Saclay, CNRS, Inst Phys Theor, URA 2306, F-91191 Gif Sur Yvette, France. [Liao, Jinfeng] Indiana Univ, Dept Phys, Bloomington, IN 47408 USA. [Liao, Jinfeng] Indiana Univ, CEEM, Bloomington, IN 47408 USA. [McLerran, Larry] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. [Liao, Jinfeng; McLerran, Larry] Brookhaven Natl Lab, RIKEN, BNL Res Ctr, Upton, NY 11973 USA. [McLerran, Larry] Cent China Normal Univ, Dept Phys, Wuhan, Peoples R China. RP Liao, JF (reprint author), Indiana Univ, Dept Phys, 2401 N Milo B Sampson Lane, Bloomington, IN 47408 USA. FU European Research Council [ERC-AD-267258]; NSF [PHY-1352368]; DOE [DE-ACO2-98CH10886]; RIKEN BNL Research Center FX The research of J.P.B. is supported by the European Research Council under the Advanced Investigator Grant ERC-AD-267258. J.L. is supported by the NSF under Grant No. PHY-1352368. The research of L.M. is supported under DOE Contract No. DE-ACO2-98CH10886. J.L. also thanks RIKEN BNL Research Center for partial support. NR 23 TC 0 Z9 0 U1 0 U2 1 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 359 EP 364 DI 10.1016/j.nuclphysa.2014.10.012 PG 6 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500043 ER PT J AU Vogt, R AF Vogt, R. CA JET Collaboration TI Predictions for p plus Pb collisions at root S-NN=5 TeV: Expectations vs. data SO NUCLEAR PHYSICS A LA English DT Article DE Cold nuclear matter effects; Charged particle production; J/psi ID CGC PREDICTIONS; LHC AB Recently a compilation of predictions for charged hadron, identified light hadron, quarkonium, photon, jet and gauge boson production in p + Pb collisions at root S-NN = 5 TeV was made available [1]. Here the predictions are compared to the data so far available. (C) 2014 Elsevier B.V. All rights reserved. C1 [Vogt, R.] Lawrence Livermore Natl Lab, Div Phys, Livermore, CA 94551 USA. [Vogt, R.] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA. RP Vogt, R (reprint author), Lawrence Livermore Natl Lab, Div Phys, Livermore, CA 94551 USA. EM vogt2@llnl.gov FU U.S. Department of Energy by Lawrence Livermore National Laboratory [AC52-07NA27344]; JET Collaboration FX I thank J. Albacete, F. Arleo, A. Dumitru, H. Fujii, F. Jing, J.-P. Lansberg, Z. Lin, A. Rezaeian, C. Roland, E. Scomparin, P. Steinberg, J. Velkovska, and X.-N. Wang for comments and contributions. This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344 and supported in part by the JET Collaboration. NR 15 TC 1 Z9 1 U1 2 U2 5 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 371 EP 376 DI 10.1016/j.nuclphysa.2014.09.075 PG 6 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500045 ER PT J AU Wang, XN AF Wang, Xin-Nian CA JET Collaboration TI Quantitative extraction of the jet transport parameter from combined data at RHIC and LHC SO NUCLEAR PHYSICS A LA English DT Article DE Jet quenching; Jet transport; Parton energy loss; Quark-gluon plasma ID ROOT-S(NN)=2.76 TEV; PB COLLISIONS AB Using theoretical tools developed by the JET Collaboration in which one employs (2 + 1)D or (3 + 1)D hydrodynamic models for the bulk medium evolution and jet quenching models, the combined data on suppression of single inclusive hadron spectra at both RHIC and LHC are systematically analyzed with five different approaches to the parton energy loss. The jet transport parameter is extracted from the best fits to the data with values of (q) over cap approximate to 1.2 +/- 0.3 and 1.9 +/- 0.7 GeV2/fm in the center of the most central Au + Au collisions at root s = 200 GeV and Pb + Pb collisions at root s = 2.67 TeV, respectively, at an initial time tau(0) = 0.6 fm/c for a quark jet with an initial energy of 10 GeV/c. (C) 2014 Elsevier B.V. All rights reserved. C1 [Wang, Xin-Nian] Cent China Normal Univ, Key Lab Quark & Lepton Phys MOE, Wuhan 430079, Peoples R China. [Wang, Xin-Nian] Cent China Normal Univ, Inst Particle Phys, Wuhan 430079, Peoples R China. [Wang, Xin-Nian] Lawrence Berkeley Natl Lab, Div Nucl Sci, Berkeley, CA 94740 USA. RP Wang, XN (reprint author), Lawrence Berkeley Natl Lab, Div Nucl Sci, Mailstop 70R0319, Berkeley, CA 94740 USA. OI Wang, Xin-Nian/0000-0002-9734-9967 FU China MOST [2014DFG02050]; NSFC [11221504]; Major State Basic Research Development Program in China [2014CB845404]; U.S. DOE [DE-AC02-05CH11231] FX This work is supported by China MOST under Grant No. 2014DFG02050, the NSFC under Grant No. 11221504, the Major State Basic Research Development Program in China (No. 2014CB845404), U.S. DOE under Contract No. DE-AC02-05CH11231 and within the framework of the JET Collaboration. NR 21 TC 1 Z9 1 U1 0 U2 3 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 404 EP 409 DI 10.1016/j.nuclphysa.2014.08.100 PG 6 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500051 ER PT J AU Perepelitsa, DV AF Perepelitsa, D. V. CA ATLAS Collaboration TI Centrality and rapidity dependence of inclusive jet production in root(NN)-N-S=5.02 TeV p plus Pb collisions with the ATLAS detector SO NUCLEAR PHYSICS A LA English DT Article DE Heavy-ion physics; Nuclear parton distribution functions; Proton-nucleus collisions; Centrality AB Measurements of reconstructed jets in high-energy proton-nucleus collisions over a wide rapidity and transverse momentum range are a fundamental probe of the partonic structure of nuclei. Inclusive jet production is sensitive to the modification of parton distribution functions (PDF) in the high-density nuclear environment. Furthermore, any modification of jet production in p + A collisions has implications for understanding the strong suppression seen in central A + A collisions. The latest results on inclusive jet production in 29/nb of proton-lead collisions at 5.02 TeV with the ATLAS detector at the LHC are presented. The centrality of p + Pb events is characterized through the sum of the transverse energy in the Pb-going forward calorimeter. In minimum bias p + Pb collisions, the jet yields are seen to be consistent with calculations incorporating nuclear PDF effects. However, the jet yields in central and peripheral p + Pb collisions are found to be strongly suppressed and enhanced, respectively, relative to geometric expectations. Furthermore, the modifications at forward rapidities are seen to be consistent with a scaling in the total jet energy, suggesting that the modifications may depend on the initial kinematics of the hard parton parton scattering. (C) 2014 CERN. Published by Elsevier B.V. All rights reserved. C1 [Perepelitsa, D. V.; ATLAS Collaboration] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. RP Perepelitsa, DV (reprint author), Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. EM gvp@bnl.gov RI Fabbri, Laura/H-3442-2012 OI Fabbri, Laura/0000-0002-4002-8353 NR 10 TC 1 Z9 1 U1 0 U2 5 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 416 EP 421 DI 10.1016/j.nuclphysa.2014.10.031 PG 6 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500053 ER PT J AU Steinberg, P AF Steinberg, Peter CA Collaboration, A TI Centrality, rapidity and p(T) dependence of isolated prompt photon production in lead-lead collisions at root(NN)-N-S=2.76 TeV with the ATLAS detector at the LHC SO NUCLEAR PHYSICS A LA English DT Article DE Lead-lead collisions; Prompt photon production; Quantum chromodynamics; LHC; ATLAS experiment ID CROSS-SECTION AB The ATLAS experiment at the LHC has measured prompt photon production in root(NN)-N-S = 2.76 TeV Pb + Pb collisions using data collected in 2011 with an integrated luminosity of 0.14 nb(-1). The measurement is performed with a hermetic, longitudinally segmented calorimeter, which gives excellent spatial and energy resolution, and detailed information about the shower shape of each measured photon. Using a selection based on shower shapes and an isolation criterion gives measured purities between approximately 50-90%, depending on p(T), eta and centrality. Photon yields, scaled by the mean nuclear thickness function, are determined as a function of collision centrality, pseudorapidity (in two intervals vertical bar eta vertical bar < 1.37 and 1.52 < vertical bar eta vertical bar < 2.37) and transverse momentum (22 < p(T) < 280 GeV). The scaled yields are shown compared to expectations from JETPHOX (perturbative QCD calculations at next to leading order), as are the ratios of the forward yields to those near mid-rapidity (for 22 < p(T) < 140 GeV). The observed photon yields agree well with the predictions for proton proton within statistical and systematic uncertainties, but are unable to distinguish between these calculations and others including isospin and nuclear PDF effects. (C) 2014 CERN. Published by Elsevier B.V. All rights reserved. C1 [Steinberg, Peter; Collaboration, A] Brookhaven Natl Lab, Upton, NY 11973 USA. RP Steinberg, P (reprint author), Brookhaven Natl Lab, Upton, NY 11973 USA. NR 17 TC 0 Z9 0 U1 0 U2 2 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 422 EP 427 DI 10.1016/j.nuclphysa.2014.10.038 PG 6 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500054 ER PT J AU Zhang, XM Collaboration, A AF Zhang, Xiaoming Collaboration, A. L. I. C. E. TI K-S(0) and A production in charged particle jets in p-Pb collisions at root S-NN=5.02 TeV with ALICE SO NUCLEAR PHYSICS A LA English DT Article DE p-Pb collisions; Particle production; Jet fragmentation; Baryon anomaly ID RANGE ANGULAR-CORRELATIONS; ROOT-S(NN)=5.02 TEV; DEPENDENCE AB We study the production of K-S(0) mesons and A baryons in jets in p-Pb collisions at root(NN)-N-S = 5.02 TeV with ALICE at the LHC. The pr-differential density of the particles produced in jets is compared to the inclusive distributions and the A/K-S(0) ratio is reported in bins of multiplicity of the collisions. The hard scatterings are selected on an event-by-event basis using the anti-k(T) clustering algorithm with resolution parameter R = 0.2, 0.3 and 0.4, reconstructed from charged particles with a minimum PT,jet of 10 (or 20) GeV/c. (C) 2014 CERN. Published by Elsevier B.V. All rights reserved. C1 [Zhang, Xiaoming; Collaboration, A. L. I. C. E.] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. RP Zhang, XM (reprint author), Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA. NR 25 TC 2 Z9 2 U1 5 U2 7 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 444 EP 448 DI 10.1016/j.nuclphysa.2014.08.102 PG 5 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500058 ER PT J AU Luo, T He, YY Wang, XN Zhu, Y AF Luo, Tan He, Yayun Wang, Xin-Nian Zhu, Yan TI Jet propagation and medium excitation in a quark-gluon plasma SO NUCLEAR PHYSICS A LA English DT Article DE Jet quenching; Jet transport; Parton energy loss; Quark gluon plasma ID COLLISIONS AB We implement the complete set of elastic 2 -> 2 parton scattering processes in the Linearized Boltzmann Transport (LBT) model to study the parton propagation inside a hot quark-gluon plasma. We calculate and compare the elastic energy loss and the transverse momentum distribution of quarks and gluons. We further simulate a single jet propagation and the induced medium excitation within a static quark-gluon plasma to study how the jet energy and profiles are modified by the jet-medium interaction and in particular the jet-induced wake. Effects of the recoiled thermal partons and the jet-induced wake on the jet energy loss and profiles are studied in detail. (C) 2014 Elsevier B.V. All rights reserved. C1 [Luo, Tan; He, Yayun; Wang, Xin-Nian] Cent China Normal Univ, Key Lab Quark & Lepton Phys MOE, Wuhan 430079, Peoples R China. [Luo, Tan; He, Yayun; Wang, Xin-Nian] Cent China Normal Univ, Inst Particle Phys, Wuhan 430079, Peoples R China. [Wang, Xin-Nian] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Nucl Sci, Berkeley, CA 94720 USA. [Zhu, Yan] Univ Santiago de Compostela, Dept Fis Particulas, E-15706 Santiago, Spain. [Zhu, Yan] Univ Santiago de Compostela, IGFAE, E-15706 Santiago, Spain. RP Luo, T (reprint author), Cent China Normal Univ, Key Lab Quark & Lepton Phys MOE, Wuhan 430079, Peoples R China. OI Wang, Xin-Nian/0000-0002-9734-9967 FU NSFC [11221504]; China MOST [2014DFG02050]; Major State Basic Research Development Program in China [2014CB845404]; U.S. DOE [DE-ACO2-05CH11231] FX This work is supported by the NSFC under Grant No. 11221504, China MOST under Grant No. 2014DFG02050, the Major State Basic Research Development Program in China (No. 2014CB845404), U.S. DOE under Contract No. DE-ACO2-05CH11231 and within the framework of the JET Collaboration. NR 15 TC 0 Z9 0 U1 0 U2 0 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 460 EP 464 DI 10.1016/j.nuclphysa.2014.08.090 PG 5 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500061 ER PT J AU Xing, HX Kang, ZB Wang, E Wang, XN AF Xing, Hongxi Kang, Zhong-Bo Wang, Enke Wang, Xin-Nian TI Transverse momentum broadening at NLO and QCD evolution of (q)over-cap SO NUCLEAR PHYSICS A LA English DT Article DE QCD factorization; Multiple scattering; Transverse momentum broadening ID PARTON ENERGY-LOSS; SCATTERING; NUCLEI AB Within the framework of a high-twist approach, we show the first complete next-to-leading order calculation of transverse momentum broadening in semi-inclusive deeply inelastic e + A scattering and Drell-Yan dilepton production in p + A collisions. We demonstrate at one-loop level how QCD factorization holds for multiple scattering in a nuclear medium, and the universality of the associated quark-gluon correlation function. Our calculation also identifies a QCD evolution equation for the quark-gluon correlation function, which determines the QCD factorization scale and the energy dependence of the jet transport parameter (q) over cap. Published by Elsevier B.V. C1 [Xing, Hongxi; Kang, Zhong-Bo] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA. [Wang, Enke; Wang, Xin-Nian] Cent China Normal Univ, Inst Particle Phys, Wuhan 430079, Peoples R China. [Wang, Enke; Wang, Xin-Nian] Cent China Normal Univ, Key Lepton & Quark Phys MOE, Wuhan 430079, Peoples R China. [Wang, Xin-Nian] Los Alamos Natl Lab, Div Nucl Sci, Los Alamos, NM 87545 USA. RP Xing, HX (reprint author), Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA. RI Kang, Zhongbo/P-3645-2014 FU U.S. DOE [DE-AC52-06NA25396, DE-AC02-05CH11231]; Major State Basic Research Development Program (MSBRDP) in China [2014CB845404]; NSFC [11221504, 10825523]; China MOST [2014DFG02050]; LDRD program at LANL FX This work is supported by U.S. DOE under Contract No. DE-AC52-06NA25396 and No. DE-AC02-05CH11231, and within the framework of the JET Collaboration, the Major State Basic Research Development Program (MSBRDP) in China (No. 2014CB845404), and the NSFC under Grants No. 11221504 and No. 10825523, and China MOST under Grant No. 2014DFG02050, and LDRD program at LANL. NR 15 TC 4 Z9 4 U1 0 U2 3 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 493 EP 498 DI 10.1016/j.nuclphysa.2014.10.030 PG 6 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500067 ER PT J AU Zha, WM AF Zha, Wangmei CA STAR Collaboration TI Recent measurements of quarkonium production in p plus p and A plus A collisions from the STAR experiment SO NUCLEAR PHYSICS A LA English DT Article DE Heavy-ion collisions; Quark-gluon plasma; Quarkonium production ID UPSILON-PRODUCTION; J/PSI PRODUCTION; AU COLLISIONS; J-PSI; SUPPRESSION AB We report the measurements by the STAR Collaboration of J/psi invariant yields as a function of transverse momentum at mid-rapidity (vertical bar y vertical bar < 1.0) in p + p collisions at root S = 500 GeV, in Au + Au collisions at root S-NN = 39, 62.4 and 200 GeV, and in U + U collisions at root S-NN = 193 GeV. The centrality, beam energy and collision system dependences of J/psi production and nuclear modification factors are discussed. We also report the ratio of psi (2S) to J/psi yields in p + p collisions at root S = 500 GeV and Upsilon production in U + U collisions at root S-NN = 193 GeV. (C) 2014 Elsevier B.V. All rights reserved. C1 [Zha, Wangmei] Univ Sci & Technol China, Dept Modem Phys, Hefei, Anhui, Peoples R China. [Zha, Wangmei] Brookhaven Natl Lab, Upton, NY 11973 USA. RP Zha, WM (reprint author), Univ Sci & Technol China, Dept Modem Phys, Hefei, Anhui, Peoples R China. NR 22 TC 7 Z9 7 U1 0 U2 6 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 596 EP 600 DI 10.1016/j.nuclphysa.2014.08.087 PG 5 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500086 ER PT J AU Durham, JM AF Durham, J. Matthew CA PHENIX Collaboration TI The fate of the weakly-bound psi(2s) in nuclear matter SO NUCLEAR PHYSICS A LA English DT Article DE Charmonia; FVTX; PHENIX ID J/PSI; SUPPRESSION; COLLISIONS; DETECTOR; PHENIX; PSI' AB We present new results of a completed PHENIX analysis of psi(2s) modification at midrapidity in 200 GeV d + Au collisions. Strong suppression of the psi(2s) relative to the J/psi is observed. This difference in suppression is too strong to be explained by breakup effects in the nucleus, due to the short nuclear crossing times at RHIC. Given the observation of long range correlations in p(d) + A collisions at LHC and RHIC, consistent with hydrodynamics, these observations raise interesting questions about the mechanism of psi (2s) suppression when it is produced in a nuclear target. In 2012, the PHENIX Collaboration installed the FVTX, a silicon tracker that precisely measures muon pair opening angles prior to any multiple scattering in the muon arm absorber, and thus provides an improved dimuon mass resolution. The FVTX allows the psi(2s) to be separated from the J/psi at forward and backward rapidity for the first time at RHIC. We present new results on psi(2s) production in p + p collisions at root s = 510 GeV from the 2013 data set. Published by Elsevier B.V. C1 [Durham, J. Matthew; PHENIX Collaboration] Los Alamos Natl Lab, Los Alamos, NM 87545 USA. RP Durham, JM (reprint author), Los Alamos Natl Lab, POB 1663, Los Alamos, NM 87545 USA. OI Durham, J. Matthew/0000-0002-5831-3398 NR 17 TC 0 Z9 0 U1 0 U2 4 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 622 EP 627 DI 10.1016/j.nuclphysa.2014.08.079 PG 6 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500091 ER PT J AU da Silva, CL AF da Silva, Cesar Luiz CA PHENIX Collaboration TI J/psi and Upsilon nuclear modification in A plus A collisions SO NUCLEAR PHYSICS A LA English DT Article DE Quarkonia; Heavy ion AB PHENIX presents new nuclear modification results on J/psi in Cu+Au and U+U collisions. The recently completed analysis of the modification of J/psi production in Cu+Au collisions at forward (1.2 < y < 2.2) and backward (-2.2 < y < 1.2) rapidity is the first measurement of the rapidity dependence of the J/psi modification in unequal mass heavy ion collisions. Both hot and CNM effects are expected to be asymmetric in rapidity in these collisions. The comparison of d+Au, Au+Au, U+U and Cu+Au J/psi modifications across rapidities provides insight on the balance of cold and hot nuclear matter effects. We also present new PHENIX results on Upsilon(1S+2S+3S) production in p+p and centrality dependence in Au+Au collisions. These results are consistent with significant suppression of the 2S and 3S states in the Quark-Gluon Plasma (QGP) environment. Published by Elsevier B.V. C1 [da Silva, Cesar Luiz; PHENIX Collaboration] Los Alamos Natl Lab, Los Alamos, NM 87544 USA. RP da Silva, CL (reprint author), Los Alamos Natl Lab, POB 1663-H846, Los Alamos, NM 87544 USA. NR 10 TC 1 Z9 1 U1 0 U2 3 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 638 EP 642 DI 10.1016/j.nuclphysa.2014.09.008 PG 5 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500094 ER PT J AU Zhou, K Xu, N Zhuang, PF AF Zhou, Kai Xu, Nu Zhuang, Pengfei TI Upsilon production in heavy ion collisions at LHC SO NUCLEAR PHYSICS A LA English DT Article DE Quarkonia; Heavy ion collisions; Heavy quark potential ID SUPPRESSION; TEV AB We investigate the Upsilon production in heavy ion collisions at LHC energy in the frame of a dynamical transport approach. Both the initial production and in-medium regeneration and both the cold and hot nuclear matter effects are included in the calculations. In comparison with the ground state Upsilon (1s), the excited state Upsilon(2s) is much more sensitive to the heavy quark potential at finite temperature. (C) 2014 Elsevier B.V. All rights reserved. C1 [Zhou, Kai; Zhuang, Pengfei] Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China. [Zhou, Kai; Zhuang, Pengfei] Collaborat Innovat Ctr Quantum Matter, Beijing 100084, Peoples R China. [Xu, Nu] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Nucl Sci, Berkeley, CA 94720 USA. [Zhuang, Pengfei] Cent China Normal Univ, Key Lab Quark & Lepton Phys MOE, Wuhan 430079, Peoples R China. [Zhuang, Pengfei] Cent China Normal Univ, Inst Particle Phys, Wuhan 430079, Peoples R China. RP Zhou, K (reprint author), Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China. FU NSFC; MOST; DOE [11335005, 2013CB922000, 2014CB845400, DE-AC03-76SF00098] FX The work is supported by the NSFC, the MOST, and the DOE grant Nos. 11335005, 2013CB922000, 2014CB845400, and DE-AC03-76SF00098. NR 20 TC 0 Z9 0 U1 0 U2 0 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 654 EP 658 DI 10.1016/j.nuclphysa.2014.08.104 PG 5 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500097 ER PT J AU Huck, P AF Huck, Patrick CA STAR Collaboration TI Beam energy dependence of dielectron production in Au plus Au collisions from STAR at RHIC SO NUCLEAR PHYSICS A LA English DT Article DE Dielectron production; Beam energy scan; LMR enhancement; Vector meson in-medium modifications ID QUARK-GLUON PLASMA; TRANSVERSE-MOMENTUM; COLLABORATION; PERSPECTIVE; PROTON; PAIRS AB We present the energy-dependent study of dielectron production in 0-80% minimum-bias Au+Au collisions at root S-NN of 19.6, 27, 39, and 62.4 GeV in STAR. Invariant mass (M-ee) and transverse momentum (P-T) differential measurements of dielectron yields are compared to cocktail simulations of known hadronic sources and semi-leptonic charmed decays. The enhancement (excess yield) prominent in the Low-Mass Region (LMR) over the cocktail at all energies, is further compared to calculations of rho in-medium modifications. Within statistical and systematic uncertainties, we find that the model consistently describes this enhancement from SPS up to top RHIC energies in its M-ee- as well as P-T-dependence. Dielectron measurements drive the statistics for the future BES Phase-II program, which promises to improve our understanding of the LMR enhancement's trend with total baryon densities. (C) 2014 Elsevier B.V. All rights reserved. C1 [Huck, Patrick] HZNU, Cent China Normal Univ, Wuhan 430079, Peoples R China. [Huck, Patrick] Goethe Univ Frankfurt, D-60438 Frankfurt, Germany. [Huck, Patrick] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. RP Huck, P (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. NR 31 TC 11 Z9 11 U1 2 U2 17 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 659 EP 664 DI 10.1016/j.nuclphysa.2014.09.090 PG 6 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500098 ER PT J AU Hidaka, Y Lin, S Pisarski, RD Satow, D Skokov, VV AF Hidaka, Yoshimasa Lin, Shu Pisarski, Robert D. Satow, Daisuke Skokov, Vladimir V. TI Production of dilepton/photon in semi-quark gluon plasma SO NUCLEAR PHYSICS A LA English DT Article DE Semi-QGP; Polyakov loop; Electromagnetic radiation; Elliptic flow ID PHOTONS AB We consider the production of dilepton/photon in deconfined Quark Gluon Plasma (QGP). In the region of semi-QGP, effective color degrees of freedom are suppressed by a small value of the Polyakov loop. We find that the effect of the Polyakov loop leads to modest enhancement in the dilepton production rate but strong suppression in the photon production rate. The suppression of photon production in the QGP phase offers a possible explanation to the puzzle of photon elliptic flow. (C) 2014 Elsevier B.V. All rights reserved. C1 [Hidaka, Yoshimasa; Satow, Daisuke] RIKEN, Nishina Ctr, Theoret Res Div, Wako, Saitama 3510198, Japan. [Lin, Shu; Pisarski, Robert D.] Brookhaven Natl Lab, RIKEN BNL Res Ctr, Upton, NY 11973 USA. [Pisarski, Robert D.; Satow, Daisuke] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. [Skokov, Vladimir V.] Western Michigan Univ, Dept Phys, Kalamazoo, MI 49008 USA. RP Lin, S (reprint author), Brookhaven Natl Lab, RIKEN BNL Res Ctr, Upton, NY 11973 USA. OI Skokov, Vladimir/0000-0001-7619-1796 FU RIKEN Foreign Postdoctoral Researchers Program; US Department of Energy [DE-AC02-98CH10886]; JSPS [R2411] FX S.L. is supported by the RIKEN Foreign Postdoctoral Researchers Program. R.D.P. is supported by the US Department of Energy under contract #DE-AC02-98CH10886. D.S. is supported by JSPS Strategic Young Researcher Overseas Visits Program for Accelerating Brain Circulation (No. R2411). NR 12 TC 4 Z9 4 U1 0 U2 0 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 681 EP 685 DI 10.1016/j.nuclphysa.2014.10.014 PG 5 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500102 ER PT J AU Yang, C AF Yang, Chi CA STAR Collaboration TI Direct photon production in Au plus Au collisions at root S-NN=200 GeV at STAR SO NUCLEAR PHYSICS A LA English DT Article DE Dielectron; Direct photon; Thermal radiation; Quark-gluon plasma (QGP) AB We present the direct photon production for 1 < P-T < 10 GeV/c derived from continuum in the dielecton invariant mass region 0.1 < M-ee < 0.3 GeV/c(2) from one billion root S-NN = 200 GeV Au + Au events taken in years 2010 and 2011. A clear excess in the invariant yield compared to the number of binary collision scaled p + p reference is observed in the P-T range 1-4 GeV/c. Model calculations with contributions from thermal radiation and initial hard parton scattering are consistent within uncertainties with the direct photon invariant yield. (C) 2014 Elsevier B.V. All rights reserved. C1 [Yang, Chi] Univ Sci & Technol China, Dept Modern Phys, Hefei 230026, Anhui, Peoples R China. [Yang, Chi] Brookhaven Natl Lab, Upton, NY 11973 USA. RP Yang, C (reprint author), Univ Sci & Technol China, Dept Modern Phys, Hefei 230026, Anhui, Peoples R China. NR 19 TC 7 Z9 7 U1 0 U2 13 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 691 EP 695 DI 10.1016/j.nuclphysa.2014.08.042 PG 5 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500104 ER PT J AU Vujanovic, G Paquet, JF Denicol, GS Luzum, M Schenke, B Jeon, S Gale, C AF Vujanovic, Gojko Paquet, Jean-Francois Denicol, Gabriel S. Luzum, Matthew Schenke, Bjoern Jeon, Sangyong Gale, Charles TI Probing the non-equilibrium dynamics of hot and dense QCD with dileptons SO NUCLEAR PHYSICS A LA English DT Article DE Shear relaxation time; Temperature dependent shear viscosity; Out-of-equilibrium initial conditions; Dilepton azimuthal momentum anisotropy; Relativistic viscous hydrodynamics ID THERMODYNAMICS AB It is argued that, in heavy ion collisions, thermal dileptons are good probes of the transport properties of the medium created in such events, and also of its early-time dynamics, usually inaccessible to hadronic observables. In this work we show that electromagnetic azimuthal momentum anisotropies do not only display a sensitivity to the shear relaxation time and to the initial shear-stress tensor profile, but also to the temperature dependence of the shear viscosity coefficient. (C) 2014 Elsevier B.V. All rights reserved. C1 [Vujanovic, Gojko; Paquet, Jean-Francois; Denicol, Gabriel S.; Luzum, Matthew; Jeon, Sangyong; Gale, Charles] McGill Univ, Dept Phys, Montreal, PQ H3A 2T8, Canada. [Luzum, Matthew] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Schenke, Bjoern] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. RP Vujanovic, G (reprint author), McGill Univ, Dept Phys, 3600 Rue Univ, Montreal, PQ H3A 2T8, Canada. RI Luzum, Matthew/C-4986-2015; Silveira Denicol, Gabriel/L-5048-2016 OI Luzum, Matthew/0000-0002-0367-7055; FU Natural Sciences and Engineering Research Council of Canada; U.S. DOE [DE-AC02-98CH10886]; Office of Energy Research, Office of High Energy and Nuclear Physics, Division of Nuclear Physics of the U.S. Department of Energy [DE-AC02-05CH11231]; Canadian Institute for Nuclear Physics; Banting Fellowship from Government of Canada; Canada Foundation for Innovation (CFI); National Science and Engineering Research Council (NSERC); Nano Quebec; Fonds Quebecois de Recherche sur la Nature et les Technologies (FQRNT) FX This work was supported in part by the Natural Sciences and Engineering Research Council of Canada, in part by U.S. DOE Contract No. DE-AC02-98CH10886, and in part by the Director, Office of Energy Research, Office of High Energy and Nuclear Physics, Division of Nuclear Physics, of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. G. Vujanovic acknowledges support by the Canadian Institute for Nuclear Physics, and G.S. Denicol acknowledges support through a Banting Fellowship from the Government of Canada. Computations were performed on the Guillimin supercomputer at McGill University under the auspices of Calcul Quebec and Compute Canada. The operation of Guillimin is funded by the Canada Foundation for Innovation (CFI), the National Science and Engineering Research Council (NSERC), Nano Quebec, and the Fonds Quebecois de Recherche sur la Nature et les Technologies (FQRNT). NR 7 TC 3 Z9 3 U1 0 U2 0 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 701 EP 705 DI 10.1016/j.nuclphysa.2014.08.078 PG 5 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500106 ER PT J AU Loshaj, F Kharzeev, DE AF Loshaj, Frasher Kharzeev, Dmitri E. TI Soft photon production from real-time dynamics of jet fragmentation SO NUCLEAR PHYSICS A LA English DT Article DE Soft photon production; Jet fragmentation; Quark-gluon plasma; Schwinger model ID SINE-GORDON EQUATION; 280 GEV/C; HADRONIC-INTERACTIONS; PI(-)P INTERACTIONS; QUARK CONFINEMENT; QED EXPECTATIONS; EXCESS; COLLISIONS; BREMSSTRAHLUNG; VACUUM AB Soft photons produced in heavy ion collisions are an important tool for probing the properties of the quark-gluon plasma. It is therefore crucial to understand the background soft photons produced in elementary collisions. Low theorem states that soft photon production in hadron collisions is dominated by Bremsstrahlung off charged initial and final state hadrons. Surprisingly, almost every experiment observed an enhancement (by a factor of 2-5) above Low theorem's prediction. This is the longstanding puzzle of "anomalous soft photon production." The phenomenon is not observed in processes with leptonic final states, which suggests that the mechanism is due to nonperturbative QCD evolution. We study this phenomenon using an exactly soluble, massless, Abelian model in 1 + 1 dimensions which shares with QCD many important properties: confinement, chiral symmetry breaking, axial anomaly and theta-vacuum. We then apply this model to the soft photon production in the fragmentation of jets produced in Z(0) decays and find a qualitative agreement with the data. (C) 2014 Elsevier B.V. All rights reserved. C1 [Loshaj, Frasher; Kharzeev, Dmitri E.] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA. [Kharzeev, Dmitri E.] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. RP Loshaj, F (reprint author), SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA. FU U.S. Department of Energy [DE-FG-88ER40388, DE-AC02-98CH10886] FX This work was supported by the U.S. Department of Energy under Contracts No. DE-FG-88ER40388 and No. DE-AC02-98CH10886. NR 30 TC 0 Z9 0 U1 0 U2 1 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 712 EP 717 DI 10.1016/j.nuclphysa.2014.08.006 PG 6 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500108 ER PT J AU Huovinen, P Petreczky, P Schmidt, C AF Huovinen, Pasi Petreczky, Peter Schmidt, Christian TI Equation of state at finite net-baryon density using Taylor coefficients up to sixth order SO NUCLEAR PHYSICS A LA English DT Article DE Lattice QCD; Equation of state; Hadron resonance gas ID QCD AB We employ the lattice QCD data on Taylor expansion coefficients up to sixth order to construct an equation of state at finite net-baryon density. When we take into account how hadron masses depend on lattice spacing and quark mass, the coefficients evaluated using the p4 action are equal to those of hadron resonance gas at low temperature. Thus the parametrised equation of state can be smoothly connected to the hadron resonance gas equation of state. We see that the equation of state using Taylor coefficients up to second order is realistic only at low densities, and that at densities corresponding to s/n(B) greater than or similar to 40, the expansion converges by the sixth order term. (C) 2014 Elsevier B.V. All rights reserved. C1 [Huovinen, Pasi] Goethe Univ Frankfurt, Inst Theoret Phys, D-60438 Frankfurt, Germany. [Huovinen, Pasi] Frankfurt Inst Adv Studies, D-60438 Frankfurt, Germany. [Petreczky, Peter] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. [Schmidt, Christian] Univ Bielefeld, Fak Phys, D-33615 Bielefeld, Germany. RP Huovinen, P (reprint author), Goethe Univ Frankfurt, Inst Theoret Phys, D-60438 Frankfurt, Germany. OI Schmidt, Christian/0000-0002-9071-4757 FU BMBF [06FY9092]; U.S. Department of Energy [DE-AC02-98CH1086] FX This work was supported by BMBF under contract No. 06FY9092, and by the U.S. Department of Energy under contract DE-AC02-98CH1086. NR 12 TC 2 Z9 2 U1 0 U2 0 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 769 EP 773 DI 10.1016/j.nuclphysa.2014.08.069 PG 5 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500118 ER PT J AU Soltz, RA AF Soltz, R. A. CA PHENIX Collaboration TI PHENIX beam energy scan results SO NUCLEAR PHYSICS A LA English DT Article DE Multiplicity; Femtoscopy; Quark-gluon plasma AB We present results from the PHENIX Experiment for Au+Au collisions with root S-NN = 7.9, 19.6, 27, 39, 62, and 200 GeV. Measurements of the charged particle multiplicity at central rapidity scale linearly with the number of participant quarks for root S-NN = 62 GeV and above; for root S-NN = 27 GeV and below the multiplicity scales with the number of participant nucleons. For the HBT radii we perform a linear interpolation for radii from PHENIX, STAR, and ALICE to a m(T) = 0.26 GeV and calculate ratios and differences in quadrature at this value of the transverse mass. We observe a non-monotonic behavior near root S-NN = 19 GeV in the form of a peak in R-o(2) - R-s(2) and a dip in (R-s -root 2 (R) over bar)/R-l. (C) 2014 Elsevier B.V. All rights reserved. C1 [Soltz, R. A.; PHENIX Collaboration] Lawrence Livermore Natl Lab, Div Phys, Livermore, CA 94550 USA. RP Soltz, RA (reprint author), Lawrence Livermore Natl Lab, Div Phys, Livermore, CA 94550 USA. FU U.S. Department of Energy, Office of Science, Office of Nuclear Physics [DE-AC52-07NA27344] FX This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under contract number DE-AC52-07NA27344. NR 9 TC 3 Z9 3 U1 0 U2 2 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 780 EP 784 DI 10.1016/j.nuclphysa.2014.08.050 PG 5 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500120 ER PT J AU Luo, XF Mohanty, B Xu, N AF Luo, Xiaofeng Mohanty, Bedangadas Xu, Nu TI Baseline for the cumulants of net-proton distributions at STAR SO NUCLEAR PHYSICS A LA English DT Article DE QCD critical point; Higher moments; Net-proton; Heavy-ion collision; Quantum chromodynamics ID PHASE-DIAGRAM AB We present a systematic comparison between the recently measured cumulants of the net-proton distributions by STAR for 0-5% central Au + Au collisions at root S-NN = 7.7-200 GeV and two kinds of possible baseline measure, the Poisson and Binomial baselines. These baseline measures are assuming that the proton and anti-proton distributions independently follow Poisson statistics or Binomial statistics. The higher order cumulant net-proton data are observed to deviate from all the baseline measures studied at 19.6 and 27 GeV. We also compare the net-proton with net-baryon fluctuations in UrQMD and AMPT model, and convert the net-proton fluctuations to net-baryon fluctuations in AMPT model by using a set of formula. (C) 2014 Elsevier B.V. All rights reserved. C1 [Luo, Xiaofeng; Xu, Nu] Cent China Normal Univ, Inst Particle Phys, Wuhan 430079, Peoples R China. [Luo, Xiaofeng; Xu, Nu] Cent China Normal Univ, Key Lab Quark & Lepton Phys, MOE, Wuhan 430079, Peoples R China. [Mohanty, Bedangadas] Natl Inst Sci Educ & Res, Sch Phys Sci, Bhubaneswar 751005, Orissa, India. [Xu, Nu] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Nucl Sci, Berkeley, CA 94720 USA. RP Luo, XF (reprint author), Cent China Normal Univ, Inst Particle Phys, Wuhan 430079, Peoples R China. EM xfluo@mail.ccnu.edu.cn OI Luo, Xiaofeng/0000-0002-4919-303X FU National Key Basic Research Program [2015CB856900]; NSFC [11205067, 11221504, 11228513]; China Post-doctoral Science Foundation [2012M511237, 2013T60732] FX The work was supported in part by the National Key Basic Research Program (2015CB856900), NSFC under grant Nos. 11205067, 11221504 and 11228513, China Post-doctoral Science Foundation (2012M511237, 2013T60732). NR 25 TC 8 Z9 8 U1 0 U2 4 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 808 EP 813 DI 10.1016/j.nuclphysa.2014.08.105 PG 6 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500125 ER PT J AU Debbe, RR AF Debbe, R. R. CA ATLAS Collaboration TI Measurement of the centrality dependence of charged particle pseudorapidity distribution in proton-lead collisions at root S-NN=5.02 TeV with the ATLAS detector SO NUCLEAR PHYSICS A LA English DT Article DE Multiplicity; Centrality; p plus A collisions ID NUCLEAR COLLISIONS AB Multiplicity distributions of charged particles as a function of pseudorapidity dN(ch)/d eta have been measured by the ATLAS Collaboration in p + Pb collisions at root S-NN = 5.02 TeV at the LHC. The multiplicity of charged particles was measured in vertical bar eta vertical bar < 2.7 using combinations of correlated space points into track-lets in the Pixel detector. These measurements are presented as a function of the centrality of the collision defined by forward energy deposited in 3.1 < eta < 4.9 and three Glauber type Monte-Carlo simulations of the collisions. The measured multiplicity distributions have similar shapes as the ones measured at RHIC in d + Au collisions. (C) 2014 CERN. Published by Elsevier B.V. All rights reserved. C1 [Debbe, R. R.; ATLAS Collaboration] Brookhaven Natl Lab, Upton, NY 11973 USA. RP Debbe, RR (reprint author), Brookhaven Natl Lab, Upton, NY 11973 USA. RI Pacheco Pages, Andres/C-5353-2011; Fabbri, Laura/H-3442-2012 OI Pacheco Pages, Andres/0000-0001-8210-1734; Fabbri, Laura/0000-0002-4002-8353 NR 12 TC 3 Z9 3 U1 0 U2 4 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 872 EP 876 DI 10.1016/j.nuclphysa.2014.08.025 PG 5 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500137 ER PT J AU Tannenbaum, MJ AF Tannenbaum, M. J. CA PHENIX Collaboration TI Transverse energy (E-T) distributions at mid-rapidity in p plus p, d plus Au and Au plus Au collisions at root S-NN=200 GeV and implications for particle production models SO NUCLEAR PHYSICS A LA English DT Article DE Transverse energy; Constituent-quarks; RHIC ID NUCLEUS-NUCLEUS COLLISIONS; CERN-ISR; CENTRALITY DEPENDENCE; ALPHA-ALPHA; SPECTRA; MULTIPLICITY; PROTON AB Measurements of the mid-rapidity transverse energy distribution dE(T)/d eta are presented for p+p, d+Au, and Au+Au collisions at root S-NN = 62.4-200 GeV. The E-T distributions are compared with the number of participants, N-part, the number of constituent-quark participants, N-qp, and the number of color-strings (Additive Quark Model - AQM) calculated from a Glauber model. For Au+Au, < dE(T)/d eta >/(0.5N(part)) increases with N-part, while < dE(T)/d eta >/N-qp is approximately constant vs. centrality for root S-NN >= 62.4 GeV. This indicates that the two component ansatz, dE(T)(AA)/d eta = (dE(T)(PP)/d eta)[(1-x)N-part/2 + xN(coll)], which has been used to represent E-T distributions, is simply a proxy for N-qp, and that the N-coll term does not represent a hard-scattering component in E-T distributions. The dE(T)/d eta distributions of d+Au, and Au+Au are calculated from the measured p+p E-T distribution using two models (AQM and N-qp) that both reproduce the Au+Au data. For the asymmetric d+Au system, the N-qp model reproduces the data while the AQM does not. (C) 2014 Elsevier B.V. All rights reserved. C1 [Tannenbaum, M. J.; PHENIX Collaboration] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. RP Tannenbaum, MJ (reprint author), Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. OI Tannenbaum, Michael/0000-0002-8840-5314 NR 22 TC 0 Z9 0 U1 0 U2 3 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 877 EP 882 DI 10.1016/j.nuclphysa.2014.07.048 PG 6 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500138 ER PT J AU Campbell, S AF Campbell, Sarah CA PHENIX Collaboration TI Spectra of identified particles, geometry categorization and bias and global observables in d plus Au collisions SO NUCLEAR PHYSICS A LA English DT Article DE Centrality; Auto-correlation bias; Identified particles; High p(T); d plus Au ID PHENIX AB Geometry selection in d + Au/p + Pb collisions is crucial for understanding the physics underlying modified nuclear parton distribution functions, gluon saturation or shadowing, initial state energy loss, and possible hydrodynamic flow in these small systems. The PHENIX Collaboration tests for auto-correlation biases in the geometry determination in small collision systems. These biases are well understood and an order of magnitude smaller at RHIC as compared to the LHC. As a result, auto-correlation biases are unable to describe the suppression of high transverse momentum (p(T)) pi(0)'s seen in the ratio of central-to-peripheral d + Au collisions. The centrality dependent d Au pion, kaon and proton yields relative to binary collision-scaled p + p yields are also reported, including the high p(T) pi(0) and K-S(0). At intermediate p(T) between 2 and 5 GeV/c, baryons are enhanced in central d + Au collisions. The baryon enhancement is present in d + Au and Au + Au collisions and increases with centrality. We compare identified particle yields in peripheral Au Au collisions to central d + Au collisions that have a comparable number of participants and binary collisions. The p(T) dependence of this ratio is strikingly similar for mesons and baryons. (C) 2014 Elsevier B.V. All rights reserved. C1 [Campbell, Sarah; PHENIX Collaboration] PHENIX, Brookhaven Natl Lab, Upton, NY 11973 USA. RP Campbell, S (reprint author), PHENIX, Brookhaven Natl Lab, Bldg 510C, Upton, NY 11973 USA. OI Campbell, Sarah/0000-0001-6717-9744 NR 10 TC 0 Z9 0 U1 0 U2 2 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 893 EP 898 DI 10.1016/j.nuclphysa.2014.08.075 PG 6 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500141 ER PT J AU Rose, JB Paquet, JF Denicol, GS Luzum, M Schenke, B Jeon, S Gale, C AF Rose, Jean-Bernard Paquet, Jean-Francois Denicol, Gabriel S. Luzum, Matthew Schenke, Bjoem Jeon, Sangyong Gale, Charles TI Extracting the bulk viscosity of the quark-gluon plasma SO NUCLEAR PHYSICS A LA English DT Article DE Quark-gluon plasma; Bulk viscosity; Ultracentral relativistic heavy ion collisions AB We investigate the implications of a nonzero bulk viscosity coefficient on the azimuthal momentum anisotropy of ultracentral relativistic heavy ion collisions at the Large Hadron Collider. We find that, with IP-Glasma initial conditions, a finite bulk viscosity coefficient leads to a better description of the flow harmonics in ultracentral collisions. We then extract optimal values of bulk and shear viscosity coefficients that provide the best agreement with flow harmonic coefficients data in this centrality class. (C) 2014 Elsevier B.V. All rights reserved. C1 [Rose, Jean-Bernard; Paquet, Jean-Francois; Denicol, Gabriel S.; Luzum, Matthew; Jeon, Sangyong; Gale, Charles] McGill Univ, Dept Phys, Montreal, PQ H3A 2T8, Canada. [Luzum, Matthew] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Schenke, Bjoem] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. RP Denicol, GS (reprint author), McGill Univ, Dept Phys, 3600 Rue Univ, Montreal, PQ H3A 2T8, Canada. RI Luzum, Matthew/C-4986-2015; Silveira Denicol, Gabriel/L-5048-2016 OI Luzum, Matthew/0000-0002-0367-7055; FU Natural Sciences and Engineering Research Council of Canada; U.S. Department of Energy [DE-AC02-98CH10886]; Banting Fellowship of the Natural Sciences and Engineering Research Council of Canada; Hessian Initiative for Excellence (LOEWE) through the Helmholtz International Center for FAIR (HIC for FAIR) FX The authors thank H. Niemi and J. Jia for fruitful discussions. This work was supported in part by the Natural Sciences and Engineering Research Council of Canada, and by the U.S. Department of Energy Contract No. DE-AC02-98CH10886. G.S. Denicol acknowledges support through a Banting Fellowship of the Natural Sciences and Engineering Research Council of Canada, and C.G. acknowledges support from the Hessian Initiative for Excellence (LOEWE) through the Helmholtz International Center for FAIR (HIC for FAIR). NR 14 TC 15 Z9 15 U1 0 U2 0 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 926 EP 930 DI 10.1016/j.nuclphysa.2014.09.044 PG 5 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500147 ER PT J AU Gyulassy, M Levai, P Vitev, I Biro, TS AF Gyulassy, M. Levai, P. Vitev, I. Biro, T. S. TI Initial-state bremsstrahlung versus final-state hydrodynamic sources of azimuthal harmonics in p plus A at RHIC and LHC SO NUCLEAR PHYSICS A LA English DT Article DE Initial-state QCD radiation; Final-state viscous hydrodynamics; High energy nuclear collisions ID QUARK-GLUON PLASMA; ABELIAN ENERGY-LOSS; ANGULAR-CORRELATIONS; ROOT-S(NN)=2.76 TEV; LONG-RANGE; COLLISIONS; COLLABORATION; SIDE; FLOW AB Recent PT < 2 GeV azimuthal correlation data from the Beam Energy Scan (BES) and d + Au runs at RHIC/BNL and, especially, the surprising similarity of 2l = 2,4, ...-particle cummulant azimuthal n = 2,3,4,5 harmonics, v(n) {2l} (p(T)), in p + Pb and Pb + Pb at LHC have challenged the uniqueness of local equilibrium "perfect fluid" interpretations of those data. We report results derived in [1] on azimuthal harmonics arising from non-equilibrium initial-state non-abelian "wave interference" effects predicted by perturbative QCD gluon bremsstrahlung and sourced by Color Scintillation Arrays (CSA) of color antennas. CSA are naturally identified with multiple projectile and target beam jets produced in inelastic p + A reactions. We find a remarkable similarity between azimuthal harmonics sourced by initial state CSA and those predicted with final state perfect fluid models of high energy p + A reactions. The question of which mechanism dominates in p + A and A + A remains open at this time. (C) 2014 Elsevier B.V. All rights reserved. C1 [Gyulassy, M.; Levai, P.; Biro, T. S.] RMI, MTA WIGNER Res Ctr Phys, Budapest, Hungary. [Gyulassy, M.] Columbia Univ, Dept Phys, New York, NY 10027 USA. [Vitev, I.] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA. RP Gyulassy, M (reprint author), RMI, MTA WIGNER Res Ctr Phys, Budapest, Hungary. OI Gyulassy, Miklos/0000-0002-8106-9872 FU U.S. DOE [DE-FG02-93ER40764, DE-AC02-05CH1123]; Hungarian OTKA [K104260, NK106119]; NIH [TET_12_CN-1-2012-0016]; U.S. Department of Energy, Office of Science, Office of Nuclear Physics FX MG acknowledges support from the U.S. DOE DE-FG02-93ER40764, DE-AC02-05CH1123. PL, TB, and MG acknowledge support from Hungarian OTKA grants K104260, NK106119, and NIH TET_12_CN-1-2012-0016. IV was supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics. NR 32 TC 2 Z9 2 U1 0 U2 7 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 943 EP 948 DI 10.1016/j.nuclphysa.2014.08.013 PG 6 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500150 ER PT J AU Guursoy, U Kharzeev, D Rajagopal, K AF Gursoy, Umut Kharzeev, Dmitri Rajagopal, Krishna TI Magnetohydrodynamics and charged currents in heavy ion collisions SO NUCLEAR PHYSICS A LA English DT Article DE Magnetohydrodynamics; Quark gluon plasma; Heavy ion collisions AB The hot QCD matter produced in any heavy ion collision with a nonzero impact parameter is produced within a strong magnetic field. We study the imprint the magnetic fields produced in non-central heavy ion collisions leave on the azimuthal distributions and correlations of the produced charged hadrons. The magnetic field is time-dependent and the medium is expanding, which leads to the induction of charged currents due to the combination of Faraday and Hall effects. We find that these currents result in a charge-dependent directed flow v(1) that is odd in rapidity and odd under charge exchange. It can be detected by measuring correlations between the directed flow of charged hadrons at different rapidities, < v(1)(+/-)(y(1))v(1)(+/-)(y(2))>. (C) 2014 Elsevier B.V. All rights reserved. C1 [Gursoy, Umut] Univ Utrecht, Inst Theoret Phys, NL-3584 CE Utrecht, Netherlands. [Kharzeev, Dmitri] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA. [Kharzeev, Dmitri] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. [Rajagopal, Krishna] MIT, Ctr Theoret Phys, Cambridge, MA 02139 USA. RP Guursoy, U (reprint author), Univ Utrecht, Inst Theoret Phys, Leuvenlaan 4, NL-3584 CE Utrecht, Netherlands. FU DOE [DE-SC0011090, DE-FG-88ER40388, DE-AC02-98CH10886]; D-ITP consortium FX We are grateful to Sergei Voloshin for helpful suggestions. This work was supported by DOE grants DE-SC0011090, DE-FG-88ER40388 and DE-AC02-98CH10886 and is a part of the D-ITP consortium. NR 22 TC 0 Z9 0 U1 0 U2 3 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 986 EP 991 DI 10.1016/j.nuclphysa.2014.09.039 PG 6 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500158 ER PT J AU Yan, L Ollitrault, JY Poskanzer, AM AF Yan, Li Ollitrault, Jean-Yves Poskanzer, Arthur M. TI Universal parameterization of initial-state fluctuations and its applications to event-by-event anisotropy SO NUCLEAR PHYSICS A LA English DT Article DE Heavy-ion collisions; Fluctuations; Anisotropic flow ID COLLISIONS; FLOW AB We propose Elliptic Power and Power parameterizations for the probability distribution of initial state anisotropies in heavy-ion collisions. By assuming a linear eccentricity scaling, the new parameterizations can also be applied to fluctuations of harmonic flow. In particular, the recently measured flow multiparticle cumulants and event-by-event distributions are analyzed. (C) 2014 Elsevier B.V. All rights reserved. C1 [Yan, Li; Ollitrault, Jean-Yves] CNRS, Inst Phys Theor Saclay, IPhT, URA2306, F-91191 Gif Sur Yvette, France. [Poskanzer, Arthur M.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. RP Yan, L (reprint author), CNRS, Inst Phys Theor Saclay, IPhT, URA2306, F-91191 Gif Sur Yvette, France. OI Poskanzer, Arthur/0000-0001-9348-5868 FU European Research Council [ERC-AD-267258]; Office of Science, Office of Nuclear Science of the U.S. Department of Energy [DE-AC02-05CH11231] FX L.Y. and J.Y.O. are funded by the European Research Council under the Advanced Investigator Grant ERC-AD-267258. A.M.P. was supported by the Director, Office of Science, Office of Nuclear Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. NR 13 TC 1 Z9 1 U1 0 U2 0 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 1007 EP 1011 DI 10.1016/j.nuclphysa.2014.09.021 PG 5 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500162 ER PT J AU Schenke, B Venugopalan, R AF Schenke, Bjoern Venugopalan, Raju TI Collective effects in light-heavy ion collisions SO NUCLEAR PHYSICS A LA English DT Article DE Heavy ion collisions; Fluctuations; Fluid dynamics ID ENERGY NUCLEAR COLLISIONS; MULTIPLICITY; PPB AB We present results for the azimuthal anisotropy of charged hadron distributions in A+A, p+A, d+A, and He-3+A collisions within the IP-Glasma+musfc model. Obtained anisotropies are due to the fluid dynamic response of the system to the fluctuating initial geometry of the interaction region. While the elliptic and triangular anisotropies in peripheral Pb+Pb collisions at root s = 2.76 TeV are well described by the model, the same quantities in root s = 5.02 TeV p+Pb collisions underestimate the experimental data. This disagreement can be due to neglected initial state correlations or the lack of a detailed description of the fluctuating spatial structure of the proton, or both. We further present predictions for azimuthal anisotropies in p+Au, d+Au, and He-3+Au collisions at root s = 200 GeV. For d+Au and He-3+Au collisions we expect the detailed substructure of the nucleon to become less important. (C) 2014 Elsevier B.V. All rights reserved. C1 [Schenke, Bjoern; Venugopalan, Raju] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. RP Schenke, B (reprint author), Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA. FU DOE [DE-AC02-98CH10886]; DOE Office of Science Early Career Award; Office of Science of the U.S. Department of Energy [DE-AC02-05CH11231] FX We thank Jamie Nagle for providing us with the 3He nucleon configurations. This work was supported under DOE Contract No. DE-AC02-98CH10886. BPS acknowledges support from a DOE Office of Science Early Career Award. This research used resources of the National Energy Research Scientific Computing Center, which is supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. NR 31 TC 8 Z9 8 U1 0 U2 0 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 1039 EP 1044 DI 10.1016/j.nuclphysa.2014.08.092 PG 6 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500168 ER PT J AU Kozlov, I Luzum, M Denicol, GS Jeon, S Gale, C AF Kozlov, I. Luzum, M. Denicol, G. S. Jeon, S. Gale, C. TI Signatures of collective behavior in small systems SO NUCLEAR PHYSICS A LA English DT Article DE Heavy-ion collisions; Quark-gluon plasma; Hydrodynamics; Flow; Factorization ID ANGULAR-CORRELATIONS; PB COLLISIONS; LONG-RANGE; SIDE; PPB; TEV AB We perform 3 + 1D viscous hydrodynamics calculations of proton nucleus (pA) and nucleus nucleus (AA) collisions. Our goal is to understand the apparent collective behavior recently observed in pA collisions and to verify whether the highest multiplicity collision systems can be accurately described as a relativistic fluid. We compare our calculations of flow variables to existing measurements, and demonstrate that hydrodynamics correctly captures the measured trends. We show that our predictions for the pair correlation observable r(n) are validated by recent experimental pA measurements, and that our results are sensitive to the granularity of the initial state. We also compare our results with measurements done for nucleus nucleus collisions. (C) 2014 Elsevier B.V. All rights reserved. C1 [Kozlov, I.; Luzum, M.; Denicol, G. S.; Jeon, S.; Gale, C.] McGill Univ, Dept Phys, Montreal, PQ H3A 2T8, Canada. [Luzum, M.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Gale, C.] Frankfurt Inst Adv Studies, D-60438 Frankfurt, Germany. RP Kozlov, I (reprint author), McGill Univ, Dept Phys, 3600 Univ St, Montreal, PQ H3A 2T8, Canada. EM ikozlov@physics.mcgill.ca RI Luzum, Matthew/C-4986-2015; Silveira Denicol, Gabriel/L-5048-2016 OI Luzum, Matthew/0000-0002-0367-7055; FU Natural Sciences and Engineering Research Council of Canada; Office of High Energy and Nuclear Physics, Division of Nuclear Physics, of the U.S. Department of Energy [DE-AC02-05CH11231]; Canadian Institute of Nuclear Physics; Banting Fellowship of the Natural Sciences and Engineering Research Council of Canada FX The authors thank P. Bozek for fruitful discussions. This work was supported in part by the Natural Sciences and Engineering Research Council of Canada, and in part by the Director, Office of Energy Research, Office of High Energy and Nuclear Physics, Division of Nuclear Physics, of the U.S. Department of Energy under Contact No. DE-AC02-05CH11231. I.K. acknowledges support from the Canadian Institute of Nuclear Physics, G.S.D. acknowledges support through a Banting Fellowship of the Natural Sciences and Engineering Research Council of Canada. NR 20 TC 4 Z9 4 U1 0 U2 6 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 1045 EP 1050 DI 10.1016/j.nuclphysa.2014.09.054 PG 6 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500169 ER PT J AU Gangadharan, DR AF Gangadharan, Dhevan Raja CA ALICE Collaboration TI Freeze-out radii extracted using two- and three-pion Bose-Einstein correlations in pp, p-Pb, and Pb-Pb collisions at the LHC SO NUCLEAR PHYSICS A LA English DT Article DE p-Pb collisions; Femtoscopy; HBT radii ID COULOMB CORRECTIONS AB We report the results of two- and three-pion Bose-Einstein correlations measured in pp, p-Pb and Pb-Pb collisions with ALICE at the LHC. The femtoscopic radii, which characterize the system size at kinetic freeze-out, are extracted. One- and three-dimensional radii are extracted from two-pion correlations. In addition, one-dimensional radii are extracted also from three-pion correlations. The obtained radii increase with event multiplicity and decrease with pair transverse momentum. At comparable multiplicity, the radii measured in p-Pb collisions are more similar to those in pp collisions than in Pb-Pb collisions. The three-dimensional two-pion radii are compared to hydrodynamic predictions at large event multiplicity. Published by Elsevier B.V. C1 [Gangadharan, Dhevan Raja; ALICE Collaboration] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. RP Gangadharan, DR (reprint author), Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA. NR 15 TC 2 Z9 2 U1 5 U2 7 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 1066 EP 1071 DI 10.1016/j.nuclphysa.2014.08.098 PG 6 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500173 ER PT J AU Asakawa, M Bass, SA Mueller, B AF Asakawa, Masayuki Bass, Steffen A. Mueller, Berndt TI Center domains and their phenomenological consequences in ultrarelativistic heavy ion collisions SO NUCLEAR PHYSICS A LA English DT Article DE Quark-gluon plasma; Polyakov loop; Domain structure ID QUARK-GLUON PLASMA; POLYAKOV LOOP; COLLABORATION; PERSPECTIVE; CONDENSATE; MATTER AB We argue that the domain structure of deconfined QCD matter, which can be inferred from the properties of the Polyakov loop, can simultaneously explain the two most prominent experimental features of the quark-gluon plasma, namely its near ideal fluid properties and its large opacity. (C) 2014 Elsevier B.V. All rights reserved. C1 [Asakawa, Masayuki] Osaka Univ, Dept Phys, Toyonaka, Osaka 5620043, Japan. [Bass, Steffen A.; Mueller, Berndt] Duke Univ, Dept Phys, Durham, NC 27708 USA. [Mueller, Berndt] Brookhaven Natl Lab, Upton, NY 11973 USA. RP Asakawa, M (reprint author), Osaka Univ, Dept Phys, Toyonaka, Osaka 5620043, Japan. OI Bass, Steffen/0000-0002-9451-0954 FU U.S. Department of Energy [DE-FG02-05ER41367, DE-SC0005396]; JSPS of Japan [26400272] FX B.M. and S.A.B. acknowledge support by U.S. Department of Energy grants DE-FG02-05ER41367 and DE-SC0005396. M.A. was supported by Grants-in-Aid for Scientific Research 26400272 from JSPS of Japan. NR 21 TC 0 Z9 0 U1 0 U2 1 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 1120 EP 1124 DI 10.1016/j.nuclphysa.2014.08.005 PG 5 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500183 ER PT J AU Qiu, H AF Qiu, Hao CA STAR Collaboration TI STAR heavy flavor tracker SO NUCLEAR PHYSICS A LA English DT Article DE Heavy flavor; Silicon detector; Monolithic Active Pixel Sensor AB Hadrons containing heavy quarks are a clean probe of the early dynamic evolution of the dense and hot medium created in high-energy nuclear collisions. To explore heavy quark production at RHIC, the Heavy Flavor Tracker (HFT) for the STAR experiment was built and installed in time for RHIC Run 14. The HFT consists of four layers of silicon detectors. The two outermost layers are silicon strip detectors and the two innermost layers are made from state-of-the-art ultra-thin CMOS Monolithic Active Pixel Sensors (MAPS). This is the first application of a CMOS MAPS detector in a collider experiment. The use of thin pixel sensors plus the use of carbon fiber supporting material limits the material budget to be only 0.4% radiation length per pixel detector layer, enabling the reconstruction of low PT heavy flavor hadrons. The status and performance of the HFT in the RHIC 200 GeV Au + Au run in 2014 are reported. Very good detector efficiency, hit residuals and track resolution (DCAs) were observed in the cosmic ray data and in the Au + Au data. (C) 2014 Elsevier B.V. All rights reserved. C1 [Qiu, Hao; STAR Collaboration] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. RP Qiu, H (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA. NR 5 TC 4 Z9 4 U1 4 U2 12 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 1141 EP 1146 DI 10.1016/j.nuclphysa.2014.08.056 PG 6 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500187 ER PT J AU Sako, H Chujo, T Gunji, T Harada, H Imai, K Kaneta, M Kinsho, M Liu, Y Nagamiya, S Nishio, K Ozawa, K Saha, PK Sakaguchi, T Sato, S Tamura, J AF Sako, H. Chujo, T. Gunji, T. Harada, H. Imai, K. Kaneta, M. Kinsho, M. Liu, Y. Nagamiya, S. Nishio, K. Ozawa, K. Saha, P. K. Sakaguchi, T. Sato, S. Tamura, J. TI Towards the heavy-ion program at J-PARC SO NUCLEAR PHYSICS A LA English DT Article DE QCD phase diagram; High baryon density; Heavy ion acceleration AB A future heavy-ion program at J-PARC has been discussed. The QCD phase structure in high baryon density regime will be explored with heavy ions at the beam momenta of around 10 A GeV/c at the beam rate of 10(10)-10(11) Hz. For this quest, a large acceptance spectrometer is designed to measure electrons and muons, and rare probes such as multi-strangeness and charmed hadrons/nuclei. A heavy-ion acceleration scheme is under study with a new heavy-ion linac and a new booster ring, which accelerate and inject beams into the existing Rapid-Cycling Synchrotron and Main Ring synchrotron. An overview of the heavy-ion program and an accelerator design, as well as physics goals and a conceptual design of the heavy-ion experiment are discussed. (C) 2014 Elsevier B.V. All rights reserved. C1 [Sako, H.; Imai, K.; Nagamiya, S.; Nishio, K.; Sato, S.] Japan Atom Energy Agcy, Adv Sci Res Ctr, Naka, Ibaraki 3191195, Japan. [Sako, H.; Harada, H.; Kinsho, M.; Saha, P. K.; Tamura, J.] Japan Atom Energy Agcy, J PARC Ctr, Naka, Ibaraki 3191195, Japan. [Chujo, T.] Univ Tsukuba, Tsukuba, Ibaraki 3058577, Japan. [Gunji, T.] Univ Tokyo, Ctr Nucl Study, Wako, Saitama 3510198, Japan. [Kaneta, M.] Tohoku Univ, Sendai, Miyagi 9808578, Japan. [Liu, Y.; Nagamiya, S.; Ozawa, K.] High Energy Accelerator Res Org, J PARC Ctr, Tsukuba, Ibaraki 3050801, Japan. [Nagamiya, S.] RIKEN, Wako, Saitama 3510198, Japan. [Sakaguchi, T.] Brookhaven Natl Lab, Upton, NY 11973 USA. RP Sako, H (reprint author), Japan Atom Energy Agcy, Adv Sci Res Ctr, Naka, Ibaraki 3191195, Japan. NR 9 TC 5 Z9 5 U1 0 U2 0 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 1158 EP 1162 DI 10.1016/j.nuclphysa.2014.08.065 PG 5 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500190 ER PT J AU Sun, X AF Sun, Xu CA STAR Collaboration TI Triangular flow of identified hadrons in Au plus Au collisions at root S-NN=39 and 200 GeV SO NUCLEAR PHYSICS A LA English DT Article DE v(3); Mass ordering; NCQ scaling ID NUCLEAR COLLISIONS; STAR AB We present triangular flow (v(3)) measured by STAR for identified particles (pi(+/-), K-+/-, p, (p) over bar and phi) relative to the third-harmonic event plane as a function of p(T) for minimum bias (0%-80%) Au + Au collisions at root S-NN = 39 GeV and 200 GeV. We discuss the hydrodynamic description of the mass ordering at low p(T) (p(T) < 1.5 GeV/c), number-of-constituent-quark (NCQ) scaling at intermediate p(T) (0.5 GeV/c < p(T)/n(q) < 1.5 GeV/c), and the ratio of v(2)/v(3) at the p(T) of the crossing of the identified particle v3. (C) 2014 Elsevier B.V. All rights reserved. C1 [Sun, Xu] Harbin Inst Technol, Dept Phys, Harbin 150001, Peoples R China. [Sun, Xu] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Nucl Sci, Berkeley, CA 94720 USA. RP Sun, X (reprint author), Harbin Inst Technol, Dept Phys, Harbin 150001, Peoples R China. NR 13 TC 3 Z9 3 U1 0 U2 7 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0375-9474 EI 1873-1554 J9 NUCL PHYS A JI Nucl. Phys. A PD NOV PY 2014 VL 931 BP 1194 EP 1198 DI 10.1016/j.nuclphysa.2014.09.058 PG 5 WC Physics, Nuclear SC Physics GA AY5FN UT WOS:000347598500197 ER PT J AU Kravchenko, AN Negassa, WC Guber, AK Hildebrandt, B Marsh, TL Rivers, ML AF Kravchenko, Alexandra N. Negassa, Wakene C. Guber, Andrey K. Hildebrandt, Britton Marsh, Terence L. Rivers, Mark L. TI Intra-aggregate Pore Structure Influences Phylogenetic Composition of Bacterial Community in Macroaggregates SO SOIL SCIENCE SOCIETY OF AMERICA JOURNAL LA English DT Article ID SOIL MICROBIAL COMMUNITIES; RAY COMPUTED-TOMOGRAPHY; SPATIAL-DISTRIBUTION; ORGANIC-MATTER; COVER CROPS; AGRICULTURAL MANAGEMENT; GAMMA-IRRADIATION; CROPPING SYSTEMS; RIBOSOMAL-RNA; CARBON AB It is known that variability in the characteristics of soil physical microenvironments, e.g., locations and characteristics of soil pores, can have a major influence on microorganisms. This study compared the characteristics of intra-aggregate pores and their relationships with bacterial community composition in 4-to 6-mm soil macroaggregates from two contrasting agricultural systems, namely a corn (Zea mays L.)-soybean [Glycine max (L.) Merr.]-wheat (Triticum aestivum L.) rotation (i) with conventional chemical inputs and (ii) without chemical inputs but with legume cover crops. Characteristics of intra-aggregate pores and particulate organic matter (POM) were obtained from three-dimensional X-ray computed microtomography aggregate images at 13-mm resolution. Microbial community analyses were conducted using 16S rRNA pyrosequencing. We found that the aggregates from long-term (>20 yr) organic management with cover crops differed from the aggregates from conventional management in terms of intra-aggregate pore-size distribution, intra-aggregate pore variability, POM contents, as well as microbial community compositions. Relative abundances of Actinobacteria, Proteobacteria, and Firmicutes in the aggregates from cover-crop-based management were positively correlated with the presence of large (>110 mm) pores, while the presence of medium-sized pores (32-84 mm) was significantly correlated with 30 to 40% of the top 100 bacterial operational taxonomic units identified during sequencing. The results suggested that the legacy of rhizosphere presence in terms of intra-aggregate pore structure and microbial community composition can last in the studied soil for at least 4 to 9 mo. Our study demonstrated that working with bulk sieved soil samples can mask substantial differences present within distinct soil aggregate units. C1 [Kravchenko, Alexandra N.; Negassa, Wakene C.; Guber, Andrey K.] Michigan State Univ, Dept Plant Soil & Microbial Sci, E Lansing, MI 48824 USA. [Hildebrandt, Britton; Marsh, Terence L.] Michigan State Univ, Dept Microbiol & Mol Genet, E Lansing, MI 48824 USA. [Rivers, Mark L.] Univ Chicago, Argonne Natl Lab, Ctr Adv Radiat Sources, Argonne, IL 60439 USA. RP Kravchenko, AN (reprint author), Michigan State Univ, Dept Plant Soil & Microbial Sci, E Lansing, MI 48824 USA. EM kravche1@msu.edu FU USDA-NIFA cropping systems Coordinated Agricultural Project (CAP) [2011-68002-30190.7]; U.S. National Science Foundation LTER Program at the Kellogg Biological Station [DEB 1027253]; Kellogg Biological Station; Michigan State University's "Project GREEEN" Program; Michigan State University's "Discretionary Fund Initiative" Program FX Support for this research was provided in part by USDA-NIFA Award no. 2011-68002-30190.7 cropping systems Coordinated Agricultural Project (CAP); by the U.S. National Science Foundation LTER Program at the Kellogg Biological Station (DEB 1027253); by Kellogg Biological Station; by Michigan State University's "Project GREEEN" Program; and by Michigan State University's "Discretionary Fund Initiative" Program. NR 93 TC 7 Z9 7 U1 10 U2 54 PU SOIL SCI SOC AMER PI MADISON PA 677 SOUTH SEGOE ROAD, MADISON, WI 53711 USA SN 0361-5995 EI 1435-0661 J9 SOIL SCI SOC AM J JI Soil Sci. Soc. Am. J. PD NOV-DEC PY 2014 VL 78 IS 6 BP 1924 EP 1939 DI 10.2136/sssaj2014.07.0308 PG 16 WC Soil Science SC Agriculture GA AY5PN UT WOS:000347624500011 ER PT J AU Harding, SA Xue, LJ Du, L Nyamdari, B Lindroth, RL Sykes, R Davis, MF Tsai, CJ AF Harding, Scott A. Xue, Liang-Jiao Du, Lei Nyamdari, Batbayar Lindroth, Richard L. Sykes, Robert Davis, Mark F. Tsai, Chung-Jui TI Condensed tannin biosynthesis and polymerization synergistically condition carbon use, defense, sink strength and growth in Populus SO TREE PHYSIOLOGY LA English DT Article DE flavonoid; glycolysis; MYB; phenylethylamine; phenylpropanoid; salicortin ID PHENYLPROPANOID METABOLISM; NUTRIENT AVAILABILITY; SECONDARY METABOLISM; INSECT PERFORMANCE; GENE-EXPRESSION; PLANTS; ASPEN; PHYTOCHEMISTRY; TREMULOIDES; TOBACCO AB The partitioning of carbon for growth, storage and constitutive chemical defenses is widely framed in terms of a hypothetical sink-source differential that varies with nutrient supply. According to this framework, phenolics accrual is passive and occurs in source leaves when normal sink growth is not sustainable due to a nutrient limitation. In assessing this framework, we present gene and metabolite evidence that condensed tannin (CT) accrual is strongest in sink leaves and sequesters carbon in a way that impinges upon foliar sink strength and upon phenolic glycoside ( PG) accrual in Populus. The work was based on two Populus fremontii x angustifolia backcross lines with contrasting rates of CT accrual and growth, and equally large foliar PG reserves. However, foliar PG accrual was developmentally delayed in the high-CT, slow-growth line (SG), and nitrogenlimitation led to increased foliar PG accrual only in the low-CT, fast-growth line (FG). Metabolite profiling of developing leaves indicated comparatively carbon-limited amino acid metabolism, depletion of several Krebs cycle intermediates and reduced organ sink strength in SG. Gene profiling indicated that CT synthesis decreased as leaves expanded and PGs increased. A most striking finding was that the nitrogenous monoamine phenylethylamine accumulated only in leaves of SG plants. The potential negative impact of CT hyper-accumulation on foliar sink strength, as well as a mechanism for phenylethylamine involvement in CT polymerization in Populus are discussed. Starch accrual in source leaves and CT accrual in sink leaves of SG may both contribute to the maintenance of a slow-growth phenotype suited to survival in nutrient-poor habitats. C1 [Harding, Scott A.; Xue, Liang-Jiao; Du, Lei; Nyamdari, Batbayar; Tsai, Chung-Jui] Univ Georgia, Warnell Sch Forestry & Nat Resources, Athens, GA 30602 USA. [Harding, Scott A.; Xue, Liang-Jiao; Du, Lei; Nyamdari, Batbayar; Tsai, Chung-Jui] Univ Georgia, Dept Genet, Athens, GA 30602 USA. [Xue, Liang-Jiao; Du, Lei; Tsai, Chung-Jui] Univ Georgia, Inst Bioinformat, Athens, GA 30602 USA. [Lindroth, Richard L.] Univ Wisconsin, Dept Entomol, Madison, WI 53706 USA. [Sykes, Robert; Davis, Mark F.] Natl Renewable Energy Lab, Golden, CO 80401 USA. RP Harding, SA (reprint author), Univ Georgia, Warnell Sch Forestry & Nat Resources, Athens, GA 30602 USA. EM sharding@uga.edu; cjtsai@uga.edu RI Tsai, CJ/C-2450-2009; Xue, Liangjiao/F-3554-2016; Xue, Liang-Jiao/N-3675-2014; OI Tsai, CJ/0000-0002-9282-7704; Xue, Liang-Jiao/0000-0003-1766-5298; davis, mark/0000-0003-4541-9852 FU US Department of Energy, Biological and Environmental Research Program [DE-FG02-05ER64112]; National Science Foundation Plant Genome Program [DBI-0421756] FX This work was supported by the US Department of Energy, Biological and Environmental Research Program DE-FG02-05ER64112 and by the National Science Foundation Plant Genome Program DBI-0421756. NR 52 TC 5 Z9 5 U1 3 U2 29 PU OXFORD UNIV PRESS PI OXFORD PA GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND SN 0829-318X EI 1758-4469 J9 TREE PHYSIOL JI Tree Physiol. PD NOV PY 2014 VL 34 IS 11 BP 1240 EP 1251 DI 10.1093/treephys/tpt097 PG 12 WC Forestry SC Forestry GA CA0KM UT WOS:000348606700008 PM 24336515 ER PT J AU Fujii, A Marques, O AF Fujii, Akihiro Marques, Osni TI Axis Communication Method for Algebraic Multigrid Solver SO IEICE TRANSACTIONS ON INFORMATION AND SYSTEMS LA English DT Article DE strong scaling; liner solver; Algebraic multigrid method AB Communication costs have become a performance bottleneck in many applications, and are a big issue for high performance computing on massively parallel machines. This paper proposes a halo exchange method for unstructured sparse matrix vector products within the algebraic multigrid method, and evaluate it on a supercomputer with mesh/torus networks. In our numerical tests with a Poisson problem, the proposed method accelerates the linear solver more than 14 times with 23040 cores. C1 [Fujii, Akihiro] Kogakuin Univ, Tokyo 1638677, Japan. [Marques, Osni] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. RP Fujii, A (reprint author), Kogakuin Univ, Tokyo 1638677, Japan. EM fujii@cc.kogakuin.ac.jp FU JST, CREST FX This research was supported by JST, CREST. NR 5 TC 0 Z9 0 U1 1 U2 1 PU IEICE-INST ELECTRONICS INFORMATION COMMUNICATIONS ENG PI TOKYO PA KIKAI-SHINKO-KAIKAN BLDG, 3-5-8, SHIBA-KOEN, MINATO-KU, TOKYO, 105-0011, JAPAN SN 1745-1361 J9 IEICE T INF SYST JI IEICE Trans. Inf. Syst. PD NOV PY 2014 VL E97D IS 11 BP 2955 EP 2958 DI 10.1587/transinf.2014EDL8052 PG 4 WC Computer Science, Information Systems; Computer Science, Software Engineering SC Computer Science GA AZ3QH UT WOS:000348141300014 ER PT J AU Allison, T AF Allison, Tim TI FREIGHT-HANDLING TECHNOLOGIES AND INDUSTRIAL BUILDING DESIGN: FREIGHTHOUSE AND WAREHOUSE FACILITIES OF THE CHICAGO JUNCTION RAILWAY, 1900-30 SO INDUSTRIAL ARCHAEOLOGY REVIEW LA English DT Article AB Among the first US railway companies to use the electric tractor and elevator in freight-handling buildings, the Chicago Junction Railway (CJR) primarily served industries in the rapidly growing Central Manufacturing District. CJR freight-handling services were initially provided in single-storey, and subsequently multi-storey, brick and mill buildings, using hand trucks, with only limited storage and warehousing space available. Labour cost savings, and changes in the scale and flexibility of freighthouse operations, possible with the electric tractor and elevator, allowed the CJR to meet the demand for increased freight-handling and warehousing capacity by augmenting older facilities with multi-storey, integrated freighthouse and warehouse buildings, latterly built with steel-reinforced concrete. C1 [Allison, Tim] Argonne Natl Lab, Argonne, IL 60439 USA. RP Allison, T (reprint author), Argonne Natl Lab, Div Energy Syst, ES202,9700 South Cass Ave, Argonne, IL 60439 USA. EM tallison@anl.gov NR 31 TC 0 Z9 0 U1 0 U2 1 PU MANEY PUBLISHING PI LEEDS PA STE 1C, JOSEPHS WELL, HANOVER WALK, LEEDS LS3 1AB, W YORKS, ENGLAND SN 0309-0728 EI 1745-8196 J9 IND ARCHAEOL REV JI Ind. Archaeol. Rev. PD NOV PY 2014 VL 36 IS 2 BP 109 EP 127 DI 10.1179/0309072814Z.00000000034 PG 19 WC Archaeology; History SC Archaeology; History GA AY5OW UT WOS:000347622800004 ER PT J AU Baboly, MG Soliman, Y Su, MF Reinke, CM Leseman, ZC El-Kady, I AF Baboly, Mohammadhosein Ghasemi Soliman, Yasser Su, Mehmet F. Reinke, Charles M. Leseman, Zayd C. El-Kady, Ihab TI Enhanced plane wave expansion analysis for the band structure of bulk modes in two-dimensional high-contrast solid-solid phononic crystals SO PHOTONICS AND NANOSTRUCTURES-FUNDAMENTALS AND APPLICATIONS LA English DT Article DE Phononic crystals; Plane wave expansion; Bandgap; High contrast; Inverse rule; Laurents rule ID ACOUSTIC-WAVES; COMPOSITE-MATERIALS; ELASTIC-WAVES; GAPS; SYSTEMS; SURFACE; GUIDES AB Plane wave expansion analyses that use the inverse rule to obtain the Fourier coefficients of the elastic tensor instead of the more conventional Laurent's rule, exhibit faster convergence rates for solid-solid phononic crystals. In this work, the band structure convergence of calculations using the inverse rule is investigated and applied to the case of high acoustic impedance contrast solid solid phononic crystals, previously known for convergence difficulties. Results are contrasted to those obtained with the conventional plane wave expansion method. The inverse rule is found to converge at a much rate for all ranges of impedance contrast, and the ratio between the computational times needed to obtain a convergent band structure for a high-contrast solid solid phononic crystal with the conventional plane wave expansion method using 1369 reciprocal lattice vectors is as large as 6800:1. This ratio decreases for material sets with lower impedance contrast; however, the inverse rule is still faster for a given error threshold for even the lowest impedance contrast phononic crystals reported in the literature. This convergence enhancement is a major factor in reconsidering the plane wave expansion method as an important tool in obtaining propagating elastic modes in phononic crystals. Published by Elsevier B.V. C1 [Baboly, Mohammadhosein Ghasemi; Su, Mehmet F.; Leseman, Zayd C.; El-Kady, Ihab] Univ New Mexico, Dept Mech Engn, Albuquerque, NM 87131 USA. [Soliman, Yasser; Su, Mehmet F.; El-Kady, Ihab] Univ New Mexico, Dept Elect & Comp Engn, Albuquerque, NM 87131 USA. [Reinke, Charles M.; El-Kady, Ihab] Sandia Natl Labs, Dept Appl Photon Microsyst, Albuquerque, NM 87185 USA. RP El-Kady, I (reprint author), Sandia Natl Labs, Dept Appl Photon Microsyst, POB 5800, Albuquerque, NM 87185 USA. EM ielkady@sandia.gov FU National Science Foundation, Division of CMMI Award [1056077]; U.S. Department of Energy's National Nuclear Security Administration [DE-AC04-94AL85000] FX MGB and ZCL were supported under an award from the National Science Foundation, Division of CMMI Award 1056077. Sandia National Laboratories is a multi-program laboratory managed and operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the U.S. Department of Energy's National Nuclear Security Administration under contract DE-AC04-94AL85000. NR 29 TC 4 Z9 4 U1 1 U2 11 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 1569-4410 EI 1569-4429 J9 PHOTONIC NANOSTRUCT JI Photonics Nanostruct. PD NOV PY 2014 VL 12 IS 5 BP 487 EP 492 DI 10.1016/j.photonics.2014.08.001 PG 6 WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Optics; Physics, Applied SC Science & Technology - Other Topics; Materials Science; Optics; Physics GA AY7WZ UT WOS:000347767900011 ER PT J AU Jarvis, KG Grim, CJ Beaubrun, JJ Ewing, L Dudley, K Ottesen, A Wang, C Pettengill, J Brown, E Hanes, D AF Jarvis, K. G. Grim, C. J. Beaubrun, J. J. Ewing, L. Dudley, K. Ottesen, A. Wang, C. Pettengill, J. Brown, E. Hanes, D. TI Evaluation of a metagenomics approach for the early detection of Salmonella in cilantro SO PHYTOPATHOLOGY LA English DT Meeting Abstract CT APS-CPS Joint Meeting CY AUG 09-13, 2014 CL Minneapolis, MN SP APS, CPS C1 [Jarvis, K. G.; Beaubrun, J. J.; Ewing, L.; Dudley, K.; Ottesen, A.; Hanes, D.] US FDA, Laurel, MD USA. [Grim, C. J.] Oak Ridge Inst Sci & Technol, Oak Ridge, TN USA. [Wang, C.; Pettengill, J.; Brown, E.] US FDA, College Pk, MD USA. NR 0 TC 0 Z9 0 U1 1 U2 1 PU AMER PHYTOPATHOLOGICAL SOC PI ST PAUL PA 3340 PILOT KNOB ROAD, ST PAUL, MN 55121 USA SN 0031-949X EI 1943-7684 J9 PHYTOPATHOLOGY JI Phytopathology PD NOV PY 2014 VL 104 IS 11 SU 3 BP 55 EP 55 PG 1 WC Plant Sciences SC Plant Sciences GA AW5GG UT WOS:000346303300310 ER PT J AU Wang, D Han, CS Lo, CC Dichosa, AE Chain, PS Yu, JM Dorosky, RJ Pierson, LS Pierson, EA AF Wang, D. Han, C. S. Lo, C. -C. Dichosa, A. E. Chain, P. S. Yu, J. M. Dorosky, R. J. Pierson, L. S., III Pierson, E. A. TI Adaptation genomics of a small colony variant (SCV) in the biofilm of Pseudomonas chlororaphis 30-84 SO PHYTOPATHOLOGY LA English DT Meeting Abstract CT APS-CPS Joint Meeting CY AUG 09-13, 2014 CL Minneapolis, MN SP APS, CPS C1 [Wang, D.; Han, C. S.; Lo, C. -C.; Dichosa, A. E.; Chain, P. S.] LANL, Los Alamos, NM USA. [Yu, J. M.; Dorosky, R. J.; Pierson, L. S., III; Pierson, E. A.] TAMU, College Stn, TX USA. NR 0 TC 0 Z9 0 U1 0 U2 0 PU AMER PHYTOPATHOLOGICAL SOC PI ST PAUL PA 3340 PILOT KNOB ROAD, ST PAUL, MN 55121 USA SN 0031-949X EI 1943-7684 J9 PHYTOPATHOLOGY JI Phytopathology PD NOV PY 2014 VL 104 IS 11 SU 3 BP 125 EP 125 PG 1 WC Plant Sciences SC Plant Sciences GA AW5GG UT WOS:000346303300715 ER PT J AU Watkins, JP Ellis, ED Girardi, DJ Cragle, DL Richter, BS AF Watkins, Janice P. Ellis, Elizabeth D. Girardi, David J. Cragle, Donna L. Richter, Bonnie S. TI Illness Absences Among Beryllium Sensitized Workers SO AMERICAN JOURNAL OF PUBLIC HEALTH LA English DT Article ID DISEASE; RISK AB Objectives. This study examined absence rates among US Department of Energy workers who had beryllium sensitization (BeS) or were diagnosed with chronic beryllium disease (CBD) compared with those of other workers. Methods. We used the lymphocyte proliferation test to determine beryllium sensitivity. In addition, we applied multivariable logistic regression to compare absences from 2002 to 2011 between workers with BeS or CBD to those without, and survival analysis to compare time to first absence by beryllium sensitization status. Finally, we examined beryllium status by occupational group. Results. Fewer than 3% of the 19 305 workers were BeS, and workers with BeS or CBD had more total absences (odds ratio [OR] = 1.31; 95% confidence interval [CI] = 1.18, 1.46) and respiratory absences (OR = 1.51; 95% CI = 1.24, 1.84) than did other workers. Time to first absence for all causes and for respiratory conditions occurred earlier for workers with BeS or CBD than for other workers. Line operators and crafts personnel were at increased risk for BeS or CBD. Conclusions. Although not considered "diseased," workers with BeS have higher absenteeism compared with nonsensitized workers. C1 [Watkins, Janice P.; Ellis, Elizabeth D.; Girardi, David J.; Cragle, Donna L.] Oak Ridge Associated Univ, Oak Ridge, TN USA. [Richter, Bonnie S.] US DOE, Off Hlth & Safety, Washington, DC 20585 USA. RP Richter, BS (reprint author), 19901 Germantown Rd, Germantown, MD 20874 USA. EM bonnie.richter@hq.doe.gov FU US Department of Energy [DE-AC05-06OR23100]; Oak Ridge Associated Universities [DE-AC05-06OR23100] FX This document describes activities performed under contract number DE-AC05-06OR23100 between the US Department of Energy and Oak Ridge Associated Universities. The US Government retains a nonexclusive, royalty-free license to publish or reproduce the published form of this work, or to allow others to do so for US Government purposes. NR 18 TC 1 Z9 1 U1 0 U2 0 PU AMER PUBLIC HEALTH ASSOC INC PI WASHINGTON PA 800 I STREET, NW, WASHINGTON, DC 20001-3710 USA SN 0090-0036 EI 1541-0048 J9 AM J PUBLIC HEALTH JI Am. J. Public Health PD NOV PY 2014 VL 104 IS 11 BP E165 EP E169 DI 10.2105/AJPH.2014.302132 PG 5 WC Public, Environmental & Occupational Health SC Public, Environmental & Occupational Health GA AX8UR UT WOS:000347184400026 PM 25211750 ER PT J AU Sadykov, AF Gerashchenko, AP Piskunov, YV Ogloblichev, VV Smol'nikov, AG Verkhovskii, SV Buzlukov, AL Arapova, IY Furukawa, Y Yakubovskii, AY Bush, AA AF Sadykov, A. F. Gerashchenko, A. P. Piskunov, Yu V. Ogloblichev, V. V. Smol'nikov, A. G. Verkhovskii, S. V. Buzlukov, A. L. Arapova, I. Yu Furukawa, Y. Yakubovskii, A. Yu Bush, A. A. TI Magnetic structure of the low-dimensional magnet NaCu2O2: Cu-63,Cu-65 and Na-23 NMR studies SO JOURNAL OF EXPERIMENTAL AND THEORETICAL PHYSICS LA English DT Article ID CHAIN CUPRATES LICU2O2; WEAK FERROMAGNETISM; CRYSTALS; SYSTEMS; GROWTH; ORDER AB The magnetic structure of a quasi-one-dimensional frustrated NaCu2O2 magnet single crystal is studied by NMR. The spatial orientation of the planar spin spirals in the copper-oxygen Cu2+-O chains is determined, and its evolution as a function of the applied magnetic field direction is analyzed. C1 [Sadykov, A. F.; Gerashchenko, A. P.; Piskunov, Yu V.; Ogloblichev, V. V.; Smol'nikov, A. G.; Verkhovskii, S. V.; Buzlukov, A. L.; Arapova, I. Yu] Russian Acad Sci, Inst Met Phys, Ural Branch, Ekaterinburg 620990, Russia. [Furukawa, Y.] Iowa State Univ, Ames Lab, Ames, IA 50011 USA. [Yakubovskii, A. Yu] Natl Res Ctr Kurchatov Inst, Moscow 123182, Russia. [Bush, A. A.] Moscow State Tech Univ Radio Engn Elect & Automat, Moscow 119454, Russia. RP Sadykov, AF (reprint author), Russian Acad Sci, Inst Met Phys, Ural Branch, Ul S Kovalevskoi 18, Ekaterinburg 620990, Russia. EM sadykov@imp.uran.ru RI Arapova, Irina/I-3795-2013; Piskunov, Yuri/J-7799-2013; Verkhovskii, Stanislav/K-2863-2013; Ogloblichev, Vasily/K-3399-2013; Sadykov, Almaz/J-3528-2013; Smolnikov, Alex/J-9285-2013; Alexandr, Bush/R-2287-2016; Buzlukov, Anton/J-8078-2013; Gerashenko, Alexander/J-9321-2013 OI Arapova, Irina/0000-0001-8034-592X; Piskunov, Yuri/0000-0002-6115-6207; Verkhovskii, Stanislav/0000-0002-8035-9544; Ogloblichev, Vasily/0000-0003-0520-7521; Sadykov, Almaz/0000-0003-1742-278X; Smolnikov, Alex/0000-0001-6295-9530; Alexandr, Bush/0000-0003-3990-9847; Buzlukov, Anton/0000-0002-2728-0503; Gerashenko, Alexander/0000-0002-9114-7141 FU Russian Foundation for Basic Research [12-03-31814]; Ural Branch of the Russian Academy of Sciences [14-2-NP-199, 12-U-2-1025] FX This work was supported by the Russian Foundation for Basic Research (project no. 12-03-31814) and the Ural Branch of the Russian Academy of Sciences (project nos. 14-2-NP-199, 12-U-2-1025). NR 29 TC 3 Z9 3 U1 5 U2 12 PU MAIK NAUKA/INTERPERIODICA/SPRINGER PI NEW YORK PA 233 SPRING ST, NEW YORK, NY 10013-1578 USA SN 1063-7761 EI 1090-6509 J9 J EXP THEOR PHYS+ JI J. Exp. Theor. Phys. PD NOV PY 2014 VL 119 IS 5 BP 870 EP 879 DI 10.1134/S1063776114110107 PG 10 WC Physics, Multidisciplinary SC Physics GA AX4JC UT WOS:000346898100011 ER PT J AU Ripoll, JF Albert, JM Cunningham, GS AF Ripoll, J. -F. Albert, J. M. Cunningham, G. S. TI Electron lifetimes from narrowband wave-particle interactions within the plasmasphere SO JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS LA English DT Article DE lifetime; electron; plasmasphere; narrowband; wave-particle interactions; DSX ID RADIATION-BELT ELECTRONS; PITCH-ANGLE DIFFUSION; EARTHS INNER MAGNETOSPHERE; SCATTERING LOSS; ION-CYCLOTRON; COEFFICIENTS; ENERGY; CHORUS; MODEL; ACCELERATION AB This paper is devoted to the systematic study of electron lifetimes from narrowband wave-particle interactions within the plasmasphere. It relies on a new formulation of the bounce-averaged quasi-linear pitch angle diffusion coefficients parameterized by a single frequency, , and wave normal angle, . We first show that the diffusion coefficients scale with /(ce), where (ce) is the equatorial electron gyrofrequency, and that maximal pitch angle diffusion occurs along the line (0)=/2-, where (0) is the equatorial pitch angle. Lifetimes are computed for L shell values in the range [1.5, 3.5] and energies, E, in the range [0.1, 6] MeV as a function of frequency and wave normal angle. The maximal pitch angle associated with a given lifetime is also given, revealing the frequencies that are able to scatter nearly equatorial pitch angle particles. The lifetimes are relatively independent of frequency and wave normal angle after taking into consideration the scaling law, with a weak dependence on wave normal angle up to 60-70 degrees, increasing to infinity as the wave normal angle approaches the resonance cone. We identify regions in the (L, E) plane in which a single wave type (hiss, VLF transmitters, or lightning-generated waves) is dominant relative to the others. We find that VLF waves dominate the lifetime for 0.2-0.4MeV at L2 and for 0.5-0.8MeV at L1.5, while hiss dominates the lifetime for 2-3MeV at L=3-3.5. The influence of lightning-generated waves is always mixed with the other two and cannot be easily differentiated. Limitations of the method for addressing effects due to restricted latitude or pitch angle domains are also discussed. Finally, for each (L, E) we search for the minimum lifetime and find that the optimal frequency that produces this lifetime increases as L diminishes. Restricting the search to very oblique waves, which could be emitted during the Demonstration and Science Experiments satellite mission, we find that the optimal frequency is always close to 0.16(ce). C1 [Ripoll, J. -F.] CEA, DAM, DIF, Arpajon, France. [Albert, J. M.] Air Force Res Lab, Kirtland AFB, NM USA. [Cunningham, G. S.] Los Alamos Natl Lab, Los Alamos, NM USA. RP Ripoll, JF (reprint author), CEA, DAM, DIF, Arpajon, France. EM jean-francois.ripoll@cea.fr OI Albert, Jay/0000-0001-9494-7630; Cunningham, Gregory/0000-0001-8819-4345 FU CEA/DAM; NNSA/DP FX This work was performed under the auspices of an agreement between CEA/DAM and NNSA/DP on cooperation on fundamental science. For further information or right to access to the material used in this paper, readers can contact the authors. NR 68 TC 9 Z9 9 U1 0 U2 10 PU AMER GEOPHYSICAL UNION PI WASHINGTON PA 2000 FLORIDA AVE NW, WASHINGTON, DC 20009 USA SN 2169-9380 EI 2169-9402 J9 J GEOPHYS RES-SPACE JI J. Geophys. Res-Space Phys. PD NOV PY 2014 VL 119 IS 11 BP 8858 EP 8880 DI 10.1002/2014JA020217 PG 23 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AX2RO UT WOS:000346792100011 ER PT J AU Zhou, QH Xiao, FL Yang, C Liu, S Kletzing, CA Kurth, WS Hospodarsky, GB Spence, HE Reeves, GD Funsten, HO Blake, JB Baker, DN Wygant, JR AF Zhou, Qinghua Xiao, Fuliang Yang, Chang Liu, Si Kletzing, C. A. Kurth, W. S. Hospodarsky, G. B. Spence, H. E. Reeves, G. D. Funsten, H. O. Blake, J. B. Baker, D. N. Wygant, J. R. TI Excitation of nightside magnetosonic waves observed by Van Allen Probes SO JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS LA English DT Article DE RBSP results; magnetosonic wave; wave-particle interaction ID PROTON RING DISTRIBUTIONS; RADIATION-BELT ELECTRONS; RELATIVISTIC ELECTRONS; EQUATORIAL NOISE; ACCELERATION; GENERATION; CHORUS; MODEL; STORM AB During the recovery phase of the geomagnetic storm on 30-31 March 2013, Van Allen Probe A detected enhanced magnetosonic (MS) waves in a broad range of L = 1.8-4.7 and magnetic local time (MLT) = 17-22 h, with a frequency range approximate to 10-100 Hz. In the meanwhile, distinct proton ring distributions with peaks at energies of approximate to 10 keV, were also observed in L = 3.2-4.6 and L = 5.0-5.6. Using a subtracted bi-Maxwellian distribution to model the observed proton ring distribution, we perform three-dimensional ray tracing to investigate the instability, propagation, and spatial distribution of MS waves. Numerical results show that nightside MS waves are produced by proton ring distribution and grow rapidly from the source location L = 5.6 to the location L = 5.0 but remain nearly stable at locations L < 5.0. Moreover, waves launched toward lower L shells with different initial azimuthal angles propagate across different MLT regions with divergent paths at first, then gradually turn back toward higher L shells and propagate across different MLT regions with convergent paths. The current results further reveal that MS waves are generated by a ring distribution of approximate to 10 keV proton and proton ring in one region can contribute to the MS wave power in another region. C1 [Zhou, Qinghua; Xiao, Fuliang; Yang, Chang; Liu, Si] Changsha Univ Sci & Technol, Sch Phys & Elect Sci, Changsha, Hunan, Peoples R China. [Kletzing, C. A.; Kurth, W. S.; Hospodarsky, G. B.] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA. [Spence, H. E.] Univ New Hampshire, Inst Study Earth Oceans & Space, Durham, NH 03824 USA. [Reeves, G. D.] Los Alamos Natl Lab, Space Sci & Applicat Grp, Los Alamos, NM USA. [Funsten, H. O.] Los Alamos Natl Lab, ISR Div, Los Alamos, NM USA. [Blake, J. B.] Aerosp Corp, Los Angeles, CA 90009 USA. [Baker, D. N.] Univ Colorado, Lab Atmospher & Space Phys, Boulder, CO 80309 USA. [Wygant, J. R.] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA. RP Xiao, FL (reprint author), Changsha Univ Sci & Technol, Sch Phys & Elect Sci, Changsha, Hunan, Peoples R China. EM flxiao@126.com RI Xiao, Fuliang/B-9245-2011; Reeves, Geoffrey/E-8101-2011; OI Xiao, Fuliang/0000-0003-1487-6620; Reeves, Geoffrey/0000-0002-7985-8098; Kletzing, Craig/0000-0002-4136-3348; Funsten, Herbert/0000-0002-6817-1039; Kurth, William/0000-0002-5471-6202; Hospodarsky, George/0000-0001-9200-9878 FU 973 Program [2012CB825603]; National Natural Science Foundation of China [41204114, 41274165]; Aid Program for Science and Technology Innovative Research Team in Higher Educational Institutions of Hunan Province; Construct Program of the Key Discipline in Hunan Province; JHU/APL [921647, 967399]; JHU/APL under NASA [NAS5-01072] FX This work is supported by 973 Program 2012CB825603, the National Natural Science Foundation of China grants 41204114 and 41274165, the Aid Program for Science and Technology Innovative Research Team in Higher Educational Institutions of Hunan Province, and the Construct Program of the Key Discipline in Hunan Province. All the Van Allen Probes data are publicly available at https://emfisis.physics.uiowa.edu/data/index by the EMFISIS instrument and at http://www.rbsp-ect.lanl.gov/data_pub/ by the HOPE instrument. This work was also supported from JHU/APL contracts 921647 and 967399 under NASA Prime contract NAS5-01072. NR 39 TC 9 Z9 9 U1 3 U2 14 PU AMER GEOPHYSICAL UNION PI WASHINGTON PA 2000 FLORIDA AVE NW, WASHINGTON, DC 20009 USA SN 2169-9380 EI 2169-9402 J9 J GEOPHYS RES-SPACE JI J. Geophys. Res-Space Phys. PD NOV PY 2014 VL 119 IS 11 BP 9125 EP 9133 DI 10.1002/2014JA020481 PG 9 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA AX2RO UT WOS:000346792100029 ER PT J AU Nica, N AF Nica, N. TI Nuclear Data Sheets for A=141 SO NUCLEAR DATA SHEETS LA English DT Article ID DELAYED-NEUTRON EMISSION; HALF-LIFE MEASUREMENTS; GAMMA-RAY ENERGIES; ISOBARIC ANALOG RESONANCES; PHOTONEUTRON CROSS-SECTION; GASEOUS FISSION-PRODUCTS; PROTON DRIP-LINE; HIGH-SPIN STATES; CIRCULAR-POLARIZATION CORRELATION; SINGLE-PARTICLE ENERGIES AB Nuclear spectroscopic information for experimentally investigated nuclides of mass 141 (To, I, Xe, Cs, Ba, La, Ce, Pr, Nd, Pm, Sm, Eu, Gd, Tb, Dy, and Ho) has been evaluated. A summary of information obtained in various reaction and decay experiments is presented, together with data tables and adopted level schemes. C1 [Nica, N.] Texas A&M Univ, Inst Cyclotron, College Stn, TX 77843 USA. [Nica, N.] Brookhaven Natl Lab, Subcontract Natl Nucl Data Ctr 100586, Upton, NY 11973 USA. RP Nica, N (reprint author), Texas A&M Univ, Inst Cyclotron, College Stn, TX 77843 USA. FU Office of Nuclear Physics, Office Science of the DOE of the United States FX Work supported by the Office of Nuclear Physics, Office Science of the DOE of the United States. NR 455 TC 2 Z9 2 U1 0 U2 1 PU ACADEMIC PRESS INC ELSEVIER SCIENCE PI SAN DIEGO PA 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA SN 0090-3752 EI 1095-9904 J9 NUCL DATA SHEETS JI Nucl. Data Sheets PD NOV-DEC PY 2014 VL 122 BP 1 EP 204 DI 10.1016/j.nds.2014.11.001 PG 204 WC Physics, Nuclear SC Physics GA AX6GB UT WOS:000347020000001 ER PT J AU Browne, E Tuli, JK AF Browne, E. Tuli, J. K. TI Nuclear Data Sheets for A=235 SO NUCLEAR DATA SHEETS LA English DT Article ID NEUTRON-DEFICIENT ISOTOPE; ALPHA-PARTICLE SPECTRA; ELECTRON-CAPTURE DECAY; CHARGE RADII CHANGES; MUON-INDUCED FISSION; HALF-LIVES; URANIUM ISOTOPES; EMISSION PROBABILITIES; CROSS-SECTIONS; CLUSTER RADIOACTIVITY AB Spectroscopic data and level schemes from radioactive decay and nuclear reaction studies are presented here for all nuclei with mass number A=235. The highlight of this evaluation consists of the precise and comprehensive Coulomb excitation study (2012Wa35) on U-235, which in addition to the 712[743] ground state rotational band, extended the 1/2[631], 5/216221, 5/2[752], and 3/2[631] rotational bands up to J pi=53/2+, 49/2+, 41/2-, and 43/2+, respectively. This evaluation presents a study (2010Hu02) of the Np-237(Sn-116,Sn-118 gamma) reaction where the ground state rotational band 5/2[642] was observed up to J pi(53/2+). It is worth for historical knowledge to mention the report on the "Discovery of isotopes of the transuranium elements with 93<= Z <=98 " (2013Fr02), where the information for elements Np, Pu, and Am with mass number A= 235 is given. Cf-235 has not been observed. The alpha hindrance factors (HP) presented in this evaluation were calculated using values of the radius parameter (r(0)) interpolated from those for even-even adjacent nuclei given by 1998Ak04. C1 [Browne, E.] Brookhaven Natl Lab, Lawrence Berkeley Natl Lab, Subcontract Natl Nucl Data Ctr, Upton, NY 11973 USA. [Tuli, J. K.] Brookhaven Natl Lab, Natl Nucl Data Ctr, Upton, NY 11973 USA. RP Browne, E (reprint author), Brookhaven Natl Lab, Lawrence Berkeley Natl Lab, Subcontract Natl Nucl Data Ctr, Upton, NY 11973 USA. FU Office of Nuclear Physics, Office of Science, US Department of Energy [DE-AC02-98CH10946] FX Research sponsored by Office of Nuclear Physics, Office of Science, US Department of Energy, under contract DE-AC02-98CH10946. NR 261 TC 2 Z9 2 U1 2 U2 8 PU ACADEMIC PRESS INC ELSEVIER SCIENCE PI SAN DIEGO PA 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA SN 0090-3752 EI 1095-9904 J9 NUCL DATA SHEETS JI Nucl. Data Sheets PD NOV-DEC PY 2014 VL 122 BP 205 EP 291 DI 10.1016/j.nds.2014.11.002 PG 87 WC Physics, Nuclear SC Physics GA AX6GB UT WOS:000347020000002 ER PT J AU Browne, E Tuli, JK AF Browne, E. Tuli, J. K. TI Nuclear Data Sheets for A=239 SO NUCLEAR DATA SHEETS LA English DT Article ID CAPTURE CROSS-SECTION; SPONTANEOUSLY FISSIONING ISOMERS; INTERNAL-CONVERSION COEFFICIENTS; PARTICLE-EMISSION PROBABILITIES; GAMMA-ANGULAR CORRELATIONS; NEUTRON-INDUCED FISSION; RANGE 0.01-6 MEV; HALF-LIVES; ALPHA-DECAY; ENERGY-RANGE AB Spectroscopic data and level schemes from radioactive decay and nuclear reaction studies are presented here for all nuclei with mass number A=239. In general, a relatively small amount of new data on this mass chain has been reported since the previous evaluation in 2003. However, special evaluations, such as "Database of prompt gamma rays from slow neutron-capture from elemental analysis" (2007ChZX), have provided additional precise data for levels in U-239. Also, new Coulomb excitation measurements in Pu-239 have extended the knowledge of the 1/2[631] rotational band up to J pi(55/2+), and that of the octupole vibrational band up to J pi=(53/2-). For historical knowledge it is worth mentioning the report on the "Discovery of isotopes of the transuranium elements with 93<= Z <=98" (2013Fr02), where the information for elements Np, Pu, Am, and Cf with mass number A=239 is presented. The alpha hindrance factors (HF) presented in this evaluation were calculated using values of the radius parameter (r(0)) interpolated from those for even-even adjacent nuclei given by 1998Ak04. C1 [Browne, E.] Brookhaven Natl Lab, Lawrence Berkeley Natl Lab, Subcontract Natl Nucl Data Ctr, Upton, NY 11973 USA. [Tuli, J. K.] Brookhaven Natl Lab, Natl Nucl Data Ctr, Upton, NY 11973 USA. RP Browne, E (reprint author), Brookhaven Natl Lab, Lawrence Berkeley Natl Lab, Subcontract Natl Nucl Data Ctr, Upton, NY 11973 USA. FU Office of Nuclear Physics, Office of Science, US Department of Energy [DE-AC02-98CH10946] FX Research sponsored by Office of Nuclear Physics, Office of Science, US Department of Energy, under contract DE-AC02-98CH10946. NR 324 TC 3 Z9 3 U1 1 U2 7 PU ACADEMIC PRESS INC ELSEVIER SCIENCE PI SAN DIEGO PA 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA SN 0090-3752 EI 1095-9904 J9 NUCL DATA SHEETS JI Nucl. Data Sheets PD NOV-DEC PY 2014 VL 122 BP 293 EP 375 DI 10.1016/j.nds.2014.11.003 PG 83 WC Physics, Nuclear SC Physics GA AX6GB UT WOS:000347020000003 ER PT J AU Martin, MJ AF Martin, M. J. TI Nuclear Data Sheets for A=248 SO NUCLEAR DATA SHEETS LA English DT Article ID INELASTIC DEUTERON SCATTERING; LIGHT EINSTEINIUM ISOTOPES; ALPHA-DECAY PROPERTIES; SPONTANEOUS-FISSION; HALF-LIVES; COULOMB-EXCITATION; ACTINIDE NUCLEI; CROSS-SECTIONS; EVEN NUCLEI; HIGH-SPIN AB Detailed level schemes, decay schemes, and the experimental data on which they are based are presented for all nuclei with mass number A=248. The experimental reaction and decay data are evaluated; inconsistencies and discrepancies are noted; and adopted values are given for various level properties (including spin and parity, halflife, and configuration), gamma properties (including energy, intensity, and multipole character) and alpha properties (including energy, intensity, and hindrance factor). This evaluation replaces the A=248 evaluation published by A. Akovali in Nuclear Data Sheets 87, 249 (1999). C1 Oak Ridge Natl Lab, Oak Ridge, TN 37831 USA. RP Martin, MJ (reprint author), Oak Ridge Natl Lab, Oak Ridge, TN 37831 USA. FU Office of Nuclear Physics, Office of Science, US Department of Energy [DE-AC05-00OR22725] FX Research sponsored by the Office of Nuclear Physics, Office of Science, US Department of Energy under contract DE-AC05-00OR22725. NR 72 TC 2 Z9 2 U1 0 U2 0 PU ACADEMIC PRESS INC ELSEVIER SCIENCE PI SAN DIEGO PA 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA SN 0090-3752 EI 1095-9904 J9 NUCL DATA SHEETS JI Nucl. Data Sheets PD NOV-DEC PY 2014 VL 122 BP 377 EP 409 DI 10.1016/j.nds.2014.11.004 PG 33 WC Physics, Nuclear SC Physics GA AX6GB UT WOS:000347020000004 ER PT J AU Leonard, EM Plummer, MA Carrara, PE AF Leonard, Eric M. Plummer, Mitchell A. Carrara, Paul E. TI Numerical modeling of the Snowmass Creek paleoglacier, Colorado, and climate in the Rocky Mountains during the Bull Lake glaciation (MIS 6) SO QUATERNARY RESEARCH LA English DT Article DE Numerical glacier modeling; Rocky Mountains; Bull Lake glaciation; Paleoclimate; MIS 6 ID SOUTHERN SAWATCH RANGE; LATE-PLEISTOCENE; ICE-FLOW; UINTA MOUNTAINS; UNITED-STATES; GLACIER; MAXIMUM; INFERENCES; RECONSTRUCTION; COMPLEX AB Well-preserved moraines from the penultimate, or Bull Lake, glaciation of Snowmass Creek Valley in the Elk Range of Colorado (USA) present an opportunity to examine the character of the high-altitude climate in the Rocky Mountains during Marine Oxygen Isotope Stage 6. This study employs a 2-D coupled mass/energy balance and flow model to assess the magnitudes of temperature and precipitation change that could have sustained the glacier in mass-balance equilibrium at its maximum extent during the Bull Lake glaciation. Variable substrate effects on glacier flow and ice thickness make the modeling somewhat more complex than in geologically simpler settings. Model results indicate that a temperature depression of about 6.7 degrees C compared with the present (1971-2000 AD) would have been necessary to sustain the Snowmass Creek glacier in mass-balance equilibrium during the Bull Lake glaciation, assuming no change in precipitation amount or seasonality. A 50% increase or decrease from modern precipitation would have been coupled with 5.2 degrees C and 9.1 degrees C Bull Lake temperature depressions respectively. Uncertainty in these modeled temperature depressions is about 1 degrees C. (C) 2014 University of Washington. Published by Elsevier Inc All rights reserved. C1 [Leonard, Eric M.] Colorado Coll, Dept Geol, Colorado Springs, CO 80903 USA. [Plummer, Mitchell A.] Idaho Natl Lab, Idaho Falls, ID 83415 USA. [Carrara, Paul E.] US Geol Survey, Denver Fed Ctr, Denver, CO 80225 USA. RP Leonard, EM (reprint author), Colorado Coll, Dept Geol, Colorado Springs, CO 80903 USA. EM eleonard@coloradocollege.edu NR 30 TC 5 Z9 5 U1 0 U2 2 PU ACADEMIC PRESS INC ELSEVIER SCIENCE PI SAN DIEGO PA 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA SN 0033-5894 EI 1096-0287 J9 QUATERNARY RES JI Quat. Res. PD NOV PY 2014 VL 82 IS 3 BP 533 EP 541 DI 10.1016/j.yqres.2014.03.001 PG 9 WC Geography, Physical; Geosciences, Multidisciplinary SC Physical Geography; Geology GA AX5DB UT WOS:000346946100006 ER PT J AU Miller, IM Pigati, JS Anderson, RS Johnson, KR Mahan, SA Ager, TA Baker, RG Blaauw, M Bright, J Brown, PM Bryant, B Calamari, ZT Carrara, PE Cherney, MD Demboski, JR Elias, SA Fisher, DC Gray, HJ Haskett, DR Honke, JS Jackson, ST Jimenez-Moreno, G Kline, D Leonard, EM Lifton, NA Lucking, C McDonald, HG Miller, DM Muhs, DR Nash, SE Newton, C Paces, JB Petrie, L Plummer, MA Porinchu, DF Rountrey, AN Scott, E Sertich, JJW Sharpe, SE Skipp, GL Strickland, LE Stucky, RK Thompson, RS Wilson, J AF Miller, Ian M. Pigati, Jeffrey S. Anderson, R. Scott Johnson, Kirk R. Mahan, Shannon A. Ager, Thomas A. Baker, Richard G. Blaauw, Maarten Bright, Jordon Brown, Peter M. Bryant, Bruce Calamari, Zachary T. Carrara, Paul E. Cherney, Michael D. Demboski, John R. Elias, Scott A. Fisher, Daniel C. Gray, Harrison J. Haskett, Danielle R. Honke, Jeffrey S. Jackson, Stephen T. Jimenez-Moreno, Gonzalo Kline, Douglas Leonard, Eric M. Lifton, Nathaniel A. Lucking, Carol McDonald, H. Gregory Miller, Dane M. Muhs, Daniel R. Nash, Stephen E. Newton, Cody Paces, James B. Petrie, Lesley Plummer, Mitchell A. Porinchu, David F. Rountrey, Adam N. Scott, Eric Sertich, Joseph J. W. Sharpe, Saxon E. Skipp, Gary L. Strickland, Laura E. Stucky, Richard K. Thompson, Robert S. Wilson, Jim TI Summary of the Snowmastodon Project Special Volume A high-elevation, multi-proxy biotic and environmental record of MIS 6-4 from the Ziegler Reservoir fossil site, Snowmass Village, Colorado, USA SO QUATERNARY RESEARCH LA English DT Article DE Rocky Mountains; Sangamon interglacial; Paleoclimate; Ziegler Reservoir; Marine Oxygen Isotope Stage; Mammut americanum; Mammuthus columbi ID LAST INTERGLACIAL PERIOD; SCALE CLIMATE VARIABILITY; MARINE ISOTOPE STAGE-11; NORTH-AMERICA; MILLENNIAL-SCALE; POLLEN RECORD; ORBITAL-SCALE; UNITED-STATES; DEVILS-HOLE; DEEP-OCEAN AB In North America, terrestrial records of biodiversity and climate change that span Marine Oxygen Isotope Stage (MIS) 5 are rare. Where found, they provide insight into how the coupling of the ocean-atmosphere system is manifested in biotic and environmental records and how the biosphere responds to climate change. In 2010-2011, construction at Ziegler Reservoir near Snowmass Village, Colorado (USA) revealed a nearly continuous, lacustrine/wetland sedimentary sequence that preserved evidence of past plant communities between similar to 140 and 55 lea, including all of MIS 5. At an elevation of 2705 m, the Ziegler Reservoir fossil site also contained thousands of well-preserved bones of late Pleistocene megafauna, including mastodons, mammoths, ground sloths, horses, camels, deer, bison, black bear, coyotes, and bighorn sheep. In addition, the site contained more than 26,000 bones from at least 30 species of small animals including salamanders, otters, muskrats, minks, rabbits, beavers, frogs, lizards, snakes, fish, and birds. The combination of macro- and micro-vertebrates, invertebrates, terrestrial and aquatic plant macrofossils, a detailed pollen record, and a robust, directly dated stratigraphic framework shows that high-elevation ecosystems in the Rocky Mountains of Colorado are climatically sensitive and varied dramatically throughout MIS 5. (C) 2014 University of Washington. Published by Elsevier Inc. All rights reserved. C1 [Miller, Ian M.; Johnson, Kirk R.; Demboski, John R.; Kline, Douglas; Lucking, Carol; Nash, Stephen E.; Sertich, Joseph J. W.] Denver Museum Nat & Sci, Denver, CO 80205 USA. [Pigati, Jeffrey S.; Mahan, Shannon A.; Ager, Thomas A.; Carrara, Paul E.; Gray, Harrison J.; Honke, Jeffrey S.; Muhs, Daniel R.; Paces, James B.; Strickland, Laura E.; Thompson, Robert S.] US Geol Survey, Denver Fed Ctr, Denver, CO 80225 USA. [Anderson, R. Scott] No Arizona Univ, Sch Earth Sci & Environm Sustainabil, Flagstaff, AZ 86011 USA. [Johnson, Kirk R.] Smithsonian Inst, Natl Museum Nat Hist, Washington, DC 20013 USA. [Baker, Richard G.] Univ Iowa, Dept Earth & Environm Sci, Iowa City, IA 52242 USA. [Blaauw, Maarten] Queens Univ Belfast, Sch Geog Archaeol & Palaeoecol, Belfast BT7 1NN, Antrim, North Ireland. [Bright, Jordon] Univ Arizona, Dept Geosci, Tucson, AZ 85721 USA. Rocky Mt Tree Ring Res, Ft Collins, CO 80526 USA. [Calamari, Zachary T.; Cherney, Michael D.; Fisher, Daniel C.] Univ Michigan, Dept Earth & Environm Sci, Ann Arbor, MI 48109 USA. [Elias, Scott A.] Univ London, Dept Geog, Egham TW20 0EX, Surrey, England. [Calamari, Zachary T.; Cherney, Michael D.; Fisher, Daniel C.; Rountrey, Adam N.] Univ Michigan, Museum Paleontol, Ann Arbor, MI 48109 USA. [Haskett, Danielle R.; Porinchu, David F.] Univ Georgia, Dept Geog, Athens, GA 30602 USA. [Jackson, Stephen T.; Miller, Dane M.] Univ Wyoming, Dept Bot, Laramie, WY 82071 USA. [Jackson, Stephen T.] Univ Arizona, Inst Environm, Southwest Climate Sci Ctr, Tucson, AZ 85719 USA. [Jimenez-Moreno, Gonzalo] Univ Granada, Dept Estratig & Paleontol, Granada 18002, Spain. [Leonard, Eric M.] Colorado Coll, Dept Geol, Colorado Springs, CO 80903 USA. [Lifton, Nathaniel A.] Purdue Univ, Dept Earth Atmospher & Planetary Sci, W Lafayette, IN 47907 USA. [McDonald, H. Gregory; Stucky, Richard K.] Natl Pk Serv, Museum Management Program, Ft Collins, CO 80525 USA. [Newton, Cody] Univ Colorado, Dept Anthropol, Boulder, CO 80309 USA. [Petrie, Lesley] Univ Calif Santa Cruz, Dept Earth & Planetary Sci, Santa Cruz, CA 95064 USA. [Plummer, Mitchell A.] Idaho Natl Lab, Idaho Falls, ID 83415 USA. [Rountrey, Adam N.] Univ Western Australia, Oceans Inst, Ctr Marine Futures, Crawley, WA 6009, Australia. [Scott, Eric] San Bernardino Cty Museum, Redlands, CA 92374 USA. [Sharpe, Saxon E.] Desert Res Inst, Reno, NV 89512 USA. [Wilson, Jim] Aeon Labs LLC, Tucson, AZ 85704 USA. RP Miller, IM (reprint author), Denver Museum Nat & Sci, 2001 Colorado Blvd, Denver, CO 80205 USA. EM ian.miller@dmns.org RI Lifton, Nathaniel/M-2017-2015; OI Lifton, Nathaniel/0000-0002-6976-3298; Gray, Harrison/0000-0002-4555-7473; Mahan, Shannon/0000-0001-5214-7774; Rountrey, Adam/0000-0003-0939-9102; Demboski, John/0000-0002-5163-4113 NR 61 TC 4 Z9 4 U1 2 U2 17 PU ACADEMIC PRESS INC ELSEVIER SCIENCE PI SAN DIEGO PA 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA SN 0033-5894 EI 1096-0287 J9 QUATERNARY RES JI Quat. Res. PD NOV PY 2014 VL 82 IS 3 BP 618 EP 634 DI 10.1016/j.yqres.2014.07.004 PG 17 WC Geography, Physical; Geosciences, Multidisciplinary SC Physical Geography; Geology GA AX5DB UT WOS:000346946100014 ER PT J AU Smith, RJ Stavitski, E Carr, GL AF Smith, R. J. Stavitski, E. Carr, G. L. TI Performance of an optical stabilization system at NSLS beamline U12IR SO VIBRATIONAL SPECTROSCOPY LA English DT Article; Proceedings Paper CT 7th International Workshop on Infrared Microscopy and Spectroscopy with Accelerator-Based Sources (WIRMS) CY NOV 10-13, 2014 CL Melbourne, AUSTRALIA DE Beam stabilization; Dynamic mirror; Feedback Noise reduction; Infrared synchrotron beamline AB A low-cost optical feedback system using dynamic mirrors has been developed at the NSLS for stabilizing the position and direction of an infrared synchrotron beam against thermal drift and mechanical noise. The system design has some unique features that potentially simplify installation into an existing infrared beamline. We describe the system and its features along with some performance results. (C) 2014 Elsevier B.V. All rights reserved. C1 [Smith, R. J.; Stavitski, E.; Carr, G. L.] Brookhaven Natl Lab, Photon Sci, Upton, NY 11973 USA. RP Smith, RJ (reprint author), Brookhaven Natl Lab, Photon Sci, Upton, NY 11973 USA. NR 3 TC 0 Z9 0 U1 0 U2 0 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0924-2031 EI 1873-3697 J9 VIB SPECTROSC JI Vib. Spectrosc. PD NOV PY 2014 VL 75 BP 118 EP 122 DI 10.1016/j.vibspec.2014.09.003 PG 5 WC Chemistry, Analytical; Chemistry, Physical; Spectroscopy SC Chemistry; Spectroscopy GA AX6HA UT WOS:000347022400015 ER PT J AU Zhang, S Gao, HL Naz, BS AF Zhang, Shuai Gao, Huilin Naz, Bibi S. TI Monitoring reservoir storage in South Asia from multisatellite remote sensing SO WATER RESOURCES RESEARCH LA English DT Article ID DIFFERENCE WATER INDEX; SATELLITE IMAGERY; RADAR ALTIMETER; LEVEL CHANGES; LAKES; SERIES; MODEL; LAND AB Reservoir storage information is essential for accurate flood monitoring and prediction. South Asia, however, is dominated by international river basins where communications among neighboring countries about reservoir storage and management are extremely limited. A suite of satellite observations were combined to achieve high-quality estimation of reservoir storage and storage variations in South Asia from 2000 to 2012. The approach used water surface area estimations from the Moderate Resolution Imaging Spectroradiometer (MODIS) vegetation indices product and the area-elevation relationship to estimate reservoir storage. The surface elevation measurements were from the Geoscience Laser Altimeter System (GLAS) on board the Ice, Cloud, and land Elevation Satellite (ICESat). In order to improve the accuracy of water surface area estimations for relatively small reservoirs, a novel classification algorithm was developed. In this study, storage information was retrieved for a total of 21 reservoirs, which represents 28% of the integrated reservoir capacity in South Asia. The satellite-based reservoir elevation and storage were validated by gauge observations over five reservoirs. The storage estimates were highly correlated with observations (i.e., coefficients of determination larger than 0.9), with normalized root mean square error (NRMSE) ranging from 9.51% to 25.20%. Uncertainty analysis was also conducted for the remotely sensed storage estimations. For the parameterization uncertainty associated with surface area retrieval, the storage mean relative error was 3.90%. With regard to the uncertainty introduced by ICESat/GLAS elevation measurements, the storage mean relative error was 0.67%. C1 [Zhang, Shuai; Gao, Huilin] Texas A&M Univ, Zachry Dept Civil Engn, College Stn, TX 77843 USA. [Naz, Bibi S.] Oak Ridge Natl Lab, Oak Ridge, TN USA. RP Gao, HL (reprint author), Texas A&M Univ, Zachry Dept Civil Engn, College Stn, TX 77843 USA. EM hgao@civil.tamu.edu OI Naz, Bibi/0000-0001-9888-1384 FU Texas A&M University College of Engineering; Zachry Department of Civil Engineering FX The remotely sensed reservoir data used in this study are available through the Land Surface Hydrology Research Group's website at Texas A&M University (https://ceprofs.civil.tamu.edu/hgao/). This work was supported by startup funds from the Texas A&M University College of Engineering and the Zachry Department of Civil Engineering. It has benefitted from the usage of the Texas A&M Supercomputing Facility (http://sc.tamu.edu). The authors would also like to thank David Kroodsma for his valuable comments during the early stage of this study and Huan Wu for his comments about the results. We acknowledge the three reviewers and the handling Editor for their constructive comments which greatly improved the paper. NR 43 TC 12 Z9 12 U1 5 U2 24 PU AMER GEOPHYSICAL UNION PI WASHINGTON PA 2000 FLORIDA AVE NW, WASHINGTON, DC 20009 USA SN 0043-1397 EI 1944-7973 J9 WATER RESOUR RES JI Water Resour. Res. PD NOV PY 2014 VL 50 IS 11 BP 8927 EP 8943 DI 10.1002/2014WR015829 PG 17 WC Environmental Sciences; Limnology; Water Resources SC Environmental Sciences & Ecology; Marine & Freshwater Biology; Water Resources GA AX0PQ UT WOS:000346654600030 ER PT J AU Weaver, BP Meeker, WQ AF Weaver, Brian P. Meeker, William Q. TI Methods for planning repeated measures accelerated degradation tests SO APPLIED STOCHASTIC MODELS IN BUSINESS AND INDUSTRY LA English DT Article DE nondestructive degradation; mixed-effects linear models; accelerated degradation testing; general equivalence theorem ID EXPERIMENTAL-DESIGN AB Repeated measures accelerated degradation tests can sometimes be used to assess product or component reliability when one would expect few or even no failures during a study. Such tests can be used to estimate the lifetime distributions of highly reliable items. This paper describes methods for selecting a single-variable accelerated repeated measures degradation test plan when the (possibly transformed) degradation that is linear in (possibly transformed) time and unit-to-unit variability is described by a random-effects model. To find optimum test plans, we use a criterion based on a large-sample approximation to the estimation precision of a quantile of the failure-time distribution at use conditions. We also discuss how to find compromise test plans that satisfy practical constraints. We use the general equivalence theorem to verify that a test plan is globally optimum. The resulting optimized plans are also evaluated using simulation and compared with other test plans. Copyright (c) 2014 John Wiley & Sons, Ltd. C1 [Weaver, Brian P.] Los Alamos Natl Lab, Los Alamos, NM 87544 USA. [Meeker, William Q.] Iowa State Univ, Dept Stat, Ames, IA 50010 USA. RP Weaver, BP (reprint author), Los Alamos Natl Lab, CCS-6, Los Alamos, NM 87544 USA. EM theguz@lanl.gov NR 22 TC 1 Z9 1 U1 0 U2 14 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 1524-1904 EI 1526-4025 J9 APPL STOCH MODEL BUS JI Appl. Stoch. Models. Bus. Ind. PD NOV-DEC PY 2014 VL 30 IS 6 BP 658 EP 671 DI 10.1002/asmb.2061 PG 14 WC Operations Research & Management Science; Mathematics, Interdisciplinary Applications; Statistics & Probability SC Operations Research & Management Science; Mathematics GA AX2HW UT WOS:000346765100002 ER PT J AU Weaver, BP Meeker, WQ AF Weaver, Brian P. Meeker, William Q. TI Rejoinder: Methods for planning repeated measures accelerated degradation tests SO APPLIED STOCHASTIC MODELS IN BUSINESS AND INDUSTRY LA English DT Article ID LIFE TESTS C1 [Weaver, Brian P.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA. [Meeker, William Q.] Iowa State Univ, Dept Stat, Ames, IA USA. RP Weaver, BP (reprint author), Los Alamos Natl Lab, CCS 6, Los Alamos, NM 87545 USA. EM theguz@lanl.gov; wqmeeker@iastate.edu NR 10 TC 0 Z9 0 U1 1 U2 6 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 1524-1904 EI 1526-4025 J9 APPL STOCH MODEL BUS JI Appl. Stoch. Models. Bus. Ind. PD NOV-DEC PY 2014 VL 30 IS 6 BP 686 EP 690 DI 10.1002/asmb.2096 PG 5 WC Operations Research & Management Science; Mathematics, Interdisciplinary Applications; Statistics & Probability SC Operations Research & Management Science; Mathematics GA AX2HW UT WOS:000346765100007 ER PT J AU Wiel, SV Bent, R Casleton, E Lawrence, E AF Wiel, Scott Vander Bent, Russell Casleton, Emily Lawrence, Earl TI Identification of topology changes in power grids using phasor measurements SO APPLIED STOCHASTIC MODELS IN BUSINESS AND INDUSTRY LA English DT Article DE electric power; state estimation; PMU; change detection ID STATE ESTIMATION; ERROR IDENTIFICATION AB Phasor measurement units (PMUs) are increasingly important for monitoring the state of an electrical power grid and quickly detecting topology changes caused by events such as lines going down or large loads being dropped. Phasors are complex-valued measurements of voltage and current at various points of generation and consumption. If a line goes down or a load is removed, power flows change throughout the grid according to known physical laws, and the probability distribution of phasor measurements changes accordingly. This paper develops a method to estimate the current topology of a power grid from phasor measurements and considers the design goal of placing PMUs at strategic points in a distribution system to achieve good sensitivity to single-line outages. From a vector of phasor measurements, probabilities are computed corresponding to the scenario that all power lines are operational and to alternate scenarios in which each line goes down individually. These probabilities are functions of the joint distributions of phasor measurements under each possible scenario, obtained through Monte Carlo simulations with random load profiles. We use log-spline densities to estimate marginal distributions of phasor measurements and fold these into a multivariate Gaussian copula to capture important correlations. Sensitivity to outages varies according to which line goes down and where PMUs are placed on the grid. A greedy search algorithm is demonstrated for placing PMUs at locations that provide good sensitivity to single-line outages. Published 2014. This article is a U.S. Government work and is in the public domain in the USA. C1 [Wiel, Scott Vander; Casleton, Emily] Los Alamos Natl Lab, Stat Sci Grp, Los Alamos, NM 87545 USA. [Bent, Russell; Lawrence, Earl] Los Alamos Natl Lab, Los Alamos, NM 87545 USA. [Casleton, Emily] Iowa State Univ, Dept Stat, Ames, IA USA. RP Wiel, SV (reprint author), Los Alamos Natl Lab, Stat Sci Grp, MS F600, Los Alamos, NM 87545 USA. EM scottv@lanl.gov OI Bent, Russell/0000-0002-7300-151X NR 28 TC 0 Z9 0 U1 1 U2 5 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 1524-1904 EI 1526-4025 J9 APPL STOCH MODEL BUS JI Appl. Stoch. Models. Bus. Ind. PD NOV-DEC PY 2014 VL 30 IS 6 BP 740 EP 752 DI 10.1002/asmb.2082 PG 13 WC Operations Research & Management Science; Mathematics, Interdisciplinary Applications; Statistics & Probability SC Operations Research & Management Science; Mathematics GA AX2HW UT WOS:000346765100011 ER PT J AU Beresnyak, A AF Beresnyak, Andrey TI Asymmetric diffusion of magnetic field lines in turbulence SO PHYSICA SCRIPTA LA English DT Article; Proceedings Paper CT 11th International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas CY AUG 05-09, 2013 CL Mons, BELGIUM DE turbulence; diffusion; plasma ID MAGNETOHYDRODYNAMIC TURBULENCE AB Stochasticity of magnetic field lines is paramount to understanding particle transport and mixing (Rechester and Rosenbluth 1978 Phys. Rev. Lett. 40 38-41). In this paper we study magnetic field separation in turbulent plasmas, which feature so-called superdiffusion, where field lines separate faster than diffusively. We discovered that turbulent superdiffusion can be pronouncedly asymmetric, so that the separation of field lines will be different if one follows magnetic field lines along the direction of the field or follows them in the opposite direction. Particle transport perpendicular to the magnetic field is primarily due to the field line separation in collisionless, well-magnetized plasmas. The asymmetry in diffusion, however, was certainly unexpected, as it will create free energy in particles that follow field lines, e. g. it will create large-scale streaming out of particle gradients perpendicular to the mean magnetic field. While the symmetry of the flow is broken by the so-called imbalance or cross-helicity, the difference between forward and backward diffusion is not directly due to imbalance, but a non-trivial consequence of both imbalance and non-reversibility of turbulence. It therefore follows that this peculiar property of field lines is directly related to turbulence being a dissipative phenomenon, and that turbulence can directly channel part of its free energy to particles. C1 Los Alamos Natl Lab, Los Alamos, NM 87545 USA. RP Beresnyak, A (reprint author), Los Alamos Natl Lab, POB 1663, Los Alamos, NM 87545 USA. NR 12 TC 1 Z9 1 U1 0 U2 0 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0031-8949 EI 1402-4896 J9 PHYS SCRIPTA JI Phys. Scr. PD NOV PY 2014 VL 89 IS 11 AR 118001 DI 10.1088/0031-8949/89/11/118001 PG 5 WC Physics, Multidisciplinary SC Physics GA AX0QK UT WOS:000346656500038 ER PT J AU Trabert, E AF Traebert, E. TI E1-forbidden transition rates in ions of astrophysical interest SO PHYSICA SCRIPTA LA English DT Article; Proceedings Paper CT 11th International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas CY AUG 05-09, 2013 CL Mons, BELGIUM DE oscillator strengths; lifetimes; visible and ultraviolet spectra; absolute and relative intensities ID ATOMIC LIFETIME MEASUREMENTS; HIGHLY-CHARGED IONS; STORAGE-RING; RADIATIVE LIFETIME; METASTABLE LEVELS; ISOELECTRONIC-SEQUENCES; GROUND-CONFIGURATION; DECAY-RATES; FE-X; FORBIDDEN TRANSITIONS AB Transition rates in atomic systems may appear to be of little importance in steady-state plasmas that are observed at great distances from Earth. However, some of the transition rates compete with collision rates, and in these cases certain line intensity ratios are affected and can serve as remote indicators of density. In the low-density environments of stellar coronae and planetary nebulae, the transition rates of interest are mostly spin-forbidden E1 decays, higher-multipole order transitions (M1, E2, M2, M3), and hyperfine-induced transitions. On Earth, measurements of the long upper level lifetimes of these atomic systems require the use of ion traps. A fair number of test cases with lifetimes in the range from nanoseconds to many seconds have been treated successfully, and the evolution of calculations along with the experimental progress is notable. A new generation of cold ion traps is expected to extend the atomic lifetime measurements on multiply charged ions into the range of many minutes. C1 [Traebert, E.] Ruhr Univ Bochum, Fak Phys & Astron, Astron Inst, D-44780 Bochum, Germany. [Traebert, E.] Lawrence Livermore Natl Lab, Div Phys, Livermore, CA 94550 USA. RP Trabert, E (reprint author), Ruhr Univ Bochum, Fak Phys & Astron, Astron Inst, D-44780 Bochum, Germany. EM traebert@astro.rub.de NR 130 TC 4 Z9 4 U1 0 U2 7 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0031-8949 EI 1402-4896 J9 PHYS SCRIPTA JI Phys. Scr. PD NOV PY 2014 VL 89 IS 11 AR 114003 DI 10.1088/0031-8949/89/11/114003 PG 14 WC Physics, Multidisciplinary SC Physics GA AX0QK UT WOS:000346656500003 ER PT J AU Tom, N Yeung, RW AF Tom, Nathan Yeung, Ronald W. TI Nonlinear Model Predictive Control Applied to a Generic Ocean-Wave Energy Extractor SO JOURNAL OF OFFSHORE MECHANICS AND ARCTIC ENGINEERING-TRANSACTIONS OF THE ASME LA English DT Article ID CONVERTERS; POWER AB This paper evaluates the theoretical application of nonlinear model predictive control (NMPC) to a model-scale point absorber for wave energy conversion. The NMPC strategy will be evaluated against a passive system, which utilizes no controller, using a performance metric based on the absorbed energy. The NMPC strategy was setup as a nonlinear optimization problem utilizing the interior point optimizer (IPOPT) package to obtain a time-varying optimal generator damping from the power-take-off (PTO) unit. This formulation is different from previous investigations in model predictive control, as the current methodology only allows the PTO unit to behave as a generator, thereby unable to return energy to the waves. Each strategy was simulated in the time domain for regular and irregular waves, the latter taken from a modified Pierson-Moskowitz spectrum. In regular waves, the performance advantages over a passive system appear at frequencies near resonance while at the lower and higher frequencies they become nearly equivalent. For irregular waves, the NMPC strategy leads to greater energy absorption than the passive system, though strongly dependent on the prediction horizon. It was found that the ideal NMPC strategy required a generator that could be turned on and off instantaneously, leading to sequences where the generator can be inactive for up to 50% of the wave period. C1 [Tom, Nathan] Univ Calif Berkeley, Dept Mech Engn, Ocean Engn Major Field Grp, Berkeley, CA 94720 USA. [Yeung, Ronald W.] Univ Calif Berkeley, Dept Mech Engn, Computat Marine Mech Lab CMML, Amer Bur Shipping,Inaugural Chair Ocean Engn, Berkeley, CA 94720 USA. RP Yeung, RW (reprint author), Natl Renewable Energy Lab, 15103 Denver W Pkwy, Golden, CO 80401 USA. EM nathan.m.tom@gmail.com; rwyeung@berkeley.edu FU American Bureau of Shipping FX We are grateful to Professor Francesco Borelli, S. Vichik, and T. Kelman from BLOM at UC Berkeley for their invaluable assistance and helpful discussions. Partial support for this research by the American Bureau of Shipping to the second author is gratefully acknowledged. NR 40 TC 9 Z9 9 U1 1 U2 6 PU ASME PI NEW YORK PA TWO PARK AVE, NEW YORK, NY 10016-5990 USA SN 0892-7219 EI 1528-896X J9 J OFFSHORE MECH ARCT JI J. Offshore Mech. Arct. Eng. Trans. ASME PD NOV PY 2014 VL 136 IS 4 AR UNSP 041901 DI 10.1115/1.4027651 PG 12 WC Engineering, Ocean; Engineering, Mechanical SC Engineering GA AX1GP UT WOS:000346696200015 ER PT J AU Durack, PJ Wijffels, SE Gleckler, PJ AF Durack, Paul J. Wijffels, Susan E. Gleckler, Peter J. TI Long-term sea-level change revisited: the role of salinity SO ENVIRONMENTAL RESEARCH LETTERS LA English DT Article DE oceanography; sea level; salinity; climate model; CMIP5; global change; water cycle ID EQUATION-OF-STATE; ICE-SHEET; CYCLE INTENSIFICATION; OCEAN SALINITIES; WATER CYCLE; RISE; TRENDS; TEMPERATURE; VARIABILITY; SIMULATIONS AB Of the many processes contributing to long-term sea-level change, little attention has been paid to the large-scale contributions of salinity-driven halosteric changes. We evaluate observed and simulated estimates of long-term (1950-present) halosteric patterns and compare these to corresponding thermosteric changes. Spatially coherent halosteric patterns are visible in the historical record, and are consistent with estimates of long-term water cycle amplification. Our results suggest that long-term basin-scale halosteric changes in the Pacific and Atlantic are substantially larger than previously assumed, with observed estimates and coupled climate models suggesting magnitudes of similar to 25% of the corresponding thermosteric changes. In both observations and simulations, Pacific basin-scale freshening leads to a density reduction that augments coincident thermosteric expansion, whereas in the Atlantic halosteric changes partially compensate strong thermosteric expansion via a basin-scale enhanced salinity density increase. Although regional differences are apparent, at basin-scales consistency is found between the observed and simulated partitioning of halosteric and thermosteric changes, and suggests that models are simulating the processes driving observed long-term basin-scale steric changes. Further analysis demonstrates that the observed halosteric changes and their basin partitioning are consistent with CMIP5 simulations that include anthropogenic CO2 forcings (Historical), but are found to be inconsistent with simulations that exclude anthropogenic forcings (HistoricalNat). C1 [Durack, Paul J.; Gleckler, Peter J.] Lawrence Livermore Natl Lab, Program Climate Model Diag & Intercomparison, Livermore, CA 94550 USA. [Durack, Paul J.; Wijffels, Susan E.] CSIRO Marine & Atmospher Res, Ctr Australian Weather & Climate Res, Hobart, Tas, Australia. [Durack, Paul J.; Wijffels, Susan E.] CSIRO, Oceans & Atmosphere Flagship, Hobart, Tas, Australia. RP Durack, PJ (reprint author), Lawrence Livermore Natl Lab, Program Climate Model Diag & Intercomparison, Livermore, CA 94550 USA. EM pauldurack@llnl.gov RI Durack, Paul/A-8758-2010 OI Durack, Paul/0000-0003-2835-1438 FU US Department of Energy, Office of Science, Climate and Environmental Sciences Division, Regional and Global Climate Modeling Program [DE-AC5207NA27344] FX The work of PJD and PJG from the Climate Program at Lawrence Livermore National Laboratory is a contribution to the US Department of Energy, Office of Science, Climate and Environmental Sciences Division, Regional and Global Climate Modeling Program under contract DE-AC5207NA27344. The Australian Government Department of Environment, the Bureau of Meteorology and CSIRO through the Australian Climate Change Science Program supported the work of SEW. We thank J Durack of the University of California, San Francisco and J A Church from CSIRO, Hobart, Australia for helpful comments with early drafts of this manuscript. We acknowledge the efforts of F Fernandes in writing and maintaining the python seawater toolbox (Fernandes 2014) and D Williams, C Doutriaux and their team for developing and maintaining the UV-CDAT analysis package (Williams et al 2014). We acknowledge the sources of observed data used in this study: M Ishii and M Kimoto (Ish09) and the International Argo Program and the national programmes that contribute to it. We acknowledge the World Climate Research Programme's Working Group on Coupled Modeling, which is responsible for CMIP, and we thank the climate modeling groups (listed in table 1) for producing and making available their model output. For CMIP the US Department of Energy's Program for Climate Model Diagnosis and Intercomparison provides coordinating support and led development of software infrastructure in partnership with the Global Organization for Earth System Science Portals. The DW10 data presented in this study can be downloaded from the CSIRO Ocean Change website at www. cmar. csiro. au/ oceanchange. LLNL Release #: LLNL-JRNL-653602. NR 88 TC 14 Z9 14 U1 10 U2 42 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 1748-9326 J9 ENVIRON RES LETT JI Environ. Res. Lett. PD NOV PY 2014 VL 9 IS 11 AR 114017 DI 10.1088/1748-9326/9/11/114017 PG 11 WC Environmental Sciences; Meteorology & Atmospheric Sciences SC Environmental Sciences & Ecology; Meteorology & Atmospheric Sciences GA AW9JS UT WOS:000346573900023 ER PT J AU Thebo, AL Drechsel, P Lambin, EF AF Thebo, A. L. Drechsel, P. Lambin, E. F. TI Global assessment of urban and peri-urban agriculture: irrigated and rainfed croplands SO ENVIRONMENTAL RESEARCH LETTERS LA English DT Article DE urban croplands; spatial analysis; food security; irrigated croplands; rainfed croplands; urban and peri-urban agriculture; urban land use ID DEVELOPING-COUNTRIES; CITIES; GROWTH AB The role of urban agriculture in global food security is a topic of increasing discussion. Existing research on urban and peri-urban agriculture consists largely of case studies that frequently use disparate definitions of urban and peri-urban agriculture depending on the local context and study objectives. This lack of consistency makes quantification of the extent of this practice at the global scale difficult. This study instead integrates global data on croplands and urban extents using spatial overlay analysis to estimate the global area of urban and peri-urban irrigated and rainfed croplands. The global area of urban irrigated croplands was estimated at about 24 Mha (11.0 percent of all irrigated croplands) with a cropping intensity of 1.48. The global area of urban rainfed croplands found was approximately 44 Mha (4.7 percent of all rainfed croplands) with a cropping intensity of 1.03. These values were derived from the MIRCA2000 Maximum Monthly Cropped Area Grids for irrigated and rainfed crops and therefore their sum does not necessarily represent the total urban cropland area when the maximum extent of irrigated and rainfed croplands occurs in different months. Further analysis of croplands within 20 km of urban extents show that 60 and 35 percent of, respectively, all irrigated and rainfed croplands fall within this distance range. C1 [Thebo, A. L.] Univ Calif Berkeley, Dept Civil & Environm Engn, Berkeley, CA 94720 USA. [Drechsel, P.] Int Water Management Inst, Pelawatte, Battaramulla, Sri Lanka. [Lambin, E. F.] Stanford Univ, Sch Earth Sci, Stanford, CA 94305 USA. [Lambin, E. F.] Stanford Univ, Woods Inst Environm, Stanford, CA 94305 USA. [Lambin, E. F.] Catholic Univ Louvain, Earth & Life Inst, Georges Lemaitre Ctr Earth & Climate Res, B-1348 Louvain0 La Neuve, Belgium. RP Thebo, AL (reprint author), Univ Calif Berkeley, Dept Civil & Environm Engn, OBrien Hall, Berkeley, CA 94720 USA. EM thebo@berkeley.edu FU USAID Collaborative Research-CGIAR Linkage Fund [4500012834]; Stanford UPS Endowment [1139780]; US Environmental Protection Agency (EPA) [91750501-0] FX Research support was provided through grants from the USAID Collaborative Research-CGIAR Linkage Fund (Award no. 4500012834) and the Stanford UPS Endowment (Grant no. 1139780). This publication was also developed under STAR Fellowship Assistance Agreement no. 91750501-0 awarded by the US Environmental Protection Agency (EPA). It has not been formally reviewed by EPA. The views expressed in this publication are solely those of Anne Thebo, and EPA does not endorse any products or commercial services mentioned in this publication. NR 35 TC 12 Z9 12 U1 4 U2 37 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 1748-9326 J9 ENVIRON RES LETT JI Environ. Res. Lett. PD NOV PY 2014 VL 9 IS 11 AR 114002 DI 10.1088/1748-9326/9/11/114002 PG 9 WC Environmental Sciences; Meteorology & Atmospheric Sciences SC Environmental Sciences & Ecology; Meteorology & Atmospheric Sciences GA AW9JS UT WOS:000346573900008 ER PT J AU Van Buskirk, RD Kantner, CLS Gerke, BF Chu, S AF Van Buskirk, R. D. Kantner, C. L. S. Gerke, B. F. Chu, S. TI A retrospective investigation of energy efficiency standards: policies may have accelerated long term declines in appliance costs SO ENVIRONMENTAL RESEARCH LETTERS LA English DT Article DE energy efficiency; learning; policy analysis ID TECHNOLOGY; INNOVATION AB We perform a retrospective investigation of multi-decade trends in price and life-cycle cost (LCC) for home appliances in periods with and without energy efficiency (EE) standards and labeling polices. In contrast to the classical picture of the impact of efficiency standards, the introduction and updating of appliance standards is not associated with a long-term increase in purchase price; rather, quality-adjusted prices undergo a continued or accelerated long-term decline. In addition, long term trends in appliance LCCs-which include operating costs-consistently show an accelerated long term decline with EE policies. We also show that the incremental price of efficiency improvements has declined faster than the baseline product price for selected products. These observations are inconsistent with a view of EE standards that supposes a perfectly competitive market with static supply costs. These results suggest that EE policies may be associated with other forces at play, such as innovation and learning-by-doing in appliance production and design, that can affect long term trends in quality-adjusted prices and LCCs. C1 [Van Buskirk, R. D.; Kantner, C. L. S.; Gerke, B. F.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Environm Energy Technol Div, Berkeley, CA 94720 USA. [Chu, S.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA. [Chu, S.] Stanford Univ, Dept Mol & Cellular Physiol, Stanford, CA 94305 USA. RP Van Buskirk, RD (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Environm Energy Technol Div, 1 Cyclotron Rd, Berkeley, CA 94720 USA. EM RDVanBuskirk@lbl.gov FU US Department of Energy, Office of Energy Efficiency and Renewable Energy [DE-AC02-05CH11231]; Collaborative Labeling and Appliance Standards Program FX This research is supported, in part, by the US Department of Energy, Office of Energy Efficiency and Renewable Energy, under contract No. DE-AC02-05CH11231. Louis-Benoit Desroches, Jia Li, Richard Newell, Alan Sanstad, Gabrielle Dreyfus, and Jeffery Greenblatt provided valuable input and feedback on earlier versions of the manuscript. The corresponding author acknowledges funding support from the Collaborative Labeling and Appliance Standards Program (www.clasponline.org). NR 49 TC 5 Z9 5 U1 1 U2 6 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 1748-9326 J9 ENVIRON RES LETT JI Environ. Res. Lett. PD NOV PY 2014 VL 9 IS 11 AR 114010 DI 10.1088/1748-9326/9/11/114010 PG 11 WC Environmental Sciences; Meteorology & Atmospheric Sciences SC Environmental Sciences & Ecology; Meteorology & Atmospheric Sciences GA AW9JS UT WOS:000346573900016 ER PT J AU Kresin, V Ovchinnikov, Y Friedel, J AF Kresin, Vladimir Ovchinnikov, Yurii Friedel, Jacques TI Pair correlation and dynamic Jahn-Teller effect: High-T-c in nanoclusters SO EPL LA English DT Article ID ELECTRONIC SHELL STRUCTURE; METALLIC NANOCLUSTERS; ALUMINUM CLUSTERS; CADMIUM CLUSTERS; ATOMIC CLUSTERS; INDIUM CLUSTERS; SUPERCONDUCTIVITY; DISTRIBUTIONS; TEMPERATURE; TRANSITIONS AB Electronic states in metallic nanoclusters form energy shells and degree of their filling depends on the number of delocalized electrons. In the region close to half-filling the cluster's geometry oscillates between the prolate and oblate configurations (dynamic Jahn-Teller effect). For large clusters (N > 10(2); N is the number of delocalized electrons) this effect competes with pair correlation and, as a result, it is perfectly realistic to observe the transition to the superconducting state. For some clusters (e.g., for Zn-76, Al-70) the value of the critical temperature is rather high (greater than or similar to 140 K). Copyright (C) EPLA, 2014 C1 [Kresin, Vladimir] Univ Calif Berkeley, Lawrence Berkeley Lab, Berkeley, CA 94720 USA. [Ovchinnikov, Yurii] RAN, LD Landau Theoret Phys Inst, Moscow 117334, Russia. [Friedel, Jacques] Univ Paris 11, Lab Phys Solids, F-91405 Orsay, France. RP Kresin, V (reprint author), Univ Calif Berkeley, Lawrence Berkeley Lab, Berkeley, CA 94720 USA. NR 38 TC 0 Z9 0 U1 6 U2 14 PU EPL ASSOCIATION, EUROPEAN PHYSICAL SOCIETY PI MULHOUSE PA 6 RUE DES FRERES LUMIERE, MULHOUSE, 68200, FRANCE SN 0295-5075 EI 1286-4854 J9 EPL-EUROPHYS LETT JI EPL PD NOV PY 2014 VL 108 IS 4 AR 43001 DI 10.1209/0295-5075/108/43001 PG 4 WC Physics, Multidisciplinary SC Physics GA AW6BR UT WOS:000346355000010 ER PT J AU Zhang, YX Jaegle, L Thompson, L Streets, DG AF Zhang, Yanxu Jaegle, Lyatt Thompson, LuAnne Streets, David G. TI Six centuries of changing oceanic mercury SO GLOBAL BIOGEOCHEMICAL CYCLES LA English DT Article DE mercury; anthropogenic perturbation; anthropocene; ocean; lake sediment; atmosphere ID AIR-SEA EXCHANGE; ANTHROPOGENIC CO2; NORTH-ATLANTIC; PACIFIC-OCEAN; MODEL; EMISSIONS; CYCLE; GOLD; DISTRIBUTIONS; SPECIATION AB Mercury (Hg) is a global and persistent contaminant, affecting human health primarily via marine fish consumption. Large anthropogenic releases of Hg to the atmosphere by mining and coal combustion have resulted in a significant perturbation to the biogeochemical cycling of Hg. The magnitude of this perturbation and the relative roles of the ocean and land as sinks for anthropogenic Hg remain unclear. Here we use a 3-D global ocean biogeochemical model to show that surface ocean Hg concentrations have increased fourfold over the last 600years. We find that anthropogenic Hg enters the ocean's interior predominantly by absorption onto sinking organic matter particulates, which decompose and release Hg at a depth of 500-800m, implying that the human perturbation is largest in subsurface waters of biologically productive regions. Our model simulation predicts that over the last six centuries half of emitted anthropogenic Hg has accumulated in the oceans and marine sediments. C1 [Zhang, Yanxu; Jaegle, Lyatt] Univ Washington, Dept Atmospher Sci, Seattle, WA 98195 USA. [Thompson, LuAnne] Univ Washington, Sch Oceanog, Seattle, WA 98195 USA. [Streets, David G.] Argonne Natl Lab, Decis & Informat Sci Div, Argonne, IL 60439 USA. RP Jaegle, L (reprint author), Univ Washington, Dept Atmospher Sci, Seattle, WA 98195 USA. EM jaegle@atmos.washington.edu RI Zhang, Yanxu/E-8583-2013; Zhang, Yanxu/H-6165-2016 NR 59 TC 13 Z9 14 U1 7 U2 37 PU AMER GEOPHYSICAL UNION PI WASHINGTON PA 2000 FLORIDA AVE NW, WASHINGTON, DC 20009 USA SN 0886-6236 EI 1944-9224 J9 GLOBAL BIOGEOCHEM CY JI Glob. Biogeochem. Cycle PD NOV PY 2014 VL 28 IS 11 BP 1251 EP 1261 DI 10.1002/2014GB004939 PG 11 WC Environmental Sciences; Geosciences, Multidisciplinary; Meteorology & Atmospheric Sciences SC Environmental Sciences & Ecology; Geology; Meteorology & Atmospheric Sciences GA AW9RE UT WOS:000346594100006 ER PT J AU Girsang, IP Dhupia, JS Muljadi, E Singh, M Pao, LY AF Girsang, Irving P. Dhupia, Jaspreet S. Muljadi, Eduard Singh, Mohit Pao, Lucy Y. TI Gearbox and Drivetrain Models to Study Dynamic Effects of Modern Wind Turbines SO IEEE TRANSACTIONS ON INDUSTRY APPLICATIONS LA English DT Article DE Gears; mechanical power transmission; resonance; variable-speed drives; vibration; wind energy ID PLANETARY; VIBRATION AB Wind turbine drivetrains consist of components that directly convert kinetic energy from the wind to electrical energy. Therefore, guaranteeing robust and reliable drivetrain designs is important to prevent turbine downtime. Current drivetrain models often lack the ability to model both the impacts of electrical transients as well as wind turbulence and shear in one package. In this paper, the capability of the FAST wind turbine computer-aided-engineering tool, developed by the National Renewable Energy Laboratory, is enhanced through the integration of a dynamic model of the drivetrain. The dynamic drivetrain model is built using Simscape in the MATLAB/Simulink environment and incorporates detailed electrical generator models. This model can be used to evaluate internal drivetrain loads due to excitations from both the wind and generator. C1 [Girsang, Irving P.; Dhupia, Jaspreet S.] Nanyang Technol Univ, Singapore 639798, Singapore. [Muljadi, Eduard; Singh, Mohit] Natl Renewable Energy Lab, Golden, CO 80401 USA. [Pao, Lucy Y.] Univ Colorado Boulder, Boulder, CO 80309 USA. RP Girsang, IP (reprint author), Nanyang Technol Univ, Singapore 639798, Singapore. EM irving1@e.ntu.edu.sg; djaspreet@ntu.edu.sg; eduard.muljadi@nrel.gov; mohit.singh@nrel.gov; pao@colorado.edu RI Dhupia, Jaspreet /A-3818-2011 OI Dhupia, Jaspreet /0000-0001-7181-1917 NR 34 TC 15 Z9 17 U1 2 U2 25 PU IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC PI PISCATAWAY PA 445 HOES LANE, PISCATAWAY, NJ 08855-4141 USA SN 0093-9994 EI 1939-9367 J9 IEEE T IND APPL JI IEEE Trans. Ind. Appl. PD NOV-DEC PY 2014 VL 50 IS 6 BP 3777 EP 3786 DI 10.1109/TIA.2014.2321029 PG 10 WC Engineering, Multidisciplinary; Engineering, Electrical & Electronic SC Engineering GA AW5RP UT WOS:000346332000017 ER PT J AU Xi, XX Smith, RJ Stanislaychuk, TN Sirenko, AA Gilbert, SN Tu, JJ Carr, GL AF Xi, Xiaoxiang Smith, R. J. Stanislaychuk, T. N. Sirenko, A. A. Gilbert, S. N. Tu, J. J. Carr, G. L. TI A broadband silicon quarter-wave retarder for far-infrared spectroscopic circular dichroism SO INFRARED PHYSICS & TECHNOLOGY LA English DT Article DE 1/4 wave retarder; Circularly polarized light; Circular dichroism; Far-infrared magnetospectroscopy; Cyclotron resonance; Excitons ID MONOLAYER; GRAPHENE AB The high brightness, broad spectral coverage and pulsed characteristics of infrared synchrotron radiation enable time-resolved spectroscopy under throughput-limited optical systems, as can occur with the high-field magnet cryostat systems used to study electron dynamics and cyclotron resonance by far-infrared techniques. A natural extension for magnetospectroscopy is to sense circular dichroism, i.e. the difference in a material's optical response for left and right circularly polarized light. A key component for spectroscopic circular dichroism is an achromatic 1/4 wave retarder functioning over the spectral range of interest. We report here the development of an in-line retarder using total internal reflection in high-resistivity silicon. We demonstrate its performance by distinguishing electronic excitations of differing handedness for GaAs in a magnetic field. This wave retarder is expected to be useful for far-infrared spectroscopy of circular dichroism in many materials. (C) 2014 Elsevier B.V. All rights reserved. C1 [Xi, Xiaoxiang; Smith, R. J.; Carr, G. L.] Brookhaven Natl Lab, Upton, NY 11973 USA. [Stanislaychuk, T. N.; Sirenko, A. A.] New Jersey Inst Technol, Dept Phys, Newark, NJ 07102 USA. [Gilbert, S. N.] Vanderbilt Univ, Dept Phys, Nashville, TN 37235 USA. [Tu, J. J.] CUNY City Coll, Dept Phys, New York, NY 10031 USA. RP Xi, XX (reprint author), Brookhaven Natl Lab, Upton, NY 11973 USA. EM xi.xiaoxiang@gmail.com RI Gilbert Corder, Stephanie/F-3658-2015 OI Gilbert Corder, Stephanie/0000-0002-5041-8670 FU U.S. Department of Energy under Brookhaven National Laboratory [DE-AC02-98CH10886] FX This research was supported by the U.S. Department of Energy under contract DE-AC02-98CH10886 at Brookhaven National Laboratory. Technical contributions from Gary Nintzel are gratefully acknowledged. NR 24 TC 1 Z9 1 U1 2 U2 10 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 1350-4495 EI 1879-0275 J9 INFRARED PHYS TECHN JI Infrared Phys. Technol. PD NOV PY 2014 VL 67 BP 436 EP 440 DI 10.1016/j.infrared.2014.09.004 PG 5 WC Instruments & Instrumentation; Optics; Physics, Applied SC Instruments & Instrumentation; Optics; Physics GA AW9AH UT WOS:000346549700066 ER PT J AU Leveille, RJ Bridges, J Wiens, RC Mangold, N Cousin, A Lanza, N Forni, O Ollila, A Grotzinger, J Clegg, S Siebach, K Berger, G Clark, B Fabre, C Anderson, R Gasnault, O Blaney, D Deflores, L Leshin, L Maurice, S Newsom, H AF Leveille, Richard J. Bridges, John Wiens, Roger C. Mangold, Nicolas Cousin, Agnes Lanza, Nina Forni, Olivier Ollila, Ann Grotzinger, John Clegg, Samuel Siebach, Kirsten Berger, Gilles Clark, Ben Fabre, Cecile Anderson, Ryan Gasnault, Olivier Blaney, Diana Deflores, Lauren Leshin, Laurie Maurice, Sylvestre Newsom, Horton TI Chemistry of fracture-filling raised ridges in Yellowknife Bay, Gale Crater: Window into past aqueous activity and habitability on Mars SO JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS LA English DT Article DE Mars; diagenesis; mudstone; smectite; magnesium; LIBS ID INDUCED BREAKDOWN SPECTROSCOPY; DEPTH-PROFILE ANALYSIS; CLAY MINERAL FORMATION; CEMENT STRATIGRAPHY; MERIDIANI-PLANUM; SNC METEORITE; SAPONITE; CHEMCAM; INSTRUMENT; HISTORY AB The ChemCam instrument package on the Curiosity rover was used to characterize distinctive raised ridges in the Sheepbed mudstone, Yellowknife Bay formation, Gale Crater. The multilayered, fracture-filling ridges are more resistant to erosion than the Sheepbed mudstone rock in which they occur. The bulk average composition of the raised ridges is enriched in MgO by 1.2-1.7 times (average of 8.3-11.4 wt %; single-shot maximum of 17.0 wt %) over that of the mudstone. Al2O3 is anticorrelated with MgO, while Li is somewhat enriched where MgO is highest. Some ridges show a variation in composition with different layers on a submillimeter scale. In particular, the McGrath target shows similar high-MgO resistant outer layers and a low-MgO, less resistant inner layer. This is consistent with the interpretation that the raised ridges are isopachous fracture-filling cements with a stratigraphy that likely reveals changes in fluid composition or depositional conditions over time. Overall, the average composition of the raised ridges is close to that of a Mg- and Fe-rich smectite, or saponite, which may also be the main clay mineral constituent of the host mudstone. These analyses provide evidence of diagenesis and aqueous activity in the early postdepositional history of the Yellowknife Bay formation, consistent with a low salinity to brackish fluid at near-neutral or slightly alkaline pH. The fluids that circulated through the fractures likely interacted with the Sheepbed mudstone and (or) other stratigraphically adjacent rock units of basaltic composition and leached Mg from them preferentially. C1 [Leveille, Richard J.] Canadian Space Agcy, St Hubert, PQ, Canada. [Leveille, Richard J.] McGill Univ, Dept Nat Resource Sci, Montreal, PQ, Canada. [Bridges, John] Univ Leicester, Dept Phys & Astron, Space Res Ctr, Leicester LE1 7RH, Leics, England. [Wiens, Roger C.; Cousin, Agnes; Lanza, Nina; Clegg, Samuel] Los Alamos Natl Lab, Los Alamos, NM USA. [Mangold, Nicolas] Univ Nantes, Lab Planetol & Geodynam Nantes, Nantes, France. [Forni, Olivier; Berger, Gilles; Gasnault, Olivier; Maurice, Sylvestre] Univ Toulouse, UPS OMP, IRAP, Toulouse, France. [Forni, Olivier; Berger, Gilles; Gasnault, Olivier; Maurice, Sylvestre] CNRS, IRAP, Toulouse, France. [Ollila, Ann; Newsom, Horton] Univ New Mexico, Inst Meteorit, Albuquerque, NM 87131 USA. [Grotzinger, John; Siebach, Kirsten] CALTECH, Lab Planetol & Geodynam Nantes, Pasadena, CA 91125 USA. [Clark, Ben] Space Sci Inst, Boulder, CO USA. [Fabre, Cecile] Univ Lorraine, GeoRessources UMR CNRS, Nancy, France. [Anderson, Ryan] US Geol Survey, Flagstaff, AZ 86001 USA. [Blaney, Diana; Deflores, Lauren] CALTECH, Jet Prop Lab, Pasadena, CA USA. [Leshin, Laurie] Rensselaer Polytech Inst, Troy, NY USA. RP Leveille, RJ (reprint author), Canadian Space Agcy, St Hubert, PQ, Canada. EM rich.leveille@gmail.com RI BERGER, Gilles/F-7118-2016; OI Gasnault, Olivier/0000-0002-6979-9012; Siebach, Kirsten/0000-0002-6628-6297; Clegg, Sam/0000-0002-0338-0948 FU NASA's Mars Program Office; Canadian Space Agency; Centre National d'Etudes Spatiales (CNES) FX The MSL mission is funded by NASA's Mars Program Office. R.J.L. received financial support from the Canadian Space Agency. The French contribution to ChemCam on MSL is supported by the Centre National d'Etudes Spatiales (CNES). We acknowledge the whole MSL team and JPL, in particular, for developing and leading this successful mission. We also thank the reviewers for their excellent comments, which greatly helped to improve the manuscript. The data reported in this paper are archived at the Planetary Data System, accessible at http://pds-geosciences.wustl.edu/missions/msl/index.htm. NR 72 TC 21 Z9 21 U1 2 U2 24 PU AMER GEOPHYSICAL UNION PI WASHINGTON PA 2000 FLORIDA AVE NW, WASHINGTON, DC 20009 USA SN 2169-9097 EI 2169-9100 J9 J GEOPHYS RES-PLANET JI J. Geophys. Res.-Planets PD NOV PY 2014 VL 119 IS 11 BP 2398 EP 2415 DI 10.1002/2014JE004620 PG 18 WC Geochemistry & Geophysics SC Geochemistry & Geophysics GA AW5XU UT WOS:000346345100008 ER PT J AU Pershenkov, VS Ullan, M Wilder, M Spieler, H Spencer, E Rescia, S Newcomer, FM Martinez-McKinney, F Kononenko, W Grillo, AA Diez, S AF Pershenkov, V. S. Ullan, M. Wilder, M. Spieler, H. Spencer, E. Rescia, S. Newcomer, F. M. Martinez-McKinney, F. Kononenko, W. Grillo, A. A. Diez, S. TI Mechanism of anomalous recovery in advanced SiGe bipolar transistors after low dose rate irradiation for very high total doses SO MICROELECTRONICS RELIABILITY LA English DT Article DE Radiation effects; ELDRS; Gamma irradiation; SiGe bipolar transistors; Anomalous recovery ID INTERFACE; DEPENDENCE; CIRCUITS; OXIDES; ELDRS AB The possible physical mechanism of the anomalous recovery effect in SiGe bipolar transistors is described. The qualitative analysis of saturated oxide trapped charge and interface trap densities at very high total doses as a function of dose rate affords an explain of decreasing excess base current and increasing current gain during further low dose rate irradiation. (C) 2014 Elsevier Ltd. All rights reserved. C1 [Pershenkov, V. S.] Moscow Engn Phys Inst, NRNU MEPhI, Moscow 115409, Russia. [Ullan, M.; Diez, S.] CSIC, Ctr Nacl Microelect, Barcelona 08193, Spain. [Wilder, M.; Spencer, E.; Martinez-McKinney, F.; Grillo, A. A.] UCSC, SCIPP, Santa Cruz Inst Particle Phys, Santa Cruz, CA USA. [Spieler, H.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Phys, Berkeley, CA 94720 USA. [Rescia, S.] Brookhaven Natl Lab, Upton, NY 11973 USA. [Newcomer, F. M.; Kononenko, W.] Univ Penn, Philadelphia, PA 19104 USA. RP Ullan, M (reprint author), CSIC, Ctr Nacl Microelect, Campus Univ Bellaterra, Barcelona 08193, Spain. EM Miguel.Ullan@imb-cnm.csic.es RI Ullan, Miguel/P-7392-2015 FU Spanish Ministry of Economy and Competitiveness through the Particle Physics National Program [FPA2012-39055-C02-02]; FEDER funds FX The authors thank A.T. Yastrebov for technical support. This work is supported and financed in part by the Spanish Ministry of Economy and Competitiveness through the Particle Physics National Program (ref. FPA2012-39055-C02-02) and co-financed with FEDER funds. NR 12 TC 1 Z9 1 U1 0 U2 4 PU PERGAMON-ELSEVIER SCIENCE LTD PI OXFORD PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, ENGLAND SN 0026-2714 J9 MICROELECTRON RELIAB JI Microelectron. Reliab. PD NOV PY 2014 VL 54 IS 11 BP 2360 EP 2363 DI 10.1016/j.microrel.2014.04.009 PG 4 WC Engineering, Electrical & Electronic; Nanoscience & Nanotechnology; Physics, Applied SC Engineering; Science & Technology - Other Topics; Physics GA AW3WB UT WOS:000346212900003 ER PT J AU Zhang, QH Guy, RD Philip, B AF Zhang, Qinghai Guy, Robert D. Philip, Bobby TI A Projection Preconditioner for Solving the Implicit Immersed Boundary Equations SO NUMERICAL MATHEMATICS-THEORY METHODS AND APPLICATIONS LA English DT Article DE Fluid-structure interaction; immersed boundary method; projection method; preconditioning ID NAVIER-STOKES EQUATIONS; NUMERICAL-SOLUTION; BLOOD-FLOW; HEART AB This paper presents a method for solving the linear semi-implicit immersed boundary equations which avoids the severe time step restriction presented by explicit-time methods. The Lagrangian variables are eliminated via a Schur complement to form a purely Eulerian saddle point system, which is preconditioned by a projection operator and then solved by a Krylov subspace method. From the viewpoint of projection methods, we derive an ideal preconditioner for the saddle point problem and compare the efficiency of a number of simpler preconditioners that approximate this perfect one. For low Reynolds number and high stiffness, one particular projection preconditioner yields an efficiency improvement of the explicit IB method by a factor around thirty. Substantial speed-ups over explicit-time method are achieved for Reynolds number below 100. This speedup increases as the Eulerian grid size and/or the Reynolds number are further reduced. C1 [Zhang, Qinghai] Univ Utah, Dept Math, Salt Lake City, UT 84112 USA. [Guy, Robert D.] Univ Calif Davis, Dept Math, Davis, CA 95616 USA. [Philip, Bobby] Oak Ridge Natl Lab, Oak Ridge, TN 37831 USA. RP Zhang, QH (reprint author), Univ Utah, Dept Math, Salt Lake City, UT 84112 USA. EM qinghai@math.utah.edu; guy@math.ucdavis.edu; philipb@ornl.gov RI Zhang, Qinghai/A-3637-2009; OI Zhang, Qinghai/0000-0002-3655-4190; Philip, Bobby/0000-0001-6716-3515 FU NSF-DMS grant [1160438, 1226386] FX This work was supported in part by NSF-DMS grants 1160438 and 1226386 to RDG. NR 25 TC 1 Z9 1 U1 1 U2 3 PU GLOBAL SCIENCE PRESS PI WANCHAI PA ROOM 3208, CENTRAL PLAZA, 18 HARBOUR RD, WANCHAI, HONG KONG 00000, PEOPLES R CHINA SN 1004-8979 J9 NUMER MATH-THEORY ME JI Numer. Math.-Theory Methods Appl. PD NOV PY 2014 VL 7 IS 4 BP 473 EP 498 DI 10.4208/nmtma.2014.1304si PG 26 WC Mathematics, Applied; Mathematics SC Mathematics GA AW6TI UT WOS:000346400800005 ER PT J AU Shi, X Lin, G AF Shi, Xing Lin, Guang TI Modeling the Sedimentation of Red Blood Cells in Flow under Strong External Magnetic Body Force Using a Lattice Boltzmann Fictitious Domain Method SO NUMERICAL MATHEMATICS-THEORY METHODS AND APPLICATIONS LA English DT Article DE Sediment; erythrocyte; fictitious domain method; lattice Boltzmann method; flow-structure interaction; red blood cell ID DLM/FD METHOD; DEFORMATION; CAPILLARIES; ERYTHROCYTE; CYTOSKELETON; MECHANICS; RHEOLOGY AB Experimental observations show that a strong magnetic field has a dramatic influence on the sedimentation of RBCs, which motivates us to model the sedimentation of red blood cell (RBC) under strong external magnetic body force. To model the sedimentation of a RBC in a square duct and a circular pipe, a recently developed technique derived from the lattice Boltzmann and the distributed Lagrange multiplier/fictitious domain methods (LBM-DLM/FD) is extended to employ the mesoscopic network model for simulations of the sedimentation of a RBC in flow. The flow is simulated by the LBM with a strong magnetic body force, while the network model is used for modeling RBC deformation. The fluid-RBC interactions are enforced by the Lagrange multiplier. The sedimentation of RBC in a square duct and a circular pipe is simulated, which demonstrates the developed method's capability to model the sedimentation of RBCs in various flows. Numerical results illustrate that the terminal settling velocity increases incrementally with the exerted body force. The deformation of RBC has a significant effect on the terminal settling velocity due to the change in the frontal area. The larger the exerted force, the smaller the frontal area and the larger the RBC deformation become. Additionally, the wall effect on the motion and deformation of RBC is also investigated. C1 [Shi, Xing] Zhejiang Univ, Dept Aeronaut & Aerosp, Hangzhou 310027, Zhejiang, Peoples R China. [Lin, Guang] Purdue Univ, Sch Mech Engn, Dept Math, W Lafayette, IN 47907 USA. [Lin, Guang] Pacific NW Natl Lab, Computat Math Grp, Fundamental & Computat Sci Directorate, Richland, WA 99352 USA. RP Lin, G (reprint author), Purdue Univ, Sch Mech Engn, Dept Math, W Lafayette, IN 47907 USA. EM guanglin@purdue.edu FU National Natural Science Foundation of China [10902098, 11372278]; Fundamental Research Funds of the Central Universities [2010QNA40107]; Applied Mathematics Program within the Department of Energys (DOE) Office of Advanced Scientific Computing Research (ASCR) as part of the Collaboratory on Mathematics for Mesoscopic Modeling of Materials (CM4); DOE [DE-AC05-76RL01830] FX Xing Shi would like to acknowledge support from the National Natural Science Foundation of China (Grant Nos. 10902098, 11372278) and the Fundamental Research Funds of the Central Universities (Program No. 2010QNA40107). Guang Lin would like to acknowledge support from the Applied Mathematics Program within the Department of Energys (DOE) Office of Advanced Scientific Computing Research (ASCR) as part of the Collaboratory on Mathematics for Mesoscopic Modeling of Materials (CM4). The research was performed using Pacific Northwest National Laboratory (PNNL) Institutional Computing, as well as the National Energy Research Scientific Computing Center at Lawrence Berkeley National Laboratory. PNNL is operated by Battelle for the DOE under Contract DE-AC05-76RL01830. NR 23 TC 0 Z9 0 U1 3 U2 10 PU GLOBAL SCIENCE PRESS PI WANCHAI PA ROOM 3208, CENTRAL PLAZA, 18 HARBOUR RD, WANCHAI, HONG KONG 00000, PEOPLES R CHINA SN 1004-8979 J9 NUMER MATH-THEORY ME JI Numer. Math.-Theory Methods Appl. PD NOV PY 2014 VL 7 IS 4 BP 512 EP 523 DI 10.4208/nmtma.2014.1306si PG 12 WC Mathematics, Applied; Mathematics SC Mathematics GA AW6TI UT WOS:000346400800007 ER PT J AU Behbahani, SR Mirbabayi, M Senatore, L Smith, KM AF Behbahani, Siavosh R. Mirbabayi, Mehrdad Senatore, Leonardo Smith, Kendrick M. TI New natural shapes of non-Gaussianity from high-derivative interactions and their optimal limits from WMAP 9-year data SO JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS LA English DT Article DE inflation; non-gaussianity ID PRIMORDIAL NON-GAUSSIANITY; ANISOTROPIES; MODELS AB Given the fantastic experimental effort, it is important to thoroughly explore the signature space of inflationary models. The fact that higher derivative operators do not renormalize lower derivative ones allows us to find a large class of technically natural single-clock inflationary models where, in the context of the Effective Field Theory of Inflation, the leading interactions have many derivatives. We systematically explore the 3-point function induced by these models and their overlap with the standard equilateral and orthogonal templates. We find that in order to satisfactorily cover the signature space of these models, two new additional templates need to be included. We then perform the optimal analysis of the WMAP 9-year data for the resulting four templates, finding that the overall significance of a non-zero signal is between 2-2.5 sigma, depending on the choice of parameter space, partially driven by the preference for nonzero f(NL)(orth) in WMAP9. C1 [Behbahani, Siavosh R.] Boston Univ, Dept Phys, Boston, MA 02215 USA. [Mirbabayi, Mehrdad] Inst Adv Study, Sch Nat Sci, Princeton, NJ 08540 USA. [Senatore, Leonardo] Stanford Univ, Stanford Inst Theoret Phys, Stanford, CA 94306 USA. [Senatore, Leonardo] SLAC, Kavli Inst Particle Astrophys & Cosmol, Menlo Pk, CA 94025 USA. [Senatore, Leonardo] Stanford Univ, Menlo Pk, CA 94025 USA. [Smith, Kendrick M.] Perimeter Inst Theoret Phys, Waterloo, ON N2L 2Y5, Canada. RP Behbahani, SR (reprint author), Boston Univ, Dept Phys, Boston, MA 02215 USA. EM siavoshrezvan@gmail.com; mehrdadm@ias.edu; senatore@standford.edu; kmsmith@perimeterinstitute.ca FU DOE [DE-FG02-01ER-40676]; NSF [PHY-1314311, PHY-1068380]; DOE Early Career Award [DE-FG02-12ER41854]; Government of Canada through Industry Canada; Province of Ontario through the Ministry of Research Innovation; Canada Foundation for Innovation under the auspices of Compute Canada; Government of Ontario; University of Toronto; NSERC Discovery Grant FX We thank Andrei Gruzinov, Ami Katz, and Matias Zaldarriaga for useful discussions. The research of S.R.B. is supported by the DOE under grant numbers DE-FG02-01ER-40676 and DE-FG02-01ER-40676. M.M. is supported by NSF Grant PHY-1314311. L.S. is supported by DOE Early Career Award DE-FG02-12ER41854 and by NSF grant PHY-1068380. Research at Perimeter Institute is supported by the Government of Canada through Industry Canada and by the Province of Ontario through the Ministry of Research & Innovation. Some computations were performed on the GPC cluster at the SciNet HPC Consortium. SciNet is funded by the Canada Foundation for Innovation under the auspices of Compute Canada, the Government of Ontario, and the University of Toronto. K.M.S. was supported by an NSERC Discovery Grant. NR 36 TC 3 Z9 3 U1 0 U2 1 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 1475-7516 J9 J COSMOL ASTROPART P JI J. Cosmol. Astropart. Phys. PD NOV PY 2014 IS 11 AR 035 DI 10.1088/1475-7516/2014/11/035 PG 31 WC Astronomy & Astrophysics; Physics, Particles & Fields SC Astronomy & Astrophysics; Physics GA AW2GF UT WOS:000346105300036 ER PT J AU O'Donnell, JA Aiken, GR Walvoord, MA Raymond, PA Butler, KD Dornblaser, MM Heckman, K AF O'Donnell, Jonathan A. Aiken, George R. Walvoord, Michelle A. Raymond, Peter A. Butler, Kenna D. Dornblaser, Mark M. Heckman, Katherine TI Using dissolved organicmatter age and composition to detect permafrost thaw in boreal watersheds of interior Alaska SO JOURNAL OF GEOPHYSICAL RESEARCH-BIOGEOSCIENCES LA English DT Article DE permafrost; dissolved organic matter; radiocarbon; rivers; boreal; carbon ID BLACK SPRUCE ECOSYSTEM; DISCONTINUOUS PERMAFROST; CARBON ACCUMULATION; CLIMATE-CHANGE; MINERAL SOILS; YUKON RIVER; DOC EXPORT; MATTER; CATCHMENT; NORTHERN AB Recent warming at high latitudes has accelerated permafrost thaw, which can modify soil carbon dynamics and watershed hydrology. The flux and composition of dissolved organic matter (DOM) from soils to rivers are sensitive to permafrost configuration and its impact on subsurface hydrology and groundwater discharge. Here, we evaluate the utility of DOM composition and age as a tool for detecting permafrost thaw in three rivers (Beaver, Birch, and Hess Creeks) within the discontinuous permafrost zone of interior Alaska. We observed strong temporal controls on C-14 content of hydrophobic acid isolates (C-14-HPOA) across all rivers, with the most enriched values occurring during spring snowmelt (758) and most depleted during winter flow (-218). Radiocarbon ages of winter flow samples ranged from 35 to 445yr BP, closely tracking estimated median base flow travel times for this region (335years). During spring snowmelt, young DOM was composed of highly aromatic, high molecular-weight compounds, whereas older DOM of winter flow had lower aromaticity and molecular weight. We observed a significant correlation between C-14-HPOA and UV absorbance coefficient at 254nm ((254)) across all study rivers. Using (254) as an optical indicator for C-14-HPOA, we also observed a long-term decline in (254) during maximum annual thaw depth over the last decade at the Hess Creek study site. These findings suggest a shift in watershed hydrology associated with increasing active layer thickness. Further development of DOM optical indicators may serve as a novel and inexpensive tool for detecting permafrost degradation in northern watersheds. C1 [O'Donnell, Jonathan A.] Natl Pk Serv, Arctic Network, Fairbanks, AK 99709 USA. [Aiken, George R.; Butler, Kenna D.; Dornblaser, Mark M.] US Geol Survey, Boulder, CO USA. [Walvoord, Michelle A.] US Geol Survey, Lakewood, CO 80225 USA. [Raymond, Peter A.] Yale Univ, Sch Forestry & Environm Studies, New Haven, CT 06511 USA. [Heckman, Katherine] US Forest Serv, USDA, Livermore, CA USA. [Heckman, Katherine] Lawrence Livermore Natl Lab, Livermore, CA USA. RP O'Donnell, JA (reprint author), Natl Pk Serv, Arctic Network, Fairbanks, AK 99709 USA. EM jaodonnell@nps.gov RI Raymond, Peter/C-4087-2009 OI Raymond, Peter/0000-0002-8564-7860 FU National Research Program and Climate Effects Network of the Water, Climate, and Land Use Change Mission Areas of the US Geological Survey FX Funding for this project was provided by the National Research Program and Climate Effects Network of the Water, Climate, and Land Use Change Mission Areas of the US Geological Survey. The manuscript was greatly improved thanks to comments by the Editor, Associate Editor, two anonymous reviewers, and Brett Poulin. We would like to thank Karena Schmidt (Michigan Tech) for graphitizing HPOA isolates and Jennifer Eikenberry (Michigan Tech) for analyzing 13C content of HPOA isolates. We also thank Heather Best (USGS Fairbanks) for helping with field logistics and sample collection and Jennifer Barnes for assistance in making Figure 8b. Interested users can contact the corresponding author for access to data presented and analyzed here. Any use of trade, firm, or product names is for descriptive purposes only and does not imply endorsement by the U.S. Government. NR 88 TC 9 Z9 9 U1 3 U2 60 PU AMER GEOPHYSICAL UNION PI WASHINGTON PA 2000 FLORIDA AVE NW, WASHINGTON, DC 20009 USA SN 2169-8953 EI 2169-8961 J9 J GEOPHYS RES-BIOGEO JI J. Geophys. Res.-Biogeosci. PD NOV PY 2014 VL 119 IS 11 BP 2155 EP 2170 DI 10.1002/2014JG002695 PG 16 WC Environmental Sciences; Geosciences, Multidisciplinary SC Environmental Sciences & Ecology; Geology GA AW3LS UT WOS:000346188800007 ER PT J AU Pilli, SP Smith, LV Vaithiyalingam, S AF Pilli, Siva P. Smith, Lloyd V. Vaithiyalingam, Shutthanandan TI Measuring time-dependent diffusion in polymer matrix composites SO MECHANICS OF TIME-DEPENDENT MATERIALS LA English DT Article DE Polymer matrix composites; Time-dependent diffusion ID NUCLEAR-REACTION ANALYSIS; MOISTURE AB Moisture plays a significant role in influencing the mechanical behavior and long-term durability of polymer matrix composites (PMCs). The common methods used to determine the moisture diffusion coefficients of PMCs are based on the solution of Fickian diffusion in the one-dimensional domain. Fick's Law assumes that equilibrium between the material surface and the external vapor is established instantaneously. A time-dependent boundary condition has been shown to improve correlation with some bulk diffusion measurements, but has not been validated experimentally. The surface moisture content in a Toray 800S/3900-2B toughened quasi-isotropic laminate system, [0/+/- 60] (s) , was analyzed experimentally using Nuclear Reaction Analysis (NRA). It was found that the surface moisture content showed a rapid increase to an intermediate concentration C (0), followed by a slow linear increase to the saturation level. C1 [Pilli, Siva P.; Vaithiyalingam, Shutthanandan] Pacific NW Natl Lab, Richland, WA 99352 USA. [Smith, Lloyd V.] Washington State Univ, Pullman, WA 99164 USA. RP Pilli, SP (reprint author), Pacific NW Natl Lab, Richland, WA 99352 USA. EM siva.pilli@pnnl.gov FU Department of Energy's Office of Biological and Environmental Research FX A portion of the research (particularly NRA) was performed using EMSL, a national scientific user facility sponsored by the Department of Energy's Office of Biological and Environmental Research and located at Pacific Northwest National Laboratory. NR 17 TC 0 Z9 0 U1 2 U2 7 PU SPRINGER PI DORDRECHT PA VAN GODEWIJCKSTRAAT 30, 3311 GZ DORDRECHT, NETHERLANDS SN 1385-2000 EI 1573-2738 J9 MECH TIME-DEPEND MAT JI Mech. Time-Depend. Mater. PD NOV PY 2014 VL 18 IS 4 BP 633 EP 641 DI 10.1007/s11043-012-9175-z PG 9 WC Mechanics; Materials Science, Characterization & Testing SC Mechanics; Materials Science GA AW0GT UT WOS:000345970000001 ER PT J AU Mizukami, Y Konczykowski, M Kawamoto, Y Kurata, S Kasahara, S Hashimoto, K Mishra, V Kreisel, A Wang, Y Hirschfeld, PJ Matsuda, Y Shibauchi, T AF Mizukami, Y. Konczykowski, M. Kawamoto, Y. Kurata, S. Kasahara, S. Hashimoto, K. Mishra, V. Kreisel, A. Wang, Y. Hirschfeld, P. J. Matsuda, Y. Shibauchi, T. TI Disorder-induced topological change of the superconducting gap structure in iron pnictides SO NATURE COMMUNICATIONS LA English DT Article ID TEMPERATURE PENETRATION DEPTH; UNCONVENTIONAL SUPERCONDUCTORS AB In superconductors with unconventional pairing mechanisms, the energy gap in the excitation spectrum often has nodes, which allow quasiparticle excitations at low energies. In many cases, such as in d-wave cuprate superconductors, the position and topology of nodes are imposed by the symmetry, and thus the presence of gapless excitations is protected against disorder. Here we report on the observation of distinct changes in the gap structure of ironpnictide superconductors with increasing impurity scattering. By the successive introduction of nonmagnetic point defects into BaFe2(As1 - P-x(x))(2) crystals via electron irradiation, we find from the low-temperature penetration depth measurements that the nodal state changes to a nodeless state with fully gapped excitations. Moreover, under further irradiation the gapped state evolves into another gapless state, providing bulk evidence of unconventional sign-changing s-wave superconductivity. This demonstrates that the topology of the superconducting gap can be controlled by disorder, which is a strikingly unique feature of iron pnictides. C1 [Mizukami, Y.; Kawamoto, Y.; Kurata, S.; Kasahara, S.; Hashimoto, K.; Matsuda, Y.; Shibauchi, T.] Kyoto Univ, Dept Phys, Sakyo Ku, Kyoto 6068502, Japan. [Mizukami, Y.; Kurata, S.; Shibauchi, T.] Univ Tokyo, Dept Adv Mat Sci, Kashiwa, Chiba 2778561, Japan. [Konczykowski, M.] Ecole Polytech, CNRS, Lab Solides Irradies, UMR 7642, F-91128 Palaiseau, France. [Konczykowski, M.] Ecole Polytech, IRAMIS, DSM, CEA, F-91128 Palaiseau, France. [Hashimoto, K.] Tohoku Univ, Inst Mat Res, Aoba Ku, Sendai, Miyagi 9808577, Japan. [Mishra, V.] Argonne Natl Lab, Div Mat Sci, Lemont, IL 60439 USA. [Kreisel, A.; Wang, Y.; Hirschfeld, P. J.] Univ Florida, Dept Phys, Gainesville, FL 32611 USA. RP Shibauchi, T (reprint author), Kyoto Univ, Dept Phys, Sakyo Ku, Kyoto 6068502, Japan. EM shibauchi@k.u-tokyo.ac.jp RI Hashimoto, Kenichiro/C-4925-2012; Shibauchi, Takasada/B-9349-2008; Kasahara, Shigeru/H-3064-2014 OI Hashimoto, Kenichiro/0000-0003-4651-4077; Shibauchi, Takasada/0000-0001-5831-4924; Kasahara, Shigeru/0000-0002-6007-9617 FU Japan Society for the Promotion of Science (JSPS); Ministry of Education, Culture, Sports, Science and Technology (MEXT) of Japan [25103713]; EMIR network [11-10-8071]; Center for Emergent Superconductivity; Energy Frontier Research Center - US DOE, Office of Science [DE-AC0298CH1088]; DOE [DE-FG02-05ER46236] FX We thank C.J. van der Beek, A. Carrington, H. Kontani and R. Prozorov for fruitful discussion. We also thank B. Boizot, J. Losco and V. Metayer for technical assistance. This work was supported by Grants-in-Aid for Scientific Research (KAKENHI) from Japan Society for the Promotion of Science (JSPS), and by the 'Topological Quantum Phenomena' (No. 25103713) Grant-in Aid for Scientific Research on Innovative Areas from the Ministry of Education, Culture, Sports, Science and Technology (MEXT) of Japan. Irradiation experiments were supported by EMIR network, proposal No. 11-10-8071. V.M. acknowledges support from the Center for Emergent Superconductivity, an Energy Frontier Research Center funded by the US DOE, Office of Science, under Award No. DE-AC0298CH1088. A.K., Y.W. and P.J.H. were supported by DOE DE-FG02-05ER46236. NR 39 TC 25 Z9 25 U1 4 U2 34 PU NATURE PUBLISHING GROUP PI LONDON PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND SN 2041-1723 J9 NAT COMMUN JI Nat. Commun. PD NOV PY 2014 VL 5 AR 5657 DI 10.1038/ncomms6657 PG 6 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AW2WA UT WOS:000346146100001 PM 25430419 ER PT J AU Johnston, R AF Johnston, Roger TI Challenges in national nuclear security need specific, viable solutions SO PHYSICS TODAY LA English DT Letter C1 Argonne Natl Lab, Argonne, IL 60439 USA. RP Johnston, R (reprint author), Argonne Natl Lab, 9700 S Cass Ave, Argonne, IL 60439 USA. EM rbsekurity@gmail.com NR 0 TC 0 Z9 0 U1 0 U2 0 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0031-9228 EI 1945-0699 J9 PHYS TODAY JI Phys. Today PD NOV PY 2014 VL 67 IS 11 BP 8 EP 8 PG 1 WC Physics, Multidisciplinary SC Physics GA AW2MJ UT WOS:000346122000001 ER PT J AU Walker, P Stuchbery, A Kondev, F AF Walker, Philip Stuchbery, Andrew Kondev, Filip TI George Dionisios Dracoulis obituary SO PHYSICS TODAY LA English DT Biographical-Item C1 [Walker, Philip] Univ Surrey, Guildford GU2 5XH, Surrey, England. [Stuchbery, Andrew] Australian Natl Univ, Canberra, ACT, Australia. [Kondev, Filip] Argonne Natl Lab, Argonne, IL 60439 USA. RP Walker, P (reprint author), Univ Surrey, Guildford GU2 5XH, Surrey, England. NR 1 TC 0 Z9 0 U1 0 U2 0 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 0031-9228 EI 1945-0699 J9 PHYS TODAY JI Phys. Today PD NOV PY 2014 VL 67 IS 11 BP 66 EP 66 PG 1 WC Physics, Multidisciplinary SC Physics GA AW2MJ UT WOS:000346122000020 ER PT J AU Lei, QY Golalikhani, M Yang, DY Withanage, WK Rafti, A Qiu, J Hambe, M Bauer, ED Ronning, F Jia, QX Weiss, JD Hellstrom, EE Wang, XF Chen, XH Williams, F Yang, Q Temple, D Xi, XX AF Lei, Q. Y. Golalikhani, M. Yang, D. Y. Withanage, W. K. Rafti, A. Qiu, J. Hambe, M. Bauer, E. D. Ronning, F. Jia, Q. X. Weiss, J. D. Hellstrom, E. E. Wang, X. F. Chen, X. H. Williams, F. Yang, Q. Temple, D. Xi, X. X. TI Structural and transport properties of epitaxial Ba(Fe1-xCox)(2)As-2 thin films on various substrates SO SUPERCONDUCTOR SCIENCE & TECHNOLOGY LA English DT Article DE superconductor; thin films; microstructure ID SUPERCONDUCTIVITY; BAFE2AS2 AB A comprehensive microstructural study was conducted on optimally-doped epitaxial Ba(Fe1-xCox)(2)As-2 thin films grown by pulsed laser deposition on various substrates of a wide range of lattice constants: SrTiO3, LaAlO3, (La, Sr)(Al, Ta)O-3, MgO, CaF2, and BaF2. We found that epitaxial strain directly affects the superconductivity in the film, with the transition temperature decreasing linearly with increasing in-plane lattice constant of the film. However, the strain is not determined by the lattice mismatch between the film and substrate. Instead, the mosaic spread of the grain orientation in the film and the thermal expansion coefficient of the substrate were found to correlate well with the in-plane lattice constant of the film. The result confirms the importance of structural distortions to the superconductivity in the Ba(Fe1-xCox)(2)As-2 films. C1 [Lei, Q. Y.; Golalikhani, M.; Yang, D. Y.; Withanage, W. K.; Rafti, A.; Qiu, J.; Hambe, M.; Xi, X. X.] Temple Univ, Dept Phys, Philadelphia, PA 19122 USA. [Bauer, E. D.; Ronning, F.; Jia, Q. X.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA. [Weiss, J. D.; Hellstrom, E. E.] Florida State Univ, Natl High Magnet Field Lab, Ctr Appl Superconduct, Tallahassee, FL 32310 USA. [Wang, X. F.; Chen, X. H.] Univ Sci & Technol China, Hefei Natl Lab Phys Sci Microscale, Hefei 230026, Anhui, Peoples R China. [Wang, X. F.; Chen, X. H.] Univ Sci & Technol China, Dept Phys, Hefei 230026, Anhui, Peoples R China. [Williams, F.; Yang, Q.; Temple, D.] Norfolk State Univ, Ctr Mat Res, Appl Res Ctr, Norfolk, VA 23504 USA. RP Lei, QY (reprint author), Temple Univ, Dept Phys, Philadelphia, PA 19122 USA. EM qingyu.lei@temple.edu RI Wang, Xiangfeng/I-2848-2014; OI Wang, Xiangfeng/0000-0001-9845-1659; Ronning, Filip/0000-0002-2679-7957; Bauer, Eric/0000-0003-0017-1937 FU NSF [DMR-1310087, DMR-1006584, DMR-1306785]; DoD DURIP Award from the Office of Naval Research [N0014-12-1-0777]; Los Alamos National Laboratory LDRD Program; National Nuclear Security Administration of the US Department of Energy [DE-AC52-06NA25396]; State of Florida; NHMFL; National Science Foundation [DMR-1157490]; College of Engineering, Temple University FX The work at Temple University was supported by NSF under grant number DMR-1310087. The EDS measurement was performed in the CoE-NIC facility at Temple University. The CoE-NIC is based on DoD DURIP Award N0014-12-1-0777 from the Office of Naval Research and is sponsored by the College of Engineering, Temple University. The work at Los Alamos was partially supported by the Los Alamos National Laboratory LDRD Program, and was performed, in part, at the Center for Integrated Nanotechnologies, a US Department of Energy, Office of Basic Energy Sciences Nanoscale Science Research Center. Los Alamos National Laboratory is operated by Los Alamos National Security, LLC, for the National Nuclear Security Administration of the US Department of Energy under contract DE-AC52-06NA25396. The work at The National High Magnetic Field Laboratory was supported by NSF DMR-1006584 and DMR-1306785, the State of Florida, and by NHMFL which is supported by the National Science Foundation under DMR-1157490. NR 25 TC 3 Z9 3 U1 1 U2 30 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0953-2048 EI 1361-6668 J9 SUPERCOND SCI TECH JI Supercond. Sci. Technol. PD NOV PY 2014 VL 27 IS 11 AR 115010 DI 10.1088/0953-2048/27/11/115010 PG 9 WC Physics, Applied; Physics, Condensed Matter SC Physics GA AW3OL UT WOS:000346196100011 ER PT J AU Rouco, V Bartolome, E Maiorov, B Palau, A Civale, L Obradors, X Puig, T AF Rouco, V. Bartolome, E. Maiorov, B. Palau, A. Civale, L. Obradors, X. Puig, T. TI Vortex creep in TFA-YBCO nanocomposite films SO SUPERCONDUCTOR SCIENCE & TECHNOLOGY LA English DT Article DE flux relaxation; YBCO nanocomposite films; vortex pinning ID HIGH-TEMPERATURE SUPERCONDUCTORS; FLUX-CREEP; COLUMNAR DEFECTS; II SUPERCONDUCTORS; YBA2CU3O7-DELTA; RELAXATION; CRYSTALS AB Vortex creep in YBa2Cu3O7-x (YBCO) films grown from the trifluoracetate (TFA) chemical route with BaZrO3 and Ba2YTaO6 second-phase nanoparticles (NPs) has been investigated by magnetic relaxation measurements. We observe that in YBCO nanocomposites the phenomenological crossover line from the elastic to the plastic creep regime is shifted to higher magnetic fields and temperatures. The origin of this shift lies on the new isotropic-strong vortex pinning contribution appearing in these nanocomposites, induced by local lattice distortions. As a consequence, we demonstrate that the addition of non-coherent NPs produces a decrease in the creep rate S in most of the phase diagram, particularly, in the range of fields and temperatures (T > 60 K, H-mu 0 > 0.5 T) relevant for large scale applications. C1 [Rouco, V.; Palau, A.; Obradors, X.; Puig, T.] CSIC, Inst Ciencia Mat, ICMAB, E-08193 Barcelona, Spain. [Bartolome, E.] EUSS, E-08017 Barcelona, Spain. [Maiorov, B.; Civale, L.] Los Alamos Natl Lab, Condensed Matter & Magnet Sci Grp MPA CMMS, Los Alamos, NM 87545 USA. RP Rouco, V (reprint author), CSIC, Inst Ciencia Mat, ICMAB, Campus Univ Autonoma Barcelona, E-08193 Barcelona, Spain. EM teresa.puig@icmab.es RI Obradors, Xavier/A-8146-2012; Palau, Anna/C-2947-2014; OI Palau, Anna/0000-0002-2217-164X; Maiorov, Boris/0000-0003-1885-0436; Civale, Leonardo/0000-0003-0806-3113 FU MINECO [MAT2011-28874-C02, CSD2007-0041, IPT-2011-1090-920000]; EU-FP7 [NMP-LA-2012-280432]; Cost Action; JAE-CSIC; Generalitat de Catalunya [SGR-770]; US Department of Energy, Office of Basic Energy Sciences, Division of Materials Sciences and Engineering FX This work was supported by MINECO (MAT2011-28874-C02, CSD2007-0041, IPT-2011-1090-920000, Generalitat de Catalunya (Pla de Recerca SGR-770 and XaRMAE). The research leading to these results has also received funding from EU-FP7 NMP-LA-2012-280432 EUROTAPES project and Cost Action MP1201. VR acknowledges the JAE-CSIC PhD grant. Research at LANL (flux creep studies) was supported by the US Department of Energy, Office of Basic Energy Sciences, Division of Materials Sciences and Engineering. NR 42 TC 6 Z9 6 U1 1 U2 21 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0953-2048 EI 1361-6668 J9 SUPERCOND SCI TECH JI Supercond. Sci. Technol. PD NOV PY 2014 VL 27 IS 11 AR 115008 DI 10.1088/0953-2048/27/11/115008 PG 7 WC Physics, Applied; Physics, Condensed Matter SC Physics GA AW3OL UT WOS:000346196100009 ER PT J AU Beese, AM Wei, XD Sarkar, S Ramachandramoorthy, R Roenbeck, MR Moravsky, A Ford, M Yavari, F Keane, DT Loutfy, RO Nguyen, ST Espinosa, HD AF Beese, Allison M. Wei, Xiaoding Sarkar, Sourangsu Ramachandramoorthy, Rajaprakash Roenbeck, Michael R. Moravsky, Alexander Ford, Matthew Yavari, Fazel Keane, Denis T. Loutfy, Raouf O. Nguyen, SonBinh T. Espinosa, Horacio D. TI Key Factors Limiting Carbon Nanotube Yarn Strength: Exploring Processing-Structure-Property Relationships SO ACS NANO LA English DT Article DE carbon nanotube; yarn; processing-structure-property relationships; multiscale Monte Carlo modeling; hierarchical composites design ID COMPOSITE YARNS; ELECTRICAL-CONDUCTIVITY; MECHANICAL-PROPERTIES; STATISTICAL STRENGTH; TENSILE-STRENGTH; LENGTH SCALES; SPUN YARNS; FIBERS; POLYMER; LOAD AB Studies of carbon nanotube (CNT) based composites have been unable to translate the extraordinary load-bearing capabilities of individual CNTs to macroscale composites such as yarns. A key challenge lies in the lack of understanding of how properties of filaments and interfaces across yarn hierarchical levels govern the properties of macroscale yarns. To provide insight required to enable the development of superior CNT yarns, we investigate the fabrication-structure-mechanical property relationships among CNT yarns prepared by different techniques and employ a Monte Carlo based model to predict upper bounds on their mechanical properties. We study the correlations between different levels of alignment and porosity and yarn strengths up to 2.4 GPa. The uniqueness of this experimentally informed modeling approach is the models ability to predict when filament rupture or interface sliding dominates yarn failure based on constituent mechanical properties and structural organization observed experimentally. By capturing this transition and predicting the yarn strengths that could be obtained under ideal fabrication conditions, the model provides critical insights to guide future efforts to improve the mechanical performance of CNT yarn systems. This multifaceted study provides a new perspective on CNT yarn design that can serve as a foundation for the development of future composites that effectively exploit the superior mechanical performance of CNTs. C1 [Beese, Allison M.; Wei, Xiaoding; Ramachandramoorthy, Rajaprakash; Roenbeck, Michael R.; Ford, Matthew; Yavari, Fazel; Espinosa, Horacio D.] Northwestern Univ, Dept Mech Engn, Evanston, IL 60208 USA. [Beese, Allison M.] Penn State Univ, Dept Mat Sci & Engn, University Pk, PA 16802 USA. [Sarkar, Sourangsu; Nguyen, SonBinh T.] Northwestern Univ, Dept Chem, Evanston, IL 60208 USA. [Moravsky, Alexander; Loutfy, Raouf O.] MER Corp, Tucson, AZ 85706 USA. [Keane, Denis T.] Northwestern Univ, DND CAT, Adv Photon Source, Argonne Natl Lab, Argonne, IL 60439 USA. [Keane, Denis T.] Northwestern Univ, Dept Mat Sci & Engn, Evanston, IL 60208 USA. RP Espinosa, HD (reprint author), Northwestern Univ, Dept Mech Engn, 2145 Sheridan Rd, Evanston, IL 60208 USA. EM espinosa@northwestern.edu RI Espinosa, Horatio/B-6693-2009; Wei, Xiaoding/A-9952-2011; Nguyen, SonBinh/C-1682-2014; OI Wei, Xiaoding/0000-0002-5173-4923; Nguyen, SonBinh/0000-0002-6977-3445; Ford, Matthew/0000-0002-1053-7149; Beese, Allison/0000-0002-7022-3387 FU ARO MURI [W911NF-09-1-0541]; E.I. DuPont de Nemours Co.; Dow Chemical Company; Northwestern University; U.S. DOE [DE-AC02-06CH11357]; NSF-NSEC; NSF-MRSEC; Keck Foundation; State of Illinois; Department of Defense (DoD) through National Defense Science & Engineering Graduate Fellowship (NDSEG) Program; Northwestern University Ryan Fellowship FX This work was supported by ARO MURI award W911NF-09-1-0541. Portions of this work were performed at the DuPont-Northwestern-Dow Collaborative Access Team (DND-CAT) located at Sector 5 of the Advanced Photon Source (APS). DND-CAT is supported by E.I. DuPont de Nemours & Co., The Dow Chemical Company, and Northwestern University. Use of the APS, an Office of Science User Facility operated for the U.S. Department of Energy (DOE) Office of Science by Argonne National Laboratory, was supported by the U.S. DOE under Contract No. DE-AC02-06CH11357. Part of this work was performed in the EPIC facility of NUANCE Center at Northwestern University. The NUANCE Center is supported by NSF-NSEC, NSF-MRSEC, the Keck Foundation, the State of Illinois, and Northwestern University. M.R.R. acknowledges support from the Department of Defense (DoD) through the National Defense Science & Engineering Graduate Fellowship (NDSEG) Program. M.R.R. and M.F. acknowledge the Northwestern University Ryan Fellowship. We thank Rafael Soler-Crespo for helpful discussions. NR 43 TC 7 Z9 7 U1 6 U2 66 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1936-0851 EI 1936-086X J9 ACS NANO JI ACS Nano PD NOV PY 2014 VL 8 IS 11 BP 11454 EP 11466 DI 10.1021/nn5045504 PG 13 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Chemistry; Science & Technology - Other Topics; Materials Science GA AU4BC UT WOS:000345553000049 PM 25353651 ER PT J AU Mahjouri-Samani, M Tian, M Wang, K Boulesbaa, A Rouleau, CM Puretzky, AA McGuire, MA Srijanto, BR Xiao, K Eres, G Duscher, G Geohegan, DB AF Mahjouri-Samani, Masoud Tian, Mengkun Wang, Kai Boulesbaa, Abdelaziz Rouleau, Christopher M. Puretzky, Alexander A. McGuire, Michael A. Srijanto, Bernadeta R. Xiao, Kai Eres, Gyula Duscher, Gerd Geohegan, David B. TI Digital Transfer Growth of Patterned 2D Metal Chalcogenides by Confined Nanoparticle Evaporation SO ACS NANO LA English DT Article DE 2D layered materials; metal chalcogenides; gallium selenide; molybdenum diselenide; pulsed laser deposition; vapor transport growth ID CHEMICAL-VAPOR-DEPOSITION; LAYER MOSE2; SINGLE-CRYSTALLINE; HIGH-PERFORMANCE; MONOLAYER MOS2; ATOMIC LAYERS; THIN-FILMS; BAND-GAPS; NANOSHEETS; PHOTODETECTORS AB Developing methods for the facile synthesis of two-dimensional (2D) metal chalcogenides and other layered materials is crucial for emerging applications in functional devices. Controlling the stoichiometry, number of the layers, crystallite size, growth location, and areal uniformity is challenging in conventional vapor-phase synthesis. Here, we demonstrate a method to control these parameters in the growth of metal chalcogenide (GaSe) and dichalcogenide (MoSe2) 2D crystals by precisely defining the mass and location of the source materials in a confined transfer growth system. A uniform and precise amount of stoichiometric nanoparticles are first synthesized and deposited onto a substrate by pulsed laser deposition (PLD) at room temperature. This source substrate is then covered with a receiver substrate to form a confined vapor transport growth (VTG) system. By simply heating the source substrate in an inert background gas, a natural temperature gradient is formed that evaporates the confined nanoparticles to grow large, crystalline 2D nanosheets on the cooler receiver substrate, the temperature of which is controlled by the background gas pressure. Large monolayer crystalline domains (similar to 100 mu m lateral sizes) of GaSe and MoSe2 are demonstrated, as well as continuous monolayer films through the deposition of additional precursor materials. This PLD-VTG synthesis and processing method offers a unique approach for the controlled growth of large-area metal chalcogenides with a controlled number of layers in patterned growth locations for optoelectronics and energy related applications. C1 [Mahjouri-Samani, Masoud; Wang, Kai; Boulesbaa, Abdelaziz; Rouleau, Christopher M.; Puretzky, Alexander A.; Srijanto, Bernadeta R.; Xiao, Kai; Geohegan, David B.] Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA. [McGuire, Michael A.; Eres, Gyula; Duscher, Gerd] Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37831 USA. [Tian, Mengkun; Duscher, Gerd] Univ Tennessee, Dept Mat Sci & Engn, Knoxville, TN 37996 USA. RP Mahjouri-Samani, M (reprint author), Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA. EM mahjourisamm@orni.gov RI McGuire, Michael/B-5453-2009; Wang, Kai/H-4361-2011; Mahjouri-Samani, Masoud/Q-2239-2015; Rouleau, Christopher/Q-2737-2015; Puretzky, Alexander/B-5567-2016; Srijanto, Bernadeta/D-4213-2016; Duscher, Gerd/G-1730-2014; Boulesbaa, Abdelaziz/J-3314-2016; Geohegan, David/D-3599-2013; Eres, Gyula/C-4656-2017 OI McGuire, Michael/0000-0003-1762-9406; Wang, Kai/0000-0002-6405-7837; Mahjouri-Samani, Masoud/0000-0002-6080-7450; Rouleau, Christopher/0000-0002-5488-3537; Puretzky, Alexander/0000-0002-9996-4429; Srijanto, Bernadeta/0000-0002-1188-1267; Duscher, Gerd/0000-0002-2039-548X; Boulesbaa, Abdelaziz/0000-0003-4519-4403; Geohegan, David/0000-0003-0273-3139; Eres, Gyula/0000-0003-2690-5214 FU U.S. Department of Energy, Office of Science, Basic Energy Sciences (BES), Materials Sciences and Engineering Division; Scientific User Facilities Division, BES FX Synthesis science including in situ PLD diagnostics, TEM analysis, SEM and AFM studies, bulk crystal growth, and transfer technique development (MMS, KW, GE, DBG, CMR, AAP, MAM, GD, and MT) was supported by the U.S. Department of Energy, Office of Science, Basic Energy Sciences (BES), Materials Sciences and Engineering Division, and performed in part as a user project at the Center for Nanophase Materials Sciences, which is a DOE Office of Science User Facility. Characterization science at CNMS including optical characterization and lithography techniques (AB, KX, BRS, AAP, and CMR) was supported by the Scientific User Facilities Division, BES. NR 45 TC 13 Z9 13 U1 9 U2 99 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1936-0851 EI 1936-086X J9 ACS NANO JI ACS Nano PD NOV PY 2014 VL 8 IS 11 BP 11567 EP 11575 DI 10.1021/nn5048124 PG 9 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Chemistry; Science & Technology - Other Topics; Materials Science GA AU4BC UT WOS:000345553000061 PM 25343499 ER PT J AU Sanii, B Haxton, TK Olivier, GK Cho, A Barton, B Proulx, C Whitelam, S Zuckermann, RN AF Sanii, Babak Haxton, Thomas K. Olivier, Gloria K. Cho, Andrew Barton, Bastian Proulx, Caroline Whitelam, Stephen Zuckermann, Ronald N. TI Structure-Determining Step in the Hierarchical Assembly of Peptoid Nanosheets SO ACS NANO LA English DT Article DE two-dimensional materials; supramolecular assembly; protein-mimetic materials; coarse-grained modeling; bioinspired polymers; interfacial assembly; monolayer compression ID SOLID-PHASE SYNTHESIS; 2-DIMENSIONAL POLYMER; SUPRAMOLECULAR CHEMISTRY; MOLECULAR RECOGNITION; WATER-INTERFACE; MONOLAYERS; CRYSTALS; SURFACE; GRAPHENE; COLLAPSE AB Organic two-dimensional nanomaterials are of growing importance, yet few general synthetic methods exist to produce them in high yields and to precisely functionalize them. We previously developed an efficient hierarchical supramolecular assembly route to peptoid bilayer nanosheets, where the organization of biomimetic polymer sequences is catalyzed by an airwater interface. Here we determine at which stages of assembly the nanoscale and atomic-scale order appear. We used X-ray scattering, grazing incidence X-ray scattering at the airwater interface, electron diffraction, and a recently developed computational coarse-grained peptoid model to probe the molecular ordering at various stages of assembly. We found that lateral packing and organization of the chains occurs during the formation of a peptoid monolayer, prior to its collapse into a bilayer. Identifying the structure-determining step enables strategies to influence nanosheet order, to predict and optimize production yields, and to further engineer this class of material. More generally, our results provide a guide for using fluid interfaces to catalytically assemble 2D nanomaterials. C1 [Sanii, Babak; Haxton, Thomas K.; Olivier, Gloria K.; Cho, Andrew; Barton, Bastian; Proulx, Caroline; Whitelam, Stephen; Zuckermann, Ronald N.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Mol Foundry, Berkeley, CA 94720 USA. RP Zuckermann, RN (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Mol Foundry, 1 Cyclotron Rd, Berkeley, CA 94720 USA. EM rnzuckermann@lbl.gov RI Foundry, Molecular/G-9968-2014; Barton, Bastian/H-9268-2016 FU Defense Threat Reduction Agency [IACRO-B1144571]; Advanced Light Source; National Energy Research Scientific Computing Center, at Lawrence Berkeley National Laboratory; Office of Science, Office of Basic Energy Sciences, U.S. Department of Energy [DE-AC02-05CH11231]; U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-AC02-06CH11357] FX This project was funded by the Defense Threat Reduction Agency under Contract No. IACRO-B1144571. The work was conducted at the Molecular Foundry with support from the Advanced Light Source and the National Energy Research Scientific Computing Center, at Lawrence Berkeley National Laboratory, all of which are supported by the Office of Science, Office of Basic Energy Sciences, U.S. Department of Energy, under Contract No. DE-AC02-05CH11231. Experiments performed at the Advanced Photon Source at Argonne National Laboratory was supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract No. DE-AC02-06CH11357. We also thank I. Kuzmenko (Argonne beamline), J. Holton (ALS beamline) and C. Kisielowski (electron microscopy). NR 59 TC 15 Z9 15 U1 3 U2 96 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1936-0851 EI 1936-086X J9 ACS NANO JI ACS Nano PD NOV PY 2014 VL 8 IS 11 BP 11674 EP 11684 DI 10.1021/nn505007u PG 11 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Chemistry; Science & Technology - Other Topics; Materials Science GA AU4BC UT WOS:000345553000073 PM 25327498 ER PT J AU Das, S Demarteau, M Roelofs, A AF Das, Saptarshi Demarteau, Marcel Roelofs, Andreas TI Ambipolar Phosphorene Field Effect Transistor SO ACS NANO LA English DT Article DE phosphorene; ambipolar field effect transistor; contact resistance; logic inverter ID MOS2 TRANSISTORS; GRAPHENE; CIRCUITS; MOBILITY; CONTACTS AB In this article, we demonstrate enhanced electron and hole transport in few-layer phosphorene field effect transistors (FETs) using titanium as the source/drain contact electrode and 20 nm SiO2 as the back gate dielectric. The field effect mobility values were extracted to be similar to 38 cm(2)/Vs for electrons and similar to 172 cm(2)/Vs for the holes. On the basis of our experimental data, we also comprehensively discuss how the contact resistances arising due to the Schottky barriers at the source and the drain end effect the different regime of the device characteristics and ultimately limit the ON state performance. We also propose and implement a novel technique for extracting the transport gap as well as the Schottky barrier height at the metalphosphorene contact interface from the ambipolar transfer characteristics of the phosphorene FETs. This robust technique is applicable to any ultrathin body semiconductor which demonstrates symmetric ambipolar conduction. Finally, we demonstrate a high gain, high noise margin, chemical doping free, and fully complementary logic inverter based on ambipolar phosphorene FETs. C1 [Das, Saptarshi; Roelofs, Andreas] Argonne Natl Lab, Ctr Nanoscale Mat, Argonne, IL 60439 USA. [Das, Saptarshi; Demarteau, Marcel] Argonne Natl Lab, Div High Energy Phys, Argonne, IL 60439 USA. RP Das, S (reprint author), Argonne Natl Lab, Ctr Nanoscale Mat, 9700 S Cass Ave, Argonne, IL 60439 USA. EM das.sapt@gmail.com RI Roelofs, Andreas/H-1742-2011 OI Roelofs, Andreas/0000-0003-4141-3082 FU DOE Office of High Energy Physics under DoE [DE-AC02-06CH11357]; U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-AC02-06CH11357] FX The work of S.D. is supported by the DOE Office of High Energy Physics under DoE Contract No. DE-AC02-06CH11357. Use of the Center for Nanoscale Materials was supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract No. DE-AC02-06CH11357. NR 33 TC 80 Z9 80 U1 19 U2 149 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1936-0851 EI 1936-086X J9 ACS NANO JI ACS Nano PD NOV PY 2014 VL 8 IS 11 BP 11730 EP 11738 DI 10.1021/nn505868h PG 9 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Chemistry; Science & Technology - Other Topics; Materials Science GA AU4BC UT WOS:000345553000079 PM 25329532 ER PT J AU Liu, B Wu, CH Miao, JW Yang, PD AF Liu, Bin Wu, Cheng-Hao Miao, Jianwei Yang, Peidong TI All Inorganic Semiconductor Nanowire Mesh for Direct Solar Water Splitting SO ACS NANO LA English DT Article DE semiconductor nanowire; BiVO4; Rh-SrTiO3; artificial photosynthesis; solar water splitting ID VISIBLE-LIGHT IRRADIATION; HYDROGEN-PRODUCTION; FACILE FABRICATION; ELECTRON MEDIATOR; DOPED SRTIO3; PHOTOCATALYST; O-2; H-2; NANOSTRUCTURE; SYSTEMS AB The generation of chemical fuels via direct solar-to-fuel conversion from a fully integrated artificial photosynthetic system is an attractive approach for clean and sustainable energy, but so far there has yet to be a system that would have the acceptable efficiency, durability and can be manufactured at a reasonable cost. Here, we show that a semiconductor mesh made from all inorganic nanowires can achieve unassisted solar-driven, overall water-splitting without using any electron mediators. Free-standing nanowire mesh networks could be made in large scales using solution synthesis and vacuum filtration, making this approach attractive for low cost implementation. C1 [Liu, Bin; Wu, Cheng-Hao; Yang, Peidong] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA. [Yang, Peidong] Univ Calif Berkeley, Dept Mat Sci & Engn, Berkeley, CA 94720 USA. [Wu, Cheng-Hao; Yang, Peidong] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA. [Liu, Bin; Miao, Jianwei] Nanyang Technol Univ, Sch Chem & Biomed Engn, Singapore 637459, Singapore. RP Liu, B (reprint author), Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA. EM liubin@ntu.edu.sg; p_yang@berkeley.edu RI Liu, Bin/C-4638-2013; Wu, Cheng Hao/C-9565-2014; Miao, Jianwei/B-7946-2016 FU Office of Science, Office of Basic Energy Sciences, Materials Sciences and Engineering Division, of the U.S. Department of Energy [DE-AC02-05CH11231]; Singapore-Berkeley Research Initiative for Sustainable Energy (SinBeRISE) FX This work was supported by the Director, Office of Science, Office of Basic Energy Sciences, Materials Sciences and Engineering Division, of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231(P-Chem) and the Singapore-Berkeley Research Initiative for Sustainable Energy (SinBeRISE). These authors thank C. K. Chan, C. Liu, and J. W. Sun for helpful discussions. NR 31 TC 28 Z9 29 U1 19 U2 214 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1936-0851 EI 1936-086X J9 ACS NANO JI ACS Nano PD NOV PY 2014 VL 8 IS 11 BP 11739 EP 11744 DI 10.1021/nn5051954 PG 6 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Chemistry; Science & Technology - Other Topics; Materials Science GA AU4BC UT WOS:000345553000080 PM 25365141 ER PT J AU He, Y Piper, DM Gu, M Travis, JJ George, SM Lee, SH Genc, A Pullan, L Liu, J Mao, SX Zhang, JG Ban, CM Wang, CM AF He, Yang Piper, Daniela Molina Gu, Meng Travis, Jonathan J. George, Steven M. Lee, Se-Hee Genc, Arda Pullan, Lee Liu, Jun Mao, Scott X. Zhang, Ji-Guang Ban, Chunmei Wang, Chongmin TI In Situ Transmission Electron Microscopy Probing of Native Oxide and Artificial Layers on Silicon Nanoparticles for Lithium Ion Batteries SO ACS NANO LA English DT Article DE lithium ion battery; silicon nanoparticle; coating; native oxide; aluminum glycerol; in situ TEM ID THIN-FILM ELECTRODE; ELECTROCHEMICAL PERFORMANCE; ANODES; LITHIATION; DEPOSITION; NANOWIRES; EFFICIENCY; STORAGE; AL2O3 AB Surface modification of silicon nanoparticles via molecular layer deposition (MLD) has been recently proved to be an effective way for dramatically enhancing the cyclic performance in lithium ion batteries. However, the fundamental mechanism of how this thin layer of coating functions is not known, which is complicated by the inevitable presence of native oxide of several nanometers on the silicon nanoparticle. Using in situ TEM, we probed in detail the structural and chemical evolution of both uncoated and coated silicon particles upon cyclic lithiation/delithation. We discovered that upon initial lithiation, the native oxide layer converts to crystalline Li2O islands, which essentially increases the impedance on the particle, resulting in ineffective lithiation/delithiation and therefore low Coulombic efficiency. In contrast, the alucone MLD-coated particles show extremely fast, thorough, and highly reversible lithiation behaviors, which are clarified to be associated with the mechanical flexibility and fast Li+/e(-) conductivity of the alucone coating. Surprisingly, the alucone MLD coating process chemically changes the silicon surface, essentially removing the native oxide layer, and therefore mitigates side reactions and detrimental effects of the native oxide. This study provides a vivid picture of how the MLD coating works to enhance the Coulombic efficiency, preserves capacity, and clarifies the role of the native oxide on silicon nanoparticles during cyclic lithiation and delithiation. More broadly, this work also demonstrates that the effect of the subtle chemical modification of the surface during the coating process may be of equal importance to the coating layer itself. C1 [Gu, Meng; Wang, Chongmin] Pacific NW Natl Lab, Environm Mol Sci Lab, Richland, WA 99352 USA. [He, Yang; Mao, Scott X.] Univ Pittsburgh, Dept Mech Engn & Mat Sci, Pittsburgh, PA 15261 USA. [Piper, Daniela Molina; Travis, Jonathan J.; George, Steven M.; Lee, Se-Hee] Univ Colorado, Boulder, CO 80309 USA. [Genc, Arda; Pullan, Lee] FEI Co, Hillsboro, OR 97124 USA. [Liu, Jun; Zhang, Ji-Guang] Pacific NW Natl Lab, Energy & Environm Directorate, Richland, WA 99352 USA. [Ban, Chunmei] Natl Renewable Energy Lab, Golden, CO 80401 USA. RP Mao, SX (reprint author), Univ Pittsburgh, Dept Mech Engn & Mat Sci, 3700 OHara St, Pittsburgh, PA 15261 USA. EM sxm2@pitt.edu; Chunmei.Ban@nrel.gov; Chongmin.Wang@pnnl.gov RI Lee, Sehee/A-5989-2011; George, Steven/O-2163-2013; Gu, Meng/B-8258-2013 OI George, Steven/0000-0003-0253-9184; FU Office of Vehicle Technologies of the U.S. Department of Energy under the Batteries for Advanced Transportation Technologies program [DE-AC02-05CH11231, 18769, DE-AC-36-08GO28308]; Laboratory Directed Research and Development Program as part of the Chemical Imaging Initiative at Pacific Northwest National Laboratory (PNNL); DOE's Office of Biological and Environmental Research at PNNL; DOE [DE-AC05-76RLO1830] FX This work at PNNL and NREL is supported by the Assistant Secretary for Energy Efficiency and Renewable Energy, Office of Vehicle Technologies of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231, Subcontract No. 18769 and DE-AC-36-08GO28308 under the Batteries for Advanced Transportation Technologies program. The in situ microscopic study described in this paper is supported by the Laboratory Directed Research and Development Program as part of the Chemical Imaging Initiative at Pacific Northwest National Laboratory (PNNL). The work was conducted in the William R. Wiley Environmental Molecular Sciences Laboratory (EMSL), a national scientific user facility sponsored by DOE's Office of Biological and Environmental Research and located at PNNL. PNNL is operated by Battelle for the DOE under Contract DE-AC05-76RLO1830. NR 37 TC 26 Z9 26 U1 14 U2 150 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1936-0851 EI 1936-086X J9 ACS NANO JI ACS Nano PD NOV PY 2014 VL 8 IS 11 BP 11816 EP 11823 DI 10.1021/nn505523c PG 8 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Chemistry; Science & Technology - Other Topics; Materials Science GA AU4BC UT WOS:000345553000089 PM 25347792 ER PT J AU Leite, MS Abashin, M Lezec, HJ Gianfrancesco, A Talin, AA Zhitenev, NB AF Leite, Marina S. Abashin, Maxim Lezec, Henri J. Gianfrancesco, Anthony Talin, A. Alec Zhitenev, Nikolai B. TI Nanoscale Imaging of Photo current and Efficiency in CdTe Solar Cells SO ACS NANO LA English DT Article DE photovoltaics; CdTe; scanning photocurrent microscopy; solar cells; NSOM ID BEAM-INDUCED CURRENT; ATOMIC-FORCE MICROSCOPY; ELECTRICAL-PROPERTIES; GRAIN-BOUNDARIES; DEVICES AB The local collection characteristics of grain interiors and grain boundaries in thin-film CdTe polycrystalline solar cells are investigated using scanning photocurrent microscopy. The carriers are locally generated by light injected through a small aperture (50-300 nm) of a near-field scanning optical microscope in an illumination mode. Possible influence of rough surface topography on light coupling is examined and eliminated by sculpting smooth wedges on the granular CdTe surface. By varying the wavelength of light, nanoscale spatial variations in external quantum efficiency are mapped. We find that the grain boundaries (GBs) are better current collectors than the grain interiors (GIs). The increased collection efficiency is caused by two distinct effects associated with the material composition of GBs. First, GBs are charged, and the corresponding built-in field facilitates the separation and the extraction of the photogenerated carriers. Second, the GB regions generate more photocurrent at long wavelength corresponding to the band edge, which can be caused by a smaller local band gap. Resolving carrier collection with nanoscale resolution in solar cell materials is crucial for optimizing the polycrystalline device performance through appropriate thermal processing and passivation of defects and surfaces. C1 [Leite, Marina S.] Univ Maryland, Inst Res Elect & Appl Phys, Dept Mat Sci & Engn, College Pk, MD 20742 USA. [Leite, Marina S.; Abashin, Maxim; Lezec, Henri J.; Gianfrancesco, Anthony; Talin, A. Alec; Zhitenev, Nikolai B.] NIST, Ctr Nanoscale Sci & Technol, Gaithersburg, MD 20899 USA. [Leite, Marina S.; Abashin, Maxim] Univ Maryland, Maryland Nanoctr, College Pk, MD 20742 USA. [Talin, A. Alec] Sandia Natl Labs, Livermore, CA 94550 USA. RP Leite, MS (reprint author), Univ Maryland, Inst Res Elect & Appl Phys, Dept Mat Sci & Engn, College Pk, MD 20742 USA. EM mleite@umd.edu RI Zhitenev, Nikolai/N-1780-2014 FU University of Maryland through the University of Maryland [70NANB10H193]; National Institute of Standards and Technology Center for Nanoscale Science and Technology through the University of Maryland [70NANB10H193]; U.S. DOE National Nuclear Security Administration [DE-AC04-94AL85000] FX The authors thank A. Band, M. Davanco, T. Land in, A. Myers, B. Nikoobakht, K. Srinivasan, J. Schumacher, K. Siebein, and all the CNST NanoFab staff. This work was partially supported by the Cooperative Research Agreement between the University of Maryland and the National Institute of Standards and Technology Center for Nanoscale Science and Technology, Award 70NANB10H193, through the University of Maryland. Sandia is a multiprogram laboratory operated by Sandia Corporation, a Lockheed Martin Company, for the U.S. DOE National Nuclear Security Administration under Contract DE-AC04-94AL85000. NR 35 TC 18 Z9 18 U1 11 U2 75 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1936-0851 EI 1936-086X J9 ACS NANO JI ACS Nano PD NOV PY 2014 VL 8 IS 11 BP 11883 EP 11890 DI 10.1021/nn5052585 PG 8 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary SC Chemistry; Science & Technology - Other Topics; Materials Science GA AU4BC UT WOS:000345553000096 PM 25317926 ER PT J AU Grapes, MD LaGrange, T Woll, K Reed, BW Campbell, GH Lavan, DA Weihs, TP AF Grapes, Michael D. LaGrange, Thomas Woll, Karsten Reed, Bryan W. Campbell, Geoffrey H. LaVan, David A. Weihs, Timothy P. TI In situ transmission electron microscopy investigation of the interfacial reaction between Ni and Al during rapid heating in a nanocalorimeter SO APL MATERIALS LA English DT Article ID THIN-FILM REACTIONS; MEMS APPLICATIONS; PHASE; NUCLEATION; SILICON; TEMPERATURE; KINETICS; COUPLES; GROWTH; ISSUES AB The Al/Ni formation reaction is highly exothermic and of both scientific and technological significance. In this report, we study the evolution of intermetallic phases in this reaction at a heating rate of 830 K/s. 100-nm-thick Al/Ni bilayers were deposited onto nanocalorimeter sensors that enable the measurement of temperature and heat flow during rapid heating. Time-resolved transmission electron diffraction patterns captured simultaneously with thermal measurements allow us to identify the intermetallic phases present and reconstruct the phase transformation sequence as a function of time and temperature. The results show a mostly unaltered phase transformation sequence compared to lower heating rates. (C) 2014 Author(s). All article content, except where otherwise noted, is licensed under a Creative Commons Attribution 3.0 Unported License. C1 [Grapes, Michael D.; Woll, Karsten; Weihs, Timothy P.] Johns Hopkins Univ, Dept Mat Sci & Engn, Baltimore, MD 21218 USA. [Grapes, Michael D.; LaVan, David A.] Natl Inst Stand & Technol, Mat Measurement Sci Div, Mat Measurement Lab, Gaithersburg, MD 20899 USA. [LaGrange, Thomas; Reed, Bryan W.; Campbell, Geoffrey H.] Lawrence Livermore Natl Lab, Mat Sci & Technol Div, Livermore, CA 94550 USA. [Woll, Karsten] Karlsruhe Inst Technol, Inst Appl Mat, D-76344 Eggenstein Leopoldshafen, Germany. RP Grapes, MD (reprint author), Johns Hopkins Univ, Dept Mat Sci & Engn, Baltimore, MD 21218 USA. EM mgrapes1@jhu.edu; david.lavan@nist.gov; weihs@jhu.edu RI Weihs, Timothy/A-3313-2010 FU Summer Undergraduate Research Fellowship student at the National Institute of Standards and Technology (NIST); NIST [70NANB9H9146]; National Science Foundation [DMR-1308966]; U.S. Department of Energy [DE-FG02-09ER46648]; U.S. Department of Energy by LLNL [DE-AC52-07NA27344]; U.S. Department of Energy, Office of Basic Energy Sciences, Division of Materials Science and Engineering [FWP SCW0974]; Open Access Promotion Fund of the Johns Hopkins University Libraries FX The authors are grateful to Bernadette Cannon for her help calibrating nanocalorimeter sensors during her time as a Summer Undergraduate Research Fellowship student at the National Institute of Standards and Technology (NIST). M.D.G. and T.P.W. were supported in part by NIST Grant No. 70NANB9H9146 and in part by National Science Foundation Grant No. DMR-1308966. M.D.G., K.W., and T.P.W. were supported in part by U.S. Department of Energy Grant No. DE-FG02-09ER46648. Nanocalorimeter fabrication was performed at the NIST Center for Nanoscale Science & Technology. The work presented in this article was conducted at the Lawrence Livermore National Laboratory (LLNL) DTEM facility under the auspices of the U.S. Department of Energy by LLNL under Contract No. DE-AC52-07NA27344. The DTEM experiments conducted at LLNL and effort of T.L., B.W.R., and G.H.C. were supported by the U.S. Department of Energy, Office of Basic Energy Sciences, Division of Materials Science and Engineering under FWP SCW0974. Certain commercial equipment, instruments, or materials are identified in this document. Such identification does not imply recommendation or endorsement by the National Institute of Standards and Technology, nor does it imply that the products identified are necessarily the best available for the purpose. Since the completion of this work, T.L. and B.W.R. have become employees at Integrated Dynamic Electron Solutions, Inc., a start-up company marketing time-resolved electron microscope technology. Publication of this article was funded in part by the Open Access Promotion Fund of the Johns Hopkins University Libraries. NR 37 TC 4 Z9 5 U1 7 U2 39 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 2166-532X J9 APL MATER JI APL Mater. PD NOV PY 2014 VL 2 IS 11 DI 10.1063/1.4900818 PG 7 WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied SC Science & Technology - Other Topics; Materials Science; Physics GA AU5HZ UT WOS:000345638800021 ER PT J AU Li, L Zhou, HD Yan, JQ Mandrus, D Keppens, V AF Li, Ling Zhou, Haidong Yan, Jiaqiang Mandrus, David Keppens, Veerle TI Research Update: Magnetic phase diagram of EuTi1-xBxO3 (B = Zr, Nb) SO APL MATERIALS LA English DT Article ID ELECTRICAL-PROPERTIES; PEROVSKITE; EUZRO3 AB We report the magnetic phase diagram of EuTi1-xBxO3 (B = Zr, Nb), determined from magnetization and heat capacity measurements. Upon Zr-doping, the anti-ferromagnetic ordering temperature T-N of EuTi1-xZrxO3 gradually decreases from 5.6 K (x = 0) to 4.1 K (x = 1). Whereas a similar decrease in T-N is observed for small amounts of Nb doping (x <= 0.05), ferromagnetism is induced in EuTi1-xNbxO3 with x > 0.05. The ferromagnetic interaction between localized Eu 4f spins mediated by itinerant electrons introduced by Nb doping results in the ferromagnetism in EuTi1-xNbxO3. (C) 2014 Author(s). All article content, except where otherwise noted, is licensed under a Creative Commons Attribution 3.0 Unported License. C1 [Li, Ling; Yan, Jiaqiang; Mandrus, David; Keppens, Veerle] Univ Tennessee, Dept Mat Sci & Engn, Knoxville, TN 37996 USA. [Zhou, Haidong] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA. [Yan, Jiaqiang; Mandrus, David] Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA. RP Li, L (reprint author), Univ Tennessee, Dept Mat Sci & Engn, Knoxville, TN 37996 USA. RI Li , Ling /J-3322-2016; Zhou, Haidong/O-4373-2016 OI Li , Ling /0000-0002-2866-8323; FU NSF-DMR [DMR-1350002]; U.S. Department of Energy, Basic Energy Sciences, Materials Sciences and Engineering Division; Gordon and Betty Moore foundation FX It is a pleasure to thank Dr. Michael Koehler for a critical reading of the manuscript. H.D.Z. is supported by NSF-DMR through award DMR-1350002. J.-Q. Yan acknowledges support from the U.S. Department of Energy, Basic Energy Sciences, Materials Sciences and Engineering Division. D.G. M. and L.L. acknowledge support from the Gordon and Betty Moore foundation. NR 18 TC 3 Z9 3 U1 0 U2 17 PU AMER INST PHYSICS PI MELVILLE PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA SN 2166-532X J9 APL MATER JI APL Mater. PD NOV PY 2014 VL 2 IS 11 AR 110701 DI 10.1063/1.4902137 PG 6 WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied SC Science & Technology - Other Topics; Materials Science; Physics GA AU5HZ UT WOS:000345638800001 ER PT J AU Alberi, K Mialitsin, AV Fluegel, B Crooker, SA Reno, JL Mascarenhas, A AF Alberi, Kirstin Mialitsin, Aleksej V. Fluegel, Brian Crooker, Scott A. Reno, John L. Mascarenhas, Angelo TI Magnetic field-induced direct-indirect crossover in AlxGa1-xAs SO APPLIED PHYSICS EXPRESS LA English DT Article ID SEMICONDUCTOR ALLOYS; HYDROSTATIC-PRESSURE; STATES AB We induce a direct-indirect band gap crossover in a single AlxGa1-xAs sample by using high magnetic fields. A reduction in the photoluminescence (PL) peak energy and onset of an asymmetric peak lineshape at magnetic fields >38 T result from a competition between the radiative recombination lifetime and the carrier migration time as the alloy becomes indirect. By analyzing the progression of the PL lineshape as the magnetic field is increased we show that the crossover is an alloy disorder-broadened, first-order phase transition. (C) 2014 The Japan Society of Applied Physics C1 [Alberi, Kirstin; Mialitsin, Aleksej V.; Fluegel, Brian; Mascarenhas, Angelo] Natl Renewable Energy Lab, Golden, CO 80401 USA. [Crooker, Scott A.] Los Alamos Natl Lab, Natl High Magnet Field Lab, Los Alamos, NM 87545 USA. [Reno, John L.] Sandia Natl Labs, Ctr Integrated Nanotechnol, Albuquerque, NM 87123 USA. RP Alberi, K (reprint author), Natl Renewable Energy Lab, Golden, CO 80401 USA. FU DOE, Office of Science, Basic Energy Sciences [DE-AC36-08GO28308]; State of Florida; U.S. DOE National Nuclear Security Administration [DE-AC04-94AL85000]; [NSF-DMR-1157490] FX We acknowledge the financial support of the DOE, Office of Science, Basic Energy Sciences under DE-AC36-08GO28308. Work at LANL was supported by NSF-DMR-1157490, and the State of Florida. Sample growth was performed at the Center for Integrated Nanotechnologies, a U.S. Department of Energy, Office of Basic Energy Sciences user facility. Sandia National Laboratory is a multi-program laboratory managed and operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the U.S. DOE National Nuclear Security Administration under contract DE-AC04-94AL85000. NR 18 TC 1 Z9 1 U1 2 U2 9 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 1882-0778 EI 1882-0786 J9 APPL PHYS EXPRESS JI Appl. Phys. Express PD NOV PY 2014 VL 7 IS 11 AR 111201 DI 10.7567/APEX.7.111201 PG 4 WC Physics, Applied SC Physics GA AW2LO UT WOS:000346119500005 ER PT J AU Poelen, JH Simons, JD Mungall, CJ AF Poelen, Jorrit H. Simons, James D. Mungall, Chris J. TI Global biotic interactions: An open infrastructure to share and analyze species-interaction datasets SO ECOLOGICAL INFORMATICS LA English DT Article DE Species interactions; Data integration; Taxonomy; Ontology ID ECOREGIONS; NETWORKS; VISUALIZATION; BIODIVERSITY; ENVIRONMENT; ECOSYSTEM; SCIENCES; ONTOLOGY; SYSTEM; WORLD AB An intricate network of interactions between organisms and their environment form the ecosystems that sustain life on earth. With a detailed understanding of these interactions, ecologists and biologists can make better informed predictions about the ways different environmental factors will impact ecosystems. Despite the abundance of research data on biotic and abiotic interactions, no comprehensive and easily accessible data collection is available that spans taxonomic, geospatial, and temporal domains. Biotic-interaction datasets are effectively siloed, inhibiting cross-dataset comparisons. In order to pool resources and bring to light individual datasets, specialized research tools are needed to aggregate, normalize, and integrate existing datasets with standard taxonomies, ontologies, vocabularies, and structured data repositories. Global Biotic Interactions (GloBI) provides such tools by way of an open, community-driven infrastructure designed to lower the barrier for researchers to perform ecological systems analysis and modeling. GloBI provides a tool that (a) ingests, normalizes, and aggregates datasets, (b) integrates interoperable data with accepted ontologies (e.g., OBO Relations Ontology, Uberon, and Environment Ontology), vocabularies (e.g., Coastal and Marine Ecological Classification Standard), and taxonomies (e.g., Integrated Taxonomic Information System and National Center for Biotechnology Information Taxonomy Database), (c) makes data accessible through an application programming interface (API) and various data archives (Darwin Core, Turtle, and Neo4j), and (d) houses a data collection of about 700,000 species interactions across about 50,000 taxa, covering over 1100 references from 19 data sources. GloBI has taken an open-source and open-data approach in order to make integrated species-interaction data maximally accessible and to encourage users to provide feedback, contribute data, and improve data access methods. The GloBI collection of datasets is currently used in the Encyclopedia of Life (EOL) and Gulf of Mexico Species Interactions (GoMexSI). (C) 2014 The Authors. Published by Elsevier B.V. C1 [Simons, James D.] Ctr Coastal Studies, Nat Resource Ctr, Corpus Christi, TX 78412 USA. [Mungall, Chris J.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Genom Div, Berkeley, CA 94720 USA. RP Poelen, JH (reprint author), 400 Perkins St,Apt 104, Oakland, CA 94610 USA. EM jhpoelen@xs4all.nl RI Trivedi, Kruti/E-7558-2015 FU Encyclopedia of Life, EOL Rubenstein Fellows Program; David M. Rubenstein Grant (CRDF), Smithsonian Institution [EOL-33066-13/F33066] FX We thank Jen Hammock, Brian Hayden, Peter Roopnarine, Jeff Holmes, and Cyndy Parr for sharing their ideas, participating in discussions, and supporting our efforts. Also, thanks to Robert Reiz, Goran Bodenschatz, Stephan Gosnell, and Sergey Slyusarev for using and providing feedback on GloBI data as part of developing software and visualizations. Thanks to Pepper Luboff for editing this article. Last but not least, we thank all the data contributors that have opened up their datasets and answered many of our questions: Malcolm Storey; Joel Sachs; Ken-ichi Ueda; Allen Hurlbert; Ben Raymond; Carolyn Barnes; Jarrett Byrnes; Colt Cook; Jos Ferrer-Paris; Anne Thessen; Institute for Marine Resources and Ecosystem Studies (IMARES); International Council for Exploration of the Sea (ICES); UK Species Inventory at the Angela Marmont Centre for UK Biodiversity, the Natural History Museum, London; and many others. This work has been supported by the Encyclopedia of Life, EOL Rubenstein Fellows Program and the David M. Rubenstein Grant (CRDF EOL-33066-13/F33066), Smithsonian Institution. NR 52 TC 15 Z9 16 U1 3 U2 16 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 1574-9541 EI 1878-0512 J9 ECOL INFORM JI Ecol. Inform. PD NOV PY 2014 VL 24 BP 148 EP 159 DI 10.1016/j.ecoinf.2014.08.005 PG 12 WC Ecology SC Environmental Sciences & Ecology GA AU7WU UT WOS:000345810000016 ER PT J AU Handley, KM Bartels, D O'Loughlin, EJ Williams, KH Trimble, WL Skinner, K Gilbert, JA Desai, N Glass, EM Paczian, T Wilke, A Antonopoulos, D Kemner, KM Meyer, F AF Handley, Kim M. Bartels, Daniela O'Loughlin, Edward J. Williams, Kenneth H. Trimble, William L. Skinner, Kelly Gilbert, Jack A. Desai, Narayan Glass, Elizabeth M. Paczian, Tobias Wilke, Andreas Antonopoulos, Dionysios Kemner, Kenneth M. Meyer, Folker TI The complete genome sequence for putative H-2- and S-oxidizer Candidatus Sulfuricurvum sp., assembled de novo from an aquifer-derived metagenome SO ENVIRONMENTAL MICROBIOLOGY LA English DT Article ID URANIUM-CONTAMINATED GROUNDWATER; CBB(3)-TYPE CYTOCHROME-OXIDASE; SULFATE-REDUCING BACTERIA; RIBOSOMAL-RNA SEQUENCES; C-SULFIDE DEHYDROGENASE; THIOBACILLUS SP W5; ESCHERICHIA-COLI; MICROBIAL COMMUNITY; PHYLOGENETIC DIVERSITY; EPSILON-PROTEOBACTERIA AB We reconstructed the complete 2.4Mb-long genome of a previously uncultivated epsilonproteobacterium, Candidatus Sulfuricurvum sp. RIFRC-1, via assembly of short-read shotgun metagenomic data using a complexity reduction approach. Genome-based comparisons indicate the bacterium is a novel species within the Sulfuricurvum genus, which contains one cultivated representative, S.kujiense. Divergence between the species appears due in part to extensive genomic rearrangements, gene loss and chromosomal versus plasmid encoding of certain (respiratory) genes by RIFRC-1. Deoxyribonucleic acid for the genome was obtained from terrestrial aquifer sediment, in which RIFRC-1 comprised approximate to 47% of the bacterial community. Genomic evidence suggests RIFRC-1 is a chemolithoautotrophic diazotroph capable of deriving energy for growth by microaerobic or nitrate-/nitric oxide-dependent oxidation of S-0, sulfide or sulfite or H-2 oxidation. Carbon may be fixed via the reductive tricarboxylic acid cycle. Consistent with these physiological attributes, the local aquifer was microoxic with small concentrations of available nitrate, small but elevated concentrations of reduced sulfur and NH4+/NH3-limited. Additionally, various mechanisms for heavy metal and metalloid tolerance and virulence point to a lifestyle well-adapted for metal(loid)-rich environments and a shared evolutionary past with pathogenic Epsilonproteobacteria. Results expand upon recent findings highlighting the potential importance of sulfur and hydrogen metabolism in the terrestrial subsurface. C1 [Handley, Kim M.; Gilbert, Jack A.] Univ Chicago, Dept Ecol & Evolut, Chicago, IL 60637 USA. [Bartels, Daniela; Glass, Elizabeth M.; Paczian, Tobias; Wilke, Andreas; Meyer, Folker] Univ Chicago, Computat Inst, Chicago, IL 60637 USA. [Handley, Kim M.; Bartels, Daniela; Gilbert, Jack A.; Antonopoulos, Dionysios; Meyer, Folker] Argonne Natl Lab, Inst Genom & Syst Biol, Lemont, IL 60439 USA. [O'Loughlin, Edward J.; Skinner, Kelly; Gilbert, Jack A.; Antonopoulos, Dionysios; Kemner, Kenneth M.] Argonne Natl Lab, Biosci Div, Argonne, IL 60439 USA. [Trimble, William L.; Desai, Narayan; Glass, Elizabeth M.; Paczian, Tobias; Wilke, Andreas; Meyer, Folker] Argonne Natl Lab, Math & Comp Sci Div, Argonne, IL 60439 USA. [Williams, Kenneth H.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Earth Sci, Berkeley, CA 94720 USA. RP Meyer, F (reprint author), Argonne Natl Lab, Inst Genom & Syst Biol, Lemont, IL 60439 USA. EM folker@anl.gov RI Williams, Kenneth/O-5181-2014; OI Williams, Kenneth/0000-0002-3568-1155; Trimble, William L./0000-0001-7029-2676; Handley, Kim/0000-0003-0531-3009; Meyer, Folker/0000-0003-1112-2284; O'Loughlin, Edward/0000-0003-1607-9529 FU Argonne National Laboratory (ANL) through the Subsurface Science Scientific Focus Area (SFA) - Biological and Environmental Research (BER) program at the US Department of Energy (DOE) Office of Science [DE-AC02-06CH11357]; Rifle IFRC; Lawrence Berkeley National Laboratory's (LBNL) Sustainable Systems Scientific Focus Area - US DOE Office of Science, BER program [DE-AC02-05CH11231] FX Funding was provided by Argonne National Laboratory (ANL) partially through the Subsurface Science Scientific Focus Area (SFA), which was supported by the Biological and Environmental Research (BER) program at the US Department of Energy (DOE) Office of Science under contract DE-AC02-06CH11357. Work was equally supported through the Rifle IFRC and the Lawrence Berkeley National Laboratory's (LBNL) Sustainable Systems Scientific Focus Area, supported by the US DOE Office of Science, BER program under contract DE-AC02-05CH11231. Access to sediment and groundwater was granted by the Rifle IFRC under the auspices of P.E. Long (LBNL). DNA library preparation and sequencing were performed by M. Domanus and A. Ammar through the Institute for Genomics and Systems Biology's Next Generation Sequencing Core (IGSB-NGS, ANL). NR 163 TC 16 Z9 16 U1 4 U2 40 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 1462-2912 EI 1462-2920 J9 ENVIRON MICROBIOL JI Environ. Microbiol. PD NOV PY 2014 VL 16 IS 11 SI SI BP 3443 EP 3462 DI 10.1111/1462-2920.12453 PG 20 WC Microbiology SC Microbiology GA AU5FF UT WOS:000345631900007 PM 24628880 ER PT J AU Meyer, B Kuehl, JV Price, MN Ray, J Deutschbauer, AM Arkin, AP Stahl, DA AF Meyer, Birte Kuehl, Jennifer V. Price, Morgan N. Ray, Jayashree Deutschbauer, Adam M. Arkin, Adam P. Stahl, David A. TI The energy-conserving electron transfer system used by Desulfovibrio alaskensis strain G20 during pyruvate fermentation involves reduction of endogenously formed fumarate and cytoplasmic and membrane-bound complexes, Hdr-Flox and Rnf SO ENVIRONMENTAL MICROBIOLOGY LA English DT Article ID SULFATE-REDUCING BACTERIA; REDOX LOOP MECHANISM; VULGARIS HILDENBOROUGH; METHANOGENIC BACTERIA; ESCHERICHIA-COLI; GENE-EXPRESSION; METHANOSPIRILLUM-HUNGATEI; DESULFURICANS ATCC-27774; WOLINELLA-SUCCINOGENES; RESPIRATORY COMPLEX AB The adaptation capability of Desulfovibrio to natural fluctuations in electron acceptor availability was evaluated by studying Desulfovibrio alaskensis strain G20 under varying respiratory, fermentative and methanogenic coculture conditions in chemostats. Transition from lactate to pyruvate in coculture resulted in a dramatic shift in the population structure and closer interspecies cell-to-cell interactions. Lower methane production rates in coculture than predicted from pyruvate input was attributed to redirection of electron flow to fumarate reduction. Without a methanogenic partner, accumulation of H-2 and formate resulted in greater succinate production. Comparative transcript and gene fitness analysis in concert with physiological data of G20 wildtype and mutants demonstrated that pyruvate fermentation involves respiration of cytoplasmically formed fumarate using cytoplasmic and membrane-bound energy-conserving complexes, Rnf, Hdr-Flox-1 and Hmc. At the low H-2/formate levels maintained in coculture, Rnf likely functions as proton-pumping ferredoxin (Fd):type-I cytochrome c oxidoreductase, which transitions to a proton-pumping Fd(red):nicotinamide adenine dinucleotide (NAD(+)) oxidoreductase at high H-2/formate levels during fermentation in monoculture. Hdr-Flox-1 is postulated to recycle Fd(red) via a flavin-based electron bifurcation involving NADH, Fd(ox) and the thiol/disulphide-containing DsrC. In a menaquinone (MQ)-based electron confurcation reaction, the high-molecular-weight cytochrome-c(3) complex, Hmc, is proposed to then couple DsrC(red) and periplasmic H-2/formate oxidation using the MQ pool to fuel a membrane-bound fumarate reductase. C1 [Meyer, Birte; Stahl, David A.] Univ Washington, Dept Civil & Environm Engn, Seattle, WA 98195 USA. [Kuehl, Jennifer V.; Price, Morgan N.; Ray, Jayashree; Deutschbauer, Adam M.; Arkin, Adam P.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Phys Biosci Div, Berkeley, CA 94704 USA. RP Stahl, DA (reprint author), Univ Washington, Dept Civil & Environm Engn, Seattle, WA 98195 USA. EM dastahl@u.washington.edu RI Ray, Jayashree/F-9162-2016; Arkin, Adam/A-6751-2008; OI Arkin, Adam/0000-0002-4999-2931; Price, Morgan/0000-0002-4251-0362 FU Office of Science, Office of Biological and Environmental Research of the U. S. Department of Energy [DE-AC02-05CH11231] FX We thank Marcin Zemla (Lawrence Berkeley National Laboratory, Berkeley) for assistance as well as M. Auer (Lawrence Berkeley National Laboratory, Berkeley) for the use of the Hitachi S5000 Scanning Electron Microscope and the courtesy of providing the SEM images. This work conducted by Ecosystems and Networks Integrated with Genes and Molecular Assemblies (ENIGMA; http://enigma.lbl.gov), a Scientific Focus Area Program at Lawrence Berkeley National Laboratory, was supported by the Office of Science, Office of Biological and Environmental Research of the U. S. Department of Energy under Contract No. DE-AC02-05CH11231. NR 87 TC 8 Z9 9 U1 4 U2 27 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 1462-2912 EI 1462-2920 J9 ENVIRON MICROBIOL JI Environ. Microbiol. PD NOV PY 2014 VL 16 IS 11 SI SI BP 3463 EP 3486 DI 10.1111/1462-2920.12405 PG 24 WC Microbiology SC Microbiology GA AU5FF UT WOS:000345631900008 PM 24447568 ER PT J AU Vasin, R Lebensohn, RA Matthies, S Tome, CN Wenk, HR AF Vasin, Roman Lebensohn, Ricardo A. Matthies, Siegfried Tome, Carlos N. Wenk, Hans-Rudolf TI The influence of grain shape and volume fraction of sheet silicates on elastic properties of aggregates: Biotite platelets in an isotropic matrix SO GEOPHYSICS LA English DT Article ID PREFERRED ORIENTATION; SHALE ANISOTROPY; SELF-CONSISTENT; POLYCRYSTALS; MICROCRACKS; OUTOKUMPU; CRYSTAL; GNEISS; FIELD AB Elastic anisotropy of sheet-silicate-rich rocks such as shales and slates strongly depends on the orientation distribution of platelet-shaped minerals, as well as shape and orientation of pores. Bulk elastic anisotropy of the rock results in the anisotropy with respect to the propagation of elastic waves, and consequently, the fastest P-waves can travel with velocities exceeding the slowest velocities by a factor of two or even greater. An important factor is the sheet-silicate's grain shapes. We approached a model system of biotite platelets in an isotropic matrix with different methods: A mean-field self-consistent method that considered ellipsoidal particles in an effective anisotropic matrix, and a full-field method based on fast Fourier transforms that considered the microstructure, the topology of the polycrystal, and local interactions. Both methods provided numerically very close results. Using these results, we predicted that the aggregate with more oblate grain shape (thinner platelets) was elastically more anisotropic than the material with grains of less oblate shape, but only for small volume fractions of oriented platelets. For large fractions of platelets, the opposite was true. This switchover in the elastic anisotropy depended on texture strength, platelet shape, and elastic properties of the isotropic matrix. C1 [Vasin, Roman; Matthies, Siegfried; Wenk, Hans-Rudolf] Univ Calif Berkeley, Dept Earth & Planetary Sci, Berkeley, CA 94720 USA. [Vasin, Roman] Joint Nucl Res Inst, Frank Lab Neutron Phys, Dubna, Russia. [Lebensohn, Ricardo A.; Tome, Carlos N.] Los Alamos Natl Lab, Div Mat Sci & Technol, Los Alamos, NM 87545 USA. RP Vasin, R (reprint author), Univ Calif Berkeley, Dept Earth & Planetary Sci, Berkeley, CA 94720 USA. EM olddragon@mail.ru; lebenso@lanl.gov; matthies.vinel@gmail.com; tome@lanl.gov; wenk@berkeley.edu RI Vasin, Roman/C-9486-2015; Tome, Carlos/D-5058-2013; Lebensohn, Ricardo/A-2494-2008 OI Vasin, Roman/0000-0001-5236-0268; Lebensohn, Ricardo/0000-0002-3152-9105 FU National Science Foundation (NSF) [EAR-1343908]; Department of Energy (DOE) [DE-FG02-05ER15637] FX The authors would like to acknowledge support from National Science Foundation (NSF) (EAR-1343908) and Department of Energy (DOE) (DE-FG02-05ER15637). We are appreciative for comments from the editor and three reviewers that helped improve the manuscript. NR 28 TC 4 Z9 4 U1 0 U2 6 PU SOC EXPLORATION GEOPHYSICISTS PI TULSA PA 8801 S YALE ST, TULSA, OK 74137 USA SN 0016-8033 EI 1942-2156 J9 GEOPHYSICS JI Geophysics PD NOV-DEC PY 2014 VL 79 IS 6 BP D433 EP D441 DI 10.1190/GEO2014-0148.1 PG 9 WC Geochemistry & Geophysics SC Geochemistry & Geophysics GA AU9JM UT WOS:000345908500013 ER PT J AU Zhang, C Revil, A Fujita, Y Munakata-Marr, J Redden, G AF Zhang, Chi Revil, Andre Fujita, Yoshiko Munakata-Marr, Junko Redden, George TI Quadrature conductivity: A quantitative indicator of bacterial abundance in porous media SO GEOPHYSICS LA English DT Article ID SPECTRAL INDUCED POLARIZATION; OIL-BEARING SANDS; COMPLEX CONDUCTIVITY; DIELECTRIC-PROPERTIES; REDOX CONDITIONS; BIODEGRADED OIL; GROUNDWATER; DIFFUSION; SIGNALS AB The abundance and growth stages of bacteria in subsurface porous media affect the concentrations and distributions of charged species within the solid-solution interfaces. Therefore, spectral induced polarization (SIP) measurements can be used to monitor changes in bacterial biomass and growth stage. Our goal was to gain a better understanding of the SIP response of bacteria present in a porous material. Bacterial cell surfaces possess an electric double layer and therefore become polarized in an electric field. We performed SIP measurements over the frequency range of 0.1-1 kHz on cell suspensions alone and cell suspensions mixed with sand at four pore water conductivities. We used Zymomonas mobilis at four different cell densities (including the background). The quadrature conductivity spectra exhibited two peaks, one around 0.05-0.10 Hz and the other around 1-10 Hz. Because SIP measurements on bacterial suspensions are typically made at frequencies greater than 1 Hz, these peaks have not been previously reported. In the bacterial suspensions in growth medium, the quadrature conductivity at peak I was linearly proportional to the density of the bacteria. For the case of the suspensions mixed with sands, we observed that peak II presented a smaller increase in the quadrature conductivity with the cell density. A comparison of the experiments with and without sand grains illustrated the effect of the porous medium on the overall quadrature conductivity response (decrease in the amplitude and shift of the peaks to the lower frequencies). Our results indicate that for a given porous medium, time-lapse SIP has potential for monitoring changes in bacterial abundance within porous media. C1 [Zhang, Chi; Revil, Andre] Colorado Sch Mines, Dept Geophys, Golden, CO 80401 USA. [Zhang, Chi] Idaho Natl Labs, Idaho Falls, ID USA. [Revil, Andre] Univ Savoie, ISTerre, CNRS, UMR, Le Bourget Du Lac, France. [Fujita, Yoshiko] Idaho Natl Lab, Idaho Falls, ID 83415 USA. [Fujita, Yoshiko; Redden, George] Univ Copenhagen, Dept Chem, Nanogeosci Grp, DK-2100 Copenhagen, Denmark. [Munakata-Marr, Junko] Colorado Sch Mines, Dept Civil & Environm Engn, Golden, CO 80401 USA. RP Zhang, C (reprint author), Rutgers State Univ, Dept Earth & Environm Sci, Newark, NJ 07102 USA. EM chi.zhang15@gmail.com; arevil@mines.edu; yfujita@nano.ku.dk; jmmarr@mines.edu; gredden@alumni.stanford.edu RI Fujita, Yoshiko/S-2007-2016; OI Fujita, Yoshiko/0000-0002-4472-4102; Munakata Marr, Junko/0000-0002-3705-6265 FU Idaho National Laboratory Scientific Focus Area; Office of Science; Chevron Energy Technology Company [CW852844] FX This work is funded by Idaho National Laboratory Scientific Focus Area, the Office of Science, and Chevron Energy Technology Company (grant #CW852844). We thank J. Henriksen for advice regarding the choice of bacterial species for the experiments and G. Abdel Aal and E. Atekwana for their comments on a previous version of the manuscript. Y. Fujita and G. Redden would also like to express their deep gratitude to the NanoGeoScience program at Copenhagen University for facilitating their contributions to the preparation of this manuscript, and especially to the National Bank of Denmark for helping to make their residence with Copenhagen University possible. We also thank the three referees for the constructive reviews and the associate editor E. Saenger for handling our manuscript. NR 54 TC 3 Z9 3 U1 1 U2 10 PU SOC EXPLORATION GEOPHYSICISTS PI TULSA PA 8801 S YALE ST, TULSA, OK 74137 USA SN 0016-8033 EI 1942-2156 J9 GEOPHYSICS JI Geophysics PD NOV-DEC PY 2014 VL 79 IS 6 BP D363 EP D375 DI 10.1190/GEO2014-0107.1 PG 13 WC Geochemistry & Geophysics SC Geochemistry & Geophysics GA AU9JM UT WOS:000345908500006 ER PT J AU Dou, S Ajo-Franklin, JB AF Dou, Shan Ajo-Franklin, Jonathan B. TI Full-wavefield inversion of surface waves for mapping embedded low-velocity zones in permafrost SO GEOPHYSICS LA English DT Article ID SIMULATED ANNEALING INVERSION; RAYLEIGH-WAVES; MULTIMODAL INVERSION; SEISMIC TOMOGRAPHY; DISPERSION-CURVES; PHASE-VELOCITY; SEARCH; LAYER; OPTIMIZATION; TEMPERATURES AB Surface waves are advantageous for mapping seismic structures of permafrost, in which irregular velocity gradients are common and thus the effectiveness of refraction methods are limited. Nevertheless, the complex velocity structures that are common in permafrost environments often yield unusual dispersion spectra, in which higher-order and leaky modes are dominant. Such unusual dispersion spectra were prevalent in the multichannel surface-wave data acquired from our permafrost study site at Barrow, Alaska. Owing to the difficulties in picking and identifying dispersion curves from these dispersion spectra, conventional surface-wave inversion methods become problematic to apply. To overcome these difficulties, we adopted a full-wavefield method to invert for velocity models that can best fit the dispersion spectra instead of the dispersion curves. The inferred velocity models were consistent with collocated electric resistivity results and with subsequent confirmation cores, which indicated the reliability of the recovered seismic structures. The results revealed embedded low-velocity zones underlying the ice-rich permafrost at our study site - an unexpected feature considering the low ground temperatures of -10 degrees C to -8 degrees C. The low velocities in these zones (similar to 70%-80% lower than the overlying ice-rich permafrost) were most likely caused by saline pore-waters that prevent the ground from freezing, and the resultant velocity structures are vivid examples of complex subsurface properties in permafrost terrain. We determined that full-wavefield inversion of surface waves, although carrying higher computational costs than conventional methods, can be an effective tool for delineating the seismic structures of permafrost. C1 [Dou, Shan] Univ Calif Berkeley, Dept Earth & Planetary Sci, Berkeley, CA 94720 USA. [Ajo-Franklin, Jonathan B.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Earth Sci, Berkeley, CA 94720 USA. RP Dou, S (reprint author), Univ Calif Berkeley, Dept Earth & Planetary Sci, Berkeley, CA 94720 USA. EM shandou@berkeley.edu; jbajo-franklin@lbl.gov RI Dou, Shan/H-5085-2016; Ajo-Franklin, Jonathan/G-7169-2015; OI Dou, Shan/0000-0001-5420-8489; Ajo-Franklin, Jonathan/0000-0002-6666-4702 FU Office of Biological and Environmental Research in the DOE Office of Science [DEAC0205CH11231, DE-AC05-00OR22725] FX As part of the Next-Generation Ecosystem Experiments (NGEE-Arctic) project sponsored by the Office of Biological and Environmental Research in the DOE Office of Science, this study is supported through contract DEAC0205CH11231 to Lawrence Berkeley National Laboratory and through contract DE-AC05-00OR22725 to Oak Ridge National Laboratory. We thank S. Hubbard (Lawrence Berkeley National Laboratory) and S. Wullschleger (Oak Ridge National Laboratory) for their leadership within the NGEE-Arctic program. We also thank J. Peterson, B. Dafflon, C. Ulrich (all of Lawrence Berkeley National Laboratory), and A. Gusmeroli (University of Alaska, Fairbanks) for their generous help in performing the seismic survey in the harsh field environment at Barrow. We appreciate the valuable suggestions offered by D. Dreger (University of California, Berkeley) and R. Herrmann (Saint Louis University). M. Robertson (Lawrence Berkeley National Laboratory) provided substantial assistance in making maps of the study site. B. Dafflon significantly assisted our analysis by providing preliminary data on the core samples relevant to this study. Last but not least, we would like to thank the three reviewers - M. Haney and two anonymous reviewers, the assistant editor L. Valentina Socco, and the associate editor M. Asten for their constructive reviews and comments. NR 79 TC 7 Z9 7 U1 0 U2 15 PU SOC EXPLORATION GEOPHYSICISTS PI TULSA PA 8801 S YALE ST, TULSA, OK 74137 USA SN 0016-8033 EI 1942-2156 J9 GEOPHYSICS JI Geophysics PD NOV-DEC PY 2014 VL 79 IS 6 BP EN107 EP EN124 DI 10.1190/GEO2013-0427.1 PG 18 WC Geochemistry & Geophysics SC Geochemistry & Geophysics GA AU9JM UT WOS:000345908500023 ER PT J AU Chen, JS Glinsky, ME AF Chen, Jinsong Glinsky, Michael E. TI Stochastic inversion of seismic PP and PS data for reservoir parameter estimation SO GEOPHYSICS LA English DT Article ID VELOCITY; DENSITY; MODEL AB We have investigated the value of isotropic seismic converted-wave (i.e., PS) data for reservoir parameter estimation using stochastic approaches based on a floating-grain rock-physics model. We first performed statistical analysis on a simple two-layer model built on actual borehole logs and compared the relative value of PS data versus amplitude-variation-with-offset (AVO) gradient data for estimating the floating-grain fraction. We found that PS data were significantly more informative than AVO gradient data in terms of likelihood functions, and the combination of PS and AVO gradient data together with PP data provided the maximal value for the reservoir parameter estimation. To evaluate the value of PS data under complex situations, we developed a hierarchical Bayesian model to combine seismic PP and PS data and their associated time registration. We extended a model-based Bayesian method developed previously for inverting seismic PP data only, by including PS responses and time registration as additional data and PS traveltime and reflectivity as additional variables. We applied the method to a synthetic six-layer model that closely mimics real field scenarios. We found that PS data provided more information than AVO gradient data for estimating the floating-grain fraction, porosity, net-to-gross, and layer thicknesses when their corresponding priors were weak. C1 [Chen, Jinsong] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Earth Sci, Berkeley, CA 94720 USA. [Glinsky, Michael E.] ION Geophys, Houston, TX USA. RP Chen, JS (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Earth Sci, Berkeley, CA 94720 USA. EM jchen@lbl.gov; michael.glinsky@iongeo.com RI Chen, Jinsong/A-1374-2009 FU Ion Geophysical FX We thank Ion Geophysical for funding and for permission to publish this work. We thank J. Gunning from the Commonwealth Scientific and Industrial Research Organisation for providing help in understanding the Delivery codes and D. Sassen from Ion Geophysical for helping to answer some questions. We also thank S. Kaplan, H. H. Veire, M. Bosch, and one anonymous reviewer for their constructive comments. NR 21 TC 2 Z9 3 U1 0 U2 2 PU SOC EXPLORATION GEOPHYSICISTS PI TULSA PA 8801 S YALE ST, TULSA, OK 74137 USA SN 0016-8033 EI 1942-2156 J9 GEOPHYSICS JI Geophysics PD NOV-DEC PY 2014 VL 79 IS 6 BP R233 EP R246 DI 10.1190/GEO2013-0456.1 PG 14 WC Geochemistry & Geophysics SC Geochemistry & Geophysics GA AU9JM UT WOS:000345908500036 ER PT J AU Chen, Y Zhang, YX Lin, Y Yang, ZB Su, D Han, MF Chen, FL AF Chen, Yu Zhang, Yanxiang Lin, Ye Yang, Zhibin Su, Dong Han, Minfang Chen, Fanglin TI Direct-methane solid oxide fuel cells with hierarchically porous Ni-based anode deposited with nanocatalyst layer SO NANO ENERGY LA English DT Article DE Coking resistance; Heterogeneous catalyst; Solid oxide fuel cells; Freeze-drying tape-casting; Nano nickel carbide ID TAPE-CASTING PROCESS; NICKEL-BASED ANODES; DIRECT OXIDATION; SURFACE MODIFICATION; NATURAL-GAS; PERFORMANCE; IMPREGNATION; ELECTRODE; POWER; SOFC AB Current development of solid oxide fuel cells (SOFCs) is impeded by direct utilization of hydrocarbon fuels since SOFC anodes suffer from coking readily. We present an innovative design for enhancing the coking resistance of the conventional SOFC anode. A thin nano samaria doped ceria (SDC) catalyst layer has been deposited efficiently via infiltration on the wall surface of the Ni-yttria-stabilized zirconia (Ni-YSZ) anode internal gas diffusion channel (5-200 mu m in size) fabricated from freeze-drying tape-casting and vacuum-free infiltration. The efficiency for catalyst infiltration has been significantly improved by using hierarchically porous anode structure with open and straight channels. Single cells with nano SDC layer show very stable cell performance and a peak power density of 0.65 W cm(-2) at 800 degrees C using methane as the fuel. High resolution transmission electron microscopy (HRTEM) analysis indicates for the first time that SDC layer can effectively prevent the formation or growth of nickel carbide (onset of coking), accounting for the excellent performance and structural stability of the Ni-based cermet anode. (C) 2014 Elsevier Ltd. All rights reserved. C1 [Chen, Yu; Zhang, Yanxiang; Lin, Ye; Chen, Fanglin] Univ S Carolina, Dept Mech Engn, Columbia, SC 29208 USA. [Zhang, Yanxiang] Harbin Inst Technol, Sch Mat Sci & Engn, Harbin 150001, Peoples R China. [Yang, Zhibin; Han, Minfang] China Univ Min & Technol, Sch Chem & Environm Engn, Beijing 100083, Peoples R China. [Su, Dong] Brookhaven Natl Lab, Ctr Funct Nanomat, Upton, NY 11973 USA. [Han, Minfang] Tsinghua Univ, Dept Thermal Engn, Beijing 100084, Peoples R China. RP Han, MF (reprint author), China Univ Min & Technol, Sch Chem & Environm Engn, Beijing 100083, Peoples R China. EM hanminfang@sina.com; chenfa@cec.sc.edu RI 杨, 志宾/B-2311-2015; Chen, Fanglin/K-1039-2012; Liu, Tong/N-7904-2013; OI 杨, 志宾/0000-0003-3845-1133; Chen, Fanglin/0000-0001-9942-8872; Liu, Tong/0000-0001-5311-9687; Lin, Ye/0000-0003-4289-894X FU U.S. National Science Foundation [DMR-1210792]; 973 Project [2012CB215404]; National Natural Science Foundation of China [51261120378]; U.S. Department of Energy, Office of Basic Energy Sciences [DE-AC02-98CH10886] FX We are grateful for the financial support from the U.S. National Science Foundation (DMR-1210792), the 973 Project (2012CB215404) and the National Natural Science Foundation of China (51261120378). Electron microscopy research has been carried out at the Center for Functional Nanomaterials, Brookhaven National Laboratory, which is supported by the U.S. Department of Energy, Office of Basic Energy Sciences, under Contract no. DE-AC02-98CH10886. NR 55 TC 26 Z9 26 U1 11 U2 184 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 2211-2855 EI 2211-3282 J9 NANO ENERGY JI Nano Energy PD NOV PY 2014 VL 10 BP 1 EP 9 DI 10.1016/j.nanoen.2014.08.016 PG 9 WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AW0ML UT WOS:000345986500001 ER PT J AU Yang, JC He, Q Zhu, YM Lin, JC Liu, HJ Hsieh, YH Wu, PC Chen, YL Lee, SF Chin, YY Lin, HJ Chen, CT Zhan, Q Arenholz, E Chu, YH AF Yang, Jan-Chi He, Qing Zhu, Yuan-Min Lin, Jheng-Cyuan Liu, Heng-Jui Hsieh, Ying-Hui Wu, Ping-Chun Chen, Yen-Lin Lee, Shang-Fan Chin, Yi-Ying Lin, Hong-Ji Chen, Chien-Te Zhan, Qian Arenholz, Elke Chu, Ying-Hao TI Magnetic Mesocrystal-Assisted Magnetoresistance in Manganite SO NANO LETTERS LA English DT Article DE mesocrystal; self-assembled; nanocomposite; colossal magnetoresistance; complex oxide; nanocrystal ID LOW-FIELD MAGNETORESISTANCE; GRAIN-BOUNDARIES; FILMS; NANORODS; CRYSTALLIZATION; NANOSTRUCTURES; EVOLUTION; STRATEGY; GROWTH; OXIDE AB Mesocrystal, a new class of crystals as compared to conventional and well-known single crystals and polycrystalline systems, has captured significant attention in the past decade. Recent studies have been focused on the advance of synthesis mechanisms as well as the potential on device applications. In order to create further opportunities upon functional mesocrystals, we fabricated a self-assembled nanocomposite composed of magnetic CoFe2O4 mesocrystal in Sr-doped manganites. This combination exhibits intriguing structural and magnetic tunabilities. Furthermore, the antiferromagnetic coupling of the mesocrystal and matrix has induced an additional magnetic perturbation to spin-polarized electrons, resulting in a significantly enhanced magnetoresistance in the nanocomposite. Our work demonstrates a new thought toward the enhancement of intrinsic functionalities assisted by mesocrystals and advanced design of novel mesocrystal-embedded nanocomposites. C1 [Yang, Jan-Chi; Lin, Jheng-Cyuan; Liu, Heng-Jui; Hsieh, Ying-Hui; Wu, Ping-Chun; Chu, Ying-Hao] Natl Chiao Tung Univ, Dept Mat Sci & Engn, Hsinchu 300, Taiwan. [He, Qing] Univ Durham, Dept Phys, Durham DH1 3LE, England. [Zhu, Yuan-Min; Zhan, Qian] Univ Sci & Technol Beijing, Sch Mat Sci & Engn, Beijing 100083, Peoples R China. [Chen, Yen-Lin; Lee, Shang-Fan; Chu, Ying-Hao] Acad Sinica, Inst Phys, Taipei 155, Taiwan. [Chin, Yi-Ying; Lin, Hong-Ji; Chen, Chien-Te] Natl Synchrotron Radiat Res Ctr, Hsinchu 30076, Taiwan. [Arenholz, Elke] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94720 USA. [Chu, Ying-Hao] Natl Chiao Tung Univ, Dept Electrophys, Hsinchu 300, Taiwan. RP He, Q (reprint author), Room 235,Rochester Bldg,Sci Site,South Rd, Durham DH1 3LE, England. EM qing.he@durham.ac.uk; yhc@nctu.edu.tw RI He, Qing/E-3202-2010; Ying-Hao, Chu/A-4204-2008 OI Ying-Hao, Chu/0000-0002-3435-9084 FU Ministry of Science and Technology, R.O.C. [MOST 103-2119-M-009-003-MY3]; Center for Interdisciplinary Science of National Chiao Tung University, Ministry of Education, Taiwan [MOE-ATU 101W961]; National Natural Science Foundation of China [50971015, 51371031] FX Our work is supported by Ministry of Science and Technology, R.O.C. (MOST 103-2119-M-009-003-MY3), Center for Interdisciplinary Science of National Chiao Tung University, Ministry of Education, Taiwan (MOE-ATU 101W961), and National Natural Science Foundation of China with Grant Nos. 50971015 and 51371031. NR 29 TC 13 Z9 13 U1 7 U2 75 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1530-6984 EI 1530-6992 J9 NANO LETT JI Nano Lett. PD NOV PY 2014 VL 14 IS 11 BP 6073 EP 6079 DI 10.1021/n15019172 PG 7 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied; Physics, Condensed Matter SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AU6PE UT WOS:000345723800007 PM 25313666 ER PT J AU Yoo, J Dayeh, SA Bartelt, NC Tang, W Findikoglu, AT Picraux, ST AF Yoo, Jinkyoung Dayeh, Shadi A. Bartelt, Norman C. Tang, Wei Findikoglu, Alp T. Picraux, S. Tom TI Size-Dependent Silicon Epitaxy at Mesoscale Dimensions SO NANO LETTERS LA English DT Article DE Epitaxy; Nanowires; Mesoscale; Silicon; Chemical Vapor Deposition ID CHEMICAL-VAPOR-DEPOSITION; FIELD-EFFECT TRANSISTORS; MOLECULAR-BEAM EPITAXY; NANOWIRE GROWTH; SURFACE-REACTIONS; KINETICS; SILANE AB New discoveries on collective processes in materials fabrication and performance are emerging in the mesoscopic size regime between the nanoscale, where atomistic effects dominate, and the macroscale, where bulk-like behavior rules. For semiconductor electronics and photonics, dimensional control of the architecture in this regime is the limiting factor for device performance. Epitaxial crystal growth is the major tool enabling simultaneous control of the dimensions and properties of such architectures. Although size-dependent effects have been studied for many small-scale systems, they have not been reported for the epitaxial growth of Si crystalline surfaces. Here, we show a strong dependence of epitaxial growth rates on size for nano to microscale radial wires and planar stripes. A model for this unexpected size-dependent vapor phase epitaxy behavior at small dimensions suggests that these effects are universal and result from an enhanced surface desorption of the silane (SiH4) growth precursor near facet edges. Introducing phosphorus or boron dopants during the silicon epitaxy further decreases the growth rates and, for phosphorus, gives rise to a critical layer thickness for single crystalline epitaxial growth. This previously unknown mesoscopic size-dependent growth effect at mesoscopic dimensions points to a new mechanism in vapor phase growth and promises greater control of advanced device geometries. C1 [Yoo, Jinkyoung; Picraux, S. Tom] Los Alamos Natl Lab, Ctr Integrated Nanotechnol, Los Alamos, NM 87545 USA. [Dayeh, Shadi A.] Univ Calif San Diego, Dept Elect & Comp Engn, La Jolla, CA 92093 USA. [Bartelt, Norman C.] Sandia Natl Labs, Livermore, CA 94550 USA. [Tang, Wei] Univ Calif Los Angeles, Dept Mat Sci & Engn, Los Angeles, CA 90095 USA. [Findikoglu, Alp T.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA. RP Yoo, J (reprint author), Los Alamos Natl Lab, Ctr Integrated Nanotechnol, POB 1663, Los Alamos, NM 87545 USA. EM jyoo@lanl.gov; picraux@lanl.gov RI Yoo, Jinkyoung/B-5291-2008; Tang, Wei/A-6917-2015 OI Yoo, Jinkyoung/0000-0002-9578-6979; Tang, Wei/0000-0001-6113-7201 FU U.S. Department of Energy, Office of Basic Energy Sciences User Facility at Los Alamos National Laboratory [DE-AC52-06NA25396]; Sandia National Laboratories [DE-AC04-94AL85000]; Laboratory Directed Research and Development Program at LANL; DOE Office of Energy Efficiency and Renewable Energy, Solar Energy Program [EB2101010]; UC San Diego FX This work was performed in part at CINT, a U.S. Department of Energy, Office of Basic Energy Sciences User Facility at Los Alamos National Laboratory (Contract DE-AC52-06NA25396) and Sandia National Laboratories (Contract DE-AC04-94AL85000), and funded in part by the Laboratory Directed Research and Development Program at LANL and the DOE Office of Energy Efficiency and Renewable Energy, Solar Energy Program (EB2101010), and a faculty start-up fund for S.A.D. at UC San Diego. We thank Chris Sheehan and Yung-Chen Lin for high-resolution scanning electron microscopy and sample preparation for cross-sectional transmission electron microscopy and Brian Swartzentruber for helpful discussions. NR 29 TC 2 Z9 2 U1 2 U2 30 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1530-6984 EI 1530-6992 J9 NANO LETT JI Nano Lett. PD NOV PY 2014 VL 14 IS 11 BP 6121 EP 6126 DI 10.1021/n1502085z PG 6 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied; Physics, Condensed Matter SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AU6PE UT WOS:000345723800015 PM 25315228 ER PT J AU Klinkova, A Therien-Aubin, H Ahmed, A Nykypanchuk, D Choueiri, RM Gagnon, B Muntyanu, A Gale, O Walker, GC Kumacheva, E AF Klinkova, Anna Therien-Aubin, Heloise Ahmed, Aftab Nykypanchuk, Dmytro Choueiri, Rachelle M. Gagnon, Brandon Muntyanu, Anastasiya Gale, Oleg Walker, Gilbert C. Kumacheva, Eugenia TI Structural and Optical Properties of Self-Assembled Chains of Plasmonic Nanocubes SO NANO LETTERS LA English DT Article DE Nanoparticle; nanocube; nanosphere; self-assembly; nanoparticle chain; SERS; plasmonics ID ENHANCED RAMAN-SCATTERING; GOLD NANORODS; INORGANIC NANOPARTICLES; METAL NANOPARTICLES; HOT-SPOTS; POLYMERIZATION; GENERATION; NANOWIRES; POLYMERS; ANALOGS AB Solution-based linear self-assembly of metal nanoparticles offers a powerful strategy for creating plasmonic polymers, which, so far, have been formed from spherical nanoparticles and cylindrical nanorods. Here we report linear solution-based self-assembly of metal nanocubes (NCs), examine the structural characteristics of the NC chains, and demonstrate their advanced optical characteristics. In comparison with chains of nanospheres with similar dimensions, composition, and surface chemistry, predominant face-to-face assembly of large NCs coated with short polymer ligands led to a larger volume of hot spots in the chains, a nearly uniform E-field enhancement in the gaps between colinear NCs, and a new coupling mode for NC chains due to the formation of a FabryPerot resonator structure formed by face-to-face bonded NCs. The NC chains exhibited stronger surface-enhanced Raman scattering in comparison with linear assemblies of nanospheres. The experimental results were in agreement with finite difference time domain simulations. C1 [Klinkova, Anna; Therien-Aubin, Heloise; Choueiri, Rachelle M.; Gagnon, Brandon; Muntyanu, Anastasiya; Walker, Gilbert C.; Kumacheva, Eugenia] Univ Toronto, Dept Chem, Toronto, ON M5S 3H6, Canada. [Ahmed, Aftab] Argonne Natl Lab, Ctr Nanoscale Mat, Argonne, IL 60439 USA. [Nykypanchuk, Dmytro; Gale, Oleg] Brookhaven Natl Lab, Ctr Funct Nanomat, Upton, NY 11973 USA. RP Kumacheva, E (reprint author), Univ Toronto, Dept Chem, 80 St George St, Toronto, ON M5S 3H6, Canada. EM ekumache@chem.utoronto.ca RI Therien-Aubin, Heloise/O-9906-2016; OI Therien-Aubin, Heloise/0000-0003-4567-516X; Walker, Gilbert/0000-0002-5248-5498 FU NSERC Canada; NSERC; U.S. Department of Energy, Office of Basic Energy Sciences [DE-AC02-06CH11357, DE-AC02-98CH10886] FX A.K, R.M.C., and A.M. thank I. Gourevich and Dr. N. Coombs (Centre for Nanostructure Imaging at Department of Chemistry, University of Toronto) for their help with TEM imaging. E.K., A.K., H. T.-A., R.M.C, and A.M. thank Engage Grant and Discovery Grant (NSERC Canada) for financial support of this work. G.W. and B.G. acknowledge financial support from NSERC. A.M. thanks University of Toronto Undergraduate Research Fund. A.K. acknowledges Ontario Trillium Scholarship. A.A. acknowledges Center for Nanoscale Materials at Argonne National Laboratory for using the computing facility. Use of the Center for Nanoscale Materials at Argonne National Laboratory was supported by the U.S. Department of Energy, Office of Basic Energy Sciences, under Contract No. DE-AC02-06CH11357. Research in part was carried out at the Center for Functional Nanomaterials, Brookhaven National Laboratory, which was supported by the U.S. Department of Energy, Office of Basic Energy Sciences, under Contract No. DE-AC02-98CH10886. NR 32 TC 22 Z9 22 U1 14 U2 150 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1530-6984 EI 1530-6992 J9 NANO LETT JI Nano Lett. PD NOV PY 2014 VL 14 IS 11 BP 6314 EP 6321 DI 10.1021/nl502746h PG 8 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied; Physics, Condensed Matter SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AU6PE UT WOS:000345723800045 PM 25275879 ER PT J AU Song, JX Yu, ZX Gordin, ML Hu, S Yi, R Tang, DH Walter, T Regula, M Choi, D Li, XL Maniyannan, A Wang, DH AF Song, Jiangxuan Yu, Zhaoxin Gordin, Mikhail L. Hu, Shi Yi, Ran Tang, Duihai Walter, Timothy Regula, Michael Choi, Daiwon Li, Xiaolin Maniyannan, Ayyakkannu Wang, Donghai TI Chemically Bonded Phosphorus/Graphene Hybrid as a High Performance Anode for Sodium-Ion Batteries SO NANO LETTERS LA English DT Article DE Phosphorus; graphene nanosheets; chemical bonding sodium-ion battery; solid electrolyte interphase (sei) ID RECHARGEABLE LITHIUM BATTERIES; ENERGY-STORAGE; HIGH-CAPACITY; REVERSIBLE CAPACITY; LOW-COST; GRAPHENE; COMPOSITE; NANOPARTICLES; STABILITY; CHALLENGES AB Room temperature sodium-ion batteries are of great interest for high-energy-density energy storage systems because of low-cost and natural abundance of sodium. Here, we report a novel phosphorus/graphene nanosheet hybrid as a high performance anode for sodium-ion batteries through facile ball milling of red phosphorus and graphene stacks. The graphene stacks are mechanically exfoliated to nanosheets that chemically bond with the surfaces of phosphorus particles. This chemical bonding can facilitate robust and intimate contact between phosphorus and graphene nanosheets, and the graphene at the particle surfaces can help maintain electrical contact and stabilize the solid electrolyte interphase upon the large volume change of phosphorus during cycling. As a result, the phosphorus/graphene nanosheet hybrid nanostructured anode delivers a high reversible capacity of 2077 mAh/g with excellent cycling stability (1700 mAh/g after 60 cycles) and high Coulombic efficiency (>98%). This simple synthesis approach and unique nanostructure can potentially be applied to other phosphorus-based alloy anode materials for sodium-ion batteries. C1 [Song, Jiangxuan; Yu, Zhaoxin; Gordin, Mikhail L.; Hu, Shi; Yi, Ran; Tang, Duihai; Walter, Timothy; Regula, Michael; Wang, Donghai] Penn State Univ, Dept Mech & Nucl Engn, University Pk, PA 16802 USA. [Choi, Daiwon; Li, Xiaolin] Pacific NW Natl Lab, Dept Stationary Energy Storage, Richland, WA 99354 USA. [Maniyannan, Ayyakkannu] US DOE, Mat Performance Div, Natl Energy Technol Lab, Morgantown, WV 26507 USA. RP Wang, DH (reprint author), Penn State Univ, Dept Mech & Nucl Engn, University Pk, PA 16802 USA. EM dwang@psu.edu RI Choi, Daiwon/B-6593-2008; Song, Jiangxuan/G-8536-2015; Wang, Donghai/L-1150-2013 OI Wang, Donghai/0000-0001-7261-8510 FU U.S. Department of Energy's (DOE's) Office of Electricity Delivery & Energy Reliability (OE) [57558] FX The authors would like to acknowledge financial support from the U.S. Department of Energy's (DOE's) Office of Electricity Delivery & Energy Reliability (OE) (under Contract No. 57558). We also are grateful for enlightening discussions with Dr. Imre Gyuk of the DOE-OE Grid Storage Program. NR 51 TC 104 Z9 107 U1 65 U2 387 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1530-6984 EI 1530-6992 J9 NANO LETT JI Nano Lett. PD NOV PY 2014 VL 14 IS 11 BP 6329 EP 6335 DI 10.1021/nl502759z PG 7 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied; Physics, Condensed Matter SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AU6PE UT WOS:000345723800047 PM 25354313 ER PT J AU Kang, YJ Snyder, J Chi, MF Li, DG More, KL Markovic, NM Stamenkovic, VR AF Kang, Yijin Snyder, Joshua Chi, Miaofang Li, Dongguo More, Karren L. Markovic, Nenad M. Stamenkovic, Vojislav R. TI Multimetallic Core/Interlayer/Shell Nanostructures as Advanced Electrocatalysts SO NANO LETTERS LA English DT Article DE Core-shell; oxygen reduction reaction; electrocatalysis; nanoparticle; durability; activity ID SHAPE-CONTROLLED SYNTHESIS; OXYGEN REDUCTION REACTION; MEMBRANE FUEL-CELLS; METAL NANOCRYSTALS; PLATINUM NANOCRYSTALS; ELECTRONIC-STRUCTURE; BIMETALLIC SURFACES; ALLOY SURFACES; PT-SKIN; NANOPARTICLES AB The fine balance between activity and durability is crucial for the development of high performance electrocatalysts. The importance of atomic structure and compositional gradients is a guiding principle in exploiting the knowledge from well-defined materials in the design of novel class of coreshell electrocatalysts comprising Ni core, Au interlayer, and PtNi shell (Ni@Au@PtNi). This multimetallic system is found to have the optimal balance of activity and durability due to the synergy between the stabilizing effect of subsurface Au and modified electronic structure of surface Pt through interaction with subsurface Ni atoms. The electrocatalysts with Ni@Au@PtNi core-interlayer-shell structure exhibit high intrinsic and mass activities as well as superior durability for the oxygen reduction reaction with less than 10% activity loss after 10 000 potential cycles between 0.6 and 1.1 V vs the reversible hydrogen electrode. C1 [Kang, Yijin; Snyder, Joshua; Li, Dongguo; Markovic, Nenad M.; Stamenkovic, Vojislav R.] Argonne Natl Lab, Div Mat Sci, Argonne, IL 60439 USA. [Chi, Miaofang; More, Karren L.] Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA. RP Stamenkovic, VR (reprint author), Argonne Natl Lab, Div Mat Sci, 9700 S Cass Ave, Argonne, IL 60439 USA. EM vrstamenkovic@anl.gov RI Chi, Miaofang/Q-2489-2015; More, Karren/A-8097-2016; Li, Dongguo/O-6253-2016 OI Chi, Miaofang/0000-0003-0764-1567; More, Karren/0000-0001-5223-9097; Li, Dongguo/0000-0001-7578-7811 FU U.S. Department of Energy, the Office of Energy Efficiency and Renewable Energy, Fuel Cell Technologies [DE-AC02-06CH11357]; Scientific User Facilities Division, Office of Basic Energy Sciences, U.S. Department of Energy FX The research performed at Argonne National Laboratory (MSD, EMC, and CNM), which is a U.S. Department of Energy Office of Science Laboratory operated by UChicago Argonne, LLC under Contract No. DE-AC02-06CH11357, was supported by U.S. Department of Energy, the Office of Energy Efficiency and Renewable Energy, Fuel Cell Technologies. Part of the microscopy was performed at the Center for Nanophase Materials Sciences, which is sponsored at ORNL by the Scientific User Facilities Division, Office of Basic Energy Sciences, U.S. Department of Energy. NR 50 TC 41 Z9 42 U1 19 U2 211 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1530-6984 EI 1530-6992 J9 NANO LETT JI Nano Lett. PD NOV PY 2014 VL 14 IS 11 BP 6361 EP 6367 DI 10.1021/nl5028205 PG 7 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied; Physics, Condensed Matter SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AU6PE UT WOS:000345723800052 PM 25299322 ER PT J AU Liang, LB Wang, J Lin, WZ Sumpter, BG Meunier, V Pan, MH AF Liang, Liangbo Wang, Jun Lin, Wenzhi Sumpter, Bobby G. Meunier, Vincent Pan, Minghu TI Electronic Bandgap and Edge Reconstruction in Phosphorene Materials SO NANO LETTERS LA English DT Article DE Phosphorene; scanning tunneling microscopy/spectroscopy; direct bandgap monatomic step-edges; density functional theory; self-passivation ID BLACK PHOSPHORUS; GRAPHENE NANORIBBONS; SINGLE-CRYSTALS; MOS2; PHOTOLUMINESCENCE; RIBBONS; STATES; 1ST-PRINCIPLES; SPECTROSCOPY; TRANSISTORS AB Single-layer black phosphorus (BP), or phosphorene, is a highly anisotropic two-dimensional elemental material possessing promising semiconductor properties for flexible electronics. However, the direct bandgap of single-layer black phosphorus predicted theoretically has not been directly measured, and the properties of its edges have not been considered in detail. Here we report atomic scale electronic variation related to strain-induced anisotropic deformation of the puckered honeycomb structure of freshly cleaved black phosphorus using a high-resolution scanning tunneling spectroscopy (STS) survey along the light (x) and heavy (y) effective mass directions. Through a combination of STS measurements and first-principles calculations, a model for edge reconstruction is also determined. The reconstruction is shown to self-passivate most dangling bonds by switching the coordination number of phosphorus from 3 to 5 or 3 to 4. C1 [Liang, Liangbo; Meunier, Vincent] Rensselaer Polytech Inst, Dept Phys Appl Phys & Astron, Troy, NY 12180 USA. [Wang, Jun; Lin, Wenzhi; Sumpter, Bobby G.; Pan, Minghu] Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA. [Sumpter, Bobby G.] Oak Ridge Natl Lab, Comp Sci & Math Div, Oak Ridge, TN 37831 USA. [Pan, Minghu] Huazhong Univ Sci & Technol, Sch Phys, Wuhan 430074, Hubei, Peoples R China. RP Pan, MH (reprint author), Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA. EM meuniv@rpi.edu; mhupan@gmail.com RI Wang, Jun/N-6882-2014; Liang, Liangbo/H-4486-2011; Meunier, Vincent/F-9391-2010; Sumpter, Bobby/C-9459-2013 OI Wang, Jun/0000-0003-4974-1240; Liang, Liangbo/0000-0003-1199-0049; Meunier, Vincent/0000-0002-7013-179X; Sumpter, Bobby/0000-0001-6341-0355 FU Scientific User Facilities Division, Office of Basic Energy Sciences, U.S. Department of Energy; New York State under NYSTAR program [C080117]; Office of Naval Research FX Part of this research was conducted at the Center for Nanophase Materials Sciences (J.W., B.G.S., M.P.), which is sponsored at Oak Ridge National Laboratory by the Scientific User Facilities Division, Office of Basic Energy Sciences, U.S. Department of Energy. The work at Rensselaer Polytechnic Institute (RPI) was supported by New York State under NYSTAR program C080117 and the Office of Naval Research. The computations were performed using the resources of the Center for Computational Innovation at RPI. NR 44 TC 106 Z9 106 U1 36 U2 283 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1530-6984 EI 1530-6992 J9 NANO LETT JI Nano Lett. PD NOV PY 2014 VL 14 IS 11 BP 6400 EP 6406 DI 10.1021/nl502892t PG 7 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied; Physics, Condensed Matter SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AU6PE UT WOS:000345723800058 PM 25343376 ER PT J AU Zhang, LM Liu, KH Wong, AB Kim, J Hong, XP Liu, C Cao, T Louie, SG Wang, F Yang, PD AF Zhang, Liming Liu, Kaihui Wong, Andrew Barnabas Kim, Jonghwan Hong, Xiaoping Liu, Chong Cao, Ting Louie, Steven G. Wang, Feng Yang, Peidong TI Three-Dimensional Spirals of Atomic Layered MoS2 SO NANO LETTERS LA English DT Article DE Molybdenum disulfide (MoS2); spirals; symmetry breaking; chemical vapor deposition; screw dislocation ID MONOLAYER MOLYBDENUM-DISULFIDE; VALLEY POLARIZATION; ESHELBY TWIST; GRAPHENE; GROWTH; DRIVEN; PHASE AB Atomically thin two-dimensional (2D) layered materials, including graphene, boron nitride, and transition metal dichalcogenides (TMDs), can exhibit novel phenomena distinct from their bulk counterparts and hold great promise for novel electronic and optoelectronic applications. Controlled growth of such 2D materials with different thickness, composition, and symmetry are of central importance to realize their potential. In particular, the ability to control the symmetry of TMD layers is highly desirable because breaking the inversion symmetry can lead to intriguing valley physics, nonlinear optical properties, and piezoelectric responses. Here we report the first chemical vapor deposition (CVD) growth of spirals of layered MoS2 with atomically thin helical periodicity, which exhibits a chiral structure and breaks the three-dimensional (3D) inversion symmetry explicitly. The spirals composed of tens of connected MoS2 layers with decreasing areas: each basal plane has a triangular shape and shrinks gradually to the summit when spiraling up. All the layers in the spiral assume an AA lattice stacking, which is in contrast to the centrosymmetric AB stacking in natural MoS2 crystals. We show that the noncentrosymmetric MoS2 spiral leads to a strong bulk second-order optical nonlinearity. In addition, we found that the growth of spirals involves a dislocation mechanism, which can be generally applicable to other 2D TMD materials. C1 [Zhang, Liming; Wong, Andrew Barnabas; Liu, Chong; Yang, Peidong] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA. [Liu, Kaihui; Kim, Jonghwan; Hong, Xiaoping; Cao, Ting; Louie, Steven G.; Wang, Feng] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA. [Liu, Kaihui] Peking Univ, State Key Lab Mesoscop Phys, Beijing 100871, Peoples R China. [Liu, Kaihui] Peking Univ, Collaborat Innovat Ctr Quantum Matter, Beijing 100871, Peoples R China. [Wong, Andrew Barnabas; Liu, Chong; Louie, Steven G.; Wang, Feng; Yang, Peidong] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA. [Wang, Feng; Yang, Peidong] Univ Calif Berkeley, Kavli Energy NanoSci Inst, Berkeley, CA 94720 USA. [Wang, Feng; Yang, Peidong] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA. [Yang, Peidong] Univ Calif Berkeley, Dept Mat Sci & Engn, Berkeley, CA 94720 USA. RP Wang, F (reprint author), Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA. EM fengwang76@berkeley.edu; p_yang@berkeley.edu RI Hong, Xiaoping/G-8673-2013; Liu, Kaihui/A-9938-2014; Foundry, Molecular/G-9968-2014; wang, Feng/I-5727-2015; OI Hong, Xiaoping/0000-0002-5864-4533; Liu, Chong/0000-0001-5546-3852 FU Office of Science, Office of Basic Energy Sciences, Materials Sciences and Engineering Division, of the U.S. Department of Energy [DE-AC02-05CH11231, DE-SC0003949]; National Program for Thousand Young Talents of China FX This work was supported by the Director, Office of Science, Office of Basic Energy Sciences, Materials Sciences and Engineering Division, of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231(P-Chem) and No. DE-SC0003949 (Early Career Award). We thank the Molecular Foundry and Lawrence Berkeley National Laboratory for use of their facilities. We would especially like to thank Professor William Nix at Stanford University for the help discussion on the formation mechanism of spirals. K.L. acknowledges support from National Program for Thousand Young Talents of China. NR 33 TC 35 Z9 35 U1 25 U2 229 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1530-6984 EI 1530-6992 J9 NANO LETT JI Nano Lett. PD NOV PY 2014 VL 14 IS 11 BP 6418 EP 6423 DI 10.1021/nl502961e PG 6 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied; Physics, Condensed Matter SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AU6PE UT WOS:000345723800061 PM 25343743 ER PT J AU Shcherbakov, MR Neshev, DN Hopkins, B Shorokhov, AS Staude, I Melik-Gaykazyan, EV Decker, M Ezhov, AA Miroshnichenko, AE Brener, I Fedyanin, AA Kivshar, YS AF Shcherbakov, Maxim R. Neshev, Dragomir N. Hopkins, Ben Shorokhov, Alexander S. Staude, Isabelle Melik-Gaykazyan, Elizaveta V. Decker, Manuel Ezhov, Alexander A. Miroshnichenko, Andrey E. Brener, Igal Fedyanin, Andrey A. Kivshar, Yuri S. TI Enhanced Third-Harmonic Generation in Silicon Nanoparticles Driven by Magnetic Response SO NANO LETTERS LA English DT Article DE nonlinear optics; third-harmonic generation; silicon nanoparticles; optical magnetism; multiple decomposition ID METAMATERIALS; RESONANCES; EMISSION; LIGHT AB We observe enhanced third-harmonic generation from silicon nanodisks exhibiting both electric and magnetic dipolar resonances. Experimental characterization of the nonlinear optical response through third-harmonic microscopy and spectroscopy reveals that the third-harmonic generation is significantly enhanced in the vicinity of the magnetic dipole resonances. The field localization at the magnetic resonance results in two orders of magnitude enhancement of the harmonic intensity with respect to unstructured bulk silicon with the conversion efficiency limited only by the two-photon absorption in the substrate. C1 [Shcherbakov, Maxim R.; Shorokhov, Alexander S.; Melik-Gaykazyan, Elizaveta V.; Ezhov, Alexander A.; Fedyanin, Andrey A.] Moscow MV Lomonosov State Univ, Fac Phys, Moscow 119991, Russia. [Neshev, Dragomir N.; Hopkins, Ben; Staude, Isabelle; Decker, Manuel; Miroshnichenko, Andrey E.; Kivshar, Yuri S.] Australian Natl Univ, Res Sch Phys & Engn, Nonlinear Phys Ctr, Canberra, ACT 0200, Australia. [Brener, Igal] Sandia Natl Labs, Ctr Integrated Nanotechnol, Albuquerque, NM 87185 USA. RP Shcherbakov, MR (reprint author), Moscow MV Lomonosov State Univ, Fac Phys, Moscow 119991, Russia. EM shcherbakov@nanolab.phys.msu.ru RI Hopkins, Ben/J-1498-2015; Shcherbakov, Maxim/D-7571-2012; Shorokhov, Alexander/H-5523-2015; Melik-Gaykazyan, Elizaveta/J-9073-2015; Staude, Isabelle/N-4270-2015; Neshev, Dragomir/A-3759-2008; Fedyanin, Andrey/G-1803-2010; Miroshnichenko, Andrey/C-2170-2016; OI Hopkins, Ben/0000-0002-4570-4269; Shcherbakov, Maxim/0000-0001-7198-5482; Melik-Gaykazyan, Elizaveta/0000-0001-7633-2376; Neshev, Dragomir/0000-0002-4508-8646; Fedyanin, Andrey/0000-0003-4708-6895; Miroshnichenko, Andrey/0000-0001-9607-6621; Decker, Manuel/0000-0002-9125-0851 FU Russian Science Foundation [14-12-01144]; Russian Foundation for Basic Research; U.S. Department of Energy's National Nuclear Security Administration [DE-AC04-94AL85000]; Australian Research Council FX The authors would like to thank L. Novotny and H. Giessen for useful comments and suggestions, as well as A. Fedotova for her assistance with the experiment automatization. The authors acknowledge the financial support from Russian Science Foundation (grant #14-12-01144) and Russian Foundation for Basic Research. This work was performed, in part, at the Center for Integrated Nanotechnologies, an Office of Science User Facility operated for the U.S. Department of Energy (DOE) Office of Science. Sandia National Laboratories is a multiprogram laboratory managed and operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the U.S. Department of Energy's National Nuclear Security Administration under contract DE-AC04-94AL85000. The authors also acknowledge a support from the Australian Research Council. NR 24 TC 88 Z9 88 U1 6 U2 46 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1530-6984 EI 1530-6992 J9 NANO LETT JI Nano Lett. PD NOV PY 2014 VL 14 IS 11 BP 6488 EP 6492 DI 10.1021/nl503029j PG 5 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied; Physics, Condensed Matter SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AU6PE UT WOS:000345723800072 PM 25322350 ER PT J AU Shirato, N Cummings, M Kersell, H Li, Y Stripe, B Rosenmann, D Hla, SW Rose, V AF Shirato, Nozomi Cummings, Marvin Kersell, Heath Li, Yang Stripe, Benjamin Rosenmann, Daniel Hla, Saw-Wai Rose, Volker TI Elemental Fingerprinting of Materials with Sensitivity at the Atomic Limit SO NANO LETTERS LA English DT Article DE X-ray microscopy; chemical imaging; scanning tunneling microscopy; smart tips; synchrotron ID SCANNING-TUNNELING-MICROSCOPY; X-RAY MICROSCOPY; SYNCHROTRON-RADIATION; RESOLUTION; MICROBEAM; INSULATOR; TIP; STM AB By using synchrotron X-rays as a probe and a nanofabricated smart tip of a tunneling microscope as a detector, we have achieved chemical fingerprinting of individual nickel clusters on a Cu(111) surface at 2 nm lateral resolution, and at the ultimate single-atomic height sensitivity. Moreover, by varying the photon energy, we have succeeded to locally measure photoionization cross sections of just a single Ni nanocluster, which opens new exciting opportunities for chemical imaging of nanoscale materials. C1 [Shirato, Nozomi; Cummings, Marvin; Stripe, Benjamin; Rose, Volker] Argonne Natl Lab, Adv Photon Source, Argonne, IL 60439 USA. [Kersell, Heath; Li, Yang; Hla, Saw-Wai] Ohio Univ, Dept Phys & Astron, Nanoscale & Quantum Phenomena Inst, Athens, OH 45701 USA. [Rosenmann, Daniel; Hla, Saw-Wai; Rose, Volker] Argonne Natl Lab, Ctr Nanoscale Mat, Argonne, IL 60439 USA. RP Hla, SW (reprint author), Ohio Univ, Dept Phys & Astron, Nanoscale & Quantum Phenomena Inst, Athens, OH 45701 USA. EM shla@anl.gov; vrose@anl.gov RI Rose, Volker/B-1103-2008 OI Rose, Volker/0000-0002-9027-1052 FU Office of Science Early Career Research Program through the Division of Scientific User Facilities, Office of Basic Energy Sciences, U.S. Department of Energy [SC70705]; U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-AC02-06CH11357, DE-FG02-02ER46012] FX This work was funded by the Office of Science Early Career Research Program through the Division of Scientific User Facilities, Office of Basic Energy Sciences, U.S. Department of Energy, through Grant SC70705. Work at the Advanced Photon Source, the Center for Nanoscale Materials, and the Electron Microscopy Center was supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract DE-AC02-06CH11357. H.K. and Y.L acknowledge the support by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, Grant DE-FG02-02ER46012. The authors acknowledge engineering support by Curt Preissner and help with tip fabrication by Jon Hiller. The authors also thank the team of the CNM/APS nanoprobe for support at the beamline. NR 29 TC 11 Z9 11 U1 5 U2 45 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1530-6984 EI 1530-6992 J9 NANO LETT JI Nano Lett. PD NOV PY 2014 VL 14 IS 11 BP 6499 EP 6504 DI 10.1021/nl5030613 PG 6 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied; Physics, Condensed Matter SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AU6PE UT WOS:000345723800074 PM 25275823 ER PT J AU Zhu, JL Quan, ZW Lin, YS Jiang, YB Wang, ZW Zhang, JZ Jin, CQ Zhao, YS Liu, ZX Brinker, CJ Xu, HW AF Zhu, Jinlong Quan, Zewei Lin, Yu-Shen Jiang, Ying-Bing Wang, Zhongwu Zhang, Jianzhong Jin, Changqing Zhao, Yusheng Liu, Zhenxian Brinker, C. Jeffrey Xu, Hongwu TI Porous Ice Phases with VI and Distorted VII Structures Constrained in Nanoporous Silica SO NANO LETTERS LA English DT Article DE Nanoporous ice; high pressure; DAC; SAXS; WAXS ID CARBON NANOTUBES; UNDISSOCIATED SURFACE; CLATHRATE WATERS; HIGH-PRESSURE; MODEL; INTERFACE; HYDRATION; DIFFRACTION; DYNAMICS; STATE AB High-pressure compression of water contained in nanoporous silica allowed fabrication of novel porous ice phases as a function of pressure. The starting liquid nanoporous H2O transformed to ice VI and VII at 1.7 and 2.5 GPa, respectively, which are 0.6 and 0.4 GPa higher than commonly accepted pressures for bulk H2O. The continuous increase of pressure drives the formation of a tetragonally distorted VII structure with the space group I4mm, rather than a cubic Pn3m phase in bulk ice. The enhanced incompressibility of the tetragonal ice is related to the unique nanoporous configuration, and the distortion ratio c/a gradually increases with increasing pressure. The structural changes and enhanced thermodynamic stability may be interpreted by the two-dimensional distribution of silanol groups on the porous silica surfaces and the associated anisotropic interactions with H2O at the interfaces. C1 [Zhu, Jinlong; Jin, Changqing] Chinese Acad Sci, Inst Phys, Nat Lab Condensed Matter Phys, Beijing 100190, Peoples R China. [Zhu, Jinlong; Zhang, Jianzhong] Los Alamos Natl Lab, Los Alamos Neutron Scattering Ctr, Los Alamos, NM 87545 USA. [Zhu, Jinlong; Zhang, Jianzhong] Los Alamos Natl Lab, EES Div, Los Alamos, NM 87545 USA. [Lin, Yu-Shen; Brinker, C. Jeffrey] Univ New Mexico, Ctr MicroEngineered Mat, Albuquerque, NM 87131 USA. [Lin, Yu-Shen] Univ New Mexico, Dept Internal Med, Div Mol Med, Albuquerque, NM 87131 USA. [Jiang, Ying-Bing] Univ New Mexico, TEM Lab, Albuquerque, NM 87131 USA. [Wang, Zhongwu] Cornell Univ, Wilson Lab, Cornell High Energy Synchrotron Source, Ithaca, NY 14853 USA. [Zhao, Yusheng] Univ Nevada, Dept Phys & Astron, HiPSEC, Las Vegas, NV 89154 USA. [Liu, Zhenxian] Carnegie Inst Sci, Geophys Lab, Washington, DC 20015 USA. RP Zhu, JL (reprint author), Chinese Acad Sci, Inst Phys, Nat Lab Condensed Matter Phys, Beijing 100190, Peoples R China. EM jlzhu04@iphy.ac.cn; zquan@lanl.gov; hxu@lanl.gov RI Quan, Zewei/G-4759-2011; OI Xu, Hongwu/0000-0002-0793-6923; Zhang, Jianzhong/0000-0001-5508-1782 FU NSF; MOST of China; laboratory-directed research and development (LDRD) program of Los Alamos National Laboratory; DOE [DE-AC52-06NA25396]; U.S. Department of Energy's Office of Basic Energy Sciences; NSF [DMR-0936384]; COMPRES under NSF [EAR 11-57758]; DOE-NNSA (CDAC) [DE-FC-52-O8NA28554]; U.S. Department of Energy, Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division; Air Force Office of Scientific Research [FA9550-14-1-0066]; U.S. Department of Energy, Office of Science, Catalysis Science program [DE-FG02-02ER15368] FX We acknowledge the support from NSF & MOST of China through research projects at Institute of Physics, Chinese Academy of Sciences. This work is also supported by the laboratory-directed research and development (LDRD) program of Los Alamos National Laboratory, which is operated by Los Alamos National Security LLC under DOE Contract No. DE-AC52-06NA25396. The neutron experiment has benefited from the use of the Lujan Neutron Scattering Center at Los Alamos Neutron Science Center, which is funded by the U.S. Department of Energy's Office of Basic Energy Sciences. CHESS is supported by the NSF award DMR-0936384. U2A is supported by COMPRES under NSF Cooperative Agreement EAR 11-57758 and DOE-NNSA (DE-FC-52-O8NA28554, CDAC). Use of the NSLS was supported by the U.S. Department of Energy's Office of Basic Energy Sciences. C.J.B. acknowledges support from the U.S. Department of Energy, Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division. Y.-S.L. acknowledges support from the Air Force Office of Scientific Research under grant #FA9550-14-1-0066 and the U.S. Department of Energy, Office of Science, Catalysis Science program under grant DE-FG02-02ER15368. NR 31 TC 0 Z9 0 U1 9 U2 44 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1530-6984 EI 1530-6992 J9 NANO LETT JI Nano Lett. PD NOV PY 2014 VL 14 IS 11 BP 6554 EP 6558 DI 10.1021/nl503165n PG 5 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied; Physics, Condensed Matter SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AU6PE UT WOS:000345723800083 PM 25338300 ER PT J AU Zhao, H Wang, ZH Lu, P Jiang, M Shi, FF Song, XY Zheng, ZY Zhou, X Fu, YB Abdelbast, G Xiao, XC Liu, Z Battaglia, VS Zaghib, K Liu, G AF Zhao, Hui Wang, Zhihui Lu, Peng Jiang, Meng Shi, Feifei Song, Xianyun Zheng, Ziyan Zhou, Xin Fu, Yanbao Abdelbast, Guerfi Xiao, Xingcheng Liu, Zhi Battaglia, Vincent S. Zaghib, Karim Liu, Gao TI Toward Practical Application of Functional Conductive Polymer Binder for a High-Energy Lithium-Ion Battery Design SO NANO LETTERS LA English DT Article DE silicon monozide conductive polymer binder; stabilized lithium metal powder (SLMP); lithum ion battery ID ANODE MATERIAL; RECHARGEABLE BATTERIES; NEGATIVE ELECTRODE; SILICON; LI; CAPACITY; SI; PERFORMANCE; PRELITHIATION; CRYSTALLINE AB Silicon alloys have the highest specific capacity when used as anode material for lithium-ion batteries; however, the drastic volume change inherent in their use causes formidable challenges toward achieving stable cycling performance. Large quantities of binders and conductive additives are typically necessary to maintain good cell performance. In this report, only 2% (by weight) functional conductive polymer binder without any conductive additives was successfully used with a micron-size silicon monoxide (SiO) anode material, demonstrating stable and high gravimetric capacity (>1000 mAh/g) for similar to 500 cycles and more than 90% capacity retention. Prelithiation of this anode using stabilized lithium metal powder (SLMP) improves the first cycle Coulombic efficiency of a SiO/NMC full cell from similar to 48% to similar to 90%. The combination enables good capacity retention of more than 80% after 100 cycles at C/3 in a lithium-ion full cell. C1 [Zhao, Hui; Wang, Zhihui; Song, Xianyun; Zheng, Ziyan; Zhou, Xin; Fu, Yanbao; Battaglia, Vincent S.; Liu, Gao] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Environm Energy Technol Div, Berkeley, CA 94720 USA. [Shi, Feifei] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA. [Lu, Peng; Jiang, Meng; Xiao, Xingcheng] Gen Motors, Global Res & Dev Ctr, Warren, MI 48090 USA. [Zheng, Ziyan] Univ Calif Berkeley, Berkeley, CA 94720 USA. [Zhou, Xin] Univ Calif Los Angeles, Los Angeles, CA 90095 USA. [Abdelbast, Guerfi; Zaghib, Karim] Inst Rech Elect Hydroquebec IREQ, Montreal, PQ J3X 1S1, Canada. [Liu, Zhi] Chinese Acad Sci, Shanghai Inst Microsyst & Informat Technol, State Key Lab Funct Mat Informat, Shanghai 200050, Peoples R China. RP Liu, G (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Environm Energy Technol Div, Berkeley, CA 94720 USA. EM gliu@lbl.gov RI Liu, Zhi/B-3642-2009; Fu, Yanbao/F-9583-2011; Foundry, Molecular/G-9968-2014 OI Liu, Zhi/0000-0002-8973-6561; Fu, Yanbao/0000-0001-7752-680X; FU Vehicle Technologies Office of the U.S. Department of Energy (U.S. DOE) under the Batteries for Advanced Transportation Technologies (BATT) Program; National Center for Electron Microscopy, Lawrence Berkeley Lab; U.S. Department of Energy [DE-AC02-05 CH11231] FX This work was funded by the Assistant Secretary for Energy Efficiency, Vehicle Technologies Office of the U.S. Department of Energy (U.S. DOE) under the Batteries for Advanced Transportation Technologies (BATT) Program. The authors acknowledge support of the National Center for Electron Microscopy, Lawrence Berkeley Lab, which is supported by the U.S. Department of Energy under Contract # DE-AC02-05 CH11231. G.L. thanks Robert R. Powell at General Motors for the helpful discussion and guidance. NR 40 TC 30 Z9 30 U1 34 U2 253 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1530-6984 EI 1530-6992 J9 NANO LETT JI Nano Lett. PD NOV PY 2014 VL 14 IS 11 BP 6704 EP 6710 DI 10.1021/nl503490h PG 7 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied; Physics, Condensed Matter SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AU6PE UT WOS:000345723800107 PM 25314674 ER PT J AU Sapi, A Liu, FD Cai, XJ Thompson, CM Wang, HL An, KJ Krier, JM Somorjai, GA AF Sapi, Andras Liu, Fudong Cai, Xiaojun Thompson, Christopher M. Wang, Hailiang An, Kwangjin Krier, James M. Somorjai, Gabor A. TI Comparing the Catalytic Oxidation of Ethanol at the Solid-Gas and Solid Liquid Interfaces over Size-Controlled Pt Nanoparticles: Striking Differences in Kinetics and Mechanism SO NANO LETTERS LA English DT Article DE Heterogeneous catalysis; ethanol oxidation; size control; platinum nanoparticles; sum frequency generation ID SELF-ASSEMBLED MONOLAYERS; PLATINUM NANOPARTICLES; STRUCTURE SENSITIVITY; PARTICLE-SIZE; SELECTIVITY; HYDROGENATION; MONODISPERSE; METHANOL; SILICA; OXYGEN AB Pt nanoparticles with controlled size (2, 4, and 6 nm) are synthesized and tested in ethanol oxidation by molecular oxygen at 60 degrees C to acetaldehyde and carbon dioxide both in the gas and liquid phases. The turnover frequency of the reaction is similar to 80 times faster, and the activation energy is similar to 5 times higher at the gas-solid interface compared to the liquid-solid interface. The catalytic activity is highly dependent on the size of the Pt nanoparticles; however, the selectivity is not size sensitive. Acetaldehyde is the main product in both media, while twice as much carbon dioxide was observed in the gas phase compared to the liquid phase. Added water boosts the reaction in the liquid phase; however, it acts as an inhibitor in the gas phase. The more water vapor was added, the more carbon dioxide was formed in the gas phase, while the selectivity was not affected by the concentration of the water in the liquid phase. The differences in the reaction kinetics of the solid-gas and solid-liquid interfaces can be attributed to the molecular orientation deviation of the ethanol molecules on the Pt surface in the gas and liquid phases as evidenced by sum frequency generation vibrational spectroscopy. C1 [Somorjai, Gabor A.] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA. Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA. Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA. RP Somorjai, GA (reprint author), Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA. EM somorjai@berkeley.edu RI Liu, Fudong/H-2050-2012; Cai, Xiaojun/C-1864-2015; Sapi, Andras/G-3527-2015 OI Cai, Xiaojun/0000-0002-3802-8389; Sapi, Andras/0000-0001-6557-0731 FU U.S. Department of Energy, Office of Science, Division of Chemical Sciences, Geological and Biosciences [DE-AC02-05CH11231] FX This work was supported by the U.S. Department of Energy, Office of Science, Division of Chemical Sciences, Geological and Biosciences under contract No. DE-AC02-05CH11231. NR 18 TC 5 Z9 5 U1 6 U2 78 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 1530-6984 EI 1530-6992 J9 NANO LETT JI Nano Lett. PD NOV PY 2014 VL 14 IS 11 BP 6727 EP 6730 DI 10.1021/nl5035545 PG 4 WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied; Physics, Condensed Matter SC Chemistry; Science & Technology - Other Topics; Materials Science; Physics GA AU6PE UT WOS:000345723800110 PM 25337984 ER PT J AU Chen, Z Wong, C Lubner, S Yee, S Miller, J Jang, W Hardin, C Fong, A Garay, JE Dames, C AF Chen, Zhen Wong, Carlaton Lubner, Sean Yee, Shannon Miller, John Jang, Wanyoung Hardin, Corey Fong, Anthony Garay, Javier E. Dames, Chris TI A photon thermal diode SO NATURE COMMUNICATIONS LA English DT Article ID HEAT-FLOW; RECTIFICATION; RECTIFIER; TRANSPORT AB A thermal diode is a two-terminal nonlinear device that rectifies energy carriers (for example, photons, phonons and electrons) in the thermal domain, the heat transfer analogue to the familiar electrical diode. Effective thermal rectifiers could have an impact on diverse applications ranging from heat engines to refrigeration, thermal regulation of buildings and thermal logic. However, experimental demonstrations have lagged far behind theoretical proposals. Here we present the first experimental results for a photon thermal diode. The device is based on asymmetric scattering of ballistic energy carriers by pyramidal reflectors. Recent theoretical work has predicted that this ballistic mechanism also requires a nonlinearity in order to yield asymmetric thermal transport, a requirement of all thermal diodes arising from the second Law of Thermodynamics, and realized here using an ' inelastic thermal collimator' element. Experiments confirm both effects: with pyramids and collimator the thermal rectification is 10.9 +/- 0.8%, while without the collimator no rectification is detectable ( < 0.3%). C1 [Chen, Zhen; Lubner, Sean; Yee, Shannon; Jang, Wanyoung; Dames, Chris] Univ Calif Berkeley, Dept Mech Engn, Berkeley, CA 94720 USA. [Wong, Carlaton; Miller, John; Hardin, Corey; Fong, Anthony; Garay, Javier E.] Univ Calif Riverside, Dept Mech Engn, Riverside, CA 92521 USA. [Dames, Chris] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA. RP Dames, C (reprint author), Univ Calif Berkeley, Dept Mech Engn, Berkeley, CA 94720 USA. EM cdames@berkeley.edu RI Chen, Zhen/M-2072-2015 OI Chen, Zhen/0000-0002-5422-8807 FU DARPA YFA [N66001-09-1-2098]; AFOSR MURI [FA9550-08-1-0407] FX This work was supported in part by a DARPA YFA (Grant No. N66001-09-1-2098) and an AFOSR MURI (Grant No. FA9550-08-1-0407). NR 27 TC 24 Z9 24 U1 4 U2 37 PU NATURE PUBLISHING GROUP PI LONDON PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND SN 2041-1723 J9 NAT COMMUN JI Nat. Commun. PD NOV PY 2014 VL 5 DI 10.1038/ncomms6446 PG 5 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AU9JR UT WOS:000345909000001 PM 25399761 ER PT J AU De Luca, GM Ghiringhelli, G Perroni, CA Cataudella, V Chiarella, F Cantoni, C Lupini, AR Brookes, NB Huijben, M Koster, G Rijnders, G Salluzzo, M AF De Luca, G. M. Ghiringhelli, G. Perroni, C. A. Cataudella, V. Chiarella, F. Cantoni, C. Lupini, A. R. Brookes, N. B. Huijben, M. Koster, G. Rijnders, G. Salluzzo, M. TI Ubiquitous long-range antiferromagnetic coupling across the interface between superconducting and ferromagnetic oxides SO NATURE COMMUNICATIONS LA English DT Article ID X-RAY-ABSORPTION; HETEROSTRUCTURES; MAGNETISM; STATES AB The so-called proximity effect is the manifestation, across an interface, of the systematic competition between magnetic order and superconductivity. This phenomenon has been well documented and understood for conventional superconductors coupled with metallic ferromagnets; however it is still less known for oxide materials, where much higher critical temperatures are offered by copper oxide-based superconductors. Here we show that, even in the absence of direct Cu-O-Mn covalent bonding, the interfacial CuO2 planes of superconducting La1.85Sr0.15CuO4 thin films develop weak ferromagnetism associated to the charge transfer of spin-polarised electrons from the La0.66Sr0.33MnO3 ferromagnet. Theoretical modelling confirms that this effect is general to all cuprate/manganite heterostructures and the presence of direct bonding only affects the strength of the coupling. The Dzyaloshinskii-Moriya interaction, also at the origin of the weak ferromagnetism of bulk cuprates, propagates the magnetisation from the interface CuO2 planes into the superconductor, eventually depressing its critical temperature. C1 [De Luca, G. M.; Perroni, C. A.; Cataudella, V.; Chiarella, F.; Salluzzo, M.] Univ Naples Federico II, CNR SPIN, I-80126 Naples, Italy. [De Luca, G. M.; Perroni, C. A.; Cataudella, V.; Chiarella, F.; Salluzzo, M.] Univ Naples Federico II, Dipartimento Fis, I-80126 Naples, Italy. [Ghiringhelli, G.] CNR SPIN, I-20133 Milan, Italy. [Ghiringhelli, G.] Politecn Milan, Dipartimento Fis, I-20133 Milan, Italy. [Cantoni, C.; Lupini, A. R.] Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA. [Brookes, N. B.] European Synchrotron Radiat Facil, F-38043 Grenoble, France. [Huijben, M.; Koster, G.; Rijnders, G.] Univ Twente, Fac Sci & Technol, NL-7500 AE Enschede, Netherlands. [Huijben, M.; Koster, G.; Rijnders, G.] Univ Twente, MESA Inst Nanotechnol, NL-7500 AE Enschede, Netherlands. RP De Luca, GM (reprint author), Univ Naples Federico II, CNR SPIN, Complesso Univ Monte St Angelo,Via Cinthia, I-80126 Naples, Italy. EM gabriella.deluca@spin.cnr.it; giacomo.ghiringhelli@polimi.it RI Cataudella, Vittorio /B-4164-2015; salluzzo, marco/C-5919-2009; Ghiringhelli, Giacomo/D-1159-2014; Chiarella, Fabio/G-2739-2015 OI Cataudella, Vittorio /0000-0002-1835-1429; salluzzo, marco/0000-0001-8372-6963; Ghiringhelli, Giacomo/0000-0003-0867-7748; Chiarella, Fabio/0000-0003-2537-5282 FU European Union [264098-MAMA]; Italian MIUR Grant [PRIN 20094W2LAY]; U.S. Department of Energy, Basic Energy Sciences, Materials Sciences and Engineering Division; ORNL's Center for Nanophase Materials Sciences (CNMS); Scientific User Facilities Division, Office of Basic Energy Sciences, Department of Energy FX G.M.D.L. research was funded by the European Union Seventh Framework Program under Grant Agreement No. 264098-MAMA, G.G., V.C., A.P., M.S. research was supported from the Italian MIUR Grant No. PRIN 20094W2LAY. C.C. and A.R.L. research was supported by the U.S. Department of Energy, Basic Energy Sciences, Materials Sciences and Engineering Division and through a user project by ORNL's Center for Nanophase Materials Sciences (CNMS), which is sponsored by the Scientific User Facilities Division, Office of Basic Energy Sciences, Department of Energy. NR 37 TC 8 Z9 8 U1 7 U2 75 PU NATURE PUBLISHING GROUP PI LONDON PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND SN 2041-1723 J9 NAT COMMUN JI Nat. Commun. PD NOV PY 2014 VL 5 AR 5626 DI 10.1038/ncomms6626 PG 7 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AW1XY UT WOS:000346083100003 PM 25418631 ER PT J AU Guo, JJ Lee, J Contescu, CI Gallego, NC Pantelides, ST Pennycook, SJ Moyer, BA Chisholm, MF AF Guo, Junjie Lee, Jaekwang Contescu, Cristian I. Gallego, Nidia C. Pantelides, Sokrates T. Pennycook, Stephen J. Moyer, Bruce A. Chisholm, Matthew F. TI Crown ethers in graphene SO NATURE COMMUNICATIONS LA English DT Article ID GRAPHITE OXIDE; 12-METALLACROWN-3 COMPLEXES; FUNCTIONALIZED GRAPHENE; TRANSPARENT CONDUCTORS; FILMS; BANDGAP; SHEETS; CARBON; LITHOGRAPHY; PERFORMANCE AB Crown ethers are at their most basic level rings constructed of oxygen atoms linked by two- or three-carbon chains. They have attracted attention for their ability to selectively incorporate various atoms or molecules within the cavity formed by the ring. However, crown ethers are typically highly flexible, frustrating efforts to rigidify them for many uses that demand higher binding affinity and selectivity. Here we present atomic-resolution images of the same basic structures of the original crown ethers embedded in graphene. This arrangement constrains the crown ethers to be rigid and planar. First-principles calculations show that the close similarity of the structures should also extend to their selectivity towards specific metal cations. Crown ethers in graphene offer a simple environment that can be systematically tested and modelled. Thus, we expect that our finding will introduce a new wave of investigations and applications of chemically functionalized graphene. C1 [Guo, Junjie; Lee, Jaekwang; Contescu, Cristian I.; Gallego, Nidia C.; Pantelides, Sokrates T.; Pennycook, Stephen J.; Chisholm, Matthew F.] Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA. [Guo, Junjie; Pennycook, Stephen J.; Chisholm, Matthew F.] Univ Tennessee, Dept Mat Sci & Engn, Knoxville, TN 37996 USA. [Lee, Jaekwang; Pantelides, Sokrates T.] Vanderbilt Univ, Dept Phys & Astron, Nashville, TN 37235 USA. [Moyer, Bruce A.] Oak Ridge Natl Lab, Div Chem Sci, Oak Ridge, TN 37831 USA. RP Chisholm, MF (reprint author), Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA. EM chisholmmf@ornl.gov RI guo, junjie/I-3189-2012; Moyer, Bruce/L-2744-2016; OI guo, junjie/0000-0002-3414-3734; Moyer, Bruce/0000-0001-7484-6277; Contescu, Cristian/0000-0002-7450-3722; Gallego, Nidia/0000-0002-8252-0194 FU U.S. Department of Energy Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division; Division of Chemical Sciences, Geosciences, and Biosciences; DOE [DE-FG02-09ER46554]; ORNL's Center for Nanophase Materials Sciences (CNMS); Scientific User Facilities Division, Office of Science, Basic Energy Sciences, U.S. Department of Energy; Office of Science of the U.S. DOE [DE-AC02-05CH11231] FX We are grateful to Dr Suk-kyun Ahn (ORNL) for his very helpful comments. This work was supported by the U.S. Department of Energy Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division (J.G., J.L., C.I.C., N.C.G., S.T.P., S.J.P. and M.F.C.) and Division of Chemical Sciences, Geosciences, and Biosciences (B.A.M.), by DOE grant DE-FG02-09ER46554 (S.T.P.), and through a user project supported by ORNL's Center for Nanophase Materials Sciences (CNMS), which is sponsored by the Scientific User Facilities Division, Office of Science, Basic Energy Sciences, U.S. Department of Energy. This research used resources of the National Energy Research Scientific Computing Center, which is supported by the Office of Science of the U.S. DOE (contract no. DE-AC02-05CH11231). NR 47 TC 13 Z9 13 U1 13 U2 98 PU NATURE PUBLISHING GROUP PI LONDON PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND SN 2041-1723 J9 NAT COMMUN JI Nat. Commun. PD NOV PY 2014 VL 5 AR 5389 DI 10.1038/ncomms6389 PG 6 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AU5CN UT WOS:000345624800010 PM 25391367 ER PT J AU Li, Q Lin, WZ Yan, JQ Chen, X Gianfrancesco, AG Singh, DJ Mandrus, D Kalinin, SV Pan, MH AF Li, Qing Lin, Wenzhi Yan, Jiaqiang Chen, Xin Gianfrancesco, Anthony G. Singh, David J. Mandrus, David Kalinin, Sergei V. Pan, Minghu TI Bond competition and phase evolution on the IrTe2 surface SO NATURE COMMUNICATIONS LA English DT Article ID TRANSITION; SPECTROSCOPY; MODEL AB Compounds with incommensurate structural modulations have been extensively studied in last several decades. However, the relationship between structurally incommensurate/commensurate phases and associated electronic states remains enigmatic. Here we report the coexisting of complex incommensurate structures and highly unusual electronic roughness on the surface of in situ cleaved IrTe2 by using scanning tunnelling microscopy/spectroscopy, corroborated with extensive density-functional theory calculations. This behaviour is traced to structural instability, which induces a structural transition from a trigonal to a triclinic lattice below transition temperature, giving rise to the formation of unidirectional structural modulations with distinct wavelengths, accompanied by the opening of a 'pseudo'-gap in the surface layer. With further cooling the surface adopts a structure that reflects an similar to 6 x periodicity that is different from the bulk 5 x periodicity. Calculations show that the structure distortion is not associated with a charge density wave, but is rather associated with Te p-electron bonding. C1 [Li, Qing; Lin, Wenzhi; Kalinin, Sergei V.; Pan, Minghu] Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA. [Li, Qing] Soochow Univ, Inst Funct Nano & Soft Mat FUNSOM, Suzhou 215123, Jiangsu, Peoples R China. [Li, Qing] Soochow Univ, Collaborat Innovat Ctr Suzhou Sci & Technol, Suzhou 215123, Jiangsu, Peoples R China. [Yan, Jiaqiang; Mandrus, David] Univ Tennessee, Dept Mat Sci & Engn, Knoxville, TN 37996 USA. [Yan, Jiaqiang; Chen, Xin; Singh, David J.; Mandrus, David] Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA. [Gianfrancesco, Anthony G.] Univ Tennessee, UT ORNL Bredesen Ctr, Knoxville, TN 37996 USA. [Pan, Minghu] Huazhong Univ Sci & Technol, Sch Phys, Wuhan 430074, Peoples R China. RP Pan, MH (reprint author), Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA. EM sergei2@ornl.gov; mhupan@gmail.com RI Kalinin, Sergei/I-9096-2012 OI Kalinin, Sergei/0000-0001-5354-6152 FU Oak Ridge National Laboratory; Scientific User Facilities Division, Office of Basic Energy Sciences, US Department of Energy; US Department of Energy, Basic Energy Sciences, Materials Sciences and Engineering Division; UT/ORNL Bredesen Center for Interdisciplinary Research and Graduate Education FX This research was conducted (M.P. and Q.L.) at the Center for Nanophase Materials Sciences, which is sponsored at Oak Ridge National Laboratory by the Scientific User Facilities Division, Office of Basic Energy Sciences, US Department of Energy. Research was supported (W.L., A.G.G., S.V.K., J.Y., X.C., D.J.S. and D.M.) by the US Department of Energy, Basic Energy Sciences, Materials Sciences and Engineering Division. Anthony Gianfrancesco acknowledges fellowship support from the UT/ORNL Bredesen Center for Interdisciplinary Research and Graduate Education. NR 30 TC 8 Z9 8 U1 8 U2 51 PU NATURE PUBLISHING GROUP PI LONDON PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND SN 2041-1723 J9 NAT COMMUN JI Nat. Commun. PD NOV PY 2014 VL 5 AR 5358 DI 10.1038/ncomms6358 PG 7 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AU6UR UT WOS:000345740100001 PM 25377130 ER PT J AU Nemsak, S Shavorskiy, A Karslioglu, O Zegkinoglou, I Rattanachata, A Conlon, CS Keqi, A Greene, PK Burks, EC Salmassi, F Gullikson, EM Yang, SH Liu, K Bluhm, H Fadley, CS AF Nemsak, Slavomir Shavorskiy, Andrey Karslioglu, Osman Zegkinoglou, Ioannis Rattanachata, Arunothai Conlon, Catherine S. Keqi, Armela Greene, Peter K. Burks, Edward C. Salmassi, Farhad Gullikson, Eric M. Yang, See-Hun Liu, Kai Bluhm, Hendrik Fadley, Charles S. TI Concentration and chemical-state profiles at heterogeneous interfaces with sub-nm accuracy from standing-wave ambient-pressure photoemission SO NATURE COMMUNICATIONS LA English DT Article ID RAY PHOTOELECTRON-SPECTROSCOPY; OXIDE ELECTROCHEMICAL-CELLS; AQUEOUS-SOLUTION INTERFACES; ELECTRON-SPECTROSCOPY; SURFACE; WATER; ADSORPTION; SIMULATION; HYDROSOLS; SPECTRA AB Heterogeneous processes at solid/gas, liquid/gas and solid/liquid interfaces are ubiquitous in modern devices and technologies but often difficult to study quantitatively. Full characterization requires measuring the depth profiles of chemical composition and state with enhanced sensitivity to narrow interfacial regions of a few to several nm in extent over those originating from the bulk phases on either side of the interface. We show for a model system of NaOH and CsOH in an similar to 1-nm thick hydrated layer on alpha-Fe2O3 (haematite) that combining ambient-pressure X-ray photoelectron spectroscopy and standing-wave photoemission spectroscopy provides the spatial arrangement of the bulk and interface chemical species, as well as local potential energy variations, along the direction perpendicular to the interface with sub-nm accuracy. Standing-wave ambient-pressure photoemission spectroscopy is thus a very promising technique for measuring such important interfaces, with relevance to energy research, heterogeneous catalysis, electrochemistry, and atmospheric and environmental science. C1 [Nemsak, Slavomir; Rattanachata, Arunothai; Conlon, Catherine S.; Keqi, Armela; Greene, Peter K.; Burks, Edward C.; Liu, Kai; Fadley, Charles S.] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA. [Nemsak, Slavomir; Conlon, Catherine S.; Keqi, Armela; Salmassi, Farhad; Gullikson, Eric M.; Fadley, Charles S.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA. [Shavorskiy, Andrey; Karslioglu, Osman; Zegkinoglou, Ioannis; Bluhm, Hendrik] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA. [Yang, See-Hun] IBM Corp, Almaden Res Ctr, San Jose, CA 95120 USA. RP Nemsak, S (reprint author), Forschungszentrum Julich, Peter Grunberg Inst 6, D-52425 Julich, Germany. EM s.nemsak@fz-juelich.de; hbluhm@lbl.gov; fadley@physics.ucdavis.edu RI Liu, Kai/B-1163-2008; Zegkinoglou, Ioannis/H-2343-2013 OI Liu, Kai/0000-0001-9413-6782; FU Office of Science, Office of Basic Energy Sciences, Division of Chemical Sciences, Geosciences, and Biosciences and Materials Sciences Division of the US Department of Energy at the Lawrence Berkeley National Laboratory [DE-AC02-05CH11231]; Julich Research Center, Peter Grunberg Institute [PGI-6]; French National Research Agency (ANR) [ANR-10-LABX-0039]; National Science Foundation [DMR-1008791] FX The Advanced Light Source and the Molecular Environmental Science beamline 11.0.2 are supported by the Director, Office of Science, Office of Basic Energy Sciences, Division of Chemical Sciences, Geosciences, and Biosciences and Materials Sciences Division of the US Department of Energy at the Lawrence Berkeley National Laboratory under Contract No. DE-AC02-05CH11231. C.S.F. and S.N. also acknowledge support from the Julich Research Center, Peter Grunberg Institute, PGI-6; and from the APTCOM Project of a grant from the 'Laboratoire d'Excellence Physics Atom Light Matter' (LabEx PALM) overseen by the French National Research Agency (ANR) as part of the 'Investissements d'Avenir' program (reference: ANR-10-LABX-0039). P.K.G., E.C.B. and K.L. acknowledges support from the National Science Foundation (DMR-1008791). NR 37 TC 18 Z9 18 U1 2 U2 51 PU NATURE PUBLISHING GROUP PI LONDON PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND SN 2041-1723 J9 NAT COMMUN JI Nat. Commun. PD NOV PY 2014 VL 5 AR 5441 DI 10.1038/ncomms6441 PG 7 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AU9JQ UT WOS:000345908900001 PM 25399688 ER PT J AU Park, J Lee, J Liu, L Clark, KW Durand, C Park, C Sumpter, BG Baddorf, AP Mohsin, A Yoon, M Gu, G Li, AP AF Park, Jewook Lee, Jaekwang Liu, Lei Clark, Kendal W. Durand, Corentin Park, Changwon Sumpter, Bobby G. Baddorf, Arthur P. Mohsin, Ali Yoon, Mina Gu, Gong Li, An-Ping TI Spatially resolved one-dimensional boundary states in graphene-hexagonal boron nitride planar heterostructures SO NATURE COMMUNICATIONS LA English DT Article ID EDGE STATES; QUANTUM DOTS; NANORIBBONS; INTERFACES; GROWTH; SUPERCONDUCTIVITY; COEXISTENCE; MONOLAYER; CU(111) AB Two-dimensional interfaces between crystalline materials have been shown to generate unusual interfacial electronic states in complex oxides. Recently, a one-dimensional interface has been realized in hexagonal boron nitride and graphene planar heterostructures, where a polar-on-nonpolar one-dimensional boundary is expected to possess peculiar electronic states associated with edge states of graphene and the polarity of boron nitride. Here we present a combined scanning tunnelling microscopy and first-principles theory study of the graphene-boron nitride boundary to provide a first glimpse into the spatial and energetic distributions of the one-dimensional boundary states down to atomic resolution. The revealed boundary states are about 0.6 eV below or above the Fermi level depending on the termination of the boron nitride at the boundary, and are extended along but localized at the boundary. These results suggest that unconventional physical effects similar to those observed at two-dimensional interfaces can also exist in lower dimensions. C1 [Park, Jewook; Lee, Jaekwang; Durand, Corentin; Park, Changwon; Sumpter, Bobby G.; Baddorf, Arthur P.; Yoon, Mina; Li, An-Ping] Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA. [Liu, Lei; Mohsin, Ali; Gu, Gong] Univ Tennessee, Knoxville, TN 37996 USA. [Clark, Kendal W.] Cent Methodist Univ, Fayette, MO 65248 USA. RP Yoon, M (reprint author), Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA. EM myoon@ornl.gov; ggu1@utk.edu; apli@ornl.gov RI Liu, Lei/E-6267-2014; Gu, Gong/L-5919-2015; Park, Jewook/N-2856-2015; Sumpter, Bobby/C-9459-2013; Yoon, Mina/A-1965-2016; Park, Changwon/B-3417-2016; Baddorf, Arthur/I-1308-2016; Li, An-Ping/B-3191-2012 OI Gu, Gong/0000-0002-3888-1427; Sumpter, Bobby/0000-0001-6341-0355; Yoon, Mina/0000-0002-1317-3301; Park, Changwon/0000-0002-1788-045X; Baddorf, Arthur/0000-0001-7023-2382; Li, An-Ping/0000-0003-4400-7493 FU Office of Science of the US DOE [DE-AC02-05CH11231]; NSF [ECCS-1231808]; DARPA; Laboratory Directed Research and Development Program of Oak Ridge National Laboratory; Scientific User Facilities Division, Office of Basic Energy Sciences, US Department of Energy (DOE) FX This research was conducted at the Center for Nanophase Materials Sciences, which is sponsored at Oak Ridge National Laboratory by the Scientific User Facilities Division, Office of Basic Energy Sciences, US Department of Energy (DOE). A portion of theory work (J.L.) is supported by the Laboratory Directed Research and Development Program of Oak Ridge National Laboratory, managed by UT-Battelle, LLC, for the US DOE. This research used resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the US DOE under contract no. DE-AC02-05CH11231. The work at UTK was supported by NSF (ECCS-1231808) and DARPA (approved for public release; distribution is unlimited). NR 37 TC 14 Z9 14 U1 9 U2 105 PU NATURE PUBLISHING GROUP PI LONDON PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND SN 2041-1723 J9 NAT COMMUN JI Nat. Commun. PD NOV PY 2014 VL 5 AR 5403 DI 10.1038/ncomms6403 PG 6 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AU5CN UT WOS:000345624800024 PM 25377633 ER PT J AU Shen, X Hernandez-Pagan, EA Zhou, W Puzyrev, YS Idrobo, JC Macdonald, JE Pennycook, SJ Pantelides, ST AF Shen, Xiao Hernandez-Pagan, Emil A. Zhou, Wu Puzyrev, Yevgeniy S. Idrobo, Juan-Carlos Macdonald, Janet E. Pennycook, Stephen J. Pantelides, Sokrates T. TI Interlaced crystals having a perfect Bravais lattice and complex chemical order revealed by real-space crystallography SO NATURE COMMUNICATIONS LA English DT Article ID DOMAIN BOUNDARIES; CHALCOPYRITE AB The search for optimal thermoelectric materials aims for structures in which the crystalline order is disrupted to lower the thermal conductivity without degradation of the electron conductivity. Here we report the synthesis and characterisation of ternary nanoparticles (two cations and one anion) that exhibit a new form of crystalline order: an uninterrupted, perfect, global Bravais lattice, in which the two cations exhibit a wide array of distinct ordering patterns within the cation sublattice, forming interlaced domains and phases. Partitioning into domains and phases is not unique; the corresponding boundaries have no structural defects or strain and entail no energy cost. We call this form of crystalline order 'interlaced crystals' and present the example of hexagonal CuInS2. Interlacing is possible in multi-cation tetrahedrally bonded compound with an average of two electrons per bond. Interlacing has minimal effect on electronic properties, but should strongly reduce phonon transport, making interlaced crystals attractive for thermoelectric applications. C1 [Shen, Xiao; Puzyrev, Yevgeniy S.; Pantelides, Sokrates T.] Vanderbilt Univ, Dept Phys & Astron, Nashville, TN 37235 USA. [Hernandez-Pagan, Emil A.; Macdonald, Janet E.] Vanderbilt Univ, Dept Chem, Nashville, TN 37235 USA. [Hernandez-Pagan, Emil A.; Macdonald, Janet E.; Pantelides, Sokrates T.] Vanderbilt Univ, Vanderbilt Inst Nanoscale Sci & Engn, Nashville, TN 37235 USA. [Zhou, Wu; Pantelides, Sokrates T.] Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA. [Idrobo, Juan-Carlos] Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA. [Pennycook, Stephen J.] Univ Tennessee, Dept Mat Sci & Engn, Knoxville, TN 37996 USA. [Pantelides, Sokrates T.] Vanderbilt Univ, Dept Elect Engn & Comp Sci, Nashville, TN 37235 USA. RP Shen, X (reprint author), Vanderbilt Univ, Dept Phys & Astron, Nashville, TN 37235 USA. EM xiao.shen@vanderbilt.edu; wu.zhou.stem@gmail.com RI Idrobo, Juan/H-4896-2015; Zhou, Wu/D-8526-2011; OI Idrobo, Juan/0000-0001-7483-9034; Zhou, Wu/0000-0002-6803-1095; Macdonald, Janet Elizabeth/0000-0001-6256-0706 FU Wigner Fellowship through the Laboratory Directed Research and Development Program of Oak Ridge National Laboratory; National Science Foundation [DMR-0938330]; NSF [EPS-1004083, CHE-1253105]; US-Israel Binational Foundation; Bergmann Memorial Award; ORNL's Center for Nanophase Materials Sciences (CNMS); U.S. DOE Office of Basic Energy Sciences, Scientific User Facilities Division; U.S. DOE Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division; DOE [DE-FG02-0946554]; DOE Office of Science [DE-AC02-05CH11231] FX This work is supported by a Wigner Fellowship through the Laboratory Directed Research and Development Program of Oak Ridge National Laboratory, managed by UT-Battelle, LLC, for DOE (W.Z.), by the National Science Foundation grant no. DMR-0938330 (W.Z., for work at Vanderbilt prior to 2013), by NSF EPS-1004083 (J.E.M., E.A.H.-P.), by NSF CHE-1253105 (J.E.M.), by the US-Israel Binational Foundation and the Bergmann Memorial Award (J.E.M.), by ORNL's Center for Nanophase Materials Sciences (CNMS), which is sponsored by the U.S. DOE Office of Basic Energy Sciences, Scientific User Facilities Division, (J.-C.I.), by the U.S. DOE Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division (S.J.P., X.S.), and by DOE grant DE-FG02-0946554 (S.T.P., Y.S.P.). The work used resources of the National Energy Research Scientific Computing Center, supported by the DOE Office of Science under Contract No. DE-AC02-05CH11231. We thank Lasse Noren, Ray Withers, Barry Carter, and Laurie Marks for useful discussions and Young-Min Kim and Ryo Ishikawa, and Christoph Koch for their help in strain analysis. We thank Jonathan G.C. Veinot and Tapas Purkait at the University of Alberta Chemistry Department for their assistance in obtaining the XRD pattern. NR 28 TC 6 Z9 6 U1 6 U2 56 PU NATURE PUBLISHING GROUP PI LONDON PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND SN 2041-1723 J9 NAT COMMUN JI Nat. Commun. PD NOV PY 2014 VL 5 AR 5431 DI 10.1038/ncomms6431 PG 6 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AU5CO UT WOS:000345625000011 PM 25394496 ER PT J AU Zhou, YN Ma, J Hu, EY Yu, XQ Gu, L Nam, KW Chen, LQ Wang, ZX Yang, XQ AF Zhou, Yong-Ning Ma, Jun Hu, Enyuan Yu, Xiqian Gu, Lin Nam, Kyung-Wan Chen, Liquan Wang, Zhaoxiang Yang, Xiao-Qing TI Tuning charge-discharge induced unit cell breathing in layer-structured cathode materials for lithium-ion batteries SO NATURE COMMUNICATIONS LA English DT Article ID X-RAY-DIFFRACTION; HIGH-ENERGY DENSITY; IN-SITU XRD; INSERTION MATERIAL; PHASE-TRANSITIONS; CRYSTAL-STRUCTURE; LI2MOO3; LICO1/3NI1/3MN1/3O2; ELECTRODES; CHEMISTRY AB For LiMO2 (M - Co, Ni, Mn) cathode materials, lattice parameters, a(b), contract during charge. Here we report such changes in opposite directions for lithium molybdenum trioxide (Li2MoO3). A 'unit cell breathing' mechanism is proposed based on crystal and electronic structural changes of transition metal oxides during charge-discharge. Metal-metal bonding is used to explain such 'abnormal' behaviour and a generalized hypothesis is developed. The expansion of the metal-metal bond becomes the controlling factor for a(b) evolution during charge, in contrast to the shrinking metal-oxygen bond as controlling factor in 'normal' materials. The cation mixing caused by migration of molybdenum ions at higher oxidation state provides the benefits of reducing the c expansion range in the early stage of charging and suppressing the structure collapse at high voltage charge. These results may open a new strategy for designing layered cathode materials for high energy density lithium-ion batteries. C1 [Zhou, Yong-Ning; Hu, Enyuan; Yu, Xiqian; Yang, Xiao-Qing] Brookhaven Natl Lab, Dept Chem, Upton, NY 11973 USA. [Ma, Jun; Chen, Liquan; Wang, Zhaoxiang] Chinese Acad Sci, Inst Phys, Key Lab Renewable Energy, Beijing Key Lab New Energy Mat & Devices,Beijing, Beijing 100190, Peoples R China. [Gu, Lin] Chinese Acad Sci, Inst Phys, Beijing Natl Lab Condensed Matter Phys, Lab Adv Mat & Electron Microscopy, Beijing 100190, Peoples R China. [Nam, Kyung-Wan] Dongguk Univ Seoul, Dept Energy & Mat Engn, Seoul 100715, South Korea. RP Wang, ZX (reprint author), Chinese Acad Sci, Inst Phys, Key Lab Renewable Energy, Beijing Key Lab New Energy Mat & Devices,Beijing, POB 603, Beijing 100190, Peoples R China. EM zxwang@iphy.ac.cn; xyang@bnl.gov RI Gu, Lin/D-9631-2011; Nam, Kyung-Wan/E-9063-2015; Hu, Enyuan/D-7492-2016; Yu, Xiqian/B-5574-2014 OI Gu, Lin/0000-0002-7504-031X; Nam, Kyung-Wan/0000-0001-6278-6369; Hu, Enyuan/0000-0002-1881-4534; Yu, Xiqian/0000-0001-8513-518X FU US Department of Energy, the Assistant Secretary for Energy Efficiency and Renewable Energy, Office of Vehicle Technologies [DE-AC02-98CH10886]; National Natural Science Foundation of China [51372268]; National 973 Program of China [2015CB251100]; US Department of Energy, Basic Energy Science [DE-AC02-06CH11357] FX The work at the Brookhaven National Laboratory was supported by the US Department of Energy, the Assistant Secretary for Energy Efficiency and Renewable Energy, Office of Vehicle Technologies under Contract No. DE-AC02-98CH10886. The work at the Institute of Physics, Chinese Academy of Sciences was supported by the National Natural Science Foundation (No. 51372268) of China and the National 973 Program of China (2015CB251100). We thank technical supports by the NSLS's beamline scientists at X14A, Dr Jianming Bai and X18B, Syed Khalid. We gratefully acknowledge the help by beamline scientists Sungsik Lee and Benjamin Reinhart at 12BM of Advanced Photon Source, supported by the US Department of Energy, Basic Energy Science, under Contract No. DE-AC02-06CH11357. NR 33 TC 21 Z9 21 U1 27 U2 168 PU NATURE PUBLISHING GROUP PI LONDON PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND SN 2041-1723 J9 NAT COMMUN JI Nat. Commun. PD NOV PY 2014 VL 5 AR 5381 DI 10.1038/ncomms6381 PG 8 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA AU5CN UT WOS:000345624800002 PM 25451540 ER PT J AU Amendt, P Ross, JS Milovich, JL Schneider, M Storm, E Callahan, DA Hinkel, D Lasinski, B Meeker, D Michel, P Moody, J Strozzi, D AF Amendt, Peter Ross, J. Steven Milovich, Jose L. Schneider, Marilyn Storm, Erik Callahan, Debra A. Hinkel, Denise Lasinski, Barbara Meeker, Don Michel, Pierre Moody, John Strozzi, David TI Low-adiabat rugby hohlraum experiments on the National Ignition Facility: Comparison with high-flux modeling and the potential for gas-wall interpenetration SO PHYSICS OF PLASMAS LA English DT Article ID RAYLEIGH-TAYLOR INSTABILITY; LASER; TARGETS; GROWTH AB Rugby-shaped gold hohlraums driven by a nominal low-adiabat laser pulse shape have been tested on the National Ignition Facility. The rugby affords a higher coupling efficiency than a comparably sized cylinder hohlraum or, alternatively, improved drive symmetry and laser beam clearances for a larger hohlraum with similar cylinder wall area and laser energy. A first (large rugby hohlraum) shot at low energy (0.75 MJ) to test laser backscatter resulted in a moderately oblate CH capsule implosion, followed by a high energy shot (1.3MJ) that gave a highly oblate compressed core according to both time-integrated and -resolved x-ray images. These implosions used low wavelength separation (1.0 angstrom) between the outer and inner cones to provide an alternative platform free of significant cross-beam energy transfer for simplified hohlraum dynamics. Post-shot 2- and 3-D radiation-hydrodynamic simulations using the high-flux model [M. D. Rosen et al., High Energy Density Phys. 7, 180 (2011)], however, give nearly round implosions for both shots, in striking contrast with observations. An analytic assessment of Rayleigh-Taylor hydrodynamic instability growth on the gold-helium gas-fill interface shows the potential for significant linear growth, saturation and transition to a highly nonlinear state. Candidate seeds for instability growth include laser speckle during the early-time laser picket episode in the presence of only partial temporal beam smoothing (1-D smoothing by spectral dispersion and polarization smoothing) and intensity modulations from quad-to-quad and beam overlap. Radiation-hydrodynamic 2-D simulations adapted to include a dynamic fall-line mix model across the unstable Au-He interface show good agreement with the observed implosion symmetry for both shots using an interface-to-fall-line penetration fraction of 100%. Physically, the potential development of an instability layer in a rugby hohlraum is tantamount to an enhanced wall motion leading to hindered inner-beam propagation, due largely to the confluence of rugby shape and low ray angles relative to the hohlraum symmetry axis. A significant inward pointing shift of 500 mu m in the outer cones for the third (full energy) shot of the series was used to improve the inner-beam propagation, resulting in a nearly symmetric x-ray self-emission image of the compressed core and reduced sensitivity to mix. Comparatively low time-dependent symmetry swings were also measured, and a significantly lower hot electron fraction was measured for potentially favorable fuel adiabat control. The outer cone stimulated Brillouin scatter levels jumped significantly, but remedial measures such as the use of a boron dopant in the Au wall are planned. A continuing trend of delayed implosion times is found in rugby hohlraums, suggesting levels of unaccounted hohlraum energy (similar to 150-200 kJ) similar to what is inferred in cylinder hohlraums. A mix-based physical scenario is described, based on suppressed channel heat flux to the dense gold wall from a temperature-gradient reversal induced by a multispecies plasma lapse rate [P. Amendt, C. Bellei, and S. C. Wilks, Phys. Rev. Lett. 109, 075002 (2012)]. (C) 2014 AIP Publishing LLC. C1 [Amendt, Peter; Ross, J. Steven; Milovich, Jose L.; Schneider, Marilyn; Storm, Erik; Callahan, Debra A.; Hinkel, Denise; Lasinski, Barbara; Meeker, Don; Michel, Pierre; Moody, John; Strozzi, David] Lawrence Livermore Natl Lab, Livermore, CA 94551 USA. RP Amendt, P (reprint author), Lawrence Livermore Natl Lab, Livermore, CA 94551 USA. EM amendt1@llnl.gov OI Strozzi, David/0000-0001-8814-3791 FU Lawrence Livermore National Security, LLC (LLNS) [DE-AC52-07NA27344]; [LDRD-11-SI-002] FX Useful discussions and scientific exchanges with P. Gauthier and J.-P. Leidinger at CEA-DAM-DIF (Arpajon, France) are gratefully acknowledged. We thank Nino Landen for a careful reading of the manuscript. This work was performed under the auspices of Lawrence Livermore National Security, LLC (LLNS) under Contract No. DE-AC52-07NA27344 and supported by LDRD-11-SI-002. NR 35 TC 16 Z9 16 U1 0 U2 13 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 1070-664X EI 1089-7674 J9 PHYS PLASMAS JI Phys. Plasmas PD NOV PY 2014 VL 21 IS 11 AR 112703 DI 10.1063/1.4901195 PG 11 WC Physics, Fluids & Plasmas SC Physics GA AU5JZ UT WOS:000345644200042 ER PT J AU Berkery, JW Betti, R Sabbagh, SA Guazzotto, L Manickam, J AF Berkery, J. W. Betti, R. Sabbagh, S. A. Guazzotto, L. Manickam, J. TI The effect of an anisotropic pressure of thermal particles on resistive wall mode stability SO PHYSICS OF PLASMAS LA English DT Article ID BALLOONING STABILITY; TOKAMAK EQUILIBRIA; ENERGY PRINCIPLE; PLASMA; WAVES; FLOW; INSTABILITIES; EQUATIONS; PHYSICS; MHD AB The effect of an anisotropic pressure of thermal particles on resistive wall mode stability in tokamak fusion plasmas is derived through kinetic theory and assessed through calculation with the MISK code [B. Hu et al., Phys. Plasmas 12, 0 57301 (2005)]. The fluid anisotropy is treated as a small perturbation on the plasma equilibrium and modeled with a bi-Maxwellian distribution function. A complete stability treatment without an assumption of high frequency mode rotation leads to anisotropic kinetic terms in the dispersion relation in addition to anisotropy corrections to the fluid terms. With the density and the average pressure kept constant, when thermal particles have a higher temperature perpendicular to the magnetic field than parallel, the fluid pressure-driven ballooning destabilization term is reduced. Additionally, the stabilizing kinetic effects of the trapped thermal ions can be enhanced. Together these two effects can lead to a modest increase in resistive wall mode stability. (C) 2014 AIP Publishing LLC. C1 [Berkery, J. W.; Sabbagh, S. A.] Columbia Univ, Dept Appl Phys & Appl Math, New York, NY 10027 USA. [Betti, R.] Univ Rochester, Laser Energet Lab, Rochester, NY 14623 USA. [Guazzotto, L.] Auburn Univ, Dept Phys, Auburn, AL 36849 USA. [Manickam, J.] Princeton Univ, Princeton Plasma Phys Lab, Princeton, NJ 08543 USA. RP Berkery, JW (reprint author), Columbia Univ, Dept Appl Phys & Appl Math, New York, NY 10027 USA. EM jberkery@pppl.gov FU U.S. Department of Energy [DE-FG02-99ER54524, DE-AC02-09CH11466, DE-FG02-93ER54215] FX This research was supported by the U.S. Department of Energy under Contract Nos. DE-FG02-99ER54524, DE-AC02-09CH11466, and DE-FG02-93ER54215. NR 71 TC 4 Z9 4 U1 2 U2 7 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 1070-664X EI 1089-7674 J9 PHYS PLASMAS JI Phys. Plasmas PD NOV PY 2014 VL 21 IS 11 AR 112505 DI 10.1063/1.4901568 PG 12 WC Physics, Fluids & Plasmas SC Physics GA AU5JZ UT WOS:000345644200032 ER PT J AU Chowdhury, J Wan, WG Chen, Y Parker, SE Groebner, RJ Holland, C Howard, NT AF Chowdhury, J. Wan, Weigang Chen, Yang Parker, Scott E. Groebner, Richard J. Holland, C. Howard, N. T. TI Study of the L-mode tokamak plasma "shortfall" with local and global nonlinear gyrokinetic delta f particle-in-cell simulation SO PHYSICS OF PLASMAS LA English DT Article ID KINETIC ELECTRONS; ZONAL FLOW; TURBULENCE; TRANSPORT; DRIVEN AB The delta f particle-in-cell code GEM is used to study the transport "shortfall" problem of gyrokinetic simulations. In local simulations, the GEM results confirm the previously reported simulation results of DIII-D [Holland et al., Phys. Plasmas 16, 052301 (2009)] and Alcator C-Mod [Howard et al., Nucl. Fusion 53, 123011 (2013)] tokamaks with the continuum code GYRO. Namely, for DIII-D the simulations closely predict the ion heat flux at the core, while substantially underpredict transport towards the edge; while for Alcator C-Mod, the simulations show agreement with the experimental values of ion heat flux, at least within the range of experimental error. Global simulations are carried out for DIII-D L-mode plasmas to study the effect of edge turbulence on the outer core ion heat transport. The edge turbulence enhances the outer core ion heat transport through turbulence spreading. However, this edge turbulence spreading effect is not enough to explain the transport underprediction. (C) 2014 AIP Publishing LLC. C1 [Chowdhury, J.; Wan, Weigang; Chen, Yang; Parker, Scott E.] Univ Colorado, Dept Phys, Boulder, CO 80309 USA. [Groebner, Richard J.] Gen Atom Co, San Diego, CA 92186 USA. [Holland, C.] Univ Calif San Diego, La Jolla, CA 92093 USA. [Howard, N. T.] ORISE, Oak Ridge, TN 37831 USA. RP Chowdhury, J (reprint author), Univ Colorado, Dept Phys, Boulder, CO 80309 USA. FU U.S. Department of Energy, Office of Science, Office of Fusion Energy Sciences [DE-FC02-04ER54698, DOE-SC0008801, DE-FG02-07ER54917, DE-FG02-08ER54954] FX This material is based upon work supported in part by the U.S. Department of Energy, Office of Science, Office of Fusion Energy Sciences, using the DIII-D National Fusion Facility, a DOE Office of Science user facility, under Award Nos. DE-FC02-04ER54698, DOE-SC0008801, DE-FG02-07ER54917, and DE-FG02-08ER54954. DIII-D data shown in this paper can be obtained in digital format by following the links at https://fusion.gat.com/global/D3D_DMP. This research also used resources of the National Energy Research Scientific Computing Center (NERSC), which is a DOE Office of Science user facility. NR 41 TC 8 Z9 8 U1 0 U2 1 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 1070-664X EI 1089-7674 J9 PHYS PLASMAS JI Phys. Plasmas PD NOV PY 2014 VL 21 IS 11 AR 112503 DI 10.1063/1.4901031 PG 11 WC Physics, Fluids & Plasmas SC Physics GA AU5JZ UT WOS:000345644200030 ER PT J AU Clark, DS Milovich, JL Hinkel, DE Salmonson, JD Peterson, JL Hopkins, LFB Eder, DC Haan, SW Jones, OS Marinak, MM Robey, HF Smalyuk, VA Weber, CR AF Clark, D. S. Milovich, J. L. Hinkel, D. E. Salmonson, J. D. Peterson, J. L. Hopkins, L. F. Berzak Eder, D. C. Haan, S. W. Jones, O. S. Marinak, M. M. Robey, H. F. Smalyuk, V. A. Weber, C. R. TI A survey of pulse shape options for a revised plastic ablator ignition design SO PHYSICS OF PLASMAS LA English DT Article ID DECELERATION-PHASE; TAYLOR INSTABILITY; FACILITY TARGETS; CAPSULE DESIGN AB Recent experimental results using the "high foot" pulse shape for inertial confinement fusion ignition experiments on the National Ignition Facility (NIF) [Moses et al., Phys. Plasmas 16, 041006 (2009)] have shown encouraging progress compared to earlier "low foot" experiments. These results strongly suggest that controlling ablation front instability growth can significantly improve implosion performance even in the presence of persistent, large, low-mode distortions. Simultaneously, hydrodynamic growth radiography experiments have confirmed that ablation front instability growth is being modeled fairly well in NIF experiments. It is timely then to combine these two results and ask how current ignition pulse shapes could be modified to improve one-dimensional implosion performance while maintaining the stability properties demonstrated with the high foot. This paper presents such a survey of pulse shapes intermediate between the low and high foot extremes in search of an intermediate foot optimum. Of the design space surveyed, it is found that a higher picket version of the low foot pulse shape shows the most promise for improved compression without loss of stability. (C) 2014 AIP Publishing LLC. C1 [Milovich, J. L.; Hinkel, D. E.; Salmonson, J. D.; Peterson, J. L.; Hopkins, L. F. Berzak; Eder, D. C.; Haan, S. W.; Jones, O. S.; Marinak, M. M.; Robey, H. F.; Smalyuk, V. A.; Weber, C. R.] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA. RP Clark, DS (reprint author), Lawrence Livermore Natl Lab, Livermore, CA 94550 USA. OI Peterson, Luc/0000-0002-5167-5708 FU U.S. Department of Energy by Lawrence Livermore National Laboratory [DE-AC52-07NA27344] FX This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344. NR 53 TC 30 Z9 30 U1 1 U2 15 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 1070-664X EI 1089-7674 J9 PHYS PLASMAS JI Phys. Plasmas PD NOV PY 2014 VL 21 IS 11 AR 112705 DI 10.1063/1.4901572 PG 14 WC Physics, Fluids & Plasmas SC Physics GA AU5JZ UT WOS:000345644200044 ER PT J AU Ferrario, L Little, JM Choueiri, EY AF Ferrario, Lorenzo Little, Justin M. Choueiri, Edgar Y. TI Propulsive performance of a finite-temperature plasma flow in a magnetic nozzle with applied azimuthal current SO PHYSICS OF PLASMAS LA English DT Article ID FIELD CURRENT DRIVE; HALL THRUSTER; FUSION ROCKET; DETACHMENT; ACCELERATORS AB The plasma flow in a finite-electron-temperature magnetic nozzle, under the influence of an applied azimuthal current at the throat, is modeled analytically to assess its propulsive performance. A correction to the nozzle throat boundary conditions is derived by modifying the radial equilibrium of a magnetized infinite two-population cylindrical plasma column with the insertion of an external azimuthal body force for the electrons. Inclusion of finite-temperature effects, which leads to a modification of the radial density profile, is necessary for calculating the propulsive performance, which is represented by nozzle divergence efficiency and thrust coefficient. The solutions show that the application of the azimuthal current enhances all the calculated performance parameters through the narrowing of the radial density profile at the throat, and that investing power in this beam focusing effect is more effective than using the same power to pre-heat the electrons. The results open the possibility for the design of a focusing stage between the plasma source and the nozzle that can significantly enhance the propulsive performance of electron-driven magnetic nozzles. (C) 2014 AIP Publishing LLC. C1 [Ferrario, Lorenzo] Politecn Milan, I-20133 Milan, Italy. [Little, Justin M.; Choueiri, Edgar Y.] Princeton Univ, Elect Prop & Plasma Dynam Lab, Princeton, NJ 08540 USA. RP Ferrario, L (reprint author), Politecn Milan, I-20133 Milan, Italy. EM lorenzo.ferrario@polimi.it; jml@princeton.edu; choueiri@princeton.edu FU scholarship Borsa di Studio Tesi All'Estero of the Politecnico di Milano; Program in Plasma Science and Technology through DOE [DE-AC02-09CH11466]; Department of Defense (DoD) National Defense Science and Engineering Graduate Fellowship (NDSEG) Program FX The authors would like to thank Professor Nat Fisch for insightful comments regarding relevance to other devices. The work of the first author has been supported by the scholarship Borsa di Studio Tesi All'Estero 2012-2013 of the Politecnico di Milano. We also thank the Program in Plasma Science and Technology for support through DOE Contract No. DE-AC02-09CH11466 and the Department of Defense (DoD) National Defense Science and Engineering Graduate Fellowship (NDSEG) Program. NR 44 TC 2 Z9 2 U1 4 U2 7 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 1070-664X EI 1089-7674 J9 PHYS PLASMAS JI Phys. Plasmas PD NOV PY 2014 VL 21 IS 11 AR 113507 DI 10.1063/1.4901587 PG 11 WC Physics, Fluids & Plasmas SC Physics GA AU5JZ UT WOS:000345644200067 ER PT J AU Greenwald, M Bader, A Baek, S Bakhtiari, M Barnard, H Beck, W Bergerson, W Bespamyatnov, I Bonoli, P Brower, D Brunner, D Burke, W Candy, J Churchill, M Cziegler, I Diallo, A Dominguez, A Duval, B Edlund, E Ennever, P Ernst, D Faust, I Fiore, C Fredian, T Garcia, O Gao, C Goetz, J Golfinopoulos, T Granetz, R Grulke, O Hartwig, Z Horne, S Howard, N Hubbard, A Hughes, J Hutchinson, I Irby, J Izzo, V Kessel, C LaBombard, B Lau, C Li, C Lin, Y Lipschultz, B Loarte, A Marmar, E Mazurenko, A McCracken, G McDermott, R Meneghini, O Mikkelsen, D Mossessian, D Mumgaard, R Myra, J Nelson-Melby, E Ochoukov, R Olynyk, G Parker, R Pitcher, S Podpaly, Y Porkolab, M Reinke, M Rice, J Rowan, W Schmidt, A Scott, S Shiraiwa, S Sierchio, J Smick, N Snipes, JA Snyder, P Sorbom, B Stillerman, J Sung, C Takase, Y Tang, V Terry, J Terry, D Theiler, C Tronchin-James, A Tsujii, N Vieira, R Walk, J Wallace, G White, A Whyte, D Wilson, J Wolfe, S Wright, G Wright, J Wukitch, S Zweben, S AF Greenwald, M. Bader, A. Baek, S. Bakhtiari, M. Barnard, H. Beck, W. Bergerson, W. Bespamyatnov, I. Bonoli, P. Brower, D. Brunner, D. Burke, W. Candy, J. Churchill, M. Cziegler, I. Diallo, A. Dominguez, A. Duval, B. Edlund, E. Ennever, P. Ernst, D. Faust, I. Fiore, C. Fredian, T. Garcia, O. Gao, C. Goetz, J. Golfinopoulos, T. Granetz, R. Grulke, O. Hartwig, Z. Horne, S. Howard, N. Hubbard, A. Hughes, J. Hutchinson, I. Irby, J. Izzo, V. Kessel, C. LaBombard, B. Lau, C. Li, C. Lin, Y. Lipschultz, B. Loarte, A. Marmar, E. Mazurenko, A. McCracken, G. McDermott, R. Meneghini, O. Mikkelsen, D. Mossessian, D. Mumgaard, R. Myra, J. Nelson-Melby, E. Ochoukov, R. Olynyk, G. Parker, R. Pitcher, S. Podpaly, Y. Porkolab, M. Reinke, M. Rice, J. Rowan, W. Schmidt, A. Scott, S. Shiraiwa, S. Sierchio, J. Smick, N. Snipes, J. A. Snyder, P. Sorbom, B. Stillerman, J. Sung, C. Takase, Y. Tang, V. Terry, J. Terry, D. Theiler, C. Tronchin-James, A. Tsujii, N. Vieira, R. Walk, J. Wallace, G. White, A. Whyte, D. Wilson, J. Wolfe, S. Wright, G. Wright, J. Wukitch, S. Zweben, S. TI 20 years of research on the Alcator C-Mod tokamak SO PHYSICS OF PLASMAS LA English DT Review ID SCRAPE-OFF-LAYER; INTERNAL TRANSPORT BARRIERS; ION-CYCLOTRON RANGE; PLASMA-FACING COMPONENTS; L-H TRANSITION; IMPURITY TOROIDAL ROTATION; X-RAY OBSERVATIONS; LOWER-HYBRID WAVES; NO MOMENTUM INPUT; PRESSURE GAS INJECTION AB The object of this review is to summarize the achievements of research on the Alcator C-Mod tokamak [Hutchinson et al., Phys. Plasmas 1, 1511 (1994) and Marmar, Fusion Sci. Technol. 51, 261 (2007)] and to place that research in the context of the quest for practical fusion energy. C-Mod is a compact, high-field tokamak, whose unique design and operating parameters have produced a wealth of new and important results since it began operation in 1993, contributing data that extends tests of critical physical models into new parameter ranges and into new regimes. Using only high-power radio frequency (RF) waves for heating and current drive with innovative launching structures, C-Mod operates routinely at reactor level power densities and achieves plasma pressures higher than any other toroidal confinement device. C-Mod spearheaded the development of the vertical-target divertor and has always operated with high-Z metal plasma facing components-approaches subsequently adopted for ITER. C-Mod has made ground-breaking discoveries in divertor physics and plasma-material interactions at reactor-like power and particle fluxes and elucidated the critical role of cross-field transport in divertor operation, edge flows and the tokamak density limit. C-Mod developed the I-mode and the Enhanced D alpha H-mode regimes, which have high performance without large edge localized modes and with pedestal transport self-regulated by short-wavelength electromagnetic waves. C-Mod has carried out pioneering studies of intrinsic rotation and demonstrated that self-generated flow shear can be strong enough in some cases to significantly modify transport. C-Mod made the first quantitative link between the pedestal temperature and the H-mode's performance, showing that the observed self-similar temperature profiles were consistent with critical-gradient-length theories and followed up with quantitative tests of nonlinear gyrokinetic models. RF research highlights include direct experimental observation of ion cyclotron range of frequency (ICRF) mode-conversion, ICRF flow drive, demonstration of lower-hybrid current drive at ITER-like densities and fields and, using a set of novel diagnostics, extensive validation of advanced RF codes. Disruption studies on C-Mod provided the first observation of non-axisymmetric halo currents and non-axisymmetric radiation in mitigated disruptions. A summary of important achievements and discoveries are included. (C) 2014 AIP Publishing LLC. C1 [Greenwald, M.; Baek, S.; Barnard, H.; Beck, W.; Bonoli, P.; Brunner, D.; Burke, W.; Ennever, P.; Ernst, D.; Faust, I.; Fiore, C.; Fredian, T.; Gao, C.; Golfinopoulos, T.; Granetz, R.; Hartwig, Z.; Hubbard, A.; Hughes, J.; Hutchinson, I.; Irby, J.; LaBombard, B.; Li, C.; Lin, Y.; Marmar, E.; Mumgaard, R.; Parker, R.; Porkolab, M.; Rice, J.; Shiraiwa, S.; Sierchio, J.; Sorbom, B.; Stillerman, J.; Sung, C.; Terry, J.; Terry, D.; Vieira, R.; Walk, J.; Wallace, G.; White, A.; Whyte, D.; Wolfe, S.; Wright, G.; Wright, J.; Wukitch, S.] MIT Plasma Sci & Fusion Ctr, Cambridge, MA 02139 USA. [Bader, A.; Bakhtiari, M.; Goetz, J.] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA. [Bergerson, W.; Brower, D.] Univ Calif Los Angeles, Inst Plasma & Fusion Res, Los Angeles, CA 90095 USA. [Bespamyatnov, I.; Rowan, W.] Univ Texas Austin, Fus Res Ctr, Austin, TX 78712 USA. [Candy, J.; Meneghini, O.; Snyder, P.] Gen Atom Co, San Diego, CA 92186 USA. [Churchill, M.; Diallo, A.; Dominguez, A.; Edlund, E.; Kessel, C.; Mikkelsen, D.; Scott, S.; Wilson, J.; Zweben, S.] Princeton Plasma Phys Lab, Princeton, NJ 08540 USA. [Cziegler, I.; Izzo, V.] Univ Calif San Diego, Ctr Momentum Transport & Flow Org, La Jolla, CA 92093 USA. [Duval, B.; Theiler, C.] Ecole Polytech Fed Lausanne, Ctr Rech Phys Plasmas, CH-1015 Lausanne, Switzerland. [Garcia, O.] Univ Tromso, Dept Phys & Technol, N-9037 Tromso, Norway. [Grulke, O.] EURATOM, MPI Plasma Phys, D-17491 Greifswald, Germany. [Grulke, O.] Ernst Moritz Arndt Univ Greifswald, D-17489 Greifswald, Germany. [Horne, S.] Energetiq Technol, Woburn, MA 01801 USA. [Howard, N.] Oak Ridge Inst Sci & Educ, Oak Ridge, TN 37830 USA. [Lau, C.] ORNL, Oak Ridge, TN 37831 USA. [Lipschultz, B.; Reinke, M.] Univ York, York YO10 5DD, N Yorkshire, England. [Loarte, A.; Pitcher, S.; Snipes, J. A.] ITER Org, F-13067 St Paul Les Durance, France. [Mazurenko, A.] Block Engn, Marlborough, MA 01752 USA. [McCracken, G.] UKAEA, Culham Ctr Fus Energy, Abingdon OX14 3DB, Oxon, England. [McDermott, R.; Ochoukov, R.] Max Planck Inst Plasma Phys, EURATOM Assoc, D-85748 Garching, Germany. [Mossessian, D.] AllianceBernstein, New York, NY 10105 USA. [Myra, J.] Lodestar Res Corp, Boulder, CO 80301 USA. [Nelson-Melby, E.] Raytheon Co, Tucson, AZ 85756 USA. [Olynyk, G.] McKinsey & Co Inc, Toronto, ON M5S 1K9, Canada. [Podpaly, Y.] Natl Inst Sci & Technol, Gaithersburg, MD 20899 USA. [Schmidt, A.; Tang, V.] LLNL, Livermore, CA 94550 USA. [Smick, N.] GT Adv Technol, Merrimack, NH 03054 USA. [Takase, Y.; Tsujii, N.] Univ Tokyo, Tokyo 113033, Japan. [Tronchin-James, A.] Facebook LLC, Menlo Pk, CA 94205 USA. RP Greenwald, M (reprint author), MIT Plasma Sci & Fusion Ctr, Cambridge, MA 02139 USA. RI Garcia, Odd Erik/A-4417-2013; Lipschultz, Bruce/J-7726-2012; EPFL, Physics/O-6514-2016; OI Garcia, Odd Erik/0000-0002-2377-8718; Lipschultz, Bruce/0000-0001-5968-3684; Theiler, Christian/0000-0003-3926-1374; Greenwald, Martin/0000-0002-4438-729X FU DOE [DE-FC02-99ER54512, DE-FG03-94ER-54241, DE-AC02-78ET-51013, DE-AC02-09CH11466, DE-FG02-95ER54309, DE-AC02-05CH11231, DE-AC52-07NA27344, DE-FG02-97ER54392, DE-SC00-02060]; NSF [DMR-08-19762]; Swiss National Science Foundation; Alexander-von-Humboldt Foundation FX The authors wish to thank the extraordinarily able Alcator staff, students, and collaborators who have worked on this program since its inception. A full list of those contributors, which is as complete as we can make it given the imperfection of our records and our memories, is included in the Appendix. The work described here only touches on a selection of the research highlights produced by this team; much must be left out due to limits on space and time. The authors also wish to thank DOE, our principal funding agency under who have supported this work mainly under cooperative agreement C-Mod: DE-FC02-99ER54512 but also under DE-FG03-94ER-54241, DE-AC02-78ET-51013, DE-AC02-09CH11466, DE-FG02-95ER54309, DE-AC02-05CH11231, DE-AC52-07NA27344, DE-FG02-97ER54392, and DE-SC00-02060. International Contributors have been funded through NSF DMR-08-19762, the Swiss National Science Foundation and the Alexander-von-Humboldt Foundation among others. NR 400 TC 11 Z9 11 U1 3 U2 78 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 1070-664X EI 1089-7674 J9 PHYS PLASMAS JI Phys. Plasmas PD NOV PY 2014 VL 21 IS 11 AR 110501 DI 10.1063/1.4901920 PG 50 WC Physics, Fluids & Plasmas SC Physics GA AU5JZ UT WOS:000345644200001 ER PT J AU Gui, B Xu, XQ Myra, JR D'Ippolito, DA AF Gui, B. Xu, X. Q. Myra, J. R. D'Ippolito, D. A. TI Mitigating impact of thermal and rectified radio-frequency sheath potentials on edge localized modes SO PHYSICS OF PLASMAS LA English DT Article ID PLASMA INTERACTIONS; MHD STABILITY; ICRF; BOUNDARY; ANTENNA; TEXTOR; INSTABILITIES; CONFINEMENT; SIMULATION AB The mitigating impact of thermal and rectified radio frequency (RF) sheath potentials on the peeling-ballooning modes is studied non-linearly by employing a two-fluid three-field simulation model based on the BOUT++framework. Additional shear flow and the Kelvin-Helmholtz effect due to the thermal and rectified RF sheath potential are induced. It is found that the shear flow increases the growth rate while the K-H effect decreases the growth rate slightly when there is a density gradient, but the energy loss of these cases is suppressed in the nonlinear phase. The stronger external electrostatic field due to the sheaths has a more significant effect on the energy loss suppression. From this study, it is found the growth rate in the linear phase mainly determines the onset of edge-localized modes, while the mode spectrum width in the nonlinear phase has an important impact on the turbulent transport. The wider mode spectrum leads to weaker turbulent transport and results in a smaller energy loss. Due to the thermal sheath and rectified RF sheath potential in the scrape-off-layer, the modified shear flow tears apart the peeling-ballooning filament and makes the mode spectrum wider, resulting in less energy loss. The perturbed electric potential and the parallel current near the sheath region is also suppressed locally due to the sheath boundary condition. (C) 2014 AIP Publishing LLC. C1 [Gui, B.] Chinese Acad Sci, Inst Plasma Phys, Hefei, Peoples R China. [Gui, B.; Xu, X. Q.] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA. [Myra, J. R.; D'Ippolito, D. A.] Lodestar Res Corp, Boulder, CO 80301 USA. RP Gui, B (reprint author), Chinese Acad Sci, Inst Plasma Phys, Hefei, Peoples R China. OI Myra, James/0000-0001-5939-8429 FU U.S. Department of Energy by Lawrence Livermore National Laboratory [DE-AC52-07NA27344]; U.S. Department of Energy, Office of Science, Office of Fusion Energy Sciences; LLNL LDRD [12-ERD-022]; LDRD [11-ERD-058]; China Scholarship Committee [2011601099]; ITER [2011GB101001, LLNL-JRNL-658251] FX The authors wish to acknowledge Dr. T. Y. Xia, Mr. P. W. Xi, and Mr. C. H. Ma for useful discussions. This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract No. DE-AC52-07NA27344. This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Fusion Energy Sciences. LLNL LDRD project 12-ERD-022 and LDRD project 11-ERD-058, the China Scholarship Committee under Contract No. 2011601099, and the ITER project under Contract No. 2011GB101001, LLNL-JRNL-658251. Lodestar Research Corporation under DE-FG02-97ER54392. NR 38 TC 4 Z9 4 U1 3 U2 18 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 1070-664X EI 1089-7674 J9 PHYS PLASMAS JI Phys. Plasmas PD NOV PY 2014 VL 21 IS 11 AR 112302 DI 10.1063/1.4901306 PG 11 WC Physics, Fluids & Plasmas SC Physics GA AU5JZ UT WOS:000345644200022 ER PT J AU Howard, NT Holland, C White, AE Greenwald, M Candy, J AF Howard, N. T. Holland, C. White, A. E. Greenwald, M. Candy, J. TI Synergistic cross-scale coupling of turbulence in a tokamak plasma SO PHYSICS OF PLASMAS LA English DT Article ID ELECTRON-TEMPERATURE-GRADIENT; TRANSPORT; MODEL AB For the first time, nonlinear gyrokinetic simulations spanning both the ion and electron spatiotemporal scales have been performed with realistic electron mass ratio ((m(D)/m(e))(1/2) = 60.0), realistic geometry, and all experimental inputs, demonstrating the coexistence and synergy of ion (k(theta)rho(s) similar to O(1.0)) and electron-scale (k(theta)rho(e) similar to O(1.0)) turbulence in the core of a tokamak plasma. All multi-scale simulations utilized the GYRO code [J. Candy and R. E. Waltz, J. Comput. Phys. 186, 545 (2003)] to study the coupling of ion and electron-scale turbulence in the core (r/a = 0.6) of an Alcator C-Mod L-mode discharge shown previously to exhibit an under-prediction of the electron heat flux when using simulations only including ion-scale turbulence. Electron-scale turbulence is found to play a dominant role in setting the electron heat flux level and radially elongated (k(r) << k(theta)) "streamers" are found to coexist with ion-scale eddies in experimental plasma conditions. Inclusion of electron-scale turbulence in these simulations is found to increase both ion and electron heat flux levels by enhancing the transport at the ion-scale while also driving electron heat flux at sub-rho(i) scales. The combined increases in the low and high-k driven electron heat flux may explain previously observed discrepancies between simulated and experimental electron heat fluxes and indicates a complex interaction of short and long wavelength turbulence. (C) 2014 AIP Publishing LLC. C1 [Howard, N. T.] ORISE, Oak Ridge, TN 37831 USA. [Holland, C.] Univ Calif San Diego, La Jolla, CA 92093 USA. [White, A. E.; Greenwald, M.] MIT, Plasma Sci & Fus Ctr, Cambridge, MA 02139 USA. [Candy, J.] Gen Atom Co, San Diego, CA 92186 USA. RP Howard, NT (reprint author), ORISE, Oak Ridge, TN 37831 USA. EM nthoward@psfc.mit.edu OI Greenwald, Martin/0000-0002-4438-729X FU Office of Science of the U.S. Department of Energy [DE-AC02-05CH11231]; DOE [DE-FC02-99ER54512-CMOD]; U.S. DOE Fusion Energy Postdoctoral Research Program FX The authors would like to thank the entire Alcator C-Mod team. Specifically we thank Dr. Matt Reinke for the ion temperature and rotation profiles and Dr. Tobias Gorler for valuable discussion and input on multi-scale simulation. Computer simulations are part of research performed for the Center for Simulation of Plasma Microturbulence (CSPM) and were carried out at the National Energy Research Scientific Computing Center, supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. This work was also supported by DOE Contract No. DE-FC02-99ER54512-CMOD and in part by an appointment to the U.S. DOE Fusion Energy Postdoctoral Research Program administered by ORISE. NR 24 TC 18 Z9 18 U1 0 U2 14 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 1070-664X EI 1089-7674 J9 PHYS PLASMAS JI Phys. Plasmas PD NOV PY 2014 VL 21 IS 11 AR 112510 DI 10.1063/1.4902366 PG 6 WC Physics, Fluids & Plasmas SC Physics GA AU5JZ UT WOS:000345644200037 ER PT J AU Mikkelsen, DR Nunami, M Watanabe, TH Sugama, H Tanaka, K AF Mikkelsen, D. R. Nunami, M. Watanabe, T. -H. Sugama, H. Tanaka, K. TI Verification of gyrokinetic microstability codes with an LHD configuration SO PHYSICS OF PLASMAS LA English DT Article ID TEMPERATURE-GRADIENT TURBULENCE; SIMULATIONS AB We extend previous benchmarks of the GS2 and GKV-X codes to verify their algorithms for solving the gyrokinetic Vlasov-Poisson equations for plasma microturbulence. Code benchmarks are the most complete way of verifying the correctness of implementations for the solution of mathematical models for complex physical processes such as those studied here. The linear stability calculations reported here are based on the plasma conditions of an ion-ITB plasma in the LHD configuration. The plasma parameters and the magnetic geometry differ from previous benchmarks involving these codes. We find excellent agreement between the independently written pre-processors that calculate the geometrical coefficients used in the gyrokinetic equations. Grid convergence tests are used to establish the resolution and domain size needed to obtain converged linear stability results. The agreement of the frequencies, growth rates, and eigenfunctions in the benchmarks reported here provides additional verification that the algorithms used by the GS2 and GKV-X codes are correctly finding the linear eigenvalues and eigenfunctions of the gyrokinetic Vlasov-Poisson equations. (C) 2014 AIP Publishing LLC. C1 [Mikkelsen, D. R.] Princeton Plasma Phys Lab, Princeton, NJ 08543 USA. [Nunami, M.; Sugama, H.; Tanaka, K.] Natl Inst Fus Sci, Toki, Gifu 5095292, Japan. [Watanabe, T. -H.] Nagoya Univ Furo cho, Dept Phys, Chikusa Ku, Nagoya, Aichi 4648602, Japan. RP Mikkelsen, DR (reprint author), Princeton Plasma Phys Lab, POB 451, Princeton, NJ 08543 USA. EM dmikkelsen@pppl.gov OI Hideo, Sugama/0000-0001-5444-1758 FU Japanese Ministry of Education, Culture, Sports, Science and Technology [22760660, 26820398]; Japan/U.S. Cooperation in Fusion Research and Development; U.S. Department of Energy [DE-AC02-76CH03073] FX We thank J. A. Baumgaertel, G. W. Hammett, and P. Xanthopoulos for helpful discussions. This work has been done under the collaboration research of the National Institute for Fusion Science. It is a pleasure to acknowledge cooperation and discussions with Professor K. Komori, Professor O. Kaneko, and Professor H. Yamada of the National Institute for Fusion Science. One of the authors (M.N.) was supported in part by the Japanese Ministry of Education, Culture, Sports, Science and Technology, Grant (Nos. 22760660 and 26820398), and by Japan/U.S. Cooperation in Fusion Research and Development. This work was supported by U.S. Department of Energy Contract No. DE-AC02-76CH03073. Use of parallel computer clusters at PPPL is gratefully acknowledged. NR 33 TC 2 Z9 2 U1 0 U2 3 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 1070-664X EI 1089-7674 J9 PHYS PLASMAS JI Phys. Plasmas PD NOV PY 2014 VL 21 IS 11 AR 112305 DI 10.1063/1.4902124 PG 8 WC Physics, Fluids & Plasmas SC Physics GA AU5JZ UT WOS:000345644200025 ER PT J AU Ott, T Bonitz, M Stanton, LG Murillo, MS AF Ott, T. Bonitz, M. Stanton, L. G. Murillo, M. S. TI Coupling strength in Coulomb and Yukawa one-component plasmas SO PHYSICS OF PLASMAS LA English DT Article ID CRYSTALS; SYSTEMS AB In a non-ideal classical Coulomb one-component plasma (OCP), all thermodynamic properties are known to depend only on a single parameter-the coupling parameter Gamma. In contrast, if the pair interaction is screened by background charges (Yukawa OCP) the thermodynamic state depends, in addition, on the range of the interaction via the screening parameter kappa. How to determine in this case an effective coupling parameter has been a matter of intensive debate. Here we propose a consistent approach for defining and measuring the coupling strength in Coulomb and Yukawa OCPs based on a fundamental structural quantity, the radial pair distribution function (RPDF). The RPDF is often accessible in experiments by direct observation or indirectly through the static structure factor. Alternatively, it is directly computed in theoretical models or simulations. Our approach is based on the observation that the build-up of correlation from a weakly coupled system proceeds in two steps: First, a monotonically increasing volume around each particle becomes devoid of other particles (correlation hole), and second (upon further increase of the coupling), a shell structure emerges around each particle giving rise to growing peaks of the RPDF. Using molecular dynamics simulation, we present a systematic study for the dependence of these features of the RPDF on Gamma and kappa and derive a simple expression for the effective coupling parameter. (C) 2014 AIP Publishing LLC. C1 [Ott, T.; Bonitz, M.] Univ Kiel, Inst Theoret Phys & Astrophys, D-24098 Kiel, Germany. [Stanton, L. G.] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA. [Murillo, M. S.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA. RP Ott, T (reprint author), Univ Kiel, Inst Theoret Phys & Astrophys, Leibnizstr 15, D-24098 Kiel, Germany. RI Bonitz, Michael/A-6873-2010 OI Bonitz, Michael/0000-0001-7911-0656 FU Deutsche Forschungsgemeinschaft [SFB-TR 24]; North-German Supercomputing Alliance (HLRN) [shp00006] FX This work was supported by the Deutsche Forschungsgemeinschaft via SFB-TR 24 (project A7) and the North-German Supercomputing Alliance (HLRN) via Grant shp00006. NR 31 TC 19 Z9 19 U1 0 U2 13 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 1070-664X EI 1089-7674 J9 PHYS PLASMAS JI Phys. Plasmas PD NOV PY 2014 VL 21 IS 11 AR 113704 DI 10.1063/1.4900625 PG 7 WC Physics, Fluids & Plasmas SC Physics GA AU5JZ UT WOS:000345644200074 ER PT J AU Ryutov, DD Dorf, MA AF Ryutov, D. D. Dorf, M. A. TI Evolution of helical perturbations in a thin-shell model of an imploding liner SO PHYSICS OF PLASMAS LA English DT Article ID Z-PINCHES; KINK INSTABILITY; PHYSICS; LAYER AB A thin-shell model of the liner stability has been revisited and applied to the stability of the helical perturbations. Several stages of the implosion have been identified, starting from a long initial "latent" phase of an almost resting liner, continuing to the second stage of a rapid contraction and significant perturbation growth, and then transitioning to the third stage where perturbations become ballistic and highly non-linear. The stage of stagnation and rebound is beyond the scope of this paper. An importance of vorticity conservation during the late stages is emphasized. Nonlinear evolution of perturbations is followed up to the point of the formation of cusp structures. Effects of in-surface flows and of their enhancement due to the vorticity conservation are discussed. It is shown that the pre-machined perturbations created only on the outer surface of the liner grow much slower than one could anticipate. The limitations on the thin-shell description are discussed. (C) 2014 AIP Publishing LLC. C1 [Ryutov, D. D.; Dorf, M. A.] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA. RP Ryutov, DD (reprint author), Lawrence Livermore Natl Lab, Livermore, CA 94550 USA. FU U.S. Department of Energy by Lawrence Livermore National Laboratory [DE-AC52-07NA27344]; Sandia National Laboratories (Albuquerque) FX One of the authors (D.R.) is grateful to Dr. A. L. Velikovich for a valuable discussion. This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344, with support from Sandia National Laboratories (Albuquerque). NR 33 TC 6 Z9 6 U1 0 U2 6 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 1070-664X EI 1089-7674 J9 PHYS PLASMAS JI Phys. Plasmas PD NOV PY 2014 VL 21 IS 11 AR 112704 DI 10.1063/1.4901197 PG 17 WC Physics, Fluids & Plasmas SC Physics GA AU5JZ UT WOS:000345644200043 ER PT J AU Sati, P Verma, U Tripathi, VK AF Sati, Priti Verma, Updesh Tripathi, V. K. TI Self-focusing and frequency broadening of laser pulse in water SO PHYSICS OF PLASMAS LA English DT Article ID FEMTOSECOND FILAMENTS; GENERATION; PICOSECOND; BREAKDOWN; MEDIA; KERR AB An analytical model for the avalanche breakdown of water by an intense short laser pulse of finite spot size is developed. Initially, the laser undergoes self-focusing due to Kerr nonlinearity. As it acquires large intensity, it causes heating and avalanche breakdown of water. The plasma thus created on the laser axis causes nonlinear refraction induced defocusing of the laser. Thermal conduction tends to flatten the temperature profile and reduce the nonlinear refraction. The plasma density modification leads to frequency broadening of the laser. (C) 2014 AIP Publishing LLC. C1 [Sati, Priti; Tripathi, V. K.] Indian Inst Technol Delhi, Dept Phys, New Delhi 110016, India. [Verma, Updesh] Princeton Plasma Phys Lab, Princeton, NJ 08540 USA. RP Sati, P (reprint author), Indian Inst Technol Delhi, Dept Phys, New Delhi 110016, India. FU LASTEC; Government P. G. College Bilaspur; UGC [F 5-55/2013(IC)] FX The authors are grateful to Professor N. J. Fisch, PPPL, for fruitful discussion. Specially thankful to Dr. Ilya, Dr. Ammar, Dr. Peter, Dr. Wang, Dr. Rualdo, Dr. Anuraj, Dr. Arti, and Dr. Malkin for their important inputs and discussion. The authors are also thankful to LASTEC, Government P. G. College Bilaspur, and UGC (Raman Postdoctoral Fellowship No.F 5-55/2013(IC)) for financial support. NR 25 TC 2 Z9 2 U1 2 U2 9 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 1070-664X EI 1089-7674 J9 PHYS PLASMAS JI Phys. Plasmas PD NOV PY 2014 VL 21 IS 11 AR 112110 DI 10.1063/1.4901952 PG 6 WC Physics, Fluids & Plasmas SC Physics GA AU5JZ UT WOS:000345644200013 ER PT J AU Weber, SV Casey, DT Eder, DC Kilkenny, JD Pino, JE Smalyuk, VA Grim, GP Remington, BA Rowley, DP Yeamans, CB Tipton, RE Barrios, M Benedetti, R Hopkins, LB Bleuel, DL Bond, EJ Bradley, DK Caggiano, JA Callahan, DA Cerjan, CJ Clark, DS Divol, L Edgell, DH Edwards, MJ Eckart, MJ Fittinghoff, D Frenje, JA Gatu-Johnson, M Glebov, VY Glenn, S Guler, N Haan, SW Hamza, A Hatarik, R Herrmann, H Hoover, D Hsing, WW Izumi, N Jones, OS Kervin, M Khan, S Kline, J Knauer, J Kritcher, A Kyrala, G Landen, OL Le Pape, S Ma, T Mackinnon, AJ MacPhee, AG Marinak, MM Mcnaney, JM Meezan, NB Merrill, FE Mintz, M Moore, A Munro, DH Nikroo, A Pak, A Parham, T Petrasso, R Rinderknecht, HG Sayre, DB Sepke, SM Spears, BK Stoeffl, W Tommasini, R Town, RP Volegov, P Widmann, K Wilson, DC Zylstra, AB AF Weber, S. V. Casey, D. T. Eder, D. C. Kilkenny, J. D. Pino, J. E. Smalyuk, V. A. Grim, G. P. Remington, B. A. Rowley, D. P. Yeamans, C. B. Tipton, R. E. Barrios, M. Benedetti, R. Hopkins, L. Berzak Bleuel, D. L. Bond, E. J. Bradley, D. K. Caggiano, J. A. Callahan, D. A. Cerjan, C. J. Clark, D. S. Divol, L. Edgell, D. H. Edwards, M. J. Eckart, M. J. Fittinghoff, D. Frenje, J. A. Gatu-Johnson, M. Glebov, V. Y. Glenn, S. Guler, N. Haan, S. W. Hamza, A. Hatarik, R. Herrmann, H. Hoover, D. Hsing, W. W. Izumi, N. Jones, O. S. Kervin, M. Khan, S. Kline, J. Knauer, J. Kritcher, A. Kyrala, G. Landen, O. L. Le Pape, S. Ma, T. Mackinnon, A. J. MacPhee, A. G. Marinak, M. M. Mcnaney, J. M. Meezan, N. B. Merrill, F. E. Mintz, M. Moore, A. Munro, D. H. Nikroo, A. Pak, A. Parham, T. Petrasso, R. Rinderknecht, H. G. Sayre, D. B. Sepke, S. M. Spears, B. K. Stoeffl, W. Tommasini, R. Town, R. P. Volegov, P. Widmann, K. Wilson, D. C. Zylstra, A. B. TI Simulations of indirectly driven gas-filled capsules at the National Ignition Facility SO PHYSICS OF PLASMAS LA English DT Article ID RAYLEIGH-TAYLOR INSTABILITY; INERTIAL CONFINEMENT FUSION; IMPLOSIONS; GROWTH; NEUTRONS; MIX AB Gas-filled capsules imploded with indirect drive on the National Ignition Facility have been employed as symmetry surrogates for cryogenic-layered ignition capsules and to explore interfacial mix. Plastic capsules containing deuterated layers and filled with tritium gas provide a direct measure of mix of ablator into the gas fuel. Other plastic capsules have employed DT or (DHe)-He-3 gas fill. We present the results of two-dimensional simulations of gas-filled capsule implosions with known degradation sources represented as in modeling of inertial confinement fusion ignition designs; these are time-dependent drive asymmetry, the capsule support tent, roughness at material interfaces, and prescribed gas-ablator interface mix. Unlike the case of cryogenic-layered implosions, many observables of gas-filled implosions are in reasonable agreement with predictions of these simulations. Yields of TT and DT neutrons as well as other x-ray and nuclear diagnostics are matched for CD-layered implosions. Yields of DT-filled capsules are over-predicted by factors of 1.4-2, while (DHe)-He-3 capsule yields are matched, as well as other metrics for both capsule types. (C) 2014 AIP Publishing LLC. C1 [Weber, S. V.; Casey, D. T.; Eder, D. C.; Pino, J. E.; Smalyuk, V. A.; Remington, B. A.; Rowley, D. P.; Yeamans, C. B.; Tipton, R. E.; Barrios, M.; Benedetti, R.; Hopkins, L. Berzak; Bleuel, D. L.; Bond, E. J.; Bradley, D. K.; Caggiano, J. A.; Callahan, D. A.; Cerjan, C. J.; Clark, D. S.; Divol, L.; Edwards, M. J.; Eckart, M. J.; Fittinghoff, D.; Glenn, S.; Haan, S. W.; Hamza, A.; Hatarik, R.; Hsing, W. W.; Izumi, N.; Jones, O. S.; Kervin, M.; Khan, S.; Kritcher, A.; Landen, O. L.; Le Pape, S.; Ma, T.; Mackinnon, A. J.; MacPhee, A. G.; Marinak, M. M.; Mcnaney, J. M.; Meezan, N. B.; Mintz, M.; Munro, D. H.; Pak, A.; Parham, T.; Sayre, D. B.; Sepke, S. M.; Spears, B. K.; Stoeffl, W.; Tommasini, R.; Town, R. P.; Widmann, K.] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA. [Kilkenny, J. D.; Hoover, D.; Nikroo, A.] Gen Atom Co, San Diego, CA 92121 USA. [Grim, G. P.; Guler, N.; Herrmann, H.; Kline, J.; Kyrala, G.; Merrill, F. E.; Volegov, P.; Wilson, D. C.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA. [Edgell, D. H.; Glebov, V. Y.; Knauer, J.] Univ Rochester, Laser Energet Lab, Rochester, NY 14623 USA. [Frenje, J. A.; Gatu-Johnson, M.; Petrasso, R.; Rinderknecht, H. G.; Zylstra, A. B.] MIT, Cambridge, MA 02139 USA. [Moore, A.] AWE Aldermaston, Reading RG7 4PR, Berks, England. RP Weber, SV (reprint author), Lawrence Livermore Natl Lab, Livermore, CA 94550 USA. RI MacKinnon, Andrew/P-7239-2014; lepape, sebastien/J-3010-2015; IZUMI, Nobuhiko/J-8487-2016; Tommasini, Riccardo/A-8214-2009; OI MacKinnon, Andrew/0000-0002-4380-2906; IZUMI, Nobuhiko/0000-0003-1114-597X; Tommasini, Riccardo/0000-0002-1070-3565; Kline, John/0000-0002-2271-9919; Merrill, Frank/0000-0003-0603-735X; /0000-0003-4969-5571 FU U.S. Department of Energy by Lawrence Livermore National Laboratory [DE-AC52-07NA27344] FX This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract No. DE-AC52-07NA27344. NR 54 TC 3 Z9 3 U1 4 U2 33 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 1070-664X EI 1089-7674 J9 PHYS PLASMAS JI Phys. Plasmas PD NOV PY 2014 VL 21 IS 11 AR 112706 DI 10.1063/1.4901598 PG 9 WC Physics, Fluids & Plasmas SC Physics GA AU5JZ UT WOS:000345644200045 ER PT J AU Zylstra, AB Frenje, JA Seguin, FH Hicks, DG Dewald, EL Robey, HF Rygg, JR Meezan, NB Rosenberg, MJ Rinderknecht, HG Friedrich, S Bionta, R Olson, R Atherton, J Barrios, M Bell, P Benedetti, R Hopkins, LB Betti, R Bradley, D Callahan, D Casey, D Collins, G Dixit, S Doppner, T Edgell, D Edwards, MJ Johnson, MG Glenn, S Glenzer, S Grim, G Hatchett, S Jones, O Khan, S Kilkenny, J Kline, J Knauer, J Kritcher, A Kyrala, G Landen, O LePape, S Li, CK Lindl, J Ma, T Mackinnon, A Macphee, A Manuel, MJE Meyerhofer, D Moody, J Moses, E Nagel, SR Nikroo, A Pak, A Parham, T Petrasso, RD Prasad, R Ralph, J Rosen, M Ross, JS Sangster, TC Sepke, S Sinenian, N Sio, HW Spears, B Springer, P Tommasini, R Town, R Weber, S Wilson, D Zacharias, R AF Zylstra, A. B. Frenje, J. A. Seguin, F. H. Hicks, D. G. Dewald, E. L. Robey, H. F. Rygg, J. R. Meezan, N. B. Rosenberg, M. J. Rinderknecht, H. G. Friedrich, S. Bionta, R. Olson, R. Atherton, J. Barrios, M. Bell, P. Benedetti, R. Hopkins, L. Berzak Betti, R. Bradley, D. Callahan, D. Casey, D. Collins, G. Dixit, S. Doeppner, T. Edgell, D. Edwards, M. J. Johnson, M. Gatu Glenn, S. Glenzer, S. Grim, G. Hatchett, S. Jones, O. Khan, S. Kilkenny, J. Kline, J. Knauer, J. Kritcher, A. Kyrala, G. Landen, O. LePape, S. Li, C. K. Lindl, J. Ma, T. Mackinnon, A. Macphee, A. Manuel, M. J. -E. Meyerhofer, D. Moody, J. Moses, E. Nagel, S. R. Nikroo, A. Pak, A. Parham, T. Petrasso, R. D. Prasad, R. Ralph, J. Rosen, M. Ross, J. S. Sangster, T. C. Sepke, S. Sinenian, N. Sio, H. W. Spears, B. Springer, P. Tommasini, R. Town, R. Weber, S. Wilson, D. Zacharias, R. TI The effect of shock dynamics on compressibility of ignition-scale National Ignition Facility implosions SO PHYSICS OF PLASMAS LA English DT Article ID INERTIAL-CONFINEMENT-FUSION; OMEGA; PLASMAS; TARGETS; DESIGN AB The effects of shock dynamics on compressibility of indirect-drive ignition-scale surrogate implosions, CH shells filled with (DHe)-He-3 gas, have been studied using charged-particle spectroscopy. Spectral measurements of (DHe)-He-3 protons produced at the shock-bang time probe the shock dynamics and in-flight characteristics of an implosion. The proton shock yield is found to vary by over an order of magnitude. A simple model relates the observed yield to incipient hot-spot adiabat, suggesting that implosions with rapid radiation-power increase during the main drive pulse may have a 2x higher hot-spot adiabat, potentially reducing compressibility. A self-consistent 1-D implosion model was used to infer the areal density (rho R) and the shell center-of-mass radius (R-cm) from the downshift of the shock-produced (DHe)-He-3 protons. The observed rho R at shock-bang time is substantially higher for implosions, where the laser drive is on until near the compression bang time ("short-coast"), while longer-coasting implosions have lower rho R. This corresponds to a much larger temporal difference between the shock- and compression-bang time in the long-coast implosions (similar to 800 ps) than in the short-coast (similar to 400 ps); this will be verified with a future direct bang-time diagnostic. This model-inferred differential bang time contradicts radiation-hydrodynamic simulations, which predict constant 700-800 ps differential independent of coasting time; this result is potentially explained by uncertainties in modeling late-time ablation drive on the capsule. In an ignition experiment, an earlier shock-bang time resulting in an earlier onset of shell deceleration, potentially reducing compression and, thus, fuel rho R. (C) 2014 AIP Publishing LLC. C1 [Zylstra, A. B.; Frenje, J. A.; Seguin, F. H.; Rosenberg, M. J.; Rinderknecht, H. G.; Johnson, M. Gatu; Li, C. K.; Manuel, M. J. -E.; Petrasso, R. D.; Sinenian, N.; Sio, H. W.] MIT, Plasma Sci & Fus Ctr, Cambridge, MA 02139 USA. [Hicks, D. G.; Dewald, E. L.; Robey, H. F.; Rygg, J. R.; Meezan, N. B.; Friedrich, S.; Bionta, R.; Atherton, J.; Barrios, M.; Bell, P.; Benedetti, R.; Hopkins, L. Berzak; Bradley, D.; Callahan, D.; Casey, D.; Collins, G.; Dixit, S.; Doeppner, T.; Edwards, M. J.; Glenn, S.; Glenzer, S.; Hatchett, S.; Jones, O.; Khan, S.; Kritcher, A.; Landen, O.; LePape, S.; Lindl, J.; Ma, T.; Mackinnon, A.; Macphee, A.; Moody, J.; Moses, E.; Nagel, S. R.; Pak, A.; Parham, T.; Prasad, R.; Ralph, J.; Rosen, M.; Ross, J. S.; Sepke, S.; Spears, B.; Springer, P.; Tommasini, R.; Town, R.; Weber, S.; Zacharias, R.] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA. [Olson, R.] Sandia Natl Labs, Albuquerque, NM 87185 USA. [Olson, R.; Grim, G.; Kline, J.; Kyrala, G.; Wilson, D.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA. [Betti, R.; Edgell, D.; Knauer, J.; Meyerhofer, D.; Sangster, T. C.] Univ Rochester, Laser Energet Lab, Rochester, NY 14623 USA. [Kilkenny, J.; Nikroo, A.] Gen Atom Co, San Diego, CA 92186 USA. RP Zylstra, AB (reprint author), MIT, Plasma Sci & Fus Ctr, 77 Massachusetts Ave, Cambridge, MA 02139 USA. EM zylstra@mit.edu RI Hicks, Damien/B-5042-2015; MacKinnon, Andrew/P-7239-2014; lepape, sebastien/J-3010-2015; Manuel, Mario/L-3213-2015; Tommasini, Riccardo/A-8214-2009 OI Hicks, Damien/0000-0001-8322-9983; MacKinnon, Andrew/0000-0002-4380-2906; Kline, John/0000-0002-2271-9919; /0000-0003-4969-5571; Manuel, Mario/0000-0002-5834-1161; Tommasini, Riccardo/0000-0002-1070-3565 FU U.S. DoE [DE-NA0001857, DE-FC52-08NA28752]; LLNL [B597367]; LLE [415935-G]; Fusion Science Center at the University of Rochester [524431]; National Laser Users Facility [DE-NA0002035]; National Science Foundation Graduate Research Fellowship Program [1122374] FX We thank the operations crews and engineering staff at NIF for supporting these experiments, and M. McKernan, M. Cairel, and M. Valadez for their work processing the CR-39. This work is part of the first author's Ph.D. thesis, and was supported in part by the U.S. DoE (Grant Nos. DE-NA0001857 and DE-FC52-08NA28752), LLNL (No. B597367), LLE (No. 415935-G), the Fusion Science Center at the University of Rochester (No. 524431), and the National Laser Users Facility (No. DE-NA0002035). This material was based upon work supported by the National Science Foundation Graduate Research Fellowship Program under Grant No. 1122374. NR 51 TC 8 Z9 8 U1 1 U2 21 PU AMER INST PHYSICS PI MELVILLE PA CIRCULATION & FULFILLMENT DIV, 2 HUNTINGTON QUADRANGLE, STE 1 N O 1, MELVILLE, NY 11747-4501 USA SN 1070-664X EI 1089-7674 J9 PHYS PLASMAS JI Phys. Plasmas PD NOV PY 2014 VL 21 IS 11 AR 112701 DI 10.1063/1.4900621 PG 18 WC Physics, Fluids & Plasmas SC Physics GA AU5JZ UT WOS:000345644200040 ER PT J AU Wang, YC Schreiber, DK Neeway, JJ Thevuthasan, S Evans, JE Ryan, JV Zhu, ZH Wei, WD AF Wang, Yi-Chung Schreiber, Daniel K. Neeway, James J. Thevuthasan, Suntharampillai Evans, James E. Ryan, Joseph V. Zhu, Zihua Wei, Wei David TI NanoSIMS imaging alteration layers of a leached SON68 glass via a FIB-made wedged crater SO SURFACE AND INTERFACE ANALYSIS LA English DT Article; Proceedings Paper CT 19th International Conference on Secondary Ion Mass Spectrometry (SIMS) CY SEP 29-OCT 04, 2013 CL Jeju, SOUTH KOREA SP ULVAC PHI Inc, CAMECA, ION TOF GmbH DE NanoSIMS; imaging; glass; corrosion; focused ion beam ID ION MASS-SPECTROMETRY AB Currently, nuclear wastes are commonly immobilized into glasses because of their long-term durability. Exposure to water for long periods, however, will eventually corrode the waste form and is the leading potential avenue for radionuclide release into the environment. Because such slow processes cannot be experimentally tested, the prediction of release requires a thorough understanding of the mechanisms governing glass corrosion. In addition, because of the exceptional durability of glass, much of the testing must be performed on high-surface area powders. A technique that can provide accurate compositional profiles with nanometer scale depth resolution for non-flat samples would be a major benefit to the field. In this study, NanoSIMS was used to image the cross section of the corrosion layers of a leached SON68 glass sample. A wedged crater was prepared by a focused ion beam instrument to obtain a five-fold improvement in depth information for NanoSIMS measurements. This improvement allowed us to confirm that the breakdown of the silica glass network is further from the pristine glass than a second dissolution front for boron, another glass former, despite only similar to 50nm distance between them. More importantly, NanoSIMS images show that the roughness majorly exists in Si corrosion layer. This novel sample geometry will be a major benefit to efficient NanoSIMS sampling of irregular interfaces at the nanometer scale that would otherwise be obscured within time-of-flight secondary ion mass spectroscopy depth profiles. Copyright (c) 2014 John Wiley & Sons, Ltd. C1 [Wang, Yi-Chung; Thevuthasan, Suntharampillai; Evans, James E.; Zhu, Zihua] Pacific NW Natl Lab, WR Wiley Environm Mol Sci Lab, Richland, WA 99354 USA. [Schreiber, Daniel K.; Neeway, James J.; Ryan, Joseph V.] Pacific NW Natl Lab, Energy & Environm Directorate, Richland, WA 99354 USA. [Wang, Yi-Chung; Wei, Wei David] Univ Florida, Dept Chem, Gainesville, FL 32611 USA. [Wang, Yi-Chung; Wei, Wei David] Univ Florida, Ctr Nanostruct Elect Mat, Gainesville, FL 32611 USA. RP Zhu, ZH (reprint author), Pacific NW Natl Lab, WR Wiley Environm Mol Sci Lab, Richland, WA 99354 USA. EM joe.ryan@pnnl.gov; zihua.zhu@pnnl.gov; wei@chem.ufl.edu RI Zhu, Zihua/K-7652-2012; OI Neeway, Jim/0000-0001-7046-8408 NR 12 TC 1 Z9 1 U1 1 U2 13 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0142-2421 EI 1096-9918 J9 SURF INTERFACE ANAL JI Surf. Interface Anal. PD NOV PY 2014 VL 46 SU 1 SI SI BP 233 EP 237 DI 10.1002/sia.5585 PG 5 WC Chemistry, Physical SC Chemistry GA AU6EN UT WOS:000345696200058 ER PT J AU Wang, ZY Jin, K Zhang, YW Wang, FY Zhu, ZH AF Wang, Zhaoying Jin, Ke Zhang, Yanwen Wang, Fuyi Zhu, Zihua TI ToF-SIMS depth profiling of insulating samples, interlaced mode or non-interlaced mode? SO SURFACE AND INTERFACE ANALYSIS LA English DT Article; Proceedings Paper CT 19th International Conference on Secondary Ion Mass Spectrometry (SIMS) CY SEP 29-OCT 04, 2013 CL Jeju, SOUTH KOREA SP ULVAC PHI Inc, CAMECA, ION TOF GmbH DE ToF-SIMS; dual-beam depth profiling; interlaced mode; non-interlaced mode; insulator ID ION MASS-SPECTROMETRY; CLUSTER AB Dual-beam depth profiling strategy has been widely adopted in time-of-flight secondary ion mass spectrometry depth profiling, in which two basic operation modes, interlaced mode and non-interlaced mode, are commonly used. Generally, interlaced mode is recommended for conductive or semi-conductive samples, whereas non-interlaced mode is recommended for insulating samples, where charge compensation can be an issue. Recent publications, however, show that the interlaced mode can be used effectively for glass depth profiling, despite the fact that glass is an insulator. In this study, we provide a simple guide for choosing between interlaced mode and non-interlaced mode for insulator depth profiling. Two representative cases are presented: (i) depth profiling of a leached glass sample and (ii) depth profiling of a single-crystal MgO sample. In summary, the interlaced mode should be attempted first, because (i) it may provide data with reasonable quality, (ii) it is time-saving for most cases, and (iii) it introduces low H/C/O background. If data quality is the top priority and measurement time is flexible, non-interlaced mode is recommended because interlaced mode may suffer from low signal intensity and poor mass resolution. A big challenge is tracking trace H/C/O in a highly insulating sample (e.g., MgO), because non-interlaced mode may introduce strong H/C/O background, but interlaced mode may suffer from low signal intensity. Meanwhile, a C or Au coating is found to be very effective to improve the signal intensity. Surprisingly, the best analyzing location is not on the C or Au coating but at the edge (outside) of the coating. Copyright (c) 2014 John Wiley & Sons, Ltd. C1 [Wang, Zhaoying; Wang, Fuyi] Chinese Acad Sci, Inst Chem, Beijing 100190, Peoples R China. [Wang, Zhaoying; Zhu, Zihua] Pacific NW Natl Lab, WR Wiley Environm Mol Sci Lab, Richland, WA 99354 USA. [Jin, Ke; Zhang, Yanwen] Univ Tennessee, Dept Mat Sci & Engn, Knoxville, TN 37996 USA. [Zhang, Yanwen] Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37831 USA. RP Zhu, ZH (reprint author), Pacific NW Natl Lab, WR Wiley Environm Mol Sci Lab, Richland, WA 99354 USA. EM fuyi.wang@iccas.ac.cn; zihua.zhu@pnnl.gov RI Wang, Fuyi/H-9449-2014; Zhu, Zihua/K-7652-2012 OI Wang, Fuyi/0000-0003-0962-1260; NR 14 TC 3 Z9 3 U1 6 U2 25 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0142-2421 EI 1096-9918 J9 SURF INTERFACE ANAL JI Surf. Interface Anal. PD NOV PY 2014 VL 46 SU 1 SI SI BP 257 EP 260 DI 10.1002/sia.5419 PG 4 WC Chemistry, Physical SC Chemistry GA AU6EN UT WOS:000345696200064 ER PT J AU Maheshwari, P Stevie, FA Myneni, GR Ciovati, G Rigsbee, JM Dhakal, P Griffis, DP AF Maheshwari, P. Stevie, F. A. Myneni, G. R. Ciovati, G. Rigsbee, J. M. Dhakal, P. Griffis, D. P. TI SIMS analysis of high-performance accelerator niobium SO SURFACE AND INTERFACE ANALYSIS LA English DT Article; Proceedings Paper CT 19th International Conference on Secondary Ion Mass Spectrometry (SIMS) CY SEP 29-OCT 04, 2013 CL Jeju, SOUTH KOREA SP ULVAC PHI Inc, CAMECA, ION TOF GmbH DE SIMS depth profile; superconducting radio frequency; accelerator niobium ID DIFFUSION; METALS AB Niobium is used to fabricate superconducting radio frequency accelerator modules because of its high critical temperature, high critical magnetic field, and easy formability. Recent experiments have shown a very significant improvement in performance (over 100%) after a high-temperature bake at 1400 degrees C for 3h. SIMS analysis of this material showed the oxygen profile was significantly deeper than the native oxide with a shape that is indicative of diffusion. Positive secondary ion mass spectra showed the presence of Ti with a depth profile similar to that of O. It is suspected that Ti is associated with the performance improvement. The source of Ti contamination in the anneal furnace has been identified, and a new furnace was constructed without Ti. Initial results from the new furnace do not show the yield improvement. Further analyses should determine the relationship of Ti to cavity performance. Copyright (c) 2014 John Wiley & Sons, Ltd. C1 [Maheshwari, P.; Stevie, F. A.; Griffis, D. P.] N Carolina State Univ, Analyt Instrumentat Facil, Raleigh, NC 27695 USA. [Myneni, G. R.; Ciovati, G.; Dhakal, P.] Jefferson Lab, Newport News, VA 23606 USA. [Rigsbee, J. M.; Griffis, D. P.] N Carolina State Univ, Raleigh, NC 27695 USA. RP Stevie, FA (reprint author), N Carolina State Univ, Analyt Instrumentat Facil, 2410 Campus Shore Dr, Raleigh, NC 27695 USA. EM fred_stevie@ncsu.edu NR 9 TC 1 Z9 1 U1 1 U2 8 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0142-2421 EI 1096-9918 J9 SURF INTERFACE ANAL JI Surf. Interface Anal. PD NOV PY 2014 VL 46 SU 1 SI SI BP 288 EP 290 DI 10.1002/sia.5461 PG 3 WC Chemistry, Physical SC Chemistry GA AU6EN UT WOS:000345696200072 ER PT J AU Tuggle, J Giordani, A Kulkarni, N Warmack, B Hunter, J AF Tuggle, Jay Giordani, Andrew Kulkarni, Nagraj Warmack, Bruce Hunter, Jerry TI Secondary ion mass spectrometry for Mg tracer diffusion: issues and solutions SO SURFACE AND INTERFACE ANALYSIS LA English DT Article; Proceedings Paper CT 19th International Conference on Secondary Ion Mass Spectrometry (SIMS) CY SEP 29-OCT 04, 2013 CL Jeju, SOUTH KOREA SP ULVAC PHI Inc, CAMECA, ION TOF GmbH DE SIMS; Mg alloys; diffusion; annealing; tracer diffusion; self-diffusion; induced topography; Mg diffusivities; topography formation AB A secondary ion mass spectrometry (SIMS) method has been developed to measure stable Mg isotope tracer diffusion. This SIMS method was then used to calculate Mg self-diffusivities, and the data was verified against historical data measured using radiotracers. The SIMS method has been validated as a reliable alternative to the radiotracer technique for the measurement of Mg self-diffusion coefficients and can be used as a routine method for determining diffusion coefficients. Copyright (c) 2014 John Wiley & Sons, Ltd. C1 [Tuggle, Jay; Giordani, Andrew; Hunter, Jerry] Virginia Polytech Inst & State Univ, Blacksburg, VA 24061 USA. [Kulkarni, Nagraj; Warmack, Bruce] Oak Ridge Natl Lab, Oak Ridge, TN USA. RP Hunter, J (reprint author), Virginia Polytech Inst & State Univ, Blacksburg, VA 24061 USA. EM hunterje@vt.edu NR 7 TC 3 Z9 3 U1 0 U2 4 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0142-2421 EI 1096-9918 J9 SURF INTERFACE ANAL JI Surf. Interface Anal. PD NOV PY 2014 VL 46 SU 1 SI SI BP 291 EP 293 DI 10.1002/sia.5618 PG 3 WC Chemistry, Physical SC Chemistry GA AU6EN UT WOS:000345696200073 ER PT J AU Mangel, WF San Martin, C AF Mangel, Walter F. San Martin, Carmen TI Structure, Function and Dynamics in Adenovirus Maturation SO VIRUSES-BASEL LA English DT Review DE adenovirus; protease; DNA sliding; virus stability; uncoating; infectivity ID CRYOELECTRON MICROSCOPY STRUCTURE; 11-AMINO-ACID PEPTIDE COFACTOR; MULTIPLE SEQUENCE ALIGNMENT; L1 52/55-KILODALTON PROTEIN; NUCLEAR-PORE COMPLEX; VIRAL-DNA; TERMINAL PROTEIN; PRETERMINAL PROTEIN; CRYSTAL-STRUCTURE; IVA2 PROTEIN AB Here we review the current knowledge on maturation of adenovirus, a non-enveloped icosahedral eukaryotic virus. The adenovirus dsDNA genome fills the capsid in complex with a large amount of histone-like viral proteins, forming the core. Maturation involves proteolytic cleavage of several capsid and core precursor proteins by the viral protease (AVP). AVP uses a peptide cleaved from one of its targets as a "molecular sled" to slide on the viral genome and reach its substrates, in a remarkable example of one-dimensional chemistry. Immature adenovirus containing the precursor proteins lacks infectivity because of its inability to uncoat. The immature core is more compact and stable than the mature one, due to the condensing action of unprocessed core polypeptides; shell precursors underpin the vertex region and the connections between capsid and core. Maturation makes the virion metastable, priming it for stepwise uncoating by facilitating vertex release and loosening the condensed genome and its attachment to the icosahedral shell. The packaging scaffold protein L1 52/55k is also a substrate for AVP. Proteolytic processing of L1 52/55k disrupts its interactions with other virion components, providing a mechanism for its removal during maturation. Finally, possible roles for maturation of the terminal protein are discussed. C1 [Mangel, Walter F.] Brookhaven Natl Lab, Biol Environm & Climate Sci Dept, Upton, NY 11973 USA. [San Martin, Carmen] CSIC, CNB, Dept Macromol Struct, Madrid 28049, Spain. [San Martin, Carmen] CSIC, CNB, NanoBiomed Initiat, Madrid 28049, Spain. RP San Martin, C (reprint author), CSIC, CNB, Dept Macromol Struct, Darwin 3, Madrid 28049, Spain. EM mangel@bnl.gov; carmen@cnb.csic.es RI San Martin, Carmen/A-4074-2010 OI San Martin, Carmen/0000-0001-9799-175X FU National Institute of Allergy and Infectious Diseases of the National Institutes of Health [R01AI41599, R21AI113565]; Spanish Interdisciplinary Network on the Biophysics of Viruses (Biofivinet) from the Ministerio de Economia y Competitividad of Spain [FIS2011-16090-E]; [BFU2010-16382]; [BFU2013-41249-P] FX We would like to acknowledge the contributions of Joseph M. Weber of the University of Sherbrook for his early work on the AdV protease. He was the first to show that the AdV protease is both an important and an interesting enzyme, and he isolated a most useful reagent to study it, the ts1 virus. Walter F. Mangel would also like to acknowledge three invaluable colleagues: Paul Blainey, William J. McGrath, and Diana Toledo. Some of the research reported in this publication was supported by the National Institute of Allergy and Infectious Diseases of the National Institutes of Health under Awards Numbered R01AI41599 and R21AI113565, to Walter F. Mangel. The content is solely the responsibility of the authors and does not necessarily represent the official views of the National Institutes of Health. Carmen San Martin acknowledges invaluable input from past and present group members and collaborators, in particular Jane Flint (Princeton University) who provided superior ts1 preparations for many of the studies reviewed here. Work at the Carmen San Martin laboratory was funded by grants BFU2010-16382, BFU2013-41249-P, and the Spanish Interdisciplinary Network on the Biophysics of Viruses (Biofivinet, FIS2011-16090-E) from the Ministerio de Economia y Competitividad of Spain. NR 145 TC 15 Z9 16 U1 3 U2 22 PU MDPI AG PI BASEL PA POSTFACH, CH-4005 BASEL, SWITZERLAND SN 1999-4915 J9 VIRUSES-BASEL JI Viruses-Basel PD NOV PY 2014 VL 6 IS 11 BP 4536 EP 4570 DI 10.3390/v6114536 PG 35 WC Virology SC Virology GA AU4FL UT WOS:000345565200025 PM 25421887 ER PT J AU Ferry, VE Smith, JM Alivisatos, AP AF Ferry, Vivian E. Smith, Jessica M. Alivisatos, A. Paul TI Symmetry Breaking in Tetrahedral Chiral Plasmonic Nanoparticle Assemblies SO ACS PHOTONICS LA English DT Article DE plasmonics; circular dichroism; optical chirality; numerical simulation; self-assembly ID CIRCULAR-DICHROISM; DNA NANOSTRUCTURES; OPTICAL-ACTIVITY; GOLD; DIMERS; METAMOLECULES AB Self-assembled plasmonic structures combine the specificity and tunability of chemical synthesis with collective plasmonic properties. Here we systematically explore the effects of symmetry breaking on the chiroptical response of an assembly of plasmonic nanoparticles using simulation. The design is based on a tetrahedral nanoparticle frame with two different types of nanoparticles, where chirality is induced by targeted stimuli that change the distance along one edge of the assembly. We show that the intensity, spectral position, and handedness of the CD response are tunable with small structural changes, making it usable as a nanoscale plasmonic ruler. We then build upon this initial design to show that the symmetry breaking principle may also be used to design a chiral pyramid using a mixture of different nanoparticle materials, which affords tunability over a broad spectral range, and retrieves nanoscale conformational changes over a range of length scales. C1 [Ferry, Vivian E.; Alivisatos, A. Paul] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA. [Smith, Jessica M.; Alivisatos, A. Paul] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA. RP Ferry, VE (reprint author), Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Mat Sci, 1 Cyclotron Rd, Berkeley, CA 94720 USA. RI Alivisatos , Paul /N-8863-2015 OI Alivisatos , Paul /0000-0001-6895-9048 FU National Science Foundation [DMR-1344290] FX We are grateful to Mario Hentschel for useful discussions. This material is based upon work supported by the National Science Foundation under Grant DMR-1344290. NR 39 TC 12 Z9 12 U1 12 U2 87 PU AMER CHEMICAL SOC PI WASHINGTON PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA SN 2330-4022 J9 ACS PHOTONICS JI ACS Photonics PD NOV PY 2014 VL 1 IS 11 BP 1189 EP 1196 DI 10.1021/ph5002632 PG 8 WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary; Optics; Physics, Applied; Physics, Condensed Matter SC Science & Technology - Other Topics; Materials Science; Optics; Physics GA AU3WW UT WOS:000345542400014 ER EF