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| Content Provider | World Health Organization (WHO)-Global Index Medicus |
|---|---|
| Author | Adare, A. Aidala, C. Ajitanand, N. N. Akiba, Y. Al-Bataineh, H. Alexander, J. Alfred, M. Angerami, A. Aoki, K. Apadula, N. Aramaki, Y. Asano, H. Atomssa, E. T. Averbeck, R. Awes, T. C. Azmoun, B. Babintsev, V. Bai, M. Baksay, G. Baksay, L. Bandara, N. S. Bannier, B. Barish, K. N. Bassalleck, B. Basye, A. T. Bathe, S. Baublis, V. Baumann, C. Bazilevsky, A. Beaumier, M. Beckman, S. Belikov, S. Belmont, R. Bennett, R. Berdnikov, A. Berdnikov, Y. Bhom, J. H. Blau, D. S. Bok, J. S. Boyle, K. Brooks, M. L. Bryslawskyj, J. Buesching, H. Bumazhnov, V. Bunce, G. Butsyk, S. Campbell, S. Caringi, A. Chen, C-H Chi, C. Y. |
| Organization | PHENIX Collaboration |
| Description | Country affiliation: United States Author Affiliation: Adare A ( University of Colorado, Boulder, Colorado 80309, USA.); Aidala C ( Department of Physics, University of Massachusetts, Amherst, Massachusetts 01003-9337, USA.); Ajitanand NN ( Department of Physics, University of Michigan, Ann Arbor, Michigan 48109-1040, USA.); Akiba Y ( Chemistry Department, Stony Brook University, SUNY, Stony Brook, New York 11794-3400, USA.); Al-Bataineh H ( RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan.); Alexander J ( RIKEN BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973-5000, USA.); Alfred M ( New Mexico State University, Las Cruces, New Mexico 88003, USA.); Angerami A ( Chemistry Department, Stony Brook University, SUNY, Stony Brook, New York 11794-3400, USA.); Aoki K ( Department of Physics and Astronomy, Howard University, Washington, DC 20059, USA.); Apadula N ( Columbia University, New York, New York 10027 and Nevis Laboratories, Irvington, New York 10533, USA.); Aramaki Y ( KEK, High Energy Accelerator Research Organization, Tsukuba, Ibaraki 305-0801, Japan.); Asano H ( Kyoto University, Kyoto 606-8502, Japan.); Atomssa ET ( RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan.); Averbeck R ( Iowa State University, Ames, Iowa 50011, USA.); Awes TC ( Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA.); Azmoun B ( Center for Nuclear Study, Graduate School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033, Japan.); Babintsev V ( RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan.); Bai M ( Kyoto University, Kyoto 606-8502, Japan.); Baksay G ( RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan.); Baksay L ( Laboratoire Leprince-Ringuet, Ecole Polytechnique, CNRS-IN2P3, Route de Saclay, F-91128, Palaiseau, France.); Bandara NS ( Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA.); Bannier B ( Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA.); Barish KN ( Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA.); Bassalleck B ( IHEP Protvino, State Research Center of Russian Federation, Institute for High Energy Physics, Protvino, 142281, Russia.); Basye AT ( Collider-Accelerator Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA.); Bathe S ( Florida Institute of Technology, Melbourne, Florida 32901, USA.); Baublis V ( Florida Institute of Technology, Melbourne, Florida 32901, USA.); Baumann C ( Department of Physics, University of Massachusetts, Amherst, Massachusetts 01003-9337, USA.); Bazilevsky A ( Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA.); Beaumier M ( University of California-Riverside, Riverside, California 92521, USA.); Beckman S ( University of New Mexico, Albuquerque, New Mexico 87131, USA.); Belikov S ( Abilene Christian University, Abilene, Texas 79699, USA.); Belmont R ( Baruch College, City University of New York, New York, New York 10010, USA.); Bennett R ( University of California-Riverside, Riverside, California 92521, USA.); Berdnikov A ( RIKEN BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973-5000, USA.); Berdnikov Y ( PNPI, Petersburg Nuclear Physics Institute, Gatchina, Leningrad region, 188300, Russia.); Bhom JH ( Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA.); Blau DS ( Institut für Kernphysik, University of Muenster, D-48149 Muenster, Germany.); Bok JS ( Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA.); Boyle K ( University of California-Riverside, Riverside, California 92521, USA.); Brooks ML ( University of Colorado, Boulder, Colorado 80309, USA.); Bryslawskyj J ( Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA.); Buesching H ( University of Colorado, Boulder, Colorado 80309, USA.); Bumazhnov V ( Department of Physics, University of Michigan, Ann Arbor, Michigan 48109-1040, USA.); Bunce G ( Vanderbilt University, Nashville, Tennessee 37235, USA.); Butsyk S ( Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA.); Campbell S ( Saint Petersburg State Polytechnic University, St. Petersburg, 195251 Russia.); Caringi A ( Saint Petersburg State Polytechnic University, St. Petersburg, 195251 Russia.); Chen CH ( Yonsei University, IPAP, Seoul 120-749, Korea.); Chi CY ( National Research Center 'Kurchatov Institute,' Moscow, 123098 Russia.) |
| Abstract | Jet production rates are measured in $ p + p $ and $ d + Au $ collisions at $ s _{ N N } = 200 GeV $ recorded in 2008 with the PHENIX detector at the Relativistic Heavy Ion Collider. Jets are reconstructed using the $ R = 0.3 $ anti- $ k _{ t } $ algorithm from energy deposits in the electromagnetic calorimeter and charged tracks in multiwire proportional chambers, and the jet transverse momentum ( $ p _{ T } $ ) spectra are corrected for the detector response. Spectra are reported for jets with $ 12 < p _{ T } < 50 GeV / c $ , within a pseudorapidity acceptance of $ | η | < 0.3 $ . The nuclear-modification factor ( $ R _{ d Au } $ ) values for 0%–100% $ d + Au $ events are found to be consistent with unity, constraining the role of initial state effects on jet production. However, the centrality-selected $ R _{ d Au } $ values and central-to-peripheral ratios ( $ R _{ CP } $ ) show large, $ p _{ T } $ -dependent deviations from unity, challenging the conventional models that relate hard-process rates and soft-particle production in collisions involving nuclei. |
| File Format | HTM / HTML |
| ISSN | 00319007 |
| e-ISSN | 10797114 |
| Journal | Physical Review Letters |
| Issue Number | 12 |
| Volume Number | 116 |
| Language | English |
| Publisher | American Physical Society |
| Publisher Date | 2016-03-25 |
| Publisher Place | United States |
| Access Restriction | Open |
| Subject Keyword | Physics |
| Content Type | Text |
| Resource Type | Article |
| Subject | Physics and Astronomy |
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