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Production of bb¯ at forward rapidity in p+p collisions at s=510GeV

U. Acharya20, A. Adare11, C. Aidala42, N. N. Ajitanand60,*, Y. Akiba55,56,†, R. Akimoto10, M. Alfred23, N. Apadula28,61, Y. Aramaki55 et al. (PHENIX Collaboration)

Y. Aramaki55, H. Asano35,55, E. T. Atomssa61, T. C. Awes51, B. Azmoun7, V. Babintsev24, M. Bai6, N. S. Bandara41, B. Bannier61, K. N. Barish8, S. Bathe5,56, A. Bazilevsky7, M. Beaumier8, S. Beckman11, R. Belmont11,42,49, A. Berdnikov58, Y. Berdnikov58, L. Bichon65, D. Black8, B. Blankenship65, J. S. Bok48, V. Borisov58, K. Boyle56, M. L. Brooks38, J. Bryslawskyj5,8, H. Buesching7, V. Bumazhnov24, S. Campbell12,28, V. Canoa Roman61, C.-H. Chen56, C. Y. Chi12, M. Chiu7, I. J. Choi25,*, J. B. Choi30, T. Chujo64, Z. Citron66, M. Connors20, M. Csanád15, T. Csörgő67, A. Datta47, M. S. Daugherity1, G. David7,61, K. DeBlasio47, K. Dehmelt61, A. Denisov24, A. Deshpande56,61, E. J. Desmond7, L. Ding28, A. Dion61, J. H. Do68, A. Drees61, K. A. Drees6, J. M. Durham38, A. Durum24, A. Enokizono55,57, H. En’yo55, R. Esha61, S. Esumi64, B. Fadem43, W. Fan61, N. Feege61, D. E. Fields47, M. Finger9, M. Finger, Jr.9, D. Firak14, D. Fitzgerald42, S. L. Fokin34, J. E. Frantz50, A. Franz7, A. D. Frawley19, C. Gal61, P. Gallus13, P. Garg3,61, H. Ge61, F. Giordano25, A. Glenn37, Y. Goto55,56, N. Grau2, S. V. Greene65, M. Grosse Perdekamp25, Y. Gu60, T. Gunji10, H. Guragain20, T. Hachiya45,55,56, J. S. Haggerty7, K. I. Hahn17, H. Hamagaki10, S. Y. Han17,33, J. Hanks61, S. Hasegawa29, X. He20, T. K. Hemmick61, J. C. Hill28, A. Hodges20, R. S. Hollis8, K. Homma22, B. Hong33, T. Hoshino22, J. Huang7,38, S. Huang65, Y. Ikeda55, K. Imai29, Y. Imazu55, M. Inaba64, A. Iordanova8, D. Isenhower1, D. Ivanishchev53, B. V. Jacak61, S. J. Jeon44, M. Jezghani20, Z. Ji61, J. Jia7,60, X. Jiang38, B. M. Johnson7,20, E. Joo33, K. S. Joo44, D. Jouan52, D. S. Jumper25, J. H. Kang68, J. S. Kang21, D. Kawall41, A. V. Kazantsev34, J. A. Key47, V. Khachatryan61, A. Khanzadeev53, A. Khatiwada38, K. Kihara64, C. Kim33, D. H. Kim17, D. J. Kim31, E.-J. Kim30, H.-J. Kim68, M. Kim59, Y. K. Kim21, D. Kincses15, E. Kistenev7, J. Klatsky19, D. Kleinjan8, P. Kline61, T. Koblesky11, M. Kofarago15,67, J. Koster56, D. Kotov53,58, B. Kurgyis15, K. Kurita57, M. Kurosawa55,56, Y. Kwon68, R. Lacey60, J. G. Lajoie28, D. Larionova58, M. Larionova58, A. Lebedev28, K. B. Lee38, S. H. Lee28,42,61, M. J. Leitch38, M. Leitgab25, N. A. Lewis42, X. Li38, S. H. Lim11,54,68, M. X. Liu38, S. Lökös15, D. Lynch7, T. Majoros14, Y. I. Makdisi6, M. Makek66,69, A. Manion61, V. I. Manko34, E. Mannel7, M. McCumber38, P. L. McGaughey38, D. McGlinchey11,38, C. McKinney25, A. Meles48, M. Mendoza8, B. Meredith12, W. J. Metzger16, Y. Miake64, A. C. Mignerey40, A. J. Miller1, A. Milov66, D. K. Mishra4, J. T. Mitchell7, Iu. Mitrankov58, S. Miyasaka55,63, S. Mizuno55,64, P. Montuenga25, T. Moon33,68, D. P. Morrison7, S. I. Morrow65, T. V. Moukhanova34, B. Mulilo33,55, T. Murakami35,55, J. Murata55,57, A. Mwai60, S. Nagamiya32,55, J. L. Nagle11, M. I. Nagy15, I. Nakagawa55,56, H. Nakagomi55,64, K. Nakano55,63, C. Nattrass62, S. Nelson18, P. K. Netrakanti4, M. Nihashi22,55, T. Niida64, R. Nouicer7,56, N. Novitzky31,61,64, A. S. Nyanin34, E. O’Brien7, C. A. Ogilvie28, J. D. Orjuela Koop11, J. D. Osborn42,51, A. Oskarsson39, K. Ozawa32,64, R. Pak7, V. Pantuev26, V. Papavassiliou48, S. Park59,61, S. F. Pate48, L. Patel20, M. Patel28, J.-C. Peng25, W. Peng65, D. V. Perepelitsa7,11,12, G. D. N. Perera48, D. Yu. Peressounko34, C. E. PerezLara61, J. Perry28, R. Petti7,61, C. Pinkenburg7, R. Pinson1, R. P. Pisani7, M. Potekhin7, A. Pun48,50, M. L. Purschke7, P. V. Radzevich58, J. Rak31, N. Ramasubramanian61, I. Ravinovich66, K. F. Read51,62, D. Reynolds60, V. Riabov46,53, Y. Riabov53,58, D. Richford5, T. Rinn25,28, N. Riveli50, D. Roach65, S. D. Rolnick8, M. Rosati28, Z. Rowan5, J. G. Rubin42, J. Runchey28, N. Saito32, T. Sakaguchi7, H. Sako29, V. Samsonov46,53, M. Sarsour20, S. Sato29, S. Sawada32, B. Schaefer65, B. K. Schmoll62, K. Sedgwick8, J. Seele56, R. Seidl55,56, A. Sen28,62, R. Seto8, P. Sett4, A. Sexton40, D. Sharma61, I. Shein24, T.-A. Shibata55,63, K. Shigaki22, M. Shimomura28,45, P. Shukla4, A. Sickles7,25, C. L. Silva38, D. Silvermyr39,51, B. K. Singh3, C. P. Singh3, V. Singh3, M. Slunečka9, K. L. Smith19, R. A. Soltz37, W. E. Sondheim38, S. P. Sorensen62, I. V. Sourikova7, P. W. Stankus51, M. Stepanov41,*, S. P. Stoll7, T. Sugitate22, A. Sukhanov7, T. Sumita55, J. Sun61, X. Sun20, Z. Sun14, J. Sziklai67, A. Takahara10, A. Taketani55,56, K. Tanida29,56,59, M. J. Tannenbaum7, S. Tarafdar65,66, A. Taranenko46,60, A. Timilsina28, T. Todoroki55,56,64, M. Tomášek13, H. Torii10, M. Towell1, R. Towell1, R. S. Towell1, I. Tserruya66, Y. Ueda22, B. Ujvari14, H. W. van Hecke38, M. Vargyas15,67, J. Velkovska65, M. Virius13, V. Vrba13,27, E. Vznuzdaev53, X. R. Wang48,56, D. Watanabe22, Y. Watanabe55,56, Y. S. Watanabe10,32, F. Wei48, S. Whitaker28, S. Wolin25, C. P. Wong20,38, C. L. Woody7, Y. Wu8, M. Wysocki51, B. Xia50, Q. Xu65, L. Xue20, S. Yalcin61, Y. L. Yamaguchi10,61, A. Yanovich24, I. Yoon59, I. Younus36, I. E. Yushmanov34, W. A. Zajc12, A. Zelenski6, Y. Zhai28, S. Zharko58, and L. Zou8 (PHENIX Collaboration)

  • 1Abilene Christian University, Abilene, Texas 79699, USA
  • 2Department of Physics, Augustana University, Sioux Falls, South Dakota 57197, USA
  • 3Department of Physics, Banaras Hindu University, Varanasi 221005, India
  • 4Bhabha Atomic Research Centre, Bombay 400 085, India
  • 5Baruch College, City University of New York, New York, New York 10010, USA
  • 6Collider-Accelerator Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
  • 7Physics Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
  • 8University of California-Riverside, Riverside, California 92521, USA
  • 9Charles University, Ovocný trh 5, Praha 1, 116 36, Prague, Czech Republic
  • 10Center for Nuclear Study, Graduate School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033, Japan
  • 11University of Colorado, Boulder, Colorado 80309, USA
  • 12Columbia University, New York, New York 10027 and Nevis Laboratories, Irvington, New York 10533, USA
  • 13Czech Technical University, Zikova 4, 166 36 Prague 6, Czech Republic
  • 14Debrecen University, H-4010 Debrecen, Egyetem tér 1, Hungary
  • 15ELTE, Eötvös Loránd University, H-1117 Budapest, Pázmány P. s. 1/A, Hungary
  • 16Eszterházy Károly University, Károly Róbert Campus, H-3200 Gyöngyös, Mátrai út 36, Hungary
  • 17Ewha Womans University, Seoul 120-750, Korea
  • 18Florida A&M University, Tallahassee, Florida 32307, USA
  • 19Florida State University, Tallahassee, Florida 32306, USA
  • 20Georgia State University, Atlanta, Georgia 30303, USA
  • 21Hanyang University, Seoul 133-792, Korea
  • 22Hiroshima University, Kagamiyama, Higashi-Hiroshima 739-8526, Japan
  • 23Department of Physics and Astronomy, Howard University, Washington, DC 20059, USA
  • 24IHEP Protvino, State Research Center of Russian Federation, Institute for High Energy Physics, Protvino, 142281, Russia
  • 25University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA
  • 26Institute for Nuclear Research of the Russian Academy of Sciences, prospekt 60-letiya Oktyabrya 7a, Moscow 117312, Russia
  • 27Institute of Physics, Academy of Sciences of the Czech Republic, Na Slovance 2, 182 21 Prague 8, Czech Republic
  • 28Iowa State University, Ames, Iowa 50011, USA
  • 29Advanced Science Research Center, Japan Atomic Energy Agency, 2-4 Shirakata Shirane, Tokai-mura, Naka-gun, Ibaraki-ken 319-1195, Japan
  • 30Jeonbuk National University, Jeonju, 54896, Korea
  • 31Helsinki Institute of Physics and University of Jyväskylä, P.O.Box 35, FI-40014 Jyväskylä, Finland
  • 32KEK, High Energy Accelerator Research Organization, Tsukuba, Ibaraki 305-0801, Japan
  • 33Korea University, Seoul 02841, Korea
  • 34National Research Center “Kurchatov Institute”, Moscow 123098, Russia
  • 35Kyoto University, Kyoto 606-8502, Japan
  • 36Physics Department, Lahore University of Management Sciences, Lahore 54792, Pakistan
  • 37Lawrence Livermore National Laboratory, Livermore, California 94550, USA
  • 38Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
  • 39Department of Physics, Lund University, Box 118, SE-221 00 Lund, Sweden
  • 40University of Maryland, College Park, Maryland 20742, USA
  • 41Department of Physics, University of Massachusetts, Amherst, Massachusetts 01003-9337, USA
  • 42Department of Physics, University of Michigan, Ann Arbor, Michigan 48109-1040, USA
  • 43Muhlenberg College, Allentown, Pennsylvania 18104-5586, USA
  • 44Myongji University, Yongin, Kyonggido 449-728, Korea
  • 45Nara Women’s University, Kita-uoya Nishi-machi Nara 630-8506, Japan
  • 46National Research Nuclear University, MEPhI, Moscow Engineering Physics Institute, Moscow 115409, Russia
  • 47University of New Mexico, Albuquerque, New Mexico 87131, USA
  • 48New Mexico State University, Las Cruces, New Mexico 88003, USA
  • 49Physics and Astronomy Department, University of North Carolina at Greensboro, Greensboro, North Carolina 27412, USA
  • 50Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701, USA
  • 51Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
  • 52IPN-Orsay, Univ. Paris-Sud, CNRS/IN2P3, Université Paris-Saclay, BP1, F-91406, Orsay, France
  • 53PNPI, Petersburg Nuclear Physics Institute, Gatchina, Leningrad region, 188300, Russia
  • 54Pusan National University, Pusan 46241, Korea
  • 55RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan
  • 56RIKEN BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973-5000, USA
  • 57Physics Department, Rikkyo University, 3-34-1 Nishi-Ikebukuro, Toshima, Tokyo 171-8501, Japan
  • 58Saint Petersburg State Polytechnic University, St. Petersburg, 195251 Russia
  • 59Department of Physics and Astronomy, Seoul National University, Seoul 151-742, Korea
  • 60Chemistry Department, Stony Brook University, SUNY, Stony Brook, New York 11794-3400, USA
  • 61Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, New York 11794-3800, USA
  • 62University of Tennessee, Knoxville, Tennessee 37996, USA
  • 63Department of Physics, Tokyo Institute of Technology, Oh-okayama, Meguro, Tokyo 152-8551, Japan
  • 64Tomonaga Center for the History of the Universe, University of Tsukuba, Tsukuba, Ibaraki 305, Japan
  • 65Vanderbilt University, Nashville, Tennessee 37235, USA
  • 66Weizmann Institute, Rehovot 76100, Israel
  • 67Institute for Particle and Nuclear Physics, Wigner Research Centre for Physics, Hungarian Academy of Sciences (Wigner RCP, RMKI) H-1525 Budapest 114, P.O. Box 49, Budapest, Hungary
  • 68Yonsei University, IPAP, Seoul 120-749, Korea
  • 69Department of Physics, Faculty of Science, University of Zagreb, Bijenička c. 32 HR-10002 Zagreb, Croatia

  • *Deceased.
  • akiba@rcf.rhic.bnl.gov

Phys. Rev. D 102, 092002 – Published 10 November, 2020

DOI: https://doi.org/10.1103/PhysRevD.102.092002

Abstract

The cross section of bottom quark-antiquark (bb¯) production in p+p collisions at s=510GeV is measured with the PHENIX detector at the Relativistic Heavy Ion Collider. The results are based on the yield of high mass, like-sign muon pairs measured within the PHENIX muon arm acceptance (1.2<|y|<2.2). The bb¯ signal is extracted from like-sign dimuons by utilizing the unique properties of neutral B meson oscillation. We report a differential cross section of dσbb¯μ±μ±/dy=0.16±0.01(stat)±0.02(syst)±0.02(global)nb for like-sign muons in the rapidity and pT ranges 1.2<|y|<2.2 and pT>1GeV/c, and dimuon mass of 510GeV/c2. The extrapolated total cross section at this energy for bb¯ production is 13.1±0.6(stat)±1.5(syst)±2.7(global)μb. The total cross section is compared to a perturbative quantum chromodynamics calculation and is consistent within uncertainties. The azimuthal opening angle between muon pairs from bb¯ decays and their pT distributions are compared to distributions generated using ps pythia6, which includes next-to-leading order processes. The azimuthal correlations and pair pT distribution are not very well described by pythia calculations, but are still consistent within uncertainties. Flavor creation and flavor excitation subprocesses are favored over gluon splitting.

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