| Energy dependence of J/Psi production in Au plus Au collisions at root S-NN=39, 62.4 and 200 GeV |
| Adamczyk, L; Adkins, JK; Agakishiev, G; Aggarwal, MM; Ahammed, Z; Ajitanand, NN; Alekseev, I; Anderson, DM; Aoyama, R; Aparin, A; Arkhipkin, D; Aschenauer, EC; Ashraf, MU; Attri, A; Averichev, GS; Bai, X; Bairathi, V; Behera, A; Bellwied, R; Bhasin, A; Bhati, AK; Bhattarai, P; Bielcik, J; Bielcikova, J; Bland, LC; Bordyuzhin, IG; Bouchet, J; Brandenburg, JD; Brandin, AV; Brown, D; Bunzarov, I; Butterworth, J; Caines, H; Sanchez, MCD; Campbell, JM; Cebra, D; Chakaberia, I; Chaloupka, P; Chang, Z; Chankova-Bunzarova, N; Chatterjee, A; Chattopadhyay, S; Chen, X; Chen, JH; Chen, X; Cheng, J; Cherney, M; Christie, W; Contin, G; Crawford, HJ; Das, S; De Silva, LC; Debbe, RR; Dedovich, TG; Deng, J; Derevschikov, AA; Didenko, L; Dilks, C; Dong, X; Drachenberg, JL; Draper, JE; Dunkelberger, LE; Dunlop, JC; Efimov, LG; Elsey, N; Engelage, J; Eppley, G; Esha, R; Esumi, S; Evdokimov, O; Ewigleben, J; Eyser, O; Fatemi, R; Fazio, S; Federic, P; Federicova, P; Fedorisin, J; Feng, Z; Filip, P; Finch, E; Fisyak, Y; Flores, CE; Fujita, J; Fulek, L; Gagliardi, CA; Garand, D; Geurtsa, F; Gibson, A; Girard, M; Grosnick, D; Gunarathne, DS; Guo, Y; Gupta, A; Gupta, S; Guryn, W; Hamad, AI; Hamed, A; Harlenderova, A; Harris, JW; He, L; Heppelmann, S; Heppelmann, S; Hirsch, A; Hoffmann, GW; Horvat, S; Huang, B; Huang, HZ; Huang, T; Huang, X; Humanic, TJ; Hou, P; Igo, G; Jacobs, WW; Jentsch, A; Jia, J; Jiang, K; Jowzaee, S; Judd, EG; Kabana, S; Kalinkin, D; Kang, K; Kauder, K; Ke, HW; Keane, D; Kechechyan, A; Khan, Z; Kikola, DP; Kisel, I; Kisiel, A; Kochenda, L; Kocmanek, M; Kollegger, T; Kosarzewski, LK; Kraishan, AF; Kravtsov, P; Krueger, K; Kulathunga, N; Kumar, L; Kvapil, J; Kwasizur, JH; Lacey, R; Landgraf, JM; Landry, KD; Lauret, J; Lebedev, A; Lednicky, R; Lee, JH; Li, Y; Li, X; Li, W; Li, C; Lidrych, J; Lin, T; Lisa, MA; Liu, Y; Liu, H; Liu, F; Liu, P; Ljubicic, T; Llope, WJ; Lomnitz, M; Longacre, RS; Luo, S; Luo, X; Ma, GL; Ma, L; Ma, YG; Ma, R; Magdy, N; Majka, R; Mallick, D; Margetis, S; Markert, C; Matis, HS; Meehan, K; Mei, JC; Miller, ZW; Minaev, NG; Mioduszewski, S; Mishra, D; Mizuno, S; Mohanty, B; Mondal, MM; Morozov, DA; Mustafa, MK; Nasim, M; Nayak, TK; Nelson, JM; Nie, M; Nigmatkulov, G; Niida, T; Nogach, LV; Nonaka, T; Nurushev, SB; Odyniec, G; Ogawa, A; Oh, K; Okorokov, VA; Olvitt, D; Page, BS; Pak, R; Pandit, Y; Panebratsev, Y; Pawlik, B; Pei, H; Perkins, C; Pile, P; Pluta, J; Poniatowska, K; Porter, J; Posik, M; Pruthi, NK; Przybycien, M; Putschke, J; Qiu, H; Quintero, A; Ramachandran, S; Ray, RL; Reed, R; Rehbein, MJ; Ritter, HG; Roberts, JB; Rogachevskiy, OV; Romero, JL; Roth, JD; Ruan, L; Rusnak, J; Rusnakovat, O; Sahoo, NR; Sahu, PK; Salur, S; Sandweiss, J; Saur, M; Schambach, J; Schmah, AM; Schmidke, WB; Schmitz, N; Schweid, BR; Seger, J; Sergeeva, M; Seyboth, R; Shah, N; Shahaliev, E; Shanmuganathan, PV; Shao, M; Sharma, A; Sharma, MK; Shen, WQ; Shi, SS; Shi, Z; Shou, QY; Sichtermann, EP; Sikora, R; Simko, M; Singha, S; Skoby, MJ; Smirnov, N; Smirnov, D; Solyst, W; Song, L; Sorensen, R; Spinka, HM; Srivastava, B; Stanislaus, TDS; Strikhanov, M; Stringfellow, B; Sugiura, T; Sumbera, M; Summa, B; Sun, X; Sun, Y; Sun, XM; Surrow, B; Svirida, DN; Tang, AH; Tang, Z; Taranenko, A; Tarnowsky, T; Tawfik, A; Thader, J; Thomas, JH; Timmins, AR; Tlusty, D; Todoroki, T; Tokarev, M; Trentalange, S; Tribble, RE; Tribedy, R; Tripathy, SK; Trzeciak, BA; Tsai, OD; Ullrich, T; Underwood, DG; Upsal, I; Van Buren, G; van Nieuwenhuizen, G; Vasiliev, AN; Videbaek, F; Vokal, S; Voloshin, SA; Vossen, A; Wang, G; Wang, Y; Wang, F; Wang, Y; Webb, JC; Webb, G; Wen, L; Westfall, GD; Wieman, H; Wissink, SW; Witt, R; Wu, Y; Xiao, ZG; Xie, W; Xie, G; Xu, J; Xu, N; Xu, QH; Xu, YF; Xu, Z; Yang, Y; Yang, Q; Yang, C; Yang, S; Ye, Z; Ye, Z; Yi, L; Yip, K; Yoo, IK; Yu, N; Zbroszczyk, H; Zha, W; Zhang, Z; Zhang, XP; Zhang, JB; Zhang, S; Zhang, J; Zhang, Y; Zhang, J; Zhang, S; Zhao, J; Zhong, C; Zhou, L; Zhou, C; Zhu, X; Zhu, Z; Zyzak, M
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| 2017
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Source Publication | PHYSICS LETTERS B
 |
ISSN | 0370-2693
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Volume | 771Issue:-Pages:13-20 |
Subtype | 期刊论文
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Abstract | The inclusive J/Psi transverse momentum spectra and nuclear modification factors are reported at midrapidity (|y| < 1.0) in Au + Au collisions at root S-NN = 39, 62.4 and 200 GeV taken by the STAR experiment. A suppression of J/Psi production, with respect to the production in p + p scaled by the number of binary nucleon-nucleon collisions, is observed in central Au + Au collisions at these three energies. No significant energy dependence of nuclear modification factors is found within uncertainties. The measured nuclear modification factors can be described by model calculations that take into account both suppression of direct J/Psi production due to the color screening effect and J/Psi regeneration from recombination of uncorrelated charm-anticharm quark pairs. (C) 2017 The Author. Published by Elsevier B.V. |
Keyword | Quark-gluon Plasma
Pb-pb Collisions
Proton-nucleus Collisions
Charmonium Production
Transverse-momentum
Psi Production
Drell-yan
Cern-sps
Suppression
Collaboration
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DOI | 10.1016/j.physletb.2017.04.078
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Indexed By | SCI
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WOS Keyword | QUARK-GLUON PLASMA
; PB-PB COLLISIONS
; PROTON-NUCLEUS COLLISIONS
; CHARMONIUM PRODUCTION
; TRANSVERSE-MOMENTUM
; PSI PRODUCTION
; DRELL-YAN
; CERN-SPS
; SUPPRESSION
; COLLABORATION
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Language | 英语
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WOS ID | WOS:000406183300004
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Citation statistics |
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Document Type | 期刊论文
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Identifier | http://ir.sinap.ac.cn/handle/331007/28640
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Collection | 中科院上海应用物理研究所2011-2020年
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Recommended Citation GB/T 7714 |
Adamczyk, L,Adkins, JK,Agakishiev, G,et al. Energy dependence of J/Psi production in Au plus Au collisions at root S-NN=39, 62.4 and 200 GeV[J]. PHYSICS LETTERS B,2017,771(-):13-20.
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APA |
Adamczyk, L.,Adkins, JK.,Agakishiev, G.,Aggarwal, MM.,Ahammed, Z.,...&Zyzak, M.(2017).Energy dependence of J/Psi production in Au plus Au collisions at root S-NN=39, 62.4 and 200 GeV.PHYSICS LETTERS B,771(-),13-20.
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MLA |
Adamczyk, L,et al."Energy dependence of J/Psi production in Au plus Au collisions at root S-NN=39, 62.4 and 200 GeV".PHYSICS LETTERS B 771.-(2017):13-20.
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