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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
2017
Source PublicationPHYSICS LETTERS B
ISSN0370-2693
Volume771Issue:-Pages:13-20
Subtype期刊论文
AbstractThe 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.
KeywordQuark-gluon Plasma Pb-pb Collisions Proton-nucleus Collisions Charmonium Production Transverse-momentum Psi Production Drell-yan Cern-sps Suppression Collaboration
DOI10.1016/j.physletb.2017.04.078
Indexed BySCI
WOS KeywordQUARK-GLUON PLASMA ; PB-PB COLLISIONS ; PROTON-NUCLEUS COLLISIONS ; CHARMONIUM PRODUCTION ; TRANSVERSE-MOMENTUM ; PSI PRODUCTION ; DRELL-YAN ; CERN-SPS ; SUPPRESSION ; COLLABORATION
Language英语
WOS IDWOS:000406183300004
Citation statistics
Cited Times:11[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.sinap.ac.cn/handle/331007/28640
Collection中科院上海应用物理研究所2011-2019年
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.
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.
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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