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The STAR beam energy scan phase II physics and upgrades
Yang, C; Adamczyk, L; Adkins, JK; Agakishiev, G; Aggarwal, MM; Ahammed, Z; Alekseev, I; Aparin, A; Arkhipkin, D; Aschenauer, EC; Ashraf, MU; Attri, A; Averichev, GS; Bai, X; Bairathi, V; Bellwied, R; Bhasin, A; Bhati, AK; Bhattarai, P; Bielcik, J; Bielcikova, J; Bland, LC; Bordyuzhin, IG; Bouchet, J; Brandenburg, JD; Brandin, AV; Bunzarov, I; Butterworth, J; Caines, H; Sanchez, MCDL; Campbell, JM; Cebra, D; Chakaberia, I; Chaloupka, P; Chang, Z; Chatterjee, A; Chattopadhyay, S; Chen, X; Chen, JH; Cheng, J; Cherney, M; Christie, W; Contin, G; Crawford, HJ; Das, S; De Silva, LC; Debbe, RR; Dedovich, TG; Deng, J; Derevschikov, AA; di Ruzza, B; Didenko, L; Dilks, C; Dong, X; Drachenberg, JL; Draper, JE; Du, CM; Dunkelberger, LE; Dunlop, JC; Efimov, LG; Engelage, J; Eppley, G; Esha, R; Evdokimov, O; Eyser, O; Fatemi, R; Fazio, S; Federic, P; Fedorisin, J; Feng, Z; Filip, P; Fisyak, Y; Flores, CE; Fulek, L; Gagliardi, CA; Garand, D; Geurts, F; Gibson, A; Girard, M; Greiner, L; Grosnick, D; Gunarathne, DS; Guo, Y; Gupta, S; Gupta, A; Guryn, W; Hamad, AI; Hamed, A; Hague, R; Harris, JW; He, L; Heppelmann, S; Heppelmann, S; Hirsch, A; Hoffmann, GW; Horvat, S; Huang, T; Huang, B; Huang, X; Huang, HZ; Huck, P; Humanic, TJ; Igo, G; Jacobs, WW; Jang, H; Jentsch, A; Jia, J; Jiang, K; Judd, EG; Kabana, S; Kalinldn, D; Kang, K; Kauder, K; Ke, HW; Keane, D; Kechechyan, A; Khan, ZH; Kikola, DP; Kisel, I; Kisiel, A; Kochenda, L; Koetke, DD; Kosarzewski, LK; Kraishan, AF; Kravtsov, P; Krueger, K; Kumar, L; Lamont, MAC; Landgraf, JM; Landry, KD; Lauret, J; Lebedev, A; Lednicky, R; Lee, JH; Li, X; Li, Y; Li, C; Li, W; Li, X; Lin, T; Lisa, MA; Liu, F; Ljubicic, T; Llope, WJ; Lomnitz, M; Longacre, RS; Luo, X; Luo, S; Ma, GL; Ma, L; Me, YG; Ma, R; Magdy, N; Majka, R; Manion, A; Margetis, S; Markert, C; Matis, HS; McDonald, D; McKinzie, S; Meehan, K; Mei, JC; Miller, ZW; Minaev, NG; Mioduszewski, S; Mishra, D; Mohanty, B; Mondal, MM; Morozov, DA; Mustafa, MK; Nandi, BK; Nasim, M; Nayak, TK; Nigmatkulov, G; Niida, T; Nogach, LV; Noh, SY; Novak, J; Nurushev, SB; Odyniec, G; Ogawa, A; Oh, K; Okorokov, VA; Olvitt, D; Page, BS; Pak, R; Pan, YX; Pandit, Y; Panebratsev, Y; Pawlik, B; Pei, H; Perkins, C; Pile, P; Pluta, J; Poniatowska, K; Porter, J; Posik, M; Poskanzer, AM; Pruthi, NK; Przybycien, M; Putschke, J; Qiu, H; Quintero, A; Ramachandran, S; Ray, RL; Reed, R; Ritter, HG; Roberts, JB; Rogachevskiy, OV; Romero, JL; Ruan, L; Rusnak, J; Rusnakova, O; Sahoo, NR; Sahu, PK; Sakrejda, I; Salur, S; Sandweiss, J; Sarkar, A; Schambach, J; Scharenberg, RP; Schmah, AM; Schmidke, WB; Schmitz, N; Seger, J; Seyboth, P; Shah, N; Shahaliev, E; Shanmuganathan, PV; Shao, M; Sharma, A; Sharma, B; Sharma, MK; Shen, WQ; Shi, Z; Shi, SS; Shou, QY; Sichtermann, EP; Sikora, R; Simko, M; Singha, S; Skoby, MJ; Smirnov, D; Smirnov, N; Solyst, W; Song, L; Sorensen, P; Spinka, HM; Srivastava, B; Stanislaus, TDS; Stepanov, M; Stock, R; Strikhanov, M; Stringfellow, B; Sumbera, M; Summa, B; Sun, Y; Sun, Z; Sun, XM; Surrow, B; Svirida, DN; Tang, Z; Tang, AH; Tarnowsky, T; Tawfik, A; Thader, J; Thomas, JH; Timmins, AR; Tlusty, D; Todoroki, T; Tokarev, M; Trentalange, S; Tribble, RE; Tribedy, P; Tripathy, SK; Tsai, OD; Ullrich, T; Underwood, DG; Upsal, I; Van Buren, G; van Nieuwenhuizen, G; Vandenbroucke, M; Varma, R; Vasiliev, AN; Vertesi, R; Videaek, F; Vokal, S; Voloshin, SA; Vossen, A; Wang, H; Wang, F; Wang, Y; Wang, JS; Wang, G; Wang, Y; Webb, JC; Webb, G; Wen, L; Westfall, GD; Wieman, H; Wissink, SW; Witt, R; Wu, Y; Xiao, ZG; Xie, W; Xie, G; Xin, K; Xu, N; Xu, QH; Xu, Z; Xu, J; Xu, H; Xu, YF; Yang, S; Yang, Y; Yang, C; Yang, Y; Yang, Y; Yang, Q; Ye, Z; Ye, Z; Yi, L; Yip, K; Yoo, IK; Yu, N; Zbroszczyk, H; Zha, W; Zhang, Z; Zhang, JB; Zhang, S; Zhang, S; Zhang, XP; Zhang, Y; Zhang, J; Zhang, J; Zhao, J; Zhong, C; Zhou, L; Zhu, X; Zoulkarneeva, Y; Zyzak, M
2017
Source PublicationNUCLEAR PHYSICS A
ISSN0375-9474
Volume967Issue:-Pages:800-803
Subtype期刊论文
AbstractThe second phase of the Beam Energy Scan at RHIC, BPS-II, is scheduled for 2019-2020 and will explore with precision measurements the high baryon density region of the QCD phase diagram. The program will examine the energy region of interest determined from the results of BES-I. Some of the key measurements anticipated are: the net-protons kurtosis that could pinpoint the position of a critical point, the directed flow that might prove a softening of the EOS, and the chiral restoration in the dilepton channel. The measurements will be possible with the order of magnitude better statistics provided by the electron cooling upgrade of RHIC and with the detector upgrades planned to extend STAR's experimental reach. The upgrades are: the inner TPC sectors (iTPC), the Event Plane Detector (EPD), and the end -cap TOF (eTOF). We present the BES-II program details and the physics opportunities enabled by these upgrades.
DOI10.1016/j.nuclphysa.2017.05.042
Indexed BySCI
Language英语
WOS IDWOS:000413384100168
Citation statistics
Cited Times:9[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.sinap.ac.cn/handle/331007/28871
Collection中科院上海应用物理研究所2011-2019年
Recommended Citation
GB/T 7714
Yang, C,Adamczyk, L,Adkins, JK,et al. The STAR beam energy scan phase II physics and upgrades[J]. NUCLEAR PHYSICS A,2017,967(-):800-803.
APA Yang, C.,Adamczyk, L.,Adkins, JK.,Agakishiev, G.,Aggarwal, MM.,...&Zyzak, M.(2017).The STAR beam energy scan phase II physics and upgrades.NUCLEAR PHYSICS A,967(-),800-803.
MLA Yang, C,et al."The STAR beam energy scan phase II physics and upgrades".NUCLEAR PHYSICS A 967.-(2017):800-803.
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