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
发表期刊NUCLEAR PHYSICS A
ISSN0375-9474
卷号967期号:-页码:800-803
文章类型期刊论文
摘要The 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
收录类别SCI
语种英语
WOS记录号WOS:000413384100168
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被引频次:3[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.sinap.ac.cn/handle/331007/28871
专题中科院上海应用物理研究所2011-2018年
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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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