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Shusu SHI. Collective Flow of Identified Particles in Heavy Ion Collisions at RHIC-STAR[J]. Nuclear Physics Review, 2020, 37(3): 668-673. DOI: 10.11804/NuclPhysRev.37.2019CNPC72
Citation: Shusu SHI. Collective Flow of Identified Particles in Heavy Ion Collisions at RHIC-STAR[J]. Nuclear Physics Review, 2020, 37(3): 668-673. DOI: 10.11804/NuclPhysRev.37.2019CNPC72

Collective Flow of Identified Particles in Heavy Ion Collisions at RHIC-STAR

Funds: National Natural Science Foundation of China (11890711); Self-determined Research Funds of CCNU from the Colleges Basic Research and Operation of MOE (CCNU20TS009)
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  • Received Date: March 19, 2020
  • Revised Date: June 09, 2020
  • In this paper, we review the recent key results on anisotropic flow in heavy ion collisions at RHIC-STAR experiment. It mainly includes the results of elliptic flow of multi-strange and charm hadrons in top energy heavy ion collisions, and the results of elliptic and directed flow from RHIC Beam Energy Scan Program I. The results of 54.4 and 27 GeV are brand-new. We find the new results of directed flow follow the energy dependence trend; the Number of Constituent Quark scaling of elliptic flow indicates the partonic collectivity has been built-up in Au+Au collisions at 54.4 and 27 GeV. We also introduce the future plans of Beam Energy Scan experiments and the research focus of the anisotropic flow.
  • [1]
    RHISCHKE D. Heavy Ion Physics, 1995, 1: 309.
    [2]
    STOCKER H. Nucl Phys A, 2005, 750: 121. DOI: 10.1016/j.nuclphysa.2004.12.074
    [3]
    HE L, EDMONDS T, LIN Z W, et al. Phys Lett B, 2016, 753: 506. DOI: 10.1016/j.physletb.2015.12.051
    [4]
    POSKANZER A, VOLOSHIN S. Phys Rev C, 1998, 58: 1671. DOI: 10.1103/PhysRevC.58.1671
    [5]
    VOLOSHIN S, POSKANZER A, SNELLINGS R. 2008, arXiv: 0809.2949.
    [6]
    ADAMCZYK L, ADKINS J K, AGAKISHIEV G, et al (STAR Collaboration). Phys Rev Lett, 2016, 116: 062301. DOI: 10.1103/PhysRevLett.116.062301
    [7]
    ADAMCZYK L, ADKINS J K, AGAKISHIEV G, et al (STAR Collaboration). Phys Rev Lett, 2017, 118: 212301. DOI: 10.1103/PhysRevLett.118.212301
    [8]
    ADAMCZYK L, ADKINS J K, AGAKISHIEV G, et al (STAR Collaboration). Phys Rev Lett, 2014, 112: 162301. DOI: 10.1103/PhysRevLett.112.162301
    [9]
    ADAMCZYK L, ADAMS J R, ADKINS J K, et al(STAR Collaboration). Phys Rev Lett, 2018, 120: 062301. DOI: 10.1103/PhysRevLett.120.062301
    [10]
    NAYAK K(for the STAR collaboration). 2020, arXiv: 2002.12066.
    [11]
    ADAMCZYK L, AGAKISHIEV G, AGGARWAL M M, et al (STAR Collaboration). Phys Rev C, 2012, 86: 054908. DOI: 10.1103/PhysRevC.86.054908
    [12]
    ADAMCZYK L, ADKINS J K, AGAKISHIEV G, et al (STAR Collaboration). Phys Rev Lett, 2013, 110: 142301. DOI: 10.1103/PhysRevLett.110.142301
    [13]
    ADAMCZYK L, ADKINS J K, AGAKISHIEV G, et al (STAR Collaboration). Phys Rev C, 2013, 88: 014902. DOI: 10.1103/PhysRevC.88.014902
    [14]
    ADAMCZYK L, ADKINS J K, AGAKISHIEV G, et al (STAR Collaboration). Phys Rev C, 2016, 93: 014907. DOI: 10.1103/PhysRevC.93.014907
    [15]
    STEINHEIMER J, KOCH V, BLEICHE M, et al. Phys Rev C, 2012, 86: 044903. DOI: 10.1103/PhysRevC.86.044903
    [16]
    XU J, SONG T, KO C M. Phys Rev Lett, 2014, 112: 012301. DOI: 10.1103/PhysRevLett.112.012301
    [17]
    LIU H, WANG F T, SUN K J, et al. Phys Lett B, 2019, 798: 135002. DOI: 10.1016/j.physletb.2019.135002
    [18]
    HATTA Y, MONNAI A, XIAO B W. Phys Rev D, 2015, 92: 114010. DOI: 10.1103/PhysRevD.92.114010
    [19]
    LUO X F, SHI S S, XU N, et al. Particles, 2020, 3: 278. DOI: 10.3390/particles3020022
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