Light nuclei collectivity from sNN=3 GeV Au+Au collisions at RHIC

STAR Collaboration

研究成果: Article同行評審

26 引文 斯高帕斯(Scopus)

摘要

In high-energy heavy-ion collisions, partonic collectivity is evidenced by the constituent quark number scaling of elliptic flow anisotropy for identified hadrons. A breaking of this scaling and dominance of baryonic interactions is found for identified hadron collective flow measurements in sNN = 3 GeV Au+Au collisions. In this paper, we report measurements of the first- and second-order azimuthal anisotropic parameters, v1 and v2, of light nuclei (d, t, 3He, 4He) produced in sNN = 3 GeV Au+Au collisions at the STAR experiment. An atomic mass number scaling is found in the measured v1 slopes of light nuclei at mid-rapidity. For the measured v2 magnitude, a strong rapidity dependence is observed. Unlike v2 at higher collision energies, the v2 values at mid-rapidity for all light nuclei are negative and no scaling is observed with the atomic mass number. Calculations by the Jet AA Microscopic Transport Model (JAM), with baryonic mean-field plus nucleon coalescence, are in good agreement with our observations, implying baryonic interactions dominate the collective dynamics in 3 GeV Au+Au collisions at RHIC.

原文English
文章編號136941
期刊Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
827
DOIs
出版狀態Published - 2022 4月 10

All Science Journal Classification (ASJC) codes

  • 核能與高能物理

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