English

Energy dependence of longitudinal flow decorrelation from STAR

Nuclear Experiment 2021-02-03 v1

Abstract

Measurements of longitudinal flow decorrelations for charged particles are presented in the pseudorapidity range η<1|\eta| < 1 using a reference detector at 2.1 <ηref<< |\eta_{\mathrm{ref}}| < 5.1 in Au+Au collisions at sNN\sqrt{s_{NN}} = 27 GeV by STAR. The flow decorrelation for v2v_2 shows a strong centrality dependence, while a weak centrality dependence for v3v_3. Results are compared with the results in Au+Au collisions at 200 GeV as a function of η\eta scaled by beam-rapidity, i.e. η/ybeam\eta/y_{beam}. No energy dependence is observed for v2v_2 decorrelation, but clear energy dependence for v3v_3 decorrelation. These results provide new insights into the longitudinal structure of the initial-state geometry in heavy-ion collisions.

Keywords

Cite

@article{arxiv.2005.03252,
  title  = {Energy dependence of longitudinal flow decorrelation from STAR},
  author = {Maowu Nie},
  journal= {arXiv preprint arXiv:2005.03252},
  year   = {2021}
}