English

Beam-energy and collision-system dependence of the linear and mode-coupled flow harmonics from STAR

Nuclear Experiment 2020-12-18 v1

Abstract

Recent measurements and hydrodynamic model calculations suggest that the higher-order flow coefficients v4v_{4} and v5v_{5} have two contributions: a linear contribution driven by the initial-state eccentricities, εn\varepsilon_{n}, and a mode-coupled contribution derived from the lower-order eccentricity coefficients ε2\varepsilon_{2} and ε3\varepsilon_{3}. Measurements of these two contributions to v4v_{4} and v5v_{5} provide crucial insights to discern initial-state models and to constrain the temperature-dependent specific shear viscosity, η/s\eta/s, of the plasma produced in heavy-ion collisions. In this work, we have employed the two-subevents cumulant technique to provide the first beam-energy and collision-system dependence of the linear and mode-coupled contributions to the higher-order flow harmonics. Our results are shown and discussed for several centrality intervals for U+U collisions at sNN\mathrm{\sqrt{s_{NN}}}= 193 GeV, Au+Au collisions at sNN\mathrm{\sqrt{s_{NN}}}=200, and 54.4 GeV and Cu+Au collisions at sNN\mathrm{\sqrt{s_{NN}}}=200 GeV. The results are compared with similar studies performed by the ALICE experiment at LHC.

Keywords

Cite

@article{arxiv.2002.08223,
  title  = {Beam-energy and collision-system dependence of the linear and mode-coupled flow harmonics from STAR},
  author = {Niseem Magdy},
  journal= {arXiv preprint arXiv:2002.08223},
  year   = {2020}
}