Hydrodynamic simulations of directed flow for light hadrons in Au+Au and isobar collisions sNN= 200 GeV
Abstract
Using a (3+1)-D hydrodynamic model CLVisc, we study the directed flow (v1) of light hadrons produced in Au+Au, Ru+Ru and Zr+Zr collisions at sNN= 200 GeV. The evolution of tilted energy density, pressure gradient and radial flow along the x-direction are systematically investigated. Counter-clockwise tilt of initial fireball is shown to be a vital source of the directed flow for final light hadrons. A good description of directed flow is provided for light hadrons in central and mid-central Au+Au and isobar collisions at RHIC. Our numerical results show a clear system size dependence for light hadron v1 across different collision systems. We further study the effect of nuclear structure on the directed flow and find that the v1 for light hadrons is insensitive to the nuclei with quadrupole deformation.
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