Pre-equilibrium dynamics and heavy-ion observables

preprint2016arXivOpen access

Abstract

To bracket the importance of the pre-equilibrium stage on relativistic heavy-ion collision observables, we compare simulations where it is modeled by either free-streaming partons or fluid dynamics. These cases implement the assumptions of extremely weak vs. extremely strong coupling in the initial collision stage. Accounting for flow generated in the pre-equilibrium stage, we study the sensitivity of radial, elliptic and triangular flow on the switching time when the hydrodynamic description becomes valid. Using the hybrid code iEBE-VISHNU we perform a multi-parameter search, constrained by particle ratios, integrated elliptic and triangular charged hadron flow, the mean transverse momenta of pions, kaons and protons, and the second moment ⟨pT2⟩\langle p_T^2\rangle of the proton transverse momentum spectrum, to identify optimized values for the switching time τsτ_s from pre-equilibrium to hydrodynamics, the specific shear viscosity η/sη/s, the normalization factor of the temperature-dependent specific bulk viscosity (ζ/s)(T)(ζ/s)(T), and the switching temperature TswT_\mathrm{sw} from viscous hydrodynamics to the hadron cascade UrQMD. With the optimized parameters, we predict and compare with experiment the pTp_T-distributions of ππ, KK, pp, ΛΛ, ΞΞ and ΩΩ yields and their elliptic flow coefficients, focusing specifically on the mass-ordering of the elliptic flow for protons and Lambda hyperons which is incorrectly described by VISHNU without pre-equilibrium flow.

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