A SIMPLE FAMILY OF SOLUTIONS OF RELATIVISTIC VISCOUS HYDRODYNAMICS FOR FIREBALLS WITH HUBBLE FLOW AND ELLIPSOIDAL SYMMETRY

M. Csanád, M. Nagy, Z. F. Jiang, T. Csorgo
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引用次数: 2

Abstract

New, analytic solutions of relativistic viscous hydrodynamics are presented, describing expanding fireballs with Hubble-like velocity profile and ellipsoidal symmetry, similar to fireballs created in heavy ion collisions. We find that with these specifications, one obtains solutions where the shear viscosity essentially does not influence the time evolution of the system, thus these solutions are particularly adept tools to study the effect of bulk viscosity alone, which always results in a slower decrease of energy density as well as temperature compared to the case of perfect fluid. We investigate different scenarios for the bulk viscosity and find qualitatively different effects on the time evolution which suggests that there is a possibility to infer the value of bulk viscosity from energy density and temperature measurements in high-energy heavy-ion collisions.
具有哈勃流和椭球对称的火球的相对论粘性流体动力学的一个简单解族
提出了相对论粘性流体动力学的新解析解,描述了膨胀火球具有类似于哈勃的速度分布和椭球对称,类似于重离子碰撞产生的火球。我们发现,通过这些规范,我们可以得到剪切粘度基本上不影响系统时间演化的解,因此这些解是研究单独体粘度影响的特别有效的工具,与完美流体的情况相比,体粘度总是导致能量密度和温度的下降速度较慢。我们研究了不同情况下的体粘度,并发现了质性上不同的对时间演化的影响,这表明有可能从高能重离子碰撞中的能量密度和温度测量来推断体粘度的值。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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