Effects of friction on the chiral symmetry restoration in high energy heavy-ion collisions
M. Ishihara, F.Takagi

TL;DR
This paper investigates how friction influences the duration and characteristics of chiral symmetry restoration in high energy heavy-ion collisions using a linear sigma model with various friction types, revealing conditions for prolonged symmetry restoration.
Contribution
It introduces a detailed numerical study of friction effects on chiral symmetry restoration, highlighting the importance of friction strength and temperature thresholds in heavy-ion collision dynamics.
Findings
Chiral symmetry restoration duration depends on friction strength and initial temperature.
Maximum temperature must be at least 230 MeV for significant symmetry restoration.
Entropy production due to friction occurs mainly during early cooling stages.
Abstract
We study the effects of friction on the chiral symmetry restoration which may take place temporarily in high energy heavy ion collisions. The equations of motion with friction are introduced to describe the time evolution of the chiral condensates within the framework of the linear model. Four types of friction are used to study how the result is sensitive to the choice of the friction. For the thermalization stage, the time dependent temperature is parameterized so as to simulate the result of the parton-cascade model. It is parameterized according to the one dimensional scaling hydrodynamics for the subsequent cooling stage. The time development of the condensates and the entropy production due to friction are calculated numerically. The time interval in which the chiral symmetry is restored approximately is investigated in detail for four types of friction. It is found that;…
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