Equation of state and transport coefficients of relativistic nuclear matter

被引：1
|
作者：
Muronga, Azwinndini [1 ,2 ]
机构：
[1] Univ Cape Town, Dept Phys, Ctr Theoret Phys & Astrophys, ZA-7701 Cape Town, South Africa
[2] Univ Cape Town, Dept Phys, CERN Res Ctr, UCT, ZA-7701 Cape Town, South Africa
来源：
JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS | 2008年 / 35卷 / 04期
关键词：
D O I：
10.1088/0954-3899/35/4/044073
中图分类号：
O57 [原子核物理学、高能物理学];
学科分类号：
070202 ;
摘要：
In order to evaluate qualitatively the spacetime evolution of hot and dense nuclear matter the underlying equation of state and transport coefficients must be known. In this study, a specific equation of state is studied: the pion gas. The classical or standard transport coefficients, namely the bulk viscosity, shear viscosity and thermal conductivity are divided by the relaxation times for the corresponding dissipative fluxes and then studied as a function of mass to temperature ratio.
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页数：5
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