Behaviour of charged collapsing fluids after hydrostatic equilibrium in Rn gravity

被引：0
|
作者：
Kausar, Hafiza Rizwana [1 ]
机构：
[1] Univ Cent Punjab, UCP Business Sch, Ctr Applicable Math & Stat, Fac Management Studies, Lahore, Pakistan
来源：
EUROPEAN PHYSICAL JOURNAL C | 2017年 / 77卷 / 06期
关键词：
TRANSIENT RELATIVISTIC THERMODYNAMICS; GRAVITATIONAL COLLAPSE; ROTATION CURVES; ENERGY;
D O I：
10.1140/epjc/s10052-017-4929-z
中图分类号：
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号：
摘要：
The purpose of this paper is to study the transport equation and its coupling with the Maxwell equation in the framework of R-n gravity. Using Muller-Israel-Stewart theory for the conduction of dissipative fluids, we analyze the temperature, heat flux, viscosity and thermal conductivity in the scenario of relaxation time. All these thermodynamical variables appear in the form of a single factor whose influence is discussed on the evolution of relativistic model for the heat conducting collapsing star.
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页数：7
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