Behaviour of Charged Collapsing Fluids after Hydrostatic Equilibrium in Rn Gravity
Abstract
The purpose of this paper is to study the transport equation and its coupling with Maxwell equation in the framework of Rn 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 are appeared 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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