# Behaviour of Charged Collapsing Fluids after Hydrostatic Equilibrium in R^n Gravity

## TL;DR

This paper investigates the behavior of charged, dissipative collapsing fluids in R^n gravity, focusing on thermodynamical variables and their influence on the evolution of relativistic star models.

## Contribution

It introduces a coupling of transport and Maxwell equations within R^n gravity using Muller-Israel-Stewart theory, analyzing thermodynamics in collapsing star scenarios.

## Key findings

- Thermal conductivity and heat flux are affected by relaxation time.
- Thermodynamical variables influence collapse dynamics.
- Coupling of Maxwell and transport equations impacts star evolution.

## Abstract

The purpose of this paper is to study the transport equation and its coupling with 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 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.