Effect of Electromagnetism upon the Collapse of Cylindrical Symmetric Stars in f(R; T) Gravity

TL;DR

This paper investigates how electromagnetic effects influence the stability and evolution of charged, cylindrically symmetric stars within f(R; T) gravity, revealing that charge increases stellar instability.

Contribution

It introduces a detailed analysis of charged stellar stability in f(R; T) gravity using perturbation methods and the adiabatic index, highlighting the destabilizing role of charge.

Findings

Charge enhances stellar instability.

Stability conditions differ between Newtonian and post-Newtonian regimes.

Electromagnetic effects are significant in stellar evolution within modified gravity.

Abstract

By the end of the evaluation of this research artifact, readers would be able to describe the effect of conducted plasma on evolution of stellar objects. In this script, we have analyzed the stability of charged cylindrically symmetric stellar objects in the context of f(R; T) theory of gravity. We have fabricated field equations and their conforming dynamical equations and then we have used perturbation scheme for additional analysis. Adiabatic index {\Gamma} has been used to sort inequalities in the Newtonian and the post Newtonian regimes. At the end we caught some extra limitations due to which we have concluded that effect of charge on star upsurges its instability