Instability ranges of collapsing star through adiabatic index in f(T, Θ) theory of gravity

Abstract

The main purpose of this paper is to study the stability analysis of collapsing star in the scenario of Newtonian and post Newtonian approximations. We consider the cylindrical symmetry of collapsing object which is filled with anisotropic fluid. The f(T, Θ) theory of gravity, where T is the torsion scalar and Θ is the trace of energy-momentum tensor is taken into account. The dynamical field equations are constructed which help to derive collapse equation by applying the perturbation method. The stability behavior of collapsing star is defined in both Newtonian and post Newtonian approximations with the help of an adiabatic index.