Charged Compact Stars in $f(\mathcal{G})$ Gravity

TL;DR

This paper explores the internal structure and physical properties of charged compact stars within the framework of $f( ext{Gauss-Bonnet})$ gravity, analyzing stability, anisotropy, and charge distribution through specific models.

Contribution

It applies $f( ext{Gauss-Bonnet})$ gravity to model charged anisotropic stars, extending previous solutions and analyzing their physical viability and stability.

Findings

Charged stars can be modeled consistently in $f( ext{Gauss-Bonnet})$ gravity.

Physical properties like density, stresses, and charge distribution are physically viable.

Models satisfy energy conditions and exhibit stable configurations.

Abstract

This work is devoted to investigate some of the interior configuration of static anisotropic spherical stellar charged structures in the regime of $f(\mathcal{G})$ gravity, where $\mathcal{G}$ is the Gauss Bonnet invariant. The structure of particular charged stars is analyzed with the help of solution obtained by Krori and Barua under different viable models in $f(\mathcal{G})$ gravity theory. The behavior of some physical aspects is investigated with the help of plots and the viability of our modeling is analyzed through different energy conditions. We have also studied some behavior of these realistic charged compact stars and discuss some aspects like density variation, evolution of stresses, different forces, stability of these stars, measure of anisotropy, equation of state parameters and the distribution of charges.