A New Class of Anisotropic Charged Compact Star

TL;DR

This paper introduces a novel model for charged compact stars by solving Einstein-Maxwell equations, providing explicit expressions for physical parameters and comparing charged and uncharged cases through graphical analysis.

Contribution

It presents a new analytical model for charged compact stars with well-behaved parameters, expanding understanding of their internal structure.

Findings

Parameters are in closed form and physically consistent.

Charged and uncharged models are compared graphically.

The model enhances understanding of anisotropic charged stellar objects.

Abstract

A new model of charged compact star is reported by solving the Einstein-Maxwell field equations by choosing a suitable form of radial pressure. The model parameters $\rho$, $p_r$, $p_{\perp}$ and $E^{2}$ are in closed form and all are well behaved inside the stellar interior. A comparative study of charged and uncharged model is done with the help of graphical analysis.