All spherically symmetric charged anisotropic solutions for compact star

TL;DR

This paper develops a comprehensive algorithm to generate physically realistic spherically symmetric charged anisotropic solutions for compact stars, demonstrating their relevance to strange star models through detailed physical property analysis.

Contribution

Introduces a new solution-generating algorithm using a novel source function for charged anisotropic fluids, applicable to modeling compact stars including strange stars.

Findings

Models are consistent with observed mass-radius data.

Solutions satisfy energy conditions and stability criteria.

Models exhibit realistic charge content and surface redshift.

Abstract

In the present paper we develop an algorithm for all spherically symmetric anisotropic charged fluid distribution. Considering a new source function $\nu(r)$ we find out a set of solutions which is physically well behaved and represent compact stellar models. A detailed study specifically shows that the models actually correspond to strange stars in terms of their mass and radius. In this connection we investigate about several physical properties like energy conditions, stability, mass-radius ratio, electric charge content, anisotropic nature and surface redshift through graphical plots and mathematical calculations. All the features from these studies are in excellent agreement with the already available evidences in theory as well as observations.