Anisotropic Quintessence Strange Stars in f(T) Gravity with Modified Chaplygin Gas

TL;DR

This paper investigates the properties and stability of anisotropic strange stars within f(T) gravity, incorporating modified Chaplygin gas, and compares theoretical predictions with observational data.

Contribution

It introduces a new model of strange stars in f(T) gravity with anisotropic matter and modified Chaplygin gas, deriving physical quantities and matching conditions for observational consistency.

Findings

Derived equations of motion in f(T) gravity for anisotropic strange stars.

Calculated physical quantities like mass and redshift for the model.

Compared theoretical results with observational data for validation.

Abstract

In this paper, we study the existence of strange star in the background of f (T) modified gravity where T is a scalar torsion. In KB metric space, we derive the equations of motion using anisotropic property within the spherically strange star with modified chaplygin gas in the framework of modified f (T) gravity. Then we obtain many physical quantities to describe the physical status such as anisotropic behavior, energy conditions and stability. By the matching condition, we calculate the unknown parameters to evaluate the numerical values of mass, surface redshift etc. from our model to make comparison with the observational data.