Strange Stars in $f(T)$ Gravity With MIT Bag Model

TL;DR

This study explores the existence and properties of strange stars within $f(T)$ gravity, using the MIT bag model and specific metric assumptions, analyzing their stability, regularity, and observational features.

Contribution

It introduces a new model of strange stars in $f(T)$ gravity with charged anisotropic matter, incorporating the MIT bag model and parametric metric functions.

Findings

Model satisfies energy conditions and stability criteria.

Derived relations connect star properties with observational data.

Analyzed surface redshift and anisotropy for the stellar configurations.

Abstract

This paper deals with existence of strange stars in $f\left(T\right) $ modified gravity. For this purpose, we have taken the diagonal tetrad field of static spacetime with charged anisotropic fluid and MIT bag model, which provide the linear relation between radial pressure and density of the matter. Further, the analysis of the resulting equations have been done by assuming the parametric form of the metric functions in term of the radial profiles with some unknown constant (introduced by Krori and Barua). By the matching of two metrices, unknown constant of the metric functions appear in terms of mass, radius and charge of the stars, the observed values of these quantities have been used for the detail analysis of the the derived model. We have discuss the regularity, anisotropy, energy conditions, stability and surface redshift of the model.