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Study on Anisotropic Strange Stars in f(T,T) Gravity
Version 1
: Received: 26 August 2020 / Approved: 31 August 2020 / Online: 31 August 2020 (10:43:38 CEST)
A peer-reviewed article of this Preprint also exists.
Salako, I.G.; Khlopov, M.; Ray, S.; Arouko, M.; Saha, P.; Debnath, U. Study on Anisotropic Strange Stars in
Abstract
In this work, we study the existence of strange star in the background of f(T,T) gravity in the Einstein spacetime geometry, where T is the torsion tensor and T is the trace of the energy-momentum tensor. The equations of motion are derived for anisotropic pressure within the spherically symmetric strange star. We explore the physical features like energy conditions, mass-radius relations, modified TOV equations, principal of causality, adiabatic index, redshift and stability analysis of our model. These features are realistic and appealing to further investigation of properties of compact objects in f(T,T) gravity as well as their observational signatures.
Keywords
general relativity; alternative gravity; compact stars; anisotropic fluid
Subject
Physical Sciences, Particle and Field Physics
Copyright: This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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