Modeling compact stars in f(T) gravity: Insights from modified chaplygin gas and MIT bag equations of state

Abstract

The consequences of [Formula: see text] gravity for neutron stars, strange stars, and compact stars are examined in this work. The pressure of the compact star for linear [Formula: see text] theory and a few viable nonlinear [Formula: see text] theories, including (i) exponential [Formula: see text] theory, (ii) logarithmic [Formula: see text] theory, and (iii) combined [Formula: see text] theory, was numerically derived. First, we reported a reconstruction scheme for [Formula: see text] gravity in the presence of a quintessence field. First, we have assessed the compact star density distribution for the MIT bag model and modified Chaplygin gas (MCG) backgrounds. It is important to note that we do not attempt a detailed treatment of hadronic matter EoS, which is required for realistic modeling of neutron stars. Instead, our analysis focuses on strange star configurations, which is required within the MIT bag model and generalized fluid descriptions using the MCG background. We have examined the energy conditions and the EoS parameter of the previously described [Formula: see text] theories to verify the stability and behavioral pattern of our model.