Modeling Compact Stars in f ( T ) Gravity: Insights from Modified Chaplygin Gas and MIT Bag Equations of State

The consequences of f(T) gravity for neutron stars, strange stars, and compact stars are examined in this work. The pressure of the compact star for linear f(T) theory and a few viable non-linear f(T) theories, including (i) exponential f(T) theory, (ii) logarithmic f(T) theory, and (iii) combined f(T) theory, was numerically derived. First, we reported a reconstruction scheme for f(T) gravity in the presence of a quintessence field. Firstly, 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 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 f(T) theories to verify the stability and behavioral pattern of our model.