Abstract
This paper investigates the outcomes of polytropic matter distribution with a gravitational source in f(T) gravity, where f(T) is torsion scalar’s arbitrary function. We study the influence of f(T) gravity on the distribution of energy between fluids in the interior of a stellar object using polytropic equation of state. We provide a comprehensive framework for determining generic relativistic polytropes by means of minimal geometric decoupling strategy. A few physical characteristics of polytropes with perfect fluids, like effective pressure, energy exchange, polytropic index, thermal properties, etc using Tolman IV solution are noticed.
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