Interacting LRS Bianchi Type-I Cosmological Model in f(R, T) Gravity with Modified Chaplygin Gas

Abstract

The present study deals with spatially homogeneous LRS Bianchi type – I cosmological model in f(R, T) gravity with modified Chaplygin gas. To get the deterministic models of the Universe, we have used a power law between the metric potentials of the Universe. All the models obtained and presented here are expanding, non-rotating and accelerating. Also some important features of the models including look-back time, distance modulus and luminosity distance versus red shift with their significances are discussed.