Study of physical parameters of the cosmological models of the universe in plane symmetric space-time in modified gravity

Abstract

In this paper, we have intended to study the dynamics of the anisotropic universe in modified gravity using the functional f(R,T) in the form f(R,T) = λR + λT . The cosmological models are constructed using the volumetric exponen- tial expansion in Bianchi type V Ih (BV Ih) universe for three different values of h = −1, 0, 1. The physical behaviors of the models are also studied.