LRS Bianchi Type-I Cosmological Model with Late Time Acceleration

Abstract

A new class of spatially homogeneous and anisomorpic LRS binachi type-I cosmological model in f(R, T) theory gravity. To solve Einstein field equation in f(R, T) gravity, by taking f(R, T) = R+ 2f(T) and Hubble parameter H is a suitable function of cosmic time t which yields model is tranensition phase. The physical and kinematical parameters of the models are discussed. The models are found to be compatible with the result of recent observations.
Keywords: LRS Binachi type-I,Hubble parameter H, anisotropy.