Dark Energy Cosmological Model in f(R,T) Theory of Gravity

Abstract

The main purpose of this paper is to study LRS Bianchi type I metric in the presence of dark energy. To obtain the solutions of the field equations we have assumed the special law of variation of Hubble's parameter(proposed by Berman)that yields constant deceleration parameter. Here we considered that the scalar expansion theta is proportional to shear scalar which leads to the condition A=B^n. Also in this paper we have discussed Some physical properties of the model.