Anisotropic tilted cosmological model in f(R,T) theory of gravity

An anisotropic Tilted Marder's Cosmological Model is investigated in the framework of f(R, T) theory of gravity, where R is the Ricci scalar and T is the trace of stress energy momentum tensor. Here we study the class of f(R, T) = R + 2f(T). To decipher the solutions of field equations, we used a power law relation between metric potentials proposed by Thorne (1967) and the special law of variation of Hubble's parameter proposed by Berman (1983) which yields constant deceleration parameter. The solution of field equations represent an expanding model of the Universe. The physical behavior and energy conditions of the model are discussed with the help of some physical parameters.