Dynamics of tilted Bianchi type-III cosmological model in f(R, T) gravity

Tilted Bianchi type-III cosmological model filled with perfect fluid is investigated in 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 + 2 f ( T ) . To decipher the solutions of field equations, we used time power-law form of a metric potential C , i.e. C = t m , where m is a positive constant, which yields constant deceleration parameter. The solution of field equations represent an expanding model of the Universe. The physical behavior of the model are discussed by using some physical parameters.