Higher Dimensional Bianchi V Models in f (R,T) Theory with Perfect Fluid Distribution

In this paper we have studied five-dimensional Bianchi type-V spacetime in the f (R,T) theory. To solve Einstein’s field equations, we have assumed that the Hubble parameter is inversely proportional toݎ ℎݐ power of the scale factor alpha i.e. H alpha 1/alphar. We have obtained a singular model for r >0, non-singular model for r=0. The physical behavior of the models has also been discussed using some physical parameters.