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 i.e.
H 1/r. 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.