"LRS Bianchi Type I Cosmological Model with Late Time Acceleration"

A new class of spatially homogeneous and anisomorpic LRS binachi type-I cosmological model in f (R, T ) theory gravity. To solve Einstein field equation in f (R, T ) gravity, by taking f (R, T ) = R + 2f (T ) and Hubble param- eter H is a suitable function of cosmic time t which yields model is tranensition phase. The physical and kinematical parameters of the models are discussed. The models are found to be compatible with the result of recent observations.