A spatially homogeneous anisotropic LRS Bianchi type-I cosmological model is
studied in f(R,T) gravity with a special form of Hubble's parameter, which
leads to constant deceleration parameter. The parameters involved in the
considered form of Hubble parameter can be tuned to match, our models with the
ΛCDM model. With the present observed value of the deceleration
parameter, we have discussed physical and kinematical properties of a specific
model. Moreover, we have discussed the cosmological distances for our model.Comment: Published versio