“…Here we confine ourselves to model LRS Bianchi-I whose spatial sections are flat but the expansion or contraction rate are direction dependent. For studying the possible effects of anisotropy in the early Universe based on the present day observations many researchers [22,23,24,25,26,27,28] have investigated Bianchi type-I models from different point of view. We notice that, in connection to anisotropic equation of state for dark energy, several works are now available in the literature [29,30,31].…”