In this paper we discuss the law of variation of scale factor a=(t^ke^t)^1n which yields a time-
dependent deceleration parameter (DP) representing a new class of models that generate a …

Evolution of dark energy parameter within scope of a spatially homogeneous and isotropic
Friedmann–Robertson–Walker model filled with perfect fluid and dark energy components is …

The exact solutions of the field equations for Hypersurface-homogeneous space time under
the assumption on the anisotropy of the fluid (dark energy) are obtained for exponential and …

Today dark energy cosmological models have become essential to explain the accelerated
expansion of the universe. Motivated by this we investigate, in this paper, a dark energy …

When the source for the energy-momentum tensor is a bulk viscous fluid containing one-
dimensional cosmic strings, a spatially homogeneous and anisotropic Bianchi type-V …

Abstract Five dimensional Kaluza-Klein space-time is considered in the presence of
anisotropic dark energy in f (R, T) gravity proposed by Harko et al.(Phys. Rev. D 84: 024020 …

Abstract The Five dimensional anisotropic Bianchi type-III cosmological model has been
investigated within the framework of Brans-Dicke (Phys. Rev. 124: 925, 1961) scalar-tensor …

A new class of a spatially homogeneous and anisotropic Bianchi type-I cosmological models
of the universe for perfect fluid distribution within the framework of scalar-tensor theory of …

In this paper, we have explored the features of the five-dimensional Bianchi type-I
cosmological universe filled with barotropic fluid and dark energy within the framework of …

In this paper, we have presented a cosmological model that represents spatially
homogenous and isotropic accelerating universe from the perspective of the latest …