In this review we discuss the evolution of the universe filled with dark energy with or without
perfect fluid. In doing so we consider a number of cosmological models, namely Bianchi type …

A system of minimally coupled nonlinear spinor and scalar fields within the scope of a
Bianchi type-I (BI) cosmological model in the presence of a perfect fluid and a cosmological …

This paper is devoted to identify some physical causes of energy density inhomogeneity and
stability of self-gravitating relativistic fluids in plane symmetry such as Weyl tensor, local …

Within the scope of the isotropic FRW cosmological model the role of nonlinear spinor field
in the evolution of the Universe is studied. It is found that unlike in anisotropic cosmological …

Within the scope of Bianchi type VI, VI0, V, III, I, LRSBI and FRW cosmological models we
have studied the role of nonlinear spinor field on the evolution of the Universe and the …

In this paper we investigate a class of solutions of Einstein equations for the plane-
symmetric perfect fluid case with shear and vanishing acceleration. If these solutions have …

This paper analyzes the stability of a collapsing matter distribution enclosed by plane
symmetry in the presence of electromagnetic field. The field equations, matching conditions …

This paper aims to explore anisotropic planar analytical models for dissipative as well as
non-dissipative matter distributions. We relate the Weyl tensor and physical variables of …

The objective of this paper is to explore exact solutions of the Einstein field equations for
shear-free plane symmetry with non-viscous heat-conducting isotropic fluid as a collapsing …

An enigmatic prediction of Einstein's general theory of relativity is gravitational waves. With
the observed decay in the orbit of the Hulse-Taylor binary pulsar agreeing within a fraction of …