The paper deals with Bianchi type V Universe, which has dynamical energy density. We
consider Bianchi type V space-time, introducing three different skewness parameters along …

In this paper we study the evolution of the dark energy parameter within the scope of a
spatially homogeneous and isotropic Friedmann-Robertson-Walker (FRW) model filled with …

In the present work our aim is to construct FRW cosmological models in the framework of f
(Q) theory of gravity. We explore the accelerating behavior of the universe for particular form …

The paper deals with a spatially homogeneous and anisotropic Bianchi type-I universe filled
with two minimally interacting fluids; matter and holographic dark energy components. The …

We present two dark energy (DE) models with an anisotropic fluid in Bianchi type-VI 0 space-
time by considering time dependent deceleration parameter (DP). The equation of state …

In this paper, we have investigated a bulk viscous anisotropic Universe and constrained its
model parameters with recent and Pantheon compilation data. Using cosmic chronometric …

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 …

In this paper, we have studied a homogeneous and anisotropic universe filled with matter
and holographic dark energy components. Assuming deceleration parameter to be a …

In this paper, we study a Bianchi type-I model of universe filled with barotropic and dark
energy (DE) type fluids. The present values of cosmological parameters, such as Hubble …

The present study deals with spatially homogeneous and anisotropic locally rotationally
symmetric (LRS) Bianchi type I cosmological model with dominance of dark energy. To get …