Modern cosmology establishes the scenario of accelerated expansion of the universe and
the reason for this is supposed to be the exotic negative pressure named dark energy. In …

In the present investigation we are mainly concerned with a massive scalar field in an axially
symmetric Bianchi type–I space-time. Einstein field equations are solved to obtain an exact …

The goal of this paper is to investigate the cosmic evolution of a cosmological model with a
massive scalar field in f (R, T) gravity (R and T denote the Ricci scalar and the energy …

This paper deals with the construction of locally rotationally symmetric (LRS) Bianchi type-II
(B-II) cosmological models obtained by solving Einstein field equations coupled with an …

This paper aims to investigate the dynamical behaviour of Kaluza-Klein (KK) FRW type dark
energy cosmological models in the context of Saez and Ballester's scalartensor theory of …

The purpose of this paper is to construct anisotropic and spatially homogeneous Bianchi
type-VI 0 Kaniadakis holographic dark energy (KHDE) model in general relativity. For this …

This article examines the physical behaviour of the Kaluza-Klein FRW type space-time with f
(R, T) gravity proposed by Harko et al.(Phys. Rev. D 84: 024020, 2011) in the presence of a …

A spatially homogenous and anisotropic locally rotationally symmetric (LRS) Bianchi type-I
space-time is considered in the presence of a massive scalar field containing domain walls …

This article is devoted to the study of Kaluza-Klein space-time filled with cosmic string and
attractive massive scalar field in the presence of minimally interacting dark energy in general …

We investigate the cosmological scenario involving spatially homogeneous and anisotropic
Bianchi type-VI 0 space-time in the context of the Sharma-Mittal holographic dark energy …