The Hubble constant ($ H_0 $) tension is one of the major open problems in modern
cosmology. This tension is the discrepancy, ranging from 4 to 6$\sigma $, between the …

We investigate a bounce realization in the framework of higher order curvature in f (R, T)
modified theory of gravity. We perform a detailed analysis of the cosmological parameters to …

The evolution of the universe in a modified gravity theory that includes the terms Ricci scalar
(RR) and the Gauss‐Bonnet invariant (GG) is studied. The function f (R, G) f(R,G) is obtained …

We have developed a Bianchi I cosmological model of the universe in f (R, T) gravity theory
which fit good with the present-day scenario of accelerating universe. The model displays …

In the present work, we investigate the power-law entropy corrected holographic dark
energy (PLECHDE) model with Hubble horizon cutoff. We use 46 observational Hubble data …

In the present study, we have explored an axially symmetric Bianchi I universe with Lyra's
geometry. We assumed variable displacement vector as component of Lyra's geometry in …

The homogeneous and isotropic cosmological model in generalized f (R, T ϕ) theories
associated with the scalar field is discussed, which is motivated by the f (R, T) theory of …

We investigate the Universe's evolution within the framework of Rastall gravity, which is an
extension of the standard ΛCDM model. Utilizing a linear parametrization of the Equation of …

We examine the qualitative features of anisotropic models sourced by the fluid having an
inhomogeneous equation of state (EoS). In particular, we study the asymptotic behavior and …

In this study, we have explored a scalar field cosmological model in the axially symmetric
Bianchi type-I universe. In this study, our aim is to constrain the scalar field dark energy …