In this paper, we focus on the parametrization of the effective equation of state (EoS)
parameter within the framework of f (Q) symmetric teleparallel gravity. Here, the gravitational …

In this paper, using Barrow entropy, we propose an interacting model of Barrow holographic
dark energy (BHDE). In particular, we study the evolution of a spatially flat FLRW universe …

The presented paper is a comprehensive analysis of two dark energy (DE) cosmological
models wherein exact solutions of the Einstein field equations (EFEs) are obtained in a …

Holographic dark energy with the Hubble radius as infrared cutoff has been considered as a
candidate to explain the late-time cosmic acceleration and it can solve the coincidence …

This study proposes a novel parametrization approach for the dimensionless Hubble
parameter ie E 2 (z)= A (z)+ β (1+ γ B (z)) in the context of scalar field dark energy models …

In this article, we introduce an innovative parametric representation of the Hubble
parameter, providing a model-independent means to explore the dynamics of an …

This article introduces a novel parametric form of the Hubble parameter for exploring the
accelerating cosmos in a model-independent manner. The model parameters are …

In this work, we have proposed a simple parametrization for the pressure component p (z) of
the dark energy model and have studied the cosmological implications of this model in the …

We reconstruct the effective equation of state (EoS) within the framework of the general
theory of relativity in a homogeneous and isotropic Friedmann–Lemaître–Robertson–Walker …

This work investigates the background of flat FLRW metric within the framework of f (Q, T)
gravity theory. We construct two cosmological models whose functional form in f (Q, T) …