This study investigates accelerated cosmic expansion using the Viscous Modified Chaplygin
Gas (VMMG) and Generalized Cosmic Chaplygin Gas (GCCM) within Horava–Lifshitz …

In this work, we assume that the FLRW universe, which is filled with dark matter along with
dark energy, is in the framework of Hořava–Lifshitz (HL) gravity. The dark energy is …

In this work, we assume the FRLW Universe which is filled with dark matter along with dark
energy in the framework of Horava-Lifshitz (HL) gravity. The dark energy is considered as …

This study investigates accelerated cosmic expansion using various cosmological models
within Horava-Lifshitz gravity, including BBCCFHKO, Seljak, ASSS, PADE-I, PADE-II, and …

We consider the interacting Tsallis Holographic Dark Energy (THDE), with the Granda–
Oliveros (GO) scale as the infrared (IR) cutoff, as dynamical vacuum. We analytically solved …

Abstract f (R) gravity is an extension of Einstein's General Relativity derived from relaxing the
hypothesis that the Hilbert-Einstein action for the gravitational field is strictly linear in the …

In this paper, we investigate the late-time cosmic accelerated expansion using various
equations of state parametrizations within the framework of Hořava-Lifshitz gravity. We …

In the present study, a homogeneous and anisotropic LRS Bianchi type-I universe model is
considered with an interacting dark matter and Renyi holographic dark energy model …

We have probed spatially homogeneous anisotropic Bianchi type-I universe in f (Q) gravity
in the presence of dark matter, Tsallis holographic dark energy (THDE) and Rényi …

The main motivation of our study is to explore Rényi holographic dark energy, Sharma–
Mittal holographic dark energy, Rényi new agegraphic dark energy, and Sharma–Mittal new …