In this paper, we investigate a cosmological model based on viscous f (R, T) gravity as a
potential alternative to dark energy. This model incorporates bulk viscosity and is analyzed …

In this study, we investigate the cosmological evolution of the universe, focusing on the
KMMS models in a model-independent approach, particularly the scenario involving linear …

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

In the present paper, we have investigated dark energy scenarios in higher derivative f (R, L
m) gravity theory in a flat spacetime universe by constraining cosmographic series of Hubble …

This study explores the extension of teleparallel gravity within the framework of general
relativity, introducing an algebraic function f (T) dependent on the torsion scalar T. Motivated …

This work explores the dark energy nature of logarithmic f (R, Lm)-gravity models with
observational constraints, where Lm represents the matter Lagrangian for perfect fluid and R …

This article explores the cosmological scenario of the universe in the context of the f (T)
power law model, where T represents the torsion scalar. To obtain the deterministic solution …

This paper explores models of the FLRW universe that incorporate a time-varying
cosmological term Λ (t). Specifically, we assume a power-law form for the cosmological term …

Motivated by anomalies in cosmic microwave background observations, we investigate the
implications of f (Q, T) gravity in Bianchi type-I spacetime, aiming to characterize the …

Understanding the evolution of dark energy poses a significant challenge in modern
cosmology, as it is responsible for the universe's accelerated expansion. In this study, we …