In the present communication, we have studied the existence of wormholes described by a
logarithmic shape function, in the exponential f (R, T) gravity given by f (R, T)= R+ 2 ξ e ζt …

In this paper, we have studied anisotropic axially symmetric perfect fluid cosmological model
in f (R, T) gravity. As proposed by Harko et al., by assuming the particular choice f (R, T)= f 1 …

This research explores the Tsallis holographic quintessence, k-essence, and tachyon
models of dark energy in the modified f (R, T) gravity framework with Granda–Oliveros cutoff …

In the current study, a theoretical model for non-interacting new Tsallis holographic dark
energy is constructed using the Granda–Oliveros as the IR cutoff with specified scale factor a …

This study focuses on the cosmological evolution of Barrow holographic dark energy
(BHDE) in a flat FLRW-universe. We take into account a time-dependent scale factor a …

The present study concerns an examination of a cosmological model that exhibits axially
symmetric and incorporates perfect fluid within the context of Lyra geometry. The field …

In order to analyze Barrow holographic dark energy (BHDE) in a flat FRW universe, the time-
dependent scale factor a (t)=[sinh (α t)] 1 n is employed. The Hubble horizon as the IR-cutoff …

Present study deals with homogeneous and isotropic) 2 (+ n dimensional flat Friedman-
Robertson-Walker (FRW) model with thick domain wall coupled with bulk viscous fluid within …