In this paper, we study a spatially homogeneous and isotropic FLRW cosmological model in
framework of the symmetric teleparallel f (Q) gravity proposed by Jimenez et al.(Physical …

In this paper, an attempt is made to construct a Friedmann–Lemaitre–Robertson–Walker
model in f (R, T) gravity with a perfect fluid that yields acceleration at late times. We take f (R …

Modelling of matter bounce in f (R, T) gravity has been presented with no violation of the null
energy condition. Only a closed universe with negative pressure is allowed in good …

In this research, we examine a spatially homogeneous anisotropic locally rotationally
symmetric (LRS) Bianchi type-I cosmological model in f (R, T) gravity, for some choices of …

This paper investigates the impact of bulk viscosity within the framework of f (T, B) gravity.
We consider a time-dependent viscosity model with a particular Hubble parameter …

A Friedmann–Lemaitre–Robertson–Walker space–time model with all curvatures k= 0,±1 is
explored in f (R, T) gravity, where R is the Ricci scalar, and T is the trace of the energy …

In the f (R, T) modified theory of gravity, where R, T denote the curvature scalar and the trace
of the stress-energy-momentum tensor, respectively, the work is concerned with the general …

This work deals with the two fluid Bianchi type-V cosmological models consisting of matter
and radiating source in the f (R, T) theory of gravity studied by Harko et al.[Phys. Rev. D 84 …

We consider the gravitational collapse of a quark binding string fluid in theory of gravity. A
quark binding string state of a fluid is expected to occur as a combination of quark matter …

We obtain exact solutions to the field equations for five-dimensional locally rotationally
symmetric (LRS) Bianchi type-I spacetime in the f (R, T) theory of gravity, where specifically …