Abstract The Einstein–Maxwell (or Einstein) system of field equations plays a substantial
role in the modeling of compact stars. Although due to its non-linearity getting an exact …

A complete theory of gravity impels us to go beyond Einstein's general relativity. One
promising approach lies in a new class of teleparallel theory of gravity named f (Q), where …

In this paper, we consider the Bianchi type-I space–time with perfect fluid as matter content
of the Universe in the framework of f (Q) gravity (where Q is the non-metricity scalar) recently …

In this work, we propose the modeling of static wormholes within the f (R, T) extended theory
of gravity perspective. We present some models of wormholes, which are constructed from …

The present work is focused on the investigation of the existence of compact structures
describing anisotropic matter distributions within the framework of modified gravity theories …

The current study emphasizes the impact of electric charge for static spherically symmetric
stellar structures using isotropic distribution in f (R, T) theory of gravity. For this purpose, we …

A cosmological model with a specific form of the Hubble parameter is constructed in a flat
homogeneous, and isotropic background in the framework of f (R, T) gravity, where R is the …

In this paper, we review the so-called Myrzakulov Gravity models (MG-N, with N= I, II,…, VIII)
and derive their respective metric-affine generalizations (MAMG-N), discussing also their …

A bstract A bouncing scenario of a flat homogeneous and isotropic universe is explored by
using the reconstruction technique for the power-law parametrization of the Hubble …

In this paper, we investigate the accelerated expansion of the Universe in the context of f (Q)
modified theory of gravity, where Q is a non-metricity scalar which characterizes the …