In this article, we explore some emerging properties of the stellar objects in the frame of the f
(R, T) gravity by employing the well-known Karmarkar condition, where R and T represent …

This work aims to investigate the behaviour of compact stars in the background of f (R, T)
f(R,T) theory of gravity. For current work, we consider the Krori‐Barua metric potential ie, ν …

In this manuscript, we study the construction of static cylindrically symmetric thin shell
wormhole models with an electric charge in the background of f (R, T) gravity. We utilized …

Recent advances in nuclear theory and new astrophysical observations have led to the
need for specific theoretical models applicable to dense-matter physics phenomena …

The aim of this manuscript is to investigate the charged anisotropic compact stars in f (R, A)
theory of gravity, namely Ricci-Inverse gravity. By employing the Karmarkar condition, we …

Many physically inspired general relativity (GR) modifications predict significant deviations
in the properties of spacetime surrounding massive neutron stars. Among these …

We work out the junction conditions for the Palatini f (R, T) extension of general relativity,
where f is an arbitrary function of the curvature scalar R of an independent connection, and …

In the context of linear f (R, T)= R+ χ T gravity, where R is the Ricci scalar, T is the trace of the
energy-momentum tensor, and χ is a dimensionless parameter, we have obtained exact …

As a potential candidate for the late-time accelerating expansion of the Universe, the
Chaplygin gas and its generalized models have significant implications to modern …

In this work, we study the influence of f (R, T) gravity on rapidly rotating neutron stars. First
we discuss the main aspects of this modified theory of gravity where the gravitational …