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 …

The main objective of this paper is to examine the viability and stability of anisotropic
compact stellar objects adopting the Karmarkar condition in energy-momentum squared …

In this work we have extended the Maurya-Gupta isotropic fluid solution to Einstein field
equations to an aniso-tropic domain. To do so, we have employed the gravitational …

This work aims to study a charged compact star in the scenario of f (R) theory of gravity. We
use some matching condition of spherically symmetric space-time with Bardeen's model as …

We obtain a new anisotropic solution for spherically symmetric spacetimes by analyzing the
Karmarkar embedding condition. For this purpose we construct a suitable form of one of the …

In this work, we present a new class of analytic and well-behaved solution to Einstein's field
equations describing anisotropic matter distribution. It's achieved in the embedding class …

In the present article, we have obtained a new solution for the charged compact star model
through the gravitational decoupling (GD) by using a complete geometric deformation (CGD) …

In this study, the geometrically deformed compact objects in the f (Q, T) gravity theory under
an electric field through gravitational decoupling via minimal geometric deformation (MGD) …

This manuscript examines how effective matter variables influence the geometry of compact
stellar objects with anisotropic matter configuration in modified f (R, φ, χ) gravity, where R …

The main goal of this work is to provide a comprehensive study of relativistic structures in the
context of recently proposed R+ α A gravity, where R is the Ricci scalar, and A is the anti …