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 …

In this work, we construct stellar models based on the complexity factor as a supplementary
condition which allows to close the system of differential equations arising from the …

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 …

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 …

The present study explores the f (R, T) f (R, T) modified gravity on the basis of observational
data for three different compact stars with matter profile as anisotropic fluid without electric …

In this work, we study the existence of strange stars in the background of f (T, T) gravity in the
Einstein spacetime geometry, where T is the torsion tensor and T is the trace of the energy …

In this work, we get an idea of the existence of compact stars in the background of f (T)
modified gravity where T is a scalar torsion. We acquire the equations of motion using …

This study delves into the realm of solving Einstein's field equations within the framework of
general relativity. In this paper, we present an exact solution derived through the vanishing …

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 solution for the …

This paper's main aim is to investigate the existence of a new classification of embedded
class-I solutions of compact stars, by using Karmarkar condition in f (R) gravity background …