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 manuscript, we use the conformal killing vectors to solve the Einstein–Maxwell field
equations in the background of modified f (G) gravity. We consider the observational data for …

This paper investigates the concept of cracking and overturning to analyze the impact of
local density perturbations on the stability of self-gravitating compact objects in the …

The main objective of this study is to investigate the stability and viability of anisotropic
compact stellar objects using the Krori–Burua solutions in f (𝒬) gravity, where 𝒬 is a …

This paper investigate the impacts of local density perturbations on the stability of self-
gravitating compact objects by utilizing cracking technique within the context of f (R, T) …

In this article, we attempt to find a singularity free solution of Einstein's field equations for
compact stellar objects, precisely strange (quark) stars, considering Schwarzschild metric as …

In the present paper we obtain an anisotropic analog of the Durgapal and Fuloria (Gen
Relativ Gravit 17: 671, 1985) perfect fluid solution. The methodology consists of contraction …

In this manuscript, we employ the cracking technique in the Rastall gravity framework to
assess how local density perturbations affect the stability of anisotropic stellar structures. To …

In the present investigation an exact generalised model for anisotropic compact stars of
embedding class 1 is sought with a general relativistic background. The generic solutions …

This manuscript examines the compact stars in gravity f (Q), where non-metricity Q drives
gravitational interactions. To achieve this goal, we consider a spherically symmetric …