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 study, we explore several new characteristics of a static anisotropic hybrid star with
strange quark matter (SQM) and ordinary baryonic matter (OBM) distribution. Here, we use …

The aim of this study is to explore the relativistic anisotropic configuration of a hybrid star in
the proximity of strange quark matter and normal baryonic matter within the context of f (Q) …

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 …

The core objective of our study is to examine the possibilities of constructing an additional
class of precise solutions for appropriate anisotropic source configuration in the realm of f …

Alternative gravity theory is currently an incredibly significant technique for addressing some
enduring experimental difficulties, such as the universe's dark region. They may also be …

In this paper, we explore the existence of spherically symmetric strange quark configurations
coupled with anisotropic fluid setup in the framework of modified Gauss–Bonnet theory. In …

In the current article, we study anisotropic spherically symmetric strange star under the
background of f (R, T) gravity using the metric potentials of Tolman–Kuchowicz type (Tolman …

This paper studies the structural formation of various spherically symmetric anisotropic
configured stars in f (R, T, Q) f(R,T,Q) gravity under the influence of electromagnetic field …

The spherically symmetric dark energy (DE) stellar model is presented here within the
context of the f (Q) theory of gravity. In order to develop the model, we take into account the …