The understanding of stellar structure represents the crossroads of our theories of the
nuclear force and the gravitational interaction under the most extreme conditions observably …

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 dawn of the twenty-first century came with very positive prospects for gravity, cosmology,
and astrophysics. Technological progress made it possible for cosmology to enter to its …

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 …

This study simulates strange stars in f (Q) gravity with an additional source under an electric
field using gravitational decoupling by means of the complete geometric deformation (CGD) …

Very recently a compact object with a mass in the range 2.50÷ 2.67 M⊙ has been
discovered via gravitational waves detection of a compact binary coalescence. The mass of …

We derive a new interior solution for stellar compact objects in f (R) gravity assuming a
differential relation to constrain the Ricci curvature scalar. To this aim, we consider specific …

Building on the Einasto dark matter (DM) density parameterizations, this study explores the
possibility of constructing DM black holes (BHs) within the formalism of the Starobinsky …

This investigation aims to explore certain variables which are considered responsible for
generating pressure anisotropy in dynamical spherically symmetric stellar systems against …

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