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 present work is focused on the investigation of the existence of compact structures
describing anisotropic matter distributions within the framework of modified gravity theories …

We investigate irregularity factors for a self-gravitating spherical star evolving in the
presence of an imperfect fluid. We explore the gravitational field equations and the …

We set up in detail the general formalism to model polytropic general relativistic stars with
anisotropic pressure. We shall consider two different possible polytropic equations, all of …

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 …

We investigate the evolution of self-gravitating either dissipative or non-dissipative systems
satisfying the condition of minimal complexity, and whose areal radius velocity is …

We explore the evolutionary behaviors of compact objects in a modified gravitational theory
with the help of structure scalars. Particularly, we consider the spherical geometry coupled …

We investigated Rastall gravity, for an anisotropic star with a static spherical symmetry,
whereas the matter-geometry coupling as assumed in Rastall Theory (RT) is expected to …

In this work we analyze the stability of self gravitating spheres in the context of gravitational
cracking. Besides exploring the role played by the anisotropy in the occurrence of cracking …

The major goal of this work is to find solutions of Einstein–Maxwell field equations for
anisotropic, expansion-free, non-static, spherically distributed matter content. The analytical …