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 …

This paper examines traversable wormhole models in the $ f (R) $ theories of gravity by
applying the Karmarkar condition. For this purpose, we consider spherically symmetric …

Dense nuclear matter is expected to be anisotropic due to effects such as solidification,
superfluidity, strong magnetic fields, hyperons, pion-condensation. Therefore an anisotropic …

In this work we build a relativistic anisotropic admissible compact structures. To do so we
combine the class I approach with gravitational decoupling in order to generate the …

In this article, we have presented a static anisotropic solution of stellar compact objects for
self-gravitating system by using minimal geometric deformation techniques in the framework …

In this work, we present a new class of analytic and well-behaved solution to Einstein's field
equations describing anisotropic matter distribution. It's achieved in the embedding class …

In the present article, we have obtained a new solution for the charged compact star model
through the gravitational decoupling (GD) by using a complete geometric deformation (CGD) …

Durgapal's fifth isotropic solution describing spherically symmetric and static matter
distribution is extended to an anisotropic scenario. To do so we employ the gravitational …

In the present article, we have constructed a static charged anisotropic compact star model
of Einstein field equations for a spherically symmetric space-time geometry. Specifically, we …

In this paper, we use the embedding class-I technique to examine the effect of charge on
traversable wormhole geometry in the context of f (G) theory, where G is the Gauss–Bonnet …