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 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 …

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

We use the definition of complexity for static and self–gravitating objects to build up three
physical general relativistic anisotropic models fulfilling the vanishing complexity condition …

The main focus of this paper is to explore the possibility of providing a new family of exact
solutions for suitable anisotropic spherically symmetric systems in the realm of general …

In the present paper, we have explored the existence of compact structures describing
anisotropic matter distributions within the framework of f (R, T) theory, where R is Ricci scalar …

In this work we use the vanishing complexity factor as a supplementary condition to
construct uncharged and charged like-Durgapal models. We provide the g tt component of …

The main aim of this work is devoted to studying the existence of compact spherical systems
representing anisotropic matter distributions within the scenario of alternative theories of …

In this work, a spherically symmetric and static relativistic anisotropic fluid sphere solution of
the Einstein field equations is provided. To build this particular model, we have imposed …

In this work, we will analyze the complexity factor, proposed by L. Herrera, of spherically
symmetric static distribution through the gravitational decoupling method. Specifically, we …