We introduce a systematic and direct procedure to generate hairy rotating black holes by
deforming a spherically symmetric seed solution. We develop our analysis in the context of …

We show how to decoupling two spherically symmetric and static gravitational sources
through the most general possible extension of the so-called Minimal Geometric …

In this work, we attempt to find an anisotropic solution for a compact star generated by
gravitational decoupling in f (Q)-gravity theory having a null complexity factor. To do this, we …

The Rastall theory of gravity is the generalized form of the Einstein theory which describes
the conservation law of energy and momentum tensor. In our work, we compute the charged …

Black holes with hair represented by generic fields surrounding the central source of the
vacuum Schwarzschild metric are examined under the minimal set of requirements …

Using the gravitational decoupling by the minimal geometric deformation approach, we build
an anisotropic version of the well-known Tolman VII solution, determining an exact and …

We employ the gravitational decoupling approach for static and spherically symmetric
systems to develop a simple and powerful method in order to (a) continuously isotropize any …

We employ the minimal geometric deformation approach to gravitational decoupling (MGD-
decoupling) in order to build an exact anisotropic version of the Schwarzschild interior …

We present a simple, analytic and straightforward method to elucidate the effects produced
by polytropic fluids on any other gravitational source, no matter its nature, for static and …

In this work we implement the Minimal Geometric Deformation decoupling method to obtain
general static interior solutions for a BTZ vacuum from the most general isotropic solution in …