Gravitationally decoupled Non-Schwarzschild black holes and wormhole space-times

TL;DR

This paper introduces a new class of black hole solutions and explores their connection to wormhole space-times using gravitational decoupling and minimal geometric deformation methods.

Contribution

It presents a novel spherically symmetric black hole solution derived via gravitational decoupling and demonstrates how such solutions can be linked to wormhole geometries.

Findings

New black hole solutions obtained through minimal geometric deformation

Method to connect black holes with wormhole space-times

Insights into the structure of gravitational decoupling in black hole physics

Abstract

In this article, using gravitational decoupling by means of minimal geometric deformation approach, we obtain a new spherically symmetric and static black hole solution. To progress, we close the system by assuming that the average pressure of the $\theta$-sector is vanishing. Also, we tackle the problem regarding how, for a given minimally deformed black hole solution, one can connect it to a wormhole space-time.