Gravitationally decoupled non-Schwarzschild black holes and wormhole space–times.

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 θ -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. [ABSTRACT FROM AUTHOR]