https://doi.org/10.1140/epjc/s10052-023-11938-5
Regular Article - Theoretical Physics
Gravitationally decoupled non-Schwarzschild black holes and wormhole space–times
1
Instituto de Física, Pontificia Universidad Católica de Valparaíso, 4950, Casilla, Valparaíso, Chile
2
Departamento de Física Aplicada, Universidad de Alicante, Campus de San Vicente del Raspeig, 03690, Alicante, Spain
3
Sede Esmeralda, Universidad de Tarapacá, Avda. Luis Emilio Recabarren 2477, Iquique, Chile
4
Unidad de Equipamiento Científico (Maini), Universidad Católica del Norte, Av. Angamos 0610, Antofagasta, Chile
5
Centre for Cosmology, Astrophysics and Space Science (CCASS), GLA University, 281406, Mathura, Uttar Pradesh, India
a
francisco.tello@pucv.cl
b
angel.rincon@ua.es
Received:
3
July
2023
Accepted:
18
August
2023
Published online:
8
September
2023
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 
-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.
© The Author(s) 2023
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