Gravitationally decoupled non-Schwarzschild black holes and wormhole space–times
Francisco Tello‐OrtizInstituto de Física, Pontificia Universidad Católica de Valparaíso, Casilla, 4950, Valparaíso, ChileÁngel RincónDepartamento de Física Aplicada, Universidad de Alicante, Campus de San Vicente del Raspeig, Alicante, 03690, SpainA. AlvarezUnidad de Equipamiento Científico (Maini), Universidad Católica del Norte, Av. Angamos 0610, Antofagasta, ChileSaibal RayCentre for Cosmology, Astrophysics and Space Science (CCASS), GLA University, Mathura, 281406, Uttar Pradesh, India
2023en
ABI
Аннотация
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 $$\theta $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>θ</mml:mi> </mml:math> -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.
Перевод пока недоступен
Идентификаторы
Цитирования и источники
Цитирований: 2Использованных источников: 0