Kerr-de Sitter black hole revisited

J. Ovalle; E. Contreras; Z. Stuchlik

doi:10.1103/PhysRevD.103.084016

Kerr-de Sitter black hole revisited

J. Ovalle^*
, E. Contreras
, Z. Stuchlik

^*Autor correspondiente de este trabajo

Física

Silesian University in Opava

Producción científica: Contribución a una revista › Artículo › revisión exhaustiva

58 Citas (Scopus)

Resumen

We interpret the cosmological constant as the energy of the vacuum, and under a minimum amount of assumptions, we show that it is deformed in the vicinity of a black hole. This leads us to reexamine the Kerr-de Sitter solution. We provide a new solution, simpler and geometrically richer, which shows the impact of the rotation in form of a warped curvature. We carry out a detailed and exact study on the new black hole solution, and we conclude with a conjecture regarding the possible impact of our results on alternative theories.

Idioma original	Inglés
Número de artículo	084016
Publicación	Physical Review D
Volumen	103
N.º	8
DOI	https://doi.org/10.1103/PhysRevD.103.084016
Estado	Publicada - 13 abr. 2021

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AB - We interpret the cosmological constant as the energy of the vacuum, and under a minimum amount of assumptions, we show that it is deformed in the vicinity of a black hole. This leads us to reexamine the Kerr-de Sitter solution. We provide a new solution, simpler and geometrically richer, which shows the impact of the rotation in form of a warped curvature. We carry out a detailed and exact study on the new black hole solution, and we conclude with a conjecture regarding the possible impact of our results on alternative theories.

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Kerr-de Sitter black hole revisited

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