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arXiv · 2104.06359

Kerr-de Sitter Black Hole Revisited

J. Ovalle·E. Contreras·Z. Stuchlik
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Abstract

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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J. Ovalle, E. Contreras, Z. Stuchlik. 2021-04-13. Kerr-de Sitter Black Hole Revisited. https://doi.org/10.1103/physrevd.103.084016

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