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Kerr-de Sitter black hole revisited

  • J. Ovalle*
  • , E. Contreras
  • , Z. Stuchlik
  • *Corresponding author for this work
  • Silesian University in Opava

Research output: Contribution to journalArticlepeer-review

58 Scopus citations

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.

Original languageEnglish
Article number084016
JournalPhysical Review D
Volume103
Issue number8
DOIs
StatePublished - 13 Apr 2021

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