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 language | English |
|---|---|
| Article number | 084016 |
| Journal | Physical Review D |
| Volume | 103 |
| Issue number | 8 |
| DOIs | |
| State | Published - 13 Apr 2021 |
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