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Kerr-de Sitter Black Hole Revisited

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arxiv 2104.06359 v1 pith:FFFMWFUR submitted 2021-04-13 gr-qc hep-th

J. Ovalle , E. Contreras , Z. Stuchlik This is my paper · ORCID
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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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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Regular black holes with Minkowskian cores: causal structure and observational degeneracy

    gr-qc 2026-07 conditional novelty 5.0 of 10

    Regular black holes with Minkowskian cores constructed by gravitational decoupling produce shadows and accretion-disk images nearly indistinguishable from Kerr/Schwarzschild despite radically different interiors.

  2. Off-diagonal deformations of regular Schwarzschild black holes and general relativistic G. Perelman thermodynamics

    physics.gen-ph 2025-05 reject novelty 5.0 of 10

    The authors build off-diagonal deformations of regular Schwarzschild black holes and introduce Perelman-type geometric flow thermodynamic variables for them.

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