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Vacuum decays around spinning black holes

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arxiv 1909.01378 v3 pith:LKOKK6NO submitted 2019-09-03 hep-th gr-qc

Naritaka Oshita , Kazushige Ueda , Masahide Yamaguchi This is my paper · ORCID
classification hep-thgr-qc
keywords vacuumblackholearoundcasedecayspinningassumptions
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We investigate a vacuum decay around a spinning seed black hole by using the Israel junction condition and conclude that the spin of black hole would suppress a vacuum decay rate compared to that for a non-spinning case, provided that the surface of vacuum bubble has its ellipsoidal shape characterized by the Kerr geometry. We also find out that in the existence of a near-extremal black hole, a false vacuum state can be more stabilized than the case of the Coleman-de Luccia solution. A few necessary assumptions to carry the calculations are discussed.

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Cited by 1 Pith paper

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  1. Vacuum bubbles from cosmic ripples

    hep-ph 2026-04 conditional novelty 6.0 of 10

    Over-densities in the early universe reduce the Euclidean action for vacuum decay, making false-vacuum bubbles nucleate earlier; under-densities do the opposite.

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