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- W2531574757 abstract "We construct hairy black hole solutions that merge with the anti-de Sitter (AdS4) Reissner-Nordström black hole at the onset of superradiance. These hairy black holes have, for a given mass and charge, higher entropy than the corresponding AdS4-Reissner-Nordström black hole. Therefore, they are natural candidates for the endpoint of the charged superradiant instability. On the other hand, hairy black holes never dominate the canonical and grand-canonical ensembles. The zero-horizon radius of the hairy black holes is a soliton (i.e. a boson star under a gauge transformation). We construct our solutions perturbatively, for small mass and charge, so that the properties of hairy black holes can be used to testify and compare with the endpoint of initial value simulations. We further discuss the near-horizon scalar condensation instability which is also present in global AdS4-Reissner-Nordström black holes. We highlight the different nature of the near-horizon and superradiant instabilities and that hairy black holes ultimately exist because of the non-linear instability of AdS." @default.
- W2531574757 created "2016-10-21" @default.
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- W2531574757 date "2017-02-01" @default.
- W2531574757 modified "2023-09-26" @default.
- W2531574757 title "Hairy black holes and the endpoint of AdS4 charged superradiance" @default.
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- W2531574757 doi "https://doi.org/10.1007/jhep02(2017)128" @default.
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