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Overspinning BTZ black holes with test particles and fields

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arxiv 1701.07241 v1 pith:5NV4OY5F submitted 2017-01-25 gr-qc

classification gr-qc
keywords blackholeextremaltestoverspinningholesparticlessuperradiance
verification ladder T0 review T1 audit T2 compute T3 formal

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It has been claimed that in a test of an asymptotically AdS version of weak cosmic censorship conjecture by attempting to overspin a BTZ black hole with test particles, one finds that it is not possible to spin-up the black hole past its extremal limit. The result of this analysis is restricted to the case where the initial black hole is extremal. We extend this analysis to find that massive test particles can overspin the black hole, if we start with a nearly extremal black hole, instead. We also consider the interaction of the BTZ black hole with test fields. We show that overspinning of nearly extremal black holes is possible whether or not there is superradiance for the field. If there is superradiance, overspinning occurs in a narrow range of frequencies bounded below by the super-radiant limit. However, if there is no superradiance for the field, overspinning becomes generic and also applies to extremal black holes. This is in analogy with the Kerr case.

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Cited by 3 Pith papers

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

  1. Trapped Surface as a Cosmic Censor

    gr-qc 2026-06 unverdicted novelty 7.0 of 10

    A trapped-surface criterion, derived under null convergence and generic conditions, rules out superextremal Reissner-Nordström, Kerr-Newman, and related final states in overcharging thought experiments without using a...

  2. The First Law and Weak Cosmic Censorship for de Sitter Black Holes

    gr-qc 2024-11 accept novelty 6.0 of 10

    An Iyer-Wald first law is established for general perturbations of Reissner-Nordstrom-de Sitter black holes, and a second-order Sorce-Wald argument shows that near-extremal such black holes cannot be overcharged under...

  3. Six-dimensional Myers-Perry rotating black hole cannot be overspun

    gr-qc 2019-08 conditional novelty 5.0 of 10

    A six-dimensional rotating black hole with two spins cannot be overspun by test particle accretion, so weak cosmic censorship holds for this case.

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