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Cosmic Censorship of Rotating Anti-de Sitter Black Hole

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arxiv 1509.06691 v2 pith:NG5VZ3SV submitted 2015-09-22 gr-qc hep-th

classification gr-qchep-th
keywords blackholecensorshipcosmicabsorptionangularanti-deextremal
verification ladder T0 review T1 audit T2 compute T3 formal
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We test the validity of cosmic censorship in the rotating anti-de Sitter black hole. For this purpose, we investigate whether the extremal black hole can be overspun by the particle absorption. The particle absorption will change the mass and angular momentum of the black hole, which is analyzed using the Hamilton-Jacobi equations consistent with the laws of thermodynamics. We have found that the mass of the extremal black hole increases more than the angular momentum. Therefore, the outer horizon of the black hole still exists, and cosmic censorship is valid.

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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. 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. Weak Cosmic Censorship with spinning particles in Kerr-(A)dS spacetimes

    gr-qc 2025-07 conditional novelty 6.0 of 10

    Extremal Kerr-de Sitter black holes cannot be overspun by spinning test particles, and apparent Kerr-anti-de Sitter overspinning configurations are eliminated once the particle's finite size is respected.

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