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Higher-dimensional charged black holes cannot be over-charged by gedanken experiments

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arxiv 1712.07342 v4 pith:JVLXCJD6 submitted 2017-12-20 hep-th gr-qc

Boxuan Ge , Yuyu Mo , Suting Zhao , Jieping Zheng This is my paper · ORCID
classification hep-thgr-qc
keywords blackholeschargedhigher-dimensionalcannotextremalgedankennearly
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We reconsider over-charging the higher-dimensional nearly extremal charged black holes using the new version of gedanken experiment proposed recently by Sorce and Wald. As a result, we find that cosmic censorship conjecture associated with such black holes is restored by taking into account the second-order correction, albeit violated by the first-order perturbation. Namely, the higher-dimensional nearly extremal charged black holes cannot be over-charged.

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Cited by 4 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. Thermodynamics and weak cosmic censorship conjecture with pressure in the rotating BTZ black holes

    gr-qc 2019-08 reject novelty 6.0 of 10

    For charged rotating BTZ black holes, the paper reports that the weak cosmic censorship conjecture holds without pressure but can be violated in the extended phase space with pressure if the AdS radius is allowed to vary.

  4. 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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