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Destroying a near-extremal Kerr-Newman-AdS black hole

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arxiv 1705.01676 v1 pith:SF7GHEL3 submitted 2017-05-04 gr-qc

Yu Song , Rui-Hong Yue This is my paper
classification gr-qc
keywords effectskerr-newman-adsradiativeself-forcetestblackholenear-extremal
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If radiative and self-force effects are neglected, we find that feeding a test particle into a near-extremal Kerr-Newman-AdS black hole could lead to destroy their event horizon, giving rise to naked singularities. Hence radiative and self-force effects must be taken into account to further test cosmic censorship. Moreover, the allowed parameter range for this test particle is very narrow, this leaves the possibility of radiative and self-force effects considerations to cure the problem of WCC violation in Kerr-Newman-AdS spacetime.

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Cited by 1 Pith paper

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  1. 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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