2017
DOI: 10.1103/physrevd.96.104014
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Gedanken experiments to destroy a black hole. II. Kerr-Newman black holes cannot be overcharged or overspun

Abstract: We consider gedanken experiments to destroy an extremal or nearly extremal Kerr-Newman black hole by causing it to absorb matter with sufficient charge and/or angular momentum as compared with energy that it cannot remain a black hole. It was previously shown by one of us that such gedanken experiments cannot succeed for test particle matter entering an extremal Kerr-Newman black hole. We generalize this result here to arbitrary matter entering an extremal Kerr-Newman black hole, provided only that the non-ele… Show more

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Cited by 197 publications
(318 citation statements)
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“…conducted on the conjecture for not only black holes of Einstein's theory of gravity, but also anti-de Sitter (AdS), lower-dimensional, and higher-dimensional black holes [18][19][20][21][22][23][24][25][26][27][28][29][30]. From a thermodynamic point of view, the conjecture is quite consistently related to the laws of thermodynamics.…”
Section: Jhep11(2017)129mentioning
confidence: 99%
“…conducted on the conjecture for not only black holes of Einstein's theory of gravity, but also anti-de Sitter (AdS), lower-dimensional, and higher-dimensional black holes [18][19][20][21][22][23][24][25][26][27][28][29][30]. From a thermodynamic point of view, the conjecture is quite consistently related to the laws of thermodynamics.…”
Section: Jhep11(2017)129mentioning
confidence: 99%
“…In this paper, following the setup of the gedanken experiments proposed by Sorce and Wald [27], we investigated the weak cosmic censorship conjecture in EMGB gravity under the perturbation of the spherically charged infalling matter collision. First of all, based on the Iyer-Wald formalism, we derived the perturbation inequality under the second-order approximation when the matter fields satisfy the null energy condition.…”
Section: Discussionmentioning
confidence: 99%
“…Following a similar setup with [27], here we consider the case where the background geometry is a nearly extremal black hole which satisfies r m = (1 − ε)r h with some small parameter ε chosen to agree with the first-order perturbation of the matter source. Then, Eq.…”
mentioning
confidence: 99%
“…In this section, following the discussion in [26], we would like to derive the first two order perturbation inequalities for the static electrically regular black holes. Since the Lagrangian cannot be expressed explicitly, below we only consider the off-shell variation of the Lagrangian of the Einstein part, i.e.,…”
Section: Perturbation Inequalitiesmentioning
confidence: 99%