Publication:
Kerr–Newman black holes can be generically overspun

dc.contributor.authorDüztaş, Koray
dc.contributor.departmentNatural and Mathematical Sciences
dc.contributor.ozuauthorDÜZTAŞ, Koray
dc.date.accessioned2020-09-07T10:10:19Z
dc.date.available2020-09-07T10:10:19Z
dc.date.issued2019-04-08
dc.description.abstractWe construct thought experiments involving the perturbations of Kerr-Newman black holes by neutral test fields to evaluate the validity of the weak form of the cosmic censorship conjecture. We first show that neglecting backreaction effects, extremal Kerr-Newman black holes which satisfy the condition (J(2)/M-4) < (1/3) can be overspun by scalar fields. This result, which could not be discerned in the previous analyses to first order, is prone to be fixed by employing backreaction effects. However the perturbation of Kerr-Newman black holes by neutrino fields leads to a generic overspinning of the black hole due to the absence of a lower limit for the frequency of the incident wave to ensure that it is absorbed by the black hole. For this case, the destruction of the event horizon cannot be fixed by any form of backreaction effects. This result should not be interpreted as a counter-example to any of the previous results which were based on the assumption that the null energy condition is satisfied. We clarify and justify our arguments with numerical examples.en_US
dc.description.versionPublisher versionen_US
dc.identifier.doi10.1140/epjc/s10052-019-6851-zen_US
dc.identifier.issn1434-6044en_US
dc.identifier.issue4en_US
dc.identifier.scopus2-s2.0-85064231137
dc.identifier.urihttp://hdl.handle.net/10679/6907
dc.identifier.urihttps://doi.org/10.1140/epjc/s10052-019-6851-z
dc.identifier.volume79en_US
dc.identifier.wos000463876000002
dc.language.isoengen_US
dc.peerreviewedyesen_US
dc.publicationstatusPublisheden_US
dc.publisherSpringer Natureen_US
dc.relation.ispartofEuropean Physical Journal C
dc.relation.publicationcategoryInternational Refereed Journal
dc.rightsopenAccess
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.titleKerr–Newman black holes can be generically overspunen_US
dc.typearticleen_US
dspace.entity.typePublication
relation.isOrgUnitOfPublication7a8a2b87-4f48-440a-a491-3c0b2888cbca
relation.isOrgUnitOfPublication.latestForDiscovery7a8a2b87-4f48-440a-a491-3c0b2888cbca

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