Trapped surfaces in spherical stars

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dc.contributor.authorBizon, Piotr
dc.contributor.authorMalec, Edward
dc.contributor.authorÓ Murchadha, Niall
dc.date.accessioned2017-09-08T09:15:50Z
dc.date.available2017-09-08T09:15:50Z
dc.date.issued1988
dc.description.abstractWe give necessary and sufficient conditions for the existence of trapped surfaces in spherically symmetric spacetimes. These conditions show that the formation of trapped surfaces depends on both the degree of concentration and the average flow of the matter. The result can be considered as a partial validation of the cosmic-censorship hypothesis.en
dc.description.statusPeer revieweden
dc.description.versionPublished Versionen
dc.format.mimetypeapplication/pdfen
dc.identifier.citationBizon, P., Malec, E. and O'Murchadha, N. (1988) 'Trapped surfaces in spherical stars', Physical Review Letters, 61(10), 1147-1150 (4pp). doi: 10.1103/PhysRevLett.61.1147en
dc.identifier.doi10.1103/PhysRevLett.61.1147
dc.identifier.endpage1150
dc.identifier.issn0031-9007
dc.identifier.issued10
dc.identifier.journaltitlePhysical Review Lettersen
dc.identifier.startpage1147
dc.identifier.urihttps://hdl.handle.net/10468/4668
dc.identifier.volume61
dc.language.isoenen
dc.publisherAmerican Physical Societyen
dc.relation.urihttps://journals.aps.org/prl/abstract/10.1103/PhysRevLett.61.1147
dc.rights© 1988, American Physical Societyen
dc.subjectCosmic censorship hypothesisen
dc.subjectTrapped surfacesen
dc.subjectSpherical Starsen
dc.titleTrapped surfaces in spherical starsen
dc.typeArticle (peer-reviewed)en
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