Late time behavior of the maximal slicing of the Schwarzschild black hole

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dc.contributor.authorBeig, Robert
dc.contributor.authorÓ Murchadha, Niall
dc.date.accessioned2017-08-29T09:14:25Z
dc.date.available2017-08-29T09:14:25Z
dc.date.issued1998
dc.description.abstractA time-symmetric Cauchy slice of the extended Schwarzschild spacetime can evolve into a foliation of the r>3m/2 region of spacetime by maximal surfaces with the requirement that time run equally fast at both spatial ends of the manifold. This paper studies the behavior of these slices in the limit as proper time at infinity becomes arbitrarily large. It is shown that the central lapse decays exponentially and an analytic expression is given both for the exponent and for the preexponential factor.en
dc.description.statusPeer revieweden
dc.description.versionPublished Versionen
dc.format.mimetypeapplication/pdfen
dc.identifier.citationBeig, R. and Ó Murchadha, N. (1998) 'Late time behavior of the maximal slicing of the Schwarzschild black hole', Physical Review D, 57(8), 4728-4737 (10pp). doi: 10.1103/PhysRevD.57.4728en
dc.identifier.doi10.1103/PhysRevD.57.4728
dc.identifier.endpage4737
dc.identifier.issn0556-2821
dc.identifier.issued8
dc.identifier.journaltitlePhysical Review Den
dc.identifier.startpage4728
dc.identifier.urihttps://hdl.handle.net/10468/4581
dc.identifier.volume57
dc.language.isoenen
dc.publisherAmerican Physical Societyen
dc.relation.urihttps://journals.aps.org/prd/abstract/10.1103/PhysRevD.57.4728
dc.rights© 1998, American Physical Societyen
dc.subjectTrapped surfacesen
dc.subjectVacuum spacetimesen
dc.subjectRelativityen
dc.titleLate time behavior of the maximal slicing of the Schwarzschild black holeen
dc.typeArticle (peer-reviewed)en
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