Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1291
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dc.contributor.authorKang, Gungwon-
dc.date.accessioned2006-05-23T11:06:52Z-
dc.date.available2006-05-23T11:06:52Z-
dc.date.issued1996-12-15-
dc.identifier.citationPhysical Review D, 1996, Vol.54, 7483-7489en
dc.identifier.issn1550-7998 (print)-
dc.identifier.urihttp://hdl.handle.net/2289/1291-
dc.description.abstractWe show that the dynamics of the scalar field φ(x)=``G-1(x)'' in Brans-Dicke theories of gravity makes the surface area of the black hole horizon oscillatory during its dynamical evolution. It explicitly explains why the area theorem does not hold in Brans-Dicke theory. However, we show that there exists a certain nondecreasing quantity defined on the event horizon which is proportional to the black hole entropy for the case of stationary solutions in Brans-Dicke theory. Some numerical simulations are demonstrated for Oppenheimer-Snyder collapse in Brans-Dicke theory.en
dc.format.extent153214 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe American Physical Societyen
dc.relation.urihttp://link.aps.org/abstract/PRD/v54/p7483en
dc.rights(1996) by the American Physical Societyen
dc.titleBlack hole area in Brans-Dicke theoryen
dc.typeArticleen
Appears in Collections:Research Papers (TP)

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