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http://hdl.handle.net/2289/1291
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DC Field | Value | Language |
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dc.contributor.author | Kang, Gungwon | - |
dc.date.accessioned | 2006-05-23T11:06:52Z | - |
dc.date.available | 2006-05-23T11:06:52Z | - |
dc.date.issued | 1996-12-15 | - |
dc.identifier.citation | Physical Review D, 1996, Vol.54, 7483-7489 | en |
dc.identifier.issn | 1550-7998 (print) | - |
dc.identifier.uri | http://hdl.handle.net/2289/1291 | - |
dc.description.abstract | We 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.extent | 153214 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | The American Physical Society | en |
dc.relation.uri | http://link.aps.org/abstract/PRD/v54/p7483 | en |
dc.rights | (1996) by the American Physical Society | en |
dc.title | Black hole area in Brans-Dicke theory | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (TP) |
Files in This Item:
File | Description | Size | Format | |
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1996 PhyRevD V54 p7483.pdf | 7p. | 149.62 kB | Adobe PDF | View/Open |
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