Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/3151
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dc.contributor.authorSamuel, J.-
dc.contributor.authorRoy Chowdhury, Sutirtha-
dc.date.accessioned2007-06-26T10:53:54Z-
dc.date.available2007-06-26T10:53:54Z-
dc.date.issued2007-06-07-
dc.identifier.citationClassical and Quantum Gravity, 2007, Vol.24, pF47-F54en
dc.identifier.issn0264-9381-
dc.identifier.issn1361-6382 (Online)-
dc.identifier.urihttp://hdl.handle.net/2289/3151-
dc.descriptionRestricted Access.en
dc.description.abstractPerelman has given a gradient formulation for the Ricci flow, introducing an 'entropy function' which increases monotonically along the flow. We pursue a thermodynamic analogy and apply Ricci flow ideas to general relativity. We investigate whether Perelman's entropy is related to (Bekenstein–Hawking) geometric entropy as familiar from black hole thermodynamics. From a study of the fixed points of the flow, we conclude that Perelman entropy is not connected to geometric entropy. However, we note that there is a very similar flow which does appear to be connected to geometric entropy. The new flow may find applications in black hole physics suggesting, for instance, new approaches to the Penrose inequality.en
dc.format.extent154675 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIOP Publishing Ltd.en
dc.relation.urihttp://dx.doi.org/10.1088/0264-9381/24/11/F01en
dc.rights2007 IOP Publishing Ltd.en
dc.titleGeometric flows and black hole entropyen
dc.typeArticleen
Appears in Collections:Research Papers (TP)

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