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dc.contributor.authorDenef, Frederik
dc.contributor.authorMoore, Gregory W.
dc.date.accessioned2009-07-02T17:29:05Z
dc.date.issued2007
dc.identifier.citationDenef, Frederik, and Gregory W. Moore. 2007. How many black holes fit on the head of a pin? General Relativity and Gravitation 39(10): 1539-1544.en
dc.identifier.issn0001-7701en
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:3138326
dc.description.abstractThe Bekenstein–Hawking entropy of certain black holes can be computed microscopically in string theory by mapping the elusive problem of counting microstates of a strongly gravitating black hole to the tractable problem of counting microstates of a weakly coupled D-brane system, which has no event horizon, and indeed comfortably fits on the head of a pin. We show here that, contrary to widely held beliefs, the entropy of spherically symmetric black holes can easily be dwarfed by that of stationary multi-black-hole “molecules” of the same total charge and energy. Thus, the corresponding pin-sized D-brane systems do not even approximately count the microstates of a single black hole, but rather those of a zoo of entropically dominant multicentered configurations.en
dc.description.sponsorshipMathematicsen
dc.description.sponsorshipPhysicsen
dc.language.isoen_USen
dc.publisherSpringer Verlagen
dc.relation.isversionofhttp://dx.doi.org/10.1007/s10714-007-0469-4en
dc.relation.hasversionhttp://arxiv.org/PS_cache/arxiv/pdf/0705/0705.2564v1.pdfen
dash.licenseLAA
dc.titleHow Many Black Holes Fit on the Head of a Pin?en
dc.relation.journalGeneral Relativity and Gravitationen
dash.depositing.authorDenef, Frederik
dc.identifier.doi10.1007/s10714-007-0469-4*
dash.contributor.affiliatedDenef, Frederik


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