Classical and quantum gravity of brane black holes

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dc.creatorGregory, Ruth
dc.creatorRoss, Simon F.
dc.creatorZegers, Robin
dc.date2008-02-14
dc.date.accessioned2026-07-07T11:56:03Z
dc.date.available2026-07-07T11:56:03Z
dc.descriptionWe test the holographic conjecture for brane black holes: that a full classical 5D solution will correspond to a quantum corrected 4D black hole. We show that a Schwarzschild-AdS black string in the bulk can be consistently interpreted as a quantum-corrected black hole on the brane, but the form of the quantum corrections is unlike what we would expect. The stress tensor extracted from the bulk solution does not have a thermal component corresponding to Hawking radiation outside the black hole. We compare this strong coupling prediction to a weak coupling calculation to study the differences in detail. We comment on implications for asymptotically flat black holes and for black holes localised in the extra dimension.
dc.description5 pages
dc.identifierhttps://arxiv.org/abs/0802.2037
dc.identifierhttp://arxiv.org/abs/0802.2037
dc.identifierJHEP0809:029,2008
dc.identifierdoi:10.1088/1126-6708/2008/09/029
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/205454
dc.subjectHigh Energy Physics - Theory
dc.titleClassical and quantum gravity of brane black holes
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