Finite temperature resolution of the Klebanov-Tseytlin singularity

dc.creatorBuchel, Alex
dc.date2000-11-16
dc.date2001-02-19
dc.date.accessioned2026-07-07T11:31:51Z
dc.date.available2026-07-07T11:31:51Z
dc.descriptionNaked singularities in the gravitational backgrounds dual to gauge theories can be hidden behind the black hole horizon. We present an exact black hole solution in the Klebanov-Tseytlin geometry [hep-th/0002159]. Our solution realizes Maldacena dual of the finite temperature N=1 duality cascade of [hep-th/0007191] above the temperature of the chiral symmetry breaking. We compare the Bekenstein-Hawking entropy of the black hole with the entropy of the SU(N+M)xSU(N) gauge theory.
dc.description25 pages, LaTeX, v2:references added, v3:error identified that led to the incorrect conclusion. A new section and acknowledgements added
dc.identifierhttps://arxiv.org/abs/hep-th/0011146
dc.identifierhttp://arxiv.org/abs/hep-th/0011146
dc.identifierNucl.Phys.B600:219-234,2001
dc.identifierdoi:10.1016/S0550-3213(01)00051-7
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/197405
dc.subjectHigh Energy Physics - Theory
dc.titleFinite temperature resolution of the Klebanov-Tseytlin singularity
dc.typetext

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