Finite temperature resolution of the Klebanov-Tseytlin singularity

Preprint

24 November 2000

preprint
Published by arXiv in arXiv

Abstract

Naked 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.

Keywords

TSEYTLIN SINGULARITY
NAKED SINGULARITIES
FINITE TEMPERATURE
KLEBANOV TSEYTLIN
GRAVITATIONAL
BLACK HOLE
CHIRAL

All Related Versions

Version 1, 2000-11-16, ArXiv
Version 2, 2000-11-24, ArXiv
Version 3, 2001-02-19, ArXiv
Published version: Nuclear Physics B, 600 (2), 219.

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