Finite temperature resolution of the Klebanov-Tseytlin singularity
Alex Buchel
TL;DR
This paper presents an exact black hole solution in the Klebanov-Tseytlin geometry, demonstrating how finite temperature effects can resolve singularities in the dual gauge theory backgrounds.
Contribution
It introduces a novel black hole solution that models finite temperature effects in the Klebanov-Tseytlin background, extending the understanding of gauge/gravity duality at non-zero temperature.
Findings
Black hole solution in Klebanov-Tseytlin geometry
Entropy comparison between gravity and gauge theory
Resolution of singularities at finite temperature
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.
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