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Restoration of chiral symmetry: A Supergravity perspective

S.S. Gubser
(
- UC, Santa Barbara and
- Caltech and
- Princeton U.
)
,
C.P. Herzog
(
- Princeton U.
)
,
Igor R. Klebanov
(
- UC, Santa Barbara and
- Princeton U.
)
,
Arkady A. Tseytlin
(
- Ohio State U. and
- Imperial Coll., London and
- Lebedev Inst.
)

Feb, 2001

22 pages

Published in:

JHEP 05 (2001) 028

e-Print:

hep-th/0102172 [hep-th]

DOI:

10.1088/1126-6708/2001/05/028

Report number:

PUTP-1978,
OHSTPY-HEP-T-01-003,
NSF-ITP-01-15,
CALT-68-2317,
CITUSC-00-069

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Abstract: (IOP)

The supergravity dual ofNregular andMfractional D3-branes on the conifold has a naked singularity in the infrared. Supersymmetric resolution of this singularity requires deforming the conifold: this is the supergravity dual of chiral symmetry breaking. Buchel suggested that at sufficiently high temperature there is no need to deform the conifold: the singularity may be cloaked by a horizon. This would be the supergravity manifestation of chiral symmetry restoration. In previous work [hep-th/0102105] the ansatz and the system of second-order radial differential equations necessary to find such a solution were written down. In this paper we find smooth solutions to this system in a perturbation theory that is valid when the Hawking temperature of the horizon is very high.

symmetry: chiral
supergravity
finite temperature
field equations: solution
perturbation theory
membrane model
conifold
black hole: horizon
temperature: Hawking

References(25)

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(
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(
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)
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(
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)
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)

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