Thermal phase transition in a QCD-like holographic model
Creators
- 1. School of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ (United Kingdom)
Description
We investigate the high-temperature phase of a dilaton flow deformation of the anti-de Sitter/conformal field theory correspondence. We argue that these geometries should be interpreted as the N=4 gauge theory perturbed by a SO(6) invariant scalar mass and that the high-temperature phase is just the well-known anti-de Sitter-Schwarzschild solution. We compute, within supergravity, the resulting Hawking-Page phase transition, which in this model can be interpreted as a deconfining transition in which the vacuum expectation value for the operator TrF2 dissolves. In the presence of quarks the model also displays a simultaneous chiral symmetry restoring transition with the Goldstone mode and other quark bound states dissolving into the thermal bath.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.78.105020;
- arXiv
- arXiv:0805.0956v3;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 78
- Journal Issue
- 10
- Journal Page Range
- p. 105020-105020.9
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41002280
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- BOUND STATE; CHIRAL SYMMETRY; CONFORMAL INVARIANCE; DE SITTER GROUP; DEFORMATION; EXPECTATION VALUE; GAUGE INVARIANCE; HOLOGRAPHY; MASS; PHASE TRANSFORMATIONS; QUANTUM CHROMODYNAMICS; QUANTUM FIELD THEORY; QUARK MODEL; QUARKS; SCHWARZSCHILD METRIC; SIMULATION; SO-6 GROUPS; STRING MODELS; SUPERGRAVITY
- Descriptors DEC
- COMPOSITE MODELS; EXTENDED PARTICLE MODEL; FERMIONS; FIELD THEORIES; INVARIANCE PRINCIPLES; LIE GROUPS; MATHEMATICAL MODELS; METRICS; PARTICLE MODELS; QUANTUM FIELD THEORY; QUARK MODEL; SO GROUPS; SYMMETRY; SYMMETRY GROUPS; UNIFIED-FIELD THEORIES
Optional Information
- Notes
- (c) 2008 The American Physical Society