Holographic phase transition of QCD with back-reaction of flavors
Youngman Kim, Tatsuhiro Misumi, Ik Jae Shin

TL;DR
This paper investigates the confinement/deconfinement transition in holographic QCD by incorporating the back-reaction of a scalar field related to chiral symmetry breaking, analyzing how quark mass and flavor number affect the critical temperature.
Contribution
It introduces a deformed AdS black hole solution accounting for back-reaction of the scalar field, providing a more realistic holographic model of QCD phase transitions.
Findings
Critical temperature depends on quark mass and flavor number.
Unphysical phases from previous models are eliminated with back-reaction.
Results align with lattice QCD observations.
Abstract
We revisit confinement/deconfinement transition in holographic QCD to consider the back-reaction of a bulk scalar field. The bulk scalar field is dual to a quark bi-linear operator , and it encodes explicit and spontaneous chiral symmetry breaking of QCD. To perform the Hawking-Page transition analysis with the back-reaction, we first obtain a deformed AdS black hole solution due to a finite quark mass. Through the Hawking-Page analysis with the back-reacted geometry, we study the flavor number and finite quark mass dependence of the critical temperature of the QCD confinement/deconfinement transition. In addition, we confirm that unphysical QCD phase haunting around in a previous study disappears with the back-reaction. We discuss our results in the light of lattice QCD observations.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Quantum Chromodynamics and Particle Interactions
