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Is the UA(1) symmetry restored at finite temperature or density?

2004/11/24 by Pedro Costa, P. Costa, M. C. Ruivo +2
Physics and Astronomy · #Black Holes and Theoretical Physics #High-Energy Particle Collisions Research #Quantum Chromodynamics and Particle Interactions #hep-ph

paper · pdf · doi:10.1063/1.1920990

published as AIP Conf.Proc. 756 (2005) 351 · 3 pages, 1 figure. Talk given at 6th Conference on Quark Confinement and the Hadron Spectrum, Villasimius, Sardinia, Italy, 21-25 Sep 2004

arxiv created 2004/11/24 · openalex publication_date 2005/01/01 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/29

Abstract

We investigate the full U(3)⊗U(3) chiral symmetry restoration, at finite temperature and density, on the basis of the three flavor Nambu‐Jona‐Lasinio model with the anomaly term given by the ’t Hooft interaction. We implement a temperature (density) dependence of the anomaly coefficient motivated by lattice results for the topological susceptibility. The results suggest that the axial part of the symmetry is restored before the possible restoration of the full U(3)⊗U(3) chiral symmetry can occur.

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