Topology in the SU(Nf) chiral symmetry restored phase of unquenched QCD and axion cosmology

The axion is one of the more interesting candidates to make the dark matter of the universe, and the axion potential plays a fundamental role in the determination of the dynamics of the axion field. Moreover, the way in which the U(1)A anomaly manifests itself in the chiral symmetry restored phase o...

Full description

Bibliographic Details
Main Author: Azcoiti Vicente
Format: Article
Language:English
Published: EDP Sciences 2018-01-01
Series:EPJ Web of Conferences
Online Access:https://doi.org/10.1051/epjconf/201817504007
_version_ 1819132236880936960
author Azcoiti Vicente
author_facet Azcoiti Vicente
author_sort Azcoiti Vicente
collection DOAJ
description The axion is one of the more interesting candidates to make the dark matter of the universe, and the axion potential plays a fundamental role in the determination of the dynamics of the axion field. Moreover, the way in which the U(1)A anomaly manifests itself in the chiral symmetry restored phase of QCD at high temperature could be tested when probing the QCD phase transition in relativistic heavy ion collisions. With these motivations, we investigate the physical consequences of the survival of the effects of the U(1)A anomaly in the chiral symmetric phase of QCD, and show that the free energy density is a singular function of the quark mass m, in the chiral limit, and that the σ and π susceptibilities diverge in this limit at any T ≥ Tc. We also show that the difference between the π and δ susceptibilities diverges in the chiral limit at any T ≥ Tc, a result that can be contrasted with the existing lattice calculations; and discuss on the generalization of these results to the Nf ≥ 3 model.
first_indexed 2024-12-22T09:28:12Z
format Article
id doaj.art-3d59c61c705349b3b824f38b360f49f6
institution Directory Open Access Journal
issn 2100-014X
language English
last_indexed 2024-12-22T09:28:12Z
publishDate 2018-01-01
publisher EDP Sciences
record_format Article
series EPJ Web of Conferences
spelling doaj.art-3d59c61c705349b3b824f38b360f49f62022-12-21T18:31:01ZengEDP SciencesEPJ Web of Conferences2100-014X2018-01-011750400710.1051/epjconf/201817504007epjconf_lattice2018_04007Topology in the SU(Nf) chiral symmetry restored phase of unquenched QCD and axion cosmologyAzcoiti VicenteThe axion is one of the more interesting candidates to make the dark matter of the universe, and the axion potential plays a fundamental role in the determination of the dynamics of the axion field. Moreover, the way in which the U(1)A anomaly manifests itself in the chiral symmetry restored phase of QCD at high temperature could be tested when probing the QCD phase transition in relativistic heavy ion collisions. With these motivations, we investigate the physical consequences of the survival of the effects of the U(1)A anomaly in the chiral symmetric phase of QCD, and show that the free energy density is a singular function of the quark mass m, in the chiral limit, and that the σ and π susceptibilities diverge in this limit at any T ≥ Tc. We also show that the difference between the π and δ susceptibilities diverges in the chiral limit at any T ≥ Tc, a result that can be contrasted with the existing lattice calculations; and discuss on the generalization of these results to the Nf ≥ 3 model.https://doi.org/10.1051/epjconf/201817504007
spellingShingle Azcoiti Vicente
Topology in the SU(Nf) chiral symmetry restored phase of unquenched QCD and axion cosmology
EPJ Web of Conferences
title Topology in the SU(Nf) chiral symmetry restored phase of unquenched QCD and axion cosmology
title_full Topology in the SU(Nf) chiral symmetry restored phase of unquenched QCD and axion cosmology
title_fullStr Topology in the SU(Nf) chiral symmetry restored phase of unquenched QCD and axion cosmology
title_full_unstemmed Topology in the SU(Nf) chiral symmetry restored phase of unquenched QCD and axion cosmology
title_short Topology in the SU(Nf) chiral symmetry restored phase of unquenched QCD and axion cosmology
title_sort topology in the su nf chiral symmetry restored phase of unquenched qcd and axion cosmology
url https://doi.org/10.1051/epjconf/201817504007
work_keys_str_mv AT azcoitivicente topologyinthesunfchiralsymmetryrestoredphaseofunquenchedqcdandaxioncosmology