Dark confinement-deconfinement phase transition: a roadmap from Polyakov loop models to gravitational waves

Abstract We explore the confinement-deconfinement phase transition (PT) of the first order (FO) arising in SU(N) pure Yang-Mills theory, based on Polyakov loop models (PLMs), in light of the induced gravitational wave (GW) spectra. We demonstrate that the PLMs with the Haar measure term, involving m...

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Main Authors: Zhaofeng Kang, Jiang Zhu, Shinya Matsuzaki
Format: Article
Language:English
Published: SpringerOpen 2021-09-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP09(2021)060
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spelling doaj-a91bce39d0dc46f99389a16dfc6234ed2021-09-19T11:57:06ZengSpringerOpenJournal of High Energy Physics1029-84792021-09-012021912810.1007/JHEP09(2021)060Dark confinement-deconfinement phase transition: a roadmap from Polyakov loop models to gravitational wavesZhaofeng Kang0Jiang Zhu1Shinya Matsuzaki2School of physics, Huazhong University of Science and TechnologySchool of physics, Huazhong University of Science and TechnologyCenter for Theoretical Physics and College of Physics, Jilin UniversityAbstract We explore the confinement-deconfinement phase transition (PT) of the first order (FO) arising in SU(N) pure Yang-Mills theory, based on Polyakov loop models (PLMs), in light of the induced gravitational wave (GW) spectra. We demonstrate that the PLMs with the Haar measure term, involving models successful in QCD with N = 3, are potentially incompatible with the large N scaling for the thermodynamic quantities and the latent heat at around the criticality of the FOPT reported from the lattice simulations. We then propose a couple of models of polynomial form, which we call the 4-6 PLM (with four- and six-point interactions among the basic PL fields which have center charge 1) and 4-8 PLM (with four- and eight-point interactions), and discuss how such models can naturally arise in the presence of a heavy PL with charge 2. We show that those models give the consistent thermodynamic and large N properties at around the criticality. The predicted GW spectra are shown to have high enough sensitivity to be probed in the future prospected interferometers such as BBO and DECIGO.https://doi.org/10.1007/JHEP09(2021)060Phenomenological Models
collection DOAJ
language English
format Article
sources DOAJ
author Zhaofeng Kang
Jiang Zhu
Shinya Matsuzaki
spellingShingle Zhaofeng Kang
Jiang Zhu
Shinya Matsuzaki
Dark confinement-deconfinement phase transition: a roadmap from Polyakov loop models to gravitational waves
Journal of High Energy Physics
Phenomenological Models
author_facet Zhaofeng Kang
Jiang Zhu
Shinya Matsuzaki
author_sort Zhaofeng Kang
title Dark confinement-deconfinement phase transition: a roadmap from Polyakov loop models to gravitational waves
title_short Dark confinement-deconfinement phase transition: a roadmap from Polyakov loop models to gravitational waves
title_full Dark confinement-deconfinement phase transition: a roadmap from Polyakov loop models to gravitational waves
title_fullStr Dark confinement-deconfinement phase transition: a roadmap from Polyakov loop models to gravitational waves
title_full_unstemmed Dark confinement-deconfinement phase transition: a roadmap from Polyakov loop models to gravitational waves
title_sort dark confinement-deconfinement phase transition: a roadmap from polyakov loop models to gravitational waves
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2021-09-01
description Abstract We explore the confinement-deconfinement phase transition (PT) of the first order (FO) arising in SU(N) pure Yang-Mills theory, based on Polyakov loop models (PLMs), in light of the induced gravitational wave (GW) spectra. We demonstrate that the PLMs with the Haar measure term, involving models successful in QCD with N = 3, are potentially incompatible with the large N scaling for the thermodynamic quantities and the latent heat at around the criticality of the FOPT reported from the lattice simulations. We then propose a couple of models of polynomial form, which we call the 4-6 PLM (with four- and six-point interactions among the basic PL fields which have center charge 1) and 4-8 PLM (with four- and eight-point interactions), and discuss how such models can naturally arise in the presence of a heavy PL with charge 2. We show that those models give the consistent thermodynamic and large N properties at around the criticality. The predicted GW spectra are shown to have high enough sensitivity to be probed in the future prospected interferometers such as BBO and DECIGO.
topic Phenomenological Models
url https://doi.org/10.1007/JHEP09(2021)060
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