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Auteurs principaux: Zhu, Zhou-Run, Chen, Jun, Hou, Defu
Format: Preprint
Publié: 2021
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Accès en ligne:https://arxiv.org/abs/2109.09933
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author Zhu, Zhou-Run
Chen, Jun
Hou, Defu
author_facet Zhu, Zhou-Run
Chen, Jun
Hou, Defu
contents In this paper, we discuss the holographic first order QCD phase transition with gluon condensate and the generation of gravitational waves (GWs) from the phase transition. The first order QCD phase transition is dual to the first order Hawking-Page phase transition from holography. We study the first order Hawking-Page phase transition from the thermal dilatonic phase to the dilatonic black hole phase and find the phase transition temperature is proportional to the gluon condensate. After substituting into the phenomenological value of gluon condensate from QCD sum rules, we find $T_c=155.38\ MeV$. In further research, we study the GWs generated from holographic cosmic first order QCD phase transition with gluon condensate and the produced GWs might be detected by the International Pulsar Timing Array, Square Kilometre Array and Big-Bang Observer. Moreover, the gluon condensate suppresses the energy density of total GWs and peak frequency.
format Preprint
id arxiv_https___arxiv_org_abs_2109_09933
institution arXiv
publishDate 2021
record_format arxiv
spellingShingle Gravitational waves from holographic QCD phase transition with gluon condensate
Zhu, Zhou-Run
Chen, Jun
Hou, Defu
High Energy Physics - Phenomenology
In this paper, we discuss the holographic first order QCD phase transition with gluon condensate and the generation of gravitational waves (GWs) from the phase transition. The first order QCD phase transition is dual to the first order Hawking-Page phase transition from holography. We study the first order Hawking-Page phase transition from the thermal dilatonic phase to the dilatonic black hole phase and find the phase transition temperature is proportional to the gluon condensate. After substituting into the phenomenological value of gluon condensate from QCD sum rules, we find $T_c=155.38\ MeV$. In further research, we study the GWs generated from holographic cosmic first order QCD phase transition with gluon condensate and the produced GWs might be detected by the International Pulsar Timing Array, Square Kilometre Array and Big-Bang Observer. Moreover, the gluon condensate suppresses the energy density of total GWs and peak frequency.
title Gravitational waves from holographic QCD phase transition with gluon condensate
topic High Energy Physics - Phenomenology
url https://arxiv.org/abs/2109.09933