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Main Authors: He, Song, Li, Li, Wang, Sai, Wang, Shao-Jiang
Format: Preprint
Published: 2023
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Online Access:https://arxiv.org/abs/2308.07257
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author He, Song
Li, Li
Wang, Sai
Wang, Shao-Jiang
author_facet He, Song
Li, Li
Wang, Sai
Wang, Shao-Jiang
contents The underlying physics of QCD phase transition in the early Universe remains largely unknown due to its strong-coupling nature during the quark-gluon plasma/hadron gas transition, yet a holographic model has been proposed to quantitatively fit the lattice QCD data while with its duration of the first-order phase transition (FoPT) left undetermined. At specific baryon chemical potential, the first-order QCD phase transition agrees with the observational constraint of baryon asymmetry. It, therefore, provides a scenario for phase transition gravitational waves (GWs) within the Standard Model of particle physics. If these background GWs could contribute dominantly to the recently claimed common-spectrum red noise from pulsar timing array (PTA) observations, the duration of this FoPT can be well constrained, and the associated primordial black holes are still allowed by current observations.
format Preprint
id arxiv_https___arxiv_org_abs_2308_07257
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Constraints on holographic QCD phase transitions from PTA observations
He, Song
Li, Li
Wang, Sai
Wang, Shao-Jiang
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
The underlying physics of QCD phase transition in the early Universe remains largely unknown due to its strong-coupling nature during the quark-gluon plasma/hadron gas transition, yet a holographic model has been proposed to quantitatively fit the lattice QCD data while with its duration of the first-order phase transition (FoPT) left undetermined. At specific baryon chemical potential, the first-order QCD phase transition agrees with the observational constraint of baryon asymmetry. It, therefore, provides a scenario for phase transition gravitational waves (GWs) within the Standard Model of particle physics. If these background GWs could contribute dominantly to the recently claimed common-spectrum red noise from pulsar timing array (PTA) observations, the duration of this FoPT can be well constrained, and the associated primordial black holes are still allowed by current observations.
title Constraints on holographic QCD phase transitions from PTA observations
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2308.07257