QCD axion dark matter from a late time phase transition

Abstract We investigate the possibility that the Peccei-Quinn phase transition occurs at a temperature far below the symmetry breaking scale. Low phase transition temperatures are typical in supersymmetric theories, where symmetry breaking fields have small masses. We find that QCD axions are abunda...

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Main Authors: Keisuke Harigaya, Jacob M. Leedom
Format: Article
Language:English
Published: SpringerOpen 2020-06-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP06(2020)034
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author Keisuke Harigaya
Jacob M. Leedom
author_facet Keisuke Harigaya
Jacob M. Leedom
author_sort Keisuke Harigaya
collection DOAJ
description Abstract We investigate the possibility that the Peccei-Quinn phase transition occurs at a temperature far below the symmetry breaking scale. Low phase transition temperatures are typical in supersymmetric theories, where symmetry breaking fields have small masses. We find that QCD axions are abundantly produced just after the phase transition. The observed dark matter abundance is reproduced even if the decay constant is much lower than 1011 GeV. The produced axions tend to be warm. For some range of the decay constant, the effect of the predicted warmness on structure formation can be confirmed by future observations of 21 cm lines. A portion of parameter space requires a mixing between the Peccei-Quinn symmetry breaking field and the Standard Model Higgs, and predicts an observable rate of rare Kaon decays.
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spelling doaj.art-7a1449d7ecd94b3bb488b1f8518c0b982022-12-21T17:50:22ZengSpringerOpenJournal of High Energy Physics1029-84792020-06-012020611810.1007/JHEP06(2020)034QCD axion dark matter from a late time phase transitionKeisuke Harigaya0Jacob M. Leedom1School of Natural Sciences, Institute for Advanced StudyDepartment of Physics, University of CaliforniaAbstract We investigate the possibility that the Peccei-Quinn phase transition occurs at a temperature far below the symmetry breaking scale. Low phase transition temperatures are typical in supersymmetric theories, where symmetry breaking fields have small masses. We find that QCD axions are abundantly produced just after the phase transition. The observed dark matter abundance is reproduced even if the decay constant is much lower than 1011 GeV. The produced axions tend to be warm. For some range of the decay constant, the effect of the predicted warmness on structure formation can be confirmed by future observations of 21 cm lines. A portion of parameter space requires a mixing between the Peccei-Quinn symmetry breaking field and the Standard Model Higgs, and predicts an observable rate of rare Kaon decays.http://link.springer.com/article/10.1007/JHEP06(2020)034Beyond Standard ModelCosmology of Theories beyond the SM
spellingShingle Keisuke Harigaya
Jacob M. Leedom
QCD axion dark matter from a late time phase transition
Journal of High Energy Physics
Beyond Standard Model
Cosmology of Theories beyond the SM
title QCD axion dark matter from a late time phase transition
title_full QCD axion dark matter from a late time phase transition
title_fullStr QCD axion dark matter from a late time phase transition
title_full_unstemmed QCD axion dark matter from a late time phase transition
title_short QCD axion dark matter from a late time phase transition
title_sort qcd axion dark matter from a late time phase transition
topic Beyond Standard Model
Cosmology of Theories beyond the SM
url http://link.springer.com/article/10.1007/JHEP06(2020)034
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