Thermal production of astrophobic axions

Abstract Hot axions are produced in the early Universe via their interactions with Standard Model particles, contributing to dark radiation commonly parameterized as ∆N eff. In standard QCD axion benchmark models, this contribution to ∆N eff is negligible after taking into account astrophysical limi...

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Main Authors: Marcin Badziak, Keisuke Harigaya, Michał Łukawski, Robert Ziegler
Format: Article
Language:English
Published: SpringerOpen 2024-09-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP09(2024)136
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author Marcin Badziak
Keisuke Harigaya
Michał Łukawski
Robert Ziegler
author_facet Marcin Badziak
Keisuke Harigaya
Michał Łukawski
Robert Ziegler
author_sort Marcin Badziak
collection DOAJ
description Abstract Hot axions are produced in the early Universe via their interactions with Standard Model particles, contributing to dark radiation commonly parameterized as ∆N eff. In standard QCD axion benchmark models, this contribution to ∆N eff is negligible after taking into account astrophysical limits such as the SN1987A bound. We therefore compute the axion contribution to ∆N eff in so-called astrophobic axion models characterized by strongly suppressed axion couplings to nucleons and electrons, in which astrophysical constraints are relaxed and ∆N eff may be sizable. We also construct new astrophobic models in which axion couplings to photons and/or muons are suppressed as well, allowing for axion masses as large as few eV. Most astrophobic models are within the reach of CMB-S4, while some allow for ∆N eff as large as the current upper bound from Planck and thus will be probed by the Simons Observatory. The majority of astrophobic axion models predicting large ∆N eff is also within the reach of IAXO or even BabyIAXO.
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institution Kabale University
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spelling doaj-art-44fc0010db0f4baa8acec6acf42b0a7f2024-12-08T12:16:40ZengSpringerOpenJournal of High Energy Physics1029-84792024-09-012024915210.1007/JHEP09(2024)136Thermal production of astrophobic axionsMarcin Badziak0Keisuke Harigaya1Michał Łukawski2Robert Ziegler3Institute of Theoretical Physics, Faculty of Physics, University of WarsawDepartment of Physics, University of ChicagoInstitute of Theoretical Physics, Faculty of Physics, University of WarsawInstitut für Theoretische Teilchenphysik, Karlsruhe Institute of TechnologyAbstract Hot axions are produced in the early Universe via their interactions with Standard Model particles, contributing to dark radiation commonly parameterized as ∆N eff. In standard QCD axion benchmark models, this contribution to ∆N eff is negligible after taking into account astrophysical limits such as the SN1987A bound. We therefore compute the axion contribution to ∆N eff in so-called astrophobic axion models characterized by strongly suppressed axion couplings to nucleons and electrons, in which astrophysical constraints are relaxed and ∆N eff may be sizable. We also construct new astrophobic models in which axion couplings to photons and/or muons are suppressed as well, allowing for axion masses as large as few eV. Most astrophobic models are within the reach of CMB-S4, while some allow for ∆N eff as large as the current upper bound from Planck and thus will be probed by the Simons Observatory. The majority of astrophobic axion models predicting large ∆N eff is also within the reach of IAXO or even BabyIAXO.https://doi.org/10.1007/JHEP09(2024)136Axions and ALPsCosmology of Theories BSM
spellingShingle Marcin Badziak
Keisuke Harigaya
Michał Łukawski
Robert Ziegler
Thermal production of astrophobic axions
Journal of High Energy Physics
Axions and ALPs
Cosmology of Theories BSM
title Thermal production of astrophobic axions
title_full Thermal production of astrophobic axions
title_fullStr Thermal production of astrophobic axions
title_full_unstemmed Thermal production of astrophobic axions
title_short Thermal production of astrophobic axions
title_sort thermal production of astrophobic axions
topic Axions and ALPs
Cosmology of Theories BSM
url https://doi.org/10.1007/JHEP09(2024)136
work_keys_str_mv AT marcinbadziak thermalproductionofastrophobicaxions
AT keisukeharigaya thermalproductionofastrophobicaxions
AT michałłukawski thermalproductionofastrophobicaxions
AT robertziegler thermalproductionofastrophobicaxions