Production of Thermal Axions across the ElectroWeak Phase Transition

dc.contributor.authorArias Aragón, Fernando
dc.contributor.authorD'Eramo, Francesco
dc.contributor.authorFerreira, Ricardo Z.
dc.contributor.authorMerlo, Luca
dc.contributor.authorNotari, Alessio
dc.date.accessioned2026-02-13T09:33:09Z
dc.date.issued2021-03-26
dc.description.abstractLight axions can potentially leave a cosmic background, just like neutrinos. We complete the study of thermal axion production across the electroweak scale by providing a smooth and continuous treatment through the two phases. Focusing on both flavour conserving and violating couplings to third generation quarks, we compute the amount of axions produced via scatterings and decays of thermal bath particles. We perform a model independent analysis in terms of axion effective couplings, and we also make predictions for specific microscopic QCD axion scenarios. This observable effect, parameterized as it is conventional by an effective number of additional neutrinos, is above the 1σ sensitivity of future CMB-S4 surveys. Moreover, if one assumes no large hierarchies among dimensionless axion couplings to standard model particles, future axion helioscopes will provide a complementary probe for the parameter region we study.
dc.identifier.citationFernando Arias-Aragón et al JCAP03(2021)090
dc.identifier.doi10.1088/1475-7516/2021/03/090
dc.identifier.issn1475-7516
dc.identifier.urihttps://hdl.handle.net/10115/166717
dc.language.isoen
dc.publisherIOP Publishing Ltd and Sissa Medialab
dc.rights.accessRightsinfo:eu-repo/semantics/closedAccess
dc.subjectAxions
dc.subjectThermal production
dc.subjectElectroweak phase transition
dc.subjectCosmic Microwave Background
dc.titleProduction of Thermal Axions across the ElectroWeak Phase Transition
dc.typeArticle

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