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dc.contributor.authorCline, James M.
dc.contributor.authorKainulainen, Kimmo
dc.contributor.authorTucker-Smith, David
dc.date.accessioned2017-07-04T09:36:01Z
dc.date.available2017-07-04T09:36:01Z
dc.date.issued2017
dc.identifier.citationCline, J. M., Kainulainen, K., & Tucker-Smith, D. (2017). Electroweak baryogenesis from a dark sector. <i>Physical Review D</i>, <i>95</i>(11), Article 115006. <a href="https://doi.org/10.1103/PhysRevD.95.115006" target="_blank">https://doi.org/10.1103/PhysRevD.95.115006</a>
dc.identifier.otherCONVID_27056177
dc.identifier.otherTUTKAID_74084
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/54832
dc.description.abstractAdding an extra singlet scalar S to the Higgs sector can provide a barrier at tree level between a false vacuum with restored electroweak symmetry and the true one. This has been demonstrated to readily give a strong phase transition as required for electroweak baryogenesis. We show that with the addition of a fermionic dark matter particle χ coupling to S, a simple UV-complete model can realize successful electroweak baryogenesis. The dark matter gets a CP asymmetry that is transferred to the standard model through a CP portal interaction, which we take to be a coupling of χ to τ leptons and an inert Higgs doublet. The CP asymmetry induced in left-handed τ leptons biases sphalerons to produce the baryon asymmetry. The model has promising discovery potential at the LHC, while robustly providing a large enough baryon asymmetry and correct dark matter relic density with reasonable values of the couplings.en
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review D
dc.subject.otherhiukkasfysiikan standardimalli
dc.subject.otherpimeä aine
dc.subject.otherstandard model of particle physics
dc.subject.otherdark matter
dc.titleElectroweak baryogenesis from a dark sector
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201706283097
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2017-06-28T03:16:08Z
dc.type.coarjournal article
dc.description.reviewstatuspeerReviewed
dc.relation.issn2470-0010
dc.relation.numberinseries11
dc.relation.volume95
dc.type.versionpublishedVersion
dc.rights.copyright© the Authors, 2017. Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license.
dc.rights.accesslevelopenAccessfi
dc.subject.ysopimeä aine
dc.subject.ysohiukkasfysiikan standardimalli
jyx.subject.urihttp://www.yso.fi/onto/yso/p14101
jyx.subject.urihttp://www.yso.fi/onto/yso/p27292
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1103/PhysRevD.95.115006


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© the Authors, 2017. Published by the American Physical Society under the terms of
the Creative Commons Attribution 4.0 International license.
Except where otherwise noted, this item's license is described as © the Authors, 2017. Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license.