dc.contributor.author | Cline, James M. | |
dc.contributor.author | Kainulainen, Kimmo | |
dc.contributor.author | Tucker-Smith, David | |
dc.date.accessioned | 2017-07-04T09:36:01Z | |
dc.date.available | 2017-07-04T09:36:01Z | |
dc.date.issued | 2017 | |
dc.identifier.citation | Cline, 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.other | CONVID_27056177 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/54832 | |
dc.description.abstract | Adding 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.iso | eng | |
dc.publisher | American Physical Society | |
dc.relation.ispartofseries | Physical Review D | |
dc.subject.other | hiukkasfysiikan standardimalli | |
dc.subject.other | pimeä aine | |
dc.subject.other | standard model of particle physics | |
dc.subject.other | dark matter | |
dc.title | Electroweak baryogenesis from a dark sector | |
dc.type | research article | |
dc.identifier.urn | URN:NBN:fi:jyu-201706283097 | |
dc.contributor.laitos | Fysiikan laitos | fi |
dc.contributor.laitos | Department of Physics | en |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | |
dc.date.updated | 2017-06-28T03:16:08Z | |
dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
dc.description.reviewstatus | peerReviewed | |
dc.relation.issn | 2470-0010 | |
dc.relation.numberinseries | 11 | |
dc.relation.volume | 95 | |
dc.type.version | publishedVersion | |
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.accesslevel | openAccess | fi |
dc.type.publication | article | |
dc.subject.yso | pimeä aine | |
dc.subject.yso | hiukkasfysiikan standardimalli | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p14101 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p27292 | |
dc.rights.url | https://creativecommons.org/licenses/by/4.0/ | |
dc.relation.doi | 10.1103/PhysRevD.95.115006 | |
dc.type.okm | A1 | |