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dc.contributor.authorCline, James M.
dc.contributor.authorKainulainen, Kimmo
dc.date.accessioned2020-03-24T05:40:19Z
dc.date.available2020-03-24T05:40:19Z
dc.date.issued2020
dc.identifier.citationCline, J. M., & Kainulainen, K. (2020). Electroweak baryogenesis at high bubble wall velocities. <i>Physical Review D</i>, <i>101</i>(6), Article 063525. <a href="https://doi.org/10.1103/PhysRevD.101.063525" target="_blank">https://doi.org/10.1103/PhysRevD.101.063525</a>
dc.identifier.otherCONVID_35093145
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/68287
dc.description.abstractIt is widely believed that electroweak baryogenesis should be suppressed in strong phase transitions with fast-moving bubble walls, but this effect has never been quantitatively studied. We rederive fluid equations describing transport of particle asymmetries near the bubble wall without making the small-wall-velocity approximation. We show that the suppression of the baryon asymmetry is a smooth function of the wall speed and that there is no special behavior when crossing the sound speed barrier. Electroweak baryogenesis can thus be efficient also with strong detonations, generically associated with models with observably large gravitational waves. We also make a systematic and critical comparison of our improved transport equations to another one commonly used in the literature, based on the vacuum expectation value (VEV)-insertion formalism.en
dc.format.mimetypeapplication/pdf
dc.languageeng
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review D
dc.rightsCC BY 4.0
dc.subject.otherbaryogenesis
dc.subject.otherleptogenesis
dc.titleElectroweak baryogenesis at high bubble wall velocities
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202003242515
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn2470-0010
dc.relation.numberinseries6
dc.relation.volume101
dc.type.versionpublishedVersion
dc.rights.copyright© Authors, 2020
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber318319
dc.subject.ysoastrofysiikka
dc.subject.ysokosmologia
dc.subject.ysohiukkasfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p20188
jyx.subject.urihttp://www.yso.fi/onto/yso/p7160
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1103/PhysRevD.101.063525
dc.relation.funderResearch Council of Finlanden
dc.relation.funderSuomen Akatemiafi
jyx.fundingprogramAcademy Project, AoFen
jyx.fundingprogramAkatemiahanke, SAfi
jyx.fundinginformationThis work was supported by the Academy of Finland Grant No. 318319 and NSERC (Natural Sciences and Engineering Research Council, Canada).
dc.type.okmA1


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