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dc.contributor.authorMou, Zonggang
dc.contributor.authorSaffin, Paul M.
dc.contributor.authorTranberg, Anders
dc.date.accessioned2018-04-10T07:39:54Z
dc.date.available2018-04-10T07:39:54Z
dc.date.created2017-11-21T10:23:16Z
dc.date.issued2017-07
dc.identifier.citationMou, Z., Saffin, P.M., Tranberg, A. (2017) Simulations of Cold Electroweak Baryogenesis: finding the optimal quench time. Journal of High Energy Physicsnb_NO
dc.identifier.issn1029-8479
dc.identifier.urihttp://hdl.handle.net/11250/2493321
dc.description.abstractWe revisit the numerical computation of the baryon asymmetry from Cold Electroweak Baryogenesis given the physical Higgs mass. We investigate the dependence of the asymmetry on the speed at which electroweak symmetry breaking takes place. The maximum asymmetry does not occur for arbitrarily fast quenches, but at quench times of about τ q  ≃ 16m H − 1 , with no asymmetry created for quenches slower than τ q  > 30m H − 1 . Curiously, we also find that the overall sign of the asymmetry depends on the quench time.nb_NO
dc.language.isoengnb_NO
dc.publisherSpringer Verlagnb_NO
dc.rightsNavngivelse 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/deed.no*
dc.subjectfysikknb_NO
dc.subjectcsmology of teories beyond the SMnb_NO
dc.subjectlattice quantum field theorynb_NO
dc.subjectnonperturbative effectsnb_NO
dc.titleSimulations of Cold Electroweak Baryogenesis: finding the optimal quench timenb_NO
dc.typeJournal articlenb_NO
dc.typePeer reviewednb_NO
dc.description.versionpublishedVersionnb_NO
dc.subject.nsiVDP::Matematikk og Naturvitenskap: 400::Fysikk: 430nb_NO
dc.source.volume2017nb_NO
dc.source.journalJournal of High Energy Physics (JHEP)nb_NO
dc.source.issue7nb_NO
dc.identifier.doi10.1007/JHEP07(2017)010
dc.identifier.cristin1516489
dc.relation.projectNotur/NorStore: NN9275Knb_NO
cristin.unitcode217,8,2,0
cristin.unitnameInstitutt for matematikk og naturvitenskap
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2


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