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Enlarging the window for radiative leptogenesis

dc.contributor.authorBranco, G. C.
dc.contributor.authorFelipe, Ricardo Gonzalez
dc.contributor.authorJoaquim, F. R.
dc.contributor.authorNobre, B.M.
dc.date.accessioned2014-05-30T16:00:04Z
dc.date.available2014-05-30T16:00:04Z
dc.date.issued2006-02-09
dc.description.abstractWe investigate the scenario of resonant thermal leptogenesis, in which the leptonic asymmetries are generated through renormalization group corrections induced at the leptogenesis scale. In the framework of the standard model extended by three heavy Majorana neutrinos with masses M(1) = M(2) << M(3) at some high scale, we show that the mass splitting and CP-violating effects induced by renormalization group corrections can lead to values of the CP asymmetries large enough for a successful leptogenesis. In this scenario, the low-energy neutrino oscillation data can also be easily accommodated. The possibility of having an underlying symmetry behind the degeneracy in the right-handed neutrino mass spectrum is also discussed. (c) 2005 Elsevier B.V. All rights reserved.por
dc.identifier.citationBRANCO, G. C.; FELIPE, R. G.; JOAQUIM, F. R.; NOBRE, B. M. - Enlarging the window for radiative leptogenesis. Physics Letters B. ISSN 0370-2693. Vol. 633, nr. 2-3 (2006), p. 336.344.por
dc.identifier.issn0370-2693
dc.identifier.other10.1016/j.physletb.2005.11.070
dc.identifier.urihttp://hdl.handle.net/10400.21/3594
dc.language.isoengpor
dc.peerreviewedyespor
dc.publisherElsevier Science BVpor
dc.relation.publisherversionhttp://www.sciencedirect.com/science/article/pii/S0370269305017387por
dc.subjectNeutrino Mass Matrixpor
dc.subjectLepton-Flavor Violationpor
dc.subjectCP Violationpor
dc.subjectSee-sawpor
dc.subjectModelspor
dc.subjectBaryogenesispor
dc.subjectSymmetrypor
dc.subjectDemocracypor
dc.subjectAnglespor
dc.titleEnlarging the window for radiative leptogenesispor
dc.typejournal article
dspace.entity.typePublication
oaire.citation.conferencePlaceAmsterdampor
oaire.citation.endPage344por
oaire.citation.issue2-3por
oaire.citation.startPage336por
oaire.citation.titlePhysics Letters Bpor
oaire.citation.volume633por
rcaap.rightsrestrictedAccesspor
rcaap.typearticlepor

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