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dc.contributor.authorGarayoa, Julia-
dc.contributor.authorPastor, Sergio-
dc.contributor.authorPinto Cejas, Teguayco-
dc.contributor.authorRius, Nuria-
dc.contributor.authorVives, Óscar-
dc.date.accessioned2010-02-05T11:32:39Z-
dc.date.available2010-02-05T11:32:39Z-
dc.date.issued2009-09-28-
dc.identifier.citationJOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (9): 035 (2009)en_US
dc.identifier.issn1475-7516-
dc.identifier.urihttp://hdl.handle.net/10261/20751-
dc.description.abstractWe consider the full Boltzmann equations for standard and soft leptogenesis, instead of the usual integrated Boltzmann equations which assume kinetic equilibrium for all species. Decays and inverse decays may be inefficient for thermalising the heavy-(s)neutrino distribution function, leading to significant deviations from kinetic equilibrium. We analyse the impact of using the full kinetic equations in the case of a previously generated lepton asymmetry, and find that the washout of this initial asymmetry due to the interactions of the right-handed neutrino is larger than when calculated via the integrated equations. We also solve the full Boltzmann equations for soft leptogenesis, where the lepton asymmetry induced by the soft SUSY-breaking terms in sneutrino decays is a purely thermal effect, since at T=0 the asymmetry in leptons cancels the one in sleptons. In this case, we obtain that in the weak washout regime (K ~< 1) the final lepton asymmetry can change up to a factor four with respect to previous estimates.en_US
dc.format.extent415806 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoengen_US
dc.publisherInstitute of Physics Publishingen_US
dc.rightsopenAccessen_US
dc.subjectleptogenesisen_US
dc.subjectNeutrino theoryen_US
dc.subjectPhysics of the early universeen_US
dc.titleOn the full Boltzmann equations for leptogenesisen_US
dc.typeartículoen_US
dc.identifier.doi10.1088/1475-7516/2009/09/035-
dc.description.peerreviewedPeer revieweden_US
dc.relation.publisherversionhttp://dx.doi.org/10.1088/1475-7516/2009/09/035en_US
dc.type.coarhttp://purl.org/coar/resource_type/c_6501es_ES
item.openairetypeartículo-
item.languageiso639-1en-
item.fulltextWith Fulltext-
item.grantfulltextopen-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
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