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Neutrino Masses and GUT Baryogenesis

We reconsider the GUT-baryogenesis mechanism for generating the baryon asymmetry of the Universe. The baryon asymmetry is produced by the out of equilibrium decay of coloured Higgs bosons at the GUT scale, conserving B-L. If neutrinos are Majorana particles, lepton number violating interactions eras...

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Detalles Bibliográficos
Autores principales: López-Pérez, J A, Rius, N
Lenguaje:eng
Publicado: 2004
Materias:
Acceso en línea:https://dx.doi.org/10.22323/1.010.0048
http://cds.cern.ch/record/730593
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author López-Pérez, J A
Rius, N
author_facet López-Pérez, J A
Rius, N
author_sort López-Pérez, J A
collection CERN
description We reconsider the GUT-baryogenesis mechanism for generating the baryon asymmetry of the Universe. The baryon asymmetry is produced by the out of equilibrium decay of coloured Higgs bosons at the GUT scale, conserving B-L. If neutrinos are Majorana particles, lepton number violating interactions erase the lepton number excess, but part of the baryon asymmetry may be preserved, provided those interactions are not in thermal equilibrium when the sphaleron processes become effective, at $T \sim 10^{12}~ GeV$. We analyse whether this mechanism for baryogenesis is feasible in a variety of GUT models of fermion masses proposed in the literature, based on horizontal symmetries.
id cern-730593
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2004
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spelling cern-7305932019-09-30T06:29:59Zdoi:10.22323/1.010.0048http://cds.cern.ch/record/730593engLópez-Pérez, J ARius, NNeutrino Masses and GUT BaryogenesisParticle Physics - PhenomenologyWe reconsider the GUT-baryogenesis mechanism for generating the baryon asymmetry of the Universe. The baryon asymmetry is produced by the out of equilibrium decay of coloured Higgs bosons at the GUT scale, conserving B-L. If neutrinos are Majorana particles, lepton number violating interactions erase the lepton number excess, but part of the baryon asymmetry may be preserved, provided those interactions are not in thermal equilibrium when the sphaleron processes become effective, at $T \sim 10^{12}~ GeV$. We analyse whether this mechanism for baryogenesis is feasible in a variety of GUT models of fermion masses proposed in the literature, based on horizontal symmetries.hep-ph/0404124IFIC-2004-14FTUV-2004-0404oai:cds.cern.ch:7305932004-04-15
spellingShingle Particle Physics - Phenomenology
López-Pérez, J A
Rius, N
Neutrino Masses and GUT Baryogenesis
title Neutrino Masses and GUT Baryogenesis
title_full Neutrino Masses and GUT Baryogenesis
title_fullStr Neutrino Masses and GUT Baryogenesis
title_full_unstemmed Neutrino Masses and GUT Baryogenesis
title_short Neutrino Masses and GUT Baryogenesis
title_sort neutrino masses and gut baryogenesis
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.22323/1.010.0048
http://cds.cern.ch/record/730593
work_keys_str_mv AT lopezperezja neutrinomassesandgutbaryogenesis
AT riusn neutrinomassesandgutbaryogenesis