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The Neutrino Mass Window for Baryogenesis

Interactions of heavy Majorana neutrinos in the thermal phase of the early universe may be the origin of the cosmological matter-antimatter asymmetry. This mechanism of baryogenesis implies stringent constraints on light and heavy Majorana neutrino masses. We derive an improved upper bound on the CP...

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Detalles Bibliográficos
Autores principales: Buchmuller, W., Di Bari, P., Plumacher, M.
Lenguaje:eng
Publicado: 2003
Materias:
Acceso en línea:https://dx.doi.org/10.1016/S0550-3213(03)00449-8
http://cds.cern.ch/record/605131

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