I will discuss several possible choices for the mass scale M of the Majorana leptons, complementing the Standard Model to describe neutrino masses and oscillations. Depending on M, they can or cannot accommodate eV neutrino anomalies, lead to baryogenesis, provide the dark matter candidate, ensure the stability of the Higgs mass against radiative corrections, and be directly searched at some experiments.
Titre
Neutrino physics within and beyond the three flavour oscillation
Publié dans
Xiii International Workshop On Neutrino Factories, Super Beams And Beta Beams (Nufact11)
Pagination
8
Série
Journal of Physics Conference Series
Volume
408
Présenté à
13th International Workshop on Neutrino Factories, Super beams and Beta beams (NUFACT), Geneva, SWITZERLAND, AUG 01-06, 2011
Date
2013
Editeur
Bristol, Iop Publishing Ltd
ISSN
1742-6588
Date de création de la notice
2013-04-15