Neutrino physics within and beyond the three flavour oscillation

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.


Editor(s):
Blondel, A
Efthymiopoulos, I
Prior, G
Published in:
Xiii International Workshop On Neutrino Factories, Super Beams And Beta Beams (Nufact11), 408
Presented at:
13th International Workshop on Neutrino Factories, Super beams and Beta beams (NUFACT), Geneva, SWITZERLAND, AUG 01-06, 2011
Year:
2013
Publisher:
Bristol, Iop Publishing Ltd
ISSN:
1742-6588
Laboratories:




 Record created 2013-04-15, last modified 2018-03-17


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