Resum
We construct a model with two Higgs doublets where the neutrino has a magnetic moment μvO(10-10)μB. We pay particular attention to the phenomenological constraints coming from FCNC processes such as μ→eγ. The model provides an explicit scenario strictly within the standard SU (2) × U (1) framework that could solve the solar neutrino puzzle. © 1998.
Idioma original | Anglès |
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Pàgines (de-a) | 482-486 |
Revista | Physics Letters B |
Volum | 213 |
DOIs | |
Estat de la publicació | Publicada - 3 de nov. 1988 |