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.
|Journal||Physics Letters B|
|Publication status||Published - 3 Nov 1988|