Sala Seminarios IFIC (Edf. Institutos de Investigación)
Sala Seminarios IFIC
Edf. Institutos de Investigación
Descripción
If neutrino masses and mixings are suitable to explain the atmospheric and solar neutrino fluxes, this amounts to contributions to FCNC processes, in particular $\mu\rightarrow e, \gamma$. If the theory is supersymmetric and the origin of the masses is a see-saw mechanism, the predictions for BR($\mu\rightarrow e, \gamma$) naturally exceed the experimental bounds.