OSCILLATING NEUTRINOS AND MU --> E, GAMMA

por Dr. J.A. Casas (IEM-CSIC, Madrid)

jueves 23 nov. 2000 12:30 → 13:30 Europe/Madrid

Sala Seminarios IFIC (Edf. Institutos de Investigación)

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.