Speaker
Dr
Sofiane Boucenna
(KTH Royal Institute of Technology)
Description
Neutrino masses generated by physics around the weak-scale offer the advantage of testability, however from the model-building viewpoint they appear to be ad-hoc. I will present two classes of models which predict a radiative seesaw formula for neutrino masses and the presence of weakly interacting stable dark matter from (non-supersymmetric) SO(10) Grand Unified Theories. The model achieves precision unification and offers experimental tests.
Primary author
Dr
Sofiane Boucenna
(KTH Royal Institute of Technology)
