“…particles which take part in the mass generation are in O(1-100) TeV range. On top of that, there are radiative neutrino mass models on the market with various additional flavor symmetries, for instance, modular S 3 and A 4[174][175][176][177][178]. Furthermore, these models provide extra contributions to neutrinoless double beta decay, electric dipole moments, anomalous magnetic moments and meson decays as well as matter-antimatter asymmetry, and may also solve the dark matter problem.While neutrino oscillation experiments are insensitive to the nature of neutrinos, experiments looking for lepton number violating signatures can probe the Majorana nature of neutrinos.…”