Radiative Neutrino Mass Generation and Dark Matter - Institute for ...
Radiative Neutrino Mass Generation and Dark Matter - Institute for ...
Radiative Neutrino Mass Generation and Dark Matter - Institute for ...
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Concrete ModelConstraintsThe parameters are constrained by various aspects.<strong>Neutrino</strong> mass scale m ν ∼ 10 −1 eV<strong>Neutrino</strong> mixingU T PMNS m νU PMNS = diag(m 1 ,m 2 ,m 3 )Lepton flavor violation (LFV)µ → eγ : Br(µ → eγ) ≤ 2.4×10 −12 → 5.7×10 −13 (now)µ → 3e?Thermal relic density of DM· N 1 is assumed to be DM here.· Leptophilic DM.· degenerated with N 2 .Takashi Toma (IPPP) Internal Seminar 7th June 2013 16 / 34