Radiative Neutrino Mass Generation and Dark Matter - Institute for ...

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OutlineOutline1 Introduction2 Neutrino Mass Generation3 Dark Matter4 A Concrete Model of Radiative SeesawConstraintsCoannihilation Effect of DMDirect Detection of (Leptophilic) DM5 Further Extension of Radiative SeesawSUSY with anomalous U(1)Indirect detection of DM with flavor symmetry6 SummaryTakashi Toma (IPPP) Internal Seminar 7th June 2013 2 / 34
Page 5: Neutrino Mass GenerationNeutrino Ma
Page 9 and 10: Dark MatterDark MatterTakashi Toma
Page 11 and 12: Dark MatterDM Thermal ProductionDM
Page 13 and 14: Concrete ModelA Concrete Model of R
Page 15 and 16: Concrete ModelNeutrino Massesη 0 s
Page 17 and 18: Concrete ModelConstraintsTo derive
Page 19 and 20: Concrete ModelConstraintsConstraint
Page 21 and 22: Concrete ModelAllowed parameter reg
Page 23 and 24: Concrete ModelDirect Detection of D
Page 25 and 26: Concrete ModelDirect Detection of D
Page 27 and 28: Extensions of Radiative SeesawExten
Page 29 and 30: Extensions of Radiative SeesawInter
Page 31 and 32: Extensions of Radiative SeesawPosit
Page 33 and 34: Future WorksFuture Works1 Gamma-ray

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