Flavor Symmetries: Models and Implications
Flavor Symmetries: Models and Implications Neutrino mass squared splittings and angles Lisa L. Everett Nakatani, 1936 Talks by Mohapatra, Valle U. Wisconsin, Madison the first who made snow crystal in a laboratory !"#$%& '()*#+*, Absolute neutrino mass scale? The symmetry group of !"#"$#%""& '()*)+,-./0+'1'23"&0+456(5.0+1'7 8 is D6 , one of the finite groups. Introduction/Motivation Neutrino Oscillations: 2 i∆mij L 2E να νβ (L) = iα i∗β j∗α jβe− P → U U U U ij ! massive neutrinos observable lepton mixing First particle physics evidence for physics beyond SM! SM flavor puzzle ν SM flavor puzzle Ultimate goal: satisfactory and credible flavor theory (very difficult!) fits: Schwetz, Tortola, Valle ’08 The Data: Neutrino Masses Homestake, Kam, SuperK,KamLAND,SNO, SuperK, MINOS,miniBOONE,... ∆m2 m2 m2 Assume: 3 neutrino mixing ij ≡ i − j 2 2 +0.23 5 2 Solar: ∆m = ∆m12 = 7.65 0.20 10− eV ! | | − × (best fit 1 σ ) 2 +0.12 3 2 ± Atmospheric: ∆m31 = 2.4 0.11 10− eV ± − × Normal Hierarchy Inverted Hierarchy 3 2 1 2 1 3 Cosmology (WMAP): mi < 0.7 eV i ! fit: Schwetz, Tortola, Valle ’08 The Data: Lepton Mixing Homestake, Kam, SuperK,KamLAND,SNO, SuperK, Palo Verde, CHOOZ, MINOS... MNSP = 1(θ ) 2(θ13, δMNSP) 3(θ ) Maki, Nakagawa, Sakata U R ⊕ R R " P Pontecorvo cos θ sin θ " ! ! MNSP cos θ sin θ cos θ cos θ sin θ |U | ! − ⊕ ! ⊕ ! ⊕ sin θ sin θ sin θ cos θ cos θ ⊕ ! − ⊕ ! ⊕ 1σ ± Solar: θ = θ12 = 33.4◦ 1.4◦ ! ± +4.0 (best fit ) Atmospheric: θ = θ23 = 45.0◦ 3.4 ⊕ − +3.5 Reactor: ! = sin θ13, θ13 = 5.7◦ 5.7 − 2 large angles, 1 small angle (no constraints on
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