Higgs Bosons Phenomenology in the Higgs Triplet Model

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Neutrino Mass Oscillation experiments only sensitive to neutrino mass differences: i) ∆M 2 atm ∼ 10−3 eV 2 (= M) ii) ∆M 2 sol ∼ 10−5 eV 2 (= m) Other experiments constrain the absolute neutrino mass • Neutrinoless double beta decay, Cosmological observations.. • Tritium beta decay (H 3 → He 3 + e − + νe): mνe < 2.2 eV Much lighter than charged fermion masses (me = 0.5 MeV)
Neutrino mass hierarchies Three possibilities to satisfy oscillation data: 1) Hierarchical ∼ (0, m, M). 2) Inverted hierarchical ∼ (M, M + m,0) 3) Quasi-degenerate ∼ (M, M, M) m 3 2 m 2 2 m 1 2 0 m 2 atmospheric ~2×10 −3 eV 2 solar~8×10 −5 eV 2 ν e ν μ ν τ ? ? solar~8×10 −5 eV 2 atmospheric ~2×10 −3 eV 2 m 2 m 2 2 m 1 2 m 3 2 0
Page 1 and 2: Higgs Bosons Phenomenology in the H
Page 3: Neutrino Mass and Mixing Strong evi
Page 7 and 8: TeV scale models of neutrino mass g
Page 9 and 10: Higgs boson spectrum The HTM has 7
Page 11 and 12: Decays of H ±± : Decay channels f
Page 13 and 14: Limits on hij Presence of H ±± wo
Page 15 and 16: Production of H ±± at Tevatron Fi
Page 17 and 18: Tevatron search (2003) for pp → H
Page 19 and 20: Tevatron search (2007) for pp → H
Page 21 and 22: Single H ±± production via qq ′
Page 23 and 24: Inclusive single H ±± production
Page 25 and 26: Summary for qq ′ → H ±± H ∓
Page 27 and 28: Light H ±± at LHC Simulations by
Page 29 and 30: Explicit expressions for hij All hi
Page 31 and 32: Dependence of BR(H ±± → l ± l
Page 33 and 34: BR(H ±± → l ± i l± j ) agains
Page 35 and 36: BR(H ±± → l ± i l± j ) agains
Page 37 and 38: HTM prediction in the plane [BR(H
Page 39 and 40: HTM prediction in the plane [BR(H
Page 41 and 42: HTM prediction for H ± → l ± ν

Higgs Bosons Phenomenology in the Higgs Triplet Model

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