$ν$-GMSB with Type III Seesaw and Phenomenology

Details $ν$-GMSB with Type III Seesaw and Phenomenology $ν$-GMSB with Type III Seesaw and Phenomenology

2008-07-28

arxiv.org/abs/0807.4524v2

Phys.Rev.D78:075011,2008

Physics

High Energy Physics

High Energy Physics - Phenomenology

21 pages,5 figures

Scientific paper

10.1103/PhysRevD.78.075011

We show that when the supersymmetric SU(5) model is extended to explain small neutrino masses by the type III seesaw mechanism, the new {\bf 24}-dimensional fields needed for the purpose can act as messengers for transmitting SUSY breaking from a hidden sector to the visible sector. For the three {\bf 24} case, the constraints of grand unification and suppressed lepton flavor violation restrict the seesaw scale in this case to be in the narrow range of $10^{12}-10^{13}$ GeV. The model predicts (i) a stable LSP gravitino with mass in the range of 1-10 MeV which can be a cold dark matter of the universe; (ii) a stau NLSP which is detectable at LHC; (iii) a lower bound on the branching ratio $BR(\mu \to e \gamma)$ larger than $10^{-14}$ testable by the ongoing MEG experiment as well as characteristic particle spectrum different from other SUSY breaking scenarios. We also discuss the case with two {\bf 24} fields, which is the minimal case that can explain neutrino oscillation data.

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