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Radiative Two Loop Inverse Seesaw and Dark Matter · Around

2012

Radiative Two Loop Inverse Seesaw and Dark Matter

Guo, Gang, He, Xiao-Gang, Li, Guan-Nan

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Seesaw mechanism provides a natural explanation of light neutrino masses through suppression of heavy seesaw scale.

In inverse seesaw models the seesaw scale can be much lower than that in the usual seesaw models.
If terms inducing seesaw masses are further induced by loop corrections, the seesaw scale can be lowered to be in the range probed by experiments at the LHC without fine tuning.
In this paper we construct models in which inverse seesaw neutrino masses are generated at two loop level.

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The ATLAS Collaboration, Observation for an Excess of Events in the Search for the Standard Model Higgs boson with the ATLAS detector at the LHC, ATLAS-CONF-2012-093,2012; The CMS Collaboration, Observation of a resonance with a mass near 125 GeV in the search for the Higgs boson in pp collisions at s = 7 \sqrt{s}=7 TeV and 8 TeV, CMS-HIG-12-020,2012

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