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We present a three-loop model of neutrino mass in which both the weak scaleand neutrino mass arise as radiative effects. In this approach, the scales forelectroweak symmetry breaking, dark matter, and the exotics responsible forneutrino mass, are related due to an underlying scale-invariance. Thismotivates the otherwise-independent O(TeV) exotic masses usually found inthree-loop models of neutrino mass. We demonstrate the existence of viableparameter space and show that the model can be probed at colliders, precisionexperiments, and dark matter direct-detection experiments.

A Radiative Model for the Weak Scale and Neutrino Mass via Dark Matter