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

摘要: We present a three-loop model of neutrino mass in which both the weak scale and arise as radiative effects. In this approach, scales for electroweak symmetry breaking, dark matter, exotics responsible mass, are related due to an underlying scale-invariance. This motivates otherwise-independent $$ \mathcal{O}\left(\mathrm{T}\mathrm{e}\mathrm{V}\right) $$ exotic masses usually found models mass. demonstrate existence viable parameter space show that can be probed at colliders, precision experiments, matter direct-detection experiments.