A Model of Radiative Neutrino Mass: with or without Dark Matter
  We present a three-loop model of neutrino mass whose most-general Lagrangian possesses a softly-broken accidental $Z_2$ symmetry. In the limit that a single parameter vanishes, $\lambda\rightarrow0$, the $Z_2$ symmetry becomes exact and the model contains a stable dark-matter candidate. However, even for finite $\lambda\ll1$, long-lived dark matter is possible, giving a unified solution to the neutrino mass and dark matter problems that does not invoke a new symmetry. Taken purely as a neutrino mass model, the new physics can be at the TeV scale. When dark matter is incorporated, however, only a singlet scalar can remain this light, though the dark matter can be tested in direct-detection experiments. 
Amine Ahriche (Jijel U. & ICTP, Trieste), Kristian L. McDonald (Sydney   U.), Salah Nasri (United Arab Emirates U.)
hep-ph astro-ph.HE