  We present a minimal model that simultaneously accounts for neutrino masses
and the origin of dark matter (DM) and where the electroweak phase transition
is strong enough to allow for electroweak baryogenesis. The Standard Model is
enlarged with a Majorana fermion, three generations of chiral fermion pairs,
and a single complex scalar that plays a central role in DM production and
phenomenology, neutrino masses, and the strength of the phase transition. All
the new fields are singlets under the SM gauge group. Neutrino masses are
generated via a new variant of radiative inverse seesaw where the required
small mass term is generated via loops involving DM and no large hierarchy is
assumed among the mass scales. The model offers all the advantage of low-scale
neutrino mass models as well as a viable dark matter candidate that is testable
with direct detection experiments.

High Energy Physics - Phenomenology