  We propose that the radiative generation of the neutrino mass can be achieved
by incorporating the kinetic mixing of fermion fields which arises radiatively
at one-loop level. As a demonstrative example of the application of the
mechanism, we present the particular case of the Standard Model extension by
$U(1)_D$ symmetry. As a result, we show how neutrino masses can be generated
via a kinetic mixing portal instead of a mass matrix with residual symmetries
responsible for the stability of multicomponent dark matter.
