In conclusion, we sum up the results obtained here:
the electromagnetic properties of Dirac and Majorana massless
neutrinos are presented by the TDM of the order of
cm;
for massive neutrinos the toroid dipole moment is
the toroid interactions are a part of radiative corrections
to the scattering of neutrinos on electrons, quarks and nuclei both
in the vacuum and in the medium;
the above mentioned effects can manifest themselves in numerous
astrophysical and cosmological situations. Among them are neutrino
propagation through the solar interior and young supernova
envelopes, neutrino radiation of accreting neutron stars and
black holes, where inhomogeneous vortex magnetic fields can have
large values, high-energy neutrino generation
due to heavy particle emission and acceleration by saturated
superconducting cosmic strings or due to cusp radiation from
ordinary cosmic strings etc., and the toroid interactions of
neutrinos should be taken into account in each of them;
and
are maximal at low energies ( MeV);
neutrinos can produce the Vavilov-Cherenkov and transition radiations
due to its TDM.