Spin light of relativistic electrons in neutrino fluxes

A new mechanism of electromagnetic radiation by electrons under the influence of a dense neutrino flux, termed “the spin light of electron” in neutrino flux ($SL{e}_{\nu }$), is considered. It is shown that in the case when electrons are moving against the neutrino flux with relativistic energy there is a reasonable increase of the efficiency of the energy transfer from the neutrino flux to the electromagnetic radiation by the $SL{e}_{\nu }$ mechanism. The proposed radiation process is applied to an astrophysical environment with characteristics peculiar to supernovae. It is shown that a reasonable portion of energy of the neutrino flux can be transferred by the $SL{e}_{\nu }$ to gamma-rays .