Collective interactions of neutrinos with dense astrophysical plasmas

Details Collective interactions of neutrinos with dense astrophysical plasmas Collective interactions of neutrinos with dense astrophysical plasmas

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.251..321o&link_type=abstract

In ESA Proceedings of the Joint Varenna-Abastumani International School and Workshop on Plasma Astrophysics p 321-324 (SEE N87-

Astronomy and Astrophysics

Astrophysics

Cerenkov Radiation, Cosmic Plasma, Neutrinos, Particle Interactions, Kinetic Equations, Particle Charging, Polarization Characteristics, Relativistic Theory

Scientific paper

It is shown that in a dispersive medium the neutrino acquires an induced electric charge, due to medium polarization irrespective of the neutrino rest-mass. The self-consistent electromagnetic A-field is taken into account in the relativistic kinetic equation for neutrino derived by Bogolyubov's method to give the electric form factor and charge of neutrino. It is shown that the existence of a massless long-range weak Z-field provided polarization of a medium by moving neutrinos. Polarization and Vavilov-Cerenkov losses of the zero-mass neutrino in metal plasma and in cooling magnetic stars are considered.

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