Plasmon decay l,t yields nu nu(-) in the dense plasma of collapsing stars

Details Plasmon decay l,t yields nu nu(-) in the dense plasma of collapsing stars Plasmon decay l,t yields nu nu(-) in the dense plasma of collapsing stars

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..277l&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, March 1988, p. 277-280. In Russian. In Russian. In Russian.

Mathematics

Probability

Dense Plasmas, Plasma Decay, Plasmons, Supernova 1987A, Antineutrinos, Gravitational Collapse, Neutrinos

Scientific paper

Semikoz's (1987) approach is used to calculate plasmon decay into a neutrino-antineutrino pair. It is shown that the probability of the decay of a transverse plasmon into a neutrino-antineutrino pair and energy losses increase in dense astrophysical plasmas due to an additional interaction between neutrino spin and matter. The results may be of interest in connection with the investigation of neutrino pulses from the supernova SN 1987A in the LMC.

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