Neutrino emission from plasmons in strong magnetic fields

Details Neutrino emission from plasmons in strong magnetic fields Neutrino emission from plasmons in strong magnetic fields

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974ap%26ss..31..187c&link_type=abstract

Astrophysics and Space Science, vol. 31, Nov. 1974, p. 187-191. NSF-supported research.

Astronomy and Astrophysics

Astrophysics

1

Neutrinos, Particle Emission, Plasmons, Stellar Magnetic Fields, Cold Plasmas, Energy Conservation, Energy Dissipation, Maxwell Equation, Pair Production, Plasma Waves, Refractivity, Stellar Evolution, Stellar Interiors, Stellar Structure

Scientific paper

Neutrino pair emission from stellar interiors is investigated. The paper indicates that the proposed enhanced emission mode is a part of a transverse mode spectrum with a refraction index in the limit of infinity. It is concluded that in an astrophysical sense a very strong magnetic field does not have a significant effect on the emission rate of neutrinos from plasmons.

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