Comments on the solar neutrino problem

Details Comments on the solar neutrino problem Comments on the solar neutrino problem

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...125l...9o&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 125, no. 2, Sept. 1983, p. L9-L11.

Astronomy and Astrophysics

Astrophysics

Electron Distribution, Electron Energy, Plasma Oscillations, Plasma-Particle Interactions, Solar Neutrinos, Opacity

Scientific paper

It is presently suggested that the solar neutrino problem can be solved in view of the energy gain of electrons responsible for opacity from the high density electrons which produce plasma excitations. A distorted electron distribution results. This solution is not in conflict with the Taylor and Connor (1982) proof that the interaction of electrons with weakly interacting plasma excitations do not distort the Maxwell-Boltzmann distribution, since the proof is not valid for the strongly interacting plasma excitations presently in question. The solution given remains the simplest explanation extant for the solar neutrino problem.

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