The solar neutrino problem

Details The solar neutrino problem The solar neutrino problem

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pasau...2..318f&link_type=abstract

(Astronomical Society of Australia, Annual General Meeting, 9th, Parkes, New South Wales, Australia, May 14-16, 1975.) Astronomi

Astronomy and Astrophysics

Astronomy

Astronomical Models, Neutrinos, Nuclear Fusion, Solar Corpuscular Radiation, Helium, Hydrogen, Maxwell-Boltzmann Density Function, Solar Interior, Stellar Structure

Scientific paper

Recent attempts to solve the solar neutrino problem in terms of modified solar interior models are examined. A concise introductory description of the problem is presented, taking into account the discrepancy between the results obtained in the Brookhaven solar neutrino experiment and the prediction provided by standard solar models. Attention is given to Z models, hydrogen-helium inhomogeneities, modified Maxwellian distribution, questions of rapid intermittent mixing, and models with rapidly rotating cores. It is concluded that none of the hypotheses discussed provides a satisfactory solution for the considered problem.

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