Solar neutrino experiments. I - Theory

Details Solar neutrino experiments. I - Theory Solar neutrino experiments. I - Theory

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985aipc..126...60b&link_type=abstract

IN: Solar neutrinos and neutrino astronomy; Proceedings of the Conference, Lead, SD, August 23-25, 1984 (A86-37626 17-93). New Y

Astronomy and Astrophysics

Astronomy

1

Chlorine, Gallium Isotopes, Nuclear Reactions, Solar Neutrinos, Capture Effect, Flux Quantization, Monte Carlo Method, Radiation Sources

Scientific paper

The expected capture rates and their uncertainties are reevaluated for the chlorine and gallium experiments using improved laboratory data and new theoretical calculations. The author also states a minimum value for the flux of solar neutrinos that is expected provided only that the sun is currently burning light nuclei at the rate it is emitting photons from its surface and that nothing happens to solar neutrinos on their way to the earth. These results are used - together with Monte Carlo simulations performed by Cleveland - to determine how much gallium is required for a solar neutrino experiment.

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