Chlorine and gallium solar neutrino experiments

Details Chlorine and gallium solar neutrino experiments Chlorine and gallium solar neutrino experiments

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...292l..79b&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 292, May 15, 1985, p. L79-L82.

Physics

81

Chlorine, Gallium, Nuclear Fusion, Solar Neutrinos, Solar Physics, Monte Carlo Method, Solar Flux

Scientific paper

The authors reevaluate the expected capture rates and their uncertainties for the chlorine and gallium solar neutrino experiments using improved laboratory data and new theoretical calculations. They also derive a minimum value for the flux of solar neutrinos that is expected provided only (1) that the sun is currently producing energy by fusing light nuclei at the rate that it is emitting energy in the form of photons from its surface and (2) that nothing happens to solar neutrinos on their way to earth. These results are used - together with Monte Carlo simulations - to determine how much gallium is required for a solar neutrino experiment.

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