Solar neutrino production of technetium-97 and technetium-98

Details Solar neutrino production of technetium-97 and technetium-98 Solar neutrino production of technetium-97 and technetium-98

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982sci...216...51c&link_type=abstract

Science, vol. 216, Apr. 2, 1982, p. 51-54. Research supported by the U.S. Department of Energy

Physics

53

Solar Neutrinos, Technetium Isotopes, Boron Isotopes, Chlorine, Mass Spectroscopy, Molybdenum, Solar Flux, Stellar Evolution

Scientific paper

It may be possible to determine the boron-8 solar neutrino flux, averaged over the past several million years, from the concentration of technetium-98 in molybdenite. The mass spectrometry of this system is greatly simplified by the absence of stable technetium isotopes, and the presence of the fission product technetium-99 provides a monitor of uranium-induced backgrounds. This geochemical experiment could provide the first test of nonstandard solar models that suggest a relation between the chlorine-37 solar neutrino puzzle and the recent ice age.

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