Proposed neutrino monitor of long-term solar burning

Details Proposed neutrino monitor of long-term solar burning Proposed neutrino monitor of long-term solar burning

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phrvl..65..809h&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 65, Aug. 13, 1990, p. 809-812. Research supported by DOE and NSF.

Physics

13

Neutrino Beams, Nuclear Fusion, Solar Activity Effects, Solar Neutrinos, Solar Temperature, Stellar Evolution, Stellar Luminosity, Stellar Mass Ejection

Scientific paper

The standard solar model predicts that the sun's luminosity has increased by 40 percent over the past 5 Gyr of main-sequence burning, a result that has troubled geophysicists and paleoclimatologists. This increase is accompanied by an exponential growth in the B-8 neutrino flux, with a doubling time of 0.85 Gyr. It is argued that one nuclear system exists that, in principle, could yield a quantitative terrestrial record of these past changes. It is not clear whether the reading of that record is within present experimental capabilities.

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