Neutrinos from a standard solar model

Details Neutrinos from a standard solar model Neutrinos from a standard solar model

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...253..393f&link_type=abstract

Astrophysical Journal, Part 1, vol. 253, Feb. 1, 1982, p. 393-398.

Physics

24

Particle Flux Density, Solar Flux, Solar Neutrinos, Stellar Models, Stellar Structure, Abundance, Capture Effect, Chlorine, Gallium Isotopes, Monte Carlo Method, Nuclear Fusion, Standard Deviation, Stellar Evolution, Stellar Luminosity

Scientific paper

Solar model calculations are performed, as both (1) an independent check of the new value for the Cl-37 capture rate, and (2) an extension of the input parameters of a standard model to the extremes of experimental and theoretical limits with a view to implications for stellar evolution or neutrino physics. Capture rates are calculated for the on-line Cl-37 experiment and the proposed experiment employing Ga-71 as an example of a detector sensitive to the high-flux, lower-energy p-p neutrinos. The effects of uncertainties in the input parameters on the predicted capture rate in the two detectors are examined by: (1) calculating the effect of individual uncertainties on the mean standard model and summing these errors in quadrature; (2) simultaneously varying several key parameters to yield upper and lower limits; and (3) by generating a set of models whose parameters are determined by a Monte Carlo method.

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