Proton Capture by 7Be and the Solar Neutrino Problem

Details Proton Capture by 7Be and the Solar Neutrino Problem Proton Capture by 7Be and the Solar Neutrino Problem

Feb 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973phrvc...7..543r&link_type=abstract

Physical Review C, vol. 7, Issue 2, pp. 543-547

Physics

32

Scientific paper

It is shown theoretically that the 7Be(p,γ)8B reaction cross section contains substantial contributions from p and d partial waves at laboratory energies, and extrapolations to stellar energies based on the assumption of pure s-wave capture are therefore erroneous. However, there is no change in the predicted solar neutrino flux, because the calculated low-energy cross-section factor, 31 eVb, is essentially the same as the empirical value in current use.

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