Statistical theory for B-8 solar neutrino captures by newly proposed targets

Details Statistical theory for B-8 solar neutrino captures by newly proposed targets Statistical theory for B-8 solar neutrino captures by newly proposed targets

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...246..989i&link_type=abstract

Astrophysical Journal, Part 1, vol. 246, June 15, 1981, p. 989-993.

Astronomy and Astrophysics

Astrophysics

7

Absorption Cross Sections, Capture Effect, Solar Neutrinos, Statistical Analysis, Boron Isotopes, Incident Radiation, Nuclear Reactions, Targets

Scientific paper

The B-8 solar neutrino capture cross sections are calculated for the newly proposed targets by using the statistical theory. It turns out that Bahcall's (1978) result for Br-81 underestimates the cross section by an order of magnitude. The present results are valuable for the comparison with the p-p, pep, and Be-7 solar neutrino capture rates by the same targets.

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