Indirect measurements of the solar-neutrino production reaction 7Be(p/,γ)8B

Details Indirect measurements of the solar-neutrino production reaction 7Be(p/,γ)8B Indirect measurements of the solar-neutrino production reaction 7Be(p/,γ)8B

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001nupha.693..258m&link_type=abstract

Nuclear Physics A, Volume 693, Issue 1-2, p. 258-268.

Physics

Nuclear Physics

7

Scientific paper

Low-energy cross sections of the 7Be(p/,γ)8B reaction is of crucial importance, because they determine the high-energy solar neutrino flux. Coulomb dissociation with intermediate-energy 8B beams and low-energy proton-transfer reactions with 7Be beams have been investigated to determine indirectly the astrophysical S17 factors of the 7Be(p/,γ)8B reaction. The results of these studies are generally in good agreement with the ones obtained by direct capture measurements using intense proton beams and radioactive 7Be targets.

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