Indirect measurements of the solar-neutrino production reaction 7Be(p [formula omitted]) 8B
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 t...
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Published in | Nuclear physics. A Vol. 693; no. 1; pp. 258 - 268 |
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Main Author | |
Format | Journal Article |
Language | English |
Published |
Elsevier B.V
01.10.2001
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Online Access | Get full text |
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Summary: | 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
S
17
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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ISSN: | 0375-9474 |
DOI: | 10.1016/S0375-9474(01)01113-7 |