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- W1990981225 abstract "The 10B(p,α)7Be reaction is the main responsible for 10B destruction in stellar interior. In such environments this p-capture process occurs at a Gamow energy of ∼10 keV, and takes places mainly through a resonant state ( E x = 8.701 MeV ) of the compound 11C nucleus. Thus, a resonance right in the region of the Gamow peak is expected to significantly influence the behaviour of the astrophysical S(E)-factor. The 10B(p,α)7Be reaction has been investigated by means of the Trojan Horse Method (THM) applied to the 2H(10B,α7Be)n three-body process. The experiment was performed at E b e a m = 27 MeV at the Instituto de Fisica Nuclear de Sao Paulo. Preliminary results concerning the extraction of the bare-nucleus S(E)-factor will be presented." @default.
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- W1990981225 date "2007-05-01" @default.
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- W1990981225 title "Boron depletion: indirect measurement of the 10B(p,α)7Be S(E)-factor" @default.
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- W1990981225 doi "https://doi.org/10.1016/j.nuclphysa.2006.12.049" @default.
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