THE ASTROPHYSICAL S-FACTOR OF THE REACTION Be(p,γ)B IN THE DIRECT CAPTURE MODEL
نویسندگان
چکیده
The astrophysical S-factor for the reaction Be(p,γ)B up to an energy of 2 MeV (c.m.) and the capture cross section of Li(n,γ)Li up to 1 MeV (c.m.) are calculated using the Direct Capture model (DC). Both calculations are in good agreement with experimental data.
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