The astrophysical S-factor of the reaction Be-7(P,gamma)B-8 in the direct capture model
Krauss, H., Grun, K., Rauscher, T. and Oberhummer, H.
(1993)
The astrophysical S-factor of the reaction Be-7(P,gamma)B-8 in the direct capture model.
Annalen der Physik, 2 (3).
pp. 258-266.
ISSN 0003-3804
The astrophysical S-factor for the reaction Be-7(p, gamma)B-8 up to an energy of 2 MeV (c.m.) and the capture cross section of Li-7(n, gamma)Li-8 up to 1 MeV (c.m.) are calculated using the Direct Capture model (DC). Both calculations are in good agreement with experimental data.
Item Type | Article |
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Keywords | li-7(n,gamma)li-8, scattering, nuclear reactions, solar neutrinos, astrophysical s-factor, be-7(p,gamma)b-8, cross-section |
Date Deposited | 15 May 2025 12:36 |
Last Modified | 30 May 2025 23:54 |
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