The astrophysical S-factor of the reaction Be-7(P,gamma)B-8 in the direct capture model

Krauss, H.; Grun, K.; Rauscher, T.; Oberhummer, H.

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

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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
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	17 Jun 2026 19:18