Abstract
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.
Original language | English |
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Pages (from-to) | 258-266 |
Number of pages | 9 |
Journal | Annalen der Physik |
Volume | 2 |
Issue number | 3 |
Publication status | Published - 1993 |
Keywords
- LI-7(N,GAMMA)LI-8
- SCATTERING
- NUCLEAR REACTIONS
- SOLAR NEUTRINOS
- ASTROPHYSICAL S-FACTOR
- BE-7(P,GAMMA)B-8
- CROSS-SECTION