The Astrophysical S-Factor of the Reaction be(p,)B in the Direct Capture Model
arXiv:nucl-th/9301018 · doi:10.1002/andp.19935050304
Abstract
The astrophysical -factor for the reaction Be(p,)B up to an energy of 2~MeV (c.m.) and the capture cross section of Li(n,)Li up to 1~MeV (c.m.) are calculated using the Direct Capture model (DC). Both calculations are in good agreement with experimental data.
18 pages, 5 figures (available from author on request), Annalen der Physik in press, 1993