The astrophysicalS-factor of the reaction7Be (p, γ)8B in the direct capture model

The astrophysical $S$-factor for the reaction $^7$Be(p,$\gamma$)$^8$B up to an energy of 2~MeV (c.m.) and the capture cross section of $^7$Li(n,$\gamma$)$^8$Li up to 1~MeV (c.m.) are calculated using the Direct Capture model (DC). Both calculations are in good agreement with experimental data.
Comment: 18 pages, 5 figures (available from author on request), Annalen der Physik in press, 1993