The astrophysical S‐factor of the reaction 7Be (p, γ)8B in the direct capture model

Abstract
The astrophysical S‐factor for the reaction 7Be(p, γ)8B up to an energy of 2 MeV (c.m.) and the capture cross section of 7Li(n,γ)8Li up to 1 MeV (c.m.) are calculated using the Direct Capture model (DC). Both calculations are in good agreement with experimental data.