| Summary: Radiative capture of nucleons at energies of astrophysical interest is one of the most important processes for nucleosynthesis. In this thesis, the of calculations astrophysical S-factors for radiative proton capture reactions such d(p,γ)3He, 6Li(p,γ)7Be, 8B(p,γ)9C, 12C(p,γ)13N, 13C(p,γ)14N, 16O(p,γ)17F, 20Ne(p,γ)21Na were done in Potential Model. The change according to the energy of data of the resulting astrophysical S-Factor data was analyzed. The theoretical results which calculated are compatible with experimental data (particularly non-resonance reactions). |
