Astrophysical S-factor for the 13С(р, γ)14N Radiative Capture Reaction

The phase shift analysis, done on the basis of the known measurements of the differential cross-sections of the р13С elastic scattering at the energy range 250÷750 keV, shows that it is enough to take into account only 3S1 wave in the considered energy region. The potential for the triplet 3S1 state in р13С system at the resonance energy 0.55 MeV corresponding to quantum numbers J T = 1-1 as well as the potential for the 3Р1 bound state of 14N were constructed on the basis of the obtained scattering phase shifts. The possibility to describe the experimental data of the astrophysical S-factor of the р13С radiative capture at the energies 0.03÷0.8 MeV was considered within the potential cluster model with the forbidden states. It was shown that we properly succeed in explanation of the energy behavior of the astrophysical S-factor for the р13С radiative capture at the resonance energy range 0.55 MeV (laboratory system).