Radiative Capture of a Proton on 10B at Astrophysical Energies

Abstract

The possibility of description of the experimental data for the astrophysical Sfactor of the radiative proton capture on 15 N at the energies from 50 to 1500 keV was considered in the framework of the modified potential cluster model with the classification of the orbital states according to Young tableaux. It was shown that, on the basis of the M1 and the E1 transitions from different states of the p 15 N scattering to the ground state of 16 O in the p 15 N channel, it is quite succeed to explain general behavior of the S-factor in the considered energy range in the presence of two resonances.