Radiative p15N Capture in the Region of Astrophysical Energies

Resumo

Within the framework of the modified potential cluster model with classification of orbital states according to the Young schemes, the possibility of describing experimental data for the astrophysical S-factor of p¹⁵N radiative capture at energies from 50 to 1500 keV is considered. It is shown that on the basis of M1 and E1 transitions from various p¹⁵N scattering states to the ground state of the ¹⁶O nucleus in the p¹⁵N channel it is entirely possible to successfully explain the overall behavior of the S-factor in the considered energy region in the presence of two resonances.