Radiative p 15N Capture in the Region of Astrophysical Energies

• DOI: 10.1007/s11182-016-0762-3
• Publication Date: 2016-06-03T22:54:20Z
• Authors: S. B. Dubovichenko; N. Burtebaev; A. V. Dzhazairov-...; D. K. Alimov
• Keywords: 0103 physical sciences; 01 natural sciences

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 p 15N 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 p 15N scattering states to the ground state of the 16O nucleus in the p 15N 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.