Radiative p16O Capture at Astrophyiscal Energies

详细

Within the framework of the modified potential cluster model with forbidden states and classification of states according to the Young tableaux, the possibility is considered of describing experimental data for the astrophysical S-factor of radiative p¹⁶O capture to the ground state of the ¹⁷F nucleus. It is shown that on the basis of E1 transitions from p¹⁶O scattering states to the ground state of ¹⁷F in the p¹⁶O channel overall success is achieved in explaining the magnitude of the measured cross sections at astrophysical energies.