New results for radiative proton capture on 16O at astrophysical energies

The possibility of description of the experimental data for the astrophysical S -factor of the proton radiative capture on 16 O to the ground and first excited states of 17 F was considered in the frame of the modified potential cluster model with forbidden states and classification of the states according to Young tableaux. It was shown that on the basis of the E 1 transitions from the P states of p 16 O scattering to the bound states of 17 F in the p 16 O channel, it generally succeeded in explaining the values of total cross sections, astrophysical S -factor from 10 keV and reaction rate at temperatures from 0.01 to 5 T 9 .