Radiative p11C Capture Reaction Rate

Within the frame of the modified potential cluster model with classification of orbital states according to Young’s diagrams, the astrophysical S-factor of radiative p 11 C capture was calculated. The calculations considered all scattering resonances up to 3.5 MeV and were performed at energies up to 5 MeV. On the basis of the obtained total cross sections, the reaction rate was calculated at temperatures from 0.01 to 10.0 Т 9 , and its simple parameterization was proposed.