astrophysically relevant energies is calculated using the overlap integral〈 11C| 12N〉 and
the p–11C local effective potential obtained within a microscopic approach. This approach is
based on the solution of the inhomogeneous differential equation with the source term
calculated within the translation-invariant 0 ℏω shell model. The calculations resulted in a
zero-energy astrophysical S-factor S (0) equal to 0.149 keVb. This value was obtained with …