Consistent mean-field description of theC12 + C12optical potential at low energies and the astrophysicalSfactor

Abstract

The nuclear mean-field potential built up by the $^{12}\mathrm{C}+^{12}\mathrm{C}$ interaction at energies relevant for the carbon burning process is calculated in the double-folding model (DFM) using the realistic ground-state density of $^{12}\mathrm{C}$ and the CDM3Y3 density dependent nucleon-nucleon (NN) interaction, with the rearrangement term properly included. To validate the use of a density dependent NN interaction in the DFM calculation in the low-energy regime, an adiabatic approximation is suggested for the nucleus-nucleus overlap density. The reliability of the nuclear mean-field potential predicted by this low-energy version of the DFM is tested in a detailed optical model analysis of the elastic $^{12}\mathrm{C}+^{12}\mathrm{C}$ scattering data at energies below 10 MeV/nucleon. The folded mean-field potential is then used to study the astrophysical $S$ factor of $^{12}\mathrm{C}+^{12}\mathrm{C}$ fusion in the barrier penetration model. Without any adjustment of the potential strength, our results reproduce very well the nonresonant behavior of the $S$ factor of $^{12}\mathrm{C}+^{12}\mathrm{C}$ fusion over a wide range of energies.