Consistent mean-field description of the $^{12}$C+$^{12}$C optical potential at low energies and the astrophysical $S$ factor

TL;DR

This paper develops a consistent mean-field optical potential for $^{12}$C+$^{12}$C at low energies using a double-folding model with realistic densities and interactions, accurately reproducing the astrophysical $S$ factor without adjustments.

Contribution

It introduces a low-energy double-folding model with an adiabatic approximation validated against scattering data, providing a reliable potential for astrophysical fusion calculations.

Findings

The model accurately reproduces elastic scattering data below 10 MeV/nucleon.

The potential predicts the non-resonant $S$ factor behavior of $^{12}$C+$^{12}$C fusion.

No parameter adjustments were needed to match experimental $S$ factor data.

Abstract

The nuclear mean-field potential built up by the $^{12}$C+$^{12}$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 $^{12}$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 $^{12}$C+$^{12}$C scattering data at energies below 10 MeV/nucleon. The folded mean-field potential is then used to study the astrophysical $S$ factor of the $^{12}$C+$^{12}$C fusion in the barrier penetration model. Without any adjustment of the potential strength, our results reproduce very well the non-resonant behavior of the $S$ factor of the $^{12}$C+$^{12}$C fusion over a wide range of energies.