# Absence of hindrance in microscopic $^{12}$C+$^{12}$C fusion study

## TL;DR

This study uses microscopic mean-field theories to analyze low-energy $^{12}$C+$^{12}$C fusion, finding no hindrance or maximum in the astrophysical S factor at deep sub-barrier energies, contrasting some experimental results.

## Contribution

It applies static and dynamic Hartree-Fock methods to predict fusion cross sections and S factors, providing a microscopic perspective on low-energy carbon fusion without observing hindrance.

## Key findings

- No S factor maximum observed in microscopic calculations.
- Predicted S factor rises at low energies with slight damping.
- Good agreement with some experimental resonance peaks.

## Abstract

Background: Studies of low-energy fusion of light nuclei are important in astrophysical modeling, with small variations in reaction rates having a large impact on nucleosynthesis yields. Due to the lack of experimental data at astrophysical energies, extrapolation and microscopic methods are needed to model fusion probabilities. Purpose: To investigate deep sub-barrier $^{12}$C+$^{12}$C fusion cross sections and establish trends for the $S$ factor. Method: Microscopic methods based on static Hartree-Fock (HF) and time-dependent Hartree-Fock (TDHF) mean-field theory are used to obtain $^{12}$C+$^{12}$C ion-ion fusion potentials. Fusion cross sections and astrophysical $S$ factors are then calculated using the incoming wave boundary condition (IWBC) method. Results: Both density-constrained frozen Hartree-Fock (DCFHF) and density-constrained TDHF (DC-TDHF) predict a rising $S$ factor at low energies, with DC-TDHF predicting a slight damping in the deep sub-barrier region ($\approx1$~MeV). Comparison between DC-TDHF calculations and maximum experimental cross-sections in the resonance peaks are good. However the discrepancy in experimental low energy results inhibits interpretation of the trend. Conclusions: Using the fully microscopic DCFHF and DC-TDHF methods, no $S$ factor maximum is observed in the $^{12}$C+$^{12}$C fusion reaction. In addition, no extreme sub-barrier hindrance is predicted at low energies. The development of a microscopic theory of fusion including resonance effects, as well as further experiments at lower energies must be done before the deep sub-barrier behavior of the reaction can be established.