Absence of hindrance in microscopic $^{12}$C+$^{12}$C fusion study
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 C+C fusion cross sections and establish trends for the factor. Method: Microscopic methods based on static Hartree-Fock (HF) and time-dependent Hartree-Fock (TDHF) mean-field theory are used to obtain C+C ion-ion fusion potentials. Fusion cross sections and astrophysical 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 factor at low energies, with DC-TDHF predicting a slight damping in the deep sub-barrier region (~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 factor maximum is observed in the C+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.
Keywords
Cite
@article{arxiv.1906.02268,
title = {Absence of hindrance in microscopic $^{12}$C+$^{12}$C fusion study},
author = {K. Godbey and C. Simenel and A. S. Umar},
journal= {arXiv preprint arXiv:1906.02268},
year = {2019}
}
Comments
9 pages, 6 figures