Absence of hindrance in a microscopic 12C + 12C fusion study
Abstract
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. To investigate deep sub-barrier 12C+12C fusion cross sections and establish trends for the S factor. Microscopic methods based on static Hartree-Fock and time-dependent Hartree-Fock (TDHF) mean-field theory are used to obtain 12C+12C ion-ion fusion potentials. Fusion cross sections and astrophysical S factors are then calculated using the incoming wave boundary condition method. 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 (≈1 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. Using the fully microscopic DCFHF and DC-TDHF methods, no S factor maximum is observed in the 12C+12C fusion reaction. In addition, no extreme sub-barrier hindrance is predicted at low energies. Furthermore, the development of a microscopic theory of fusion including resonance effects, as well as furthermore »
- Authors:
-
- Vanderbilt Univ., Nashville, TN (United States)
- The Australian National Univ., Canberra (Australia)
- Publication Date:
- Research Org.:
- Vanderbilt Univ., Nashville, TN (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC)
- OSTI Identifier:
- 1612036
- Alternate Identifier(s):
- OSTI ID: 1558151
- Grant/Contract Number:
- SC0013847
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review C
- Additional Journal Information:
- Journal Volume: 100; Journal Issue: 2; Journal ID: ISSN 2469-9985
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 73 NUCLEAR PHYSICS AND RADIATION PHYSICS; Physics; Low & intermediate energy heavy-ion reactions; Nuclear astrophysics; Nuclear density functional theory; Nuclear fusion; Nuclear reactions
Citation Formats
Godbey, Kyle, Simenel, Cedric, and Umar, A. S. Absence of hindrance in a microscopic 12C + 12C fusion study. United States: N. p., 2019.
Web. doi:10.1103/physrevc.100.024619.
Godbey, Kyle, Simenel, Cedric, & Umar, A. S. Absence of hindrance in a microscopic 12C + 12C fusion study. United States. https://doi.org/10.1103/physrevc.100.024619
Godbey, Kyle, Simenel, Cedric, and Umar, A. S. Wed .
"Absence of hindrance in a microscopic 12C + 12C fusion study". United States. https://doi.org/10.1103/physrevc.100.024619. https://www.osti.gov/servlets/purl/1612036.
@article{osti_1612036,
title = {Absence of hindrance in a microscopic 12C + 12C fusion study},
author = {Godbey, Kyle and Simenel, Cedric and Umar, A. S.},
abstractNote = {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. To investigate deep sub-barrier 12C+12C fusion cross sections and establish trends for the S factor. Microscopic methods based on static Hartree-Fock and time-dependent Hartree-Fock (TDHF) mean-field theory are used to obtain 12C+12C ion-ion fusion potentials. Fusion cross sections and astrophysical S factors are then calculated using the incoming wave boundary condition method. 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 (≈1 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. Using the fully microscopic DCFHF and DC-TDHF methods, no S factor maximum is observed in the 12C+12C fusion reaction. In addition, no extreme sub-barrier hindrance is predicted at low energies. Furthermore, 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.},
doi = {10.1103/physrevc.100.024619},
journal = {Physical Review C},
number = 2,
volume = 100,
place = {United States},
year = {Wed Aug 21 00:00:00 EDT 2019},
month = {Wed Aug 21 00:00:00 EDT 2019}
}
Web of Science
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Works referencing / citing this record:
Influence of the tensor interaction on heavy-ion fusion cross sections
journal, November 2019
- Godbey, K.; Guo, Lu; Umar, A. S.
- Physical Review C, Vol. 100, Issue 5
Influence of the tensor interaction on heavy-ion fusion cross sections
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