Potential model with bound-to-continuum approach for low-energy nucleon radiative capture by C and O
arXiv:2109.03776 · doi:10.1103/PhysRevC.104.034622
Abstract
The nucleon radiative capture reactions are important in pure and applied nuclear physics, especially in nuclear astrophysics. The keV-nucleon radiative capture reactions are studied with C and O targets using the bound-to-continuum potential model in which both scattering and bound states are treated simultaneously and based on the Skyrme Hartree-Fock approximation. The obtained results are shown to be in good agreement with the available experimental data. Alongside astrophysical aspects, the nuclear structure features were revisited for enlarging the prospect of adopting the nucleon radiative capture processes as a spectroscopic tool.
arXiv comment9 pages, 5 figures, accepted for publication in PRC
References in corpus (12)
- NACRE II: an update of the NACRE compilation of charged-particle-induced thermonuclear reaction rates for nuclei with mass number
- Radiative capture of nucleons at astrophysical energies with single-particle states
- Direct radiative capture of p-wave neutrons
- Non-resonant direct p- and d-wave neutron capture by 12C
- The radiative neutron capture on 2H, 6Li, 7Li, 12C and 13C at astrophysical energies
- Structure of and astrophysical factor in Skyrme Hartree-Fock theory
- Re-evaluation of the O(,)O cross section at astrophysical energies and its role as neutron poison in the process
- Breakup of the weakly bound 17F nucleus
- Effects of nonlocality of nuclear potentials on direct capture reactions
- Neutron-induced nucleosynthesis
- Bound-to-continuum potential model for the reactions of the CNO cycle
- Folding model approach to the elastic C scattering at low energies and radiative capture C reactions