Folding model approach to the elastic C scattering at low energies and radiative capture C reactions
arXiv:2011.02622 · doi:10.1016/j.nuclphysa.2020.122078
Abstract
The proton radiative capture C reactions at astrophysical energies, key processes in the CNO cycle, are revisited in the potential model with the proton-nucleus potential for both the scattering and bound states obtained in the folding model, using a realistic density dependent nucleon-nucleon interaction. For the consistency, this same folding model is also used to calculate the optical potential of the elastic C scattering at energies around the Coulomb barrier. The folded C optical potentials are shown to account well for both the elastic C3 scattering and astrophysical factors of the radiative capture C reactions.
Accepted for publication in Nuclear Physics A
References in corpus (5)
- Equation of state of the neutron star matter, and the nuclear symmetry energy
- Folding model study of the isobaric analog excitation: isovector density dependence, Lane potential and nuclear symmetry energy
- Rearrangement term in the nonlocal folding model of the nucleon optical potential
- Internal and external radiative widths in the combined R-matrix and potential model formalism
- Neutron transition strengths of states in the neutron rich Oxygen isotopes determined from inelastic proton scattering
Cited by in corpus (4)
- Bound-to-continuum potential model for the reactions of the CNO cycle
- Low-energy Li()Li and Be()B radiative capture reactions within the Skyrme Hartree-Fock approach
- Study of nonlocality effects in direct capture reactions with Lagrange-mesh -matrix method
- Potential model with bound-to-continuum approach for low-energy nucleon radiative capture by C and O