Description of proton-rich nuclei in the region with the Gamow shell model
arXiv:1912.02364 · doi:10.1103/PhysRevC.100.064303
Abstract
The Gamow shell model is utilized to describe nuclear observables of the weakly bound and resonance isotonic states of O at proton drip-line. It is hereby shown that the presence of continuum coupling leads to complex Coulomb contributions in the spectrum of these isotones. The necessity to include the effects of three-body forces, either by a direct calculation or by adding an -dependence to the nucleon-nucleon interaction, already noticed in other theoretical models, is pointed out. It is also demonstrated that our approach is predictive for reaction observables.
12 pages, 10 figures
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Cited by in corpus (16)
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- The roles of three-nucleon force and continuum coupling in mirror symmetry breaking of oxygen mass region
- Unbound spectra of neutron-rich oxygen isotopes predicted by the Gamow shell model
- Neutron-rich calcium isotopes within realistic Gamow shell model calculations with continuum coupling
- Proton decays in Ne and Mg and isospin-symmetry breaking in carbon isotopes and isotones
- Gamow Shell Model description of Li isotopes and their mirror partners
- Continuum and three-nucleon force in Borromean system: The 17Ne case
- Double-magicity of proton drip-line nucleus Si with \textit{ab initio} calculation
- Recent progress in configuration-interaction shell model
- Calculation of the Thomas-Ehrman shift in F and O(p,p) cross section with the Gamow shell model
- Spectroscopic factors of resonance states with the Gamow shell model
- Observation and spectroscopy of proton-unbound nucleus Al
- Gamow shell model calculations for the Thomas-Ehrman shift in new isotopes 21Al
- Gamow shell model predictions for six-proton unbound nucleus Si
- Exploring the possible two-proton radioactivity of Ti
- Gamow shell model study of the 17Ne(p, p) reaction and of isospin symmetry breaking in 18Na