Double-magicity of proton drip-line nucleus Si with \textit{ab initio} calculation
arXiv:2512.15097 · doi:10.1016/j.physletb.2023.138197
Abstract
New magic numbers have been discovered in the neutron-rich region of the nuclear chart. However, there has been a lack of research on proton-rich nuclei. O, the mirror nucleus of Si, is a double-magic nucleus bearing a high . Whether Si exhibits double-magic characters is an intriguing topic. To investigate this matter, we utilized \textit{ab initio} valence space in-medium similarity renormalization group for Si/O, and their nearby nuclei. Our \textit{ab initio} calculations provide good descriptions for the double magicity of O, as well as the shell evolution of and through . The computed indicate that the closure of sub-shell in proton-rich nuclei is weaker than the sub-shell closure in their mirror nuclei. Particularly, the calculated of Si is 800 keV lower than the one of O. To further explore the magicity of Si, the mirror energy difference (MED) of Si/Mg, Si/Ne, as well as Si/O are calculated. The results demonstrate that the calculated MEDs agree well with available experimental data, and the values of Si are all lower than their respective mirror nuclei due to the Thomas-Ehrman shift with large occupation. Moreover, our calculation provides that the many-body configurations of the low-lying state of Si/O are nearly identical despite the fact that the states bearing large MED. In conclusion, our \textit{ab initio} results suggest that Si is a double magic nucleus, similar to its mirror nucleus O, albeit with a lower .
6 Pages, 4 Figures
References in corpus (15)
- Chiral effective field theory and nuclear forces
- Nuclear magic numbers: new features far from stability
- Improved nuclear matter calculations from chiral low-momentum interactions
- Accurate nuclear radii and binding energies from a chiral interaction
- Similarity Renormalization Group for Nucleon-Nucleon Interactions
- Evolution of shell structure in neutron-rich calcium isotopes
- A nucleus-dependent valence-space approach to nuclear structure
- Shell Model in the Complex Energy Plane
- Charge Symmetry Breaking and QCD
- Converged ab initio calculations of heavy nuclei
- Three-body forces and proton-rich nuclei
- In-medium similarity renormalization group with three-body operators
- Ab initio Gamow in-medium similarity renormalization group with resonance and continuum
- Toward Scalable Many-Body Calculations for Nuclear Open Quantum Systems using the Gamow Shell Model
- Description of proton-rich nuclei in the region with the Gamow shell model
Cited by in corpus (6)
- Ab initio study of island of inversion in odd- nuclei: Structure of Mg
- Gamow shell model predictions for six-proton unbound nucleus Si
- Gamow shell model study of the 17Ne(p, p) reaction and of isospin symmetry breaking in 18Na
- Evolution of shell structure at and 34: Insights from realistic nuclear forces
- Large scale shell model calculation for collectivity in nuclei beyond 78Ni
- Ab initio study of -decay and pairing in nuclei