Double-magicity of proton drip-line nucleus $^{22}$Si with \textit{ab initio} calculation
J.G. Li, H. H. Li, S. Zhang, Y. M. Xing, W. Zuo

TL;DR
This study uses extit{ab initio} calculations to investigate the double-magic nature of the proton-rich nucleus $^{22}$Si, revealing it shares magic characteristics with its mirror nucleus $^{22}$O despite differences in excitation energies.
Contribution
It provides the first extit{ab initio} evidence that $^{22}$Si exhibits double-magicity, expanding understanding of shell closures in proton-rich nuclei.
Findings
$^{22}$O confirmed as double-magic with high $E(2_1^+)$
$^{22}$Si shows lower $E(2_1^+)$ indicating weaker shell closure
Calculated MEDs agree with experimental data, supporting magicity of $^{22}$Si
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…
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Taxonomy
TopicsNuclear physics research studies · Astronomical and nuclear sciences · Quantum Chromodynamics and Particle Interactions
