Structure of the neutron-rich isotones: A shell model analysis
Phys. Rev. C 114, 044302 – Published 1 October, 2026
DOI: https://doi.org/10.1103/sbnc-hccd
Abstract
Shell model calculations for the neutron-rich isotones were performed with two different parametrizations. The one refined to explain the isomerism in was found to be the only one able to reproduce the more recent data on and, in general, to give a better reproduction of the nuclei in this region. For more exotic nuclei approaching the -process path, this refined parametrization predicts the existence of isomeric states with spin-parities and in the even-mass isotones and in the odd-mass isotones. Also, it predicts ground-state spin-parities of for and for and , with low-energy long-lived isomers present. The remaining deficiencies of the interaction are related to the properties of the orbital and are influenced by octupole collectivity. The presented predictions provide guidance and can be tested in the near future at radioactive-beam facilities.