Abstract
We present results of large-scale shell-model calculations for the hole nuclei below . We discuss structures of , , and with emphasis on the monopole effects and excitations across the neutron shell gap, and further predict low-lying levels for the more exotic . It is demonstrated that the monopole corrections in the Hamiltonian, which dynamically affect occupations of relevant orbits, can lead to interesting consequences for the shell evolution. It is found especially that the monopole terms, previously introduced to reproduce the cross-shell excitations of the and states in , shows more pronounced effects on the nuclei. In , the cross-shell excitations of and are pushed down significantly by the monopole terms, and in , the same monopole terms reverse the order of the single-hole states of and , causing as the ground state for this nucleus. The structure of isomeric states in the nuclei is also discussed.
- Received 19 July 2016
- Revised 3 November 2016
DOI:https://doi.org/10.1103/PhysRevC.95.011304
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