Persistence of the shell gap in isobars: Identification of a possible s isomer in Co and decay to Ni
arXiv:2101.06246 · doi:10.1103/PhysRevC.103.064328
Abstract
Background: The evolution of shell structure around doubly magic exotic nuclei is of great interest in nuclear physics and astrophysics. In the `southwest' region of Ni, the development of deformation might trigger a major shift in our understanding of explosive nucleosynthesis. To this end, new spectroscopic information on key close-lying nuclei is very valuable. Purpose: We intend to measure the isomeric and decay of Co, with one-proton and two-neutron holes relative to Ni, to access new nuclear structure information in Co and its -decay daughters Ni and Ni. Methods: The nucleus Co is produced in relativistic in-flight fission reactions of U at the Radioactive Ion Beam Factory in the RIKEN Nishina Center. Its isomeric and decay are studied exploiting the BigRIPS and EURICA setups. Results: We obtain partial -decay spectra for Ni and Ni, and report a new isomeric transition in Co. The energy [ keV] and half-life [ s] of the delayed ray lend support for the existence of a isomeric state at 1914(2) keV. A comparison with PFSDG-U shell-model calculations provides a good account for the observed states in Ni, but the first calculated level in Co, a prolate state, is predicted about 1 MeV below the observed level. Conclusions: The spherical-like structure of the lowest-lying excited states in Ni is proved. In the case of Co, the results suggest that the dominance of the spherical configurations over the deformed ones might be stronger than expected below Ni. Further experimental efforts to discern the nature of the isomer are necessary.
arXiv comment15 pages, 6 figures, 3 tables. Physical Review C
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