Abstract
Yrast levels of Ni, Cu and Zn isotopes for have been described by state-of-the-art shell model calculations with three recently available interactions using Ni as a core in the model space. The results are unsatisfactory viz. large for very neutron rich nuclei, small B(E2) values in comparison to experimental values. These results indicate an importance of inclusion of and orbitals in the model space to reproduce collectivity in this region.
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