1. Nuclear structure far off stability —Implications for nuclear astrophysics.
- Author
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Fülöp, Zsolt, Gyürky, György, Somorjai, Endre, Grawe, H., Blazhev, A., Górska, M., Grzywacz, R., Mach, H., and Mukha, I.
- Abstract
The single-particle structure and shell gap of 100Sn as inferred from previous in-beam γ-ray spectroscopy has been confirmed in recent studies of seniority and spin-gap isomers by γγ, βγ, βpγ, pγ and 2pγ spectroscopy. The results for 94,95Ag, 98Cd and its N=50 isotones 96Pd and 94Ru stress the importance of large-scale shell model calculations employing realistic interactions for the isomerism, np-nh excitations, seniority mixing and E2 polarisation of the 100Sn core. The strong monopole interaction of the Δl=0, 1 spin/isospin-flip partners πg9/2-νg7/2 along the N=50 isotones and the πf5/2-νg9/2 pair of nucleons along the Z=28 Ni isotopes are decisive for the evolution of the shell structure towards 100Sn and 78Ni. It can be traced back to the tensor force in the effective nucleon-nucleon interaction and provides a straightforward explanation for new shells in neutron-rich light nuclei, implying qualitative predictions for new N=32, 34 subshells in Ca isotopes, persistence of the 78Ni proton and neutron shell gaps and non-equivalence of the g9/2 valence mirror Ni isotopes and N=50 isotones. This is corroborated by recent experimental data on 56,58Cr and 70-76Ni. The implication of monopole driven shell evolution for apparent spin-orbit splitting towards N ≫ Z and structure along the astrophysical r-path between N=50 and N=82 is discussed [ABSTRACT FROM AUTHOR]
- Published
- 2006
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