The present status of experimental approach to 100Sn and its shell model structure is given. New developments in experimental techniques, such as low background isomer spectroscopy and charged particle detection in 4π are surveyed. Based on recent experimental data shell model calculations are used to predict the structure of the single- and two-nucleon neighbours of 100Sn. The results are compared to the systematics of Coulomb energies and spin-orbit splitting and discussed with respect to future experiments.
|Number of pages||16|
|Journal||Acta Physica Polonica B|
|Publication status||Published - 1995|