Abstract
Fully self-consistent spherical Hartree–Fock HF based random-phase approximation RPA calculations were performed for tin isotopes 100,116,132Sn using five type of Skyrme interaction: QMC2, LNS5, BsK21, NRAPR and MSKA. Isoscalar E0, E1, E2 and E3 transition strength distribution, centroid energy and transition density distribution have been investigated and compared with the available experimental data. Relations between the parameters and properties of the investigated Skyrme force, with the calculated properties of nuclei are analyzed.
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