Charge Radii Measurements of Exotic Tin Isotopes in the Proximity of $N=50$ and $N=82$
F. P. Gustafsson, L. V. Rodríguez, R. F. Garcia Ruiz, T. Miyagi, S. W. Bai, D. L. Balabanski, C. L. Binnersley, M. L. Bissell, K. Blaum, B. Cheal, T. E. Cocolios, G. J. Farooq-Smith, K. T. Flanagan, S. Franchoo, A. Galindo-Uribarri, G. Georgiev, W. Gins, C. Gorges, R. P. de Groote, H. Heylen, J. D. Holt, A. Kanellakopoulos, J. Karthein, S. Kaufmann, Á. Koszorús, K. König, V. Lagaki, S. Lechner, B. Maass, S. Malbrunot-Ettenauer, W. Nazarewicz, R. Neugart, G. Neyens, W. Nörtershäuser, T. Otsuka, P. -G. Reinhard, N. Rondelez, E. Romero-Romero, C. M. Ricketts, S. Sailer, R. Sánchez, S. Schmidt, A. Schwenk, S. R. Stroberg, N. Shimizu, Y. Tsunoda, A. R. Vernon, L. Wehner, S. G. Wilkins, C. Wraith, L. Xie, Z. Y. Xu, X. F. Yang, D. T. Yordanov
Abstract
We report nuclear charge radii for the isotopes $^{104-134}$Sn, measured using two different collinear laser spectroscopy techniques at ISOLDE-CERN. These measurements clarify the arch-like trend in charge radii along the isotopic chain and reveal an odd-even staggering that is more pronounced near the $N=50$ and $N=82$ shell closures. The observed local trends are well described by both nuclear density functional theory and valence space in-medium similarity renormalization group calculations. Both theories predict appreciable contributions from beyond-mean-field correlations to the charge radii of the neutron-deficient tin isotopes. The models, however, fall short of reproducing the magnitude of the known $B(E2)$ transition probabilities, highlighting the remaining challenges in achieving a unified description of both ground-state properties and collective phenomena.
