Gustafsson FP, Rodríguez LV, Garcia Ruiz RF, Miyagi T, Bai SW, Balabanski DL, Binnersley CL, Bissell ML, Blaum K, Cheal B, Cocolios TE, Farooq-Smith GJ, Flanagan KT, Franchoo S, Galindo-Uribarri A, Georgiev G, Gins W, Gorges C, De Groote RP, Heylen H, Holt JD, Kanellakopoulos A, Karthein J, Kaufmann S, Koszorús , König K, Lagaki V, Lechner S, Maass B, Malbrunot-Ettenauer S, Nazarewicz W, Neugart R, Neyens G, Nörtershäuser W, Otsuka T, Reinhard PG, Rondelez N, Romero-Romero E, Ricketts CM, Sailer S, Sánchez R, Schmidt S, Schwenk A, Stroberg SR, Shimizu N, Tsunoda Y, Vernon AR, Wehner L, Wilkins SG, Wraith C, Xie L, Xu ZY, Yang XF, Yordanov DT (2025)
Publication Type: Journal article
Publication year: 2025
Book Volume: 135
Article Number: 222501
Journal Issue: 22
DOI: 10.1103/wbdx-k3cd
We report nuclear charge radii for the isotopes Sn104–134, measured using two different collinear laser spectroscopy techniques at ISOLDE-CERN. These measurements clarify the archlike 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.
APA:
Gustafsson, F.P., Rodríguez, L.V., Garcia Ruiz, R.F., Miyagi, T., Bai, S.W., Balabanski, D.L.,... Yordanov, D.T. (2025). Charge Radii Measurements of Exotic Tin Isotopes in the Proximity of N=50 and N=82. Physical Review Letters, 135(22). https://doi.org/10.1103/wbdx-k3cd
MLA:
Gustafsson, F. P., et al. "Charge Radii Measurements of Exotic Tin Isotopes in the Proximity of N=50 and N=82." Physical Review Letters 135.22 (2025).
BibTeX: Download