@inproceedings{7ee2ffc30b524c8a9ee8070c6a724baf,
title = "Sub-barrier Coulomb excitation of Sn-106,Sn-108,Sn-110",
abstract = "The reduced transition probabilities between the first excited 2(+) state and the 0(+) ground state, B(E2; 0(+) -> 2(+)), have been measured in Sn-106,Sn-108,Sn-110 using sub-barrier Coulomb excitation in inverse kinematics at REX-ISOLDE. The results are, B(E2;0(+) -> 2(+)) = 0.220(22),0.226(17), and 0.228(32) e(2)b(2), for Sn-110, Sn-108, and Sn-106, respectively. The results for Sn-106,Sn-108 are preliminary. De-excitation gamma-rays were detected by the MINIBALL Ge-array. The B(E2) reveals detailed information about the nuclear wave function. A shell model prediction based on an effective CD-Bonn interaction in the nu(0g(7/2),2s, 1d, 0h(11/2)) model space using e(eff)(nu) =1.0 e follows the experimental values for the neutron rich Sn isotopes, but fails to reproduce the results presented here.",
author = "A. Ekstrom and J. Cederkaell and C. Fahlander and A. Hjorth-Jensen and F. Ames and Butler, {P. A.} and T. Davinson and J. Eberth and G. Georgiev and A. Gorgen and M. Gorska and D. Habs and M. Huyse and O. Ivanov and J. Iwanicki and O. Kester and U. Koester and Marsh, {B. A.} and P. Reiter and H. Scheit and D. Schwalm and S. Siem and I. Stefanescu and Tveten, {G. M.} and {Van de Walle}, J. and {Van Duppen}, P. and D. Voulot and N. Warr and D. Weisshaar and E. Wenander and M. Zielinska",
note = "Conference on Frontiers in Nuclear Structure, Astrophysics, and Reactions, Crete, GREECE, SEP 10-14, 2007",
year = "2008",
language = "Undefined/Unknown",
volume = "1012",
series = "AIP CONFERENCE PROCEEDINGS",
pages = "296--299",
editor = "P Demetriuo and SV Harissopulos",
booktitle = "FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS: FINUSTAR 2",
}