Sub-Barrier Coulomb Excitation of 106,108,110Sn

Details Sub-Barrier Coulomb Excitation of 106,108,110Sn Sub-Barrier Coulomb Excitation of 106,108,110Sn

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1012..296e&link_type=abstract

FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS: FINUSTAR 2. AIP Conference Proceedings, Volume 1012, pp. 296-299 (

Astronomy and Astrophysics

Astrophysics

Coulomb Energies, Shell Model, Binding Energies And Masses

Scientific paper

The reduced transition probabilities between the first excited 2+ state and the 0+ ground state, B(E20+-->2+), have been measured in 106,108,110Sn using sub-barrier Coulomb excitation in inverse kinematics at REX-ISOLDE. The results are, B(E20+-->2+) = 0.220(22), 0.226(17), and 0.228(32)e2b2, for 110Sn, 108Sn, and 106Sn, respectively. The results for 106,108Sn are preliminary. De-excitation γ-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 ν(0g7/2,2s,1d,0h11/2) model space using eeffν = 1.0 e follows the experimental values for the neutron rich Sn isotopes, but fails to reproduce the results presented here.

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