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Phys. Rev. C 65, 021302(R) (2002) [5 pages]

100Sn core excitations in 102In

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M. Lipoglavšek1,2, C. Baktash1, M. P. Carpenter3, D. J. Dean1, T. Engeland4, C. Fahlander5, M. Hjorth-Jensen4, R. V. F. Janssens3, A. Likar2, J. Nyberg6, E. Osnes4, S. D. Paul1, A. Piechaczek7, D. C. Radford1, D. Rudolph5, D. Seweryniak3, D. G. Sarantites8, M. Vencelj2, and C.-H. Yu1
1Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831-6371
2J. Stefan Institute, Ljubljana, Slovenia
3Argonne National Laboratory, Argonne, Illinois 60439
4Department of Physics, University of Oslo, Oslo, Norway
5Department of Physics, Lund University, Lund, Sweden
6Department of Neutron Research, Uppsala University, Uppsala, Sweden
7Louisiana State University, Baton Rouge, Louisiana 70803
8Department of Chemistry, Washington University, St. Louis, Missouri 63130

Received 14 October 2001; published 16 January 2002

Nuclei in the vicinity of the doubly-magic 100Sn nucleus have been studied, and an extended level scheme for 102In has been established. The level structure comprises both the negative parity states involving the νh11/2 orbital, and levels due to the breakup of the doubly-magic 100Sn core. Results of a large-scale shell model calculation, using realistic and empirical effective interactions with 88Sr as a core, are in very good agreement with the experimental data.

© 2002 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.65.021302
DOI:
10.1103/PhysRevC.65.021302
PACS:
21.10.-k, 21.60.Cs, 23.20.Lv, 27.60.+j
 
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