Phys. Rev. C 58, 108 - 115 (1998)

Structure of high spin states in 104Sn: E2 and E3 polarization of the 100Sn core

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M. Górska1,2, H. Grawe1, D. Kast3, G. de Angelis4, P. G. Bizzeti5, B. A. Brown6, A. Dewald7, C. Fahlander4, A. Gadea4, A. Jungclaus3, K. P. Lieb3, K. H. Maier8, D. R. Napoli4, Q. Pan4, R. Peusquens7, M. De Poli4, M. Rejmund1,2, and H. Tiesler7
1Gesellschaft für Schwerionenforschung, Planckstrasse 1, D-64291 Darmstadt, Germany
2Institute of Experimental Physics, University of Warsaw, Warsaw, Poland
3II. Physikalisches Institut, Universität Göttingen, Göttingen, Germany
4Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Legnaro, Legnaro (Padova), Italy
5Istituto Nazionale di Fisica Nucleare Sezione di Firenze, Firenze, Italy
6Department of Physics and Astronomy and National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan
7Universität zu Köln, Köln, Germany
8Hahn-Meitner Institute, Berlin, Germany

Received 18 March 1998

High spin states in 104Sn were identified in the reaction 58Ni(50Cr, 2p2n) at 200 and 205 MeV beam energies. The γ-ray energies, intensities, multipolarities, and lifetimes of high spin states were measured with the GASP spectrometer array in combination with a plunger apparatus by means of the recoil distance Doppler shift method. The deduced level scheme and transition probabilities are compared to the results of large-scale shell model calculations using three independent two-body interactions. The agreement of the level energies is satisfactory, except for a cascade of dipole transitions at high spins. The general good agreement found for E2 transition strengths implies a large effective neutron polarization charge. The shell-model calculations do not account for the measured enhanced E3 transitions for which a core excited octupole phonon admixture is indicated.


©1998 The American Physical Society

URL: http://link.aps.org/doi/10.1103/PhysRevC.58.108
DOI: 10.1103/PhysRevC.58.108
PACS: 21.10.Tg, 21.60.Cs, 23.20.Lv, 27.60.+j

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