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

被引:23
作者
Gorska, M
Grawe, H
Kast, D
de Angelis, G
Bizzeti, PG
Brown, BA
Dewald, A
Fahlander, C
Gadea, A
Jungclaus, A
Lieb, KP
Maier, KH
Napoli, DR
Pan, Q
Peusquens, R
De Poli, M
Rejmund, M
Tiesler, H
机构
[1] Gesell Schwerionenforsch mbH, D-64291 Darmstadt, Germany
[2] Univ Warsaw, Inst Phys Expt, Warsaw, Poland
[3] Univ Gottingen, Inst Phys 2, D-3400 Gottingen, Germany
[4] Ist Nazl Fis Nucl, Lab Nazl Legnaro, Padua, Italy
[5] Ist Nazl Fis Nucl, Sez Firenze, Florence, Italy
[6] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA
[7] Michigan State Univ, Natl Superconducting Cyclotron Lab, E Lansing, MI 48824 USA
[8] Univ Cologne, Cologne, Germany
[9] Hahn Meitner Inst Berlin GmbH, D-1000 Berlin, Germany
来源
PHYSICAL REVIEW C | 1998年 / 58卷 / 01期
关键词
D O I
10.1103/PhysRevC.58.108
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
High spin states in Sn-104 were identified in the reaction Ni-58(Cr-50, 2p2n) at 200 and 205 MeV beam energies. The gamma-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.
引用
收藏
页码:108 / 115
页数:8
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