Structure of high-spin states in 91Sr and 92Sr -: art. no. 034323

被引:28
作者
Stefanova, EA
Danchev, M
Schwenger, R
Balabanski, DL
Carpenter, MP
Djongolov, M
Fischer, SM
Hartley, DJ
Janssens, RVF
Mueller, WF
Nisius, D
Reviol, W
Riedinger, LL
Zeidan, O
机构
[1] Bulgarian Acad Sci, Inst Nucl Res & Nucl Energy, BU-1784 Sofia, Bulgaria
[2] Rossendorf Inc, Forschungszentrum Rossendorf EV, Inst Kern & Hadronenphys, D-01314 Dresden, Germany
[3] Univ Sofia, Fac Phys, Sofia 1164, Bulgaria
[4] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA
[5] Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA
[6] Michigan State Univ, NSCL, E Lansing, MI 48824 USA
[7] Washington Univ, Dept Chem, St Louis, MO 63130 USA
关键词
D O I
10.1103/PhysRevC.65.034323
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
The nuclei Sr-91 and Sr-92 were produced at high spin as fission fragments following the fusion reaction S-36+Tb-159 at 165 MeV. gamma rays were detected with the Gammasphere array. The level schemes of Sr-91 and Sr-92 were extended up to Eapproximate to6 MeV and Eapproximate to8 MeV, respectively. Level structures in Sr-91 and Sr-92 were interpreted in shell-model calculations performed in the configuration space (0f(5/2), 1p(3/2), 1p(1/2), 0g(9/2)) for the protons and (1p(1/2), 0g(9/2), 1d(5/2)) for the neutrons. Negative-parity states in the yrast sequences are described in these calculations by coupling 3(-) proton excitations to the unpaired 1d(5/2) neutrons. A possible reduction of the gap between the proton 1p(3/2) and 1p(1/2) orbitals in Sr-92 is discussed.
引用
收藏
页码:343231 / 3432310
页数:10
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