Reduced transition probabilities to the first 2+ state in 52,54,56Ti and development of shell closures at N=32,34 -: art. no. 041302

被引:134
作者
Dinca, DC [1 ]
Janssens, RVF
Gade, A
Bazin, D
Broda, R
Brown, BA
Campbell, CM
Carpenter, MP
Chowdhury, P
Cook, JM
Deacon, AN
Fornal, B
Freeman, SJ
Glasmacher, T
Honma, M
Kondev, FG
Lecouey, JL
Liddick, SN
Mantica, PF
Mueller, WF
Olliver, H
Otsuka, T
Terry, JR
Tomlin, BA
Yoneda, K
机构
[1] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA
[2] Michigan State Univ, Natl Superconducting Cyclotron Lab, E Lansing, MI 48824 USA
[3] Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA
[4] Polish Acad Sci, Inst Nucl Phys, PL-31342 Krakow, Poland
[5] Univ Massachusetts, Lowell, MA 01854 USA
[6] Univ Manchester, Schuster Lab, Dept Phys & Astron, Manchester M13 9PL, Lancs, England
[7] Univ Aizu, Ctr Math Sci, Fukushima 9658580, Japan
[8] Argonne Natl Lab, Nucl Engn Div, Argonne, IL 60439 USA
[9] Michigan State Univ, Dept Chem, E Lansing, MI 48824 USA
[10] Univ Tokyo, Dept Phys, Tokyo 1130033, Japan
[11] Univ Tokyo, Ctr Nucl Study, Tokyo 1130033, Japan
[12] RIKEN, Wako, Saitama 3510198, Japan
来源
PHYSICAL REVIEW C | 2005年 / 71卷 / 04期
关键词
D O I
10.1103/PhysRevC.71.041302
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 even Ti52-56 isotopes have been studied with intermediate-energy Coulomb excitation and absolute B(E2;0(+)-> 2(1)(+)) transition rates have been obtained. These data confirm the presence of a subshell closure at neutron number N=32 in neutron-rich nuclei above the doubly magic nucleus Ca-48 and provide no direct evidence for the predicted N=34 closure. Large-scale shell model calculations with the most recent effective interactions are unable to reproduce the magnitude of the measured strengths in the semimagic Ti nuclei and their strong variation with neutron number.
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