Yrast structure of the neutron-rich N=31 isotones 51Ca and 52Sc

被引:33
|
作者
Fornal, B. [1 ]
Janssens, R. V. F. [2 ]
Broda, R. [1 ]
Marginean, N. [3 ,4 ]
Beghini, S. [5 ,6 ]
Corradi, L. [3 ]
Carpenter, M. P. [2 ]
De Angelis, G. [3 ]
Della Vedova, F. [3 ]
Farnea, E. [6 ]
Fioretto, E. [3 ]
Gadea, A. [3 ]
Guiot, B. [3 ]
Honma, M. [7 ]
Krolas, W. [1 ,8 ]
Lauritsen, T. [2 ]
Lunardi, S. [5 ,6 ]
Mantica, P. F. [9 ]
Mason, P. [6 ]
Montagnoli, G. [5 ,6 ]
Napoli, D. R. [3 ]
Otsuka, T. [10 ,11 ]
Pawlat, T. [1 ]
Pollarolo, G. [12 ,13 ]
Scarlassara, F. [5 ,6 ]
Stefanini, A. M. [3 ]
Seweryniak, D. [2 ]
Szilner, S. [14 ]
Ur, C. A. [6 ]
Trotta, M. [15 ]
Valiente-Dobon, J. J. [3 ]
Wrzesinski, J. [1 ]
Zhu, S. [2 ]
机构
[1] Inst Nucl Phys, Polish Acad Sci, PL-31342 Krakow, Poland
[2] Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA
[3] Ist Nazl Fis Nucl, Lab Nazl Legnaro, I-35020 Legnaro, Italy
[4] Horia Hulubei Natl Inst Phys & Nucl Engn, RO-077125 Bucharest, Romania
[5] Univ Padua, Dipartimento Fis, I-35131 Padua, Italy
[6] Ist Nazl Fis Nucl, Sezione Padova, I-35131 Padua, Italy
[7] Univ Aizu, Ctr Math Sci, Fukushima 9658580, Japan
[8] Oak Ridge Natl Lab, Joint Inst Heavy Ion Res, Oak Ridge, TN 37831 USA
[9] Michigan State Univ, Natl Superconducting Cyclotron Lab, E Lansing, MI 48824 USA
[10] Univ Tokyo, Dept Phys, Tokyo 1130033, Japan
[11] RIKEN, Wako, Saitama 3510198, Japan
[12] Univ Turin, Dipartimento Fis Teor, I-10125 Turin, Italy
[13] Ist Nazl Fis Nucl, I-10125 Turin, Italy
[14] Rudjer Boskovic Inst, HR-10001 Zagreb, Croatia
[15] Ist Nazl Fis Nucl, I-80126 Naples, Italy
来源
PHYSICAL REVIEW C | 2008年 / 77卷 / 01期
关键词
D O I
10.1103/PhysRevC.77.014304
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 low-lying yrast states in the Ca-51 and Sc-52 nuclei were investigated to obtain information on the evolution of the p(1/2) and f(5/2) neutron single-particle orbitals in neutron-rich nuclei near proton number Z=20. Level structures associated with neutron excitations into these two orbitals and with proton excitations across the Z=20 shell gap were identified. Shell-model calculations with the recently proposed GXPF1A interaction account reasonably well for the fp-shell states. The energy separation between the nu p(1/2) and nu f(5/2) orbitals in the Ca isotopes appears to be overestimated by the GXPF1A Hamiltonian.
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页数:7
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