N=82 shell quenching of the classical r-process "waiting-point" nucleus 130C -: art. no. 162503

被引:195
作者
Dillmann, I [1 ]
Kratz, KL
Wöhr, A
Arndt, O
Brown, BA
Hoff, P
Hjorth-Jensen, M
Köster, U
Ostrowski, AN
Pfeiffer, B
Seweryniak, D
Shergur, J
Walters, WB
机构
[1] Johannes Gutenberg Univ Mainz, Inst Kernchem, D-6500 Mainz, Germany
[2] Univ Basel, Dept Phys & Astron, Basel, Switzerland
[3] Univ Maryland, Dept Chem, College Pk, MD 20742 USA
[4] Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA
[5] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA
[6] Michigan State Univ, NSCL, E Lansing, MI 48824 USA
[7] Univ Oslo, Dept Chem, Oslo, Norway
[8] Univ Oslo, Dept Phys, Oslo, Norway
[9] CERN, Geneva, Switzerland
[10] Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA
关键词
D O I
10.1103/PhysRevLett.91.162503
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
First beta- and gamma-spectroscopic decay studies of the N=82 r-process "waiting-point" nuclide Cd-130 have been performed at CERN/ISOLDE using the highest achievable isotopic selectivity. Several nuclear-physics surprises have been discovered. The first one is the unanticipatedly high energy of 2.12 MeV for the [pig(9/2)circle timesnug(7/2)] 1(+) level in In-130, which is fed by the main Gamow-Teller transition. The second surprise is the rather high Q(beta) value of 8.34 MeV, which is in agreement only with recent mass models that include the phenomenon of N=82 shell quenching. Possible implications of these new results on the formation of the Asimilar or equal to130 r-process abundance peak are presented.
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