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Cited 11 time in webofscience Cited 7 time in scopus
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Proton Shell Evolution below Sn-132: First Measurement of Low-Lying beta-Emitting Isomers in Ag-123,Ag-325

Authors
Chen, ZQLi, ZHHua, HWatanabe, HYuan, CXZhang, SQLorusso, GNishimura, SBaba, HBrowne, FBenzoni, GChae, K. Y.Crespi, F. C. L.Doornenbal, P.Fukuda, N.Gey, G.Gernhaeuser, R.Inabe, NIsobe, TJiang, DXJungclaus, AJung, HSJin, YKameda, DKim, GDKim, Yong KyunKojouharov, IKondev, FGKubo, TKurz, NKwon, YKLi, XQLou, JLLane, GJLi, CGLuo, DWMontaner-Piza, AMoschner, KNiu, CYNaqvi, FNiikura, MNishibata, HOdahara, AOrlandi, RPatel, ZPodolyak, ZsSumikama, TSoderstrom, PASakurai, HSchaffner, HSimpson, GSSteiger, KSuzuki, HTaprogge, JTakeda, HVajta, ZsWang, HKWu, JWendt, AWang, CGWu, HYWang, XWu, CGXu, CXu, ZYYagi, AYe, YLYoshinaga, K
Issue Date
May-2019
Publisher
AMER PHYSICAL SOC
Citation
PHYSICAL REVIEW LETTERS, v.122, no.21, pp.1 - 6
Indexed
SCIE
SCOPUS
Journal Title
PHYSICAL REVIEW LETTERS
Volume
122
Number
21
Start Page
1
End Page
6
URI
https://scholarworks.bwise.kr/hanyang/handle/2021.sw.hanyang/14180
DOI
10.1103/PhysRevLett.122.212502
ISSN
0031-9007
Abstract
The beta-delayed gamma-ray spectroscopy of neutron-rich Ag-123,Ag-325 isotopes is investigated at the Radioactive Isotope Beam Factory of RIKEN, and the long-predicted 1/2(-) beta-emitting isomers in Ag-123,Ag-325 are identified for the first time. With the new experimental results, the systematic trend of energy spacing between the lowest 9/2(+) and 1/2(-) levels is extended in Ag isotopes up to N = 78, providing a clear signal for the reduction of the Z = 40 subshell gap in Ag towards N = 82. Shell-model calculations with the state-of-the-art V-MU plus M3Y spin-orbit interaction give a satisfactory description of the low-lying states in Ag-123,Ag-325. The tensor force is found to play a crucial role in the evolution of the size of the Z = 40 subshell gap. The observed inversion of the single-particle levels around Ag-123 can be well interpreted in terms of the monopole shift of the pi 1g(9/2) orbitals mainly caused by the increasing occupation of nu 1h(11/2) orbitals.
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