1. Proton Shell Evolution below Sn132 : First Measurement of Low-Lying β -Emitting Isomers in Ag123,125
- Author
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Shudong Zhang, Naoki Fukuda, Zs. Podolyák, Shunji Nishimura, Yan-Lin Ye, T. Isobe, C. Y. Niu, Hiroki Nishibata, Xiaocan Li, Jin Wu, Ziyang Chen, Y. Jin, Toshiyuki Kubo, K. Moschner, D.X. Jiang, H.K. Wang, K. Yoshinaga, Chenyuan Li, K. Y. Chae, Jian-Ling Lou, Da Luo, G. Benzoni, A. Jungclaus, Hirofumi Watanabe, Ayumi Yagi, N. Kurz, Hiroshi Suzuki, I. Kojouharov, Hiroyoshi Sakurai, Atsuko Odahara, G. D. Kim, Young-Ki Kim, H. Y. Wu, Younghun Kwon, A. Montaner-Pizá, H. Baba, Roman Gernhäuser, G. J. Lane, Giuseppe Lorusso, Zhengyu Xu, Toshiyuki Sumikama, Hiroyuki Takeda, C. Xu, Naohito Inabe, Anna Wendt, Zs. Vajta, H. Schaffner, F. C. L. Crespi, Gary Simpson, F. G. Kondev, C. G. Wu, Z. H. Li, F. Naqvi, D. Kameda, P. A. Söderström, P. Doornenbal, K. Steiger, X. Wang, Zena Patel, F. Browne, H. S. Jung, Cenxi Yuan, Megumi Niikura, Jan Taprogge, Guillaume Gey, R. Orlandi, C. G. Wang, and Hui Hua
- Subjects
Physics ,Atomic orbital ,Isotope ,0103 physical sciences ,Magnetic monopole ,General Physics and Astronomy ,Atomic physics ,010306 general physics ,Spectroscopy ,7. Clean energy ,01 natural sciences - Abstract
The β-delayed γ-ray spectroscopy of neutron-rich 123;125Ag isotopes is investigated at the Radioactive Isotope Beam Factory of RIKEN and the long-predicted 1/2¯ β-emitting isomers in 123;125Ag 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. Shellmodel calculations with the state-of-the-art VMU plus M3Y spin-orbit interaction give a satisfactory description of the low-lying states in 123;125Ag. 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 123Ag can be well interpreted in terms of the monopole shift of the π1g9/2 orbitals mainly caused by the increasing occupation of ʋ1h11/2 orbitals.
- Published
- 2019
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