High-spin states in the semimagic nucleus Y89 and neutron-core excitations in the N=50 isotones

Z. Q. Li (李志泉), S. Y. Wang (王守宇), C. Y. Niu (牛晨阳), B. Qi (亓斌), S. Wang (王硕), D. P. Sun (孙大鹏), C. Liu (刘晨), C. J. Xu (徐长江), L. Liu (刘雷), P. Zhang (张盼), X. G. Wu (吴晓光), G. S. Li (李广生), C. Y. He (贺创业), Y. Zheng (郑云), C. B. Li (李聪博), B. B. Yu (于蓓蓓), S. P. Hu (胡世鹏), S. H. Yao (姚顺和), X. P. Cao (曹雪鹏), and J. L. Wang (汪金龙)
Phys. Rev. C 94, 014315 – Published 19 July 2016; Erratum Phys. Rev. C 102, 019902 (2020)

Abstract

The semimagic nucleus Y89 has been investigated using the Se82(B11,4n) reaction at beam energies of 48 and 52 MeV. More than 24 new transitions have been identified, leading to a considerable extension of the level structures of Y89. The experimental results are compared with the large-basis shell model calculations. They show that cross-shell neutron excitations play a pivotal role in high-spin level structures of Y89. The systematic features of neutron-core excitations in the N=50 isotones are also discussed.

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  • Received 31 January 2016

DOI:https://doi.org/10.1103/PhysRevC.94.014315

©2016 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Erratum

Erratum: High-spin states in the semimagic nucleus Y89 and neutron-core excitations in the N=50 isotones [Phys. Rev. C 94, 014315 (2016)]

Z. Q. Li (李志泉), S. Y. Wang (王守宇), C. Y. Niu (牛晨阳), B. Qi (亓斌), S. Wang (王硕), D. P. Sun (孙大鹏), C. Liu (刘晨), C. J. Xu (徐长江), L. Liu (刘雷), P. Zhang (张盼), X. G. Wu (吴晓光), G. S. Li (李广生), C. Y. He (贺创业), Y. Zheng (郑云), C. B. Li (李聪博), B. B. Yu (于蓓蓓), S. P. Hu (胡世鹏), S. H. Yao (姚顺和), X. P. Cao (曹雪鹏), and J. L. Wang (汪金龙)
Phys. Rev. C 102, 019902 (2020)

Authors & Affiliations

Z. Q. Li (李志泉)1, S. Y. Wang (王守宇)1,*, C. Y. Niu (牛晨阳)1, B. Qi (亓斌)1, S. Wang (王硕)1, D. P. Sun (孙大鹏)1, C. Liu (刘晨)1, C. J. Xu (徐长江)1, L. Liu (刘雷)1, P. Zhang (张盼)1, X. G. Wu (吴晓光)2, G. S. Li (李广生)2, C. Y. He (贺创业)2, Y. Zheng (郑云)2, C. B. Li (李聪博)2, B. B. Yu (于蓓蓓)2, S. P. Hu (胡世鹏)2, S. H. Yao (姚顺和)2, X. P. Cao (曹雪鹏)2, and J. L. Wang (汪金龙)2

  • 1Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, Institute of Space Sciences, Shandong University, Weihai 264209, China
  • 2China Institute of Atomic Energy, Beijing 102413, China

  • *Corresponding author: sywang@sdu.edu.cn

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Vol. 94, Iss. 1 — July 2016

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