Single-particle structures, high-spin isomers, and a strongly coupled band in odd-odd Sb120

L. Liu (刘雷), S. Y. Wang (王守宇), Z. Q. Chen (陈志强), C. Liu (刘晨), B. Qi (亓斌), D. P. Sun (孙大鹏), S. Wang (王硕), Q. An (安强), C. J. Xu (徐长江), P. Zhang (张盼), Z. Q. Li (李志泉), C. Y. Niu (牛晨阳), 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), S. H. Yao (姚顺和), S. P. Hu (胡世鹏), H. W. Li (李红伟), J. J. Liu (刘嘉健), and J. L. Wang (汪金龙)
Phys. Rev. C 90, 014313 – Published 17 July 2014; Erratum Phys. Rev. C 108, 059901 (2023)

Abstract

Excited states in Sb120 have been investigated using the Cd116(Li7,3n)Sb120 reaction at a beam energy of 34 MeV. A total of 15 new γ rays were added into the level scheme of Sb120. Most of the observed single-particle states can be interpreted in terms of weak coupling of the odd proton and odd neutron to an excited Sn118 core involving either vibrational states or broken neutron pairs. The previously known strongly coupled rotational band based on the πg9/21νh11/2 configuration has been extended up to the (15) state. The configuration-fixed constrained triaxial relativistic mean-field approaches and the particle rotor model are employed to discuss the high-spin isomers and strongly coupled rotational band, respectively.

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  • Received 25 November 2013
  • Revised 1 April 2014

DOI:https://doi.org/10.1103/PhysRevC.90.014313

©2014 American Physical Society

Erratum

Erratum: Single-particle structures, high-spin isomers, and a strongly coupled band in odd-odd Sb120 [Phys. Rev. C 90, 014313 (2014)]

L. Liu (刘雷), S. Y. Wang (王守宇), Z. Q. Chen (陈志强), C. Liu (刘晨), B. Qi (亓斌), D. P. Sun (孙大鹏), S. Wang (王硕), Q. An (安强), C. J. Xu (徐长江), P. Zhang (张盼), Z. Q. Li (李志泉), C. Y. Niu (牛晨阳), 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), S. H. Yao (姚顺和), S. P. Hu (胡世鹏), H. W. Li (李红伟), J. J. Liu (刘嘉健), and J. L. Wang (汪金龙)
Phys. Rev. C 108, 059901 (2023)

Authors & Affiliations

L. Liu (刘雷)1, S. Y. Wang (王守宇)1,*, Z. Q. Chen (陈志强)1, C. Liu (刘晨)1, B. Qi (亓斌)1, D. P. Sun (孙大鹏)1, S. Wang (王硕)1, Q. An (安强)1, C. J. Xu (徐长江)1, P. Zhang (张盼)1, Z. Q. Li (李志泉)1, C. Y. Niu (牛晨阳)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, S. H. Yao (姚顺和)2, S. P. Hu (胡世鹏)2, H. W. Li (李红伟)2, J. J. Liu (刘嘉健)2, and J. L. Wang (汪金龙)2

  • 1Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Shandong University, Weihai 264209, People's Republic of China
  • 2China Institute of Atomic Energy, Beijing 102413, People's Republic of China

  • *sywang@sdu.edu.cn

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Vol. 90, Iss. 1 — July 2014

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