Identification of multi-phonon γ-vibrational bands in odd-Z 105Nb

H. J. Li (李红洁), S. J. Zhu (朱胜江), J. H. Hamilton, A. V. Ramayya, J. K. Hwang, Y. X. Liu (刘艳鑫), Y. Sun (孙扬), Z. G. Xiao (肖志刚), E. H. Wang, J. M. Eldridge, Z. Zhang (张钊), Y. X. Luo, J. O. Rasmussen, I. Y. Lee, G. M. Ter-Akopian, A. V. Daniel, Yu. Ts. Oganessian, and W. C. Ma
Phys. Rev. C 88, 054311 – Published 13 November 2013

Abstract

Background: The odd-Z 105Nb nucleus is located in the A=100 neutron-rich region. The study of multi-phonon vibrational band structures is important for understanding nuclear structure in this region.

Purpose: To search for multi-phonon γ-vibrational bands in 105Nb.

Methods: The high spin states of 105Nb have been studied by measuring the prompt γ rays emitted in the spontaneous fission of 252Cf. The data analysis is carried out using triple- and four-fold γ coincidence methods.

Results: A new level scheme of 105Nb is established. The yrast band has been confirmed, and three new collective bands have been identified. Compared with previous results, a total of 14 new levels and 36 new γ transitions are observed. Two bands built on 625.9 keV and 1231.9 keV levels are proposed as one-phonon- and two-phonon γ-vibrational bands, respectively. The evidences for supporting assignments of the multi-phonon γ-vibrational bands have been discussed. Triaxial projected shell model calculations for the γ-vibrational band structures are found in good agreement with the experimental data, thus further supporting the γ-vibrational interpretations for the experimental results in 105Nb.

Conclusions: The one-phonon- and two-phonon γ-vibrational bands have been identified in 105Nb. Our results provide new data to systematically understand the characteristics of the multi-phonon γ-vibrational bands in the A=100 neutron-rich region.

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  • Received 27 June 2013

DOI:https://doi.org/10.1103/PhysRevC.88.054311

©2013 American Physical Society

Authors & Affiliations

H. J. Li (李红洁)1, S. J. Zhu (朱胜江)1,2,*, J. H. Hamilton2, A. V. Ramayya2, J. K. Hwang2, Y. X. Liu (刘艳鑫)3, Y. Sun (孙扬)4, Z. G. Xiao (肖志刚)1, E. H. Wang2, J. M. Eldridge2, Z. Zhang (张钊)1, Y. X. Luo2,5, J. O. Rasmussen5, I. Y. Lee5, G. M. Ter-Akopian6, A. V. Daniel6, Yu. Ts. Oganessian6, and W. C. Ma7

  • 1Department of Physics, Tsinghua University, Beijing 100084, People's Republic of China
  • 2Department of Physics, Vanderbilt University, Nashville, Tennessee 37235, USA
  • 3School of Science, Huzhou Teachers College, Huzhou 313000, People's Republic of China
  • 4Department of Physics, Shanghai Jiao Tong University, Shanghai 200240, People's Republic of China
  • 5Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
  • 6Flerov Laboratory for Nuclear Reactions, JINR, 141980 Dubna, Russia
  • 7Department of Physics and Astronomy, Mississippi State University, Mississippi State, Mississippi 39762, USA

  • *zhushj@mail.tsinghua.edu.cn

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Vol. 88, Iss. 5 — November 2013

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