Observation of new levels and proposed octupole correlations in neutron-rich 150Ce

S. J. Zhu (朱胜江), M. Sakhaee, J. H. Hamilton, A. V. Ramayya, N. T. Brewer, J. K. Hwang, S. H. Liu, E. Y. Yeoh (杨韵颐), Z. G. Xiao (肖志刚), Q. Xu (徐强), Z. Zhang (张钊), Y. X. Luo, J. O. Rasmussen, I. Y. Lee, K. Li, and W. C. Ma
Phys. Rev. C 85, 014330 – Published 30 January 2012

Abstract

Background: The very neutron-rich 150Ce is located at the edge of the Z=56, N=88 octupole deformed island. Studying its high spin states and octupole correlations is important for systematically understanding the nuclear structural characteristics in this region. Purpose: To investigate the high spin state levels and to search for octopole correlations in 150Ce. Methods: The high spin states of 150Ce are studied by measuring the prompt γ rays in the spontaneous fission of 252Cf. The data analysis uses the γ-γ-γ coincidence methods. The γγ(θ) angular correlation measurements are used to determine the spin and indirectly determine the parity of particular levels. Results: A new level scheme of 150Ce is established. A total of 47 new transitions and 25 new levels are identified, compared with previous results. Six collective bands have been observed, and five of them are newly established. An octupole band structure with s=+1 in 150Ce has been proposed. Systematic analysis of the B(E1)/B(E2) branching ratios, the levels of the octupole bands, the energy differences between negative- and positive-parity bands, and the moments of inertia of the bands is carried out for 144,146,148,150Ce. This analysis gives evidence for our assignment of octupole correlations in 150Ce. The other characteristics of the octupole bands are discussed. Conclusions: An octupole band structure is proposed in 150Ce. The octupole correlations in 150Ce are weaker and show more instability than the neighboring lighter Ce isotopes.

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  • Received 12 December 2011

DOI:https://doi.org/10.1103/PhysRevC.85.014330

©2012 American Physical Society

Authors & Affiliations

S. J. Zhu (朱胜江)1,2,*, M. Sakhaee1, J. H. Hamilton2, A. V. Ramayya2, N. T. Brewer2, J. K. Hwang2, S. H. Liu2,3, E. Y. Yeoh (杨韵颐)1, Z. G. Xiao (肖志刚)1, Q. Xu (徐强)1, Z. Zhang (张钊)1, Y. X. Luo2,4, J. O. Rasmussen4, I. Y. Lee4, K. Li2, and W. C. Ma5

  • 1Department of Physics, Tsinghua University, Beijing 100084, People's Republic of China
  • 2Department of Physics, Vanderbilt University, Nashville, Tennessee 37235, USA
  • 3UNIRIB/Oak Ridge Associated Universities, Oak Ridge, Tennessee 37831, USA
  • 4Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
  • 5Department of Physics and Astronomy, Mississippi State University, Mississippi State, Mississippi 39762, USA

  • *zhushj@mail.tsinghua.edu.cn

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Vol. 85, Iss. 1 — January 2012

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