Near-yrast structure of N=93 neutron-rich lanthanide nuclei

G. S. Simpson, W. Urban, J. A. Pinston, J. C. Angelique, I. Deloncle, H. R. Faust, J. Genevey, U. Köster, T. Materna, R. Orlandi, A. Scherillo, A. G. Smith, J. F. Smith, T. Rząca-Urban, I. Ahmad, and J. P. Greene
Phys. Rev. C 81, 024313 – Published 16 February 2010

Abstract

Two neutron-rich N=93 isotones, Sm155 and Nd153, have been studied by delayed γ-ray and conversion-electron spectroscopy at the Lohengrin mass spectrometer. A half-life of 2.9(5) μs has been measured for the ν5/2+[642] state at 16.5 keV in Sm155. The decay of a 1.17(7)-μs isomer in Nd153, at 191.7 keV, has been remeasured and its spin has been reassigned as (5/2)+. This state contains a strong component of the ν5/2+[642] Nilsson orbital. In addition, a new 1.00(8)-μs isomeric state at 538.6 keV, with a probable ν11/2[505] Nilsson configuration, has been observed in Sm155. Triple γ-ray coincidence data from the spontaneous fission of a Cf252 source placed inside the Gammasphere array were used to extend the collective band on top of the (5/2+) isomeric state of Nd153, and a new band with the same bandhead spin has been observed in Ce151. The observation of this new band and an additional new transition in the ground-state band has led us to change the ground-state spin of Ce151 to (3/2). Calculations using the quasiparticle-rotor model successfully reproduce the majority of the features of the γ decays of these nuclei, including branching ratios and isomeric half-lives. Because this model uses a reflection-symmetric core, we conclude that the polarizing effect of the odd particle is responsible for the dipole moment present in the ν5/2+[642] states of the three nuclei studied and the ν11/2[505] level of Sm155.

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  • Received 18 November 2009

DOI:https://doi.org/10.1103/PhysRevC.81.024313

©2010 American Physical Society

Authors & Affiliations

G. S. Simpson1,*, W. Urban2,3, J. A. Pinston1, J. C. Angelique1, I. Deloncle4, H. R. Faust3, J. Genevey1, U. Köster3, T. Materna3, R. Orlandi5, A. Scherillo6, A. G. Smith7, J. F. Smith7, T. Rząca-Urban2, I. Ahmad8, and J. P. Greene8

  • 1LPSC, Université Joseph Fourier Grenoble 1, CNRS/IN2P3, Institut National Polytechnique de Grenoble, F-38026 Grenoble Cedex, France
  • 2Faculty of Physics, University of Warsaw, ul.Hoża 69, PL-00-681 Warsaw, Poland
  • 3Institut Laue-Langevin, B.P. 156, F-38042 Grenoble Cedex 9, France
  • 4CSNSM, Université Paris-XI, CNRS/IN2P3, F-91405 Orsay Cedex, France
  • 5INFN, Laboratori Nazionali di Legnaro, I-35020 Legnaro, Italy
  • 6Rutherford Appleton Laboratory, Chilton, Didcot OX11 0QX, United Kingdom
  • 7Department of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, United Kingdom
  • 8Argonne National Laboratory, Argonne, Illinois 60439, USA

  • *simpson@lpsc.in2p3.fr

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Vol. 81, Iss. 2 — February 2010

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