High-spin spectroscopy of Ce139

S. Kaim, C. M. Petrache, A. Gargano, N. Itaco, T. Zerrouki, R. Leguillon, A. Astier, I. Deloncle, T. Konstantinopoulos, J. M. Régis, D. Wilmsen, B. Melon, A. Nannini, C. Ducoin, D. Guinet, and T. Bhattacharjee
Phys. Rev. C 91, 024318 – Published 20 February 2015

Abstract

High-spin states in Ce139 have been populated using the Te130(C14,5n) reaction. The level scheme has been extended to higher spins, including a new band of dipole transitions. The parity of several states has been changed from negative to positive, mainly based on the comparison with the level structure of the core nucleus Ce140 and the results of a realistic shell-model calculation. The dipole band is interpreted as a magnetic rotation band with πh11/22νh11/21 configuration built on small deformation axial shape with (ɛ2=0.12,γ=0).

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  • Received 21 October 2014
  • Revised 28 January 2015

DOI:https://doi.org/10.1103/PhysRevC.91.024318

©2015 American Physical Society

Authors & Affiliations

S. Kaim1,2, C. M. Petrache1, A. Gargano3, N. Itaco3, T. Zerrouki1, R. Leguillon1,*, A. Astier1, I. Deloncle1, T. Konstantinopoulos1, J. M. Régis4, D. Wilmsen4, B. Melon5, A. Nannini5, C. Ducoin6, D. Guinet6, and T. Bhattacharjee7

  • 1Centre de Sciences Nucléaires et de Sciences de la Matière, Université Paris-Sud and CNRS/IN2P3, 91405 Orsay, France
  • 2Université de Mentouri Constantine, 25017 Constantine, Algeria
  • 3Dipartimento di Scienze Fisiche, Universitá di Napoli Federico II, and Istituto Nazionale di Fisica Nucleare, Complesso Universitario di Monte S. Angelo, Via Cintia, I-80126 Napoli, Italy
  • 4Institut für Kernphysik der Universität zu Köln, 50937 Köln, Germany
  • 5Department of Physics and INFN Sezione di Firenze, Firenze, Italy
  • 6IPNL CNRS/IN2P3 and Université Lyon 1, 69622 Villeurbanne, France
  • 7Variable Energy Cyclotron Centre, Kolkata 700064, India

  • *Present address: Advanced Science Research Center, Japan Atomic Energy Agency, 2-4 Shirakata Shirane, Tokai, Ibaraki 319-1195 Japan.

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Vol. 91, Iss. 2 — February 2015

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