Rotational alignments in Np235 and the possible role of j15/2 neutrons

A. M. Hurst, C. Y. Wu, M. A. Stoyer, D. Cline, A. B. Hayes, S. Zhu, M. P. Carpenter, K. Abu Saleem, I. Ahmad, J. A. Becker, C. J. Chiara, J. P. Greene, R. V. F. Janssens, T. L. Khoo, F. G. Kondev, T. Lauritsen, C. J. Lister, G. Mukherjee, S. V. Rigby, D. Seweryniak, and I. Stefanescu
Phys. Rev. C 81, 014312 – Published 22 January 2010

Abstract

The role j15/2 neutron orbitals play in the transuranic region of actinides has been studied by exploring γ-ray transitions between yrast states in Np235, populated utilizing the nucleon-transfer reaction Np237(Sn116,Sn118). Two rotational sequences, presumably the two signatures of the ground-state band, have been delineated to high spin for the first time, with the α=+1/2 and α=1/2 signature partners reaching 49/2+ (tentatively 53/2+) and 47/2+ (tentatively 51/2+), respectively. Definite isotopic assignments for these in-band transitions were established through γ-ray cross correlations between Np235 and Sn118 and events where at least three γ rays corresponding to neptunium-like particles were detected. These transitions reveal clear upbends in the aligned angular momentum and kinematic moment of inertia plots; such a phenomenon could indicate a strong interaction between an aligned νj15/2 configuration crossing the ground-state band in Np235, which is based on a πi13/2 orbital. However, the lack of any signature splitting over the observed frequency range of the Np235 rotational sequences cannot remove the possibility of a πh9/2 assignment for the observed band. The role of the νj15/2 and πi13/2 alignment mechanisms in the deformed U-Pu region is discussed in light of the current spectroscopic data and in the context of the cranked-shell model.

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  • Received 9 September 2009

DOI:https://doi.org/10.1103/PhysRevC.81.014312

©2010 American Physical Society

Authors & Affiliations

A. M. Hurst1,*, C. Y. Wu1, M. A. Stoyer1, D. Cline2, A. B. Hayes2, S. Zhu3, M. P. Carpenter3, K. Abu Saleem4, I. Ahmad3, J. A. Becker1, C. J. Chiara3,5,6, J. P. Greene3, R. V. F. Janssens3, T. L. Khoo3, F. G. Kondev3,5, T. Lauritsen3, C. J. Lister3, G. Mukherjee7, S. V. Rigby8, D. Seweryniak3, and I. Stefanescu3,6

  • 1Lawrence Livermore National Laboratory, Livermore, California 94550, USA
  • 2Department of Physics and Astronomy, University of Rochester, Rochester, New York 14627, USA
  • 3Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
  • 4Department of Physics, University of Jordan, Amman 11942, Jordan
  • 5Nuclear Engineering Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
  • 6Department of Chemistry and Biochemistry, University of Maryland, College Park, Maryland 20742, USA
  • 7Variable Energy Cyclotron Centre, 1/AF Bidhan Nagar, Kolkata-700 064, India
  • 8Oliver Lodge Laboratory, University of Liverpool, Liverpool L69 7ZE, United Kingdom

  • *hurst10@llnl.gov

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Vol. 81, Iss. 1 — January 2010

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