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Phys. Rev. C 69, 034339 (2004) [20 pages]

High-spin spectroscopy and quasiparticle alignments in 124,125Ce

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J. F. Smith1,*, V. Medina-Chico1,†, C. J. Chiara2,3, M. P. Carpenter4, C. N. Davids4, M. Devlin3,5, J. L. Durell1, D. B. Fossan2, S. J. Freeman1, R. V. F. Janssens4, D. R. LaFosse2, M. J. Leddy1,‡, P. Reiter4, D. G. Sarantites3, D. Seweryniak4, K. Starosta2, R. Wadsworth6, A. N. Wilson6,§, and J. N. Wilson3,**
1Schuster Laboratory, University of Manchester, Manchester M13 9PL, United Kingdom
2Department of Physics and Astronomy, State University of New York at Stony Brook, Stony Brook, New York 11794-3800, USA
3Department of Chemistry, Washington University, St. Louis, Missouri 63130, USA
4Argonne National Laboratory, Argonne, Illinois 60439, USA
5LANSCE-3, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
6Department of Physics, University of York, Heslington, York YO10 5DD, United Kingdom

Received 26 July 2003; published 31 March 2004

Rotational bands have been studied to high spins in the neutron-deficient 124,125Ce nuclei. The nuclei were populated using the 64Zn(64Zn,2p2n)124Ce and 64Zn(64Zn,2pn)125Ce reactions, with a beam energy of 260 MeV. High-fold γ-ray coincidence data were collected using the Gammasphere germanium-detector array. The Microball charged-particle detector array was used to provide channel selection. The previously established level structures of both 124,125Ce have been extended to high spins (∼30). In addition, several new bands have been identified. The alignments of pairs of h11∕2 neutrons and protons are observed in both nuclei. The alignments are compared to the predictions of Woods-Saxon cranked shell model calculations and to the systematics of h11∕2 quasiparticle alignments in neighboring nuclei. The apparent ability of the cranked shell model to explain the h11∕2 neutron alignments in 124,125Ce highlights the previously reported discrepancies between experiment and theory for the 128Ce isotope and, to a lesser extent, 126Ce.

© 2004 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.69.034339
DOI:
10.1103/PhysRevC.69.034339
PACS:
21.10.Re, 23.20.Lv, 27.60.+j, 29.30.Kv

*Electronic address: john.f.smith@man.ac.uk

Present address: Universidad Autónoma de Madrid, Spain.

Present address: NNC Ltd., Chelford Road, Knutsford, Cheshire WA16 8QZ, UK.

§Present address: Australian National University, Canberra ACT 0200, Australia.

**Present address: The Niels Bohr Institute, University of Copenhagen, 4000 Roskilde, Denmark.