Near-yrast, medium-spin, excited states of Rb91, Rb93, and Rb95

G. S. Simpson, W. Urban, K. Sieja, J. A. Dare, J. Jolie, A. Linneman, R. Orlandi, A. Scherillo, A. G. Smith, T. Soldner, I. Tsekhanovich, B. J. Varley, A. Złomaniec, J. L. Durell, J. F. Smith, T. Rząca-Urban, H. Faust, I. Ahmad, and J. P. Greene
Phys. Rev. C 82, 024302 – Published 3 August 2010

Abstract

The medium-spin structure of the nuclei Rb93 and Rb95 is studied following the neutron-induced fission of U235 at the PF1B neutron guide, using the FIFI spectrometer, and at the Lohengrin mass spectrometer of the Institut Laue-Langevin Grenoble. These nuclei, plus Rb91, are also studied following the spontaneous fission of Cm248 and Cf252 sources, using the EUROGAM-II and Gammasphere detector arrays, respectively. A high-spin isomeric state, with a half-life of 111(11) ns, is found in Rb93 at an excitation energy of 4422.4 keV, which most likely corresponds to the fully aligned [π(g9/2)ν(g7/2h11/2)]27/2 configuration. An analogous configuration is proposed for the 5297.9-keV level observed in Rb91. A new E3 decay branch of the 1133.9-keV isomer in Rb91 is found, for which the rather low transition rate of B(E3)=3.8(10) W.u. is determined. The energy of the isomeric state of Rb95 is now proposed to be at 810.6 keV, with a spin of (9/2+), and its half-life determined to be T1/2=94(7) ns. A cascade of prompt transitions is observed on top of the 810.6-keV isomer in Rb95. The near-yrast structures of Rb91, Rb93, and Rb95 are compared to the results of shell-model calculations, which support the proposed 27/2 interpretation of states in Rb91 and Rb93. An analogous 27/2 state is expected to occur in Rb95, as a long-lived isomer at 3.24 MeV. No such isomeric decay could be observed in a measurement using the Lohengrin spectrometer, which shows that, if it exists, its population, following the fission of U235, is at least four times lower than that of the analogous 27/2 isomer in Y97.

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  • Received 2 April 2010

DOI:https://doi.org/10.1103/PhysRevC.82.024302

©2010 American Physical Society

Authors & Affiliations

G. S. Simpson1,*, W. Urban2,3, K. Sieja4, J. A. Dare5, J. Jolie6, A. Linneman6, R. Orlandi5, A. Scherillo7, A. G. Smith5, T. Soldner2, I. Tsekhanovich5, B. J. Varley5, A. Złomaniec3, J. L. Durell5, J. F. Smith5, T. Rząca-Urban3, H. Faust2, I. Ahmad8, and J. P. Greene8

  • 1LPSC, Université Joseph Fourier Grenoble 1, CNRS/IN2P3, Institut National Polytechnique de Grenoble, F-38026 Grenoble Cedex, France
  • 2Institut Laue-Langevin, 6 rue J. Horowitz, F-38042 Grenoble, France
  • 3Faculty of Physics, University of Warsaw, ul. Hoża 69, PL-00-681 Warsaw, Poland
  • 4Institute Pluridisciplinaire Hubert Curien, 23 rue du Loess, 67037 Strasbourg Cedex, France
  • 5Department of Physics and Astronomy, The University of Manchester, M13 9PL Manchester, United Kingdom
  • 6Institut für Kernphysik, Universität zu Köln, Zülpicherstr. 77, D-50937 Köln, Germany
  • 7Rutherford Appleton Laboratory, Chilton, Didcot OX11 0QX, United Kingdom
  • 8Argonne National Laboratory, Argonne, Illinois 60439, USA

  • *simpson@lpsc.in2p3.fr

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Vol. 82, Iss. 2 — August 2010

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