Evidence for Hyperdeformation in G147d

D. R. LaFosse, D. G. Sarantites, C. Baktash, P.-F. Hua, B. Cederwall, P. Fallon, C. J. Gross, H.-Q. Jin, M. Korolija, I. Y. Lee, A. O. Macchiavelli, M. R. Maier, W. Rathbun, D. W. Stracener, and T. R. Werner
Phys. Rev. Lett. 74, 5186 – Published 26 June 1995
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Abstract

A pair of rotational bands with 9 and 11 discrete γ rays with a regular spacing of about 29 keV extending from 1016 to 1340 keV have been identified as belonging to 147Gd. Evidence from their population, decay characteristics, very large dynamic moments of inertia of (2)=140 ħ2MeV1, and agreement with theoretical predictions support the hyperdeformed character of these bands. These band structures correspond to a spheroid with major-to-minor axis ratio of about 3:1.

  • Received 31 March 1995

DOI:https://doi.org/10.1103/PhysRevLett.74.5186

©1995 American Physical Society

Authors & Affiliations

D. R. LaFosse1, D. G. Sarantites1, C. Baktash2, P.-F. Hua3, B. Cederwall4, P. Fallon4, C. J. Gross5, H.-Q. Jin2, M. Korolija1, I. Y. Lee4, A. O. Macchiavelli4, M. R. Maier4, W. Rathbun4, D. W. Stracener2, and T. R. Werner2,6,7

  • 1Chemistry Department, Washington University, St. Louis, Missouri 63130
  • 2Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee, 37831
  • 3Physics Department, Washington University, St. Louis, Missouri 63130
  • 4Nuclear Science Division, Lawrence Berkeley Laboratory, Berkeley, California 94720
  • 5UNISOR, Oak Ridge Institute of Science and Education, Oak Ridge, Tennessee 37831
  • 6Department of Physics and Astronomy, University of Tennessee, Knoxville Tennessee 37996
  • 7Institute of Theoretical Physics, Warsaw University, PL-00-681, Warsaw, Poland

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Vol. 74, Iss. 26 — 26 June 1995

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