Triaxial bands in Ce133

K. Hauschild, R. Wadsworth, R. M. Clark, I. M. Hibbert, P. Fallon, A. O. Macchiavelli, D. B. Fossan, H. Schnare, I. Thorslund, P. J. Nolan, A. T. Semple, and L. Walker
Phys. Rev. C 54, 613 – Published 1 August 1996
PDFExport Citation

Abstract

An experiment performed on the early implementation of the GAMMASPHERE array to populate the high-spin states in Ce133 has revealed the presence of several rotational structures with energy spacings of ΔEγ∼100 keV. Some of these bands exhibit a backbend at ħω∼0.6 MeV and are observed to high rotational frequencies—ħω∼0.85 MeV. These characteristics are very different from those observed for any other rotational bands in this mass region. The properties of these new structures will be discussed within the framework of cranked Strutinsky-Woods-Saxon calculations. Currently, these bands are thought to be based on triaxial nuclear shapes. © 1996 The American Physical Society.

  • Received 25 January 1996

DOI:https://doi.org/10.1103/PhysRevC.54.613

©1996 American Physical Society

Authors & Affiliations

K. Hauschild, R. Wadsworth, R. M. Clark, and I. M. Hibbert

  • Department of Physics, University of York, Heslington, York, Y01 5DD, United Kingdom

P. Fallon and A. O. Macchiavelli

  • Nuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720

D. B. Fossan, H. Schnare, and I. Thorslund

  • Department of Physics, State University of New York, Stony Brook, New York 11794

P. J. Nolan, A. T. Semple, and L. Walker

  • Oliver Lodge Laboratory, University of Liverpool, Liverpool, L69 3BX, United Kingdom

References (Subscription Required)

Click to Expand
Issue

Vol. 54, Iss. 2 — August 1996

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review C

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×