Triaxial bands in {sup {bold 133}}Ce

Journal Article · Thu Aug 01 00:00:00 EDT 1996 · Physical Review, C

DOI:https://doi.org/10.1103/PhysRevC.54.613· OSTI ID:286803

Hauschild, K; Wadsworth, R; Clark, R M; Hibbert, I M ^[1]; Fallon, P; Macchiavelli, A O ^[2]; Fossan, D B; Schnare, H; Thorslund, I ^[3]; Nolan, P J; Semple, A T; Walker, L ^[4]

---

1. Department of Physics, University of York, Heslington, York, Y01 5DD (United Kingdom)
2. Nuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720 (United States)
3. Department of Physics, State University of New York, Stony Brook, New York 11794 (United States)
4. Oliver Lodge Laboratory, University of Liverpool, Liverpool, L69 3BX (United Kingdom)

An experiment performed on the early implementation of the GAMMASPHERE array to populate the high-spin states in {sup 133}Ce has revealed the presence of several rotational structures with energy spacings of {Delta}{ital E}{sub {gamma}}{approximately}100 keV. Some of these bands exhibit a backbend at {h_bar}{omega}{approximately}0.6 MeV and are observed to high rotational frequencies{emdash}{h_bar}{omega}{approximately}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. {copyright} {ital 1996 The American Physical Society.}

• OSTI ID: 286803
• Journal Information: Physical Review, C, Vol. 54, Issue 2; Other Information: PBD: Aug 1996
• Country of Publication: United States
• Language: English

Related Subjects

66 PHYSICS
CERIUM 133
ROTATIONAL STATES
HIGH SPIN STATES
MASS
CRANKING MODEL
WOODS-SAXON POTENTIAL
STRUTINSKY THEORY
SHAPE