Shell-Structure and Pairing Interaction in Superheavy Nuclei: Rotational Properties of the Z=104 Nucleus 256Rf
Abstract
The rotational band structure of the Z ¼ 104 nucleus 256Rf has been observed up to a tentative spin of
20@ using state-of-the-art -ray spectroscopic techniques. This represents the first such measurement in a
superheavy nucleus whose stability is entirely derived from the shell-correction energy. The observed
rotational properties are compared to those of neighboring nuclei and it is shown that the kinematic and
dynamic moments of inertia are sensitive to the underlying single-particle shell structure and the specific
location of high-j orbitals. The moments of inertia therefore provide a sensitive test of shell structure and
pairing in superheavy nuclei which is essential to ensure the validity of contemporary nuclear models in
this mass region. The data obtained show that there is no deformed shell gap at Z ¼ 104, which is
predicted in a number of current self-consistent mean-field models.
Main Authors
Format
Articles
Research article
Published
2012
Series
Subjects
Publication in research information system
Publisher
American Physical Society
The permanent address of the publication
https://urn.fi/URN:NBN:fi:jyu-201602051456Use this for linking
Review status
Peer reviewed
ISSN
0031-9007
DOI
https://doi.org/10.1103/PhysRevLett.109.012501
Language
English
Published in
Physical Review Letters
Citation
- Greenlees, P., Rubert, J., Piot, J., Gall, B., Andersson, L.L., Asai, M., Asfari, Z., Cox, D.M., Dechery, F., Dorvaux, O., Grahn, T., Hauschild, K., Henning, G., Herzan, A., Herzberg, R.-D., Hessberger, F. P., Jakobsson, U., Jones, P., Julin, R., . . . Venhart, M. (2012). Shell-Structure and Pairing Interaction in Superheavy Nuclei: Rotational Properties of the Z=104 Nucleus 256Rf. Physical Review Letters, 109(1), 012501. https://doi.org/10.1103/PhysRevLett.109.012501
Copyright© 2012 the Authors. Published by the American Physical Society under the terms of the Creative Commons Attribution 3.0 License.