Signature inversion in odd-odd nuclei

L. L. Rledinger, D. J. Hartley, A. Galindo-Uribarri, B. H. Smith, C. Baktash, M. P. Carpenter, M. Danchev, M. Devlin, C. J. Gross, R. V.F. Janssens, M. Lipoglavsek, S. D. Paul, P. C. Radford, W. Reviol, D. G. Sarantites, D. Seweryniak, C. H. Yu, O. Zeidan

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19 Scopus citations

Abstract

Trends in the energy staggering of the πh11/2νi13/2 and πh11/2νh11/2 bands in the mass 160 and 130 regions, respectively, have been investigated in order to better understand the origin of signature inversion. While the A ≈ 160 nuclei behave in a consistent manner, a more complicated'scenario is observed in the mass 130 region. As a result of our experiments on the lightest Pr nuclei, the systematics of these Z = 59 nuclei have been extended, which aids in the understanding of the latter region. Triaxial deformation, a pn interaction, and quadrupole pairing are considered as possible contributors to this effect. As all the chiral-twin bands that are known have signature inversion in the favored band, a possible link between the two phenomena should be considered.

Original languageEnglish
Pages (from-to)2613-2623
Number of pages11
JournalActa Physica Polonica B
Volume32
Issue number9
StatePublished - 2001
EventInternational Research Conference- Nato Advanced Research Workshop-HIGH SPIN PHYSICS 2001 - Warsaw, Poland
Duration: Feb 6 2001Feb 10 2001

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