Collective and quasiparticle excitations in superformed Hg-190

Superdeformed (SD) states of {sup 190}Hg have been studied with the Eurogam Phase 2 {gamma}-ray spectrometer using the {sup 160}Gd({sup 34}S,4n) reaction. Two new excited SD bands have been found and identified as belonging to this nucleus, bringing the total number of SD bands in {sup 190}Hg to 4....

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Veröffentlicht in:Physical review. C, Nuclear physics Nuclear physics, 1996-08, Vol.54 (2 ; Aug. 1996)
Hauptverfasser: Wilson, A. N., Timar, J., Sharpey-Schafer, J. F., Crowell, B., Carpenter, M. P., Janssens, R. V. F., Blumenthal, D. J., Ahmad, I., Astier, A., Azaiez, F., Bergstrom, M., Ducroux, L., Gall, B. J. P., Hannachi, F., Khoo, T. L., Korichi, A., Lauritsen, T., Lopez-Martens, A., Meyer, M., Nisius, D., Paul, E. S., Porquet, M. G., Redon, N., Wilson, J. N., Nakatsukasa, T., Physics, Univ. of Liverpool, Centre de Recherches Nucleaires, Inst. de Physique Nucleaire Lyon, I.P.N., Inst. of Physique Nucleaire Lyon, C.S.N.S.M., AECL
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Sprache:eng
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Zusammenfassung:Superdeformed (SD) states of {sup 190}Hg have been studied with the Eurogam Phase 2 {gamma}-ray spectrometer using the {sup 160}Gd({sup 34}S,4n) reaction. Two new excited SD bands have been found and identified as belonging to this nucleus, bringing the total number of SD bands in {sup 190}Hg to 4. One of the new bands has a dynamic moment of inertia that is very similar to that of the yrast SD band of {sup 190}Hg and most other SD bands in the A{approx}190 region. In contrast, the other band has a dynamic moment of inertia which is mainly constant as a function of rotational frequency and exhibits a dramatic increase at the lowest frequencies. The observed dynamic moments of inertia are compared with the results of random phase approximation calculations based on the cranked shell model. Finally, the known excited SD band has been extended towards lower frequencies and new transitions have been found linking this band to the yrast SD band. The extracted B(E1) values of the new linking transitions give further support for the possible octupole vibrational character of this band.
ISSN:0556-2813
1089-490X
DOI:10.1103/PhysRevC.54.559