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Prolate-oblate band mixing and new bands in [sup 182]Hg

In-beam [gamma]-ray spectroscopic studies of [sup 182]Hg have revealed five new bands. The 2[sup +] state of the prolate band has been identified at an energy of 548.6 keV and is higher than in [sup 184]Hg. A two parameter band mixing calculation results in an interaction energy of 83 keV between th...

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Bibliographic Details
Published in:Physical review. C, Nuclear physics Nuclear physics, 1995-01, Vol.51:1
Main Authors: Bindra, K.S., Hua, P.F., Babu, B.R.S., Baktash, C., Barreto, J., Cullen, D.M., Davids, C.N., Deng, J.K., Garrett, J.D., Halbert, M.L., Hamilton, J.H., Johnson, N.R., Kirov, A., Kormicki, J., Lee, I.Y., Ma, W.C., McGowan, F.K., Ramayya, A.V., Sarantites, D.G., Soramel, F., Winchell, D.
Format: Article
Language:English
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Summary:In-beam [gamma]-ray spectroscopic studies of [sup 182]Hg have revealed five new bands. The 2[sup +] state of the prolate band has been identified at an energy of 548.6 keV and is higher than in [sup 184]Hg. A two parameter band mixing calculation results in an interaction energy of 83 keV between the prolate 2[sup +] and the oblate 2[sup +] states. Several additional new bands are seen including some which are interpreted as quadrupole vibrational bands built on the excited prolate minimum.
ISSN:0556-2813
1089-490X
DOI:10.1103/PhysRevC.51.401