Phys. Rev. C 51, 401–404 (1995)Prolate-oblate band mixing and new bands in 182HgReceived 18 May 1994; published in the issue dated January 1995 In-beam γ-ray spectroscopic studies of 182Hg have revealed five new bands. The 2+ state of the prolate band has been identified at an energy of 548.6 keV and is higher than in 184Hg. A two parameter band mixing calculation results in an interaction energy of 83 keV between the prolate 2+ and the oblate 2+ states. Several additional new bands are seen including some which are interpreted as quadrupole vibrational bands built on the excited prolate minimum. © 1995 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevC.51.401
DOI:
10.1103/PhysRevC.51.401
PACS:
27.70.+q, 29.30.Kv, 23.20.Lv
See AlsoComment: J. Wauters, N. Bijnens, M. Huyse, and P. Van Duppen, Comment on ‘‘Prolate-oblate band mixing and new bands in 182’, Phys. Rev. C 53, 3163 (1996). Reply: K. S. Bindra, P. F. Hua, B. R. Babu, C. Baktash, J. Barreto, D. M. Cullen, C. N. Davids, J. K. Deng, J. D. Garrett, M. L. Halbert, J. H. Hamilton, N. R. Johnson, A. Kirov, J. Kormicki, I. Y. Lee, W. C. Ma, F. K. McGowan, A. V. Ramayya, D. G. Sarantites, F. Soramel, and D. Winchell, Reply to ‘‘Comment on ‘Prolate-oblate band mixing and new bands in 182’, Phys. Rev. C 53, 3165 (1996). |
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