Phys. Rev. C 51, 401 - 404 (1995)Prolate-oblate band mixing and new bands in 182Hg
K. S. Bindra, P. F. Hua, B. R. S. 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 Received 18 May 1994 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 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) [ Abstract | Previous article | Next article | Issue 1 ] |
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