Prolate-oblate band mixing and new bands in <span class="aps-inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mmultiscripts><mrow><mi mathvariant="normal">Hg</mi></mrow><mprescripts></mprescripts><mrow></mrow><mrow><mn>182</mn></mrow><mrow></mrow><mrow></mrow></mmultiscripts></mrow></math></span>

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; D. Winchell

doi:10.1103/PhysRevC.51.401

Prolate-oblate band mixing and new bands in ${}^{182}{Hg}$

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

Phys. Rev. C 51, 401 – Published 1 January 1995

Abstract

In-beam γ-ray spectroscopic studies of ${}^{182}{Hg}$ 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 ${}^{184}{Hg}$ . 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.

Received 18 May 1994

DOI:https://doi.org/10.1103/PhysRevC.51.401

Authors & Affiliations

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

Physics Department, Vanderbilt University, Nashville, Tennessee 37235
Physics Division, Argonne National Laboratory, Argonne, Illinois 60439
Chemistry Department, Washington University, St. Louis, Missouri 63130
Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831
UNISOR, Oak Ridge, Tennessee 37831

Comments & Replies

Reply to ‘‘Comment on ‘Prolate-oblate band mixing and new bands in ${}^{182}’$

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

Phys. Rev. C 53, 3165 (1996)

Comment on ‘‘Prolate-oblate band mixing and new bands in ${}^{182}’$

J. Wauters, N. Bijnens, M. Huyse, and P. Van Duppen

Phys. Rev. C 53, 3163 (1996)

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Vol. 51, Iss. 1 — January 1995

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