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

Journal Article · · Physical Review, C (Nuclear Physics); (United States)
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  1. Physics Department, Vanderbilt University, Nashville, Tennessee 37235 (United States) Physics Division, Argonne National Laboratory, Argonne, Illinois 60439 (United States) Chemistry Department, Washington University, St. Louis, Missouri 63130 (United States) Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831 (United States) UNISOR, Oak Ridge, Tennessee 37831 (United States)

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.

DOE Contract Number:
FG05-88ER40407; FG02-88ER40406; AC05-84OR21400; W-31109-ENG-38
OSTI ID:
7062576
Journal Information:
Physical Review, C (Nuclear Physics); (United States), Journal Name: Physical Review, C (Nuclear Physics); (United States) Vol. 51:1; ISSN PRVCAN; ISSN 0556-2813
Country of Publication:
United States
Language:
English