Reply to {open_quote}{open_quote}Comment on {open_quote}Prolate-oblate band mixing and new bands in {sup 182}Hg{close_quote}{close_quote}{close_quote}

Journal Article · Sat Jun 01 04:00:00 EDT 1996 · Physical Review, C

DOI:https://doi.org/10.1103/PhysRevC.53.3165· OSTI ID:284804

Bindra, K S; Hua, P F; Babu, B R; 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 ^[1]

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1. Physics Department, Vanderbilt University, Nashville, Tennessee 37235 (United States)

We reply to the preceding Comment. {copyright} {ital 1996 The American Physical Society.}

• Research Organization: Oak Ridge National Laboratory
• DOE Contract Number: AC05-84OR21400
• OSTI ID: 284804
• Journal Information: Physical Review, C, Journal Name: Physical Review, C Journal Issue: 6 Vol. 53; ISSN 0556-2813; ISSN PRVCAN
• Country of Publication: United States
• Language: English

Related Subjects

44 INSTRUMENTATION
INCLUDING NUCLEAR AND PARTICLE DETECTORS
66 PHYSICS
BAND STRUCTURE
BAND THEORY
ENERGY
GROUND STATES
HIGH SPIN STATES
MERCURY 182
MIXING
PLATINUM 180
YRAST STATES