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The structure of the negative parity bands, based on the νh11/2 orbital, in ¹²⁹Ba is revisited to search for the wobbling mode in this nucleus. Existing angular distribution/correlation and linear polarization results are indicative of a large $E2$ admixture in the 365 keV interconnecting ΔI=1 γ transition between yrast bands. This provides an indication of the existence of a wobbling mode in this nucleus. Theoretical calculations performed in this work using the quasiparticle plus triaxial rotor model have effectively replicated the available experimental results.
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Chakraborty et al. (2024) studied this question.
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