Possible wobbling phenomenon in Xe 125

dc.contributor.author	Prajapati M.; Nag S.; Singh A.K.; Al-Khatib A.; Hübel H.; Neußer-Neffgen A.; Hagemann G.B.; Sletten G.; Herskind B.; Hansen C.R.; Benzoni G.; Bracco A.; Janssens R.V.F.; Carpenter M.P.; Chowdhury P.
dc.date.accessioned	2025-05-23T11:12:44Z
dc.description.abstract	In the present paper, negative-parity bands based on the νh11/2 configuration in Xe125 have been revisited. This nucleus was populated through the reaction Se82(Ca48,5n)Xe125 at a beam energy of 205 MeV and the corresponding γ rays were observed using the Gammasphere spectrometer. Evidence for first and second phonon wobbling excitations has been established by measurements of directional correlation ratios and angular distributions of the involved γ rays. The observed wobbling energy of the bands involved were compared with the recently published results obtained within the framework of triaxial projected shell-model calculations. © 2024 American Physical Society.
dc.identifier.doi	https://doi.org/10.1103/PhysRevC.109.034301
dc.identifier.uri	http://172.23.0.11:4000/handle/123456789/5022
dc.relation.ispartofseries	Physical Review C
dc.title	Possible wobbling phenomenon in Xe 125

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