Quantised orbital alignment and Identical High-K Bands in A=180 region

dc.creatorRath, Aswini Kumar
dc.creatorNaik, Z
dc.creatorPraharaj, C R
dc.date2006-12-13
dc.date.accessioned2026-07-07T06:43:19Z
dc.date.available2026-07-07T06:43:19Z
dc.descriptionThe origin of the identical gamma-ray energies (IB) observed in the K=33/2$^+$ and K=16$^+$ bands in $^{177}$Lu and $^{178}$Hf respectively is investigated using deformed Hartree-Fock and Angular Momentum Projection technique. We find that quantised orbital (rather than spin) alignment of protons in the m=1/2$^+$ inert orbit leads to identical energy spectra. A K=16$^+$ band with identical spectrum is predicted in $^{176}$Yb at 4.48 Mev of excitation.
dc.description4 pages 4 figures 1 table
dc.identifierhttps://arxiv.org/abs/nucl-th/0612060
dc.identifierhttp://arxiv.org/abs/nucl-th/0612060
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/102371
dc.subjectNuclear Theory
dc.titleQuantised orbital alignment and Identical High-K Bands in A=180 region
dc.typetext

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