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dc.contributor.advisorGueorguieva, E. A.
dc.contributor.advisorLindsay, R.
dc.contributor.authorShirinda, Obed
dc.contributor.otherDept. of Physics
dc.contributor.otherFaculty of Science
dc.date.accessioned2013-12-03T12:31:26Z
dc.date.available2009/10/09 14:26
dc.date.available2009/10/09
dc.date.available2013-12-03T12:31:26Z
dc.date.issued2007
dc.identifier.urihttp://hdl.handle.net/11394/2492
dc.descriptionMagister Scientiae - MScen_US
dc.description.abstractThe nearly oblate deformed Au nuclei show rotational bands built on multi quasiparticle excitations [Bou89, Bou92, Gue03, Gue01, Ven92]. Several of these bands are built on rotationally aligned high-j proton and neutron excitations. In many cases bands consisting of two or three signature partner E2 sequences are observed. For some fo these bands signature inversion is found and this feature gives a great challenge to the theoretical models. In this study the researcher performed TRS and CSM calculations for all high-j rotational bands in the p186-194s Au nuclei aiming to predict the signature splitting and inversion phemomena, alignments, gains in alignments, gains in alignment and band crossing frequencies observed.en_US
dc.language.isoenen_US
dc.publisherUniversity of the Western Capeen_US
dc.subjectAu nucleien_US
dc.titleSignature splitting and inversion in the 186-194 Au Nuclei predicted by the total routhian surface (TRS) and cranked shell model (CSM) calculationsen_US
dc.typeThesisen_US
dc.rights.holderUniversity of the Western Capeen_US
dc.description.countrySouth Africa


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