Abstract
Some general systematic features of the signature inversion phenomenon in doubly-odd lighter rare-earth nuclei are presented. Schematic calculations are carried out within the framework of the two-quasiparticle plus rotor model (TQPRM) to explain these features. It is found that the systematics can be well explained if the h 9 2 : 1 2 [541] proton orbital is included in the calculations in addition to the complete set of h 11 2 proton and i 13 2 neutron orbitals.
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