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Abstract:
Using the particle-number conserving (PNC) method for treating the cranked shell model,the microscopic mechanism of the variation with rotational frequency ω of the kinematics moments of inertia for the rare-earth deformed nuclei 178,179Hf is investigated. The 2-qp and 4-qp bands in 17872Hf and 3-qp bands in 17972Hf are analyzed and calculated.The observed ω variation of J(1) is reproduced satisfactorily in PNC calculations. Our analysis shows that the difference between the ω variations of J(1) for the high K multi-quasiparticle bands and for the ground state band is mainly due to the Pauli blocking effects of high j intruder orbitals near the Fermi surface.
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