Abstract

A parameter-free investigation of the moments of inertia of ground-state rotational bands in well-deformed rare-earth nuclei is carried out using cranked relativistic Hartree-Bogoliubov (CRHB) and nonrelativistic cranked Hartree-Fock-Bogoliubov (CHFB) theories. In CRHB theory, the relativistic fields are determined by the nonlinear Lagrangian with the NL1 force and the pairing interaction by the central part of a finite-range Gogny D1S force. In CHFB theory, the properties in particle-hole and particle-particle channels are defined solely by Gogny D1S forces. Using an approximate particle number projection before variation by means of the Lipkin-Nogami method improves the agreement with the experimental data, especially in CRHB theory. The effect of the particle number projection on the moments of inertia and pairing energies is larger in relativistic than in nonrelativistic theory.

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