Background: To describe shape fluctuations associated with large-amplitude collective motion in the quadrupole degrees of freedom, the five-dimensional collective Hamiltonian (5DCH) has been widely used. The inertial functions in the 5DCH are microscopically calculated with the energy density functional (EDF) theory employing the cranking formula. However, since the cranking formula ignores dynamical residual effects, it is known to fail to reproduce the correct inertial functions, for instance, the total mass for the translational motion.

Purpose: We aim to resolve problems of the insufficient description of the inertial functions in the 5DCH. We provide a practical method to include the dynamical residual effects in the inertial functions that depend on the quadrupole deformation parameters $\beta$ and $\gamma$.

Methods: We use the local quasiparticle random-phase approximation (LQRPA) based on the constrained Hartree-Fock-Bogoliubov states in the $\beta \text{−}\gamma$ plane with the Skyrme EDF. The finite-amplitude method is used for efficient computations of the LQRPA.

Results: The inertial functions evaluated with the LQRPA significantly increase from the ones with the cranking formula due to the dynamical residual effects. This increase also shows a strong $\beta \text{−}\gamma$ dependence. We show an application of the present method to a transitional nucleus ${}^{110}\mathrm{Pd}$. The low-lying spectra are well reproduced with the LQRPA inertial functions.

Conclusions: We clarify the importance of the dynamical residual effects in the inertial functions of the 5DCH for the description of the low-lying spectra. The 5DCH with the improved inertial functions provides a reliable and efficient description of low-lying spectra in nuclei associated with the quadrupole shape fluctuation.

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• Collective levels
• Collective models
• Electromagnetic transitions
• Energy levels
• Nuclear density functional theory
• Nuclear shapes and moments
• Nuclear spin & parity