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The nucleus in the center-of-mass frame is described by 3A−3 independent coordinates, including three Euler angles and three variables ρ,β,andγ to describe orientation, size, and shape of the nuclear inertia ellipsoid as well as 3A−9 generalized Euler angles to describe internal motion of the nucleons. Based on the idea that the incompressible nucleus has constant density, we suggest a definition of the deformation parameter β. It allows us to derive the Hamiltonian, which describes large-amplitude collective motions. At β≪1 it reduces to a sum of the Bohr Hamiltonian and the Hamiltonian of monopole ρ vibrations. As a result of straightforward calculations we obtain explicit expressions for all the inertial parameters as functions of the variables ρ,β,andγ. Published by the American Physical Society 2024
Dzyublik et al. (Wed,) studied this question.
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