Triaxial superdeformed bands in 163 Lu are analysed by applying the Holstein-Primakoff transformation both to the total and single-particle angular momenta. Quite good agreements with the experimental values are reproduced in the energy difference between two superdeformed bands as a function of angular momentum, and also in the ratio of E2 transitions among these bands. The results coming from the exact diagonalization of the particle plus rotor Hamiltonian are compared with the approximate calculation. Recently, triaxial superdeformed bands in 163 Lu nucleus 1) have been observed, which are interpreted as the wobbling motion. 2) We have already proposed the theory for the triaxially deformed bands nearly thirty years ago. 3) The difference between our treatment and Bohr-Mottelson’s text book is in the quantization axis and in the order of approximation. We chose z-axis as the quantization axis, while BohrMottelson chose x-axis. We included the whole effect coming from 1/I where I is the total angular momentum. These two differences help us to get the exact energy eigenvalue at the axially symmetric limit. Moreover, our paper is the first work that applied the Holstein-Primakoff transformation to the nuclear physics. In this paper we extend our old theory to the odd nuclei by introducing two kinds of bosons for the total angular momentum I and the single-particle angular momentum j. Here, we pay attention to the symmetry of the nucleus. Both the rotor and the intrinsic Hamiltonian have D2-symmetry, and are also the function of deformations β and γ. There appears another symmetry in 5-dimensional space (three Eulerian angles, β and γ), which is called Bohr’s symmetry. 4) Thus, it is different from the classical precession around rigid body given in the text book by Landav-Lifshits. 5) We adopt an approximate wave function as, [D I φΩ +( −) I−j+κ D I −K φ−Ω], where κ = Ω − K is restricted to the even value because of the Bohr’s symmetry. Then the energy eigenvalue becomes the average of κ and −κ, and the energy difference between κ+2 and κ becomes constant independent from I. We adopt the irrotational flow formula for the moments of inertia as Ji = Cβ 2 sin 2 (γ− 2π 3 i), and the quadrupole moments are proportional to these moments of inertia. In the numerical analysis for 163 Lu, we adopt the state for the triaxially deformed superdeformed band 1 (TSD1) as K = 1 Ω = 1 (κ = 0), and for the triaxially deformed superdeformed band 2 (TSD2) as K = − 3 Ω = 1 (κ = 2). We adopt γ =1 9 ◦ , and unique-parity level i13/2 for the last nucleon. The band head energies of TSD1 and TSD2 are adjusted to the experimental energies. Three moments of inertia become J irr
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