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S. Frauendorf, Rev. Mod. Phys. 73, 463 (2001).
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The Skyrme-HF calculations (no pairing) were performed by using the
HFODD (v2.00k) code [13,14] working in the harmonic
oscillator basis (N0=14 spherical shells were taken). Only the
parity was kept as the conserved symmetry, which allowed for an
arbitrary direction of the angular momentum vector in space. The
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influence on the chiral rotation requires further separate study.
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Although we speak here of a rigid body, the values of the three
moments of inertia need not, and do not, correspond to those of a
massive body having the same shape as the nucleus[5].
See also Ref.[17] for a similar model
developed for axial shapes.
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P. Olbratowski, J. Dobaczewski, and J. Dudek, to be published in Computer
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A.M. Kamchatnov, J. Phys. G 16, 1203 (1990).
Jacek Dobaczewski
2002-11-27