A search for the self-consistent solutions for the chiral rotational bands in
the N=75 isotones, 130Cs, 132La, 134Pr and 136Pm is performed within the
Skyrme-Hartree-Fock cranking approach using SKM* and SLy4 parametrizations. The
dependence of the solutions on the time-odd contributions in the energy
functional is studied. From among the considered four isotones, self-consistent
chiral solutions are obtained only in 132La. The microscopic calculations are
compared with the 132La experimental data and with results of a classical model
that contains all the mechanisms underlying the chirality of the collective
rotational motion. Strong similarities between the HF and classical model
results are found. The suggestion formulated earlier by the authors that the
chiral rotation cannot exist below a certain critical frequency is further
illustrated and discussed, together with the microscopic origin of a transition
from the planar to chiral rotation in nuclei. We also formulate the
separability rule by which the Tilted-Axis-Cranking solutions can be inferred
from three independent Principal-Axis-Cranking solutions corresponding to three
different axes of rotation.Comment: 23 LaTeX pages, 11 PostScript Figure