Owing to an increased density of s.p. Nilsson levels in the vicinity of the Fermi surface
for nearly spherical
nuclei, there appears
another type of ambiguity in choosing the Slater determinants representing
the anti-aligned configurations. Within the set of nuclei studied in this work,
this ambiguity manifests itself particularly strongly in Sc,
where we deal with four possible
anti-aligned MF configurations built on the Nilsson orbits originating
from the spherical
and
sub-shells. These configurations can be labeled in terms of the
quantum number
as
with
, 3/2, 5/2, and 7/2.
In the extreme shell-model picture, each of these states contains
all the and
=0, 2, 4, and 6 components. Within the projected
DFT picture, owing to configuration-dependent polarizations in
time-odd and time-even channels, the situation is more complicated
because the Slater determinants
corresponding to different
-values are no longer degenerate. Consequently, for each angular momentum
, one
obtains four different linearly-dependent solutions.
Calculations show that in all
=0 and
states of
interest, the isospin mixing
is essentially
independent of the choice of the initial Slater determinant. In contrast, the calculated ISB corrections
and energies depend on
, see Fig. 4.
![]() |