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Thus far we have chosen not to let C1s depend
on the density. Little is known about the empirical density dependence
of the time-odd energy functional, and time-odd Landau parameters
calculated from a ``realistic'' one-boson exchange potential in DBHF
show only a very weak density dependence [64]. Because the
kinetic spin term
,
when evaluated in INM, also contributes to the density dependence
of the Landau parameters, the density-dependence of that term must
either be small or nearly canceled by other time-odd terms.
In any event, in the following, we investigate what happens when C1s
depends on the (isoscalar) density in the ``standard" way (10).
All nuclei we look at have finite neutron excess, which means that
the central density should be slightly smaller than .
Figure 8:
Variation of the GT resonance energy and the strength
in the resonance when the ratio
xC1s[0]/
of parameters
defining the density dependence of
in
Eq. (10) is varied. Symbols and scales
are as in Fig. 6.
|
If g0' and g1' are fixed in saturated INM, there is one free
parameter, C1s[0], with which one can vary the density
dependence (10). (
is
fixed by the value
=1.2, and we
set the exponent =0.25, as it is in the time-even energy
functional SkO'.) We continue here to assume that gauge invariance
holds, and that
.
We vary the parameter C1s[0] between
and
.
Figure 7 shows the spatial
dependence of
for several values of the ratio
xC1s[0]/
.
By changing
C1s[0], one can change both the GT resonance energy and the amount
of the low-lying strength, even with
kept
constant. As Fig. 8 shows, an increase of
C1s[0] for a given g0' has almost the same effect as an
increase of g0' for a given C1s[0]. Thus, the INM Landau
parameters do not tell the whole story in a finite nucleus.
Figures 7 and 8 show that the spin-spin
coupling has the largest effect on the GT resonance when it is located
at or even slightly outside the nuclear radius.
Next: Study of .
Up: GT resonances from generalized
Previous: Study of .
Jacek Dobaczewski
2002-03-15