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Using the solutions for the homogeneous two-component 1D Fermi gas,
Figure 8.3:
Energy per particle,
(solid lines),
and size of the cloud, (dashed lines), for an inhomogeneous two component 1D
Fermi gas as a function of
for repulsive () and
attractive () interactions.
|
we now describe the inhomogeneous gas, Eq. 8.2, within the
LDA [DLO01,MS02,RFZZ03a]. This approximation is applicable if the size
of the cloud is much larger than the harmonic oscillator length in the
longitudinal direction,
, implying
and . The chemical potential of the inhomogeneous
system can be determined from the local equilibrium condition,
|
(8.10) |
and the normalization condition
, where is measured
from the center of the trap,
, and
for and
for
. The normalization condition can be reexpressed in terms of the
dimensionless chemical potential and the dimensionless density
[
and
],
|
(8.11) |
This expression emphasizes that the coupling strength is determined by
;
corresponds to the weak coupling and
to the strong coupling regime, irrespective of whether the
interactions are attractive or repulsive [MS02].
Figure 8.3 shows the energy per particle and the size of the
cloud as a function of the coupling strength
for positive and
negative calculated within the LDA for an inhomogeneous two-component 1D
Fermi gas. Compared to the non-interacting gas, for which ,
increases for repulsive interactions and decreases for attractive interactions. For
, reaches the asymptotic value for the
strongly repulsive regime,
, and the value
for the strongly attractive regime,
.
The shrinking of the cloud for attractive interactions reflects the formation of
tightly bound molecules. In the limit
, the energy per
particle approaches
,
indicating the formation of a molecular bosonic Tonks-Girardeau gas, consisting of
molecules. The size of the cloud shrinks from
in the strongly
repulsive regime (
and ) to
in the
strongly attractive regime (
and ). We also notice
that, similarly to the homogeneous case, for large attractive interactions the
energy per particle approaches the molecular binding energy
.
Using a sum rule approach, the frequency of the lowest compressional
(breathing) mode of harmonically trapped 1D gases can be calculated from the
mean-square size of the cloud
[MS02],
|
(8.12) |
In the weak and strong coupling regime (
and ,
respectively),
has the same dependence on as the
ideal 1D Fermi gas. Consequently, is in these limits given by ,
irrespective of whether the interaction is repulsive or attractive.
Solid lines in Fig. 8.3 show , determined numerically from
Eq. 8.12, as a function of the interaction strength
.
A non-trivial behavior of as a function of
is visible.
To gain further insight, we calculate the first correction to the
breathing mode frequency
Figure 8.4:
Square of the lowest breathing mode frequency,
, as a function of the coupling strength
for an
inhomogeneous two-component 1D Fermi gas with repulsive () and attractive
() interactions determined numerically from Eq. 8.12 (solid
lines). Dashed lines show analytic expansions.
|
[
] analytically for weak repulsive
and attractive interactions, as well as for strong repulsive and attractive
interactions. For the weak coupling regime, we find
, where the minus sign applies to repulsive
interactions and the plus sign to attractive interactions. For the strong coupling
regime, we find
for
repulsive interactions and
for attractive
interactions (see Table 1.1).Dashed lines in Fig. 8.4 show the resulting analytic expansions for
, which describe the lowest breathing mode frequency quite well over a
fairly large range of interaction strengths but break down for
.
Next: Conclusions
Up: Interacting fermions in highly
Previous: Homogeneous system
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G.E. Astrakharchik
15-th of December 2004