Bogoliubov Excitations of Inhomogeneous Bose-Einstein ...
Bogoliubov Excitations of Inhomogeneous Bose-Einstein ...
Bogoliubov Excitations of Inhomogeneous Bose-Einstein ...
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2.4. Single scattering event<br />
theory for a weak potential. The trapping potential is neglected, instead,<br />
the impurity potential is placed into a finite homogeneous system with periodic<br />
boundary conditions. In order to investigate the interesting envelope<br />
function (2.59) in the scattering amplitude (2.61), the potential factor V k ′ −k<br />
should allow scattering in all directions. That means, the impurity should<br />
be pointlike in the sense that its extension r0 should be much smaller than<br />
the wave length kr0 ≪ 1. First, the Gross-Pitaevskii ground state is calculated<br />
by imaginary-time propagation, using the forth-order Runge-Kutta<br />
method [104]. Then a plane-wave <strong>Bogoliubov</strong> excitation <strong>of</strong> the unperturbed<br />
system is superposed. During the real-time evolution, the wave propagates<br />
and is scattered at the impurity. After some time t, the stationary scattering<br />
state should be reached in a square with edge length L ≈ c t around the<br />
impurity. This part <strong>of</strong> the system is Fourier transformed and compared to<br />
the condensate ground state without the excitation. In the density plot <strong>of</strong><br />
the scattered wave |δΨ k ′| 2 , figure 2.7(a), one can already observe the node<br />
<strong>of</strong> vanishing scattering amplitude (2.60) very clearly.<br />
The data shown in figure 2.7(a) still shows the Gross-Pitaevskii wave<br />
function. One can get more insight in terms <strong>of</strong> <strong>Bogoliubov</strong> amplitudes γ k ′ =<br />
uk ′δΨk ′+vk ′δΨ∗<br />
−k ′, with uk = (ɛk+ɛ0 k )/(2�ɛkɛ0 k ) and vk = (ɛk−ɛ0 k )/(2�ɛkɛ0 k ).<br />
The corresponding plot <strong>of</strong> the imaginary part <strong>of</strong> the <strong>Bogoliubov</strong>-transformed<br />
amplitude in figure 2.7(b) clearly shows the amplitude sign change across the<br />
scattering node. Note that figure 2.7(b) is much clearer than figure 2.7(a),<br />
because there <strong>Bogoliubov</strong> excitations with opposite ±k ′ interfere in the wave<br />
function densities |δΨk ′| 2 . One may wonder why the superposition <strong>of</strong> nodes<br />
stemming from opposite wave vectors still gives a density dip as clear as in<br />
figure 2.7(a). In fact, in the single-particle case kξ ≫ 1, vk/uk tends to zero<br />
such that only the node <strong>of</strong> one component is observed, whereas for sound<br />
waves kξ ≪ 1 both components contribute equally, but now with symmetric<br />
nodes at ± π<br />
2<br />
that superpose exactly. This node robustness should facilitate<br />
the experimental observation.<br />
We extract the scattering amplitude from the data on the elastic scattering<br />
circle in figure 2.7(b) and plot it together with the analytical prediction<br />
(2.61) as function <strong>of</strong> the scattering angle θ at various wave vectors kξ, as<br />
shown in figure 2.8. The agreement is very good, with residual numerical<br />
scatter due to transients and boundary effects.<br />
Equation (2.61) and figure 2.8 show that the overall magnitude <strong>of</strong> scattering<br />
peaks at kξ ≈ 1, at the crossing from waves to particles. Physically,<br />
this results from two competing scalings in (2.56):<br />
• The <strong>Bogoliubov</strong> scattering amplitude W (k, θ) ∝ ɛ 0 k /ɛk is proportional<br />
to k for kξ ≪ 1 and saturates to a constant for kξ ≫ 1.<br />
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