Bogoliubov Excitations of Inhomogeneous Bose-Einstein ...
Bogoliubov Excitations of Inhomogeneous Bose-Einstein ...
Bogoliubov Excitations of Inhomogeneous Bose-Einstein ...
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4. Disorder—Results and Limiting Cases<br />
4.1.1. Direct derivation from hydrodynamic equations <strong>of</strong><br />
motion<br />
We start from the equations <strong>of</strong> motion (2.18) for density and phase in the<br />
limit <strong>of</strong> negligible quantum pressure. For the ground state this means that<br />
the Thomas-Fermi formula (2.20) applies, n0(r) = nTF = (µ − V (r))/g. 1<br />
The speed <strong>of</strong> sound characterizes the dynamics <strong>of</strong> small deviations δn(r, t) =<br />
n(r, t) − n0(r) and δϕ(r, t) = ϕ(r, t) − ϕ0 from the ground state in the long<br />
wave-length regime kξ ≪ 1. In terms <strong>of</strong> density and superfluid velocity, the<br />
linearized equations <strong>of</strong> motion (2.18) read<br />
∂tδn + ∇ · [n0(r)v] = 0, (4.1)<br />
∂tv = − g<br />
∇δn, (4.2)<br />
m<br />
and are recognized as the linearized versions <strong>of</strong> continuity equation and<br />
Euler’s equation for an ideal compressible fluid, respectively. These can be<br />
combined to a single classical wave equation<br />
� � 2 2 2 1<br />
c ∇ − ∂t δn = m∇ · [V (r)∇δn] . (4.3)<br />
Translation invariance <strong>of</strong> the free equation suggests using a Fourier representation<br />
in space and time,<br />
� 2 2 2<br />
ω − c k � � d ′ d k<br />
δnk =<br />
(2π) d � Vkk ′δnk ′. (4.4)<br />
The disorder potential causes scattering k → k ′ <strong>of</strong> plane waves with an<br />
amplitude<br />
�V kk ′ = − 1<br />
m (k · k′ ) V k−k ′. (4.5)<br />
The factor k·k ′ originates from the mixed gradient in (4.3) and implies pure<br />
p-wave scattering <strong>of</strong> sound waves as discussed in section 2.4, in contrast to<br />
s-wave scattering <strong>of</strong> independent particles [23].<br />
In contrast to the perturbation theory in section 3.3, the starting point<br />
(4.3) is a second-order equation <strong>of</strong> motion and does not have the blockmatrix<br />
structure. Apart from that, the diagrammatic perturbation theory<br />
works exactly the same way. Analogously to (3.28), the following equation<br />
defines the Green function � G<br />
� �G −1<br />
0 − � V � � G = 1. (4.6)<br />
1 Note that within the Thomas-Fermi approximation, the average particle density does not change. Thus,<br />
we need not distinguish Λµ and ΛN (section 3.4.5) in the present section 4.1.<br />
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