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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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