research34 min studyLesson 487 in Physics

Bogoliubov excitations in trapped condensates

Linearize condensate dynamics to connect phonons, particle-like excitations, and geometry-dependent collective modes without extending a uniform dispersion beyond its domain.

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What you’ll understand

  • Derive the coupled particle–hole structure of small condensate fluctuations.
  • Identify phonon and free-particle limits using kξ.
  • Distinguish local-density excitations from discrete trapped modes and dipole calibration.

A condensate can oscillate collectively even when collisions between thermal atoms are rare. Its mean field couples a density disturbance to the surrounding phase, producing sound at long wavelength. Bogoliubov theory obtains these excitations by linearizing the Gross–Pitaevskii equation around a stationary condensate. It retains a paired fluctuation structure that differs from a single free atom in a trap. In a nonuniform cloud, the observable spectrum also depends on geometry and on how the disturbance is driven and detected.

The nonlinear background couples opposite frequencies

Write the condensate field as its stationary profile multiplied by the chemical-potential phase, plus a small fluctuation. A complex fluctuation generally contains both positive- and negative-frequency amplitudes. Expanding the density-dependent GP term couples them because a density change depends on the field and its conjugate. Neglecting that coupling recovers a particle-like approximation but loses the low-energy collective behavior that the theory was designed to capture.

For a uniform repulsive condensate, the coupled two-component eigenvalue problem yields a positive excitation energy whose square is a product of free-particle kinetic energy and that energy plus twice the mean field. The background is weakly depleted and the fluctuation is small, so the derivation is not a nonlinear saturation theory. Finite temperature, damping from quasiparticle interactions, and strongly correlated regimes require corrections beyond the elementary real Bogoliubov spectrum.

Ek=ℏωk=ϵk(ϵk+2gn),ϵk=ℏ2k22mE_k=\hbar\omega_k=\sqrt{\epsilon_k(\epsilon_k+2gn)},\qquad \epsilon_k=\frac{\hbar^2k^2}{2m}
Ek and εk are in joules, ωk in rad/s, and k in m⁻¹. This uniform three-dimensional spectrum assumes a stationary repulsive contact condensate, na³ ≪ 1, low depletion, and infinitesimal excitations. n is condensate density at this order.↔ Scroll wide equations horizontally.

Healing length marks a crossover in character

At wavevectors much smaller than inverse healing length, free-particle kinetic energy is small compared with the mean field. The square root then becomes linear in momentum and the mode is a phonon with the condensate sound speed. At large wavevector, the leading behavior is quadratic kinetic energy with a mean-field offset. A crossover mode is neither accurately described by the pure phonon line nor exactly a bare free particle.

The healing-length convention fixes where factors of two enter this comparison. With the conventional kinetic balance used previously, free-particle energy divided by mean field equals the square of k times ξ. A measured sound speed can therefore test the interaction energy if density and scattering length are calibrated. It does not alone prove that the entire observed spectrum follows uniform theory, particularly when excitation wavelengths approach cloud dimensions or the local density varies significantly.

ϵkgn=(kξ)2,Ek≃ℏck (kξ≪1),Ek≃ϵk+gn (kξ≫1)\frac{\epsilon_k}{gn}=(k\xi)^2,\qquad E_k\simeq\hbar ck\ (k\xi\ll1),\qquad E_k\simeq\epsilon_k+gn\ (k\xi\gg1)
ξ = ℏ/√(2mgn) and c = √(gn/m) use the same repulsive uniform convention. The two approximations are asymptotic limits of the displayed spectrum. The high-k expression remains within the low-energy contact description and does not authorize arbitrarily large momentum.↔ Scroll wide equations horizontally.

A trap replaces plane waves by discrete modes

In a slowly varying bulk region, a local-density approximation can use the uniform spectrum with local density when the wavelength is short compared with the profile variation scale. A global sloshing or breathing oscillation instead samples the entire trap and needs a trapped eigenmode calculation or a controlled hydrodynamic limit. Averaging one chosen density into the uniform formula does not generally reproduce a discrete collective frequency.

For perfectly harmonic confinement and translation-invariant interparticle interactions, center-of-mass motion decouples and the dipole frequency equals the corresponding trap frequency. This gives a useful calibration and numerical consistency check. Other modes do shift with interactions and geometry: in a spherical three-dimensional repulsive condensate deep in the Thomas–Fermi limit, the lowest monopole breathing frequency is square root of five times the trap frequency. Anharmonicity, anisotropy, and a thermal component can change these predictions.

ωdip,j=ωj,ωmono=5 ωtrap(spherical Thomas–Fermi limit)\omega_{\mathrm{dip},j}=\omega_j,\qquad \omega_{\mathrm{mono}}=\sqrt5\,\omega_{\mathrm{trap}}\quad\text{(spherical Thomas–Fermi limit)}
All frequencies are angular frequencies. The dipole statement assumes harmonic trapping and internal interactions depending only on relative positions. The monopole formula additionally assumes a three-dimensional spherical trap, repulsive GP hydrodynamics, low temperature, and negligible quantum pressure in the bulk.↔ Scroll wide equations horizontally.

Measure an excitation at the crossover

A uniform weakly interacting condensate has gn/h = 1000 Hz. An excitation is prepared with kξ = 1. Find its free-particle frequency εk/h, Bogoliubov frequency Ek/h, and whether a pure phonon approximation is controlled.

  1. The healing-length identity gives ϵk/(gn)=(kξ)2=1\epsilon_k/(gn)=(k\xi)^2=1. Thus εk/h is 1000 Hz.

  2. The full spectrum gives Ek/(gn)=1(1+2)=3E_k/(gn)=\sqrt{1(1+2)}=\sqrt3. Hence Ek/h is approximately 1732 Hz.

  3. The phonon requirement kξ ≪ 1 is not satisfied at unity. Its approximate value would differ appreciably, so the complete Bogoliubov expression should be used at this crossover.

The result

The free-particle scale is 1000 Hz and the Bogoliubov excitation is approximately 1732 Hz. The mode is in the crossover rather than a controlled long-wavelength phonon limit.

Explore the model

Interactive lab

Interactive lab · waves

A phase relation can reinforce or cancel a disturbance

Reset and set BOTH Phase difference to 0 degrees and Amplitude ratio to 1; predict reinforcement. Then Reset and set BOTH Phase difference to 180 degrees and Amplitude ratio to 1; predict cancellation. The instrument adds co-propagating waves at one fixed frequency. It illustrates linear superposition only, not Bogoliubov particle–hole equations, adjustable dispersion, opposite-frequency dynamics, or a trapped spectrum.

A phase relation can reinforce or cancel a disturbanceTwo waves share the same frequency and wave number. Playback advances t in sin(2x − t) + a sin(2x − t + phase). Current readings: Sum at x = 0: 0.866; Resultant amplitude: 1.732; Phase difference: 60°. All parameters are adjustable with the labeled controls below.−3.14−1.5701.573.14−3.4−1.701.73.4x · radiansAmplitude
SumFirst componentSecond component
Sum at x = 0
0.866
Resultant amplitude
1.732
Phase difference
60°
t = 0 s

Two waves share the same frequency and wave number. Playback advances t in sin(2x − t) + a sin(2x − t + phase). Parameter changes pause playback and recompute the model at the current elapsed time. Reset restores both parameters and returns time to zero. Playback starts paused. Adjust either parameter, then choose Play or Step.

Look forLinear addition is useful after the allowed excitations and their frequencies have been derived from the physical model.

Check your understanding

What frequency should a small dipole oscillation have in an exactly harmonic trap with translation-invariant internal interactions?

Try it yourself

A spherical trap has ordinary frequency 50 Hz and contains a repulsive condensate well inside the three-dimensional Thomas–Fermi low-temperature regime. Estimate the lowest monopole frequency and the dipole frequency. Explain why their interaction sensitivities differ.

Take a moment to make a prediction or work it out on paper. Open a hint when you need one.

Give me a hint

The same frequency ratios apply whether angular or ordinary frequencies are used consistently.

Compare with the solution

The monopole frequency is 5(50)≃111.8 Hz\sqrt5(50)\simeq111.8\,\mathrm{Hz}. The dipole remains 50 Hz in the ideal harmonic trap. Breathing changes internal density and therefore the pressure restoring force, whereas uniform center-of-mass displacement leaves internal relative coordinates unchanged. The monopole formula relies on the stated hydrodynamic and geometry assumptions; neither value includes anharmonic or finite-temperature shifts.

Take it with you

  • Bogoliubov coupling between conjugate amplitudes produces collective low-energy sound.
  • The dimensionless product kξ separates phonon, crossover, and particle-like regimes.
  • Local uniform response and discrete trapped collective modes require different approximations.

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