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Weakly Interacting Bose Gas

The weakly interacting Bose gas describes nonrelativistic bosons whose low-energy collisions are characterized by a scattering length. In three spatial dimensions, its dilute repulsive regime supports a condensate with sound-like collective excitations. The model connects an interatomic scattering measurement to a many-body excitation spectrum.

Consider a uniform gas at zero temperature, with no external potential. For atomic mass mm and bosonic field ψ\psi, the grand-canonical action is

S=∫dt d3x[iψ∗∂tψ−∣∇ψ∣22m+μ∣ψ∣2−g2∣ψ∣4],g=4πam.S=\int dt\,d^3x\left[ i\psi^*\partial_t\psi-\frac{|\nabla\psi|^2}{2m} +\mu|\psi|^2-\frac g2|\psi|^4 \right], \qquad g=\frac{4\pi a}{m}.

Here a>0a>0 is the low-energy ss-wave scattering length and μ\mu fixes the density. The contact coupling is matched to two-body scattering: a cutoff-dependent bare coupling inside a loop integral cannot simply be identified with 4πa/m4\pi a/m. Assume total density nn satisfies na3≪1na^3\ll1 and momenta are well below the inverse interaction range.

The field has a global U(1)U(1) symmetry and conserves atom number. This is a nonrelativistic theory with a preferred rest frame of the gas. A positive scattering length specifies the repulsive gas regime; it does not exclude molecular bound states or guarantee the absolute stability of a particular atomic species.

For a constant condensate ψ=n0\psi=\sqrt{n_0}, stationarity gives μ=gn0\mu=gn_0 at leading order. The corresponding energy density is gn02/2gn_0^2/2. Expanding ψ=n0+δψ\psi=\sqrt{n_0}+\delta\psi to quadratic order mixes δψ\delta\psi with its complex conjugate. The mode frequencies are the positive eigenvalues of

(ϵk+gn0gn0−gn0−ϵk−gn0),ϵk=k22m.\begin{pmatrix} \epsilon_k+gn_0 & gn_0\\ -gn_0 & -\epsilon_k-gn_0 \end{pmatrix}, \qquad \epsilon_k=\frac{k^2}{2m}.

Its characteristic equation gives

Ek2=ϵk(ϵk+2gn0).E_k^2=\epsilon_k(\epsilon_k+2gn_0).

This is the uniform-gas Bogoliubov dispersion Dalfovo et al. 1998, §IV.1, eq. (68). In the long-wavelength limit,

Ek≃csk,cs=gn0m,ξ=12mgn0.E_k\simeq c_s k, \qquad c_s=\sqrt{\frac{gn_0}{m}}, \qquad \xi=\frac{1}{\sqrt{2mgn_0}}.

The healing length ξ\xi locates the crossover: kξ≪1k\xi\ll1 gives sound, while kξ≫1k\xi\gg1 gives Ek=ϵk+gn0+⋯E_k=\epsilon_k+gn_0+\cdots within the contact theory’s momentum range. Setting g→0g\to0 at fixed n0n_0 recovers the free quadratic spectrum.

Density-response measurements probe this dispersion; the compressibility provides a second check through mcs2=n ∂μ/∂nmc_s^2=n\,\partial\mu/\partial n at leading order, where n0≃nn_0\simeq n. Quantum depletion makes n0n_0 differ from nn, so the mean-field relations are not exact at finite interaction strength.

The calculation assumes a weakly depleted condensate. Strong interactions, appreciable interaction range, loss dynamics, or low-dimensional infrared fluctuations require additional treatment. In particular, changing to one or two spatial dimensions changes both scattering and the conditions for long-range order.

The Weakly Interacting Bose Gas develops the condensate approximation; Bogoliubov Quasiparticles derives the mode transformation. Use Contact Interactions and Scattering Length when relating bare couplings to measured scattering. The Bose–Hubbard Model instead retains a spatial lattice.

  • Dalfovo, Franco, Stefano Giorgini, Lev P. Pitaevskii, and Sandro Stringari. Theory of Trapped Bose-Condensed Gases. Preprint (1998), arXiv:cond-mat/9806038v1. Open text.