Published January 1, 2010 | Version v1
Journal article

Propagation of sound and supersonic bright solitons in superfluid Fermi gases in BCS-BEC crossover

  • 1. Department of Physics, East China Normal University, Shanghai 200062 (China)
  • 2. Department of Physics, University of Hong Kong, Pokfulam Road (Hong Kong)
  • 3. Institute of Nonlinear Physics and Department of Physics, Zhejiang Normal University, Zhejiang 321004 (China)
  • 4. State Key Laboratory of Precision Spectroscopy and Department of Physics, East China Normal University, Shanghai 200062 (China)

Description

We investigate the linear and nonlinear sound propagations in a cigar-shaped superfluid Fermi gas with a large particle number. We first solve analytically the eigenvalue problem of linear collective excitations and provide explicit expressions of all eigenvalues and eigenfunctions, which are valid for all superfluid regimes in the Bardeen-Cooper-Schrieffer-Bose-Einstein condensation (BCS-BEC) crossover. The linear sound speed obtained agrees well with that of a recent experimental measurement. We then consider a weak nonlinear excitation and show that the time evolution of the excitation obeys a Korteweg de Vries equation. Different from the result obtained in quasi-one-dimensional case studied previously, where subsonic dark solitons are obtained via the balance between quantum pressure and nonlinear effect, we demonstrate that bright solitons with supersonic propagating velocity can be generated in the present three-dimensional system through the balance between a waveguidelike dispersion and the interparticle interaction. The supersonic bright solitons obtained display different physical properties in different superfluid regimes and hence can be used to characterize superfluid features of the BCS-BEC crossover.

Additional details

Identifiers

Publishing Information

Journal Title
Physical Review. B, Condensed Matter and Materials Physics
Journal Volume
81
Journal Issue
1
Journal Page Range
p. 014528-014528.11
ISSN
1098-0121

Optional Information

Notes
(c) 2010 The American Physical Society