Publication Date

2010

Journal or Book Title

PHYSICAL REVIEW LETTERS

Abstract

The dynamics of dark matter-wave solitons in elongated atomic condensates are discussed at finite temperatures. Simulations with the stochastic Gross-Pitaevskii equation reveal a noticeable, experimentally observable spread in individual soliton trajectories, attributed to inherent fluctuations in both phase and density of the underlying medium. Averaging over a number of such trajectories (as done in experiments) washes out such background fluctuations, revealing a well-defined temperature-dependent temporal growth in the oscillation amplitude. The average soliton dynamics is well captured by the simpler dissipative Gross-Pitaevskii equation, both numerically and via an analytically derived equation for the soliton center based on perturbation theory for dark solitons.

Comments

This is the prepublished version harvested from ArXiv. The published version is located at http://prl.aps.org/abstract/PRL/v104/i17/e174101

Pages

-

Volume

104

Issue

17

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