Journal
PHYSICAL REVIEW A
Volume 84, Issue 4, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevA.84.043640
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Funding
- EPSRC [NSF-DMS-0806762]
- Alexander von Humboldt Foundation
- University of Athens
- Engineering and Physical Sciences Research Council [EP/F055935/1] Funding Source: researchfish
- EPSRC [EP/F055935/1] Funding Source: UKRI
- Direct For Mathematical & Physical Scien
- Division Of Mathematical Sciences [0806762] Funding Source: National Science Foundation
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The fluctuating and dissipative dynamics of matter-wave dark solitons within harmonically trapped, partially condensed Bose gases is studied both numerically and analytically. A study of the stochastic Gross-Pitaevskii equation, which correctly accounts for density and phase fluctuations at finite temperatures, reveals dark-soliton decay times to be lognormally distributed at each temperature, thereby characterizing the previously predicted long-lived soliton trajectories within each ensemble of numerical realizations [ S. P. Cockburn et al., Phys. Rev. Lett. 104, 174101 (2010)]. Expectation values for the average soliton lifetimes extracted from these distributions are found to agree well with both numerical and analytic predictions based upon the dissipative Gross-Pitaevskii model (with the same ab initio damping). Probing the regime for which 0.8 k(B)T < mu < 1.6 k(B)T, we find average soliton lifetimes to scale with temperature as tau similar to T-4, in agreement with predictions previously made for the low-temperature regime k(B)T << mu. The model is also shown to capture the experimentally relevant decrease in the visibility of an oscillating soliton due to the presence of background fluctuations.
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