Fluctuating and dissipative dynamics of dark solitons in quasicondensates

被引:24
作者
Cockburn, S. P. [1 ]
Nistazakis, H. E. [2 ]
Horikis, T. P. [3 ]
Kevrekidis, P. G. [4 ]
Proukakis, N. P. [1 ]
Frantzeskakis, D. J. [2 ]
机构
[1] Newcastle Univ, Sch Math & Stat, Newcastle Upon Tyne NE1 7RU, Tyne & Wear, England
[2] Univ Athens, Dept Phys, GR-15784 Athens, Greece
[3] Univ Ioannina, Dept Math, GR-45110 Ioannina, Greece
[4] Univ Massachusetts, Dept Math & Stat, Amherst, MA 01003 USA
来源
PHYSICAL REVIEW A | 2011年 / 84卷 / 04期
基金
英国工程与自然科学研究理事会; 美国国家科学基金会;
关键词
BOSE-EINSTEIN CONDENSATION; GROSS-PITAEVSKII EQUATION; MOTION;
D O I
10.1103/PhysRevA.84.043640
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
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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页数:16
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