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arXiv:1107.3855 · Physical Review A

Fluctuating and dissipative dynamics of dark solitons in quasicondensates

S. P. Cockburn, Hector E. Nistazakis, Theodoros P. Horikis, P. G. Kevrekidis, Nick P. Proukakis, D. J. Frantzeskakis

Published Oct 28, 2011• 29 citations
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Abstract

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 ${k}_{B}T<\ensuremath{\mu}<1.6$ ${k}_{B}T$, we find average soliton lifetimes to scale with temperature as $\ensuremath{\tau}\ensuremath{\sim}{T}^{\ensuremath{-}4}$, in agreement with predictions previously made for the low-temperature regime ${k}_{B}T\ensuremath{\ll}\ensuremath{\mu}$. 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.

DOI
10.1103/physreva.84.043640

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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.
In this thesis, we apply the stochastic Gross-Pitaevskii equation, using the formulation of Stoof, to the study of weakly interacting, finite temperature atomic Bose gases, both in and out of equilibrium. Explicitly maintaining the effects of phase and density fluctuations, this state-of-the-art method is well suited to the study of low dimensional Bose systems. As such, we consider the non-equilibrium dynamics of dark matter wave solitons, oscillating within harmonically trapped, one-dimensional phase-fluctuating condensates, through numerical simulations of the stochastic Gross-Pitaevskii equation. In treating the damping due to higher lying thermal modes of the system, we include the HartreeFock contribution of the equilibrium atomic density, which is a novel feature of our work. A stochastic approach is found to be essential in capturing the shot-to-shot variation in soliton trajectories observed experimentally. Neglecting stochastic effects, we find the well-known dissipative Gross-Pitaevskii equation to recover the average dynamics of the stochastic model, on retaining the microscopically justified form for the damping of this approach. Such a coupling is found to be necessary in modelling the dissipative nature of finite temperature soliton dynamics. Furthermore, we undertake a comparison between the finite temperature equilibrium state of the stochastic Gross-Pitaevskii equation, and that predicted within a number conserving Bogoliubov approach. Through a series of numerical experiments, we compare the equilibrium properties of a harmonically trapped Bose gas, considering our results in light of those of independent theoretical treatments, and additionally assessing the sensitivity of the numerical implementation of the former method to the numerical grid spacing. In the regime in which thermal effects dominate, the stochastic Gross-Pitaevskii approach proves to be a more consistent means of generating such equilibrium states.
We consider the decay of a dark soliton in a homogeneous BEC at finite temperature, with a particular emphasis on the effect of thermal noise on the stability of the soliton. We present an analytical treatment of a damped soliton in an unbounded system, comparing the predicted dynamics with numerical stochastic simulations of a spatially confined system. By varying the system temperature we study the relative importance of noise on the motion of the soliton. In the regime of low temperature the soliton is largely immune to thermal fluctuations, and is well described by the damped Gross-Pitaevskii equation. In this regime our analytical treatment is in close agreement with numerical simulations. For sufficiently high temperature, the thermal fluctuations have the interesting effect of increasing the stability of the soliton, extending its lifetime beyond the predictions of damped Gross-Pitaevskii theory.
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We study the dynamics of dark-bright (DB) solitons in binary mixtures of Bose gases at finite temperature using a system of two coupled dissipative Gross–Pitaevskii equations. We develop a perturbation theory for the two-component system to derive an equation of motion for the soliton centers and identify different temperature-dependent damping regimes. We show that the effect of the bright ('filling') soliton component is to partially stabilize 'bare' dark solitons against temperature-induced dissipation, thus providing longer lifetimes. We also study analytically thermal effects on DB soliton 'molecules' (i.e. two in-phase and out-of-phase DB solitons), showing that they undergo expanding oscillations while interacting. Our analytical findings are in good agreement with results obtained via a Bogoliubov–de Gennes analysis and direct numerical simulations.
The stochastic projected Gross-Pitaevskii equation (SPGPE) is a finite temperature theory of Bose-Einstein condensate (BEC) dynamics. It utilizes C-field techniques, which describe the dynamics of a low-energy coherent subspace in contact with a thermal reservoir [1]. There are two distinct mechanisms when interactions between the coherent field and the incoherent field are taken into account, known as number-damping and energy-damping. Number-damping has been treated extensively, while energy-damping has had less attention due to the lack of an accurate and efficient numerical method for solving it. However, Rooney et al. [2] developed a numerical technique allowing opportunities for the investigation of the energy-damping process. Bradley and McDonald examined the analytic treatment of the energy-damping process using functional Ito calculus for a range of systems, except for dark soliton. They found there is usually a regime where energy-damping dominates number-damping. Wright [3] has done analytical work on the dissipation of dark soliton in a homogenous system via a Lagrangian approach (where the number-damping term is treated as the perturbation to GPE). Still, the effect of the energy-damping process was not considered. In this thesis, we present an analytic investigation of the dissipation effects of number-damping and energy-damping on dark solitons. This is done through the framework of the one-dimensional Damped Gross-Pitaevskii equation (1D-DGPE). We take a Lagrangian variational approach and treat the number-damping and energy-damping as perturbations to the GPE. Dynamics of the soliton position are obtained, and anti-damping of the dark soliton in a harmonically trapped prolate BEC is observed in the perturbation regime. Our analytic work shows that dissipation effects of energy- damping becomes more dominant as the chemical potential of the system increases; for even modest chemical potential, energy-damping dominates number-damping. We compare our analytic results against numerical simulations and find good agreement for dark soliton position dynamics, kinetic energy, potential energy, and interaction energy dynamics in the regime where the dark soliton is near to the trap center and moving slowly relative to the speed of sound.