Abstract
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.