Variational Monte Carlo study of soliton excitations in hard-sphere Bose gases

TL;DR

This study employs a full many-body Variational Monte Carlo approach to analyze soliton excitations in a three-dimensional hard-sphere Bose gas at zero temperature, revealing deviations from mean-field predictions at higher densities.

Contribution

It introduces a comprehensive many-body wave function and optimization method to accurately compute soliton properties beyond mean-field approximations in Bose gases.

Findings

Deviations from mean-field predictions increase with density.

Effective mass of solitons is smaller than Gross-Pitaevskii estimates.

Density profiles agree with local density approximation predictions.

Abstract

By using a full many-body approach, we calculate the excitation energy, the effective mass and the density profile of soliton states in a three dimensional Bose gas of hard spheres at zero temperature. The many-body wave function used to describe the soliton contains a one-body term, derived from the solution of the Gross-Pitaevskii equation, and a two-body Jastrow term which accounts for the repulsive correlations between atoms. We optimize the parameters in the many-body wave function via a Variational Monte Carlo procedure, calculating the grand-canonical energy and the canonical momentum of the system in a moving reference frame where the soliton is stationary. As the density of the gas is increased, significant deviations from the mean-field predictions are found for the excitation energy and the density profile of both dark and grey solitons. In particular, the soliton effective mass $m^\ast$ and the mass $m\Delta N$ of missing particles in the region of the density depression are smaller than the result from the Gross-Pitaevskii equation, their ratio being however well reproduced by this theory up to large values of the gas parameter. We also calculate the profile of the condensate density around the soliton notch finding good agreement with the prediction of the local density approximation.