Abstract

We investigate the nonlocal Gross–Pitaevskii (GP) equation with long-range dipole-dipole and contact interactions (including binary and three-body collisions). We address the impact of the three-body interaction on stabilizing trapless dipolar Bose–Einstein condensates (BECs). It is found that the dipolar BECs exhibit stability not only for the usual combination of attractive binary and repulsive three-body interactions, but also for the case when these terms have opposite signs. The trapless stability of the dipolar BECs may be further enhanced by time-periodic modulation of the three-body interaction imposed by means of Feshbach resonance. The results are produced analytically using the variational approach and confirmed by numerical simulations.

Highlights

  • The advent of Bose–Einstein condensates (BECs) in 52Cr [1,2], 164Dy [3,4] and 168Er [5]accompanied by long-range dipole-dipole (DD) interactions superimposed on the contact inter-atomic collisions has impacted the investigation of ultracold quantum gases [6]

  • The theoretical description of a dilute weakly interacting dipolar BECs (DBECs) is based on the Gross– Pitaevskii (GP) equation with the nonlocal DD-interaction term [1,2,23,24,25]

  • We further show that the introduction of the time-dependent part of the three-body interaction, χ1 may further, enhance the stability of the trapless dipolar repulsive BECs

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Summary

Introduction

The advent of Bose–Einstein condensates (BECs) in 52Cr [1,2], 164Dy [3,4] and 168Er [5]. Following the scheme of the stabilization of the inverted (Kapitza) pendulum [30], scenarios for stabilization of two-dimensional (2D) optical [31] and matter-waves [32,33,34] by means of the “nonlinearity management” [35], i.e., the cubic nonlinearity periodically switching between self-attraction and repulsion, have been elaborated. This concept has been subsequently applied to 3D vortex solitons [32,34] and extended to the model containing the three-body interaction [36] and quantum fluctuations [37].

The Model
The Variational Method
N 4 χ21 243π6d4z Ω2
Three-Dimensional Numerical Results
Conclusions
Full Text
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