Computing the ground state solution of Bose-Einstein condensates by a normalized gradient flow
Weizhu Bao, Qiang Du

TL;DR
This paper proves the energy diminishing property of a normalized gradient flow for computing Bose-Einstein condensate ground states, introduces two effective numerical discretization methods, and demonstrates their superior performance through extensive simulations.
Contribution
It provides a rigorous mathematical justification for the imaginary time method and introduces two energy-preserving numerical schemes for BEC ground state computation.
Findings
BEFD and TSSP methods preserve energy diminishing property.
Numerical results confirm effectiveness in 1D, 2D, and 3D simulations.
Normalized gradient flow can compute first excited states with specific initial data.
Abstract
In this paper, we prove the energy diminishing of a normalized gradient flow which provides a mathematical justification of the imaginary time method used in physical literatures to compute the ground state solution of Bose-Einstein condensates (BEC). We also investigate the energy diminishing property for the discretization of the normalized gradient flow. Two numerical methods are proposed for such discretizations: one is the backward Euler centered finite difference (BEFD), the other one is an explicit time-splitting sine-spectral (TSSP) method. Energy diminishing for BEFD and TSSP for linear case, and monotonicity for BEFD for both linear and nonlinear cases are proven. Comparison between the two methods and existing methods, e.g. Crank-Nicolson finite difference (CNFD) or forward Euler finite difference (FEFD), shows that BEFD and TSSP are much better in terms of preserving energy…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCold Atom Physics and Bose-Einstein Condensates · Strong Light-Matter Interactions · Quantum, superfluid, helium dynamics
