Numerical simulation of the Gross-Pitaevskii equation via vortex tracking
Thiago Carvalho Corso, Gaspard Kemlin, Christof Melcher, Benjamin Stamm
TL;DR
This work develops a reduced-order, vortex-tracking approach to the two-dimensional Gross–Pitaevskii equation in the small-$\varepsilon$ regime, leveraging the point-vortex dynamics governed by the renormalized energy $W$ and canonical harmonic maps. The authors construct well-prepared initial data, solve a one-dimensional ODE for vortex trajectories, and reconstruct GP solutions by smoothing the canonical map with a radial profile $f_{\varepsilon}$, achieving substantial computational savings while maintaining asymptotic accuracy as $\varepsilon\to0$. They provide rigorous error controls for the supercurrents and demonstrate convergence through numerical experiments, including spectral convergence in the harmonic-degree and fourth-order convergence in time, as well as explicit validation against full GP simulations. The method enables efficient, scalable GP simulations in the small-$\varepsilon$ limit, with potential extensions to more general domains and settings involving magnetic fields, while acknowledging limitations related to vortex collisions and emitted radiation.
Abstract
This paper deals with the numerical simulation of the Gross-Pitaevskii (GP) equation, for which a well-known feature is the appearance of quantized vortices with core size of the order of a small parameter $\varepsilon$. Without a magnetic field and with suitable initial conditions, these vortices interact, in the singular limit $\varepsilon\to0$, through an explicit Hamiltonian dynamics. Using this analytical framework, we develop and analyze a numerical strategy based on the reduced-order Hamiltonian system to efficiently simulate the infinite-dimensional GP equation for small, but finite, $\varepsilon$. This method allows us to avoid numerical stability issues in solving the GP equation, where small values of $\varepsilon$ typically require very fine meshes and time steps. We also provide a mathematical justification of our method in terms of rigorous error estimates of the error in the supercurrent, together with numerical illustrations.
