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A High Order IMEX Method for Generalized Korteweg de-Vries Equations

Seth Gerberding

TL;DR

The paper develops a robust high-order IMEX method for generalized Korteweg de-Vries equations by coupling $H^1$-conforming finite elements in space with a split IMEX time integrator that treats the dispersive third-order term implicitly and the nonlinear hyperbolic flux explicitly. A reformulation with auxiliary variables reduces spatial derivatives to second order, enabling $H^1$ discretization while preserving mass and achieving $L^2$-stability; high-order accuracy is attained through graph-viscosity, a limiter, consistent mass, and a high-order ERK-DIRK time integration. Theoretical results include $\ell^2$ stability and mass conservation, plus well-posed dispersive updates, complemented by extensive numerical simulations (convergence tests, Zabusky-Kruskal, and multi-soliton interactions) validating accuracy and robustness. The method offers a CFL requirement of $\tau = \mathcal{O}(h)$, avoids nonlinear solves, and generalizes to polynomial and system fluxes, indicating strong practical significance for simulating dispersive wave phenomena with general flux structures.

Abstract

In this paper, we introduce a high order space-time approximation of generalized Korteweg de-Vries equations. More specifically, the method uses continuous $H^1$-conforming finite elements for the spatial approximation and implicit-explicit methods for the temporal approximation. The method is high order in both space, provably stable, and mass-conservative. The scheme is formulated, its properties are proven, and numerical simulations are provided to illustrate the proposed methodology.

A High Order IMEX Method for Generalized Korteweg de-Vries Equations

TL;DR

The paper develops a robust high-order IMEX method for generalized Korteweg de-Vries equations by coupling -conforming finite elements in space with a split IMEX time integrator that treats the dispersive third-order term implicitly and the nonlinear hyperbolic flux explicitly. A reformulation with auxiliary variables reduces spatial derivatives to second order, enabling discretization while preserving mass and achieving -stability; high-order accuracy is attained through graph-viscosity, a limiter, consistent mass, and a high-order ERK-DIRK time integration. Theoretical results include stability and mass conservation, plus well-posed dispersive updates, complemented by extensive numerical simulations (convergence tests, Zabusky-Kruskal, and multi-soliton interactions) validating accuracy and robustness. The method offers a CFL requirement of , avoids nonlinear solves, and generalizes to polynomial and system fluxes, indicating strong practical significance for simulating dispersive wave phenomena with general flux structures.

Abstract

In this paper, we introduce a high order space-time approximation of generalized Korteweg de-Vries equations. More specifically, the method uses continuous -conforming finite elements for the spatial approximation and implicit-explicit methods for the temporal approximation. The method is high order in both space, provably stable, and mass-conservative. The scheme is formulated, its properties are proven, and numerical simulations are provided to illustrate the proposed methodology.

Paper Structure

This paper contains 25 sections, 9 theorems, 45 equations, 5 figures, 4 tables.

Key Result

Lemma 3.1

Let $(u,z,g)$ be a smooth periodic solution to eqn: disp-reform-u-eqn: disp-reform-g. Then the following energy conservation equation holds:

Figures (5)

  • Figure 1: Comparison of the IMEX method to the Leap-Frog method of Zabusky_65.
  • Figure 2: Comparison of the IMEX method to the TDSR method of Chandramouli_Farhat_Musslimani_22.
  • Figure 3: Space time plot for the single soliton solution \ref{['eqn: kdv-solution']} of the KdV equation \ref{['eqn: kdv']} with initial condition $u_0(x) = 2\mathop{\mathrm{sech}}\nolimits^2(x)$.
  • Figure 4: Space-time plots of the two-soliton interacting solution \ref{['eqn: kdv-2-soliton-solution']} for the KdV equation \ref{['eqn: kdv']}. Left: surface plot. Right: contour plot.
  • Figure 5: Space-time plots for the three-soliton interaction for the KdV equation \ref{['eqn: kdv']}. Left: Surface plot. Right: contour plot.

Theorems & Definitions (25)

  • Lemma 3.1
  • Proof 1
  • Lemma 3.2
  • Proof 2
  • Corollary 3.3: Hyperbolic stability
  • Proof 3
  • Lemma 3.4: Hyperbolic mass conservation
  • Proof 4
  • Lemma 3.5: Dispersive stability
  • Proof 5
  • ...and 15 more