Rate of convergence for numerical $α$-dissipative solutions of the Hunter-Saxton equation
Thomas Christiansen, Katrin Grunert
TL;DR
The paper establishes a robust convergence rate for numerical approximations of $\alpha$-dissipative solutions to the Hunter–Saxton equation, extending previous results to $α\in W^{1,\infty}(\mathbb{R},[0,1))$. By combining a generalized method of characteristics with a piecewise-linear projection and an NVWE-inspired pair of variable transformations, the authors control energy concentration and wave-breaking effects across Eulerian and Lagrangian coordinates. They prove that the numerical solution converges with an error of $\mathcal{O}(Δx^{1/8}+Δx^{β/4})$ in $L^{\infty}(\mathbb{R})$ under a Besov-type regularity $\bar{u}_x\in B_2^{β}$, and provide explicit convergence rates for representative data, including multipeakon and cusp profiles, supported by numerical experiments. This offers a robust, wave-breaking-tolerant framework for simulating HS dynamics with energy dissipation guided by spatially varying $α$.
Abstract
We prove that $α$-dissipative solutions to the Cauchy problem of the Hunter-Saxton equation, where $α\in W^{1, \infty}(\mathbb{R}, [0, 1))$, can be computed numerically with order $\mathcal{O}(Δx^{{1}/{8}}+Δx^{β/{4}})$ in $L^{\infty}(\mathbb{R})$, provided there exist constants $C > 0$ and $β\in (0, 1]$ such that the initial spatial derivative $\bar{u}_{x}$ satisfies $\|\bar{u}_x(\cdot + h) - \bar{u}_x(\cdot)\|_2 \leq Ch^β$ for all $h \in (0, 2]$. The derived convergence rate is exemplified by a number of numerical experiments.
