A Lipschitz metric for $\alpha$-dissipative solutions to the Hunter-Saxton equation
Katrin Grunert, Matthew Tandy

TL;DR
This paper investigates the Lipschitz stability of $\alpha$-dissipative solutions to the Hunter-Saxton equation, providing a framework to understand how solutions depend continuously on initial data, especially considering energy dissipation.
Contribution
It introduces a Lipschitz metric tailored for $\alpha$-dissipative solutions, extending stability analysis to solutions with spatially varying energy loss.
Findings
Established Lipschitz stability for $\alpha$-dissipative solutions
Developed a generalized characteristic method for stability analysis
Provided insights into energy dissipation effects on solution stability
Abstract
We explore the Lipschitz stability of solutions to the Hunter-Saxton equation with respect to the initial data. In particular, we study the stability of -dissipative solutions constructed using a generalised method of characteristics approach, where is a function determining the energy loss at each position in space.
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Taxonomy
TopicsNonlinear Waves and Solitons · Advanced Mathematical Physics Problems · Fractional Differential Equations Solutions
