Stability of travelling wave solutions to reaction-diffusion equations driven by additive noise with Hölder continuous paths
Amjad Saef, Wilhelm Stannat
TL;DR
The paper analyzes the stability of travelling wave solutions to reaction-diffusion equations under infinite-dimensional additive noise with Hölder paths, including self-similar drivers like fractional Brownian motion. It develops a pathwise, phase-adaptive framework that decomposes perturbations into a first-order stochastic component and a nonlinear residual, leveraging a dissipative linearisation and Young integration against sectorial operators. The authors derive short- and long-time error bounds for the distance to the travelling-wave orbit, revealing how stability depends on the noise’s Hurst index and Hölder regularity, and they extend the results to self-similar, possibly non-Gaussian drivers with explicit tail estimates. This framework provides quantitative, pathwise stability results that can be applied to a broad class of infinite-dimensional noise processes, with potential implications for modelling noise-driven front propagation in biological systems and other spatiotemporal phenomena.
Abstract
In this paper we investigate stability of travelling wave solutions to a class of reaction-diffusion equations perturbed by infinite-dimensional additive noise with Hölder continuous paths, covering in particular fractional Brownian motion with general Hurst index. We obtain long- and short time asymptotic error bounds on the maximal distance from the solution of the stochastic reaction-diffusion equation to the orbit of travelling wave fronts. These bounds, in terms of Hurst index and Hölder exponent, apply to a large class of infinite-dimensional self-similar drivers with Hölder continuous paths, such as linear fractional stable motion. We find that for short times, higher Hurst indices imply higher stability, while for large times, a smaller gap between Hurst index and Hölder exponent implies stability for larger noise amplitudes.
