Strong and weak rates of convergence in the Smoluchowski--Kramers approximation for stochastic partial differential equations

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Hauptverfasser: Bréhier, Charles-Edouard, Lei, Ziyi
Format: Preprint
Veröffentlicht: 2026
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author Bréhier, Charles-Edouard
Lei, Ziyi
author_facet Bréhier, Charles-Edouard
Lei, Ziyi
contents We consider a class of stochastic damped semilinear wave equations, in the small-mass limit. It has previously been established that the solution converges to the solution of a stochastic semilinear heat equation. In this work we exhibit strong and weak rates of convergence in this Smoluchowski--Kramers approximation result. The rates depend on the regularity of the driving Wiener process. For instance, for trace-class noise the strong and weak rates of convergence are $1$, whereas for space-time white noise (in dimension $1$) the strong and weak rates of convergence are $1/2$ and $1$ respectively.
format Preprint
id arxiv_https___arxiv_org_abs_2604_14752
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Strong and weak rates of convergence in the Smoluchowski--Kramers approximation for stochastic partial differential equations
Bréhier, Charles-Edouard
Lei, Ziyi
Probability
Analysis of PDEs
We consider a class of stochastic damped semilinear wave equations, in the small-mass limit. It has previously been established that the solution converges to the solution of a stochastic semilinear heat equation. In this work we exhibit strong and weak rates of convergence in this Smoluchowski--Kramers approximation result. The rates depend on the regularity of the driving Wiener process. For instance, for trace-class noise the strong and weak rates of convergence are $1$, whereas for space-time white noise (in dimension $1$) the strong and weak rates of convergence are $1/2$ and $1$ respectively.
title Strong and weak rates of convergence in the Smoluchowski--Kramers approximation for stochastic partial differential equations
topic Probability
Analysis of PDEs
url https://arxiv.org/abs/2604.14752