Global well-posedness for hyperbolic SPDEs with non-Lipschitz coefficients driven by space-time Lévy white noise

Fuente: arXiv
Salvato in:
Dettagli Bibliografici
Autori principali: Balan, Raluca M., Jiménez, Juan J., Quer-Sardanyons, Lluís
Natura: Preprint
Pubblicazione: 2025
Soggetti:
Accesso online:
Tags: Aggiungi Tag
Nessun Tag, puoi essere il primo ad aggiungerne!!
_version_ 1866908707990798336
author Balan, Raluca M.
Jiménez, Juan J.
Quer-Sardanyons, Lluís
author_facet Balan, Raluca M.
Jiménez, Juan J.
Quer-Sardanyons, Lluís
contents In this article, we study the global well-posedness of hyperbolic SPDEs on a bounded domain in $\mathbb{R}^d$, driven by a space-time Lévy white noise, when the drift and diffusion coefficients are locally Lipschitz and have linear growth. The equations are driven by two types of space-time Lévy noise: (i) a finite-variance Lévy white noise; or (ii) a symmetric Lévy basis that may have infinite variance. A typical example of noise of the second type is the symmetric $α$-stable (S$α$S) random measure with $α\in (0,2)$.
format Preprint
id arxiv_https___arxiv_org_abs_2511_23420
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Global well-posedness for hyperbolic SPDEs with non-Lipschitz coefficients driven by space-time Lévy white noise
Balan, Raluca M.
Jiménez, Juan J.
Quer-Sardanyons, Lluís
Probability
Primary 60H15, Secondary: 60G60, 60G51, 60G52
In this article, we study the global well-posedness of hyperbolic SPDEs on a bounded domain in $\mathbb{R}^d$, driven by a space-time Lévy white noise, when the drift and diffusion coefficients are locally Lipschitz and have linear growth. The equations are driven by two types of space-time Lévy noise: (i) a finite-variance Lévy white noise; or (ii) a symmetric Lévy basis that may have infinite variance. A typical example of noise of the second type is the symmetric $α$-stable (S$α$S) random measure with $α\in (0,2)$.
title Global well-posedness for hyperbolic SPDEs with non-Lipschitz coefficients driven by space-time Lévy white noise
topic Probability
Primary 60H15, Secondary: 60G60, 60G51, 60G52
url https://arxiv.org/abs/2511.23420