Growth rates for the Hölder coefficients of the linear stochastic fractional heat equation with rough dependence in space

Fuente: arXiv
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Main Authors: Liu, Chang, Qian, Bin, Wang, Ran
Format: Preprint
Published: 2025
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author Liu, Chang
Qian, Bin
Wang, Ran
author_facet Liu, Chang
Qian, Bin
Wang, Ran
contents We study the linear stochastic fractional heat equation $$ \frac{\partial}{\partial t}u(t,x)=-(-Δ)^{\fracα2}u (t,x)+\dot{W}(t,x),\ \ t> 0,\ \ x\in\RR, $$ where $-(-Δ)^{\fracα{2}}$ denotes the fractional Laplacian with power $α\in (1, 2)$, and the driving noise $\dot W$ is a centered Gaussian field which is white in time and has the covariance of a fractional Brownian motion with Hurst parameter $H\in\left(\frac {2-α}2,\frac 12\right)$. We establish exact asymptotics for the solution as both time and space variables tend to infinity and derive sharp growth rates for the Hölder coefficients. The proofs are based on Talagrand's majorizing measure theorem and Sudakov's minoration theorem.
format Preprint
id arxiv_https___arxiv_org_abs_2507_22379
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Growth rates for the Hölder coefficients of the linear stochastic fractional heat equation with rough dependence in space
Liu, Chang
Qian, Bin
Wang, Ran
Probability
60H15, 60G17, 60G22
We study the linear stochastic fractional heat equation $$ \frac{\partial}{\partial t}u(t,x)=-(-Δ)^{\fracα2}u (t,x)+\dot{W}(t,x),\ \ t> 0,\ \ x\in\RR, $$ where $-(-Δ)^{\fracα{2}}$ denotes the fractional Laplacian with power $α\in (1, 2)$, and the driving noise $\dot W$ is a centered Gaussian field which is white in time and has the covariance of a fractional Brownian motion with Hurst parameter $H\in\left(\frac {2-α}2,\frac 12\right)$. We establish exact asymptotics for the solution as both time and space variables tend to infinity and derive sharp growth rates for the Hölder coefficients. The proofs are based on Talagrand's majorizing measure theorem and Sudakov's minoration theorem.
title Growth rates for the Hölder coefficients of the linear stochastic fractional heat equation with rough dependence in space
topic Probability
60H15, 60G17, 60G22
url https://arxiv.org/abs/2507.22379