数学物理学报(英文版) ›› 2019, Vol. 39 ›› Issue (3): 764-780.doi: 10.1007/s10473-019-0309-0

• 论文 • 上一篇    下一篇

JOINT HÖLDER CONTINUITY OF PARABOLIC ANDERSON MODEL

胡耀忠1, Khoa LÊ2   

  1. 1. Department of Mathematical and Statistical Sciences, University of Alberta, Edmonton, T6G 2G1, Canada;
    2. Department of Mathematics, South Kensington Campus, Imperial College London, London, SW7 2AZ, United Kingdom
  • 收稿日期:2018-03-04 修回日期:2019-03-03 出版日期:2019-06-25 发布日期:2019-06-27
  • 作者简介:Yaozhong HU,E-mail:yaozhong@ualberta.ca;Khoa LÊ,E-mail:n.le@imperial.ac.uk
  • 基金资助:
    Y. Hu is supported by an NSERC grant and a startup fund of University of Alberta; K. Lê is supported by Martin Hairer's Leverhulme Trust leadership award.

JOINT HÖLDER CONTINUITY OF PARABOLIC ANDERSON MODEL

Yaozhong HU1, Khoa LÊ2   

  1. 1. Department of Mathematical and Statistical Sciences, University of Alberta, Edmonton, T6G 2G1, Canada;
    2. Department of Mathematics, South Kensington Campus, Imperial College London, London, SW7 2AZ, United Kingdom
  • Received:2018-03-04 Revised:2019-03-03 Online:2019-06-25 Published:2019-06-27
  • Supported by:
    Y. Hu is supported by an NSERC grant and a startup fund of University of Alberta; K. Lê is supported by Martin Hairer's Leverhulme Trust leadership award.

摘要: We obtain the Holder continuity and joint Holder continuity in space and time for the random field solution to the parabolic Anderson equation (t-1/2△)u=uW in d-dimensional space, where W is a mean zero Gaussian noise with temporal covariance γ0 and spatial covariance given by a spectral density μ(ξ). We assume that γ0(t) ≤ c|t|-α0 and |μ(ξ)| ≤ c|ξi|-αi or |μ(ξ)| ≤ c|ξ|-α, where αi, i=1,…, d (or α) can take negative value.

关键词: Gaussian process, stochastic heat equation, parabolic Anderson model, multiplicative noise, chaos expansion, hypercontractivity, Hölder continuity, joint Hölder continuity

Abstract: We obtain the Holder continuity and joint Holder continuity in space and time for the random field solution to the parabolic Anderson equation (t-1/2△)u=uW in d-dimensional space, where W is a mean zero Gaussian noise with temporal covariance γ0 and spatial covariance given by a spectral density μ(ξ). We assume that γ0(t) ≤ c|t|-α0 and |μ(ξ)| ≤ c|ξi|-αi or |μ(ξ)| ≤ c|ξ|-α, where αi, i=1,…, d (or α) can take negative value.

Key words: Gaussian process, stochastic heat equation, parabolic Anderson model, multiplicative noise, chaos expansion, hypercontractivity, Hölder continuity, joint Hölder continuity

中图分类号: 

  • 60H15