Abstract
We investigate the growth of the tallest peaks of random field solutions to the parabolic Anderson models over concentric balls as the radii approach infinity. The noise is white in time and correlated in space. The spatial correlation function is either bounded or non-negative satisfying Dalang’s condition. The initial data are Borel measures with compact supports, in particular, include Dirac masses. The results obtained are related to those of Conus et al. (Ann Probab 41(3B):2225–2260, 2013) and Chen (Ann Probab 44(2):1535–1598, 2016) where constant initial data are considered.
Original language | English |
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Pages (from-to) | 495-539 |
Number of pages | 45 |
Journal | Stochastics and Partial Differential Equations: Analysis and Computations |
Volume | 7 |
Issue number | 3 |
Early online date | 2 Mar 2019 |
DOIs | |
Publication status | Published - 15 Sept 2019 |
Keywords
- Parabolic Anderson model
- Feynman–Kac representation ·
- Brownian motion
- Spatial asymptotic