2017
DOI: 10.1007/s40072-017-0099-0
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Large time asymptotics for the parabolic Anderson model driven by space and time correlated noise

Abstract: We consider the linear stochastic heat equation on R ℓ , driven by a Gaussian noise which is colored in time and space. The spatial covariance satisfies general assumptions and includes examples such as the Riesz kernel in any dimension and the covariance of the fractional Brownian motion with Hurst parameter H ∈ ( 1 4 , 1 2 ] in dimension one. First we establish the existence of a unique mild solution and we derive a Feynman-Kac formula for its moments using a family of independent Brownian bridges and assumi… Show more

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Cited by 26 publications
(23 citation statements)
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“…There is also a literature on well-posedness and regularity theory for (1.1) when f is a distribution that is not necessarily in M + (R d ), though such results tend to be applicable in a more specialized setting as compared with the theory of Dalang [19]; see for example [13,11,30,31,32]. Henceforth, we consider the case that f is a nonnegative-definite, but possibly signed, function of the form, f = h * h, (1.8) where h : R d → R has enough regularity to ensure among other things that the convolution in (1.8) is well defined, and h(x) := h(−x) defines the reflection of h. In this case, (1.2) is equivalent to the elegant formula…”
Section: Introductionmentioning
confidence: 99%
“…There is also a literature on well-posedness and regularity theory for (1.1) when f is a distribution that is not necessarily in M + (R d ), though such results tend to be applicable in a more specialized setting as compared with the theory of Dalang [19]; see for example [13,11,30,31,32]. Henceforth, we consider the case that f is a nonnegative-definite, but possibly signed, function of the form, f = h * h, (1.8) where h : R d → R has enough regularity to ensure among other things that the convolution in (1.8) is well defined, and h(x) := h(−x) defines the reflection of h. In this case, (1.2) is equivalent to the elegant formula…”
Section: Introductionmentioning
confidence: 99%
“…An important ingredient to prove Proposition 1.2 is the following Feynman-Kac formula for the moments of the solution. In the case (H1), this formula is essentially a reformulation of Corollary 4.4 in Huang et al (2017a) and the result for (H2) is new, so we provide in Section 6 a unified proof for both cases.…”
Section: Introductionmentioning
confidence: 93%
“…. > s σ(n) > 0; we refer readers to Hu et al (2015); Huang et al (2017a); Song et al (2020) for the rigorous derivation of (2.3).…”
Section: Mild Solution Now We Definementioning
confidence: 99%
“…Since the obstacles are drawn according to a renewal process, our work provides an exemple of localization in a correlated disordered environment. Influence of spatial correlations has been investigated in other contexts such as localization of directed polymers with space-time noise [28], Brownian motion in correlated Poisson potential [29,30,36] as well as Anderson localization, both by mathematicians [25,26,31] and physicists [2,13,43]. In our model however, the extreme value statistics are more relevant than the correlation structure itself.…”
Section: Introductionmentioning
confidence: 99%