Intermittency fronts for space-time fractional stochastic partial differential equations in (d+1)(d+1) dimensions

preprint2016arXivOpen access

Abstract

We consider time fractional stochastic heat type equation ∂tβut(x)=−ν(−Δ)α/2ut(x)+It1−β[σ(u)W⋅(t,x)]\partial^β_tu_t(x)=-ν(-Δ)^{α/2} u_t(x)+I^{1-β}_t[σ(u)\stackrel{\cdot}{W}(t,x)] in (d+1)(d+1) dimensions, where ν>0ν>0, β∈(0,1)β\in (0,1), α∈(0,2]α\in (0,2], $d<\min\{2,β^{-1}\}\a$, ∂tβ\partial^β_t is the Caputo fractional derivative, −(−Δ)α/2-(-Δ)^{α/2} is the generator of an isotropic stable process, W⋅(t,x)\stackrel{\cdot}{W}(t,x) is space-time white noise, and $σ:\R \to\RR{R}$ is Lipschitz continuous. Mijena and Nane proved in \cite{JebesaAndNane1} that : (i) absolute moments of the solutions of this equation grows exponentially; and (ii) the distances to the origin of the farthest high peaks of those moments grow exactly linearly with time. The last result was proved under the assumptions α=2α=2 and d=1.d=1. In this paper we extend this result to the case α=2α=2 and d∈{1,2,3}.d\in\{1,2,3\}.

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