Regularity theory for a new class of fractional parabolic stochastic evolution equations

preprint2023arXivOpen access

Abstract

A new class of fractional-order stochastic evolution equations of the form (∂t+A)γX(t)=W˙Q(t)(\partial_t + A)^γX(t) = \dot{W}^Q(t), t∈[0,T]t\in[0,T], γ∈(0,∞)γ\in (0,\infty), is introduced, where −A-A generates a C0C_0-semigroup on a separable Hilbert space HH and the spatiotemporal driving noise W˙Q\dot{W}^Q is the formal time derivative of an HH-valued cylindrical QQ-Wiener process. Mild and weak solutions are defined; these concepts are shown to be equivalent and to lead to well-posed problems. Temporal and spatial regularity of the solution process XX are investigated, the former being measured by mean-square or pathwise smoothness and the latter by using domains of fractional powers of AA. In addition, the covariance of XX and its long-time behavior are analyzed. These abstract results are applied to the cases when A:=LβA := L^β and Q:=L~−αQ:=\tilde{L}^{-α} are fractional powers of symmetric, strongly elliptic second-order differential operators defined on (i) bounded Euclidean domains or (ii) smooth, compact surfaces. In these cases, the Gaussian solution processes can be seen as generalizations of merely spatial (Whittle-)Matérn fields to space-time.

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