Numerical solution of fractional elliptic stochastic PDEs with spatial white noise
Provides a rigorous numerical framework for a class of non-local stochastic PDEs, relevant for applications in physics and finance.
The paper develops a numerical method for solving fractional elliptic stochastic PDEs with spatial white noise, achieving strong mean-square convergence with an explicit rate. Numerical experiments in 1D, 2D, and 3D confirm the theoretical results.
The numerical approximation of solutions to stochastic partial differential equations with additive spatial white noise on bounded domains in $\mathbb{R}^d$ is considered. The differential operator is given by the fractional power $L^β$, $β\in(0,1)$, of an integer order elliptic differential operator $L$ and is therefore non-local. Its inverse $L^{-β}$ is represented by a Bochner integral from the Dunford-Taylor functional calculus. By applying a quadrature formula to this integral representation, the inverse fractional power operator $L^{-β}$ is approximated by a weighted sum of non-fractional resolvents $(I + t_j^2 L)^{-1}$ at certain quadrature nodes $t_j>0$. The resolvents are then discretized in space by a standard finite element method. This approach is combined with an approximation of the white noise, which is based only on the mass matrix of the finite element discretization. In this way, an efficient numerical algorithm for computing samples of the approximate solution is obtained. For the resulting approximation, the strong mean-square error is analyzed and an explicit rate of convergence is derived. Numerical experiments for $L=κ^2-Δ$, $κ> 0$, with homogeneous Dirichlet boundary conditions on the unit cube $(0,1)^d$ in $d=1,2,3$ spatial dimensions for varying $β\in(0,1)$ attest the theoretical results.