$\mathcal{H}$-inverses for RBF interpolation
Niklas Angleitner, Markus Faustmann, Jens Markus Melenk
TL;DR
This paper establishes that for RBF interpolation with kernels including polyharmonic splines, the inverse interpolation matrix admits an $\mathcal{H}$-matrix approximation with exponential convergence in block rank when the block partition follows standard clustering. The authors develop a function-level reduction via a native space framework, define localized harmonic spaces $V_{\mathrm{harm}}(B)$, and construct low-rank, localized operators (cut-off, $\Pi_H$, and coarsening) to approximate the inverse blocks. The key theoretical contribution is a bound of the form $\|\boldsymbol{S_{11}}-\boldsymbol{M}\|_2 \lesssim \ln(N) N^{\sigma_{\mathrm{card}}(3k-d)/d} \exp(-\sigma_{\mathrm{exp}} r^{1/(d+1)})$, underpinning log-linear storage and fast arithmetic in $\mathcal{H}$-matrix format. Numerical experiments in 2D/3D confirm the exponential decay of block approximations and illustrate practical gains for large nonuniform point clouds and various kernels, including Matérn-like and Bessel-potential variants.
Abstract
We consider the interpolation problem for a class of radial basis functions (RBFs) that includes the classical polyharmonic splines (PHS). We show that the inverse of the system matrix for this interpolation problem can be approximated at an exponential rate in the block rank in the $\mathcal{H}$-matrix format if the block structure of the $\mathcal{H}$-matrix arises from a standard clustering algorithm.
