Provable Low-Rank Tensor-Train Approximations in the Inverse of Large-Scale Structured Matrices
Chuanfu Xiao, Kejun Tang, Zhitao Zhu
TL;DR
The paper addresses the challenge of representing and computing inverses of large-scale structured matrices arising from PDE discretizations in a TT format. It introduces a computable sufficient condition guaranteeing that the inverse admits a low-rank TT representation and develops a diagonalization-based TT inversion method using Hadamard inverses and an Expanding operator. Theoretical results show the Hadamard inverse of the diagonalized tensor exhibits a displacement structure, yielding exponential decay of singular values under verifiable conditions, and the method applies to Poisson, Boltzmann-BGK, and Fokker-Planck discretizations. Numerical experiments across 3D Poisson, Boltzmann-BGK, and high-dimensional Fokker-Planck problems validate the theory and demonstrate scalable accuracy and memory efficiency for large degrees of freedom.
Abstract
This paper studies the low-rank property of the inverse of a class of large-scale structured matrices in the tensor-train (TT) format, which is typically discretized from differential operators. An interesting question that we are concerned with is: Does the inverse of the large-scale structured matrix still admit the low-rank TT representation with guaranteed accuracy? In this paper, we provide a computationally verifiable sufficient condition such that the inverse matrix can be well approximated in a low-rank TT format. It not only answers what kind of structured matrix whose inverse has the low-rank TT representation but also motivates us to develop an efficient TT-based method to compute the inverse matrix. Furthermore, we prove that the inverse matrix indeed has the low-rank tensor format for a class of large-scale structured matrices induced by differential operators involved in several PDEs, such as the Poisson, Boltzmann, and Fokker-Planck equations. Thus, the proposed algorithm is suitable for solving these PDEs with massive degrees of freedom. Numerical results on the Poisson, Boltzmann, and Fokker-Planck equations validate the correctness of our theory and the advantages of our methodology.
