On the stability and accuracy of the Empirical Interpolation Method and Gravitational Wave Surrogates
Manuel Tiglio, Aar\'on Villanueva

TL;DR
This paper analyzes the Empirical Interpolation Method's stability and accuracy in gravitational wave surrogate modeling, clarifies its node selection process, and introduces two optimized variants to improve conditioning and accuracy.
Contribution
It clarifies the node selection mechanism of the EIM in GW science and introduces two new EIM variants optimized for conditioning and Lebesgue constant.
Findings
Original EIM chooses nodes to maximize matrix invertibility
Two new EIM variants improve conditioning and Lebesgue constant
Numerical experiments compare EIM variants in GW surrogate models
Abstract
The combination of the Reduced Basis and the Empirical Interpolation Method (EIM) approaches have produced outstanding results in many disciplines. In particular, in gravitational wave (GW) science these results range from building non-intrusive surrogate models for GWs to fast parameter estimation adding the use of Reduced Order Quadratures. These surrogates have the salient feature of being essentially indistinguishable from or very close to supercomputer simulations of the Einstein equations, but can be evaluated in the order of a milisecond per multipole mode on a standard laptop. In this article we clarify a common misperception of the EIM as originally introduced and used in practice in GW science. Namely, we prove that the EIM at each iteration chooses the interpolation nodes so as to make the related Vandermonde-type matrix as invertible as possible; not necessarily optimizing…
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