mlsanityData to 7 Oct 2026

An automated parameter domain decomposition approach for gravitational wave surrogates using hp-greedy refinement

arXiv 2212.08554 ↗First posted 16 Dec 2022gr-qc cs.LG math.RTcited by 1

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Abstract (arXiv)

We introduce hp-greedy, a refinement approach for building gravitational wave surrogates as an extension of the standard reduced basis framework. Our proposal is data-driven, with a domain decomposition of the parameter space, local reduced basis, and a binary tree as the resulting structure, which are obtained in an automated way. When compared to the standard global reduced basis approach, the numerical simulations of our proposal show three salient features: i) representations of lower dimension with no loss of accuracy, ii) a significantly higher accuracy for a fixed maximum dimensionality of the basis, in some cases by orders of magnitude, and iii) results that depend on the reduced basis seed choice used by the refinement algorithm. We first illustrate the key parts of our approach with a toy model and then present a more realistic use case of gravitational waves emitted by the collision of two spinning, non-precessing black holes. We discuss performance aspects of hp-greedy, such as overfitting with respect to the depth of the tree structure, and other hyperparameter dependences. As two direct applications of the proposed hp-greedy refinement, we envision: i) a further acceleration of statistical inference, which might be complementary to focused reduced-order quadratures, and ii) the search of gravitational waves through clustering and nearest neighbors.

Key facts. Cited by 1 paper in the map (data through 7 Oct 2026). Builds on 2 of its 45 references that are in the map. First posted on arXiv 16 Dec 2022.

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2 of 45 references.

References · 2

  1. 2013Fast prediction and evaluation of gravitational waveforms using surrogate modelscited by 9
  2. 2015Fast and accurate prediction of numerical relativity waveforms from binary black hole coalescences using surrogate modelscited by 2

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