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Scattering Spectra Models for Physics

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arxiv 2306.17210 v2 pith:JFMLYGTJ submitted 2023-06-29 physics.data-an astro-ph.IMcs.CVcs.LG

classification physics.data-anastro-ph.IMcs.CVcs.LG
keywords modelsfieldsscatteringfieldspectraencounteredinferencenumber
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Physicists routinely need probabilistic models for a number of tasks such as parameter inference or the generation of new realizations of a field. Establishing such models for highly non-Gaussian fields is a challenge, especially when the number of samples is limited. In this paper, we introduce scattering spectra models for stationary fields and we show that they provide accurate and robust statistical descriptions of a wide range of fields encountered in physics. These models are based on covariances of scattering coefficients, i.e. wavelet decomposition of a field coupled with a point-wise modulus. After introducing useful dimension reductions taking advantage of the regularity of a field under rotation and scaling, we validate these models on various multi-scale physical fields and demonstrate that they reproduce standard statistics, including spatial moments up to 4th order. These scattering spectra provide us with a low-dimensional structured representation that captures key properties encountered in a wide range of physical fields. These generic models can be used for data exploration, classification, parameter inference, symmetry detection, and component separation.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Multi-branch classification of diffuse cluster radio emission

    astro-ph.CO 2026-07 conditional novelty 5.0 of 10

    DualSSN (scattering + SE dual-branch) with beam-normalised cropping and mild uv-tapering reaches ~0.86 accuracy (top-5 ensemble 0.94) on LoTSS-DR2/PSZ2 diffuse-emission labels, beating simple CNNs and fixed FoV/pixel crops.

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