mlsanityData to 14 Oct 2026

Learnable wavelet neural networks for cosmological inference

arXiv 2307.14362 ↗First posted 24 Jul 2023astro-ph.IM astro-ph.CO cs.LGcited by 0

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Abstract (arXiv)

Convolutional neural networks (CNNs) have been shown to both extract more information than the traditional two-point statistics from cosmological fields, and marginalise over astrophysical effects extremely well. However, CNNs require large amounts of training data, which is potentially problematic in the domain of expensive cosmological simulations, and it is difficult to interpret the network. In this work we apply the learnable scattering transform, a kind of convolutional neural network that uses trainable wavelets as filters, to the problem of cosmological inference and marginalisation over astrophysical effects. We present two models based on the scattering transform, one constructed for performance, and one constructed for interpretability, and perform a comparison with a CNN. We find that scattering architectures are able to outperform a CNN, significantly in the case of small training data samples. Additionally we present a lightweight scattering network that is highly interpretable.

Key facts. No citing papers in the map yet (data through 14 Oct 2026). Builds on 7 of its 18 references that are in the map. First posted on arXiv 24 Jul 2023.

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7 of 18 references.

References · 7

  1. 2020Solving high-dimensional parameter inference: marginal posterior densities & Moment Networkscited by 22
  2. 2021The CAMELS Multifield Dataset: Learning the Universe's Fundamental Parameters with Artificial Intelligencecited by 18
  3. 2021Parametric Scattering Networkscited by 16
  4. 2021Multifield Cosmology with Artificial Intelligencecited by 12
  5. 2017Estimating Cosmological Parameters from the Dark Matter Distributioncited by 11
  6. 2018Non-Gaussian information from weak lensing data via deep learningcited by 11
  7. 2021Robust marginalization of baryonic effects for cosmological inference at the field levelcited by 6

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