Keywords: Cosmology, Point Cloud, Graph Neural Networks, Equivariant Neural Networks
TL;DR: We introduce an interface for benchmarking equivariant neural networks on galaxy clustering data and comparing them against non-equivariant and traditional cosmological methods.
Abstract: Efficiently processing structured point cloud data while preserving multiscale information is a key challenge across domains, from graphics to atomistic modeling. Using a curated dataset of simulated galaxies, represented as a point cloud, we benchmark the ability of graph neural networks to simultaneously capture local clustering environments and long-range correlations. Given the homogeneous and isotropic nature of the Universe, the data exhibits a high degree of symmetry. We thus focus on evaluating the performance of Euclidean symmetry-preserving ($E(3)$-equivariant) graph neural networks, showing that they can outperform non-equivariant counterparts and domain-specific information extraction techniques in downstream performance as well as simulation-efficiency.
Submission Type: Extended abstract (max 4 main pages).
Software: https://github.com/smsharma/eqnn-jax/
Poster: jpg
Poster Preview: jpg
Submission Number: 131
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