We present DeepVoid, an application of deep learning trained on a physical definition of cosmic voids to detect voids in density fields and galaxy distributions. By semantically segmenting the IllustrisTNG simulation volume using the tidal tensor, we train a deep convolutional neural network to classify local structure using a U-Net architecture for training and prediction. The model achieves a void F1 score of 0.96 and a Matthews correlation coefficient over all structural classes of 0.81 for dark matter particles in IllustrisTNG with interparticle spacing of λ=0.33h−1Mpc. We then apply the machine learning technique of curricular learning to enable the model to classify structure in data with significantly larger intertracer separation. At the highest tracer separation tested, λ=10h−1Mpc, the model achieves a void F1 score of 0.89 and a Matthews correlation coefficient of 0.6 on IllustrisTNG subhalos.
@article{arxiv.2504.21134,
title = {DeepVoid: A Deep Learning Void Detector},
author = {Sam Kumagai and Michael S. Vogeley and Miguel A. Aragon-Calvo and Kelly A. Douglass and Segev BenZvi and Mark Neyrinck},
journal= {arXiv preprint arXiv:2504.21134},
year = {2026}
}
Comments
23 pages, 9 figures. Submitted to the Astrophysical Journal on 4/25/25. Accepted on 12/11/2025. Published on 02/04/2026