CosmoFlow: Scale-Aware Representation Learning for Cosmology with Flow Matching
On the map: Diffusion models → Inverse problems and image restoration
Abstract (arXiv)
Generative machine learning models have been demonstrated to be able to learn low dimensional representations of data that preserve information required for downstream tasks. In this work, we demonstrate that flow matching based generative models can learn compact, semantically rich latent representations of field level cold dark matter (CDM) simulation data without supervision. Our model, CosmoFlow, learns representations 32x smaller than the raw field data, usable for field level reconstruction, synthetic data generation, and parameter inference. Our model also learns interpretable representations, in which different latent channels correspond to features at different cosmological scales.
Key facts. No citing papers in the map yet (data through 14 Oct 2026). Placed in Inverse problems and image restoration, one of 14 directions in Diffusion models. Builds on 13 of its 20 references that are in the map. First posted on arXiv 16 Jul 2025.
Builds on
13 of 20 references.
References · 13
- 2020Denoising Diffusion Implicit Modelscited by 9,781
- 2020Score-Based Generative Modeling through Stochastic Differential Equationscited by 9,122
- 2022Flow Matching for Generative Modelingcited by 5,702
- 2013Auto-Encoding Variational Bayescited by 4,053
- 2017Decoupled Weight Decay Regularizationcited by 1,831
- 2023Stochastic Interpolants: A Unifying Framework for Flows and Diffusionscited by 939
- 2018Variational image compression with a scale hyperpriorcited by 935
- 2016End-to-end Optimized Image Compressioncited by 696
- 2024Flow Matching Guide and Codecited by 301
- 2023SODA: Bottleneck Diffusion Models for Representation Learningcited by 77
- 2024Exploring Diffusion Time-steps for Unsupervised Representation Learningcited by 36
- 2021Multifield Cosmology with Artificial Intelligencecited by 12
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- 2026Cosmo3DFlow: Wavelet Flow Matching for Spatial-to-Spectral Compression in Reconstructing the Early Universe
- 2025Conditional Diffusion-Flow models for generating 3D cosmic density fields: applications to f(R) cosmologies
- 2026Uncovering Physical Drivers of Dark Matter Halo Structures with Auxiliary-Variable-Guided Generative Models
- 2024Using Galaxy Evolution as Source of Physics-Based Ground Truth for Generative Models
- 2025Efficient Flow Matching using Latent Variables
- 2026Zero-Flow Encoders
- 2024Diffusion-HMC: Parameter Inference with Diffusion-model-driven Hamiltonian Monte Carlo
- 2023Cosmological Field Emulation and Parameter Inference with Diffusion Models