Published on:
8 May 2024
Primary Category:
Cosmology and Nongalactic Astrophysics
Paper Authors:
Nayantara Mudur,
Carolina Cuesta-Lazaro,
Douglas P. Finkbeiner
Trains diffusion model to emulate density fields conditional on cosmology
Uses model likelihood for accurate cosmology parameter inference
Demonstrates approach is more robust to noise than baseline methods
Model captures statistics of true distribution well
Constraints much tighter than from power spectrum alone
Using diffusion models for cosmological parameter inference
This paper trains a diffusion model to generate simulations of cosmic density fields based on input cosmological parameters. It then uses the model's likelihood estimate to infer those parameters from a given density field, showing this approach yields tight constraints and is robust to noise perturbations.
Learning representations of cosmological simulations
Removing Galactic Dust Contamination from Cosmic Microwave Background Maps
Predicting Radiation Feedback in Molecular Clouds
Modeling galaxy distributions with cosmic web environments
Modeling galaxies and dark matter with normalizing flows
Inferring galaxy cluster mass maps from mock images
No comments yet, be the first to start the conversation...
Sign up to comment on this paper