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Using diffusion models for cosmological parameter inference

Published on:

8 May 2024

Primary Category:

Cosmology and Nongalactic Astrophysics

Paper Authors:

Nayantara Mudur,

Carolina Cuesta-Lazaro,

Douglas P. Finkbeiner

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Key Details

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

AI generated summary

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.

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