PINION: physics-informed neural network for accelerating radiative transfer simulations for cosmic reionization

Author:

Korber Damien12ORCID,Bianco Michele1ORCID,Tolley Emma1ORCID,Kneib Jean-Paul1ORCID

Affiliation:

1. Institute of Physics, Laboratory of Astrophysics, École Polytechnique Fédérale de Lausanne (EPFL) , Chemin Pegasi 51, 1290 Sauverny, Switzerland

2. Observatoire de Genève, Université de Genève , Chemin Pegasi 51, 1290 Versoix, Switzerland

Abstract

ABSTRACTWith the advent of the Square Kilometre Array Observatory (SKAO), scientists will be able to directly observe the Epoch of Reionization by mapping the distribution of neutral hydrogen at different redshifts. While physically motivated results can be simulated with radiative transfer codes, these simulations are computationally expensive and cannot readily produce the required scale and resolution simultaneously. Here we introduce the Physics-Informed neural Network for reIONization (PINION), which can accurately and swiftly predict the complete 4D hydrogen fraction evolution from the smoothed gas and mass density fields from pre-computed N-body simulation. We trained PINION on the C2-Ray simulation outputs and a physics constraint on the reionization chemistry equation is enforced. With only five redshift snapshots, PINION can accurately predict the entire reionization history between z = 6 and 12. We evaluate the accuracy of our predictions by analyzing the dimensionless power spectra and morphology statistics estimations against C2-Ray results. We show that while the network’s predictions are in very good agreement with simulation to redshift z > 7, the network’s accuracy suffers for z < 7. We motivate how PINION performance could be improved using additional inputs and potentially generalized to large-scale simulations.

Funder

SNSF

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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