Bridging Simulations and EFT: A Hybrid Model of the Lyman-Alpha Forest Field

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Main Authors: de Belsunce, Roger, Hadzhiyska, Boryana, Ivanov, Mikhail M.
Format: Preprint
Published: 2025
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author de Belsunce, Roger
Hadzhiyska, Boryana
Ivanov, Mikhail M.
author_facet de Belsunce, Roger
Hadzhiyska, Boryana
Ivanov, Mikhail M.
contents The Lyman-alpha (Lya) forest is a unique probe of cosmology and the intergalactic medium at high redshift and small scales. The statistical power of the ongoing Dark Energy Spectroscopic Instrument (DESI) demands precise theoretical tools to model the Lya forest. We present a hybrid effective field theory (HEFT) forward model in redshift space that leverages the accuracy of non-linear particle displacements computed using the N-body simulation suite AbacusSummit with the predictive power of an analytical, perturbative bias forward model in the framework of the effective field theory (EFT). The residual noise between the model and the simulated Lya field has a nearly white (scale-and orientation-independent) power spectrum on quasi-linear scales, substantially simplifying its modeling compared to a purely perturbative description. As a consequence of the improved control over the 3D Lya forest stochasticity, we find agreement between the modeled and the true power spectra at the 5 per cent level down to scales of k <= 1 h/Mpc. This procedure offers a promising path toward constructing efficient and accurate emulators to predict large-scale clustering summary statistics for full-shape cosmological analyses of Lya forest data from both DESI and its successor, DESI-II.
format Preprint
id arxiv_https___arxiv_org_abs_2512_13681
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Bridging Simulations and EFT: A Hybrid Model of the Lyman-Alpha Forest Field
de Belsunce, Roger
Hadzhiyska, Boryana
Ivanov, Mikhail M.
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
The Lyman-alpha (Lya) forest is a unique probe of cosmology and the intergalactic medium at high redshift and small scales. The statistical power of the ongoing Dark Energy Spectroscopic Instrument (DESI) demands precise theoretical tools to model the Lya forest. We present a hybrid effective field theory (HEFT) forward model in redshift space that leverages the accuracy of non-linear particle displacements computed using the N-body simulation suite AbacusSummit with the predictive power of an analytical, perturbative bias forward model in the framework of the effective field theory (EFT). The residual noise between the model and the simulated Lya field has a nearly white (scale-and orientation-independent) power spectrum on quasi-linear scales, substantially simplifying its modeling compared to a purely perturbative description. As a consequence of the improved control over the 3D Lya forest stochasticity, we find agreement between the modeled and the true power spectra at the 5 per cent level down to scales of k <= 1 h/Mpc. This procedure offers a promising path toward constructing efficient and accurate emulators to predict large-scale clustering summary statistics for full-shape cosmological analyses of Lya forest data from both DESI and its successor, DESI-II.
title Bridging Simulations and EFT: A Hybrid Model of the Lyman-Alpha Forest Field
topic Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2512.13681