Galactic Alchemy: Deep Learning Map-to-Map Translation in Hydrodynamical Simulations

Fuente: arXiv
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Autori principali: Denzel, Philipp, Billeter, Yann, Schilling, Frank-Peter, Gavagnin, Elena
Natura: Preprint
Pubblicazione: 2025
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author Denzel, Philipp
Billeter, Yann
Schilling, Frank-Peter
Gavagnin, Elena
author_facet Denzel, Philipp
Billeter, Yann
Schilling, Frank-Peter
Gavagnin, Elena
contents We present the first systematic study of multi-domain map-to-map translation in galaxy formation simulations, leveraging deep generative models to predict diverse galactic properties. Using high-resolution magneto-hydrodynamical simulation data, we compare conditional generative adversarial networks and diffusion models under unified preprocessing and evaluation, optimizing architectures and attention mechanisms for physical fidelity on galactic scales. Our approach jointly addresses seven astrophysical domains - including dark matter, gas, neutral hydrogen, stellar mass, temperature, and magnetic field strength - while introducing physics-aware evaluation metrics that quantify structural realism beyond standard computer vision measures. We demonstrate that translation difficulty correlates with physical coupling, achieving near-perfect fidelity for mappings from gas to dark matter and mappings involving astro-chemical components such as total gas to HI content, while identifying fundamental challenges in weakly constrained tasks such as gas to stellar mass mappings. Our results establish GAN-based models as competitive counterparts to state-of-the-art diffusion approaches at a fraction of the computational cost (in training and inference), paving the way for scalable, physics-aware generative frameworks for forward modelling and observational reconstruction in the SKA era.
format Preprint
id arxiv_https___arxiv_org_abs_2510_23768
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Galactic Alchemy: Deep Learning Map-to-Map Translation in Hydrodynamical Simulations
Denzel, Philipp
Billeter, Yann
Schilling, Frank-Peter
Gavagnin, Elena
Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
We present the first systematic study of multi-domain map-to-map translation in galaxy formation simulations, leveraging deep generative models to predict diverse galactic properties. Using high-resolution magneto-hydrodynamical simulation data, we compare conditional generative adversarial networks and diffusion models under unified preprocessing and evaluation, optimizing architectures and attention mechanisms for physical fidelity on galactic scales. Our approach jointly addresses seven astrophysical domains - including dark matter, gas, neutral hydrogen, stellar mass, temperature, and magnetic field strength - while introducing physics-aware evaluation metrics that quantify structural realism beyond standard computer vision measures. We demonstrate that translation difficulty correlates with physical coupling, achieving near-perfect fidelity for mappings from gas to dark matter and mappings involving astro-chemical components such as total gas to HI content, while identifying fundamental challenges in weakly constrained tasks such as gas to stellar mass mappings. Our results establish GAN-based models as competitive counterparts to state-of-the-art diffusion approaches at a fraction of the computational cost (in training and inference), paving the way for scalable, physics-aware generative frameworks for forward modelling and observational reconstruction in the SKA era.
title Galactic Alchemy: Deep Learning Map-to-Map Translation in Hydrodynamical Simulations
topic Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2510.23768