The bias from hydrodynamic simulations: mapping baryon physics onto dark matter fields
Francesco Sinigaglia, Francisco-Shu Kitaura, Andr\'es, Balaguera-Antol\'inez, Kentaro Nagamine, Metin Ata, Ikkoh Shimizu, Manuel, S\'anchez-Benavente

TL;DR
This study demonstrates a method to accurately map baryon physics onto dark matter fields using hydrodynamic simulations, enabling efficient generation of mock data for large-scale structure surveys.
Contribution
It introduces a novel approach combining the Bias Assignment Method with non-local bias analysis to reconstruct baryon properties from dark matter fields with high precision.
Findings
Percent-precision in two-point statistics
Compatible three-point statistics within 1-sigma
Reduced computational time by 5-6 orders of magnitude
Abstract
This paper investigates the hierarchy of baryon physics assembly bias relations obtained from state-of-the-art hydrodynamic simulations with respect to the underlying cosmic web spanned by the dark matter field. Using the Bias Assignment Method (BAM) we find that non-local bias plays a central role. We classify the cosmic web based on the invariants of the curvature tensor defined not only by the gravitational potential, but especially by the over-density, as small scale clustering becomes important in this context. First, the gas density bias relation can be directly mapped onto the dark matter density field to high precision exploiting the strong correlation between them. In a second step, the neutral hydrogen is mapped based on the dark matter and the gas density fields. Finally, the temperature is mapped based on the previous quantities. This permits us to statistically reconstruct…
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