The picasso gas model: Painting intracluster gas on gravity-only simulations
F. K\'eruzor\'e, L. E. Bleem, N. Frontiere, N. Krishnan, M. Buehlmann,, J.D. Emberson, S. Habib, P. Larsen

TL;DR
The paper introduces 'picasso', a model that predicts intracluster gas properties from gravity-only simulations using analytical and machine learning techniques, achieving high accuracy and efficiency.
Contribution
It presents a novel hybrid model combining analytical and machine learning methods to predict intracluster medium thermodynamics from gravity-only simulations.
Findings
Achieves percent-level bias and ~20% scatter in predictions.
Can be trained on minimal halo information with modest accuracy loss.
Provides a publicly available Python package for easy application.
Abstract
We introduce picasso, a model designed to predict thermodynamic properties of the intracluster medium based on the properties of halos in gravity-only simulations. The predictions result from the combination of an analytical gas model, mapping gas properties to the gravitational potential, and of a machine learning model to predict the model parameters for individual halos based on their scalar properties, such as mass and concentration. Once trained, the model can be applied to make predictions for arbitrary potential distributions, allowing its use with flexible inputs such as N-body particle distributions or radial profiles. We present the model, and train it using pairs of gravity-only and hydrodynamic simulations. We show that when trained to learn the mapping from gravity-only to non-radiative hydrodynamic simulations, picasso can make remarkably accurate and precise predictions…
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Taxonomy
TopicsComputer Graphics and Visualization Techniques
