MINOT: Modeling the intracluster medium (non-)thermal content and observable prediction tools
R. Adam, H. Goksu, A. Leing\"artner-Goth, S. Ettori, R. Gnatyk, B., Hnatyk, M. H\"utten, J. P\'erez-Romero, M. A. S\'anchez-Conde, O. Sergijenko

TL;DR
MINOT is a comprehensive modeling framework that integrates thermal and nonthermal components of galaxy clusters to predict multiwavelength observables, aiding the understanding of cosmic-ray physics and magnetic fields.
Contribution
This work introduces MINOT, a self-consistent, publicly available tool for modeling the intracluster medium's thermal and nonthermal emissions across multiple wavelengths.
Findings
Successfully modeled clusters A1795, A2142, and A2255.
Predicted observables align with existing literature data.
Demonstrated versatility across radio, millimeter, X-ray, and gamma-ray bands.
Abstract
In the past decade, the observations of diffuse radio synchrotron emission toward galaxy clusters revealed cosmic-ray (CR) electrons and magnetic fields on megaparsec scales. However, their origin remains poorly understood, and several models have been discussed in the literature. CR protons are also expected to accumulate during the formation of clusters and probably contribute to the production of these high-energy electrons. In order to understand the physics of CRs in clusters, combining of observations at various wavelengths is particularly relevant. The exploitation of such data requires using a self-consistent approach including both the thermal and the nonthermal components, so that it is capable of predicting observables associated with the multiwavelength probes at play, in particular in the radio, millimeter, X-ray, and gamma-ray bands. We develop and describe such a…
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