Constraining cosmic ray transport models using circumgalactic medium properties and observables

TL;DR

This study uses FIRE-2 simulations to analyze how cosmic ray transport models affect circumgalactic medium properties, aiming to better constrain CR physics through synthetic observations and comparison with real data.

Contribution

It compares different CR transport models in galaxy simulations to assess their impact on CGM properties and observables, providing a framework for future constraints.

Findings

CRs influence galaxy mass and star formation rates

CRs increase cool CGM gas and ion column densities

X-ray emission is consistent with thermal and inverse Compton processes

Abstract

Cosmic rays (CRs) are a pivotal non-thermal component of galaxy formation and evolution. However, the intricacies of CR physics, particularly how they propagate in the circumgalactic medium (CGM), remain largely unconstrained. In this work, we study CGM properties in FIRE-2 (Feedback In Realistic Environments) simulations of the same Milky Way (MW)-mass halo at $z=0$ with different CR transport models that produce similar diffuse $\sim$ GeV $\gamma$-ray emission, as an attempt to further constrain CR transport models. We study the gas morphology and thermal properties, and generate synthetic observations of rest-frame UV ion absorption columns and X-ray emission. CRs lower galaxy masses and star formation rates (SFRs) while supporting more cool CGM gas, which boosts the HI and OVI column densities in the CGM, bringing simulations more in line with observations, but there can be large differences between CR transport models and resolution levels. X-ray emission within and close to galaxies is consistent with thermal (free-free and metal-line) emission plus X-ray binaries, while more extended ($\sim 100\,$kpc) CGM emission is potentially dominated by inverse Compton (IC) scattering, motivating future work on the spatially resolved X-ray profiles. Although comparisons with observations are sensitive to sample selection and mimicking the details of observations, and our analysis did not result in strong constraints on CR models, the differences between simulations are significant and could be used as a framework for future studies.