2025MNRAS.536..145J

We investigate the role of the SIMBA feedback model on the structure of the intragroup medium (IGrM) in the new HYENAS suite of cutting-edge cosmological zoom-in simulations. Using 34 high-resolution zooms of haloes spanning from $10^{13}-10^{14}$${\rm M_\odot}$ at $z=0.286$, we follow haloes for 700 Myr, over several major active galactic nuclei (AGNs) jet feedback events. We use the MOXHA package to generate mock Chandra X-ray observations, as well as predictive mocks for the upcoming LEM mission, identifying many feedback-generated features such as cavities, shock-fronts, and hot-spots, closely mimicking real observations. Our sample comprises 105 snapshots with identified cavities, 50 with single bubbles, and 55 with two, and spans three orders of magnitude in observed cavity enthalpies, from $10^{41}-10^{44}$ erg s^–1. Comparing semimajor axis length, midpoint radius, and eccentricity to a matched sample of observations, we find good agreement in cavity dimensions with real catalogues. We estimate cavity power from our mock maps following observational procedures, showing that this is typically more than enough to offset halo cooling, particularly in low-mass haloes, where we match the observed excess in energy relative to cooling. Bubble enthalpy as measured with the usual midpoint pressure typically exceeds the energy released by the most recent jet event, hinting that the mechanical work is done predominantly at a lower pressure against the IGrM. We demonstrate for the first time that X-ray cavities are observable in a modern large-scale simulation suite and discuss the use of realistic cavity mock observations as new halo-scale constraints on feedback models in cosmological simulations.