Self-regulating AGN jets in MHD simulations of cool-core clusters yield realistic FRI radio morphologies viewed along the jet axis and account for frequency-independent lobe extents via 1-50 μG fields allowing both young and old electrons to radiate.
arXiv preprint arXiv:2510.15634 , year=
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Numerical simulations predict gamma-ray and neutrino fluxes from three nearby galaxy clusters that fall below existing observational upper limits.
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Simulating realistic radio morphologies of Fanaroff-Riley I jets in a self-regulating cool-core cluster
Self-regulating AGN jets in MHD simulations of cool-core clusters yield realistic FRI radio morphologies viewed along the jet axis and account for frequency-independent lobe extents via 1-50 μG fields allowing both young and old electrons to radiate.
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High-energy Multi-messenger Emission from Galaxy Clusters in the Local Universe
Numerical simulations predict gamma-ray and neutrino fluxes from three nearby galaxy clusters that fall below existing observational upper limits.