Radiative cooling in two-temperature GRMHD simulations for M87* produces cooler inner disks, dimmer disks, brighter and more extended jets, and lower total flux at 230 GHz compared to non-cooling models.
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Flux eruptions in MADs enhance non-axisymmetry near the black hole via m=1 and m=2 modes driven by vertical magnetic flux bundles formed through reconnection and expelled by buoyancy.
citing papers explorer
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Impacts of radiative cooling on the images of a black hole shadow and extended jets in two-temperature GRMHD simulations
Radiative cooling in two-temperature GRMHD simulations for M87* produces cooler inner disks, dimmer disks, brighter and more extended jets, and lower total flux at 230 GHz compared to non-cooling models.
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The azimuthal structure of magnetically arrested disks during flux eruption events
Flux eruptions in MADs enhance non-axisymmetry near the black hole via m=1 and m=2 modes driven by vertical magnetic flux bundles formed through reconnection and expelled by buoyancy.