Accretion flows in galactic nuclei involve magnetized plasma, and it has been long known that magnetic fields strongly perturb the energetics (Shvartsman 1971

Testing the accuracy of our method by numerically stimulating hydrodynamic spherical bondi accretion.

The dominant outward energy transport mechanism is convection driven by magnetic reconnection in the magnetosphere near the BH.

To investigate the mechanism driving the turbulence, we explore the physics of the outward flow of energy.

The authors HC, RN, PN, KS, AR, and KC acknowledge support from the Gordon and Betty Moore Foundation and the John Templeton Foundation

If you want to continue learning about black holes, here's a list of all the references.

Find out the definitions of Hydrodynamic Simulation Setup and Magnetohydrodynamic Simulation Setup and how they pertain to black holes

Wrapping up our black hole study: a final rundown.