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A Survey of General Relativistic Magnetohydrodynamic Models for Black Hole Accretion Systems

  • Authors: Vedant Dhruv, Cora Prather, George N. Wong, Charles F. Gammie

Vedant Dhruv et al 2025 The Astrophysical Journal Supplement Series 277 .

  • Provider: AAS Journals

Caption: Figure 4.

Similar to Figure 3 but now plotting the contribution of various components of the fluxes (see Equations (15), (16), (17), (18), (19), and (20)). We see that magnetic fields have little-to-no contribution toward ﹩\dot{L}﹩ and ﹩\dot{E}﹩ in the SANE models. In the MAD models, the trend in total flux closely matches the trend observed in the electromagnetic components.

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