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A Study of the Accretion State of Magnetically Arrested Disks across Black Hole Spins for Radiatively Inefficient Accretion Flows

  • Authors: G.-Q. Zhang, Damien Bégué, A. Pe'er, B.-B. Zhang

G.-Q. Zhang et al 2024 The Astrophysical Journal 962 .

  • Provider: AAS Journals

Caption: Figure 14.

Radial angular momentum flux components ﹩{\dot{J}}^{r}﹩ as a function of the polar angle θ for a94b100 (top), a0b100 (middle), and aM94b100 (bottom) at three different radii, r = 10, 15, and 20r g . The solid blue line corresponds to the total radial flux ﹩{\dot{J}}_{\mathrm{total}}^{r}﹩, and the red and green dashed lines are for the advection ﹩{\dot{J}}_{\mathrm{adv}}^{r}﹩ and for the Maxwell stress ﹩{\dot{J}}_{\mathrm{stress},{\rm{M}}}^{r}﹩ contributions to the radial flux, respectively. Finally, the dotted purple line corresponds to the Reynolds stress contribution ﹩{\dot{J}}_{\mathrm{stress},{\rm{R}}}^{r}﹩.

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