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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 12.

The angular- and time-averaged gas pressure p (yellow) and magnetic pressure b 2 (blue) for aM94b100, a0b100, and a94b100. We further show each component of the magnetic pressure, b r 2 (red), ﹩{b}_{\theta }^{2}﹩ (green), and ﹩{b}_{\phi }^{2}﹩ (purple). These values are calculated by Equation (18) and are then time averaged. The dashed (light blue) curve represents the r −2 dependence.

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