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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 6.

Power spectrum of the MAD parameters in the time interval 104 t g < t < 2 × 104 t g (1.5 × 104 t g to 2.5 × 104 t g for aM94b800). In all simulations, the power is concentrated in the low-frequency region, which corresponds to periods about 500–2000t g . In the high-frequency region, the power spectrum decreases following ∼f −1. The dashed red line shows this evolution.

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