Viscous torque in turbulent magnetized active galactic nucleus accretion disks and its effects on the gravitational waves of extreme mass ratio inspirals

Open Access

Fig. 12.

Density profile and magnetic field lines for the 2D-High case (left), the meridional slice at ϕ = 0 (middle), and the equatorial slice of the same quantities for the 3D simulation (right) at the final snapshot.

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