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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 1.

Azimuthal/poloidal slice of initial conditions along with the grid geometry. The color scale denotes the logarithm of the rest-mass density, and as an example, we plot the magnetic fields structure (in black) for a SANE disk. The grid zone boundaries are represented by the white mesh. The grid zones are concentrated toward the equatorial plane and at smaller radii, where we expect most of the relevant physics to occur.

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