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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 16.

A time series of the dimensionless magnetic flux crossing the event horizon for all of the models in v3. Left column: MAD; right column: SANE simulations. Rows (from top to bottom): increasing spin from a* = −15/16 to a* = +15/16. The gray line plots the flux as computed according to Equation (12), while the gold and magenta lines plot ﹩{{\rm{\Phi }}}_{\rm{BH}\,}^{\,\rm{N}}﹩ (Equation (A1)) and ﹩{{\rm{\Phi }}}_{\rm{BH}\,}^{\,\rm{S}}﹩ (Equation (A2)), respectively.

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