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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 2.

Time series of the horizon-penetrating fluxes for six models: a* = { −15/16, 0, +15/16}, MAD and SANE. Left column: MAD simulations. Right column: SANE simulations. Top row: rest-mass accretion rate. Second row: dimensionless magnetic flux. Third row: normalized, absolute angular momentum flux. Bottom row: normalized absolute energy flux with the contribution from rest mass subtracted. a* = −15/16 simulations are plotted in indigo, a* = 0 simulations in crimson, and a* = +15/16 in gold.

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