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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 21.

Similar to Figure 20, but for SANE a* = +0.5. Compared to the MAD model, there are fewer flow hits, with the largest contributions coming from the entropy and σ ceilings.

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