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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 15.

The spin-up parameter “s” is given by Equation (30). The markers indicate the time-averaged value, and error bars represent 1σ. Red and blue markers are MAD and SANE simulations, respectively. The black dashed line is the expected thin-disk values (Equation (31)). The solid gray line is the quadratic fit (Equation (32)), and the dashed silver line is the fifth-order polynomial fit provided in R. Narayan et al. (2022).

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