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Electromagnetic Observables of Weakly Collisional Black Hole Accretion

  • Authors: Vedant Dhruv, Cora Prather, Mani Chandra, Abhishek V. Joshi, Charles F. Gammie

Vedant Dhruv et al 2025 The Astrophysical Journal Letters 993 .

  • Provider: AAS Journals

Caption: Figure 7.

GRMHD quantities from the SANE a* = 15/16 simulation. (a) Poloidal slices of the dissipative variables: heat flux normalized by the free-streaming value (left) and pressure anisotropy normalized by magnetic energy density (right). The black contour marks σ = 1. (b) Mass-weighted distribution of pressure anisotropy as a function of β within r ≤ 20rg. (c) Time-averaged radial profile of angular momentum transport in the disk.

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