Adiabatic Index in Fluid Models of Collisionless Black Hole Accretion

Abstract

Models of highly sub-Eddington accretion onto black holes commonly use a single fluid model for the collisionless, near-horizon plasma. These models must specify an equation of state. It is common to use an ideal gas with $p=(\gamma -1)u$ and $\gamma =4/3,13/9,$ or $5/3$, but these produce significantly different outcomes. We discuss the origins of this discrepancy and the assumptions underlying the single fluid model. The main result of this investigation is that under conditions relevant to low luminosity black hole accretion the best choice of single fluid adiabatic index is close to but slightly less than $5/3$. Along the way we provide a simple equilibrium model for the relation between the ion-to-electron dissipation ratio and the ion to electron temperature ratio and explore the implications for electron temperature fluctuations in Event Horizon Telescope sources.

arXiv comment8 pages, accepted to ApJ

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• Detailed Derivation of the Scalar Explicit Expressions Governing the Electric Field, Current Density, and Volumetric Power Density in the Four Types of Linear Divergent MHD Channels Under a Unidirectional Applied Magnetic Field
• Probing the disk-jet coupling in M87
• Full-polarization millimeter wavelength variability of Sagittarius A* during the 2018 EHT campaign
• Impacts of radiative cooling on the images of a black hole shadow and extended jets in two-temperature GRMHD simulations
• Observational distinguishability of the Kerr and Kerr-Hayward metrics to EHT