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What is Turbulent Convection in Thin Accretion Disks about?

This document presents a self-consistent model for thin accretion disks incorporating turbulent convection, which influences both viscosity and energy transport. The study identifies two distinct solutions for gas pressure regions and highlights the stability of radiation pressure regions under varying accretion rates. The findings suggest that the convective flux increases with luminosity, stabilizing all disk regions, contrasting with traditional models that lack a physical basis for turbulent viscosity.

Author

sonjaewon2653

Language

EN