Mass Transport, Turbulent Mixing, and Inflow in Black Hole Accretion
We investigate mass transport, mixing, and disk evolution in nonradiative black hole accretion flows using Lagrangian tracer particles embedded in general-relativistic magnetohydrodynamics simulations. Our simulation suite spans magnetically arrested disk (MAD) and standard and normal evolution (SAN...
Gardado en:
| Principais autores: | , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado: |
IOP Publishing
2025-01-01
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| Series: | The Astrophysical Journal |
| Assuntos: | |
| Acceso en liña: | https://doi.org/10.3847/1538-4357/ae14fd |
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