- Levine et al.
- http://arxiv.org/abs/0711.3478
- Simulation with high dynamic range (1E7) down to 0.1pc, i.e. to the accretion disk of a SMBH.
- Global instabilities make things quasi-stable locally due to turbulence.
- An exponential density profile for the gas in a disk arises naturally due to this.
Tags: Black Holes, Disk, Galaxies, Simulation
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