In adiabatically stratified cluster gas the MTI saturates via large plumes destroyed by shear, producing turbulent kinetic energy that scales as χ ω_T.
Living Reviews in Computational Astrophysics , volume =
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Numerical simulations indicate that particle scattering in anisotropic turbulence without a guide field is independent of correlation length and follows a mechanism distinct from pitch-angle diffusion.
Chaotic Cold Accretion reproduces the observed near-linear black hole mass-bolometric luminosity scaling (slope 0.91) in z>2 quasars while Bondi accretion underpredicts by ~2 dex.
citing papers explorer
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High-energy Particle Transport in Three-dimensional Anisotropic Turbulent Magnetic Fields
Numerical simulations indicate that particle scattering in anisotropic turbulence without a guide field is independent of correlation length and follows a mechanism distinct from pitch-angle diffusion.