Protoplanetary disk turbulence driven by the streaming instability: Nonlinear saturation and particle concentration

Physics

• Protoplanetary Disk 100%
• Transients 50%
• Angular Momentum 50%
• Larger Particle 50%
• Protoplanets 50%
• Turbulent Diffusion 50%
• Random Walk 50%
• Stellar Accretion 50%
• Equilibrium Flow 50%

Keyphrases

• Coupled Particles 66%
• Superparticles 33%
• Self-collision 33%

Engineering

• Drift Flow 100%