Adding particle collisions to the formation of asteroids and Kuiper belt objects via streaming instabilities

Keyphrases

• Planetesimals 100%
• Particle Collision 100%
• Streaming Instability 100%
• Superparticles 100%
• Kuiper Belt Objects 100%
• Asteroid Belt 100%
• Numerical Algorithms 66%
• Particle Density 33%
• Monte Carlo Method 33%
• Computational Cost 33%
• Energy Dissipation 33%
• Gas Density 33%
• Kuiper Belt 33%
• Turbulence 33%
• Self-gravity 33%
• Small Particles 33%
• Protoplanetary Disks 33%
• Particle Dynamics 33%
• Density Inhomogeneity 33%
• Inelastic Collisions 33%
• Momentum Exchange 33%
• Collision Frequency 33%
• Gravitational Collapse 33%
• Drag Force 33%
• Shear Velocity 33%
• Energy Exchange 33%
• Mid-plane 33%
• Local Particles 33%
• Collision Time 33%
• Gravity Parameter 33%
• Collision Outcome 33%
• Radial Contraction 33%

Physics

• Particle Collision 100%
• Asteroid Belt 100%
• Protoplanets 100%
• Trans-Neptunian Object 100%
• Monte Carlo 33%
• Energy Transfer 33%
• Inelastic Collision 33%
• Hydrodynamics 33%
• Protoplanetary Disk 33%
• Kuiper Belt 33%
• Gravitational Collapse 33%
• Asteroid Belts 33%