Numerical challenges in modeling gravothermal collapse in Self-Interacting Dark Matter halos

Keyphrases

• Halo 100%
• Dark Matter Halos 100%
• Self-interacting Dark Matter 100%
• Core-collapse 66%
• Dark Matter 33%
• Numerical Implementation 33%
• Stall 16%
• Gravitational Force 16%
• Particle number 16%
• Gain Loss 16%
• Inner Core 16%
• Energy Gain 16%
• Self-interaction 16%
• Rate Difference 16%
• Scattering Rate 16%
• Mass Resolution 16%
• N-body 16%
• Resolution Time 16%
• Collapse Time 16%
• Large Cross-section 16%
• High-resolution Simulation 16%
• Adaptive Force 16%
• Core Evolution 16%
• Simulation Time-step 16%
• Scattering Halos 16%

Physics

• Dark Matter 100%
• High Resolution 14%