Fast growth of magnetic fields in galaxy clusters: A self-accelerating dynamo

Keyphrases

• Magnetic Field 100%
• Galaxy Clusters 100%
• Self-acceleration 100%
• Dynamo 100%
• Fast Growth 100%
• Viscosity 50%
• Field Strength 50%
• Bootstrap 50%
• Reynolds number 50%
• Collision Frequency 50%
• Explosives 50%
• Field Amplification 50%
• Intracluster Medium 50%
• Explosive Growth 50%
• Small Fluctuation 50%
• Effective Collisions 50%
• Particle Collision 50%
• Cluster Lifetime 50%
• Effective Reynolds number 50%
• Field Growth 50%
• Plasma Microinstabilities 50%

Physics

• Magnetic Field 100%
• Galaxy Clusters 100%
• Reynolds Number 100%
• Field Strength 50%
• Intracluster Medium 50%
• Particle Collision 50%