Evolution of accretion discs around a kerr black hole using extended magnetohydrodynamics

Keyphrases

• Accretion Discs 100%
• Kerr Black Hole 100%
• Mirror Instability 100%
• Extended Magnetohydrodynamics 100%
• Collisionality 66%
• Heat Flux 66%
• Ideal Magnetohydrodynamics 66%
• Disk Evolution 66%
• Axisymmetric Model 66%
• Non-ideal Effects 66%
• Pressure Anisotropy 66%
• Field Lines 33%
• Thick Disk 33%
• Mean Free Path 33%
• Velocity Space 33%
• Temperature Gradient 33%
• Magnetic Field Lines 33%
• Magnetohydrodynamic Model 33%
• Eddington 33%
• Optically Thin 33%
• Magnetic Pressure 33%
• Angular Momentum Transfer 33%
• Coulomb 33%
• Non-ideality 33%
• Firehose Instability 33%
• Heat Conduction 33%
• New Codes 33%
• Wave-particle 33%
• Particle Scattering 33%
• Particle Velocity 33%
• Space Mirror 33%
• Magnetohydrodynamic Turbulence 33%
• Rotating Black Holes 33%

Physics

• Magnetohydrodynamics 100%
• Kerr Black Holes 100%
• Circumstellar Disks 100%
• Anisotropy 50%
• Angular Momentum 25%
• Magnetic Field 25%
• Mean Free Path 25%
• Magnetohydrodynamic Turbulence 25%
• Temperature Gradients 25%
• Conductive Heat Transfer 25%
• Rotating Black Holes 25%
• Black Hole 25%
• Transportation 25%
• Magnetic Pressure 25%