Bardeen-Petterson alignment, jets, and magnetic truncation in GRMHD simulations of tilted thin accretion discs

Keyphrases

• Truncation 100%
• Relativistic Magnetohydrodynamics 100%
• Magnetohydrodynamic Simulation 100%
• Thin Disk 100%
• Angular Momentum Vector 100%
• Bardeen 100%
• Inner Region 100%
• Thin Accretion Disk 100%
• Low Density 50%
• Numerical Simulation 50%
• Aspect Ratio 50%
• High Performance 50%
• Tilted Disc 50%
• Accretion Flow 50%
• Relativistic Jets 50%
• Viscosity 50%
• Turbulence 50%
• Magnetic Flux 50%
• Accreting Black Holes 50%
• Unexpected Results 50%
• Gravitational Radius 50%
• High Viscosity 50%
• Cooling Time 50%
• Magnetic Pressure 50%
• Effective Viscosity 50%
• Adaptive Mesh 50%
• Computational Grid 50%
• Radio-loud Quasars 50%
• Thermal Decoupling 50%
• Cooling Function 50%

Physics

• Black Holes 100%
• Accretion Disk 100%
• Magnetohydrodynamic Simulation 100%
• Angular Momentum 33%
• Anisotropic Magnetoresistance 16%
• Magnetohydrodynamic Generator 16%
• Circumstellar Disks 16%
• Computational Grid 16%
• Schwarzschild Radius 16%
• Relativistic Jets 16%
• Magnetohydrodynamics 16%
• Magnetic Flux 16%
• Aspect Ratio 16%
• Radio Loud Quasars 16%