Three-dimensional relativistic simulations of rotating neutron-star collapse to a Kerr black hole

Keyphrases

• Three-dimensional (3D) 100%
• Angular Velocity 100%
• Kerr Black Hole 100%
• Gravitational Collapse 100%
• Rotating Neutron Stars 100%
• Shock 50%
• Precise Measurement 50%
• Angular Momentum 50%
• Equation of State 50%
• Computational Domain 50%
• Fluid Equations 50%
• Black Hole Mass 50%
• Ideal Fluid 50%
• Black Hole Spin 50%
• Differential Rotation 50%
• Einstein Equations 50%
• Stellar Models 50%
• Stable Orbits 50%
• General Relativistic Hydrodynamics 50%
• Hydrodynamic Code 50%
• Polytropes 50%
• Apparent Horizon 50%
• Traceless 50%
• Dynamical Horizons 50%
• High Resolution Shock Capturing 50%
• Trapped Surfaces 50%
• Slow Rotation 50%
• Polytropic Fluid 50%

Physics

• Angular Velocity 100%
• Kerr Black Holes 100%
• Gravitational Collapse 100%
• Neutron Stars 100%
• Black Hole 100%
• Angular Momentum 50%
• High Resolution 50%
• Equations of State 50%
• Event Horizon 50%
• Shedding 50%
• Einstein Equation 50%
• Stellar Model 50%
• Relativistic Hydrodynamics 50%
• Polytropes 50%
• Ideal Fluid 50%