Three-dimensional numerical general relativistic hydrodynamics. II. Long-term dynamics of single relativistic stars

Keyphrases

• Analysis Module 33%
• Apparent Horizon 33%
• Central Differencing 33%
• Code Testing 33%
• Coupled System 33%
• Cowl 33%
• Eigenfrequency 33%
• Einstein Equations 33%
• Equilibrium Configuration 33%
• General Relativistic Hydrodynamics 100%
• General Relativity 66%
• General-relativistic Polytropic Models 33%
• Gravitational Collapse 33%
• Gravitational Waves 33%
• High Resolution Shock Capturing 33%
• Hydrodynamic Equations 33%
• Internal Energy 33%
• Long Term Evolution 33%
• Long-term Dynamical Evolution 33%
• Long-term Dynamics 100%
• Mass Density 66%
• New Physics 33%
• Non-rotating 33%
• Numerical Code 33%
• Numerical Evolution 33%
• Oscillation 66%
• Perturbation Method 33%
• Polytropic Equation of State 33%
• Quadrupolar 33%
• Rapid Rotation 33%
• Relativistic Astrophysics 33%
• Relativistic Stars 100%
• Rest Mass 66%
• Riemann Solver 33%
• Rotating Star 66%
• Slope Limiter 33%
• Space-time Evolution 33%
• Stable Equilibrium 66%
• Stellar Models 66%
• Three-dimensional (3D) 100%
• Three-dimensional Growth 33%
• Unstable Branch 33%

Physics

• Black Hole 33%
• Dynamical Evolution 33%
• Einstein Equation 33%
• Equations of State 33%
• General Relativity 66%
• Gravitational Collapse 33%
• High Resolution 33%
• Hydrodynamic Equation 33%
• Internal Energy 33%
• Physics 33%
• Relativistic Hydrodynamics 100%
• Relativistic Stars 100%
• Stellar Model 66%