A method of determining apparent horizons in three-dimensional numerical relativity

Physics Letters A

Volumn 106, Issue 5-6, 1984, Pages 235-238

  Nakamura, Takashi ^a   Kojima, Yasufumi ^a   Oohara, Ken ichi ^b  

^a KYOTO UNIVERSITY   (Japan)

^b Institute for Fundamental Chemistry   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000599994     PISSN: 03759601     EISSN: None     Source Type: Journal    
DOI: 10.1016/0375-9601(84)91016-8     Document Type: Article

References (22)

1. Gravitational collapse of supermassive stars to black holes - Numerical solution of the Einstein equations
2. Gravitational collapse to neutron stars and black holes - Computer generation of spherical spacetimes
3. General Relativistic Collapse of an Axially Symmetric Star. I: The Formulation and the Initial Value Equations
4. A New Formalism of the Einstein Equations for Relativistic Rotating Systems
5. A Method of Determining Apparent Horizons in [(2+1)+1]-Formalism of the Einstein Equations
6. General Relativistic Collapse of Axially Symmetric Stars Leading to the Formation of Rotating Black Holes
7. Numerical Relativity
8. General Relativistic Collapse of Accreting Neutron Stars with Rotation
9. General Relativistic Collapse of Rotating Stars
10. General Relativistic Collapse of Rotating Supermassive Stars
11. General Relativistic Collapse of Non-Rotating, Axisymmetric Stars
12. Time Evolution of Pure Gravitational Waves
13. Limits on Gravitational Radiation from two Gravitationally Bound Black Holes