Solving the initial value problem of two black holes
We solve the elliptic equations associated with the Hamiltonian and momentum constraints, corresponding to a system composed of two black holes with arbitrary linear and angular momentum. These new solutions are based on a Kerr-Schild spacetime slicing which provides more physically realistic soluti...
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| Veröffentlicht in: | Physical review letters 2000-12, Vol.85 (26 Pt 1), p.5500-5503 |
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| Hauptverfasser: | , |
| Format: | Artikel |
| Sprache: | eng |
| Online-Zugang: | Volltext |
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