Binary Black Hole Mergers in 3d Numerical Relativity
| dc.creator | Bruegmann, Bernd | |
| dc.date | 1997-08-18 | |
| dc.date | 1999-03-11 | |
| dc.date.accessioned | 2026-07-07T12:01:24Z | |
| dc.date.available | 2026-07-07T12:01:24Z | |
| dc.description | The standard approach to the numerical evolution of black hole data using the ADM formulation with maximal slicing and vanishing shift is extended to non-symmetric black hole data containing black holes with linear momentum and spin by using a time-independent conformal rescaling based on the puncture representation of the black holes. We give an example for a concrete three dimensional numerical implementation. The main result of the simulations is that this approach allows for the first time to evolve through a brief period of the merger phase of the black hole inspiral. | |
| dc.description | 8 pages, 9 figures, REVTeX; expanded discussion, results unchanged | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9708035 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9708035 | |
| dc.identifier | Int.J.Mod.Phys.D8:85,1999 | |
| dc.identifier | doi:10.1142/S0218271899000080 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/207086 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | Astrophysics | |
| dc.title | Binary Black Hole Mergers in 3d Numerical Relativity | |
| dc.type | text |