Numerical simulations of black-hole binaries and gravitational wave emission
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We review recent progress in numerical relativity simulations of black-hole (BH) spacetimes. Following a brief summary of the methods employed in the modeling, we summarize the key results in two major areas of BH physics: (i) BHs as sources of gravitational waves (GWs) and (ii) astrophysical systems involving BHs. We conclude with a list of the most urgent tasks for numerical relativity in these areas. (C) 2013 Academie des sciences. Published by Elsevier Masson SAS. All rights reserved.
| Original language | English |
|---|---|
| Journal | Comptes Rendus Physique |
| Volume | 14 |
| Issue number | 4 |
| Pages (from-to) | 306-317 |
| Number of pages | 12 |
| ISSN | 1631-0705 |
| DOIs | |
| Publication status | Published - Apr 2013 |
| Externally published | Yes |
- Numerical relativity, Black holes, Gravitational wave physics, Astrophysics, APPARENT-HORIZON FINDER, SPIN EVOLUTION, INITIAL DATA, FINAL SPIN, MASS, RADIATION, COALESCENCE, MERGERS, MODELS, RECOIL
Research areas
ID: 300165311