Nous passons en revue les progrès récents concernant la simulation des trous noirs en relativité numérique. Après un bref résumé des méthodes employées, nous donnons les résultats clés dans deux domaines majeurs de la physique des trous noirs : (i) les trous noirs comme sources dʼondes gravitationnelles et (ii) les systèmes astrophysiques contenant des trous noirs. Nous concluons sur la liste des travaux les plus urgents à conduire dans ces domaines.
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.
Mots clés : Relativité numérique, Trous noirs, Physique des ondes gravitationnelles, Astrophysique
Ulrich Sperhake 1, 2, 3, 4, 5 ; Emanuele Berti 2, 4 ; Vitor Cardoso 3, 4
@article{CRPHYS_2013__14_4_306_0, author = {Ulrich Sperhake and Emanuele Berti and Vitor Cardoso}, title = {Numerical simulations of black-hole binaries and gravitational wave emission}, journal = {Comptes Rendus. Physique}, pages = {306--317}, publisher = {Elsevier}, volume = {14}, number = {4}, year = {2013}, doi = {10.1016/j.crhy.2013.01.004}, language = {en}, }
TY - JOUR AU - Ulrich Sperhake AU - Emanuele Berti AU - Vitor Cardoso TI - Numerical simulations of black-hole binaries and gravitational wave emission JO - Comptes Rendus. Physique PY - 2013 SP - 306 EP - 317 VL - 14 IS - 4 PB - Elsevier DO - 10.1016/j.crhy.2013.01.004 LA - en ID - CRPHYS_2013__14_4_306_0 ER -
Ulrich Sperhake; Emanuele Berti; Vitor Cardoso. Numerical simulations of black-hole binaries and gravitational wave emission. Comptes Rendus. Physique, Volume 14 (2013) no. 4, pp. 306-317. doi : 10.1016/j.crhy.2013.01.004. https://comptes-rendus.academie-sciences.fr/physique/articles/10.1016/j.crhy.2013.01.004/
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