Comptes Rendus
Numerical simulations of black-hole binaries and gravitational wave emission
Comptes Rendus. Physique, Volume 14 (2013) no. 4, pp. 306-317.

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.

Publié le :
DOI : 10.1016/j.crhy.2013.01.004
Keywords: Numerical relativity, Black holes, Gravitational wave physics, Astrophysics
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

1 Institute of Space Sciences (CSIC–IEEC), Campus UAB, Torre C5 parells, 08193 Bellaterra, Spain
2 California Institute of Technology, 1200 E California Boulevard, Pasadena, CA 91125, USA
3 CENTRA, Departamento de Física, Instituto Superior Técnico, Universidade Técnica de Lisboa – UTL, Av. Rovisco Pais 1, 1049 Lisboa, Portugal
4 Department of Physics and Astronomy, The University of Mississippi, University, MS 38677, USA
5 Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Cambridge CB3 0WA, UK
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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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