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.
Originalsprog | Engelsk |
---|---|
Tidsskrift | Comptes Rendus Physique |
Vol/bind | 14 |
Udgave nummer | 4 |
Sider (fra-til) | 306-317 |
Antal sider | 12 |
ISSN | 1631-0705 |
DOI | |
Status | Udgivet - apr. 2013 |
Eksternt udgivet | Ja |
ID: 300165311