Numerical simulations of black-hole binaries and gravitational wave emission

被引:30
|
作者
Sperhake, Ulrich [1 ,2 ,3 ,4 ,5 ]
Berti, Emanuele [2 ,4 ]
Cardoso, Vitor [3 ,4 ]
机构
[1] Inst Space Sci CSIC IEEC, Bellaterra 08193, Spain
[2] CALTECH, Pasadena, CA 91125 USA
[3] Univ Tecn Lisboa, Inst Super Tecn, Dept Fis, CENTRA, P-1049 Lisbon, Portugal
[4] Univ Mississippi, Dept Phys & Astron, University, MS 38677 USA
[5] Univ Cambridge, Dept Appl Math & Theoret Phys, Cambridge CB3 0WA, England
关键词
Numerical relativity; Black holes; Gravitational wave physics; Astrophysics; APPARENT-HORIZON FINDER; SPIN EVOLUTION; INITIAL DATA; FINAL SPIN; MASS; RADIATION; COALESCENCE; MERGERS; MODELS; RECOIL;
D O I
10.1016/j.crhy.2013.01.004
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:306 / 317
页数:12
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