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

来源：

COMPTES RENDUS PHYSIQUE | 2013年 / 14卷 / 04期

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

页码：306 / 317

页数：12

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