机构:
Univ Cambridge, Dept Appl Math & Theoret Phys, Cambridge CB3 0WA, England
CSIC IEEC, Inst Space Sci, Bellaterra 08193, Spain
CALTECH, Pasadena, CA 91125 USA
Inst Super Tecn, CENTRA, P-1049001 Lisbon, PortugalUniv Cambridge, Dept Appl Math & Theoret Phys, Cambridge CB3 0WA, England
Sperhake, Ulrich
[1
,2
,3
,4
]
机构:
[1] Univ Cambridge, Dept Appl Math & Theoret Phys, Cambridge CB3 0WA, England
[2] CSIC IEEC, Inst Space Sci, Bellaterra 08193, Spain
[3] CALTECH, Pasadena, CA 91125 USA
[4] Inst Super Tecn, CENTRA, P-1049001 Lisbon, Portugal
来源:
INTERNATIONAL JOURNAL OF MODERN PHYSICS D
|
2013年
/
22卷
/
04期
关键词:
Black holes;
numerical relativity;
higher dimensions;
BLACK-HOLES;
GRAVITATIONAL-WAVES;
GENERAL RELATIVITY;
DUAL JETS;
FIELD;
SCHWARZSCHILD;
STABILITY;
EVOLUTION;
STRINGS;
ENERGY;
D O I:
10.1142/S021827181330005X
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We present an overview of recent developments in numerical relativity studies of higher dimensional spacetimes with a focus on time evolutions of black hole (BH) systems. After a brief review of the numerical techniques employed for these studies, we summarize results grouped into the following three areas: (i) numerical studies of fundamental properties of BHs, (ii) applications of BH collisions to the modeling of Trans-Planckian scattering and (iii) numerical studies of asymptotically anti-de Sitter spacetimes in the context of the gauge-gravity duality.