Numerical relativity: the role of black holes in gravitational wave physics, astrophysics and high-energy physics

被引：2
|
作者：
Sperhake, Ulrich [1 ]
机构：
[1] Univ Cambridge, Dept Appl Math & Theoret Phys, Ctr Math Sci, Cambridge CB3 0WA, England
来源：
GENERAL RELATIVITY AND GRAVITATION | 2014年 / 46卷 / 05期
基金：
美国国家科学基金会;
关键词：
Black holes; Numerical relativity; Gravitational waves; Higher dimensions; BOUNDARY; MERGERS; SIMULATIONS; DIMENSIONS; EXTRACTION; EVOLUTION; HIERARCHY; BINARIES; MOMENTUM; STRINGS;
D O I：
10.1007/s10714-014-1689-z
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Black holes play an important role in many areas of physics. Their modeling in the highly-dynamic, strong-field regime of general relativity requires the use of computational methods. We present a review of the main results obtained through numerical relativity simulations of black-hole spacetimes with a particular focus on the most recent developments in the areas of gravitational-wave physics, astrophysics, high-energy collisions, the gauge-gravity duality, and the study of fundamental properties of black holes.
引用
收藏
页码：1 / 23
页数：23
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