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

页码：1 / 23

页数：23

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