Quasinormal modes of black holes and black branes

被引：1613

作者：

Berti, Emanuele ^{[1
,2
]}

Cardoso, Vitor ^{[1
,3
]}

Starinets, Andrei O. ^{[4
]}

机构：

[1] Univ Mississippi, Dept Phys & Astron, University, MS 38677 USA

[2] CALTECH, Pasadena, CA 91125 USA

[3] Inst Super Tecn, Dept Fis, Ctr Multidisciplinar Astrofis CENTRA, P-1049001 Lisbon, Portugal

[4] Univ Oxford, Dept Phys, Rudolf Peierls Ctr Theoret Phys, Oxford OX1 3NP, England

来源：

CLASSICAL AND QUANTUM GRAVITY | 2009年 / 26卷 / 16期

关键词：

COLLAPSING RELATIVISTIC STARS; HYPERBOLIC STATIC SPACETIMES; GRAVITATIONAL-WAVE EMISSION; ROTATING SUPERMASSIVE STAR; ABSORPTION CROSS-SECTION; ACTIVE GALACTIC NUCLEUS; REGGE-WHEELER EQUATION; GAUSS-BONNET THEORY; NORMAL FREQUENCIES; CORE-COLLAPSE;

D O I：

10.1088/0264-9381/26/16/163001

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Quasinormal modes are eigenmodes of dissipative systems. Perturbations of classical gravitational backgrounds involving black holes or branes naturally lead to quasinormal modes. The analysis and classification of the quasinormal spectra require solving non-Hermitian eigenvalue problems for the associated linear differential equations. Within the recently developed gauge-gravity duality, these modes serve as an important tool for determining the near-equilibrium properties of strongly coupled quantum field theories, in particular their transport coefficients, such as viscosity, conductivity and diffusion constants. In astrophysics, the detection of quasinormal modes in gravitational wave experiments would allow precise measurements of the mass and spin of black holes as well as new tests of general relativity. This review is meant as an introduction to the subject, with a focus on the recent developments in the field.

引用

页数：108

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