Quasinormal modes of dirty black holes - INSPIRE

DataBETA

Quasinormal modes of dirty black holes

P.T. Leung
(
- Hong Kong, Chinese U.
)
,
Y.T. Liu
(
- Hong Kong, Chinese U.
)
,
W.M. Suen
(
- Hong Kong, Chinese U. and
- Washington U., St. Louis
)
,
C.Y. Tam
(
- Hong Kong, Chinese U.
)
,
K. Young
(
- Hong Kong, Chinese U.
)

1997

4 pages

Published in:

Phys.Rev.Lett. 78 (1997) 2894-2897

e-Print:

gr-qc/9903031 [gr-qc]

DOI:

10.1103/PhysRevLett.78.2894

View in:

reference search73 citations

Citations per year

Abstract: (arXiv)

Quasinormal mode (QNM) gravitational radiation from black holes is expected to be observed in a few years. A perturbative formula is derived for the shifts in both the real and the imaginary part of the QNM frequencies away from those of an idealized isolated black hole. The formulation provides a tool for understanding how the astrophysical environment surrounding a black hole, e.g., a massive accretion disk, affects the QNM spectrum of gravitational waves. We show, in a simple model, that the perturbed QNM spectrum can have interesting features.

gravitational radiation
black hole: Schwarzschild
perturbation theory
numerical calculations

References(15)

Figures(0)

The Collision of two black holes

Peter Anninos
(
- NCSA, Urbana
)
,
David Hobill
(
- NCSA, Urbana and
- Calgary U.
)
,
Edward Seidel
(
- NCSA, Urbana
)
,
Larry Smarr
(
- NCSA, Urbana
)
,
Wai-Mo Suen
(
- Washington U., St. Louis
)

- Phys.Rev.Lett. 71 (1993) 2851-2854
•
e-Print:
- gr-qc/9309016
•
DOI:
- 10.1103/PhysRevLett.71.2851

- Annals Phys. 224 272

Quasinormal mode expansion for linearized waves in gravitational system

E.S.C. Ching
(
- Hong Kong, Chinese U.
)
,
P.T. Leung
(
- Hong Kong, Chinese U.
)
,
W.M. Suen
(
- Washington U., St. Louis
)
,
K. Young
(
- Hong Kong, Chinese U.
)

- Phys.Rev.Lett. 74 (1995) 4588-4591
•
e-Print:
- gr-qc/9408043
•
DOI:
- 10.1103/PhysRevLett.74.4588

Wave propagation in gravitational systems: Completeness of quasinormal modes

E.S.C. Ching
(
- Hong Kong, Chinese U.
)
,
P.T. Leung
(
- Hong Kong, Chinese U.
)
,
W.M. Suen
(
- Washington U., St. Louis and
- NCSA, Urbana
)
,
K. Young
(
- Hong Kong, Chinese U.
)

- Phys.Rev.D 54 (1996) 3778-3791
•
e-Print:
- gr-qc/9507034
•
DOI:
- 10.1103/PhysRevD.54.3778

New Approach to Perturbation Theory

- Phys.Rev.Lett. 42 (1979) 24, 1582
•
DOI:
- 10.1103/PhysRevLett.42.1582

- Phys.Rev.A 29 1034

- Phys.Rev.A 49 3057

- Phys.Rev.A 49 3068

- Phys.Rev.A 49 3982

Nonspherical Perturbations of Relativistic Gravitational Collapse. II. Integer-Spin, Zero-Rest-Mass Fields

Richard H. Price
(
- Caltech
)

- Phys.Rev.D 5 (1972) 2439-2454
•
DOI:
- 10.1103/PhysRevD.5.2439

An Analytic representation for the quasi normal modes of Kerr black holes

E.W. Leaver
(
- Utah U.
)

- Proc.Roy.Soc.Lond.A 402 (1985) 285-298
•
DOI:
- 10.1098/rspa.1985.0119

- Class.Quant.Grav. 7 47

- Class.Quant.Grav. 9 1643

Quasinormal modes of a Schwarzschild black hole: Improved phase-integral treatment

- Phys.Rev.D 46 (1992) 10, 4179
•
DOI:
- 10.1103/PhysRevD.46.4179

Quasinormal modes of Schwarzschild black holes: The determination of quasinormal frequencies with very large imaginary parts

Hans-Peter Nollert
(
- Tubingen U., IAAT
)

- Phys.Rev.D 47 (1993) 5253-5258
•
DOI:
- 10.1103/PhysRevD.47.5253