Quasinormal modes of black holes: From astrophysics to string theory
RA Konoplya, A Zhidenko - Reviews of Modern Physics, 2011 - APS
Perturbations of black holes, initially considered in the context of possible observations of
astrophysical effects, have been studied for the past 10 years in string theory, brane-world …
astrophysical effects, have been studied for the past 10 years in string theory, brane-world …
[HTML][HTML] Gravitational-wave tests of general relativity with ground-based detectors and pulsar-timing arrays
This review is focused on tests of Einstein's theory of general relativity with gravitational
waves that are detectable by ground-based interferometers and pulsar-timing experiments …
waves that are detectable by ground-based interferometers and pulsar-timing experiments …
First Sagittarius A* event horizon telescope results. VI. Testing the black hole metric
Astrophysical black holes are expected to be described by the Kerr metric. This is the only
stationary, vacuum, axisymmetric metric, without electromagnetic charge, that satisfies …
stationary, vacuum, axisymmetric metric, without electromagnetic charge, that satisfies …
First Sagittarius A* Event Horizon Telescope Results. VI: Testing the Black Hole Metric
Event Horizon Telescope Collaboration - arXiv preprint arXiv …, 2023 - arxiv.org
Astrophysical black holes are expected to be described by the Kerr metric. This is the only
stationary, vacuum, axisymmetric metric, without electromagnetic charge, that satisfies …
stationary, vacuum, axisymmetric metric, without electromagnetic charge, that satisfies …
Universal Teukolsky equations and black hole perturbations in higher-derivative gravity
We reduce the study of perturbations of rotating black holes in higher-derivative extensions
of general relativity to a system of decoupled radial equations that stem from a set of …
of general relativity to a system of decoupled radial equations that stem from a set of …
Mass inflation without Cauchy horizons
Mass inflation is a well established instability, conventionally associated to Cauchy horizons
(which are also inner trapping horizons) of stationary geometries, leading to a divergent …
(which are also inner trapping horizons) of stationary geometries, leading to a divergent …
[HTML][HTML] Perturbations of a rotating black hole. I. Fundamental equations for gravitational, electromagnetic, and neutrino-field perturbations
SA Teukolsky - Astrophysical Journal, Vol. 185, pp. 635-648 …, 1973 - adsabs.harvard.edu
freedom is described in Appendix A. Choosing the directions of! and ii so that equations
(2.1) hold uses up four degrees of freedom (eqs.[Al] and [A2]). We choose tofollow …
(2.1) hold uses up four degrees of freedom (eqs.[Al] and [A2]). We choose tofollow …
Quasi-normal modes of stars and black holes
KD Kokkotas, BG Schmidt - Living Reviews in Relativity, 1999 - Springer
Perturbations of stars and black holes have been one of the main topics of relativistic
astrophysics for the last few decades. They are of particular importance today, because of …
astrophysics for the last few decades. They are of particular importance today, because of …
[图书][B] A first course in general relativity
B Schutz - 2022 - books.google.com
Clarity, readability, and rigor combine in the third edition of this widely used textbook to
provide the first step into general relativity for advanced undergraduates with a minimal …
provide the first step into general relativity for advanced undergraduates with a minimal …
Regular black holes without mass inflation instability
A bstract Generic models of regular black holes have separate outer and inner horizons,
both with nonzero surface gravity. It has been shown that a nonzero inner horizon surface …
both with nonzero surface gravity. It has been shown that a nonzero inner horizon surface …