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Journal ArticleDOI

Stability of a Schwarzschild Singularity

Tullio Regge, +1 more
- 15 Nov 1957 - 
- Vol. 108, Iss: 4, pp 1063-1069
TLDR
In this article, it was shown that a Schwarzschild singularity, spherically symmetrical and endowed with mass, will undergo small vibrations about the spherical form and therefore remain stable if subjected to a small nonspherical perturbation.
Abstract
It is shown that a Schwarzschild singularity, spherically symmetrical and endowed with mass, will undergo small vibrations about the spherical form and will therefore remain stable if subjected to a small nonspherical perturbation.

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Journal ArticleDOI

Black holes in massive gravity

TL;DR: In this paper, the authors review the stability properties of the black hole solutions of the ghost-free massive gravity theory and its bimetric extension, and outline the main results on the stability of these solutions against small perturbations.
Book ChapterDOI

Black Holes in Higher-Dimensional Gravity

TL;DR: In this paper, the phase structure of Kaluza-klein black hole solutions in higher-dimensional vacuum Einstein gravity has been investigated and the phase diagram that emerges for each of the two classes is discussed, including an intriguing connection that relates the phase structures of Kalza-Klein black holes with that of asymptotically flat rotating black holes.
Journal ArticleDOI

Faithful analytical effective-one-body waveform model for spin-aligned, moderately eccentric, coalescing black hole binaries

TL;DR: In this paper, an effective-one-body (EOB) model for eccentric binary coalescences is presented, which is based on the TEOBResumS\_SM model for circularized coalescing black-hole binaries.
Journal ArticleDOI

Area Spectrum of Kerr and extremal Kerr Black Holes from Quasinormal Modes

TL;DR: Kunstatter's method is implemented to derive the area spectrum of Kerr and extremal Kerr black holes and it is inferred that the function describing the real part of quasinormal frequencies of Kerr black hole is not the correct one.
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