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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

Metric and electromagnetic perturbations of the Reissner-Nordström black hole

TL;DR: In this paper, a method for reducible systems of differential equations is applied to the study of the metric and electromagnetic perturbations of the Reissner-Nordstrom black hole.
Journal ArticleDOI

Self-force Regularization in the Schwarzschild Spacetime

TL;DR: In this article, the authors discuss the problem of regularizing the divergent self-force on a particle in a black hole space-time and report some recent progress in solving it.
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Master Functions and Equations for Perturbations of Vacuum Spherically-Symmetric Spacetimes

TL;DR: In this paper, the authors studied the most general master function that is linear in the metric perturbations and their first-order derivatives and satisfies a wave equation with a potential.
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Quasinormal modes of five-dimensional black holes in non-commutative geometry

TL;DR: In this article, the spectrum of quasinormal frequencies of five-dimensional black holes obtained in noncommutative geometry was computed and scalar perturbations of a massive scalar field adopting the 6th order WKB approximation were studied.
Journal ArticleDOI

Scalar perturbations of nonlinear charged Lifshitz black branes with hyperscaling violation

TL;DR: In this article, the authors study scalar perturbations of nonlinear charged Lifshitz black branes with hyperscaling violating factor and find numerically the quasinormal modes for scalar fields.
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