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Asymptotic black hole quasinormal frequencies

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Motl, Lubos, Neitzke, Andrew·2003·Advances in Theoretical and Mathematical Physics

Abstract

We give a new derivation of the quasinormal frequencies of Schwarzschild black holes in d 4 and Reissner-Nordstrm black holes in d = 4 , in the limit of innite damping.For Schwarzschild in d 4 w e nd that the asymptotic real part is T Hawking log(3) for scalar perturbations and for some gravitational perturbations this conrms a result previously obtained by other means in the case d = 4 .For Reissner-Nordstrm in d = 4 w e nd a specic generally aperiodic behavior for the quasinormal frequencies, both for scalar perturbations and for electromagneticgravitational perturbations.The formulae are obtained by studying the monodromy of the perturbation analytically continued to the complex plane the analysis depends essentially on the behavior of the potential in the \unphysical" region near the black hole singularity.

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Metadata

Authors
Motl, L., & Neitzke, A.
Venue
Advances in Theoretical and Mathematical Physics
Published
2003
Volume
7
Issue
2
Pages
307-330
ISSN
  • 1095-0753 (ISSN-L)
  • 1095-0761
OpenAlex
W2077468361
Cited by
381
References
29
FWCI
18.86
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Asymptotic black hole quasinormal frequencies. https://app.cochat.ai/papers/10.4310/atmp.2003.v7.n2.a4
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Motl, L., & Neitzke, A. (2003). Asymptotic black hole quasinormal frequencies. Advances in Theoretical and Mathematical Physics. https://doi.org/10.4310/atmp.2003.v7.n2.a4

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