Quasinormal modes of near extremal stringy black holes

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

It is believed that the quasinormal modes' frequencies of black hole will encode some universal physics of quantum gravity, and is conjectured to be related to the quantum unit of the area law of Bekenstein-Hawking entropy. In this paper we show that there is no similar universal behavior for the quasinormal modes of near extremal stringy black holes, and will in general depend on the nature of radiations. The relation between quasinormal modes' frequency and the relaxation of the black hole perturbation is commented.

Original languageEnglish
Title of host publicationPARTICLES, STRINGS, AND COSMOLOGY
Subtitle of host publication11th International Symposium on Particles, Strings, and Cosmology, PASCOS 2005
Pages362-365
Number of pages4
Volume805
DOIs
Publication statusPublished - 2005 Dec 2
Event11th International Symposium on Particles, Strings and Cosmology, PASCOS 2005 - Gyeongju, Korea, Republic of
Duration: 2005 May 302005 Jun 4

Other

Other11th International Symposium on Particles, Strings and Cosmology, PASCOS 2005
CountryKorea, Republic of
CityGyeongju
Period05/5/3005/6/4

Keywords

  • Quasinormal modes
  • Stringy black holes

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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  • Cite this

    Lin, F-L. (2005). Quasinormal modes of near extremal stringy black holes. In PARTICLES, STRINGS, AND COSMOLOGY: 11th International Symposium on Particles, Strings, and Cosmology, PASCOS 2005 (Vol. 805, pp. 362-365) https://doi.org/10.1063/1.2149731