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 language | English |
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| Title of host publication | PARTICLES, STRINGS, AND COSMOLOGY |
| Subtitle of host publication | 11th International Symposium on Particles, Strings, and Cosmology, PASCOS 2005 |
| Pages | 362-365 |
| Number of pages | 4 |
| Volume | 805 |
| DOIs | |
| Publication status | Published - 2005 Dec 2 |
| Event | 11th International Symposium on Particles, Strings and Cosmology, PASCOS 2005 - Gyeongju, Korea, Republic of Duration: 2005 May 30 → 2005 Jun 4 |
Other
| Other | 11th International Symposium on Particles, Strings and Cosmology, PASCOS 2005 |
|---|---|
| Country/Territory | Korea, Republic of |
| City | Gyeongju |
| Period | 2005/05/30 → 2005/06/04 |
Keywords
- Quasinormal modes
- Stringy black holes
ASJC Scopus subject areas
- Physics and Astronomy(all)