Abstract
We investigate dynamical and thermodynamical instability of the 4-d Reissner- Nordström-Anti de-Sitter (RN-AdS) black holes. In accordance with the holographic model of superconductor, we find, by computing the quasi-normal mode, that the RN-AdS black holes are unstable below the critical temperature. We also calculate the difference of the entropy between the RN-AdS black hole and the hairy black hole that emerges below the critical temperature. It is shown that the hairy black hole carries larger entropy than the RN-AdS black hole in the micro-canonical ensemble, which implies that the RN-AdS black holes evolve towards the hairy black holes, due to the instability.
| Original language | English |
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| Title of host publication | Proceedings of the 20th Workshop on General Relativity and Gravitation in Japan, JGRG 2010 |
| Pages | 402-406 |
| Number of pages | 5 |
| Publication status | Published - 2010 |
| Event | 20th Workshop on General Relativity and Gravitation in Japan, JGRG 2010 - Kyoto Duration: 2010 Sep 21 → 2010 Sep 25 |
Other
| Other | 20th Workshop on General Relativity and Gravitation in Japan, JGRG 2010 |
|---|---|
| City | Kyoto |
| Period | 10/9/21 → 10/9/25 |
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ASJC Scopus subject areas
- Atomic and Molecular Physics, and Optics
Cite this
Koga, J. I., Maeda, K., & Fujii, S. (2010). The final fate of instability of Reissner-Nordström-AdS black holes. In Proceedings of the 20th Workshop on General Relativity and Gravitation in Japan, JGRG 2010 (pp. 402-406)