Stability of Generalised Static Black Holes in Higher Dimensions
| dc.creator | Kodama, Hideo | |
| dc.creator | Ishibashi, Akihiro | |
| dc.date | 2003-12-02 | |
| dc.date.accessioned | 2026-07-07T03:28:17Z | |
| dc.date.available | 2026-07-07T03:28:17Z | |
| dc.description | We discuss the stability of (charged) static black holes in higher-dimensional spacetimes with and without cosmological constant by using gauge-invariant master equations of the Schroedinger equation type for black hole perturbations derived by the authors recently. In particular, we show that the stability of higher-dimensional Schwarzschild black holes can be proved with the help of a technique called S-deformation of the master equations. We also point out that higher-dimensional static black holes might be unstable only against scalar-type perturbations in the neutral case and in the charged case with spherically symmetric or flat horizons. | |
| dc.description | 14 pages. A talk given at the Seventh Hungarian Relativity Workshop, 10-15 Aug. 2003, Sarospatak, Hungary. To appear in the proceedings | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0312012 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0312012 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/34770 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Stability of Generalised Static Black Holes in Higher Dimensions | |
| dc.type | text |