Quasinormal modes of black holes and dissipative open systems
| dc.creator | Kim, Sang Pyo | |
| dc.date | 2005-12-01 | |
| dc.date | 2006-01-03 | |
| dc.date.accessioned | 2026-07-07T06:53:54Z | |
| dc.date.available | 2026-07-07T06:53:54Z | |
| dc.description | After explaining the physical origin of the quasinormal modes of perturbations in the background geometry of a black hole, I critically review the recent proposal for the quantization of the black-hole area based on the real part of quasinormal modes. As instantons due to the barriers of black-hole potentials lie at the root of a discrete set of complex quasinormal modes frequencies, it is likely that the physics of quasinormal modes can be learned from quantum theory. I propose a connection of a system of quasinormal modes of black holes with a dissipative open system, in particular, the Feshbach-Tikochinsky oscillator. This argument is supported in part by the fact that these two systems have the same group structure SU(1,1) and the same group representation of Hamiltonians; thereby, their quantum states exhibit the same behavior. | |
| dc.description | RevTex 9 pages, one figure; Talks at Black Hole V, Canada, 2005 and 9th Italian-Korean Symposium, Korea, 2005; note and references added in proof | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0512005 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0512005 | |
| dc.identifier | J.Korean Phys.Soc. 49 (2006) 764-772 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/105752 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Quasinormal modes of black holes and dissipative open systems | |
| dc.type | text |