The stable problem of the black-hole connected region in the Schwarzschild black hole
| dc.creator | Tian, Guihua | |
| dc.date | 2005-12-18 | |
| dc.date.accessioned | 2026-07-07T06:53:57Z | |
| dc.date.available | 2026-07-07T06:53:57Z | |
| dc.description | The stability of the Schwarzschild black hole is studied. Using the Painlevé coordinate, our region can be defined as the black-hole-connected region(r>2m, see text) of the Schwarzschild black hole or the white-hole-connected region(r>2m, see text) of the Schwarzschild black hole. We study the stable problems of the black-hole-connected region. The conclusions are: (1) in the black-hole-connected region, the initially regular perturbation fields must have real frequency or complex frequency whose imaginary must not be greater than -1/4m, so the black-hole-connected regionis stable in physicist' viewpoint; (2) On the contrary, in the mathematicians' viewpoint, the existence of the real frequencies means that the stable problem is unsolved by the linear perturbation method in the black-hole-connected region. | |
| dc.description | 6 pages, no figures | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0512101 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0512101 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/105774 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | The stable problem of the black-hole connected region in the Schwarzschild black hole | |
| dc.type | text |