Oscillatory null singularity inside realistic spinning black holes
| dc.creator | Ori, Amos | |
| dc.date | 2001-03-05 | |
| dc.date.accessioned | 2026-07-07T12:01:18Z | |
| dc.date.available | 2026-07-07T12:01:18Z | |
| dc.description | We calculate the asymptotic behavior of the curvature scalar $(Riemann)^2$ near the null weak singularity at the inner horizon of a generic spinning black hole, and show that this scalar oscillates infinite number of times while diverging. The dominant parallelly-propagated Riemann components oscillate in a similar manner. This oscillatory behavior, which is in a remarkable contrast to the monotonic mass-inflation singularity in spherical charged black holes, is caused by the dragging of inertial frames due to the black- hole's spin. | |
| dc.description | 10 pages, Latex; This version is almost identical to the one previously published in Phys. Rev. Lett | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0103012 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0103012 | |
| dc.identifier | Phys.Rev.Lett.83:5423-5426,1999 | |
| dc.identifier | doi:10.1103/PhysRevLett.83.5423 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/207052 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Oscillatory null singularity inside realistic spinning black holes | |
| dc.type | text |