The Cauchy Horizon In Black Hole-de Sitter Spacetimes
| dc.creator | Chambers, Chris M. | |
| dc.date | 1997-09-11 | |
| dc.date.accessioned | 2026-07-07T03:31:45Z | |
| dc.date.available | 2026-07-07T03:31:45Z | |
| dc.description | The last seven years has produced a growing body of evidence which concludes that the Cauchy horizon in black hole-de Sitter spacetimes is classically stable when the surface gravity at the cosmological event horizon is greater than that at the Cauchy horizon. That stability persists for a finite, but non-zero, region of the black hole's parameter space, $(M,Q,J,Λ)$, suggests that black holes immersed in de Sitter space are counter-examples to the strong cosmic censorship hypothesis. In this review we chronicle that body of evidence and describe the first steps of a program of numerical work aimed at better understanding the interior of black hole-de Sitter spacetimes. The review ends with a speculative account of the role that future work will take. | |
| dc.description | 35 pages (including 15 eps figures), RevTex. Uses header.sty (included). To be published in the proceedings of the workshop on ``The Internal Structure of Black Holes and Spacetime Singularities", held at the Technion -- Israel Institute of Technology, Haifa, Israel. June 29 - July 3, 1997 | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9709025 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9709025 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/35975 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | The Cauchy Horizon In Black Hole-de Sitter Spacetimes | |
| dc.type | text |