The Cauchy Horizon In Black Hole-de Sitter Spacetimes

Details The Cauchy Horizon In Black Hole-de Sitter Spacetimes The Cauchy Horizon In Black Hole-de Sitter Spacetimes

1997-09-11

arxiv.org/abs/gr-qc/9709025v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

35 pages (including 15 eps figures), RevTex. Uses header.sty (included). To be published in the proceedings of the workshop on

Scientific paper

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, $(M,Q,J,\Lambda)$, 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.

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