Stability of degenerate Cauchy horizons in black hole spacetimes

Details Stability of degenerate Cauchy horizons in black hole spacetimes Stability of degenerate Cauchy horizons in black hole spacetimes

1998-10-22

arxiv.org/abs/gr-qc/9810071v2

Phys.Rev. D59 (1999) 104004

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Revtex, 4 pages, no figures, references added

Scientific paper

10.1103/PhysRevD.59.104004

In the multihorizon black hole spacetimes, it is possible that there are degenerate Cauchy horizons with vanishing surface gravities. We investigate the stability of the degenerate Cauchy horizon in black hole spacetimes. Despite the asymptotic behavior of spacetimes (flat, anti-de Sitter, or de Sitter), we find that the Cauchy horizon is stable against the classical perturbations, but unstable quantum mechanically.

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