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Non-linear instability of Kerr-type Cauchy horizons | | Patrick R Brady
; Chris M Chambers
; | | Date: |
21 Dec 1994 | | Journal: | Phys.Rev. D51 (1995) 4177-4186 | | Subject: | gr-qc | | Abstract: | Using the general solution to the Einstein equations on intersecting null surfaces developed by Hayward, we investigate the non-linear instability of the Cauchy horizon inside a realistic black hole. Making a minimal assumption about the free gravitational data allows us to solve the field equations along a null surface crossing the Cauchy Horizon. As in the spherical case, the results indicate that a diverging influx of gravitational energy, in concert with an outflux across the CH, is responsible for the singularity. The spacetime is asymptotically Petrov type N, the same algebraic type as a gravitational shock wave. Implications for the continuation of spacetime through the singularity are briefly discussed. | | Source: | arXiv, gr-qc/9501025 | | Services: | Forum | Review | PDF | Favorites | |
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