Inner-horizon instability and mass infla
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Poisson, E.; Israel, W.
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Article
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1989
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The American Physical Society
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English
β 164 KB
Gravitational collapse with rotation leaves a slowly decaying radiative tail which becomes infinitely blueshifted at the inner horizon of the resulting black hole. We study the gravitational effects of this on the inner structure of the hole, using a simple spherical model. In the presence of outflo