Inflationary Behaviour in Axial - symmetric Gravitational Collapse
نویسندگان
چکیده
We show that the interior of a charged, spinning black hole formed from a general axially symmetric gravitational collapse is unstable to inflation of both its mass and angular momentum parameters. Although our results are formulated in the context of (2 + 1)-dimensional black holes, we argue that they are applicable to (3 + 1) dimensions.
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