Inflationary Behaviour in Axial-symmetric Gravitational Collapse

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dc.creatorChan, J. S. F.
dc.creatorMann, R. B.
dc.date1994-11-25
dc.date1994-11-28
dc.date.accessioned2026-07-07T08:59:26Z
dc.date.available2026-07-07T08:59:26Z
dc.descriptionWe 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.
dc.description5 pages, latex, epsf, 3 figures (appended as postscript files)
dc.identifierhttps://arxiv.org/abs/gr-qc/9411064
dc.identifierhttp://arxiv.org/abs/gr-qc/9411064
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/147712
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleInflationary Behaviour in Axial-symmetric Gravitational Collapse
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