Quasistationary collapse to the extreme Kerr black hole
arXiv:gr-qc/0405074 · doi:10.1002/andp.200410098
Abstract
It is shown that the extreme Kerr black hole is the only candidate for a black hole limit of rotating fluid bodies in equilibrium.
6 pages, submitted to Annalen der Physik (Leipzig)
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- The Dirac propagator in the extreme Kerr metric
- On the bound states of the Dirac equation in the extreme Kerr metric
- The Parametric Transition of Strange Matter Rings to a Black Hole