Quasistationary collapse to the extreme Kerr black hole - INSPIRE

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Quasistationary collapse to the extreme Kerr black hole

Reinhard Meinel
(
- Jena U.
)

May, 2004

6 pages

Published in:

Annalen Phys. 13 (2004) 600-603

e-Print:

gr-qc/0405074 [gr-qc]

DOI:

10.1002/andp.200410098

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Abstract: (arXiv)

It is shown that the extreme Kerr black hole is the only candidate for a black hole limit of rotating fluid bodies in equilibrium.

Rotating stars
black holes
cosmic censorship

References(13)

Figures(0)

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