Quasistationary collapse to the extreme Kerr black hole

被引:13
作者
Meinel, R [1 ]
机构
[1] Univ Jena, Inst Theoret Phys, D-07743 Jena, Germany
关键词
rotating stars; black holes; cosmic censorship;
D O I
10.1002/andp.200410098
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
It is shown that the extreme Kerr black hole, i.e. the one with the maximal angular momentum for a given mass, is the only candidate for a black hole limit of rotating fluid bodies in equilibrium. (C) 2004 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.
引用
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页码:600 / 603
页数:4
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