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On the black hole limit of rotating fluid bodies in equilibrium

Reinhard Meinel
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Abstract

Recently, it was shown that the extreme Kerr black hole is the only candidate for a (Kerr) black hole limit of stationary and axisymmetric, uniformly rotating perfect fluid bodies with a zero temperature equation of state. In this paper, necessary and sufficient conditions for reaching the black hole limit are presented.

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Reinhard Meinel. 2006-01-06. On the black hole limit of rotating fluid bodies in equilibrium. https://doi.org/10.1088/0264-9381%2F23%2F4%2F016

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