On the black hole limit of rotating fluid bodies in equilibrium

Details On the black hole limit of rotating fluid bodies in equilibrium On the black hole limit of rotating fluid bodies in equilibrium

2005-06-29

arxiv.org/abs/gr-qc/0506130v2

Class.Quant.Grav.23:1359-1364,2006

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

8 pages, v2: one footnote and one reference added, accepted for publication in CQG

Scientific paper

10.1088/0264-9381/23/4/016

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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