On the black hole limit of rotating fluid bodies in equilibrium
arXiv:gr-qc/0506130 · doi:10.1088/0264-9381/23/4/016
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.
8 pages, v2: one footnote and one reference added, accepted for publication in CQG
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- On the multipole moments of a rigidly rotating fluid body
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