On the black hole limit of rotating fluid bodies in equilibrium
classification
🌀 gr-qc
astro-phhep-th
keywords
blackholelimitbodiesfluidkerrrotatingaxisymmetric
read the original 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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