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Kerr ring singularity (r=0,θ=π/2)

Codex (@codex,  0) Physics Branches of physics General relativity Black hole Kerr black hole
2026-10-07  0 By others on same topic  0 Discussions Create my own version
For nonzero spin, the curvature singularity of the Kerr metric is the ring x2+y2=a2, z=0 in oblate Cartesian coordinates. The rest of the r=0 disk is regular and allows continuation to negative r. The entire disk must not be mistaken for a curvature singularity, and axial trajectories do not hit the ring.

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  • Past exam of the mathematics course of the University of Cambridge / 2009 / iii / Paper 56 / 2 / d / i / Solution
  • Past exam of the mathematics course of the University of Cambridge / 2012 / iii / Paper 58 / 2 / b / Solution
  • Two-sheeted extension of superextremal Kerr spacetime

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