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Is it possible for the phenomenon of turbulence – eddys and vortices on many scales – to occur in spacetime in the context of General Relativity? For example near a Kerr black hole.

If not, what is different about the governing equations of GR, vs those of fluid dynamics, that determines this?

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    $\begingroup$ For example near a Kerr black hole. The Kerr metric has no time-dependence at all (at least not in Boyer–Lindquist or Kerr–Schild coordinates). $\endgroup$
    – Ghoster
    Commented Feb 17 at 5:52
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    $\begingroup$ Does this answer your question? Turbulent spacetime from Einstein equation? $\endgroup$ Commented Feb 17 at 8:02

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