PeterDonis
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Matterwave said:A Kerr black hole for example is not static (it is - however - stationary).
The exterior (outside the horizon) of Kerr spacetime is stationary. The interior (inside the horizon) is not. (Nor is the interior of Schwarzschild spacetime.)
Matterwave said:The interior of the black hole can't be material in (hydrostatic) equilibrium because all world lines for all physical particles must reach the singularity in finite proper time
"All worldlines must hit the singularity in finite proper time" is only true for Schwarzschild spacetime. It is not true for Kerr spacetime; there are worldlines in maximally extended Kerr spacetime that never hit the singularity at all (they eventually emerge into another stationary exterior region that is disconnected from the original one that the material fell in from). Also, Kerr spacetime, unlike Schwarzschild spacetime, has an inner Cauchy horizon that makes any kind of extrapolation beyond it problematic. And also again, the interior regions of both Schwarzschild and Kerr spacetime are unstable against small perturbations, which means they probably don't actually describe the interiors of physically realistic black holes, at least not well inside the horizon. (Look up "BKL singularity" for an example of a more realistic possibility.)
None of this changes the key points for this discussion: black hole interiors are not static, and they must be almost all vacuum because material falling in doesn't stay in place.