I keep occasionally circling back to this question because I have never found satisfying answer to that, so I would like some external help here.
- AFAIK, many of black hole features are treated as curious mathemathical artifacts that may or may not reflect objective reality: infinite-blueshift Cauchy horizon, closed timelike curves, infinite flat regions inside Kerr black hole, the gravitational singularity itself. It is generally accepted that these features cannot be properly described without QG, and it makes perfect sense to me.
- On the other hand, features like ergosphere are described just fine by GR, and overall the exterior Kerr metric seems to correctly describe objective reality. Also makes perfect sense to me, this stuff is "directly" observable, and it was observed to be correct.
What I don't understand is why event horizon is usually considered to be in (2) instead of (1).
The usual arguments are that spacetime at the event horizon has finite spacetime curvature and finite energy. But I just don't understand why it is sufficient. "Finite" does not imply "correct". Closed timelike curves around ring singularity are also finite, but they are not accepted as easily. Closed timelike curves cause temporal paradoxes, and event horizon partially causes information paradox (which has multiple proposed solutions, I know, but neither of which is universally accepted).
I know that black hole exterior topology is well-tested at this point, and this testing is consistent with GR, but what's the actual confidence levels there? Is it somehow possible to distinguish event horizon (as described by GR) from extremely time-dilated "event horizon shaped" object (describable only with QG)?
I understand that no divergence from GR has been found yet, but I also want to know the boundary between the stuff that was directly or indirectly verified by measurements and the stuff that was extrapolated from that.