Black hole evaporation endpoint

As a black hole radiates it loses mass and gets hotter, so evaporation speeds up toward a final burst. What is left at the end, and how the radiation reshapes spacetime along the way, requires quantum gravity or careful approximations.

Why it matters

The endpoint decides whether information is returned, stored, or lost.

Review

S. Hollands, R. M. Wald, Quantum fields in curved spacetime, Phys. Rep. 574, 1, 2015. https://arxiv.org/abs/1401.2026 reference checked

Timestamp record

Signed record
c6f0f7e9427a…
Public log
Entry 229, in checkpoint 2,123
In the log by
Block 969,698, 2026-10-03

This text was in the PubPhys log by that date. The date says nothing about when the problem was first posed.

4 problems