Comment by jodrellblank
Comment by jodrellblank a day ago
> "To maintain consistency with outside observers, this evaporation must occur fast enough that the victim can never reach any surface. Instead, the black hole recedes from them, evaporating faster and faster."
If this is radiating a star's mass worth Hawking radiation particles, is it like the Solar Wind, and if it's happening ever faster is there a point where it would start pushing the victim away from the black hole again? (the 'victim' can be a solar sail if that helps)
I don't think the hawking radiation occurs at the edge of the event horizon itself.
Arvin Ash just did a video on this
https://www.youtube.com/watch?v=UxVssUb0MsA
It appears to occur outside the event horizon in a large area.