

So I did a bit more reading. It seems like acceleration alone is not enough for invoking equivalence principle and saying we have Unruh radiation. If it was enough, non-blackholes objects would Hawking radiate like both of us were suspecting. Apparently physicists are quite confident only blackholes can Hawking radiate.
There is another picture that may work better for us. Instead of thinking of Unruh radiation (which would require doing serious QFT in curved spcetime calculations), we can think of the radiation coming from ripples popping up near the horizon (the black hole horizon for Hawking, the Rindler horizon for Unruh).
In this picture you absolutely need a horizon to get radiation. So on the centrifuge you won’t feel any radiation 🤷♂️
















Technically it’s not really a horizon if it “opens up” allowing you to observe events from the inside afterwards. But of course in any realistic setting (including that experiment) it will open up eventually, so no horizon. But nature doesn’t know that it will open up, so maybe it should behave like a horizon until nature knows, resulting in a criteria like you said. I think the criteria is loosely equivalent to saying “the acceleration must change the speed by almost c”, so your centrifuge probably wouldn’t lead to radiation.
But I really am not sure about any of this. The right way to do this is to actually calculate the mode function. One day when I’m better with QFT and all these stuff I’ll try to do it.