The Blackhole of Chapline
Imagine that 2 million light years from our current location is a collapsing shell of radiation, headed towards us. Two million years from now (minus a little bit) that shell will pass within its Schwarzschild radius and a blackhole will reside where we once stood.
But we don’t know that yet. We can’t know that yet. The shell of radiation is well outside our past lightcone. Still, despite our blissful ignorance of the doom that awaits us, an event horizon has already formed here on Earth. Light signal from our present location will never escape to infinity. The existence of this event horizon is a global geometrical statement. When, exactly, it formed depends on the total “mass” of that shell of radiation. And … we don’t know what that is.
For you and me, the horizon is undetectable. There are no local measurements that we can make that will allow us to determine whether the statements of the first paragraph of this essay are correct.
George Chapline, of Livermore National Lab (along with his apparent partner in crime, Bob Laughlin), however, can tell. He claims that when you and I cross the horizon, we can observe all sorts of weird quantum-mechanical phenomena. And the thickness of the region over which these phenomena take place is a function of the mass of the blackhole that will ultimately form.
George’s chums in the Andromeda galaxy can send him superluminal signals by manipulating the “strength” of that collapsing shell (and hence the size of the region over which one observes this quantum criticality).
Normally, I wouldn’t belabour this sort of thing. But I just sat through a Harvard Physics Colloquium by the aforementioned gentleman. It was the most surreal hour I ever spent in Jefferson Laboratory.
Luboš, in his own inimitable style, has more to say on the subject.
Re: The Blackhole of Chapline
Just to play devil’s advocate, what if you replaced `event horizon’ by `apparent horizon’?