PeterDonis
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Boing3000 said:OK, you've made up quite a new definition of vacuum (we both now its not, there is at least a singularity, and there is mass anyway)
The singularity is not part of the manifold.
The complete spacetime of a realistic black hole does include a non-vacuum region (occupied by the object that originally collapsed to form the hole). But that does not mean that non-vacuum region is "still inside" the hole forever. I am not changing the definition of "vacuum" at all.
Boing3000 said:we surely can measure the change of the horizon by shooting a laser and seeing if it hit a detector somewhere or elsewhere
This is not a local measurement. It's a global one.
Boing3000 said:We just can compute that all the particle of the universe seems to be at the center of a singularity 13.7 by old.
You're missing the point. The spacetime geometry of the universe as a whole is not the Schwarzschild geometry. It's not even close to that geometry. The Schwarzschild geometry is static outside the horizon and asymptotically flat--i.e., the metric goes to Minkowski at infinity. The spacetime geometry of the universe as a whole is static nowhere and has no "infinity" at all, let alone an asymptotically flat one. The observable universe is a portion of the universe as a whole, but also is static nowhere and has no "infinity". So any numerical similarity between some computation you make about the universe and some computation you make about the Schwarzschild geometry is physically meaningless. It's like saying the point on Earth where the prime meridian meets the equator is "somehow the same" as the origin of a Euclidean plane, because they both happen to have coordinates ##(0, 0)##.