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Guillochon said:I don't know if I agree with this. I can think of some really ridiculous ways for the sun to disappear that are HORRIBLY unlikely but not ruled out by relativity. For instance, what if the mouth of a wormhole suddenly opened up and sucked the Sun to the different part of the universe, and then the wormhole instantly evaporated? What if we measure the Sun where it is today, and then, by the uncertainty principle, the next time we measure it it has moved 10 light years away (the odds are incredibly tiny, but still, non-zero). I don't think that GR specifically prohibits these scenarios...and I'm sure there are others that would facilitate the Sun's sudden disappearance.
If you imagined a sphere in 3d space enclosing the sun and the wormhole, the total mass enclosed by the sphere would be the same before and after the sun passed through the wormhole.
I see that you've added the idea that the wormhole "instantly evaporates". This is no more possible than the sun "instantly evaporating".
As far as the wormhole part of the physics goes, here are a few popular references:
http://www.npl.washington.edu/AV/altvw69.html
If a positive electric charge Q passes through a wormhole mouth, the electric lines of force radiating away from the charge must thread through the aperture of the wormhole. The net result is that the entrance wormhole mouth has lines of force radiating away from it, and the exit wormhole mouth has lines of force radiating toward it. In effect, the entrance mouth has now been given a positive electric charge Q, and the exit mouth acquires a corresponding negative charge -Q. Similarly, if a mass M passes through a wormhole mouth, the entrance mouth has its mass increased by M, and the exit mouth has its mass reduced by an amount -M.
Another source:
http://golem.ph.utexas.edu/string/archives/000550.html
An interesting fact about wormholes is that they change in mass as an
object passes through them. To see this, imagine a wormhole connecting
two distinct asymptotically flat spacetimes. In each spacetime, the ADM
mass is conserved. Thus, if we pass an object of mass m through the
wormhole, from A to B, the ADM mass on either side
cannot change. This means that the mass of the mouth A
increases by m and the mass of mouth B decreases by m. In
other words, the wormhole has measured the mass of the object. Note
that this argument applies in any dimension in which the ADM mass makes
sense.
Note that you can read the original Suskind paper and Suskind's own rebuttal to his paper at http://arxiv.org/abs/gr-qc/0504039 http://arxiv.org/abs/gr-qc/0503097. This paper is not directly concerned with the topic, however, though it mentions the particular point I wanted to make, that when a mass passes through a wormhole, the entrance mouth gains the appropriate amount of mass, to satisfy the conservation laws.
The differential conservation law that prevents the sun from disappearing is \nabla_a T^{ab} = 0. This is the differential form of the conservation of energy and momentum. Essentially, you can move the sun around, but you just can't make it vanish.
More formally, as the second reference metions, the point is that the ADM mass (assuming an asymptotically flat background space-time, i.e. an isolated system) is conserved. This is analogous to the way that charge is conserved in classical E&M.
Just because you can imagine things happening doesn't make them physically possible. The proof of the impossibility is in the details of the conservation laws. Conservation of energy in GR is a bit trickier than the conservation of charge in E&M, but it's still not possible to make the sun instantly disappear.
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