stilt said:
Summary:: Expansion over collapse
If galaxies are now expanding away faster than light, then how would we know if this has now started to slow, stop and or reverse ? Is there a chance we may never know and the universe collapse won't be seen coming ?
Beyond a certain distance, every galaxy we can observe is now and always has been receding at faster than the speed of light. This includes most of the observable galaxies.
This sounds weird, but the fact is that in General Relativity, there is no well-defined notion of relative speed between different locations. Which means that the speed you get depends critically upon how you define your terms. In this case, the speed being talked about is rate of change in proper distance.
And we can observe galaxies that are now and always have been moving faster than the speed of light simply because they were much closer when that light was emitted, and the rate of expansion has slowed down over time. As a photon started to travel towards us from such a galaxy, at first the distance between us and that photon grew: it would move in our direction, but slower than the universe between us and the photon would expand. Eventually, the rate of expansion slowed to the point that the photon started making ground instead.
The photon by this time will have traveled a good distance away from its source galaxy. With the larger distance between us, the expansion is carrying that galaxy away faster than the now-closer photon. So the galaxy can keep moving away at faster than light while the photon eventually does reach us.
Note that in the far future, when the universe's expansion is dominated by the cosmological constant, the expansion itself will be a constant so this will no longer occur: once a galaxy starts receding at faster than light in such a universe, we no longer receive any new light from that galaxy. We continue to see light from the galaxy for a long time, but none of it from after the point it crossed that horizon.
Our universe is not currently dominated by the cosmological constant, but there is still just such a horizon (it's just way more complicated to calculate). And all of the galaxies which have always been moving faster than the speed of light away from us have, I'm pretty sure, moved past that horizon long ago. So we can never see those galaxies age beyond a certain point. Their light will just redshift away until we can't observe them any longer, similar to what happens when an object enters a black hole.
