Chalnoth said:
...
However, there is a sort of asymmetry in the way we detect other galaxies. For a galaxy currently receding at faster than the speed of light, they will never observe us at all. They can observe our distant past, but they can never observe our present. Similarly, we observe their distant past. So it turns out to be a bit of an over-simplification to just say that they see what we see. It's true in a way, but it neglects the fact that we have moved out of our respective horizons.
Chalnoth, I'm going to pick a nit. On the whole, nearly 100% you are doing a great job patiently and accurately answering Radrook's questions.
The nit is that you KNOW that there are galaxies just slightly beyond the Hubble radius, receding just slightly faster than c, that we could send a signal to, today, and it would get there. We've talked about it before, I just don't recall in what thread. I suspect you are one of a number of us who've taught that to newcomers and explained how it can happen. So in this case you are oversimplifying when you suggest it can't happen. It "almost can't" but just barely can.
Anyway thanks for the patient hard work. You and Brian Powell and others are doing a great job.
====================
For anybody else, not familiar with this effect, let's use Jorrie's model and try z = 1.45.
You should get the recession speed is >c. Yes something like 1.02c
Google "cosmocalc 2010" to get the calculator and put 1.45 in the z box.
The point is that the Hubble radius, which is currently around 14 billion LY, is expected to extend out to around 1/sqrt(0.73) of that as matter density thins out. Please correct me if I'm wrong, anybody!
So you calculate 14/sqrt(.73) and get 16.4.
So if, today, a guy in a z=1.45 galaxy sent us a message, say a photon, that photon would only be drifting away at rate 0.02c. So it would basically be hanging around at distance about 14 billion LY from us for ages and ages. Its speed towards us barely almost matching the expansion of distance.
Eventually the Hubble radius has to grow from 14 to 16, so it would reach out and take the photon into our Hubble sphere, and then it would be smooth sailing and the photon would make steady progress and eventually get to us. This isn't a detailed quantitative argument, it's just intuitive and conceptual, but I hope anyone who is interested can see how would work.