andrewkirk said:
George that is a really beautiful piece of reasoning you have written. It's a long time since I read something so technical that I understood first time and by which I was convinced. It should be pinned in a FAQ or something like that, so it doesn't get lost.
Thanks.
Lino said:
Thanks Andrew. That makes sense. May I ask a follow-up question, which I hope is still on topic, but if not please feel free to ignore? If you consider an observation (of, say, a distant galaxy, rather than a signal between observers), I appreciate that individual observations will still be of reasonably short intervals, but what about the comparison between observations from one day to the next, or one week to the next, or one year to the next. Is the logic still sound?
I don't know what you mean by "Is the logic still sound?"
If we watch a given galaxy over a long period, then, at any given time, redshift will be given by
z = \frac{R \left( t_o \right)}{R \left( t_e \right)}-1,
but z will change over time because t_o (for us) and t_e (for the observed galaxy) both change over time. If we could directly observe this effect, it would be a fantastic way to test our models of the universe!
We are close to being able to do this, but, for economic and other reasons, such a project won't start for several decades. Once started, the project would take a couple of decades to start to get good results. From
http://arxiv.org/abs/0802.1532:
we find that a 42-m telescope is capable of unambiguously detecting the redshift drift over a period of ~20 yr using 4000 h of observing time. Such an experiment would provide independent evidence for the existence of dark energy without assuming spatial flatness, using any other cosmological constraints or making any other astrophysical assumption.
Also, redshifts of individual objects don't necessarily increase with time. Figure 1 from the above paper plots redshift versus time. The three red curves are for objects in our universe. As we watch (over many years) a distant, high redshift object, A, we will see the object's redshift decrease, reach a minimum, and then increase. If we watch a much closer, lower redshift object, B, we see the object's redshift only increase.
Roughly, when light left A, the universe was in a decelerating matter-dominated phase, and when light left B, the universe was in the accelerating dark energy-dominated phase.