Looking forward to your return. Have a pleasant trip!
Thanks. We've been to http://www.ferienhof-rosenlehner.de/bauernhof.html" , but sadly there were not enough possibilities for my youngest son to practice his skills as a farmer - which he is determined to become. Still, a beautiful place.
Ich said:
There's only one thing you omit, and it throws you off the curve in your later analysis: You have to pick an origin, the preferred point without proper acceleration.
I find this an odd statement. In a FLRW universe, most significant objects are at rest with the Hubble flow and nothing has proper acceleration in the cosmological sense. When we see a distant galaxy moving away from us at some great velocity and even if we acknowledge dark energy or the cosmological constant, neither the distant galaxy or ourselves have proper acceleration with respect to each other, not the kind you can measure with an accelerometer anyway. Both the distant galaxy and ourselves will appear to be approximately at rest with respect to the CMBR.
Everything you say is true, but IIRC we've been talking about the chain of observers who are mutually at rest in this case. Such observers are not comoving, and if there is gravity, all but one will experience proper acceleration.
You'll have to define an origin for that chain. The origin will be moving inertially, all other elements generally won't.
Ich said:
I was hoping for a more detailed counter argument than "don't use it" and "forget about it" to my argument.
I thought I did, in the subsequent paragraph.
The redshifts in a chain of "stationary" observers are
not reciprocal, as they should be if we're talking about a change in time only.
Further, they are independent of expansion or contraction. They only depend on the local mass density, not its time derivative.
Is it relevant if there is neither expansion nor contraction? (i.e a static universe). I can see a spatial potential in a finite universe where clearly objects "near the edge" will have a different potential to objects near the centre, but in an infinite universe, there is no such thing as a centre or a near the edge. You have not made it clear (to me anyway) whether you are talking baout finite or infinite models.
I'm talking about infinite models, too. But if you want to use the well-known potential, you'll have to pick an origin and use quasistatic coordinates in its vicinity. In expanding FRW coordinates, there is no potential.
Ich said:
Yes, I understood. This doesn't work. The redshift indeed comes from a PLACE where the potential is lower.
I still don't get this. In an infinite homogeneous universe, WHERE is this PLACE with a lower potential?
The place with extreme (max or min) potential is just where you pick the origin of the chain of stationary observers. Pick another origin, and there will be a different potential. But it doesn't matter for your calculations.
But your idea of a "temporal potential" has some merit: In FRW coordinates, the scale factor is the equivalent of a potential in static coordinates.
The former is a scale of position as a function of time, while the latter is a scale of time as a function of position.
The former defines changes in momentum, the latter defines changes in energy.
That said, the word "potential" usually does not refer to somthing like a scale factor, and I'm not sure if this would be a good idea.
But ok, there are the complementary pairs: time - position, energy - momentum, potential - scale factor.
Just how much drag does the Hubble flow apply to an object that is not at rest with the Hubble flow? I would suggest none or very little.
Right. The Hubble fow in itself is a property of a family of observers, not a property of spacetime. It cannot possibly exert some kind of drag (usual disclaimer for nitpickers:, except for higher order corrections in the presence of mass).
For local physics, it is irrelevant whether there is outward, inward, or no Hubble flow at all. The Hubble flow is then nothing but the average motion of galaxies.
It is our experience that an object with a peculiar local velocity continues to move with velocity and is not subjected to any drag bringing it to rest with the CMBR.
Nope. Peculiar velocities tend to die out, but that's a sorting effect, not a force or drag. If something has peculiar velocity, it will simply move to a place where it hasn't.
I agree with this conclusion, but it makes your head hurt to think of a wire physically connecting here and now at one end and the big bang at the other end. Ouch!
Well, it's not so painful if you remember that the wire is not exactly a "physical connection". In the wire's frame, all its components are spacelike separated, and the supposed fate of its ends is really irrelevant for what's happening here and now.