In any single coordinate system, such as the FRW system based on cosmological time, by definition it is impossible for accumulated classical Doppler shift to yield the same result regardless of whether SR time dilation is included or excluded, unless the accumulated SR time dilation over the light path equals zero.
Sorry, you lost me. As I tried to explain, in that specific coordinate system, redshift can be calculated without resorting to descriptions like doppler effect or gravitational effects. That doesn't mean in any way that these descriptions cannot yield the same result, e.g. if calculated in a different coordinate system or especially if calculated in a coordinate independent way like the two transport scenarios I described. Coordinates are one thing, physics is another thing. And it's physics that counts, no matter what desription you prefer.
I think you are saying that SR time dilation can be part of the correct answer only if we transform from FRW coordinates to Milne or other non-FRW coordinates.
Well, I think yes. It's simply a different description of the same thing, mot concurring theories.
I don't disagree with that limited conclusion, but I think in the particular context of the point I'm trying to make, it is unhelpful in nailing down the physical kinematic basis for cosmological redshift.
Ah ok, I think I didn't make my personal point of view clear enough: while Bunn and Hogg assert something like they proved that redshift is of kinematical origin, I'd say that they merely showed that it
can be viewed as to be of kinematic origin. Personally, I'd prefer to include second order effects and explain it as a combination of kinematic and gravitational effects, as I said in a previous post. I explicitly refrain from "nailing down" the cause of redshift, I emphasize that different viewpoints are equally valid. And that one should know about as many viewpoints as possible, be it to pick the most appropriate one for a specific problem or simply to extend one's horizon.
And second because no viable alternative global SR coordinate system exists (nor could it exist) which accurately accounts for the effects of cosmic gravitation on worldlines while preserving spatially flat global geometry, homogeneity and isotropy all at the same time.
Well, that's a tautology. Of course SR does not include gravitation. But there are alternative coordinate representations of some FRW spacetimes that do include doppler and gravitational shifts as a "cause" of redshift, without "stretching of space".
Therefore your statement ... cannot be proven in a realistic model.
Hey, it
is proven (I think). It's just a matter of calculus, it must be true.
Vague statements such as that "the underlying symmetries of FRW mathematics" ensure equivalence do not add clarity.
Ok, I'll come back to that later.
(a) any definitive and complete mathematical proof of that equivalence (often the proofs are limited to distances z << 1)
I don't know of such proofs, but a proof limited to z~0 is sufficient.
(b) an explanation how accumulated SR time dilation (or cosmic gravitational time dilation, for that matter) does not logically conflict with the universal clock synchronicity of FRW fundamental observers
Now,
you have to prove that it is in conflict. Synchronicity is coordinate dependent, it's hard to imagine how this could
disprove consequences of different coordinate representations.
(c) an explanation in explicit kinematic terminology of the physical action which causes both the wavelength and the wave packet length to stretch longitudinally in exact proportion to the scale factor.
By changing to a different coordinate system, you exactly give up the symmetries that lead to this result. You can't see it easily anymore. But as the physics is the same, the results
must agree.
And I think it's fair to say that you are the only author I've seen state that accumulated classical Doppler shift can be the sole basis for cosmological redshift.
Ok, but it's trivial that relativistic doppler shift agrees with the classical one in the low speed limit. No big deal.
It is traditional in scholarly works on this subject that the observer's location is considered to be "stationary" as the origin of an FRW coordinate system...
Yes, but Bunn and Hogg explicitly do not use one single coordinate system, but are constantly switching. That's why gravitation is somebody else's problem.
Projectile 1 (P1) is launched at cosmological time t, and Projectile 2 (P2) at t + Delta t. The scale factor increases by 4 during projectiles' journey, so the RW line equation says that P2 arrives at Go at an interval of 4 Delta t after P1's arrival, in Go's reference frame.
That's interesting. I've read this assertion once, in a paper called "http://arxiv.org/abs/0707.0380" ". Now I'm again in the position to contradict a paper: this assertion is wrong.
Let's go back to the symmetry argument I mentioned earlier:
In the standard FRW metric ds²=dt²-a²dr², r does not appear explicitly. That means that at cosmological time t1 you can choose an arbitrary origin r1, start there a particle (say, a bullet), and it will be at r1+Dr at time t2. Consequently a particle started
at the same time at arbitrary r2 under the same conditions will be at r2+Dr. Their comoving distance r2-r1 will not change over time, therefore their "proper distance" a*r will increase with the scale factor. The underlying symmetry is the one concerning transformations r -> r+dr.
If you talk about particles started at the same pale but different times, this symmetry does not apply, except for light, where the speed is constant. Nonrelativistic particles startes under such conditions will simply stay at a constant proper distance. Relativistic particles will increase their distance only as length contraction (wrt the respective observers) gets smaller and smaller, and will eventually maintain constant distance also.
Generally, the main contribution to the increasing distance in the symmetric ~a case is the
relative velocity of the two starting points. If there is no such velocity difference, as in your scenario, the distance will not increase proportional to a.