JVNY said:
Do you recall our discussion about synchronization for a family of uniformly (Born-rigidly) accelerating observers? Remember that the equivalence principle equally well allows us to think of this as a system of observers at rest at different potentials in a uniform gravitational field. The 4-velocity field of this family is then given simply by ##\vec{u} = \frac{1}{x}(1,0,0,0)## where ##x## is the usual Rindler spatial coordinate. ##\vec{u}## is therefore
everywhere perpendicular to the ##t = \text{const}## surfaces, where ##t## is the usual Rindler time coordinate. If we now
define simultaneity for all observers in this family by ##dt = 0##, then the ##t = \text{const}## surfaces constitute global simultaneity surfaces for all of these observers; what we've done here is use the fact that ##\vec{u}## is
everywhere perpendicular to the ##t = \text{const}## surfaces to smoothly glue together the "local simultaneity surfaces" talked about in post #53 into a global simultaneity surface for the entire family. We can then synchronize all the clocks carried by these observers by readjusting their rates of ticking so that they all read the time coordinate ##t##. Alternatively, one can define simultaneity for each observer by directly applying the Einstein simultaneity convention to all events that can receive light signals from and send light signals to each observer; this is just the Marzke-Wheeler prescription. It just so happens that for uniformly accelerating observers, this prescription gives us back the ##t = \text{const}## surfaces!
But for a family of observers riding on a uniformly rotating disk there are a plethora of problems with regards to the above. We can again consider the observers as being at rest in a certain gravitational field, wherein they have the 4-velocity field ##\vec{u} = \gamma (1,0,\omega,0)## where ##\gamma = \frac{1}{\sqrt{1 - \omega^2 r^2}}## and ##\omega## is the angular velocity of the disk (the coordinates being used are ##(t,r,\phi,z)##). The main problem is that there are
no level sets of the form ##t = \text{const}## that ##\vec{u}## is everywhere orthogonal to; in other words there is no way for us to smoothly glue together the "local simultaneity surfaces" of each observer riding on the disk into a global simultaneity slice for the entire family. This is the result of an important theorem from differential geometry (Frobenius' theorem) which basically states that if ##\vec{\omega} := \vec{\nabla} \times \vec{u}\neq 0##, such a one-parameter family of global simultaneity slices for ##\vec{u}## cannot exist. See post #45. As a consequence, if we now resort to Marzke-Wheeler simultaneity, the observer at the center of the disk has simultaneity surfaces consisting of planes orthogonal to his world line whereas the observers elsewhere on the disk have much more complicated simultaneity surfaces that are in general non-orthogonal to their world lines.
But is there anything that says we
can't use the central observer's simultaneity planes to synchronize diametrically opposite clocks placed on the rim of the rotating disk? No.