Phrak said:
So the moral of the story is, don't use stock quotes for coordinates or don't confuse temperature with time. Which begs the question, what constitutes 'good' coordinates.
If an observer A wants to set up a "physical" coordinate system at event E.
1. Find an inertial observer B who is momentarily stationary, relative to A, at event E. An observer is inertial if they are free-falling i.e. they carry an accelerometer that measures a constant proper acceleration of zero. B is the "co-moving inertial observer" at E.
2. Observer B sets up a (local) coordinate system using his proper-time clock and a lattice of relatively-stationary clocks all synchronised to his using Einstein's synchronisation convention; and measuring distance by radar.*[/color]
3. Observer A makes local measurements near event E by asking B to make the measurement on her behalf. "Near" means over ranges where spacetime curvature can be ignored and any relative acceleration between A and B can be ignored. This rough statement can be made mathematically precise through calculus.
Under these conditions, A will measure the speed of light at E to be
c. However, if she extrapolates her coordinate system to "non-local" events, she may calculate that the speed of light somewhere other than E takes a different value. The extrapolated coordinate system is no longer a "physical" coordinate system (except at E).
It's possible to set up coordinate systems (using time, distance or related quantities such as angle, but not unrelated quantities such as temperature) that don't coincide with "physical" coordinates anywhere.
When studying black holes, it's traditional to use a spherical polar coordinate system extrapolated from a "stationary" observer notionally "at infinity". Such a coordinate system never
exactly coincides with a "physical" coordinate system as defined above, but at very large distances the difference is negligible.
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*[/color]It has just occurred to me that by specifying in step 2 that distance is measured by radar, the "physical" speed of light is
c by definition. This corresponds to the modern-day definition of the metre. However we could instead say that B uses stationary rulers to measure local distance. It's an experimentally verified hypothesis that ruler distance and radar distance are locally the same for inertial observers.