MikeGomez
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PeterDonis said:“Yes, but this "lab frame" is not a "local inertial frame" in the sense of the EP. It is localized in space but not in time. The technical term for this "lab frame" is "Riemann normal coordinates". If you look in the mainstream references we gave you, you will see that these are carefully distinguished from "local inertial coordinates". They are not the same thing.”
That I did not know. Thank you.
PeterDonis said:“Just as a note, this "lab frame" is non-inertial. More importantly, the caveats about it not being "local" apply here as well. In this case, since the "lab" is accelerated, the technical term for what you are calling the "lab frame" here is "Fermi normal coordinates". Again, in the mainstream references we gave you, these are carefully distinguished from "local inertial coordinates". They are even different from "accelerated coordinates in a local inertial frame". These are all important distinctions and you need to grasp them if you are going to understand what the mainstream references are saying.”
Blue highlight: That much I know. For the rest, thank you, I did not know that.
PeterDonis said:“In flat spacetime, there is no "gravitational field" except what is produced by the clock's proper acceleration. So if the clock's proper acceleration has a rotating component, the "gravitational field" will have a rotating component, i.e., it will not be uniform. There's no other "gravitational field" to adjust to compensate; spacetime is flat, so there are no other free parameters besides the magnitude and direction of the clock's proper acceleration.”
This I still have an issue with. That is why I was trying to establish the meaning of the relative relationship of a body in its field versus the rest of the universe, and why I was trying to establish the unambiguous terminology for what we mean when we say “gravitational field”.
I feel that the clock does not produce a field due to its proper acceleration, but rather a relative proper acceleration field exists for the clock due to its relative condition with respect to the rest of the universe.”
PeterDonis said:See, this is why I objected to your usage of the term "gravitational field" before. It has misled you into thinking that you can somehow "adjust the gravitational field" of a free-falling clock in flat spacetime. You can't; there's nothing to adjust. The clock is in free fall; the spacetime it is in is flat; there are no free parameters whatsoever that you can use to "adjust the gravitational field"..
Blue highlight: Yes, but at the same time that is why I was trying to establish the correct nomenclature for all the difference types of gravitational fields. For example when people say something along the lines of “gravity disappears for the body in freefall” or curvature is the “real” gravity, that kind of bothers me because we still have gravity in flat spacetime. In fact the flat spacetime gravity is what I would consider “real” because that type of gravity is the type of gravity directly due to the source of gravity as per the equivalence between gravity and inertia. As far as planets and stars go, then yes, curvature gravity is the “real” gravity in this arena.
As for the rest in non-highlighted blue, I was thinking that only the field in the immediate area of the individual lab frames is what is required. That is the only field “felt” by the bodies in their respective lab frames, so I thought as long as the local lab frames fields are correctly simulated (if possible) then that would satisfy the requirements of the experiment. But these issues are probably mute anymore considering we are all talking about the giant Earth frame now.