Fantasist said:
Thanks for your replies. There appears to have been a bit of a misunderstanding though: I was not trying to involve GR here, but merely the effect of the gravitational field on the usual twin paradox in SR.
Hopefully you now understand that if you don't want to involve GR, you need to use some force other than gravity? I'm not sure if we've made that point clear enough yet from your question.
The idea that gravity is "just a force" is a Newtonian idea. But in GR, gravity causes time dilation. No other "force" does this. To properly model gravity, one needs to consider curved space-time. One can't just "pick and choose" to include parts of GR, and ignore other parts, if one sets up a problem involving curved space time, and expects consistent results, one needs the necessary math. Fortunately, the absolute minimal amount of math that one needs to calculate the time dilation with GR isn't too onerous, it is just the equation I presented in post #6 in this thread.
As has been frequently stated in other threads here before, the clock difference after the return is due to the fact that the traveling twin is not all the time in an inertial frame (i.e. an accelerometer would measure a proper acceleration different from zero), whereas the stay-at-home twin is in an inertial frame. However, if the stay-at-home twin is actually on the Earth's surface, he is in reality not in an inertial frame either (as an accelerometer would confirm). So my question was, if both twins subject to the same proper acceleration over the whole period of time in this sense, would there then still be a clock difference on return (ignoring the GR effect), or would it be equivalent to the case of both twins actually traveling in a symmetrical manner (where no clock difference would be predicted)?
To answer the question in detail, one needs to have the metric of space-time, then apply the formula I gave in post #6. If you just want the answer, we can tell you that having the same magnitude of proper acceleration isn't any guarantee that the proper times will be close. There will be three paths with three proper times (well, in the scneario I envision at least). The first is a true maximum of proper time. It is necessary, but not sufficient, that the path that this observer follows to get the true maximum experiences no proper acceleration. The second path is proper time of someone sitting on the planet, and the proper time of someone who lifts off from the planet, flies around, and returns. The first proper time will be the true maximum by definition. The second proper time will be close to the first for a typical planet). The third proper time can be very much shorter than the second.
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I guess there is one more point to be made. That is that curved space-time is introduced when the non-flat metric is introduced. If you have an observer accelerating in flat space-time, you can still use the flat space-time metric form of the equation I gave in post #6 if you use inertial coordinates. You can choose to use non-inertial coordinates if you wish. You still don't have actual curvature in this case, but the mathematical form of the equations is closer to the form you'll need for full GR when you use the non-inertial coordinates. If you have actual curvature though , due to the presence of a massive body, you have no choice but to use the metric of said space-time, which cannot be reduced to a flat metric, similar to the way it's impoosible to make an accurate flat map of the curved surface of the Earth.