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Fredrik said:Thank you Chris and Pervect for your answers. They are both interesting.
However, I noticed that neither of you answered the question about what kind of objections have been presented against the obvious conclusion. Do they claim a) that GR is needed since acceleration is involved, b) that SR somehow implies that the rope will not break even though it's getting stretched, or c) some other kind of crank nonsense?
I'd say that c) is the closest answer. If you're really curious, check out the talk page, and wade through it:
http://en.wikipedia.org/wiki/Talk:Bell's_spaceship_paradox
I'm not really interested in rehashing these old arguments, and I think Chris is even less interested than I am - I wouldn't be surprised Chris would rather have a root canal without any anesthetic than rehash this again.
So let's forget about those old arguments as a whole (if you bother to read the talk page, and have some SPECIFIC question you want answered, go ahead and ask it though).
But, since there appears to be some interest, let's wipe the slate clean and start some new discussion, hopefully one that is more sensible and even-handed.
I think a lot of the underlying dispute is over distance measures. It seems that everyone has their own ideas on this topic, even excluding the cranks, and that even in the literature we don't see complete unanimity. For instance, their is a paper by Demystifier that talks about these issues that was discussed recently. I like my approach better than his, though :-). While my approach isn't published in any specific papers that I'm aware of, it's inspired by several common textbooks (specifically Wald and MTW).
With these caveats about a lack of complete unanimity in mind, the way I would describe the usual definition of distance would go like this. First, one needs to perform a global 3+1 split of space-time, by assigning every event in space-time a time coordinate. This can be done in many different ways. In the context of special relativity, every inertial frame of reference will have it's own 3+1 split. If two inertial observers in a flat Minkowski space-time are moving with respect to each other, they will assign different events as being simultaneous, generating a different space-time split. Only if two observers are stationary with respect to each other will they arrive at the same space-time split.
There are even more ways to perform a global 3+1 split in GR. The very first thing one must realize is that every different 3+1 split generates a different distance measure.
Given that one has this global 3+1 split, the mathematical process of defining a distance measure then becomes reasonably straightforward. Given this split, one defines a 3-d hypersurface of simultaneity as the set of points sharing the same time coordinate.
The 4-d metric, the invariant "Lorentz interval" will "induce" a 3-d spatial metric on every hypersurface of simultaneity. Any two nearby points on the 3-d hypersurface will have a space-like separation. The value of this space-like separation is just the space-like Lorentz interval between these points calculated via the 4-d metric, or physically by the Lorentz interval, which is an observer independent invariant that does not depend on any choice of coordinates.
Thus, given a global 3+1 split, we can use the Lorentz interval between nearby points to calculate the "induced" metric on the hypersurface, in terms of any convenient spatial coordinates we like.
This gives us a reasonably unambiguous notion of distance between two nearby points at any given "time", where "time" is the global time coordinate that we assigned to every event.
The process of defining a distance between two far-away points is slightly more complex. To define the distance between two far-away points, one must specify a specific curve connecting them. The length of this curve can be calculated by calculating the distance between each pair of nearby points on the curve (as above) and adding them together, i.e. via an integral.
The usual curve chosen is one which lies entirely in one particular hypersurface of simultaneity defined by the global 3+1 split, and it is a geodesic on that hypersurface - i.e. the curve generally comprises the set of points that gives the "shortest distance" between two points when the connecting curve is constrained to lie entirely within the hypersurface of simultaneity.
Here is where one must pay close attention, to make sure that this is indeed the curve being used to compute the distance by any particular author. It seems like the "obvious" choice, at least to me, but sometimes people (for whatever reason) don't make this "obvious" choice. So beware when you read a paper.
In curved geometries, you may have to worry about the fact that there can in general be more than one geodesic between any two points. For instance, on the surface of the Earth at the equator, is that coffee cup 1 meter to your west, or 40075159 meters to the east :-).
OK, this was the general approach. Now let's go to specifics. If we have an accelerated point-like observer, I suggest from my general analysis above that we have to first define some notion of simultaneity in order to be able to define distances. How do we do this? While there are many possible choices, one of the most common choices is to chose at any given instant, the notion of simultaneity of an instantaneously co-moving inertial observer as the appropriate notion of simultaneity for the global time coordinate 't'. This choice, when elaborated, ultimately winds up with the usual "Rindler" coordinates for an accelerated observer.
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