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著者: Albert Einstein

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This proves that the propositions of Euclidean geometry cannot
hold exactly on the rotating disc, nor in general in a
gravitational field, at least if we attribute the length 1 to the
rod in all positions and in every orientation. Hence the idea of
a straight line also loses its meaning. We are therefore not in a
position to define exactly the co-ordinates x, y, z relative to
the disc by means of the method used in discussing the special
theory, and as long as the co-ordinates and times of events have
not been defined, we cannot assign an exact meaning to the
natural laws in which these occur.
[19] Throughout this consideration we have to use the Galileian
(non-rotating) system K as reference-body, since we may only
assume the validity of the results of the special theory of
relativity relative to K (relative to K′ a gravitational field
prevails).

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