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저자: Albert Einstein

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proportional to it. Under these conditions, the natural laws
satisfying the demands of the (special) theory of relativity
assume mathematical forms, in which the time co-ordinate plays
exactly the same role as the three space co-ordinates. Formally,
these four co-ordinates correspond exactly to the three space
co-ordinates in Euclidean geometry. It must be clear even to the
non-mathematician that, as a consequence of this purely formal
addition to our knowledge, the theory perforce gained clearness
in no mean measure.
[14] Cf. the somewhat more detailed discussion in Appendix II.

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