图书 · Relativity
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作者: Albert Einstein
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[21] Cf. Appendixes I and II. The relations which are derived
there for the co-ordinates themselves are valid also for
co-ordinate differences, and thus also for co-ordinate
differentials (indefinitely small differences).
dx2 + dy2 + dz2 - c2dt2 = dx′2 + dy′2 + dz′2 - c2dt′2.
The validity of the Lorentz transformation follows from this
condition. We can express this as follows: The magnitude
ds2 = dx2 + dy2 + dz2 - c2 dt2,
which belongs to two adjacent points of the four-dimensional
space-time continuum, has the same value for all selected
(Galileian) reference-bodies. If we replace x, y, z,
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by x1, x2, x3, x4, we also obtain the result that
ds2 = dx12 + dx22 + dx32 + dx42.
is independent of the choice of the body of reference. We call
the magnitude ds the "distance" apart of the two events or
four-dimensional points.
Thus, if we choose as time-variable the imaginary variable
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