도서 · Relativity
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저자: Albert Einstein
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Since the same light-signal has to be transmitted relative to K′
with the velocity c, the propagation relative to the system K′
will be represented by the analogous formula
x′ - ct′ = 0 . . . . . (2)
Those space-time points (events) which satisfy (1) must also
satisfy (2). Obviously this will be the case when the relation
(x′ - ct′) = λ(x - ct) . . . (3).
is fulfilled in general, where λ indicates a constant; for,
according to (3), the disappearance of (x - ct) involves the
disappearance of (x′ - ct′).
If we apply quite similar considerations to light rays which are
being transmitted along the negative x-axis, we obtain the
condition
(x′ + ct′) = (x + ct) . . . (4).
By adding (or subtracting) equations (3) and (4), and introducing
for convenience the constants a and b in place of the constants λ
and μ where
image038
and
image039
we obtain the equations
image040
We should thus have the solution of our problem, if the constants
a and b were known. These result from the following discussion.
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