The evolution of scientific thought from Newton to EinsteinD'Abro, A. (Aram)
Science
The evolution of scientific thought from Newton to Einstein
D'Abro, A. (Aram)
Relativity (Physics); Science -- Methodology
Let us now state the precise nature of those modifications in lengths
and durations which will arise as a result of relative motion. The
Einstein-Lorentz equations show that a rigid material object, say a
yardstick, which, when at rest in our frame, would measure out as one
yard in length, would appear to contract more and more in value in
the direction of its relative motion (FitzGerald contraction) as this
relative velocity increased. Could the relative velocity reach that of
light, the rod would become completely flattened down to nothing.
[Pg 224]
Likewise, an observer fixed to a clock would note that the durations
between the successive second-beats of the clock were truly seconds.
But with an increase in the relative motion existing between clock
and observer, these beats would measure out as lengthened; and for
a relative speed equal to that of light an infinite duration would
separate two successive beats.
It must be noted that this lengthening in the durations defined by
the tickings of the clock must not be attributed to the fact that the
observer is moving farther and farther from the clock and therefore
that longer and longer periods of time are necessary for him to take
cognisance of these tickings. The results mentioned are those which
would be found to hold after all the necessary corrections had been
performed. It is solely the relative motion of the observer and the
clock which is involved, and not the variations in their mutual
distance. Our results would be exactly the same whether we were
approaching or receding from the clock, so long as the same magnitude
of our relative motion was maintained.
It is customary to designate by the names proper length and
proper duration the length and duration obtained by an observer
at rest with respect to the rod or clock. Beginners appear to have
considerable difficulty in convincing themselves that all these
durations, whether proper or elongated, are equally real. We have
already explained in what measure they are so, but it may be helpful to
give the following additional illustration: Suppose we are suffering
from a headache and that this headache lasts an hour when timed by
our watch. This will be the proper duration of the headache.
Now we might be inclined to claim that inasmuch as we alone
are suffering from the headache, we alone are in a position to
determine its duration; and when some rapidly moving observer tells
us that we have held our watch in our hand for one week and that our
headache has therefore lasted a week, we might be tempted to tell him
to mind his own business. But it must be realised that although the
headache is ours and ours alone, and nobody else can feel it for us,
yet the duration occupied by the headache is common property,
and any other observer is just as much entitled to live it and to
measure it as we ourselves are.
[Pg 225]
CHAPTER XXII
AND THE TRIP TO THE STAR
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