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
Inasmuch as these arguments are advanced in a spirit of criticism,
we must presume that according to Dr. Whitehead, had transmissions
other than optical ones been considered, determinations differing from
Einstein’s would have ensued.[59] But a contention of this sort would
be fundamentally untrue. Einstein’s determinations would have yielded
exactly the same results had sound transmissions been substituted for
optical ones; and the only reason optical ones are continually referred
to is because they permit observations of greater accuracy. We shall
now consider the reasons for these statements.
The problem of time determination may be divided into two parts:
First, we wish to define equal successive durations at the same point
of space, for instance, at the point where we happen to be standing.
Secondly, we wish to co-ordinate our time reckonings with those
computed by other observers situated at different points of space.
As we have already considered the problem of time-congruence at a
point, we will not dwell on it unduly. Suffice it to recall that our
direct intuition of time-congruence is far too vague and uncertain to
be of any use in scientific investigation. Accordingly, throughout
the course of history we find men relying on physical processes of
one sort or another, the burning of candles, sand clocks, mechanical
clocks, rotation of the earth, vibrations of atoms, etc. Newton gave
a theoretical definition of time-congruence when he formulated the
law of inertia, according to which a perfectly free body described
equal distances in equal times. According to this definition, by
measuring equal distances along the body’s path, we were enabled to
mark out successive equal durations. But in common practice it was
more convenient to appeal to chronometers regulated ultimately by the
earth’s rotation. We may now pass to the problem of synchronisation in
classical science.
Let us assume that we are in possession of a number of chronometers
which, when placed side by side, beat out their hours, minutes and
seconds in perfect unison, hence advance at the same rate. Suppose now
that having drawn a circle of, say, ten miles’ radius, we maintain
one chronometer at the centre and carry the remaining chronometers to
various points distributed on the circumference of the circle. If some
one were to play a prank and displace the hands of the chronometers
located on the circumference, we should be faced with the problem
of re-establishing synchronism. Classical science suggested various
methods for obtaining this result.
[Pg 181]
First, we might transport our centre chronometer to each of the
circumference chronometers in turn, and thus re-establish synchronism.
But this method was open to the objection that by displacing a
chronometer back and forth we might in some way disturb its working.
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