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
Consider, for instance, the length of an object, or again the
comparison of two lengths situated in different parts of space. We
have seen, when discussing mathematical space, that according to our
measuring standards, which were conventional, these lengths might be
equal or unequal; and it was this aspect of relativity which expressed
the fundamental mathematical relativity of length. But we also saw that
although in theory the definition of congruence was conventional, in
practice, if we wished to define congruence so as not to enter into
conflict with our sense perceptions, a definite type of congruence
(practical congruence) was imposed upon us by nature. We saw further
that bodies which were thereby defined as congruent constituted what
are known as Euclidean solids, and that these were assumed to remain
absolute in length, regardless of the observer’s motion.
Under these circumstances, when a physicist such as Einstein, in
contradistinction to a mathematician, asserts that length is relative,
he is referring to the actual length measured out by a so-called
rigid body; and he wishes to imply that this length will turn out
to be indeterminate and to depend essentially on our conditions of
observation. We see, therefore, that the relativity of the physicist
is not inevitable, as is that of the mathematician. It is not an
a priori type of relativity expressing a trivial relativity to
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standard. It is essentially an empirical type of relativity, always
subject to proof or disproof by precise empirical tests. The two
following illustrations may be helpful:
Consider a telegraph pole rising vertically from the ground. The visual
angle under which this pole will appear to us is essentially relative,
since it varies in value with the distance of the observer from the
pole. Of course, this visual angle is fundamentally relative, since
its value depends on the system of geometry we may adopt, but we are
no longer discussing this mathematical aspect of relativity. We are
assuming that our system of measurements has been fixed according
to the requirements of practical congruence, i.e., that our
measurements are performed with ordinary rigid rods and hence are
Euclidean. In this event the visual angle under which we perceive a
given pole is perfectly determinate when our distance from the pole
is specified. But, on the other hand, it is relative, inasmuch as it
is not immanent in the pole; it varies with our relative distance
and thereby reduces to a mere relationship between the pole and our
distance therefrom.
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