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
Viewing the situation as it now stands, we may say that material rods,
visually recognised as rigid, will be taken as norms of measurement
in physical space. In other words, it will be assumed that rods which
coincide when brought together will continue to remain congruent
when transferred, independently of one another, to other regions
of space. Of course, the physicist will guard himself as much as
possible against local contingent influences, such as variations of
pressure and temperature, which might influence the behaviour of his
rods. But when all these elementary precautions have been observed,
the geometry determined by our rods will automatically become the
[Pg 48]
geometry of space. This physical definition of congruence may be termed
practical congruence, as distinguished from theoretical
congruence, which is embodied by the mathematical types we have
discussed.
With his standard rigid bodies defined in this way by physical objects,
the physicist can perform measurements in the space of his frame and
in consequence obtains the numerical results of three-dimensional
Euclidean geometry. Inasmuch as the more careful he is to guard against
such contingent influences as variations of temperature, the more
accurately will his numerical results approximate to those of pure
Euclidean geometry, he feels justified in stating that rigid objects
behave like rigid Euclidean bodies and that the space of our experience
is rigorously Euclidean.
We may also recall that his rigid bodies having been defined, the
definition of a straight line as the axis of rotation of a revolving
solid, two of whose points are fixed, or as the shortest distance
between two points in space, follows immediately; and of course the
straight line thus defined satisfies Euclid’s parallel postulate, since
it is derived from the behaviour of Euclidean solids.
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