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
An elementary illustration of this would be given by considering a
curved surface of two dimensions, such as that of a sphere. On a
sphere we can trace an infinite variety of mesh-systems, but none of
these mesh-systems is made up of equal Euclidean squares. The nearest
approach to a network of squares would be afforded by a mesh-system
[Pg 263]
of meridians and parallels. But even a mesh-system of this sort
could be likened to a network of equal squares only in the immediate
vicinity of the equator. As we examined our mesh-system at regions
farther and farther removed from the equator, we should notice that
the meridians had a tendency to run closer and closer together, so
that the quadrilaterals bounded by the meridians and parallels would
depart more and more in shape from those of Euclidean squares. In the
general case, where we consider an arbitrarily curved surface and no
longer a uniformly curved one, such as a sphere, it could be shown that
the straightest type of mesh-system compatible with the surface was
assimilable to one of squares only around a point, and not, as in the
case of a sphere, along a line (such as the equator). The point could
be selected arbitrarily, and our pseudo-straight mesh-system drawn
around this point accordingly.
We see, therefore, that if space-time is unevenly curved or unevenly
non-Euclidean, the nearest approach to a Cartesian mesh-system around
any given point could be approximately Cartesian only in a restricted
region around this point. As we moved away from this point in our
mesh-system, its curvilinear characteristics would become more and more
pronounced. So far as the ’s of space-time are concerned,
this would imply that in a region where curvature was present these
’s could maintain constant values only in the more or less
immediate neighbourhood of a point. Expressed in terms of fields of
force, this assertion is equivalent to stating that in a region of
space-time curvature it would be quite impossible to rid ourselves of a
field of force throughout space. We might annul it at the point and in
its immediate neighbourhood, but the field of force would reappear for
more distant regions.
Public-domain text, read in full here on John Shaqi.
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