Einstein's Theories of Relativity and Gravitation: A selection of material from the essays submitted in the competition for the Eugene Higgins prize of $5,000Bird, J. Malcolm (James Malcolm)
Philosophy
Einstein's Theories of Relativity and Gravitation: A selection of material from the essays submitted in the competition for the Eugene Higgins prize of $5,000
Bird, J. Malcolm (James Malcolm)
Relativity (Physics)
Let us consider a circular disc rotating with a uniform peripheral
speed. According to the deductions from the "special theory" of
relativity, an observer situated near the edge of this disc, but not
rotating with it, will observe that units of length measured along
the circumference of the disc are contracted. On the other hand,
measurements along the diameter, which is at right angles to the
direction of motion of the circumference, will show no contraction
whatever, and, consequently the observer will find that the ratio
of circumference to diameter has not the well known value 3.14159
... but exceeds this value, the difference being greater and greater
as the peripheral speed approaches that of light. That is, the laws
of ordinary geometry no longer hold true.
However, we know other cases in which the ordinary or Euclidean
geometry is not applicable. Thus suppose that on the surface of a
sphere we describe a series of concentric circles. Since the surface
is curved, we are not surprised at finding that the circumference of
any one of these circles is less than 3.14159 ... times the distance
across the circle as measured on the surface of the sphere. What
this means, therefore, is that we cannot use Euclidean geometry to
describe measurements on the surface of a sphere, and every schoolboy
knows this from comparing Mercator's projection of the earth's surface
with the actual representation on a globe.
When we come to think of it, the reason we realize all this is
because our sense of three dimensions enables us to differentiate
flat surfaces from those that are curved. Let us, however, imagine
a two-dimensional being living on the surface of a large sphere. So
long as his measurements are confined to relatively small areas he
will find it possible to describe all his measurements in terms of
Euclidean geometry. As, however, his area of operation increases
he will begin to observe greater and greater discrepancies. Being
unfamiliar with the existence of such a three-dimensional object as
a sphere, and therefore not realizing that he is on the surface of
one, our intelligent two-dimensional being will conclude that the
disturbance in his geometry is due to the action of a force, and by
means of plausible assumptions on the "law" of this force he will
reconcile his observations with the laws of plane geometry.
Public-domain text, read in full here on John Shaqi.
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