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)
He will notice as he walks about on the disk that he himself and all
the objects on it, whatever their constitution or state, are acted upon
by a force directed away from a certain point upon it and increasing
with the distance from that point. This point is actually the center
of rotation, though the observer does not recognize it as such. The
space on the disk in fact presents the characteristic properties of a
gravitational field. The force differs from gravity as we know it by
the fact that it is directed away from instead of toward a center,
and it obeys a different law of distance; but this does not affect
the characteristic properties that it acts on all bodies alike, and
cannot be screened from one body by the interposition of another. An
observer aware of the rotation of the disk would say that the force
was centrifugal force; that is, the force due to inertia which a body
always exerts when it is accelerated.
Next suppose the observer to stand at the point of the disk where
he feels no force, and to watch someone else comparing, by repeated
applications of a small measuring rod, the circumference of a circle
having its center at that point, with its diameter. The measuring rod
when laid along the circumference is moving lengthwise relatively
to the observer, and is therefore subject to contraction by his
reckoning. When laid radially to measure the diameter this contraction
does not occur. The rod will therefore require a greater proportional
number of applications to the circumference than to the diameter,
and the number representing the ratio of the circumference of the
circle to the diameter thus measured will therefore be greater than
3.14159+, which is its normal value. Moreover the relative velocity
decreases as the center is approached, so that the contraction of the
measuring rod is less when applied to a smaller circle; and the ratio
of the circumference to the diameter, while still greater than the
normal, will be nearer to it than before, and the smaller the circle
the less the difference from the normal. For circles whose centers
are not at the point of zero force the confusion is still greater,
since the velocities relative to the observer of points on them now
change from point to point. The whole scheme of geometry as we know
it is thus disorganized. Rigidity becomes an unmeaning term since
the standards by which alone rigidity can be tested are themselves
subject to alteration. These facts are expressed by the statement
that the observer's measured space is non-Euclidean; that is to say,
in the region under consideration measurements do not conform to the
system of Euclid.
The same confusion arises in regard to clocks. No two clocks will in
general go at the same rate, and the same clock will alter its rate
when moved about.
THE GENERAL PRINCIPLE OF RELATIVITY
Public-domain text, read in full here on John Shaqi.
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