The Meaning of Relativity: Four lectures delivered at Princeton University, May, 1921Einstein, Albert
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The Meaning of Relativity: Four lectures delivered at Princeton University, May, 1921
Einstein, Albert
Relativity (Physics)
The case that we have been considering is analogous to that
which is presented in the two-dimensional treatment of surfaces.
It is impossible in the latter case also, to introduce co-ordinates
on a surface (e.g. the surface of an ellipsoid) which
have a simple metrical significance, while on a plane the Cartesian
co-ordinates, , , signify directly lengths measured by a
unit measuring rod. Gauss overcame this difficulty, in his theory
of surfaces, by introducing curvilinear co-ordinates which,
apart from satisfying conditions of continuity, were wholly arbitrary,
and afterwards these co-ordinates were related to the
metrical properties of the surface. In an analogous way we
shall introduce in the general theory of relativity arbitrary co-ordinates,
, , , , which shall number uniquely the space-time
points, so that neighbouring events are associated with
neighbouring values of the co-ordinates; otherwise, the choice
of co-ordinates is arbitrary. We shall be true to the principle
of relativity in its broadest sense if we give such a form to the
laws that they are valid in every such four-dimensional system
of co-ordinates, that is, if the equations expressing the laws are
co-variant with respect to arbitrary transformations.
The most important point of contact between Gauss's theory
of surfaces and the general theory of relativity lies in the metrical
properties upon which the concepts of both theories, in the
main, are based. In the case of the theory of surfaces, Gauss's
argument is as follows. Plane geometry may be based upon the
concept of the distance , between two indefinitely near points.
The concept of this distance is physically significant because
the distance can be measured directly by means of a rigid measuring
rod. By a suitable choice of Cartesian co-ordinates this
[Pg 65]
distance may be expressed by the formula .
We may base upon this quantity the concepts of the straight
line as the geodesic (), the interval, the circle, and the
angle, upon which the Euclidean plane geometry is built. A
geometry may be developed upon another continuously curved
surface, if we observe that an infinitesimally small portion of the
surface may be regarded as plane, to within relatively infinitesimal
quantities. There are Cartesian co-ordinates, , , upon
such a small portion of the surface, and the distance between
two points, measured by a measuring rod, is given by
If we introduce arbitrary curvilinear co-ordinates, , , on the
surface, then , , may be expressed linearly in terms of
, . Then everywhere upon the surface we have
where , , are determined by the nature of the surface
and the choice of co-ordinates; if these quantities are known,
then it is also known how networks of rigid rods may be laid
upon the surface. In other words, the geometry of surfaces may
be based upon this expression for exactly as plane geometry
is based upon the corresponding expression.
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