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)
That there are, nevertheless, in the general case, invariant
differential operations for tensors, is recognized most satisfactorily
in the following way, introduced by Levi-Civita and Weyl.
Let () be a contra-variant vector whose components are given
with respect to the co-ordinate system of the .
Let and
[Pg 73]
be two infinitesimally near points of the continuum. For the infinitesimal
region surrounding the point , there is, according
to our way of considering the matter, a co-ordinate system of
the (with imaginary -co-ordinate) for which the
continuum is Euclidean. Let be the co-ordinates of the vector at
the point . Imagine a vector drawn at the point , using the
local system of the , with the same co-ordinates (parallel vector
through ), then this parallel vector is uniquely determined
by the vector at and the displacement. We designate this operation,
whose uniqueness will appear in the sequel, the parallel
displacement of the vector from to the infinitesimally near
point . If we form the vector difference of the vector () at
the point and the vector obtained by parallel displacement
from to , we get a vector which may be regarded as the
differential of the vector () for the given displacement .
This vector displacement can naturally also be considered
with respect to the co-ordinate system of the . If are the
co-ordinates of the vector at , the co-ordinates of
the vector displaced to along the interval (), then
the
do not vanish in this case. We know of these quantities, which
do not have a vector character, that they must depend linearly
and homogeneously upon the and the . We therefore put
In addition, we can state that the must be symmetrical
with respect to the indices and .
For we can assume from
a representation by the aid of a Euclidean system of local co-ordinates
that the same parallelogram will be described by the
displacement of an element along a second element
[Pg 74]
as by a displacement of along .
We must therefore have
The statement made above follows from this, after interchanging
the indices of summation, and , on the right-hand side.
Since the quantities determine all the metrical properties
of the continuum, they must also determine the . If we
consider the invariant of the vector that is, the square of its
magnitude,
which is an invariant, this cannot change in a parallel displacement.
We therefore have
or, by (67),
Owing to the symmetry of the expression in the brackets
with respect to the indices and , this equation can be valid
for an arbitrary choice of the vectors () and only when
the expression in the brackets vanishes for all combinations of
the indices. By a cyclic interchange of the indices , , , we
obtain thus altogether three equations, from which we obtain,
on taking into account the symmetrical property of the
,
[Pg 75]
in which, following Christoffel, the abbreviation has been used,
If we multiply (68) by and sum over the , we obtain
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