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)
in which the are so small compared to 1 that we can neglect
the higher powers of the and their derivatives. If we do this,
we learn nothing about the structure of the gravitational held, or
of metrical space of cosmical dimensions, but we do learn about
the influence of neighbouring masses upon physical phenomena.
Before carrying through this approximation we shall transform
(96). We multiply (96) by , summed over the and
observing the relation which follows from the definition of
the ,
we obtain the equation
If we put this value of in (96) we obtain
When the approximation which has been mentioned is carried
out, we obtain for the left-hand side,
[Pg 91]
or
in which has been put
We must now note that equation (96) is valid for any system
of co-ordinates. We have already specialized the system of
co-ordinates in that we have chosen it so that within the region
considered the differ infinitely little from the constant values
. But this condition remains satisfied in any infinitesimal
change of co-ordinates, so that there are still four conditions
to which the may be subjected, provided these conditions
do not conflict with the conditions for the order of magnitude of
the . We shall now assume that the system of co-ordinates
is so chosen that the four relations—
are satisfied. Then (96a) takes the form
These equations may be solved by the method, familiar in
electrodynamics, of retarded potentials; we get, in an easily
understood notation,
[Pg 92]
In order to see in what sense this theory contains the Newtonian
theory, we must consider in greater detail the energy
tensor of matter. Considered phenomenologically, this energy
tensor is composed of that of the electromagnetic field and of
matter in the narrower sense. If we consider the different parts
of this energy tensor with respect to their order of magnitude,
it follows from the results of the special theory of relativity that
the contribution of the electromagnetic field practically vanishes
in comparison to that of ponderable matter. In our system of
units, the energy of one gram of matter is equal to 1, compared
to which the energy of the electric fields may be ignored, and
also the energy of deformation of matter, and even the chemical
energy. We get an approximation that is fully sufficient for our
purpose if we put
In this, is the density at rest, that is, the density of the ponderable
matter, in the ordinary sense, measured with the aid
of a unit measuring rod, and referred to a Galilean system of
co-ordinates moving with the matter.
We observe, further, that in the co-ordinates we have chosen,
we shall make only a relatively small error if we replace the
by , so that we put
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