The Meaning of Relativity: Four lectures delivered at Princeton University, May, 1921Einstein, Albert
Science
The Meaning of Relativity: Four lectures delivered at Princeton University, May, 1921
Einstein, Albert
Relativity (Physics)
of the Newtonian theory must serve as a model. This equation
has its foundation in the idea that the gravitational field
arises from the density of ponderable matter. It must also
be so in the general theory of relativity. But our investigations
of the special theory of relativity have shown that in place of
the scalar density of matter we have the tensor of energy per
unit volume. In the latter is included not only the tensor of
the energy of ponderable matter, but also that of the electromagnetic
energy. We have seen, indeed, that in a more complete
analysis the energy tensor can be regarded only as a provisional
means of representing matter. In reality, matter consists of electrically
charged particles, and is to be regarded itself as a part,
in fact, the principal part, of the electromagnetic field. It is
only the circumstance that we have not sufficient knowledge of
the electromagnetic field of concentrated charges that compels
us, provisionally, to leave undetermined in presenting the theory,
the true form of this tensor. From this point of view our
problem now is to introduce a tensor, . of the second rank,
[Pg 87]
whose structure we do not know provisionally, and which includes
in itself the energy density of the electromagnetic field
and of ponderable matter; we shall denote this in the following
as the "energy tensor of matter."
According to our previous results, the principles of momentum
and energy are expressed by the statement that the divergence
of this tensor vanishes (47c). In the general theory of relativity,
we shall have to assume as valid the corresponding general
co-variant equation. If () denotes the co-variant energy tensor
of matter, the corresponding mixed tensor density, then,
in accordance with (83), we must require that
be satisfied. It must be remembered that besides the energy density
of the matter there must also be given an energy density of
the gravitational field, so that there can be no talk of principles
of conservation of energy and momentum for matter alone. This
is expressed mathematically by the presence of the second term
in (95), which makes it impossible to conclude the existence of
an integral equation of the form of (49). The gravitational field
transfers energy and momentum to the "matter," in that it exerts
forces upon it and gives it energy; this is expressed by the
second term in (95).
If there is an analogue of Poisson's equation in the general
theory of relativity, then this equation must be a tensor equation
for the tensor of the gravitational potential; the energy
tensor of matter must appear on the right-hand side of this
equation. On the left-hand side of the equation there must be
a differential tensor in the . We have to find this differential
[Pg 88]
tensor. It is completely determined by the following three
conditions:—
1. It may contain no differential coefficients of the higher
than the second.
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