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 indices and run from 1 to 3 only.
The
will be such functions of , , as correspond to
a three-dimensional continuum of constant positive curvature. We must
now investigate whether such an assumption can satisfy the field
equations of gravitation.
In order to be able to investigate this, we must first find
what differential conditions the three-dimensional manifold of
constant curvature satisfies. A spherical manifold of three dimensions,
[Pg 110]
embedded in a Euclidean continuum of four dimensions,[19]
is given by the equations
By eliminating , we get
[19]The aid of a fourth space dimension has naturally no significance except
that of a mathematical artifice.
As far as terms of the third and higher degrees in the , we
can put, in the neighbourhood of the origin of co-ordinates,
Inside the brackets are the of the manifold in the neighbourhood
of the origin. Since the first derivatives of the ,
and therefore also the , vanish at the origin, the calculation
of the for this manifold, by (88), is very simple at the origin.
We have
Since the relation
is universally co-variant,
and since all points of the manifold are geometrically equivalent,
this relation holds for every system of co-ordinates, and
everywhere in the manifold. In order to avoid confusion with
[Pg 111]
the four-dimensional continuum, we shall, in the following, designate
quantities that refer to the three-dimensional continuum
by Greek letters, and put
We now proceed to apply the field equations (96) to our special
case. From (119) we get for the four-dimensional manifold,
For the right-hand side of (96) we have to consider the energy
tensor for matter distributed like a cloud of dust. According to
what has gone before we must therefore put
specialized for the case of rest. But in addition, we shall add
a pressure term that may be physically established as follows.
Matter consists of electrically charged particles. On the basis
of Maxwell's theory these cannot be conceived of as electromagnetic
fields free from singularities. In order to be consistent
with the facts, it is necessary to introduce energy terms, not
contained in Maxwell's theory, so that the single electric particles
may hold together in spite of the mutual repulsions between
their elements, charged with electricity of one sign. For the sake
of consistency with this fact, Poincaré has assumed a pressure
[Pg 112]
to exist inside these particles which balances the electrostatic
repulsion. It cannot, however, be asserted that this pressure
vanishes outside the particles. We shall be consistent with this
circumstance if, in our phenomenological presentation, we add
a pressure term. This must not, however, be confused with a
hydrodynamical pressure, as it serves only for the energetic presentation
of the dynamical relations inside matter. In this sense
we put
In our special case we have, therefore, to put
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