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)
denotes the sun's mass, centrally symmetrically placed
about the origin of co-ordinates; the solution (109) is valid only
outside of this mass, where all the vanish. If the motion
of the planet takes place in the plane then we
must replace (109a) by
[Pg 101]
The calculation of the planetary motion depends upon equation (90).
From the first of equations (110b) and (90) we get,
for the indices 1, 2, 3,
or, if we integrate, and express the result in polar co-ordinates,
From (90), for = 4, we get
From this, after multiplication by and integration, we have
In (109c), (111) and (112) we have three equations between
the four variables , , and , from which the motion of the
planet may be calculated in the same way as in classical mechanics.
The most important result we get from this is a secular
rotation of the elliptic orbit of the planet in the same sense as
the revolution of the planet, amounting in radians per revolution
to
[Pg 102]
where
This expression furnishes the explanation of the motion of the
perihelion of the planet Mercury, which has been known for a
hundred years (since Leverrier), and for which theoretical astronomy
has hitherto been unable satisfactorily to account.
There is no difficulty in expressing Maxwell's theory of the
electromagnetic field in terms of the general theory of relativity;
this is done by application of the tensor formation (81), (82)
and (77). Let be a tensor of the first rank, to be denoted
as an electromagnetic 4-potential; then an electromagnetic field
tensor may be defined by the relations,
The second of Maxwell's systems of equations is then defined by
the tensor equation, resulting from this,
and the first of Maxwell's systems of equations is defined by the
tensor-density relation
[Pg 103]
in which
If we introduce the energy tensor of the electromagnetic field
into the right-hand side of (96), we obtain (115), for the special
case = 0, as a consequence of (96) by taking the divergence.
This inclusion of the theory of electricity in the scheme of the
general theory of relativity has been considered arbitrary and
unsatisfactory by many theoreticians. Nor can we in this way
conceive of the equilibrium of the electricity which constitutes
the elementary electrically charged particles. A theory in which
the gravitational field and the electromagnetic field enter as an
essential entity would be much preferable. H. Weyl, and recently
Th. Kaluza, have discovered some ingenious theorems along this
direction; but concerning them, I am convinced that they do not
bring us nearer to the true solution of the fundamental problem.
I shall not go into this further, but shall give a brief discussion
of the so-called cosmological problem, for without this, the considerations
regarding the general theory of relativity would, in
a certain sense, remain unsatisfactory.
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