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)
we have the possibility of getting the relation between naturally
measured lengths and times, on the one hand, and the corresponding
differences of co-ordinates, on the other hand. As the
division into space and time is in agreement with respect to the
two systems of co-ordinates, so when we equate the two expressions
for we get two relations. If, by (101a), we put
we obtain, to a sufficiently close approximation,
[Pg 96]
The unit measuring rod has therefore the length,
in respect to the system of co-ordinates we have selected. The
particular system of co-ordinates we have selected insures that
this length shall depend only upon the place, and not upon the
direction. If we had chosen a different system of co-ordinates
this would not be so. But however we may choose a system of
co-ordinates, the laws of configuration of rigid rods do not agree
with those of Euclidean geometry; in other words, we cannot
choose any system of co-ordinates so that the co-ordinate differences,
, , , corresponding
to the ends of a unit measuring rod, oriented in any way,
shall always satisfy the relation
.
In this sense space is not Euclidean,
but "curved." It follows from the second of the relations above
that the interval between two beats of the unit clock ( = 1)
corresponds to the "time"
in the unit used in our system of co-ordinates. The rate of a
clock is accordingly slower the greater is the mass of the ponderable
matter in its neighbourhood. We therefore conclude that
spectral lines which are produced on the sun's surface will be
displaced towards the red, compared to the corresponding lines
produced on the earth, by about 2 • 10-6 of their wave-lengths.
At first, this important consequence of the theory appeared to
conflict with experiment; but results obtained during the past
year seem to make the existence of this effect more probable, and
[Pg 97]
it can hardly be doubted that this consequence of the theory will
be confirmed within the next year.
Another important consequence of the theory, which can be
tested experimentally, has to do with the path of rays of light.
In the general theory of relativity also the velocity of light is
everywhere the same, relatively to a local inertial system. This
velocity is unity in our natural measure of time. The law of
the propagation of light in general co-ordinates is therefore,
according to the general theory of relativity, characterized, by the
equation
To within the approximation which we are using, and in the
system of co-ordinates which we have selected, the velocity of
light is characterized, according to (106), by the equation
The velocity of light , is therefore expressed in our co-ordinates
by
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