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In order to attain the greatest possible clearness, let us return to ` `
our example of the railway carriage supposed to be travelling ` `
uniformly. We call its motion a uniform translation ("uniform" because ` `
it is of constant velocity and direction, " translation " because ` `
although the carriage changes its position relative to the embankment ` `
yet it does not rotate in so doing). Let us imagine a raven flying ` `
through the air in such a manner that its motion, as observed from the ` `
embankment, is uniform and in a straight line. If we were to observe ` `
the flying raven from the moving railway carriage. we should find that ` `
the motion of the raven would be one of different velocity and ` `
direction, but that it would still be uniform and in a straight line. ` `
Expressed in an abstract manner we may say : If a mass m is moving ` `
uniformly in a straight line with respect to a co-ordinate system K, ` `
then it will also be moving uniformly and in a straight line relative ` `
to a second co-ordinate system K1 provided that the latter is ` `
executing a uniform translatory motion with respect to K. In ` `
accordance with the discussion contained in the preceding section, it ` `
follows that: ` `
` `
If K is a Galileian co-ordinate system. then every other co-ordinate ` `
system K' is a Galileian one, when, in relation to K, it is in a ` `
condition of uniform motion of translation. Relative to K1 the ` `
mechanical laws of Galilei-Newton hold good exactly as they do with ` `
respect to K. ` `
` `
We advance a step farther in our generalisation when we express the ` `
tenet thus: If, relative to K, K1 is a uniformly moving co-ordinate ` `
system devoid of rotation, then natural phenomena run their course ` `
with respect to K1 according to exactly the same general laws as with ` `
respect to K. This statement is called the principle of relativity (in ` `
the restricted sense). ` `
` `
As long as one was convinced that all natural phenomena were capable ` `
of representation with the help of classical mechanics, there was no ` `
need to doubt the validity of this principle of relativity. But in ` `
view of the more recent development of electrodynamics and optics it ` `
became more and more evident that classical mechanics affords an ` `
insufficient foundation for the physical description of all natural ` `
phenomena. At this juncture the question of the validity of the ` `
principle of relativity became ripe for discussion, and it did not ` `
appear impossible that the answer to this question might be in the ` `
negative. ` `
` `
Nevertheless, there are two general facts which at the outset speak ` `
very much in favour of the validity of the principle of relativity. ` `
Even though classical mechanics does not supply us with a sufficiently ` `
broad basis for the theoretical presentation of all physical ` `
phenomena, still we must grant it a considerable measure of " truth," ` `
since it supplies us with the actual motions of the heavenly bodies ` `
with a delicacy of detail little short of wonderful. The principle of ` `
relativity must therefore apply with great accuracy in the domain of ` `
mechanics. But that a principle of such broad generality should hold ` `
with such exactness in one domain of phenomena, and yet should be ` `
invalid for another, is a priori not very probable. ` `
` `
We now proceed to the second argument, to which, moreover, we shall ` `
return later. If the principle of relativity (in the restricted sense) ` `
does not hold, then the Galileian co-ordinate systems K, K1, K2, etc., ` `
which are moving uniformly relative to each other, will not be ` `
equivalent for the description of natural phenomena. In this case we ` `
should be constrained to believe that natural laws are capable of ` `
being formulated in a particularly simple manner, and of course only ` `
on condition that, from amongst all possible Galileian co-ordinate ` `
systems, we should have chosen one (K[0]) of a particular state of ` `
motion as our body of reference. We should then be justified (because ` `
of its merits for the description of natural phenomena) in calling ` `
this system " absolutely at rest," and all other Galileian systems K " ` `
in motion." If, for instance, our embankment were the system K[0] then ` `
our railway carriage would be a system K, relative to which less ` `
simple laws would hold than with respect to K[0]. This diminished ` `
simplicity would be due to the fact that the carriage K would be in ` `
motion (i.e."really")with respect to K[0]. In the general laws of ` `
nature which have been formulated with reference to K, the magnitude ` `
and direction of the velocity of the carriage would necessarily play a ` `
part. We should expect, for instance, that the note emitted by an ` `
organpipe placed with its axis parallel to the direction of travel ` `
would be different from that emitted if the axis of the pipe were ` `
placed perpendicular to this direction. ` `
` `
Now in virtue of its motion in an orbit round the sun, our earth is ` `
comparable with a railway carriage travelling with a velocity of about ` `
30 kilometres per second. If the principle of relativity were not ` `
valid we should therefore expect that the direction of motion of the ` `
earth at any moment would enter into the laws of nature, and also that ` `
physical systems in their behaviour would be dependent on the ` `
orientation in space with respect to the earth. For owing to the ` `
alteration in direction of the velocity of revolution of the earth in ` `
the course of a year, the earth cannot be at rest relative to the ` `
hypothetical system K[0] throughout the whole year. However, the most ` `
careful observations have never revealed such anisotropic properties ` `
in terrestrial physical space, i.e. a physical non-equivalence of ` `
different directions. This is very powerful argument in favour of the ` `
principle of relativity. ` `
` `
` `
` `
THE THEOREM OF THE ` `
ADDITION OF VELOCITIES ` `
EMPLOYED IN CLASSICAL MECHANICS ` `
` `
` `
Let us suppose our old friend the railway carriage to be travelling ` `
along the rails with a constant velocity v, and that a man traverses ` `
the length of the carriage in the direction of travel with a velocity ` `
w. How quickly or, in other words, with what velocity W does the man ` `
advance relative to the embankment during the process ? The only ` `
possible answer seems to result from the following consideration: If ` `
the man were to stand still for a second, he would advance relative to ` `
the embankment through a distance v equal numerically to the velocity ` `
of the carriage. As a consequence of his walking, however, he ` `
traverses an additional distance w relative to the carriage, and hence ` `
also relative to the embankment, in this second, the distance w being ` `
numerically equal to the velocity with which he is walking. Thus in ` `
total be covers the distance W=v+w relative to the embankment in the ` `
second considered. We shall see later that this result, which ` `
expresses the theorem of the addition of velocities employed in ` `
classical mechanics, cannot be maintained ; in other words, the law ` `
that we have just written down does not hold in reality. For the time ` `
being, however, we shall assume its correctness. ` `
` `
` `
` `
THE APPARENT INCOMPATIBILITY OF THE ` `
LAW OF PROPAGATION OF LIGHT WITH THE ` `
PRINCIPLE OF RELATIVITY ` `
` `
` `
There is hardly a simpler law in physics than that according to which ` `
light is propagated in empty space. Every child at school knows, or ` `
believes he knows, that this propagation takes place in straight lines ` `
with a velocity c= 300,000 km./sec. At all events we know with great ` `
exactness that this velocity is the same for all colours, because if ` `
this were not the case, the minimum of emission would not be observed ` `
simultaneously for different colours during the eclipse of a fixed ` `
star by its dark neighbour. By means of similar considerations based ` `
on observa- tions of double stars, the Dutch astronomer De Sitter was ` `
also able to show that the velocity of propagation of light cannot ` `
depend on the velocity of motion of the body emitting the light. The ` `
assumption that this velocity of propagation is dependent on the ` `
direction "in space" is in itself improbable. ` `
` `
In short, let us assume that the simple law of the constancy of the ` `
velocity of light c (in vacuum) is justifiably believed by the child ` `
at school. Who would imagine that this simple law has plunged the ` `
conscientiously thoughtful physicist into the greatest intellectual ` `
difficulties? Let us consider how these difficulties arise. ` `
` `
Of course we must refer the process of the propagation of light (and ` `
indeed every other process) to a rigid reference-body (co-ordinate ` `
system). As such a system let us again choose our embankment. We shall ` `
imagine the air above it to have been removed. If a ray of light be ` `
sent along the embankment, we see from the above that the tip of the ` `
ray will be transmitted with the velocity c relative to the ` `
embankment. Now let us suppose that our railway carriage is again ` `
travelling along the railway lines with the velocity v, and that its ` `
direction is the same as that of the ray of light, but its velocity of ` `
course much less. Let us inquire about the velocity of propagation of ` `
the ray of light relative to the carriage. It is obvious that we can ` `
here apply the consideration of the previous section, since the ray of ` `
light plays the part of the man walking along relatively to the ` `
carriage. The velocity w of the man relative to the embankment is here ` `
replaced by the velocity of light relative to the embankment. w is the ` `
required velocity of light with respect to the carriage, and we have ` `
` `
w = c-v. ` `
` `
The velocity of propagation ot a ray of light relative to the carriage ` `
thus comes cut smaller than c. ` `
` `
But this result comes into conflict with the principle of relativity ` `
set forth in Section V. For, like every other general law of ` `
nature, the law of the transmission of light in vacuo [in vacuum] ` `
must, according to the principle of relativity, be the same for the ` `
railway carriage as reference-body as when the rails are the body of ` `
reference. But, from our above consideration, this would appear to be ` `
impossible. If every ray of light is propagated relative to the ` `
embankment with the velocity c, then for this reason it would appear ` `
that another law of propagation of light must necessarily hold with ` `
respect to the carriage -- a result contradictory to the principle of ` `
relativity. ` `
` `
In view of this dilemma there appears to be nothing else for it than ` `
to abandon either the principle of relativity or the simple law of the ` `
propagation of light in vacuo. Those of you who have carefully ` `
followed the preceding discussion are almost sure to expect that we ` `
should retain the principle of relativity, which appeals so ` `
convincingly to the intellect because it is so natural and simple. The ` `
law of the propagation of light in vacuo would then have to be ` `
replaced by a more complicated law conformable to the principle of ` `
relativity. The development of theoretical physics shows, however, ` `
that we cannot pursue this course. The epoch-making theoretical ` `
investigations of H. A. Lorentz on the electrodynamical and optical ` `
phenomena connected with moving bodies show that experience in this ` `
domain leads conclusively to a theory of electromagnetic phenomena, of ` `
which the law of the constancy of the velocity of light in vacuo is a ` `
necessary consequence. Prominent theoretical physicists were theref ` `
ore more inclined to reject the principle of relativity, in spite of ` `
the fact that no empirical data had been found which were ` `
contradictory to this principle. ` `
` `
At this juncture the theory of relativity entered the arena. As a ` `
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