Easy lessons in Einstein : $b A discussion of the more intelligible features of the theory of relativitySlosson, Edwin E. (Edwin Emery)
Science
Easy lessons in Einstein : $b A discussion of the more intelligible features of the theory of relativity
Slosson, Edwin E. (Edwin Emery)
Einstein, Albert, 1879-1955; Relativity (Physics)
The discovery of the pressure of a beam of light has led to some
startling conclusions. For example, what shall be done with Newton’s
law that action and reaction are equal? When a gun is fired the kick of
the gun is balanced by the momentum of the projectile. When a reflector
throws a beam of light into space, the kick of it is there all right
but where is the projectile, if light is merely the undulation of an
imponderable fluid? We may suppose that the light strikes some dark
body out in space, transmits its impulse to that and Newton’s laws is
satisfied, but it may be a long time before such a body is encountered
and it may never be: at any rate a law that remains in a state of
innocuous desuetude for several thousand years is not good for much.
We must then assume that light has mass since it has inertia and
momentum. But if light has mass it must have weight; that is, it must
be attracted by gravitation. The eclipse observations confirmed this
deduction. Newton would have expected something of this, for he says in
his _Opticks_:[6]
Query 1.--Do not Bodies act upon Light at a distance, and by their
action bend its Rays, and is not this action (_caeteris paribus_)
strongest at the least distance?
The observed deflection of light due to the sun’s gravitation is
greater than Newton would have anticipated but it would have been still
more disconcerting to the nineteenth-century physicists, for in giving
up Newton’s emission theory they had come to regard light as merely a
form of motion in a weightless medium, the ether. Disembodied energy,
like heat and light in ethereal space, was regarded as having no mass
or weight. Twentieth-century physicists are coming to the opposite
view, that the mass of a body is the measure of its internal energy.
If so, mass is not constant but changes with composition, temperature,
structure, electrification and motion.
As Einstein himself expresses it:
It is evident that it is not possible to attribute an absolute
sense to the notion of acceleration, no more than to the notion
of velocity. It is only possible to speak of the acceleration of
a material point in connection with a body taken as the body of
reference. It follows from this that there is no sense in attributing
to a body a “resistance to acceleration” in the absolute sense, like
the resistance of inertia in the classical mechanics. Further, this
resistance of inertia ought to be so much the greater when there is,
in the neighborhood of the body, more inert masses not in accelerated
movement. On the other hand, this resistance ought to disappear when
these masses participate in the acceleration of the body.
Now it is altogether remarkable that the equations of the
gravitational field contain these different aspects of the resistance
of inertia, which one might call the _relativity of inertia_.
Public-domain text, read in full here on John Shaqi.
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