Once you get started on a path, you have to follow it to the end. In rigorous
derivations, the original assumptions led to another
surprising result: lengths are also depending on the motion of the objects, so
that if an object has a length ls when stationary, when in motion it will
have a length given by
From the relativity formulae, one can see that unphysical things happen
(i.e. infinities are encountered) when an object was to increases its velocity
up to the speed of light. On the other side, Newtonian physics tells us that,
if we apply a constant force to a body, its velocity will keep increasing
and eventually reach and exceed the speed of light. How can we resolve
this inconsistency? Again the correct application of the relativity formulae
would give us the answer: another necessary consequence of the starting
assumptions is that the mass of an object depends on its velocity, according to:
General Relativity
Another way to picture the effect of accelerations is to think of what
happens when you are in an elevator. When the elevator is at rest, you feel an
attraction force towards the floor proportional to your weight, but when the
elevator starts moving (i.e. it has an acceleration) you feel yourself pushed
against the floor by a stronger force, i.e. it is as if gravity
had become stronger.
As revolutionary as these concepts were, they made a very strong prediction that
could be verified experimentally: if the space around a massive object is
warped, then its effect should be felt by any body travelling by it, including
a massless entity like light. In Einstein's view, light should be
affected by gravitation, and this is clearly in contrast with Newton's law,
which predicts that gravitation is only felt by objects with a mass.
In Einstein's words, he used to imagine how the world would appear to him
if he was to move at the speed of light : in a "gedanken experiment"
(a thought experiment) he described how looking at the time shown by a clock
at rest, and moving away from it at the speed of light, he would always see the
clock marking the same time, since he would always be moving together with the
light photons emitted by the clock at the time he went by it.
Time, as shown by the clock at rest, would then appear to have stopped, while
instead a watch carried in his hand would still tick away: time does depend on
the relative state of motion between clock and observer !!
As a more detailed example we can consider the "light clock" described in the
book : from the point of view of an observer at rest, when the clock is in
motion light has to travel longer distances to go to and from the mirror.
Assuming that the speed of light is always the same, the separation between
ticks for the moving clock is larger: time is passing more slowly for objects
in motion...
As counter-intuitive as such a result might be, it has been confirmed in
experiments performed with real, very precise, atomic clocks, and is
verified continuously in the behaviour of unstable elementary particles
generated by cosmic rays or particle accelerators. The lifetime of unstable
particles moving at extremely high velocities is stretched
consistently with the predictions of Einstein's relativity.
If we believe in the theory, and there is no reason not to believe in it, then
we can assume that similar effects will apply also to living organisms: an
astronaut leaving earth and travelling at extremely high velocities, will age
more slowly than people left on the earth. More precisely, his clocks, both
mechanical and biological, will tick more slowly than a clock on earth.
If he was away for 1 year, as measured on his clock, many years would instead
have elapsed on earth...
Einstein's theory allows to give precise formulae for time dilation.
We will skip the derivation on pages 442-445, and just give the final result:
if tm is one unit of time (i.e. the time between ticks) for the clock moving
with velocity v, and ts is the time between ticks for the stationary clock,
one has:
It is easy to estimate that, as long as we are dealing with velocities typical
of our daily lives, the time dilation effect is practically un-measurable.
Example: how much slower is the time flow if we move on a super-sonic plane at
about 1000 km/hour?
The next step is to see how we can reconcile the galileian transformation of
velocities between moving frames with the requirement that the velocity of
light is frame-independent. Relativity tells us that, if
an object is moving with velocity v with respect to a frame which is itself
moving with velocity u, then the velocity V of the object as measured by an
observer at rest is
The relativity rules we have discussed so far represent the "easy" part of
Einstein's theory, since they only handle the case of uniform motions (i.e.
motions with constant velocity); since it refers to a special case, the theory
goes under the name of Special Relativity. Einstein's next endeavour
was to work out the most
general case, i.e. the case of motions with arbitrary accelerations. The more
complete theory is known as General Relativity, and it is equally
revolutionary, since it introduces a complete new way to look at the universe.
Like before, we will only present the introductory arguments that form the base
for the theory, and then mention its most remarkable consequences.
The starting point is the realization that forces and accelerations are
indistinguishable. Newton's law, F=ma, had already recognized a correlation
between force and acceleration, but Einstein's reasoning went a step further.
The standard argument is the following :
suppose that, while standing in a room you drop an object: if you are on
earth, the object will fall with constant acceleration g. You
interpret this by saying that there is a force (the gravitational
force in this case) acting on the object and causing it to accelerate towards
the floor. Suppose now that the room you are in is somewhere in outer space,
inside some vessel moving with constant acceleration g: if you drop the object,
the floor of the room will move towards it with acceleration g, and the effect
will be the same as if it had fallen because of the gravity.
The consequence of this type of resoning, as Einstein correctly pointed out,
is that, in principle, we have no way to state whether certain effects are
caused by a force or an acceleration: if the room where we drop the object has
no windows, and we do not know where we are, we would have no way to tell
whether the object is falling to the floor because of gravity, or whether the
floor is coming towards it because it is accelerating...Given then that we have
no way of telling whether forces are at play, we might as well get rid of the
concept of force !!
Still, it is a fact that massive objects influence each other via what Newton
had called the gravitational force, so how is this effect explained in General
Relativity? Simple replies Einstein, a massive object affects the motion of
other objects not because it exerts a force upon them, but because massive
objects cause a deformation in the space around them. The earth is circling
around the sun not because it feels the sun's attraction, but because that is
the expected trajectory in the warped space-time around the sun.
The experimental test was done in 1919 (there were plans for earlier tests, but
World War I had caused an interruption in scientific research). The idea was to
compare the apparent position of stars when their light did or didn't go near
the sun. To do the measurement, one had to wait for a total solar eclipse, so
that stars would be visible even when their position was "behind the sun".
The measurement was done, and it fully confirmed Einstein's theory.
More recently, other accurate verifications of the predictions of General
Relativity were performed. If light is affected by gravitation, then light
moving away from the earth should lose energy. But, when losing energy, light
cannot change its velocity, since it always travels at speed c : light loses
energy by changing its frequency (remember E=h), so that light moving
away from the earth will be slightly red-shifted. Again this effect
was verified experimentally, to confirm the validity of General Relativity.