Now, for a ray of light going away in the form of sinusoidal
waves, we can choose
l
= (x-ct),
by observing the particular x which is
l far away from ct. So,
l˘
= x˘
-
ct˘
=
l[Ö{(c+v)/(c-v)}].
Hence,
n˘
=
n[Ö{(c-v)/(c+v)}].
This is called relativistic Doppler’s effect. The
notion of relative velocity also changes in
relativity. From Lorentz transformation,
x˘/t˘
= (x-vt)/(t-vx/c2)
Put x/t = u, velocity of a particle measured in frame L. We
get u˘, the velocity of the same particle measured in frame L˘,
as:
u˘
= (u-v)/(1-uv/c2)
These relations are sufficient to take a very different form.
In his papers, Einstein gave another important result,
the energy-mass relativity.
Mass
transforms as:
m
® m0/{Ö(1-v2/c2)}
We can easily derive the relation for energy from it:
E = m0c2/{Ö(1-v2/c2)}
by using dE = Fdx = (dP/dt)dx = vdP and p = m0v/{Ö(1-v2/c2)}.
The quantity m0c2 is looked at as the
potential energy of the particle. So, kinetic energy =
E
-
m0c2 = m0c2[1/{Ö(1-v2/c2)}
– 1].
For approximation, kinetic energy = m0c2[1
+ (1/2)(v2/c2) – 1] = (1/2)m0v2.
These quantities
-
momentum and energy also follow transformation rules:
p
® (p-vE)/
/{Ö(1-v2/c2)}
E˘
®
(E-vp)/{Ö(1-v2/c2)}
And, they follow the relation:
p2 = E2/c2
= constant,
where,
constant = -m02c2 (as
we see when velocity = 0).
This implies that E2 = p2c2
+ m02c4.
Now, look at the relation x˘2
-
c2t˘2
= x2
-
c2t2. A quantity x2
-
c2t2, which is a function of x
and t, i.e., coordinates) is invariant in relativity.
Doesn’t this look something like some form of
Pythagoras Theorem? This was the insight of Hermann
Minkowski, the former teacher of Einstein. He said
that x2
- c2t2 represented length in some form
of space-time system. So,
ds2
= dx2 – c2(dt)2
We can identify 1, –c2 to be the metric of this
space. This space is called Minkowski space and is the
gateway to general relativity.
There is a remarkable symmetry in such a
space when it comes to Lorentz transformation. Lorentz
transformation is simply rotation of Minkowski space
because distance s2 = x2
-
c2t2 has to be constant, which
allows simply rotation of coordinates.