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Figure 5.4 shows the world line of a moving object from the
point of view of two different reference frames, with the primed frame
(left panel) moving to the right at speed
relative to the unprimed
frame (right panel). The goal is to calculate the velocity of the
object relative to the unprimed frame,
, assuming its velocity in
the primed frame,
is known. The classical result is simply
We can use the geometry of figure 5.4 to come up with the
correct relativistic formula. From the right panel of this figure
we infer that
From the left panel of figure 5.4 we similarly see that
| (6.18) |
Finally, we calculate
by noticing that
Substituting equations (5.19), (5.20), and
(5.21) into equation (5.17) and simplifying
yields the relativistic velocity addition formula:
Notice how this equation behaves in various limits. If
, the denominator of equation (5.22) is nearly unity, and the
special relativistic formula reduces to the classical case. On the
other hand, if
, then equation (5.22) reduces to
.
In other words, if the object in question is moving at the speed of
light in one reference frame, it is moving at the speed of light in
all reference frames, i. e., for all possible values of
. Thus,
we have found a velocity addition formula that 1) reduces to the
classical formula for low velocities and 2) gives the observed results
for very high velocities as well.
David Raymond 2006-04-07