Here is the outline of a proof using
k-calculus and radar coordinates.
An inertial observer O is equipped with radar and
emits a pulse at time
e, and
receives a radar echo at time
r from a remote object P. For motion in a single dimension, the two values (
e,
r) (which are both measured by O's clock) uniquely determine any event and are called radar coordinates.
Similarly an observer O' can define radar coordinates (
e',
r') using the clock of O'.
See the attached spacetime diagram, in which it is assumed that O, O' and P lie in a straight line at all times.
Notice that a radar pulse emitted by O at time
e (by O's clock) travels at exactly the same speed as a pulse emitted by O' at time
e' (by the clock of O') (by Einstein's 2nd postulate), so both pulses arrive at P simultaneously and are echoed back. O' receives both pulses at time at time
r' (by the clock of O'), and O receives both pulses at time at time
r (by the clock of O).
In fact O emits a sequence of pulses at time-intervals of d
e. O' measures these intervals as d
e' =
k d
e, where
k is the Doppler factor between O and O'. We don't yet know the value of
k, just that it is constant (provided O and O' are both inertial).
Next note that the Doppler factor for O relative to O' must, by Einstein's 1st postulate, be equal to the Doppler factor for O' relative to O. It follows that the pulses traveling past O' at intervals of d
r' must be detected by O at intervals of d
r =
k d
r'.
k is the same value as above.
To summarise, we have:
d
e' =
k d
e ...(1)
d
r =
k d
r' ...(2)
Eliminating
k between these two equations gives
d
e d
r = d
e' d
r'
In other words, d
e d
r is invariant and we denote it by d
s2.
d
s2 = d
e d
r = d
e' d
r' ...(3)
It is not hard to show that O's radar coordinates (
e,
r) are related to O's standard time and distance coordinates (
t,
x) by
x =
c(
r -
e)/2
t = (
r +
e)/2
(Technical note to those who are interested. It is only when we use
t that we rely on Einstein's synchronisation convention. Results involving only
r and
e are independent of any synchronisation convention.)
Therefore
e =
t -
x/
c ...(4)
r =
t +
x/
c ...(5)
(with similar equations for the primed coordinates of O').
Substitute (4) and (5) into (3) to get the standard equation for the Lorentz interval.
Finally, substitute (4) and (5) into (1) and (2) to obtain
d
t' = (
k+
k-1)d
t/2 - (
k-
k-1)d
x/(2
c)
d
x' = (
k+
k-1)d
x/2 - (
k-
k-1)
cd
t/2
These equations are the standard Lorentz transform with
gamma = (
k+
k-1)/2 and
v = (
k-
k-1)/(
k+
k-1).
By considering the special case where
x' = 0, you can verify that
v is just the velocity of O' relative to O and that
gamma is related to
v by the usual formula.
The above proof does skate over a few of the details but I hope you can work out any missing parts yourself.
References
k-calculus:
* Bondi, Hermann (1980),
Relativity and Common Sense, Dover Publications, New York, ISBN 0-486-24021-5
*
http://www.geocities.com/autotheist/Bondi/intro.htm
Radar coordinates:
* Geroch, Robert (1978),
General Relativity from A to B, University of Chicago Press, Chicago, ISBN 0-226-28864-1