This article is from the Relativity and FTL Travel FAQ, by Jason W. Hinson jason@physicsguy.com with numerous contributions by others.
So, how do we show time dilation on our space-time diagram. Well, the
key to this can be found by expressing time dilation in the following way:
In the O observer's frame of reference, let the tick t1 of his clock be
simultaneous with the tick t1' of the O' observer's clock. Also, let the
tick t2 of his (the O observer's) clock be simultaneous with the t2 tick of
the O' observer's clock. Then, we would find that
(Eq 3:1)
t2'- t1'= (t2 - t1)/gamma
where gamma (as defined in Section 1.4) would be calculated using the
relative velocity of O and O'. What Equation 3:1 says is that in the O
observer's frame of reference, the difference in the ticks of the O'
observer's clock is smaller than the difference in the O observer's own
ticks by a factor of gamma. Thus, we see that in the frame of O, the O'
observer's clock is running slowly.
As an example, from here on we will consider the case where the
relative velocity is 0.6 c such that gamma = 1.25. Using an example like
this will make the procedure easier to understand for the reader; however,
remember that we could redo this whole process with any speed (calculating a
new gamma factor, drawing a different speed for the observers, drawing
appropriate lines of simultaneity, etc.).
Now, what if we let the t1 tick be the "zero" tick. That means that at
the origin, when both of our observers are right next to one another, t1 =
t1' = 0. So, both of the observers agree (because there is no separation
between them in space at the origin) that t1 and t1' are simultaneous, and
happen at t = t'= 0. However, after some time, there will be a tick (t2) on
the O observer's clock. In the frame of reference of O, that tick is
simultaneous with the tick t2' of the O' observer's clock. Since t1 = t1' =
0, and we are using gamma = 1.25, we know (from Equation 3:1) that
(Eq 3:2)
t2'- 0 = (t2 - 0)/1.25.
so
t2' = 0.8*t2
So, this says that in the frame of the O observer, the tick t2 of his
clock is simultaneous with the tick 0.8 t2 on the O' observer's clock. If we
draw a line of simultaneity in the O observer's frame of reference such that
it goes through the tick t2 of his clock, then it must also go through the
tick 0.8 t2 of the O' observer's clock. If we let t2 = 1 second, then we get
what is shown in Diagram 3-1. The distance from the origin, o, to the first
mark along t in that diagram is defined to be 1 second for our O observer.
Meanwhile, the distance from o to the "*" symbol along t' in that diagram is
0.8 second FOR THE O' OBSERVER. So, we begin to see that we can relate
distances in time along the axes of the different observers.
Diagram 3-1
t t' ^ / | / | / | / | / | / t = 1 + - - * - - - - - - - line of simultaneity | / t' = 0.8 for O at t = 1 | / | / | / |/ ---------o----------------------> x | | (Note: The line for t' only approximately represents an observer moving at 0.6 c. It probably more closely represents 0.5 c, but that's my ASCII for you. For our example, it _should_ represent an observer traveling at 0.6 c in the O observer's frame of reference.)
t t' line of simultaneity ^ / ' for O' at t' = 1.25 | / ' | / ' | / ' | % t' = 1.25 | ' / t = 1 + - - * - - - - - - line of simultaneity | / t' = 0.8 for O at t = 1 | / | / | / |/ ---------o----------------------> x | | (Note: The line of simultaneity for O' is a rough approximation)
 
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