altergnostic said:
The clock moves perpendicular to the direction of the light pulse (the line drawn from one mirror to another in the rest frame).
Ok, good.
altergnostic said:
There's a light pulse going from A to B, which we have been calling the beam and is the pulse that makes the clock tick by moving between the mirrors, and there's another pulse from point B to the origin to communicate the time of the reflection event to the observer, since he can't see the beam in this setup.
Ok, this was the part I hadn't understood. Now it's clear. See below for revised analysis.
altergnostic said:
And since we are looking for numbers for the beam we really need the spatial rotation so that the observer's x-axis is in line with AB.
It doesn't matter whether it's the x or the y axis; I had picked the x-axis for the direction of motion of the light clock as a whole since that's a common convention in SR problems. To humor you I'll re-do my analysis with the light pulses moving in the x-direction and the light clock as a whole moving in the y direction relative to the observer.
We have two frames, the "observer" frame (the frame in which the observer is at rest), which will be the unprimed frame, and the "clock" frame (the frame in which the clock is at rest), which will be the primed frame. The relative velocity between the two frames is v = 0.5; the light clock is moving in the positive y-direction in the observer frame (and therefore the observer is moving in the negative y-direction in the clock frame). The gamma factor associated with this v is 1.16 (approximately). So the transformation equations are:
Unprimed to Primed Frame
t' = 1.16 ( t - 0.5 y )
x' = x
y' = 1.16 ( y - 0.5 t )
Primed to Unrimed Frame
t = 1.16 ( t' + 0.5 y' )
x = x'
y = 1.16 ( y' + 0.5 t' )
We have six events of interest (two pairs of events occur at the same point in spacetime and so have identical coordinates, in either frame):
D0 - The light clock source emits a light pulse towards the mirror.
A0 - The observer is co-located with the light clock source at the instant that the pulse is emitted. Thus, events A0 and D0 happen at identical points in spacetime. This point is taken to be the common origin of both frames (moving the origin elsewhere would just add a bunch of constant offsets in all the formulas, making the math more complicated without changing any of the results).
B1a - The light pulse reflects off the mirror.
B1b - A light signal is emitted by the mirror back towards the observer, carrying the information that the light pulse has struck the mirror. Events B1a and B1b happen at identical points in spacetime.
A2 - The observer receives the light signal emitted from event B1b.
D2 - The light clock detector (which is co-located with the source) receives the light pulse that was reflected off the mirror.
We know that the spatial distance between the light clock source/detector and the mirror, in the clock frame, is 1. This, combined with the information that events A0/D0 are at the origin, fixes the following coordinates (primes on the event labels denote coordinates in the primed frame):
A0 = A0' = D0 = D0' = (0, 0, 0)
B1a' = B1b' = (1, 1, 0)
D2' = (2, 0, 0)
Simple application of the transformation equations above gives the unprimed coordinates of B1a/B1b and D2:
B1a = B1b = (1.16, 1, 0.58)
D2 = (2.32, 0, 1.16)
All of this is the same as I posted previously, just with the x and y coordinates switched, since you prefer to have the x-axis oriented in the direction the light pulse travels.
It only remains to calculate the coordinates of event A2. It is easiest to do this in the unprimed frame, since the observer is at rest at the spatial origin in this frame. Therefore, a light pulse emitted towards the observer from event B1b has to travel from spatial point (1, 0.58) to spatial point (0, 0). A light pulse's worldline must have a zero spacetime interval, so the elapsed time in the unprimed frame must satisfy the equation:
\Delta t^2 - \Delta x^2 - \Delta y^2 = 0
or
\Delta t = \sqrt{ \Delta x^2 + \Delta y^2 } = \sqrt{ 1 + (0.58)^2 } = 1.16
Which of course is just the gamma factor. We could have seen this directly by realizing that the time elapsed in the unprimed frame from event A0 to event B1a must be the same as the time elapsed in the unprimed frame from event B1b to event A2; but I wanted to calculate it explicitly to show how everything fits together. [Edit: In other words, I wanted to show that we don't have to *assume* that the light signal travels at c, which is what "zero spacetime interval" means. We can *prove* that it must, by comparing the result we get from the direct method I just gave, with the result we get from the interval calculation I just gave, and seeing that they are the same.]
So we have the unprimed coordinates for event A2:
A2 = (2.32, 0, 0)
Again, a simple calculation using the above transformation formula gives:
A2' = (2.68, 0, -1.34)
What is this telling us? Well, the observer is moving in the negative y-direction in the primed (clock) frame, so the y-coordinate of event A2 is negative in this frame. The time in this frame is *larger* than that in the unprimed frame because it takes extra time for the light signal to catch up to the observer since the observer is moving away from it. We also expect this from the relativity of simultaneity: events A2 and D2 are simultaneous in the unprimed frame (the reason why should be obvious from the discussion I gave above), so they won't be simultaneous in the primed frame; the event that is in the opposite direction from the relative motion (A2 in this case) will occur later in the primed frame.
Once again, this is all straightforward analysis and I don't see a paradox anywhere; it just requires being careful about defining events and frames. I'll put any responses I have to other comments you've made (now that I know we are both talking about the same scenario) in a separate post.
Edit: I suppose I should add that it's easy to confirm that *all* of the light pulses travel at c, in both frames, from the coordinates that I gave above.