DaleSpam said:
This conversation has become boring so I will work the problem.
Worldline of clock 1
x'=0
1.25 (0.6 c t + x) = 0
x=-0.6 c t
Worldline of clock 2
x'=6
1.25 (0.6 c t + x) = 6
x = 4.8 - 0.6 c t
So we immediately see that the distance between the clocks is 4.8 lightseconds.
Worldline of Harriet
x' = 0.6 c t
1.25 (0.6 c t+x)=0.75 c \left(\frac{0.6 x}{c}+t\right)
x = 0
Finding the intersection of Harriet's worldline with clock 1 we find:
0 = -0.6 c t
t = 0
Finding the intersection of Harriet's worldline with clock 2 we find:
0 = 4.8 - 0.6 c t
t = 8/c
So we see that the time was 8 seconds.
Claimant B is correct. QED.
Your analysis is so simple. I used the Lorentz Transform to analyze the same scenario but as you can see it is very much more complicated although I do get the same answer. Could you provide insight into how you do it so much more easily?
Here's how I explain the process in detail:
A Frame of Reference is a set of x, y, z coordinates along with time that we use in Special Relativity to define and analyze a scenario. Each set of [t, x, y, z] coordinates is called an "Event". All observers and objects (clocks & rulers) exist in any particular FoR that we are considering.
When someone refers to Harry's FoR, they are not excluding Harriet, they are merely saying that Harry is a rest in that particular FoR and Harriet is moving. In order to talk meaningfully about Harry's FoR, we need to specify each significant event for Harry and each significant event for Harriet, all within the same FoR.
When people then talk about Harriet's FoR, they are talking about a totally different FoR in which Harriet is stationary and Harry is moving. The coordinates in these two frames are different and you use the Lorentz Transform to convert all the events from one FoR to all the same events in the other FoR.
For simplicity's sake, for scenarios like the yours, since we can assign everything to the x coordinate, we can ignore y and z components (because we can set them everywhere to zero).
So let's go back to the first post in this thread and compile the events defined there according to Henry's FoR (remember, these coordinates are for t in seconds and x in light-seconds as [t,x]):
[0,0] Location of clock1 at start of scenario
[0,6] Location of Henry and clock2 at start of scenario
[10,0] Location of clock1 at end of scenario
[10,6] Location of Henry and clock2 at end of scenario
[0,0] Location of Harriet and her clock at start of scenario
[10,6] Location of Harriet and her clock at end of scenario
Note that the length of time for the scenario to progress in Henry's FoR is the distance between Henry's two clocks divided by the relative speed which is 6/0.6 or 10 seconds.
So now we use the Lorentz Transform on each of these six events in Henry's FoR to see what they are in Harriet's FoR.
First we want to calculate gamma, γ, which is equal to 1/√(1-ß²) where ß is the speed as a fraction of c. So:
γ = 1/√(1-ß²) = 1/√(1-0.6²) = 1/√(1-0.36) = 1/√(0.64) = 1/0.8 = 1.25
Then we use these two formulas for each t and x coordinate:
t' = γ(t-vx/c²)
x' = γ(x-vt)
But since we are using units in which c=1 we can simplify them to:
t' = γ(t-vx)
x' = γ(x-vt)
Note that t' and x' are the new values based on the old values, γ, t, x, and v.
The velocity, v, is 0.6 because we want Harriet to move from an x value of 0 at the start of the scenario to an x value of 6 at the end of the scenario (according to Harry's FoR).
Now we do the detailed calculations. Some of the events are used twice so we only have to do four sets of calculations.
[0,0]:
t=0 and x=0
t' = γ(t-vx) = 1.25(0-0.6*0) = 0
x' = γ(x-vt) = 1.25(0-0.6*0) = 0
[0,6]:
t=0 and x=6
t' = γ(t-vx) = 1.25(0-0.6*6) = 1.25(-3.6) = -4.5
x' = γ(x-vt) = 1.25(6-0.6*0) = 7.5
[10,0]:
t=10 and x=0
t' = γ(t-vx) = 1.25(10-0.6*0) = 12.5
x' = γ(x-vt) = 1.25(0-0.6*10) = -7.5
[10,6]:
t=10 and x=6
t' = γ(t-vx) = 1.25(10-0.6*6) = 1.25(10-3.6) = 1.25(6.4) = 8
x' = γ(x-vt) = 1.25(6-0.6*10) = 0
To summarize the four sets of calculations as [Henry's FoR] > [Harriet's FoR]:
[0,0] > [0.0]
[0,6] > [-4.5,7.5]
[10,0] > [12.5,-7.5]
[10,6] > [8,0]
And substituting the coordinates from Henry's FoR to Harriet's FoR:
[0,0] Location of clock1 at start of scenario
[-4.5,7.5] Location of Henry and clock2 at start of scenario
[12.5,-7.5] Location of clock1 at end of scenario
[8,0] Location of Henry and clock2 at end of scenario
[0,0] Location of Harriet and her clock at start of scenario
[8,0] Location of Harriet and her clock at end of scenario
From this you can see that the time from start to end of the scenario for Harriet is 8 seconds.
There are many ways that Harriet can measure the distance between Henry's two clocks. Probably the simplest is for her to measure how long it takes between clock1 and clock2 arriving at her location and knowing the speed of the clocks (and Henry) she can calculate the distance as simply the speed multiplied by the time interval. This would be 0.6 times 8 or 4.8 light-seconds.
These values agree with the ones of Claimant B from post #1.
However, you may be wondering why the values for Claimant A aren't correct because we do see a location value of 7.5 light-seconds and a time of 12.5 seconds in Harriet's FoR. Well the reason why those values are not legitimate answers is because they are for events that happened simultaneously in Henry's FoR but they are not simultaneous in Harriet's FoR. For the distance between clock1 and clock2 we have to calculate a pair of events for those two clocks that occurred at the same time in Harriet's FoR. We can pick any time we want but it makes sense to use the first event where the time is zero and the location of clock1 is 0. Then all we have to do is figure out where clock2 is at time zero. We use a normal interpolation technique to do this. Looking at the second and fourth events, we find clock2 starts out at a location of 7.5 at a time of -4.5 and ends up at location 0 at a time of 8 seconds. The total time is 8 - (-4.5) = 12.5 and the total distance is 7.5 light-seconds. We want to know the ratio of 4.5 seconds out of 12.5 seconds, which is 0.36. Now if we multiple this ratio times the 7.5 light-seconds we get 2.7 light-seconds distance from the starting location which is 7.5 so 7.5 minus 2.7 or 4.8 light-seconds is the location of clock2 at time zero and that is the answer we are looking for.