johnny_bohnny said:
Hi guys, this is my first post, I'm a newbie regarding physics and relativity so I hope you can help me here.
Welcome to PF. We're glad to help.
johnny_bohnny said:
I've just recently started learning about relativity, and my question will be about the relative simultaneity, or precisely Andromeda paradox.
I'm going to draw some spacetime diagrams for you using the Lorentz Transformation process to get from one to the other. In my diagrams, I will assume that the observer at rest with Andromeda is on the Earth and show him as the thick blue line, Andromeda as the thick red line 2.5 million miles away and the observer moving away from Andromeda at 0.4c in a rocket shown as the thick black line. Dots on each of the thick lines represent 1 million year increments of time. I show your event X as a red star exploding at Andromeda and your event Y as a yellow star exploding 1 million years earlier according to Andromeda time. The thin lines represent signals traveling at the speed of light between an observer and Andromeda. I will be showing both how a spacetime diagram depicts simultaneity and how each observer can measure it using radar techniques. In both cases, the key to understanding is Einstein's second postulate, that it takes the same amount of time for a signal to get from an observer to a target as it takes for the signal to get from the target back to the observer, and his first postulate that each observer uses his own clock to measure time and that each observer will measure the round-trip speed of light to be the same value (called c).
johnny_bohnny said:
So in the original setup, if an observer is at rest with respect to Andromeda, he will consider some event, let's call it X, as his present.
Here's the mutual Earth/Andromeda rest frame showing how the red star exploding at time 0 is simultaneous with the Earth clock being at 0. The yellow star exploded at -1 million years at both Andromeda and at Earth in this Inertial Reference Frame (IRF). You can see the black rocket observer's worldline but we are not yet concerned about his observations or measurements:
To see how the Earth observer uses radar to measure the times, consider the signals that he sent earlier and received later. He has been sending signals continually millions of years earlier but I'm only showing the ones that are significant for our purposes. The one that he sent at his time of -3.5 My (million years) hits the yellow star when it explodes and the return echo arrives at the Earth observer at his time of 1.5 My so he takes the average of those two numbers and gets -1 My as his measurement of the time when the yellow star exploded, the same as his rest frame depicts it. Similarly, he can measure the time of the red star exploding as 0 My according to his clock.
johnny_bohnny said:
If another observer moves away from Andromeda, he will consider an earlier event of Andromeda's history, let's call it Y as his present. That's at least what should be the setup.
Here's the rest frame of the black rocket observer. Except for the signals, this diagram was derived by taking the coordinates from the first diagram and Lorentz Transforming them at a speed of 0.4c. Note that the event of the yellow star exploding is simultaneous with his time of zero and the red star explodes at his time of about 1.05 million years (My):
Now we can see how he also can make these measurements. He also has been sending out radar signals continually but again, I'm only showing the ones that hit the exploding stars. The one that he sent at his time of -2.25 My hit the exploding yellow star and echoed back to him at his time +2.25 My and the average is 0 My. The radar signal that he sent at -1.6 My gets averaged with the one he received at +3.7 My for a measurement of 1.05 My.
Do you see how this works?
The observers can also measure the distance to the events by taking the difference between the received and sent times, in other words, the interval of time between sending and receiving the radar signals and dividing by two and calculating how far light travels in that amount of time.
Let's see how that works for the black rocket observer. For the yellow star, half of 4.5 My is 2.25 My which corresponds to 2.25 Mly distance, exactly as the diagram depicts. For the red star, half of 5.3 My yields 2.65 Mly distance.
johnny_bohnny said:
But if two observers are at rest mutually and of course with respect to Andromeda, and one starts moving away from it, accelerating to get in the position that I've previously mentioned, how will he be able to get from the moment that they both agree about to consider their present (since they are mutually at rest) to a moment when he considers his present to be 'earlier' than the present of the stationary observer. Basically, what happens during acceleration or the change of frames, so that one observer can get from one position of simultaneity defining to another?
For this situation, let's consider the Earth observer to hop on the rocket just as it is passing by Earth at time zero (for everybody, since it is the origin of all the IRF's). Here is a diagram similar to the first one but showing the radar signals starting prior to time zero with the blue Earth observer and ending with the echoes returning to the black rocket observer after time zero:
For the yellow star, the observer sent the radar signal at -3.5 My and received the echo at 2.3 My and calculates a time of -0.6 My at a distance of 2.9 Mly. For the red star, he sent the signal at -2.5 My and got the echo at 3.8 My for a time of 0.65 My at a distance of 3.15 Mly.
But note that these measurements are not depicted on the diagram because it is inertial and the observer is not.
Now I want to show you that he gets the same thing if we look at it from the rest IRF of the rocket:
Again, this diagram does not depict the observer's measurements for the same reason as before (he is not inertial and the diagram is).
Next I want to show you how he can construct a non-inertial rest frame by making radar measurements throughout his entire trip. We have to show this starting earlier and ending later and I'm going to show it in another IRF in which the observer's speed is the same both before and after he transfers from the Earth to the rocket. His speed is 0.208712c, first towards Andromeda and then away:
The observer keeps track of all the sent and received times and does the calculations as before and then constructs this non-inertial diagram:
Note that the times and distances that he calculated for the two stars are now depicted accurately. In fact, if you want, you can copy this diagram and drawn in all the same radar signals that were in the previous diagram to validate the process.
johnny_bohnny said:
Thanks in advance. Johnny
You're welcome. I only hope that you still feel like thanking me.