NOTE: This is a repost of post #2 which got all its special symbols clobbered when I edited a couple minor typos:
Lucy Yeats said:
I've posted on this forum before and carefully read the answers, but I'm still confused... Also, I'm familiar with the twin paradox, and understand that acceleration is the reason the twins' frames aren't symmetrical.
Question 1: Is it okay for an observer to view HIS OWN reference frame as the moving one?
It's important to realize that all observers, objects and clocks are in any reference frame you want to consider but when we talk about an observer's own reference frame, we always mean one in which he is at rest. However, it's totally permissible for an observer to view himself in any reference frame, even one that is moving with respect to himself or, equivalently, one in which he is moving, just don't call it HIS OWN reference frame or you'll just confuse everyone that is familiar with the normal terminology.
Lucy Yeats said:
For example, suppose an observer is on a planet with speed -0.6c to the right, and a rocket is at rest relative to him. The prime frame is the rocket frame.
This is confusing in terms of where the observer is but I think what is important is you have a rocket and a planet that are moving away from each other with the rocket on the right and the planet on the left and the x-axis is aligned along their line of motion and increasing x is to the right and when they were together, you're calling that the origin where x=x'=0 and t=t'=0, correct?
Lucy Yeats said:
Suppose there is a time interval of one hour on the planet. I want to find the time interval in hours on the rocket's clock.
t'=γ(t-βx)=1.25(1-0.36)=0.8 This is correct, isn't it?
This is correct if you are starting with the rest frame of the planet and you are transforming an event into the rest frame of the rocket (you did say it was the prime frame which is the one you are transforming into). But you left out a lot of important details, so I will fill them in for anyone that doesn't see how you did this.
First off, since the rocket is moving to the right, we use a value of β=0.6. From this we calculate γ as:
γ=1/√(1-β
2)=1/√(1-0.6
2)=1/√(1-0.36)=1/√0.64=1/0.8=1.25
Next we assume that the start of the hour is at the origin and the event we want to consider is one hour later when t=1. During this hour, the rocket has moved at 0.6c so it is 0.6 light-hours to the right of the origin meaning it is at x=0.6. Now we can do your calculation:
t'=γ(t-βx)=1.25(1-(0.6*0.6))=1.25(1-0.36)=1.25(0.64)=
0.8
Now what does this mean? It means in the rest frame of the planet, when 1 hour has gone by for the planet (and all of the clocks in its rest frame), 0.8 hours has gone by for the rocket. Note that the rocket is moving in this frame but wherever it is, there is a coordinate clock that is at the same time as the planet's clock that remains at location x=0. So we can meaningfully talk about how much time has transpired on the moving rocket's clock during an interval of time for the stationary planet's clock.
This also illustrates the normal time dilation factor of 1/γ based on the speed of an object in a frame of reference. We use the Greek letter tau, τ, to symbolize the Proper Time on a moving clock and compare it to t, the coordinate time for the reference frame with the equation τ=t/γ. So if we know the coordinate time interval, we can calculate the time on a moving clock, τ, using this formula. Or we can go the other way around. If we know the Proper Time interval on a moving clock, we can calculate the corresponding coordinate time, t, for the reference frame.
Lucy Yeats said:
Question 2: But it's equally valid to see the rocket as moving at 0.6c to the right and the planet as at rest. Once again, suppose there is a time interval of one hour on the planet. I want to find the time interval in hours on the rocket's clock. But this time I get t'=γ(t-βx)=1.25 since Δx=0. How come I get these two different answers?
Thanks in advance for answering, as I'm sure this is a very easy question for most of you- I've just met special relativity so I'm very confused!
This sounds like exactly what we just did for Question 1 but I think what you are asking is how you can start from the rest frame of the rocket and transform into the rest frame of the planet and get the same result as before, correct? (I think you may have gotten confused into thinking that the prime frame was the first frame but we don't mean prime that way, we simply mean it's the frame that has the prime marks on the variable names (t' and x'), the ones that we are going to transform into).
So let me rephrase your Question 2 into what I think you want:
But it's equally valid to see the planet as moving at 0.6c to the left and the rocket as at rest. Once again, suppose there is a time interval of one hour on the planet. I want to find the time interval in hours on the rocket's clock.
Now we have a totally different situation because the planet's clocks are not synchronized with the coordinate time of the reference frame (which is also equal to the time on the rocket's clock). So in order to determine a coordinate time corresponding to one hour on the planet, we can use the relationship between τ and t expressed above and calculate t=γ*τ=1.25*1=1.25. Now we can quit right here because this is the same answer you got, although I'm not sure if you actually did a correct calculation because you left out all the details.
So what does this mean? Well, time dilation is frame dependent, just like speed is. In the planet's rest frame, the rocket is moving, so it is the one that is experiencing time dilation, and one hour on the planet's clock is less time (0.8 hours) on the rocket's clock. But in the rocket's rest frame, the planet is moving, so it is the one that is experiencing time dilation, and one hour on the planet's clock is more time (1.25 hours) on the rocket's clock. You could also say that one hour on the rocket's clock is 0.8 hours on the planet's clock. This might show the symmetry a little better.
So your final numbers are correct, but they were interchanged with the situations.