goodabouthood said:
ghwellsjr,
I was under the impression that each reference frame has its own time. You are making it confusing for me.
Let me give you an example.
I am the stationary observer and I see the spaceship moving at .8c.
Now one year passes for me so that would be the clock in my reference frame correct?
Isn't it correct to say that .6 of a year elapses for the moving ship or in other words for that FOR relative to mine?
How is it possible to say that a frame of reference can have multiple clocks? That does not make sense. I say in my FOR one year has passed and in the moving ships FOR relative to me .6 of a year has passed.
It would be strange to say that the moving ship is part of my FOR and that his clock has moved .6 and mine has moved one year. I need to say in my stationary FOR one year has passed and the moving FOR has elapsed .6 of a year relative to me.
Sorry to be confusing you, I will try to make it clear.
First, I recommend you study
How did Einstein Define Time, especially towards the end where I explain the difference between Proper Time and Coordinate Time.
But I'll give you a synopsis here. A Frame of Reference in Special Relativity is defined as a coordinate system with the normal kind of x, y, and z components to specify a 3-dimensional distance for any point from a predefined origin and with synchronized clocks at every location which keep what is called Coordinate Time. These are normal clocks but they are not allowed to accelerate, that is, they must remain at the locations where they were synchronized to the clock at the origin. When they are synchronized, they all read zero. So we now add a fourth component to the coordinate system which is the time. The four components making up the location and time are called an "event", which doesn't have to imply that any thing actually happened there at that time, just like we can talk about the location of a point in a normal coordinate system, even if there isn't anything there. (Actually, we just imagine that these clocks exist at every location just as we imagine that there are grids of measuring rulers laid out in all directions from the origin.)
Now if we want to describe a scenario in this Frame of Reference, we specify the events for each real clock that we want to consider. Since these clocks are allowed to change locations and therefore experience acceleration and therefore experience speed and therefore experience time dilation with respect to the Coordinate Times on the clocks that are fixed to the Coordinate Locations, we have a different term to refer to the times on these real clocks which is called Proper Time. We can determine how fast any clock is ticking by knowing its speed in the Frame of Reference and applying the reciprocal of the Lorentz Factor to it. Adding up all the ticks allows us to keep track of the time after any period of Coordinate Time we want to consider.
So let's see how this works for the scenario you described in your first post. You started with two synchronized clocks on Earth. Let's assume that they are located at the origin so that the x, y, z and the time components are all zero and that the Proper Time on these two clocks is also zero. I like to use the nomenclature of [t,x,y,z] to specify events and since y and z are always zero in a simple scenario, I like to omit them and use [t,x] to specify each event. Remember that the "t" in this event is the Coordinate Time on the clock that is located at x=0, even though we have two more real clocks at this location at the start of the scenario, the two clocks you specified.
So let's refer to the "stationary" clock as clock S and the "traveling" clock as clock T. At the start of your scenario, both clocks are specified by the event
[0,0] and they both read 0. Then T accelerates to a speed of 0.8c (instantly, to keep things simple) for one year. Where will it be after one year? That's easy, it will be at location x=0.8 (we are using units of time in years and distance in light years.) The corresponding event is
[1,0.8] for T and for S it is
[1,0]. Now the first question is what time will be displayed on these two clocks? Well T has been at a speed of 0.8c so its time will be dilated by a factor of 0.6 (you already know how to do this calculation so I won't repeat it). So keep in mind that there are two times related to clock T at the point of turn-around, one is the Coordinate Time of the event of the turn-around which is 1 year and the other is the Proper Time displayed on the clock which is 0.6 years. Meanwhile, the Proper Time on clock S is 1 year and the Coordinate Time for the corresponding event is also 1 year.
Now clock T returns and it takes another year of Coordinate time for it to get back. The event describing its reuniting with clock S is
[2,0]. This event applies to both clocks but the Proper Time on clock T has advanced by another 0.6 years so it now reads 1.2 year while clock S has advanced by 1 year so that its Proper Time reads 2 years, again the same as the Coordinate Time, since it never moved.
Now I know that you know all the details with regard to the Proper Times because you described them in your first post but you may not have been aware of the concept of Coordinate Time or how they applied to events.
Then you asked about how to view things from the Frame of Reference of clock T. As I pointed out in post #8, clock T is not stationary in any Frame of Reference so you cannot use the Lorentz Transform to answer your question. It's actually stationary in three frames, the one it shares with clock S at the beginning and ending of the scenario, the one it is stationary in during the outbound portion of the trip and the one it is stationary in during the inbound portion of the trip.
So let's start by transforming three of the four events we have already specified from the first FoR into the FoR in which clock T is stationary during the first half of its trip. I'm not going to bother to transform the event for clock S corresponding to the time of the turn around for clock T because it has no bearing on anything.
Here at the three events in FoR 1:
[0,0] start of scenario for both clocks
[1,0.8] turn around event for clock T
[2,0] end of scenario for both clocks
The first event [0,0] will remain the same no matter what other FoR we transform to so I won't go through its calculation.
For the other events, the first thing we need to do to use the Lorentz Transform is calculate gamma, γ, where the speed as a fraction of c, is β = 0.8 according to:
γ = 1/√(1-β
2)
γ = 1/√(1-0.8
2)
γ = 1/√(1-0.64)
γ = 1/√(0.36)
γ = 1/0.6
γ = 1.667
The formulas for the Lorentz Transform are:
t' = γ(t-βx)
x' = γ(x-βt)
For the outbound portion of the trip, β=0.8, and the event of the traveling clock at the end is [1,0.8]:
t = 1
x = 0.8
t' = γ(t-βx)
t' = 1.667(1-(0.8*0.8))
t' = 1.667(1-0.64)
t' = 1.667(0.36)
t' = 0.6
x' = γ(x-βt)
x' = 1.667(0.8-(0.8*1)
x' = 1.667(0.8-0.8)
x' = 1.667(0)
x' = 0
So the turn-around event for clock T is:
[0.6,0]
We can calculate its speed by taking the difference in its starting and ending locations divided by the difference in its starting and ending times. But the starting and ending locations are both 0 so it is stationary in this FoR. So all we have to do to see how much time has advanced on clock T during the first leg of the trip is take the difference in the Coordinate Times for these two events which is 0.6-0 or 0.6 years.
Now let's jump to the last event [2,0].
t = 2
x = 0
t' = γ(t-βx)
t' = 1.667(2-(0.8*0))
t' = 1.667(2-0)
t' = 1.667(2)
t' = 3.333
x' = γ(x-βt)
x' = 1.667(0-(0.8*2)
x' = 1.667(0-1.6)
x' = 1.667(-1.6)
x' = -2.667
So the ending event for both clocks is:
[3.333,-2.667]
Now in order to calculate the speed of clock T during the inbound portion of the trip we have to do the difference thing I mentioned earlier. The coordinate location difference for clock T between the start and end of his inbound trip is -2.667-0 = -2.667 light years. The corresponding coordinate time difference for clock T is 3.333-0.6 = 2.733 years. Dividing these we get a speed for clock T of 0.9756c. Now we apply the reciprocal of the Lorentz Factor on this speed to see what time dilation clock T experiences:
1/γ = √(1-β
2)
1/γ = √(1-0.9756
2)
1/γ = √(1-0.9518)
1/γ = √(0.0482)
1/γ = 0.2159
Now we multiply this factor by the Coordinate Time difference of 2.733 years to get 0.6 years as the Proper Time difference for the clock T during the inbound portion of the trip (just like we got in the first FoR). Finally, we need to add the Proper Time at the end of the outbound portion of the trip to the additional time accumulated during the inbound portion of the trip to get the final Proper Time on clock T as
1.2 years.
Now let's see how much clock S has advanced in this FoR. We need to do the difference thing again but for this clock and we will do it from the beginning of the scenario to the end. The location difference is -2.667-0 or -2.667 light years. The time difference is 3.333-0 or 3.333 years. The speed is 2.667/3.333 or 0.8c so the reciprocal of the Lorentz Factor is 0.6. So the Proper Time on clock S has advanced by 0.6 times 3.333 or
2 years.
So as you can see, even in the FoR for the outbound portion of the traveling's clock trip, we still calculate the Proper Times for both clocks to be the same as they were in the original FoR. In fact, it won't matter what FoR we use, we will always get the same answers. If you want to do the transform for the inbound portion of the trip, you will see that it is similar to the outbound and ends up with the same Proper Times.