Special relativity- Uniform circular motion.

In summary, the trajectories of the two clocks are symmetrical, so the time elapsed for one clock in the reference frame of the other can be determined by subtracting the proper time from the velocity of the other clock in that reference frame.
  • #1
Scherejg
5
0

Homework Statement


Imagine two clocks that both perform uniform circular motion of radius a in the x-y plane, but in opposite directions: xμ(u) ={t, a cos(ωt),±a sin(ωt), 0}. Suppose these clocks are synchronized to agree when they are coincident at x = a at t = 0. How much time elapses until the next time the clocks are at x = a, as seen by each clock as well as by the inertial observer whose time is labelled by t?

Homework Equations


xμ(u) ={t, a cos(ωt),±a sin(ωt), 0}
xσ(u)= {t,0,0,0}


The Attempt at a Solution


The trajectories are symmetrical, so I only need to calculate the proper time elapsed for in one of the moving reference frames and it should be the same for the other.
First I converted each trajectory into its proper time. I set t=γτ where τ=tau

xμ(u) ={γτ, a cos(ωγτ),±a sin(ωγτ), 0}

Then I wanted the 4-velocities so I could determine how the opposite observer looks in one of the moving reference frames.

dxμ(u)/dτ =γ{1, -aωsin(ωγτ),±aωcos(ωγτ), 0}. The γ and τ are different depending on the trajectory.
I then subtracted the velocity vectors from each other.

xΩ+-{1, -aωsin(ωγ+τ+)-aωsin(ωγ-τ-),aωcos(ωγ+τ+)-aωcos(ωγ-τ-), 0}

So that equation is what the observer moving in the +sin direction would see in his reference frame for the observer moving in -sin direction. Now I need to determine how much time elapses between t=0 and the next time they meet.

I think this is at points where τ+-? This is where I am confused. Is my reasoning good so far?
 
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  • #2
Sherejg,

Welcome to Physics Forums.

It seems to me that this problem is a lot simpler than the way you are approaching it. From the problem statement, it appears that the motion of the two clocks is being described as reckoned from the inertial (stationary) frame of reference. It is easiest to do all the calculations as reckoned from this frame of reference. All you need to do is determine the proper time interval (of the clocks) between successive instances that each clock passes through the point a,0 (in the inertial frame). The differential of proper time for the traveling clocks is given by

[tex](d\tau)^2= (dt)^2(1-(\frac{dx}{cdt})^2-(\frac{dy}{cdt})^2)=(\frac{dt}{\gamma})^2[/tex]

The two clocks and and observers in the stationary frame of reference all agree on the simultaneity of the events when the two clocks meet up.

Chet
 
  • #3
Okay, so I think I misread the problem. Your equation gives the proper time elapsed for a circular moving clock of uniform speed in reference to an inertial observer. I thought I also needed to use one of the clocks as an observer with a uniform circular motion reference frame, and try to discover the time elapsed in his frame of the other clock. But its really asking for the time in inertial observer frame compared to proper time. Thanks for clearing that up! So much easier now haha.
 

1. What is special relativity?

Special relativity is a theory developed by Albert Einstein in 1905 to explain the relationship between space and time. It states that the laws of physics are the same for all observers in uniform motion and that the speed of light is constant for all observers.

2. How does special relativity apply to uniform circular motion?

In uniform circular motion, an object moves at a constant speed around a circular path. Special relativity states that the laws of physics are the same for all observers in uniform motion, so the same principles apply to objects in uniform circular motion.

3. How does special relativity affect the perception of time in uniform circular motion?

According to special relativity, time is relative and can appear to pass differently for observers in different frames of reference. In uniform circular motion, time may appear to pass slower for an observer in motion compared to an observer at rest.

4. What is the role of the speed of light in special relativity and uniform circular motion?

The speed of light is a fundamental constant in special relativity, and it plays a crucial role in the theory's explanation of space and time. In uniform circular motion, the speed of light remains constant for all observers, regardless of their relative motion.

5. How does special relativity impact the concept of mass in uniform circular motion?

In special relativity, mass is not considered a constant quantity but can change depending on the frame of reference. In uniform circular motion, an object's mass may appear to increase due to its high speed, as predicted by special relativity.

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