Special relativity- Uniform circular motion.

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SUMMARY

The discussion centers on calculating the time elapsed between two synchronized clocks performing uniform circular motion in opposite directions, described by the equations xμ(u) = {t, a cos(ωt), ±a sin(ωt), 0} and xσ(u) = {t, 0, 0, 0}. The proper time interval is determined using the equation (dτ)^2 = (dt)^2(1 - (dx/dt)^2 - (dy/dt)^2) = (dt/γ)^2, where γ is the Lorentz factor. The participants clarify that calculations should be performed from the inertial frame of reference, simplifying the problem significantly. The confusion regarding the need for an additional observer frame is resolved, emphasizing the importance of using the inertial observer's perspective.

PREREQUISITES
  • Understanding of special relativity concepts, particularly time dilation and proper time.
  • Familiarity with Lorentz transformations and the Lorentz factor (γ).
  • Knowledge of circular motion equations and their representation in spacetime.
  • Ability to differentiate between inertial and non-inertial reference frames.
NEXT STEPS
  • Study the derivation and implications of the Lorentz factor (γ) in special relativity.
  • Explore the concept of simultaneity in different reference frames, particularly in circular motion scenarios.
  • Learn about the mathematical treatment of proper time in non-inertial frames.
  • Investigate the effects of acceleration on time dilation and proper time in special relativity.
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Students of physics, particularly those studying special relativity, and anyone interested in the implications of time dilation in circular motion scenarios.

Scherejg
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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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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

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

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
 
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.
 

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