Velocity in Proper Time: Relativistic Acceleration Equation

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SUMMARY

The discussion focuses on the relativistic acceleration equation for an object under constant acceleration, denoted as g_{M}. It confirms that after a proper time τ, the coordinates are given by x = cosh(τ/τ_{0}) and t = sinh(τ/τ_{0}), leading to the velocity v = tanh(τ/τ_{0}). The participants clarify that this velocity represents the instantaneous coordinate velocity at time τ, and integration is necessary to determine the end velocity after a finite amount of proper time, considering that rapidities add rather than velocities.

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  • Understanding of special relativity concepts, particularly proper time and coordinate time.
  • Familiarity with hyperbolic functions, specifically cosh, sinh, and tanh.
  • Knowledge of calculus, particularly integration techniques.
  • Basic grasp of relativistic kinematics and acceleration.
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  • Study the derivation of the relativistic acceleration equation in detail.
  • Learn about the integration of rapidities in special relativity.
  • Explore the implications of constant acceleration in relativistic contexts.
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nomadreid
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Two questions, based on the same situation: in
http://physics.stackexchange.com/questions/34204/relativistic-acceleration-equation
(question A) it is mentioned that, for an object with a constant acceleration g_{M}, and with \tau_{0} =1/g_{M} , after proper time \tau, the coordinates are
x= cosh(\tau/\tau_{0})
t = sinh(\tau/\tau_{0})
and that therefore
v = tanh(\tau/\tau_{0})
My first reaction was that this should be coth (position/time, cosh/sinh), but then I figured that tanh comes from v=dx/dt =d(cosh ...)/d(sinh ...) = sinh.../cosh... Is this correct?
(question B) However, this is the end velocity after d\tau. So, I presume one would need to call this v= dv. If we want the end velocity after a finite amount of time, I presume integration would be in order, but since it is the rapidities that add rather than the velocities, I am not sure how this integration would look. Or perhaps there is a simpler method to find the coordinate velocity after finite proper time \tau with constant acceleration g_{M}? (Starting at (0,0).)
I would be grateful for anyone who can untangle me from this mess.
 
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nomadreid said:
My first reaction was that this should be coth (position/time, cosh/sinh), but then I figured that tanh comes from v=dx/dt =d(cosh ...)/d(sinh ...) = sinh.../cosh... Is this correct?
Yes

nomadreid said:
(question B) However, this is the end velocity after d\tau. So, I presume one would need to call this v= dv. If we want the end velocity after a finite amount of time, I presume integration would be in order, but since it is the rapidities that add rather than the velocities, I am not sure how this integration would look.
No, v = dx/dt, as you've calculated it, is the desired instantaneous coordinate velocity at time τ.
 
Thanks, Bill_K
 

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