Ehrenfest's Paradox: Resolving the Kinematical Solution

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In summary, the Ehrenfest's paradox arises when considering a rotating disk and the different Lorentz contractions experienced by different parts of the disk. The supposed kinematical solution to this paradox is to consider the disk being accelerated up to a given angular velocity, which would induce stresses and deform the disk. The resolution to the paradox lies in the assumption of Born Rigidity, where it is assumed that the disk does not stretch or deform under acceleration. This assumption allows for the determination of the spatial geometry of the disk at a given angular velocity.
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Coincidentally, this has just cropped up in another thread:
DrGreg said:
When expressed in cylindrical polar coordinates, these are known as Born coordinates
[tex]ds^2 = -\left( c^2 - \omega^2 \, r^2 \right) \, dt^2 + 2 \, \omega \, r^2 \, dt \, d\phi + dz^2 + dr^2 + r^2 \, d\phi^2[/tex]
so I might as well point out that if you "complete the square" on this formula you get[tex]
ds^2 = -\left( c^2 - \omega^2 \, r^2 \right) \left( dt - \frac{\omega r^2}{c^2 - \omega^2 r^2} d\phi \right)^2 + dz^2 + dr^2 + \frac{r^2}{c^2 - \omega^2 r^2} \, d\phi^2
[/tex]The expression[tex]
dz^2 + dr^2 + \frac{r^2}{c^2 - \omega^2 r^2} \, d\phi^2
[/tex]represents the non-flat metric of the quotient space. The same technique applies to any stationary spacetime.

Ref: Rindler (2006), Relativity: Special, General and Cosmological, 2nd ed. p. 198
 
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