Math 2.0

Relativity and gravitational theory Special relativity: kinematics Problem

Ehrenfest paradox

Builds on Minkowski spaceLorentz factorBorn rigidityHerglotz–Noether theorem

Problem

A disc of radius RR is first at rest in an inertial frame. It is then brought into rotation about its axis with constant angular speed ω\omega, where ωR<c\omega R < c. Each element of the rim moves along its own length with speed ωR\omega R. So it should be contracted by the factor 1/γ1/\gamma, where γ=1/1−ω2R2/c2\gamma = 1/\sqrt{1 - \omega^2 R^2/c^2} is the Lorentz factor. Each radius moves perpendicular to its own length, so it should not be contracted. How can a rigid disc, whose radius stays RR while its circumference shrinks, be set into rotation? What is the geometry of the rotating disc?

Remarks

A Born rigid body at rest cannot be brought into rotation; this follows from the Herglotz–Noether theorem. So the disc must deform while it is spun up; a real disc develops stresses. Once it rotates uniformly, it can move in a Born rigid way. Then rulers at rest on the rim measure the circumference 2πRγ2\pi R \gamma, while rulers along a radius measure RR. The ratio of measured circumference to measured diameter is πγ>π\pi \gamma > \pi, so the space of the rotating observers is not Euclidean. Einstein took this observation as a hint that gravity, viewed through acceleration, goes with non-Euclidean geometry. Paul Ehrenfest posed the problem in 1909.

Reading path

To understand this page from the ground up, read these 7 pages in order. The foundations come first.

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  1. Born rigidity concept
  2. Four-velocity concept
  3. Killing vector field concept
  4. Lorentz factor concept
  5. Minkowski space concept
  6. Herglotz–Noether theorem statement
  7. Ehrenfest paradox problem

Further reading

  1. Web https://en.wikipedia.org/wiki/Ehrenfest_paradox
About this page
TagJH3C399MX8
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MSC83A05
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AboutBorn rigidity
UsesMinkowski space, Lorentz factor, Born rigidity, Herglotz–Noether theorem
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Changed3 November 2026

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