Relativity and gravitational theory Definition
Born rigidity
Builds on Minkowski spaceWorld lineFour-velocityRindler coordinates
Definition
Let be Minkowski space with inertial coordinates and metric , and let be an open set. A motion of a body in is a smooth vector field on with . Its integral curves are timelike world lines parametrised by proper time, and is their four-velocity field. Let and let be the projection onto the rest space orthogonal to . The motion is Born rigid if where .
Remarks
The condition says that the distance between infinitesimally close world lines, measured orthogonally to , does not change along the motion. Equivalently, the expansion and the shear of vanish, or the Lie derivative of along vanishes. Example: uniform motion with constant is Born rigid, since . Example: the world lines of fixed in Rindler coordinates form a Born rigid motion. Each is a hyperbolic motion with proper acceleration . The metric does not depend on , so the rest-space distances between these observers are constant. Non-example: a family of world lines that all have the same constant proper acceleration along , starting at rest at different points , is not Born rigid. Their coordinate distance stays constant in the original frame, so the distance measured in their rest frames is times it, which grows with the speed. The Rindler example shows that in a Born rigid accelerated rod the rear end must accelerate harder than the front.
Reading path
To understand this page from the ground up, read these 5 pages in order. The foundations come first.
Show the path as a graph
- no evidence level
- Four-velocity concept
- Minkowski space concept
- Rindler coordinates concept
- World line concept
- Born rigidity definition
Further reading
About this page
| Tag | F46ASFTAVG |
|---|---|
| URI | m2://F46ASFTAVG |
| Kind | definition |
| Writing | W0 stub |
| MSC | 83A05, 74A05 |
| Defines | Born rigidity |
| Uses | Minkowski space, World line, Four-velocity, Rindler coordinates |
| Changed | 3 November 2026 |
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