SUMMARY
The Lorentz-Fitzgerald contraction hypothesis does not contradict classical motion of rigid bodies, as classical rigid bodies do not exist in the framework of relativity. In special relativity (SR), a rigid body is defined as retaining its shape in its instantaneous rest frame, while the concept of Born rigidity applies specifically to scenarios involving proper acceleration. A Born rigid geodesic congruence can exist in Minkowski spacetime, characterized by zero expansion and shear, but the conditions for achieving Born rigidity are significantly more restrictive than in classical Newtonian physics.
PREREQUISITES
- Understanding of special relativity (SR) principles
- Familiarity with the concept of Born rigidity
- Knowledge of Minkowski spacetime
- Basic grasp of the Herglotz-Noether theorem
NEXT STEPS
- Research the implications of Born rigidity in special relativity
- Study the Herglotz-Noether theorem and its relevance to rigid body motion
- Explore the differences between classical and relativistic definitions of motion
- Examine the concept of geodesic congruences in Minkowski spacetime
USEFUL FOR
Physicists, students of relativity, and anyone interested in the foundational concepts of motion and rigidity in the context of special relativity.