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Normal forces in stationary spacetimes

Richard H. Price
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Abstract

For geodesic motion of a particle in a stationary spacetime the $U_0$ component of particle 4-velocity is constant and is considered to be a conserved mechanical energy. We show that this concept of a conserved mechanical energy can be extended to particles that move under the influence of a ``normal force,'' a force that, in the stationary frame, is orthogonal to the motion of the particle. We illustrate the potential usefulness of the concept with a simple example.

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Richard H. Price. 2004-01-30. Normal forces in stationary spacetimes. https://doi.org/10.1023/b%3Agerg.0000038631.91084.92

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