Euler force

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In classical mechanics, the Euler acceleration (named for Leonhard Euler), also known as azimuthal acceleration[1] or transverse acceleration,[2] is the fictitious tangential force that is felt as a result of any radial acceleration. In other words, it is an acceleration that appears when a non-uniformly rotating reference frame is used for analysis of motion and there is variation in the angular velocity of the reference frame's axes. This article is restricted to a frame of reference that rotates about a fixed axis.

The Euler force is a fictitious force on a body that is related to the Euler acceleration by F = ma, where a is the Euler acceleration and m is the mass of the body.[3][4]

Intuitive example

The Euler force will be felt by a person riding a merry-go-round. As the ride starts, the Euler force will be the apparent force pushing the person to the back of the horse, and as the ride comes to a stop, it will be the apparent force pushing the person towards the front of the horse. The Euler force is perpendicular to the centrifugal force and is in the plane of rotation.

Mathematical description

Main article: Rotating reference frame

The direction and magnitude of the Euler acceleration is given by:

{\mathbf {a}}_{{\mathrm {Euler}}}=-{\frac {d{\boldsymbol \omega }}{dt}}\times {\mathbf {r}},

where ω is the angular velocity of rotation of the reference frame and r is the vector position of the point where the acceleration is measured relative to the axis of the rotation. The Euler force on an object of mass m is then

{\mathbf {F}}_{{\mathrm {Euler}}}=m{\mathbf {a}}_{{\mathrm {Euler}}}=-m{\frac {d{\boldsymbol \omega }}{dt}}\times {\mathbf {r}}.

See also

Notes and references

  1. ↑ David Morin (2008). Introduction to classical mechanics: with problems and solutions. Cambridge University Press. p. 469. ISBN 0-521-87622-2. 
  2. ↑ Grant R. Fowles and George L. Cassiday (1999). Analytical Mechanics, 6th ed. Harcourt College Publishers. p. 178. 
  3. ↑ Richard H Battin (1999). An introduction to the mathematics and methods of astrodynamics. Reston, VA: American Institute of Aeronautics and Astronautics. p. 102. ISBN 1-56347-342-9. 
  4. ↑ Jerrold E. Marsden, Tudor S. Ratiu (1999). Introduction to Mechanics and Symmetry: A Basic Exposition of Classical Mechanical Systems. Springer. p. 251. ISBN 0-387-98643-X. 
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