Euler force

In classical mechanics, the Euler acceleration (named for Leonhard Euler), also known as azimuthal acceleration[1] or transverse acceleration[2] it is the fictitious tangential force that is felt as a result of any radial acceleration. In other words, 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  = m  a , where a is the Euler acceleration and m is the mass of the body.[3] [4]

Contents

Euler Force Example

For person on 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 the person towards the front of the horse. The euler force is perpendicular to the centrifugal force.

Euler acceleration

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


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

where:

ω is the angular velocity of rotation of the reference frame;
r is the vector position of the point where the acceleration is measured relative to the axis of the rotation.

Euler force

Using the above acceleration, the Euler force is:


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

where:

m is the mass of the object upon which this fictitious force is exerted.

See also

Notes and references

  1. ^ David Morin (2008). Introduction to classical mechanics: with problems and solutions. Cambridge University Press. p. 469. ISBN 0521876222. http://books.google.com/books?id=Ni6CD7K2X4MC&pg=PA469&dq=acceleration+azimuthal+inauthor:Morin&lr=&as_brr=0. 
  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. p. 102. ISBN 1563473429. http://books.google.com/books?id=OjH7aVhiGdcC&pg=PA102&vq=Euler&dq=%22Euler+acceleration%22&lr=&as_brr=0&source=gbs_search_s&sig=ACfU3U0__alj4q5o16OHM8vGvArm0rqMdg. 
  4. ^ Jerrold E. Marsden, Tudor S. Ratiu (1999). Introduction to Mechanics and Symmetry: A Basic Exposition of Classical Mechanical Systems. Springer. p. p. 251. ISBN 038798643X. http://books.google.com/books?id=I2gH9ZIs-3AC&pg=PP1&dq=isbn:038798643X&sig=tDWUiGpvGVpbRCCQcGK0Bx5Yk3g#PPA251,M1.