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It has been suggested that Centrifugal force (rotating reference frame) be merged into this article. (Discuss) Proposed since September 2010.

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Centrifugal force (from Latin centrum "center" and fugere "to flee") represents the effects of inertia that arise in connection with rotation and which are experienced as an outward force away from the center of rotation. In Newtonian mechanics, the term centrifugal force is used to refer to one of two distinct concepts: an inertial force (also called a "fictitious" force) observed in a non-inertial reference frame, and a reaction force corresponding to a centripetal force. The term is also sometimes used in Lagrangian mechanics to describe certain terms in the generalized force that depend on the choice of generalized coordinates.

Fictitious centrifugal force

There's no such thing as a centrifugal force,get it right next time before you think you're all smart and post things on wikipedia

Centrifugal force is often confused with centripetal force. Centrifugal force is most commonly introduced as a force associated with describing motion in a non-inertial reference frame, and referred to as a fictitious or inertial force (a description that must be understood as a technical usage of these words that means only that the force is not present in a stationary or inertial frame). There are three contexts in which the concept of the fictitious force arises when describing motion using classical mechanics. In the first context, the motion is described relative to a rotating reference frame about a fixed axis at the origin of the coordinate system. For observations made in the rotating frame, all objects appear to be under the influence of a radially outward force that is proportional to the distance from the axis of rotation and to the square of the rate of rotation (angular velocity) of the frame. The second context is similar, and describes the motion using an accelerated local reference frame attached to a moving body, for example, the frame of passengers in a car as it rounds a corner. In this case, rotation is again involved, this time about the center of curvature of the path of the moving body. In both these contexts, the centrifugal force is zero when the rate of rotation of the reference frame is zero, independent of the motions of objects in the frame. The third context is the most general, and subsumes the first two, as well as stationary curved coordinates (e.g., polar coordinates), and more generally any system of abstract coordinates as in the Lagrangian formulation of mechanics.

If objects are seen as moving from a rotating frame, this movement results in another fictitious force, the Coriolis force; and if the rate of rotation of the frame is changing, a third fictitious force, the Euler force is experienced. Together, these three fictitious forces allow for the creation of correct equations of motion in a rotating reference frame.

Fictitious vs. reactive force

The table below compares various facets of the "fictitious force" and "reactive force" concepts of centrifugal force

Lagrangian formulation of centrifugal force

Lagrangian mechanics formulates mechanics in terms of generalized coordinates ${\displaystyle \{q_{k}\}}$, which can be as simple as the usual polar coordinates ${\displaystyle (r,\ \theta )}$ or a much more extensive list of variables. Within this formulation the motion is described in terms of generalized forces, using in place of Newton's laws the Euler–Lagrange equations. Among the generalized forces, those involving the square of the time derivatives ${\displaystyle \{(\mathrm {d} q_{k}/\mathrm {d} t)^{2}\}}$ are sometimes called centrifugal forces.

The Lagrangian approach to polar coordinates that treats ${\displaystyle (r,\ \theta )}$ as generalized coordinates, ${\displaystyle ({\dot {r}},\ {\dot {\theta }})}$ as generalized velocities and ${\displaystyle ({\ddot {r}},\ {\ddot {\theta }})}$ as generalized accelerations, is outlined in another article, and found in many sources. For the particular case of single-body motion found using the generalized coordinates ${\displaystyle ({\dot {r}},\ {\dot {\theta }})}$ in a central force, the Euler–Lagrange equations are the same equations found using Newton's second law in a co-rotating frame. For example, the radial equation is:

${\displaystyle \mu {\ddot {r}}=\mu r{\dot {\theta }}^{2}-{\frac {\mathrm {d} U}{\mathrm {d} r}}}$

where ${\displaystyle U(r)}$ is the central force potential. The left side is a "generalized force" and the first term on the right is the "generalized centrifugal force". However, the left side is not comparable to a Newtonian force, as it does not contain the complete radial acceleration, and likewise, therefore, the terms on the right-hand side are "generalized forces" and cannot be interpreted as Newtonian forces.

The Lagrangian centrifugal force is derived without explicit use of a rotating frame of reference, but in the case of motion in a central potential the result is the same as the fictitious centrifugal force derived in a co-rotating frame. The Lagrangian use of "centrifugal force" in other, more general cases, however, has only a limited connection to the Newtonian definition.

Centrifugal force and absolute rotation

The consideration of centrifugal force and absolute rotation is a topic of debate about relativity, cosmology, and the nature of physical laws.

Note: in the following, 'centrifugal force' is used in the 'fictitious force' sense and not the 'reactive force' sense.

Can absolute rotation be detected? In other words, can one decide whether an observed object is rotating or if it is you, the observer that is rotating? Newton suggested two experiments to resolve this problem. One is the effect of centrifugal force upon the shape of the surface of water rotating in a bucket. The second is the effect of centrifugal force upon the tension in a string joining two spheres rotating about their center of mass. A related third suggestion was that rotation of a sphere (such as a planet) could be detected from its shape (or "figure"), which is formed as a balance between containment by gravitational attraction and dispersal by centrifugal force.

History of conceptions of centrifugal and centripetal forces

The conception of centrifugal force has evolved since the time of Huygens, Newton, Leibniz, and Hooke who expressed early conceptions of it. The modern conception as a fictitious force or pseudo force due to a rotating reference frame as described above evolved in the eighteenth and nineteenth centuries.

See also

The concept of centrifugal force in its more technical aspects introduces several additional topics:

• Reference frames, which compare observations by observers in different states of motion. Among the many possible reference frames the inertial frame of reference are singled out as the frames where physical laws take their simplest form. In this context, physical forces are divided into two groups: real forces that originate in real sources, like electrical force originates in charges, and
• Fictitious forces that do not so originate, but originate instead in the motion of the observer. Naturally, forces that originate in the motion of the observer vary with the motion of the observer, and in particular vanish for some observers, namely those in inertial frames of reference.

The analogy between centrifugal force (sometimes used to create artificial gravity) and gravitational forces led to the equivalence principle of general relativity.

References

Notes

1. Takwale & Puranik 1980, p. 248.
2. Jacobson 1980, p. 80.
3. ^ See p. 5 in Donato Bini, Paolo Carini, Robert T Jantzen (1997). "The intrinsic derivative and centrifugal forces in general relativity: I. Theoretical foundations" (PDF). International Journal of Modern Physics D. 6 (1).{{cite journal}}: CS1 maint: multiple names: authors list (link). The companion paper is Donato Bini, Paolo Carini, Robert T Jantzen (1997). "The intrinsic derivative and centrifugal forces in general relativity: II. Applications to circular orbits in some stationary axisymmetric spacetimes" (PDF). International Journal of Modern Physics D. 6 (1).{{cite journal}}: CS1 maint: multiple names: authors list (link)
4. ^ Fetter & Walecka 2003, pp. 38-39.
5. "Classical Dynamics of Particles and Systems", Marion and Thornton, Brooks Cole; 5 edition 2003.
6. "Methods of Applied Mathematics" By Francis B. Hildebrand, 1992, Dover, p 156.
7. "Statistical Mechanics" By Donald Allan McQuarrie, 2000, University Science Books.
8. "Essential Mathematical Methods for Physicists" By Hans-Jurgen Weber, George Brown Arfken, Academic Press, 2004, p 843.
9. For an introduction, see for example Cornelius Lanczos (1986). The variational principles of mechanics (Reprint of 1970 University of Toronto ed.). Dover. p. 1. ISBN 0486650677.
10. For a description of generalized coordinates, see Ahmed A. Shabana (2003). "Generalized coordinates and kinematic constraints". Dynamics of Multibody Systems (2 ed.). Cambridge University Press. p. 90 ff. ISBN 0521544114.
11. Christian Ott (2008). Cartesian Impedance Control of Redundant and Flexible-Joint Robots. Springer. p. 23. ISBN 3540692533.
12. Shuzhi S. Ge, Tong Heng Lee, Christopher John Harris (1998). Adaptive Neural Network Control of Robotic Manipulators. World Scientific. pp. 47–48. ISBN 981023452X. In the above Euler–Lagrange equations, there are three types of terms. The first involves the second derivative of the generalized co-ordinates. The second is quadratic in ${\displaystyle {\boldsymbol {\dot {q}}}}$ where the coefficients may depend on ${\displaystyle {\boldsymbol {q}}}$. These are further classified into two types. Terms involving a product of the type ${\displaystyle {{\dot {q}}_{i}}^{2}}$ are called centrifugal forces while those involving a product of the type ${\displaystyle {\dot {q}}_{i}{\dot {q}}_{j}}$ for i ≠ j are called Coriolis forces. The third type is functions of ${\displaystyle {\boldsymbol {q}}}$ only and are called gravitational forces.{{cite book}}: CS1 maint: multiple names: authors list (link)
13. R. K. Mittal, I. J. Nagrath (2003). Robotics and Control. Tata McGraw-Hill. p. 202. ISBN 0070482934.
14. T Yanao & K Takatsuka (2005). "Effects of an intrinsic metric of molecular internal space". In Mikito Toda, Tamiki Komatsuzaki, Stuart A. Rice, Tetsuro Konishi, R. Stephen Berry (ed.). Geometrical Structures Of Phase Space In Multi-dimensional Chaos: Applications to chemical reaction dynamics in complex systems. Wiley. p. 98. ISBN 0471711578. As is evident from the first terms …, which are proportional to the square of ${\displaystyle {\dot {\phi }}}$, a kind of "centrifugal force" arises … We call this force "democratic centrifugal force". Of course, DCF is different from the ordinary centrifugal force, and it arises even in a system of zero angular momentum.{{cite book}}: CS1 maint: multiple names: editors list (link)
15. See, for example, Eq. 8.20 in John R Taylor (2005). Classical Mechanics. Sausalito, Calif.: Univ. Science Books. pp. 299 ff. ISBN 189138922X.
16. Francis Begnaud Hildebrand (1992). Methods of Applied Mathematics (Reprint of 1965 2nd ed.). Courier Dover Publications. p. 156. ISBN 0486670023.
17. V. B. Bhatia (1997). Classical Mechanics: With Introduction to Nonlinear Oscillations and Chaos. Alpha Science Int'l Ltd. p. 82. ISBN 8173191050.
18. Henry M. Stommel and Dennis W. Moore (1989). An Introduction to the Coriolis Force Columbia University Press. Pp. 36–38.
19. See Edmond T Whittaker (1988). A treatise on the analytical dynamics of particles and rigid bodies (Reprint of 1917 2nd ed.). Cambridge University Press. pp. 40–41. ISBN 0521358833. for an explanation of how the fictitious centrifugal force corresponds to a potential term in the Lagrangian.
20. Barbour & Pfister 1995, p. 69.
21. Eriksson 2008, p. 194.

Bibliography

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• Articles to be merged from September 2010
• Fictitious forces
• Force
• Mechanics
• Rotation