User:Jamontaldi/Relative equilibrium

A relative equilibrium is a type of motion studied in Mathematics and Physics, and to a lesser extent molecular chemistry. In an equilibrium there is no motion at all, while in a relative equilibrium there is motion but, roughly speaking, the shape of the system does not change. Relative equilibria are sometimes called stationary motions, describing for example the uniform rotational motion of a star in astrophysics or the pure rotation of a molecule.

The term relative equilibrium was introduced by Henri Poincaré (1885) in his study of the motion of a fluid mass, and given a general mathematical context by Stephen Smale (1970). The idea was already apparent in earlier work by Bernhard Riemann (1861), Edward Routh (1877), Jacobi (183?) and others.

Definition

edit

Suppose a mechanical system (or more general dynamical system) has a group of symmetries G, with Lie algebra  . Then a relative equilibrium is a motion which coincides with the action of a 1-parameter subgroup of G. In more detail, let   be a solution to the dynamical system on a manifold M. Then this is a is a relative equilibrium if there is a   for which  . Here   is the vector field on M generated by  .

There are a number of useful equivalent conditions for a relative equilibrium[1]. On is that a trajectory (solution) of the dynamical system is a relative equilibrium if it is contained entirely within a group orbit.

Examples

edit

References

edit
  1. ^ see Marsden (1992), Ch 4

Bibliography

edit
  • Abraham, Ralph; Marsden, Jerrold E. (1978). Foundations of Mechanics (2 ed.). Addison-Wesley.
  • Riemann, Bernhard (1861). "Ein Beitrag zu den Untersuchungen über die Bewegung eines flussigen gleichartigen Ellipsoides". Abhandlungen der Königlichen Gesellschaft der Wissenschaften zu Göttingen. 9: 3–36.
  • Smale, Stephen (1970). "Topology and Mechanics II". Inventiones Math. 11: 45–64. doi:10.1007/BF01389805.
edit