In classical mechanics, the precession of a rigid body such as a top under the influence of gravity is not, in general, an integrable problem. There are however three (or four) famous cases that are integrable, the Euler, the Lagrange, and the Kovalevskaya top. In addition to the energy, each of these tops involves three additional constants of motion that give rise to the integrability.
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The Euler top describes a free top without any particular symmetry, moving in the absence of any external torque in which the fixed point is the center of gravity. The Lagrange top is a symmetric top, in which two moments of inertia are the same and the center of gravity lies on the symmetry axis. The Kovalevskaya top is special symmetric top with a unique ratio of the moments of inertia satisfy the relation
and in which two moments of inertia are equal, the third is half as large, and the center of gravity is located in the plane perpendicular to the symmetry axis (parallel to the plane of the two equal points). The nonholonomic Goryachev–Chaplygin top (introduced by D. Goryachev in 1900 and integrated by Sergey Chaplygin in 1948) is also integrable (
Hamiltonian formulation of classical tops
A classical top is defined by three principal axes, defined by the three orthogonal vectors
and the z-components of the three principal axes,
The Poisson algebra of these variables is given by
If the position of the center of mass is given by
The equations of motion are then determined by
Euler top
The Euler top is an untorqued top, with Hamiltonian
The four constants of motion are the energy
Lagrange top
The Lagrange top is a symmetric top with the center of mass along the symmetry axis at location,
The four constants of motion are the energy
and the magnitude of the n-vector
Kovalevskaya top
The Kovalevskaya top is a symmetric top in which
The four constants of motion are the energy
where the variables
the angular momentum component in the z-direction,
and the magnitude of the n-vector