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Dynamical billiards
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Dynamical billiards : ウィキペディア英語版
Dynamical billiards

A billiard is a dynamical system in which a particle alternates between motion in a straight line and specular reflections from a boundary. When the particle hits the boundary it reflects from it without loss of speed. Billiard dynamical systems are Hamiltonian idealizations of the game of billiards, but where the region contained by the boundary can have shapes other than rectangular and even be multidimensional. Dynamical billiards may also be studied on non-Euclidean geometries; indeed, the very first studies of billiards established their ergodic motion on surfaces of constant negative curvature. The study of billiards which are kept out of a region, rather than being kept in a region, is known as outer billiard theory.
The motion of the particle in the billiard is a straight line, with constant energy, between reflections with the boundary (a geodesic if the Riemannian metric of the billiard table is not flat). All reflections are specular: the angle of incidence just before the collision is equal to the angle of reflection just after the collision. The sequence of reflections is described by the billiard map that completely characterizes the motion of the particle.
Billiards capture all the complexity of Hamiltonian systems, from integrability to chaotic motion, without the difficulties of integrating the equations of motion to determine its Poincaré map. Birkhoff showed that a billiard system with an elliptic table is integrable.
== Equations of motion ==
The Hamiltonian for a particle of mass ''m'' moving freely without friction on a surface is:
:H(p, q) = \frac + V(q)
where \scriptstyle V(q) is a potential designed to be zero inside the region \scriptstyle \Omega in which the particle can move, and infinity otherwise:
:V(q) =
\begin
0 &q \in \Omega \\
\infty &q \notin \Omega
\end

This form of the potential guarantees a specular reflection on the boundary. The kinetic term guarantees that the particle moves in a straight line, without any change in energy. If the particle is to move on a non-Euclidean manifold, then the Hamiltonian is replaced by:
:H(p, q) = \fracp^i p^j g_(q) + V(q)
where \scriptstyle g_(q) is the metric tensor at point \scriptstyle q \;\in\; \Omega. Because of the very simple structure of this Hamiltonian, the equations of motion for the particle, the Hamilton–Jacobi equations, are nothing other than the geodesic equations on the manifold: the particle moves along geodesics.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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