Ordinary canonical first-order differential equations describing the motion of holonomic mechanical systems acted upon by external forces, as well as describing the extremals of problems of the classical calculus of variations.
Hamilton's equations, established by W. Hamilton [1], are equivalent to the second-order Lagrange equations (in mechanics) (or to the Euler equation in the classical calculus of variations), in which the unknown magnitudes are the generalized coordinates
where
which has since received the name of Hamilton function (or Hamiltonian). In the right-hand side of (2) the variables
obtained by solving the equations (1). For dynamical systems, in which
such a solution always exists.
Hamilton's equations have the canonical form
Here
The order of the system (3) is
The transition from the variables
[1] | W.R. Hamilton, Philos. Transact. Roy. Soc. London Ser. A , 1 (1835) pp. 95–144 |
[a1] | V.I. Arnol'd, "Mathematical methods of classical mechanics" , Springer (1978) (Translated from Russian) |