The equations defined by
where 
 and 
 is the so-called Hamiltonian, 
 are called Hamilton's equations.  These
equations frequently arise in problems of celestial mechanics. 
  Another
formulation related to Hamilton's equation is
  | 
(3) | 
 
where 
 is the so-called Lagrangian. 
References
Morse, P. M. and Feshbach, H.  ``Hamilton's Principle and Classical Dynamics.''  §3.2 in
  Methods of Theoretical Physics, Part I.  New York: McGraw-Hill, pp. 280-301, 1953.
 
© 1996-9 Eric W. Weisstein 
1999-05-25