6.8: Hamilton’s Equations
( \newcommand{\kernel}{\mathrm{null}\,}\)
Having finally established that we can write, for an incremental change along the dynamical path of the system in phase space,
dH(qi,pi)=−∑i˙pidqi+∑i˙qidpi
we have immediately the so-called canonical form of Hamilton’s equations of motion:
∂H∂pi=˙qi∂H∂qi=−˙pi
Evidently going from state space to phase space has replaced the second order Euler-Lagrange equations with this equivalent set of pairs of first order equations.