Along a trajectory generated by the Hamiltonian ,Thus a time-independent observable is conserved exactly when its Poisson bracket with vanishes.
Along Hamilton's equations, spatial derivatives of the Hamiltonian function cancel in its total time derivative. Thus . An autonomous Hamiltonian function is conserved; explicit time dependence generally prevents conservation even though phase space is still preserved.
For an autonomous Lagrangian , define its action and Hamiltonian . The chain rule givesThus the identity holds along forced trajectories as well as solutions of the homogeneous Euler-Lagrange equation. Explicit time dependence adds ; stochastic work requires a consistent regularization or the Stratonovich chain rule.
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