For ordinary conservative classical mechanics, the Lagrangian is , where is the kinetic energy and the potential energy. More generally it is the function whose action satisfies the principle of stationary action. The canonical momenta and Hamiltonian are
For a regular Lagrangian, the first equations can be inverted to express the generalized velocities in terms of ; this defines the Legendre transform on phase space.
Along a solution of the Euler-Lagrange equations, . Taking a total time derivative gives
Thus an autonomous Lagrangian has
For the usual time-independent mechanical coordinates and a velocity-independent potential energy, the kinetic energy is quadratic in the generalized velocities, so and . The conservation proof itself uses the Euler-Lagrange equations, rather than assuming this special expression for energy.

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