Transport a phase-space density along Hamilton's equations. The Hamiltonian vector field is and the equation is . Its zero divergence gives volume-preserving transport. For , the density is constant along characteristics; a source is integrated by the Duhamel formula for Hamiltonian transport. This is distinct from the elliptic Liouville equation.
The Hamiltonian gives , . Its characteristic flow map is multiplication by , with and determinant one. The backward map is . This expanding-contracting linear flow preserves phase-space Lebesgue measure and every finite- integral of a transported density, despite stretching its level sets.
If and a nonzero time-independent source is invariant along the Hamiltonian flow, then the Duhamel formula for Hamiltonian transport gives . For the nonzero-frequency oscillator, is smooth and belongs to all finite Lp spaces, yet its resulting solution has infinite space-time norm on .
The Duhamel formula for Hamiltonian transport, phase space preservation and Minkowski integral inequality give the displayed bound. A time-independent source in an Lp space yields finite space-time norm on every bounded interval; it need not yield integrability on infinite time.
Smooth forcing need not be integrable in phase space. For the hyperbolic characteristic flow for an inverted oscillator, the source accumulates as . Its smallest quadratic-form eigenvalue is for . Starting with a nonnegative integrable Gaussian function, the solution is therefore unbounded and outside every finite Lp space at positive times. Locally time-integrable forcing prevents this failure by the Minkowski integral inequality.
For a complete invertible Hamiltonian flow , integrate the source along the backward characteristic ending at at time . The displayed formula solves the Hamiltonian Liouville equation. Volume preservation makes each composition with an isometry of Lp spaces.
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