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LeanPool.PoincareThreeBody.KeplerHamiltonian

Differential of the rotating Kepler Hamiltonian #

We compute the Fréchet derivative of the mass-zero Hamiltonian and identify its Hamiltonian vector field with rotatingKeplerVectorField. Consequently, a Poisson bracket with the Kepler Hamiltonian is exactly differentiation along a Kepler flow line.

Explicit differential of the rotating Kepler Hamiltonian.

Equations
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Instances For

    Fréchet derivative of the mass-zero Hamiltonian away from the Kepler collision.

    The Poisson bracket with the Kepler Hamiltonian is the directional derivative along its explicit Hamiltonian vector field.

    theorem LeanPool.PoincareThreeBody.DifferentiableAt.hasDerivAt_comp_orientedResonantKeplerPhasePoint {F : PhaseSpace} {p q : } (hp : 0 < p) (hq : 0 < q) {eccentricity orientation time : } (heccentricity : 0 eccentricity) (heccentricityOne : eccentricity < 1) (hF : DifferentiableAt F (orientedResonantKeplerPhasePoint p q eccentricity orientation time)) :
    HasDerivAt (fun (t : ) => F (orientedResonantKeplerPhasePoint p q eccentricity orientation t)) (poissonBracket F (hamiltonian 0) (orientedResonantKeplerPhasePoint p q eccentricity orientation time)) time

    Along the true resonant orbit, the time derivative of any differentiable observable is its Poisson bracket with the mass-zero Hamiltonian.