The resonant disturbing average #
Rotating the inertial ellipse by an orientation phase produces the phase family on a resonant torus. We define the first-order disturbing function on this family and its average over the common period. Nonconstancy of this average is the concrete perturbative input in Poincaré's argument.
A resonant Kepler ellipse with an arbitrary inertial orientation phase.
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The oriented resonant position embedded in phase space.
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The first-order disturbing function along an oriented resonant ellipse.
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The disturbing function averaged over one common resonant period.
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Orientation derivative of the disturbing function along a resonant ellipse.
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Differentiating the disturbing function with respect to the ellipse orientation gives the explicit rotational derivative.
Differentiation under the period integral identifies the derivative of the Poincaré disturbing average with the integral of the explicit orientation forcing.
Distinct certified values of the Poincaré average imply a nonzero resonant forcing integral at some orientation. This is the interface intended for exact analytic estimates or validated finite computation.
The averaged homological obstruction specialized to the explicit resonant disturbing function. The remaining concrete input is nonvanishing of its orientation derivative integral.
Collision-free interior ellipses automatically satisfy the integrability hypothesis in the concrete averaged obstruction.
Equivalent concrete obstruction using nonvanishing of the derivative of the Poincaré disturbing average.