The classical Poincaré set #
The classical proof does not require nonvanishing at every resonant action. It requires the set of resonant actions carrying a nonzero disturbing coefficient to be a uniqueness set; density is a convenient sufficient formulation in the real-analytic setting developed here. This file defines that set intrinsically in the full two-dimensional action region and proves the resulting leading-coefficient obstruction.
Prograde, noncircular elliptic actions whose entire ellipse stays inside the unit primary orbit.
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An interior prograde elliptic action, as a topological subtype.
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The classical Poincaré set: rational Kepler resonances at which the disturbing average has a nonzero orientation derivative.
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The exact classical celestial-mechanics input used by the density argument.
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A stronger sufficient condition: every interior positive rational resonance has a nonconstant disturbing average as the relative apsidal orientation varies.
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The open interval of admissible noncircular eccentricities for one fixed positive rational resonance.
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An admissible noncircular eccentricity for one fixed positive rational resonance.
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- LeanPool.PoincareThreeBody.AdmissibleResonantEccentricity p q = { eccentricity : ℝ // eccentricity ∈ LeanPool.PoincareThreeBody.admissibleResonantEccentricitySet p q }
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Eccentricities at a fixed resonance where the resonant disturbing average is nonconstant.
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A one-dimensional sufficient form of the classical perturbing-function calculation: at
every rational resonance, nondegenerate eccentricities are dense in their admissible interval.
Unlike ClassicalDisturbingNondegeneracy, this permits isolated zeros of individual Fourier
coefficients.
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A sharply localized analytic form of the classical disturbing-function input. For every positive rational resonance, two fixed orientations separate at one admissible eccentricity and their averaged-value difference is analytic throughout the admissible eccentricity interval.
The classical high-rank Fourier-coefficient calculation is precisely what supplies the two orientations and the nonzero witness.
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The remaining classical disturbing-function calculation, stripped of analyticity: at every positive rational resonance, two orientations give different averaged perturbations at one admissible eccentricity.
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Compact parameter integration supplies the analytic clause automatically, so the classical Fourier calculation only has to provide a separating value at each resonance.
The admissible eccentricity domain is open.
A positive resonance admits an interior eccentric ellipse exactly when its semimajor axis is strictly inside the unit primary orbit.
A nonempty admissible eccentricity domain is connected.
The Kepler frequency varies continuously on the full interior action subtype.
The represented leading differential varies continuously on the full interior action subtype.
Every member of the classical Poincaré set forces the leading differential and Kepler frequency to have zero wedge.
Density of the classical Poincaré set propagates its resonant obstruction to every interior prograde elliptic action.
Nonvanishing at every interior rational resonance implies density of the classical Poincaré set. The proof uses density of rational Kepler frequencies along the fixed-eccentricity curve through each action.
Density in eccentricity on each rational resonance is enough to make the full classical Poincaré set dense in the two-dimensional interior action region.
Analyticity plus one separating value at each resonance makes the nondegenerate eccentricities dense. Thus the classical calculation need only prove a nonidentity statement, not pointwise nonvanishing at every eccentricity.
The analytic nonidentity statement at each rational resonance supplies the full dense classical Poincaré set.
The original pointwise nondegeneracy condition implies the more flexible fiberwise density condition.