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Strict convexity away from the saddle-centers in a regularization model

Proved
BirkhoffGlobalSection.regularization_model_convex_away_from_saddle_center

by caleb · Sep 28, 2026 · Mathlib 0df444a (Lean v4.33.1)

dynamical-systemssymplectic-geometry

Strict convexity away from the equal-mass saddle-centers persists near the critical energy, in a suitable regularization.

Let U⊂R4U\subset\mathbb{R}^4U⊂R4 be an open set containing the Levi-Civita points S±=(±12,0,0,0)S_\pm=(\pm\tfrac12,0,0,0)S±​=(±21​,0,0,0), which lie over the first Lagrange point for μ=12\mu=\tfrac12μ=21​ at the critical energy c=2c=2c=2. Then there exist ε,η>0\varepsilon,\eta>0ε,η>0 with the following property. Whenever

0<μ<1,∣μ−12∣<ε,c<2+η,−c<h1(μ),0<\mu<1,\qquad |\mu-\tfrac12|<\varepsilon,\qquad c<2+\eta,\qquad -c<h_1(\mu),0<μ<1,∣μ−21​∣<ε,c<2+η,−c<h1​(μ),

the selected Levi-Civita component Σμ,c\Sigma_{\mu,c}Σμ,c​ admits a regularization model (Φ,G)(\Phi,G)(Φ,G) such that

Φ(s) is a strictly convex star-shaped point of Gfor every s∈Σμ,c∖U.\Phi(s)\ \text{is a strictly convex star-shaped point of } G\qquad\text{for every } s\in\Sigma_{\mu,c}\setminus U .Φ(s) is a strictly convex star-shaped point of Gfor every s∈Σμ,c​∖U.

A regularization model is a smooth symplectic (up to a positive constant) change of coordinates carrying the Levi-Civita flow to a model Hamiltonian flow up to a positive time change. A strictly convex star-shaped point is one where the model level set is radially transverse and has positive definite second fundamental form.

In Liu–Salomão, the equal-mass critical surface is strictly convex away from its two saddle-center singularities in the elliptic-hyperbolic regularization of Section 9.2 (Theorem 1.12, proved in Section 9). Section 10 uses this for nearby parameters on the part of the surface outside a neighborhood of the singularities. This statement makes that step explicit, with the centered elliptic-hyperbolic coordinates as the intended model. Convexity depends on the coordinates, so the statement is made in the model and not in Levi-Civita coordinates.

Formalization Note The model is RegularizationModel μ c and the pointwise condition is IsStrictlyConvexStarShapedAt, both from Def_BirkhoffGlobalSection_RegularizationModel. The model may depend on UUU and on (μ,c)(\mu,c)(μ,c).

Preamble
import Definitions.Def_BirkhoffGlobalSection_RegularizationModel
Formal statement
namespace BirkhoffGlobalSection

/-- Persistence of strict convexity away from the saddle-centers. Fix any open
set containing the Levi-Civita lifts `(±1/2, 0, 0, 0)` of the first Lagrange
point for `μ = 1/2`. For parameters in a small enough one-sided subcritical strip
around `(1/2, 2)`, the selected component admits a regularization model in which
the image of every point outside the set is strictly convex and star-shaped.
This packages the strict convexity of the equal-mass critical surface in the
elliptic-hyperbolic regularization of Liu--Salomao (Theorem 1.12, Section 9)
and its persistence under small changes of `(μ, c)`, as used in Section 10. -/
theorem regularization_model_convex_away_from_saddle_center
    (U : Set Phase) (hU : IsOpen U)
    (hplus : (![1 / 2, 0, 0, 0] : Phase) ∈ U)
    (hminus : (![-(1 / 2), 0, 0, 0] : Phase) ∈ U) :
    ∃ ε η : ℝ, 0 < ε ∧ 0 < η ∧
      ∀ μ c : ℝ, 0 < μ → μ < 1 →
        |μ - 1 / 2| < ε → c < 2 + η → belowFirstCriticalValue μ c →
        ∃ M : RegularizationModel μ c,
          ∀ s ∈ leftEnergyComponent μ c, s ∉ U →
            IsStrictlyConvexStarShapedAt M.modelHamiltonian (M.toModel s) := by sorry

end BirkhoffGlobalSection
Source
Liu--Salomao, Finite energy foliations and global dynamics in the restricted three-body problem, https://arxiv.org/html/2506.17867v2. Theorem 1.12 (strict convexity at mu = 1/2 for E <= -2, proved in Section 9 via Theorems 9.1, 9.4 and Proposition 9.9); Section 9.2 (elliptic-hyperbolic regularization); Section 10, first paragraph (convexity of the critical surface used for nearby (mu, E) outside a neighborhood of the saddle-centers).

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