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2012.04696

SYMBOLIC DYNAMICS IN THE ELLIPTIC ISOSCELES RESTRICTED THREE BODY PROBLEM

Marcel Guardia, Jaime Paradela, Tere M. Seara, Claudio Vidal

correcthigh confidence
Category
Not specified
Journal tier
Specialist/Solid
Processed
Sep 28, 2025, 12:55 AM

Audit review

The paper proves that for sufficiently large angular momentum G, the Poincaré map ψ on the pericenter section Σ+ admits an invariant set S topologically conjugate to the full shift on N^Z (a Smale horseshoe with infinitely many symbols), see Theorem 1.1 and the definition of Σ+ in the text . The proof proceeds by a conformally symplectic scaling that exhibits a parabolic periodic orbit at infinity and treats the system as a fast non-autonomous perturbation of Kepler’s problem . Then Theorem 2.1 establishes an exponentially small but nonzero splitting with an explicit first-order formula (2.8) yielding at least two transverse homoclinic connections to the infinity orbit . Finally, a Moser-type construction produces the symbolic dynamics and the conjugacy to the shift (Theorem 2.4) . The candidate solution follows this blueprint accurately overall. Two notable inaccuracies are: (i) it wrongly infers “infinitely many” primary homoclinic intersections from the Bessel factor, whereas the paper’s first-order distance uses J1(1) as a constant and guarantees at least two intersections via the sine factor in (2.8) ; and (ii) it describes the infinity orbit as “normally hyperbolic,” while it is parabolic in this setting . These do not affect the final conclusion, since countably many symbols arise from the time-of-flight coding near infinity (Theorem 2.4) rather than from having infinitely many distinct primary intersections .

Referee report (LaTeX)

\textbf{Recommendation:} minor revisions

\textbf{Journal Tier:} specialist/solid

\textbf{Justification:}

The paper delivers a rigorous and technically sophisticated proof of symbolic dynamics in the REI3BP at large angular momentum using exponentially small splitting near a parabolic periodic orbit at infinity and a Moser-type construction. The results are significant within dynamical systems and celestial mechanics. Clarifying the role of the auxiliary map in the splitting analysis versus the pericenter Poincaré map used for coding, and explicitly noting that only a finite number (at least two) of primary homoclinic intersections are required, would further improve accessibility without altering content.