ECH Constraints and Twist Dynamics in the Spatial Isosceles Three-Body Problem

Fuente: arXiv
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Hauptverfasser: Hu, Xijun, Liu, Lei, Ou, Yuwei, Qiao, Zhiwen, Salomão, Pedro A. S.
Format: Preprint
Veröffentlicht: 2026
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author Hu, Xijun
Liu, Lei
Ou, Yuwei
Qiao, Zhiwen
Salomão, Pedro A. S.
author_facet Hu, Xijun
Liu, Lei
Ou, Yuwei
Qiao, Zhiwen
Salomão, Pedro A. S.
contents We study dynamical constraints arising from Embedded Contact Homology (ECH) in the spatial isosceles three-body problem. For energies below the critical level, the dynamics on the energy surface is identified with a Reeb flow on the tight three-sphere. We obtain quantitative estimates for the Euler orbit, including monotonicity of its transverse rotation number and a strict inequality comparing its action with the contact volume. Combined with the ECH classification of Reeb flows on the tight three-sphere with two simple periodic orbits, these estimates rule out the two-orbit scenario, thus forcing every compact energy surface below the critical level to have infinitely many periodic orbits. The result admits a dynamical interpretation via disk-like global surfaces of section bounded by the Euler orbit. In this setting, the rotation number and the contact volume define a non-trivial twist interval which encodes the relative winding of periodic orbits. For energies above the critical level, where the energy surface is non-compact, we prove the existence of infinitely many periodic orbits and infinitely many parabolic trajectories via twist estimates near infinity.
format Preprint
id arxiv_https___arxiv_org_abs_2602_24025
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle ECH Constraints and Twist Dynamics in the Spatial Isosceles Three-Body Problem
Hu, Xijun
Liu, Lei
Ou, Yuwei
Qiao, Zhiwen
Salomão, Pedro A. S.
Symplectic Geometry
Mathematical Physics
Dynamical Systems
We study dynamical constraints arising from Embedded Contact Homology (ECH) in the spatial isosceles three-body problem. For energies below the critical level, the dynamics on the energy surface is identified with a Reeb flow on the tight three-sphere. We obtain quantitative estimates for the Euler orbit, including monotonicity of its transverse rotation number and a strict inequality comparing its action with the contact volume. Combined with the ECH classification of Reeb flows on the tight three-sphere with two simple periodic orbits, these estimates rule out the two-orbit scenario, thus forcing every compact energy surface below the critical level to have infinitely many periodic orbits. The result admits a dynamical interpretation via disk-like global surfaces of section bounded by the Euler orbit. In this setting, the rotation number and the contact volume define a non-trivial twist interval which encodes the relative winding of periodic orbits. For energies above the critical level, where the energy surface is non-compact, we prove the existence of infinitely many periodic orbits and infinitely many parabolic trajectories via twist estimates near infinity.
title ECH Constraints and Twist Dynamics in the Spatial Isosceles Three-Body Problem
topic Symplectic Geometry
Mathematical Physics
Dynamical Systems
url https://arxiv.org/abs/2602.24025