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 first 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 constraints 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. As a second step, this result admits a qualitative dynamical
interpretation via the open book decomposition by disk-like global surfaces of
section bounded by the Euler orbit. In this setting, the rotation number
and the contact volume define a nontrivial twist interval which encodes the
relative winding of periodic orbits. Refining Hutchings’ mean action inequality,
we prove that every rational number in the interior of the twist interval is
realized as the mean relative winding number of two distinct periodic points of
the first return map. For energies above the critical level, where the energy
surface is noncompact, we prove the existence of infinitely many periodic
orbits and infinitely many parabolic trajectories via twist estimates near
infinity.
Keywords
ECH, isosceles three-body problem, open book
decompositions, area-preserving disk maps, Hamiltonian
systems, symplectic dynamics