Symplectic invariants for parabolic orbits and cusp singularities of integrable systems with two degrees of freedom
Alexey Bolsinov, Lorenzo Guglielmi, Elena Kudryavtseva
TL;DR
The paper develops a symplectic-invariant framework for parabolic orbits and cuspidal tori in integrable Hamiltonian systems with two degrees of freedom. It first establishes a canonical parabolic model $H = \pm(x^2 + y^3 + b(\lambda) y + a(\lambda))$, $F = \lambda$, and then analyzes the symplectic structure near a parabolic orbit via a tubular $(x,y,\lambda,\varphi)$-description, reducing to a $1$-degree-of-freedom problem on each $\lambda$-slice. It derives intrinsic invariants from action variables (and associated period data) that classify parabolic singularities, both in the single-parameter and parametric contexts, and extends these ideas to semi-local invariants of cuspidal tori: two fibrations with matching cusp bifurcation diagrams and identical action data are fiberwise symplectomorphic. The results rely on complexification, versal deformation arguments, and a careful analysis of period mappings, yielding necessary and sufficient conditions for local and semi-local symplectic equivalence and highlighting the canonical affine structure of the base as the fundamental semi-local invariant. Overall, the work provides a systematic, invariant-based approach to degenerate singularities in low-dimensional integrable systems with potential generalization to more degrees of freedom.
Abstract
We discuss normal forms and symplectic invariants of parabolic orbits and cuspidal tori in integrable Hamiltonian systems with two degrees of freedom. Such singularities appear in many integrable systems in geometry and mathematical physics and can be considered as the simplest example of degenerate singularities. We also suggest some new techniques which apparently can be used for studying symplectic invariants of degenerate singularities of more general type.
