Contact geometry of Hill's approximation in a spatial restricted four-body problem
Cengiz Aydin
TL;DR
The paper proves that Hill's approximation in the spatial equilateral circular R4BP possesses the contact type property below the first critical value for all mass ratios $\mu\in[0,\tfrac{1}{2}]$. It achieves this by constructing a Liouville vector field transverse to the energy hypersurface, first in the non-regularized setting and then after Moser regularization, which interchanges position and momentum and uses a stereographic projection to $T^*S^3$. Consequently, the bounded, regularized Hill energy level is fiberwise starshaped and diffeomorphic to $S^*S^3$ with the standard contact structure, while the planar restriction corresponds to $S^*S^2$. This contact-type property opens the door to applying holomorphic curve methods and Floer theory to analyze Reeb dynamics and global surface-of-section questions in the Hill four-body context, mirroring results known for CR3BP and its planar/spatial variants.
Abstract
It is well-known that the planar and spatial circular restricted three-body problem (CR3BP) is of contact type for all energy values below the first critical value. Burgos-García and Gidea extended Hill's approach in the CR3BP to the spatial equilateral CR4BP, which can be used to approximate the dynamics of a small body near a Trojan asteroid of a Sun--planet system. Our main result in this paper is that this Hill four-body system also has the contact property. In other words, we can "contact" the Trojan. Such a result enables to use holomorphic curve techniques and Floer theoretical tools in this dynamical system in the energy range where the contact property holds.
