Existence of hyperbolic motions to a class of Hamiltonians and generalized $N$-body system via a geometric approach

TL;DR

This paper presents a new geometric proof for the existence of hyperbolic motions in the classical N-body problem and generalized Hamiltonian systems, extending previous results without relying on long-time behavior or weak KAM theory.

Contribution

It introduces a geometric approach to establish hyperbolic motions for a broader class of Hamiltonians, bypassing previous complex analytical methods.

Findings

Proves existence of hyperbolic motions for Hamiltonians with slowly decreasing potentials.

Extends results to generalized N-body systems with potentials in C^2.

Provides uniform estimates for geodesics in Ma ext{n}é's potential.

Abstract

For the classical $N$-body problem in $\mathbb{R}^d$ with $d\ge2$, Maderna-Venturelli in their remarkable paper [Ann. Math. 2020] proved the existence of hyperbolic motions with any positive energy constant, starting from any configuration and along any non-collision configuration. Their original proof relies on the long time behavior of solutions by Chazy 1922 and Marchal-Saari 1976, on the H\"{o}lder estimate for Ma\~{n}\'{e}'s potential by Maderna 2012, and on the weak KAM theory. We give a new and completely different proof for the above existence of hyperbolic motions. The central idea is that, via some geometric observation, we build up uniform estimates for Euclidean length and angle of geodesics of Ma\~{n}\'{e}'s potential starting from a given configuration and ending at the ray along a given non-collision configuration. Note that we do not need any of the above previous studies used in Maderna-Venturelli's proof. Moreover, our geometric approach works for Hamiltonians $\frac12\|p\|^2-F(x)$, where $F(x)\ge 0$ is lower semicontinuous and decreases very slowly to $0$ faraway from collisions. We therefore obtain the existence of hyperbolic motions to such Hamiltonians with any positive energy constant, starting from any admissible configuration and along any non-collision configuration. Consequently, for several important potentials $F\in C^{2}(\Omega)$, we get similar existence of hyperbolic motions to the generalized $N$-body system $\ddot{x} = \nabla_x F(x)$, which is an extension of Maderna-Venturelli [Ann. Math. 2020].