Hyperbolic motions of any shape exist in the Newtonian N-body problem

You need to know: Euclidean space E={\mathbb R}^d of dimension d, Euclidean norm ||a|| of vector a, (second) derivative of a function x:{\mathbb R}\to E, small o notation o(.).

Background: Let N point particles with masses m_i > 0 and positions x_i(t) \in E at time t are moving according to Newton’s laws of motion: m_j \frac{d^2 x_j}{dt^2} = \sum\limits_{i \neq j} \frac{m_i m_j(x_i - x j)}{r_{ij}^3}, \, 1 \leq j \leq N, where r_{ij} is the distance between x_i and x_j. The motion of particles is determined by the initial conditions: their masses and their positions and velocities at time t=0. Let \Omega be the set of configurations such that the motion has no collisions (r_{ij}(t)>0 for all i,j and t). A motion is called hyperbolic if each particle has a different limit velocity vector, that is, \lim\limits_{t\to \infty} \frac{d x_j}{dt}=a_j \in E and a_i \neq a_j whenever i \neq j.

The Theorem: On 25th August 2019, Ezequiel Maderna and Andrea Venturelli submitted to arxiv a paper in which they proved that for the Newtonian N-body problem in a space E of dimension d\geq 2, there are hyperbolic motions x:[0;+\infty) \to E^N such that x(t) = \sqrt{2h} t a + o(t) as t \to \infty for any choice of x_0 = x(0) \in E^N, for any a=(a_1, \dots, a_N) \in \Omega normalized by ||a||=1, and for any constant h>0.

Short context: The problem of describing motion of N bodies under gravitation (N-body problem) in Euclidean space is a fundamental problem in physics and mathematics, studied by many authors, see, for example, here and here. In general, the motion can be very complicated even for N=3, but can we at least understand hyperbolic motions? The only explicitly known hyperbolic motions are such that the shape of the configuration does not change with time, but it is conjectured that there are only finitely many such motions for any fixed N. In contrast, the Theorem states that hyperbolic motions exist for all initial configurations and all choices of the limited velocities.

Links: Free arxiv version of the original paper is here, journal version is here.

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