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As shown by Johannes Kepler in 1609, in the two-body problem, the shape of the orbit, a given ellipse, and a given non-vanishing constant angular momentum determines the motion of the planet completely. Even in the three-body problem, in…

Mathematical Physics · Physics 2012-01-17 Hiroshi Ozaki , Hiroshi Fukuda , Toshiaki Fujiwara

For three-body problem, R.Montgomery [3] proved a reconstruction formula which calculates the overall rotation relating two similar triangle configurations if the initial triangular configuration is similar to the configuration formed at…

Dynamical Systems · Mathematics 2021-06-30 Wentian Kuang

For 3-body problem with any given masses $m_1, \,m_2,\,m_3>0$, there exist only Eulerian collinear central configuration and Lagrangian equilateral-triangle central configuration, and in this paper, for planar 3-body problem, we prove that…

Dynamical Systems · Mathematics 2021-03-23 Liang Ding , Juan Manuel Sánchez-Cerritos , Jinlong Wei

By introducing simple topological constraints and applying a binary decomposition method, we show the existence of a set of prograde double-double orbits for any rotation angle $\theta \in (0, \pi/7]$ in the equal-mass four-body problem. A…

Dynamical Systems · Mathematics 2017-11-03 Wentian Kuang , Duokui Yan

The central component of a polygon triangulation is defined as the triangle or diameter that contain its geometric center. More generally, every polygon dissection contains a central component. Using this notion, we derive new recurrences…

Combinatorics · Mathematics 2012-10-12 Alon Regev

The Newtonian n-Body Problem is modified assuming positive inertial masses but different sign for the interacting force which is assumed with the possibility of two different signs for the gravitational masses, according to the prescription…

General Physics · Physics 2018-09-17 E. Piña , P. Lonngi

We give a new method to attempt to prove that, for a given $n$, there are finitely many equivalence classes of planar central configurations in the Newtonian $n$-body problem for generic masses. The human part of the proof relies on…

Algebraic Geometry · Mathematics 2025-08-13 Anders N. Jensen , Anton Leykin

We study the dynamics of the collinear points in the planar, restricted three-body problem, assuming that the primaries move on an elliptic orbit around a common barycenter. The equations of motion can be conveniently written in a rotating…

Dynamical Systems · Mathematics 2025-10-28 Alessandra Celletti , Christoph Lhotka , Giuseppe Pucacco

In the $n$-body problem, when a~cluster of bodies tends to a collision, then its normalized shape curve converges to the set of normalized central configurations, which has $SO(2)$ symmetry in the planar case. This leaves a possibility that…

Dynamical Systems · Mathematics 2025-04-25 Anna Gierzkiewicz , Rodrigo G. Schaefer , Piotr Zgliczyński

We study the space of (orthogonal) almost complex structures on closed six-dimensional manifolds as the space of sections of the twistor space for a given metric. For a connected six-manifold with vanishing first Betti number, we express…

Differential Geometry · Mathematics 2022-12-05 Gustavo Granja , Aleksandar Milivojević

Three-body clusters are studied in the algebraic cluster model. Particular attention is paid to the case of three identical particles. It is shown in a geometrical analysis that the harmonic oscillator, the deformed oscillator and the…

Nuclear Theory · Physics 2007-05-23 R. Bijker

This paper demonstrates the existence of twistless tori and the associated reconnection bifurcations and meandering curves in the planar circular restricted three-body problem. Near the Lagrangian equilibrium $\mathcal{L}_4$ a twistless…

Mathematical Physics · Physics 2015-06-17 Holger R Dullin , Joachim Worthington

The gravitation interaction between particles is taken into account in central configuration model. After that, the resonance perturbation of the particle of the central configuration by distant satellite is considered in the restricted…

Dynamical Systems · Mathematics 2007-05-23 A. E. Rosaev

In this paper, we consider the elliptic relative equilibria of the restricted $N$-body problems, where the $N-1$ primaries form an Euler-Moulton collinear central configuration or a $(1+n)$-gon central configuration. We obtain the…

Dynamical Systems · Mathematics 2024-09-24 Jiashengliang Xie , Bowen Liu , Qinglong Zhou

We study the equal-mass classical three rotor problem, a variant of the three body problem of celestial mechanics. The quantum $N$-rotor problem has been used to model chains of coupled Josephson junctions and also arises via a partial…

Chaotic Dynamics · Physics 2019-09-25 Govind S. Krishnaswami , Himalaya Senapati

The three-body problem has been studied for more than three centuries [1,2], and has received much attention in recent years [3-5]. It shows complex dynamical phenomena due to the mutual gravitational interaction of the three bodies. Triple…

Chaotic Dynamics · Physics 2021-01-05 Xiaoming Li , Xiaochen Li , Shijun Liao

We revisit constructions based on triads of conics with foci at pairs of vertices of a reference triangle. We find that their 6 vertices lie on well-known conics, whose type we analyze. We give conditions for these to be circles and/or…

Metric Geometry · Mathematics 2022-07-21 Ronaldo Garcia , Liliana Gheorghe , Peter Moses , Dan Reznik

The simplest solutions of the N-body problem --symmetric relative equilibria-- are shown to be organizing centers from which stem some recently studied classes of periodic solutions. We focus on the relative equilibrium of the equal-mass…

Dynamical Systems · Mathematics 2011-10-12 Alain Chenciner , Jacques Féjoz

We present for the first time an explicit, complete and closed-form solution to the three-dimensional problem of two fixed centres, based on Weierstrass elliptic and related functions. With respect to previous treatments of the problem, our…

Earth and Planetary Astrophysics · Physics 2015-12-09 Francesco Biscani , Dario Izzo

We discuss the equilibrium conditions for a body made of two homogeneous components separated by oblate spheroidal surfaces and in relative motion. While exact solutions are not permitted for rigid rotation (unless a specific ambient…

Solar and Stellar Astrophysics · Physics 2022-04-13 Jean-Marc Huré