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We classify all planar four-body central configurations where two pairs of the bodies are on parallel lines. Using Cartesian coordinates, we show that the set of four-body trapezoid central configurations with positive masses forms a…

Dynamical Systems · Mathematics 2017-12-21 Montserrat Corbera , Josep M. Cors , Jaume Llibre , Ernesto Perez-Chavela

We consider a symmetric five-body problem with three unequal collinear masses on the axis of symmetry. The remaining two masses are symmetrically placed on both sides of the axis of symmetry. Regions of possible central configurations are…

Earth and Planetary Astrophysics · Physics 2017-08-28 M. Shoaib , A. R. Kashif , I. Szucs-Csillik

In this work, we revisit the planar restricted four-body problem to study the dynamics of an infinitesimal mass under the gravitational force produced by three heavy bodies with unequal masses, forming an equilateral triangle configuration.…

Dynamical Systems · Mathematics 2022-08-31 José Alejandro Zepeda Ramírez , Martha Alvarez-Ramírez

Central configurations give rise to self-similar solutions to the Newtonian $N$-body problem, and play important roles in understanding its complicated dynamics. Even the simple question of whether or not there are finitely many planar…

Dynamical Systems · Mathematics 2019-05-20 Marshall Hampton

In this work we are interested in the central configurations of the spatial seven-body problem where six of them are at vertices of two congruents equilateral triangles belong to parallel planes and one triangle is a rotation by the angle…

Metric Geometry · Mathematics 2015-06-16 Allyson Oliveira

In this paper we discuss the central configurations of the Trapezoidal four-body Problem. We consider four point masses on the vertices of an isosceles trapezoid with two equal masses $m_1=m_4$ at positions $(\mp 0.5, r_B)$ and $m_2=m_3$ at…

Dynamical Systems · Mathematics 2015-04-01 Muhammad Shoaib

An elliptic relative equilibrium (ERE) is a special solution of the planar $N$-body problem generated by a central configuration. Its linear stability depends on the eccentricity $e$ and the masses of the bodies. However, for $e>0$, the…

Dynamical Systems · Mathematics 2025-09-15 Xijun Hu , Yuwei Ou , Jiexin Sun

A previous work introduced pair space, which is spanned by the center of mass of a system and the relative positions (pair positions) of its constituent bodies. Here, I show that in the $N$-body Newtonian problem, a configuration that does…

Mathematical Physics · Physics 2024-10-22 Alon Drory

We study the planar symmetric central configurations of the $1+4$-body problem where the symmetry axis does not contain any infinitesimal masses. Under certain assumptions we find analytically some central configurations, and also get some…

Mathematical Physics · Physics 2017-08-23 Chunhua Deng , Shiqing Zhang

In the studied axisymmetric case of the central four-body problem, the axis of symmetry is defined by two unequal-mass bodies, while the other two bodies are situated symmetrically with respect to this axis and have equal masses. Here, we…

Mathematical Physics · Physics 2020-04-22 Emese Kővári , Bálint Érdi

We introduce an algebraic method to study local stability in the Newtonian $n$-body problem when certain symmetries are present. We use representation theory of groups to simplify the calculations of certain eigenvalue problems. The method…

Dynamical Systems · Mathematics 2021-11-30 Zhihong Xia , Tingjie Zhou

A stochastic optimization algorithm for analyzing planar central and balanced configurations in the $n$-body problem is presented. We find a comprehensive list of equal mass central configurations satisfying the Morse equality up to $n=12$.…

Dynamical Systems · Mathematics 2020-12-24 Alexandru Doicu , Lei Zhao , Adrian Doicu

Continuing work initiated in an earlier publication [Yamada, Asada, Phys. Rev. D 82, 104019 (2010)], we investigate collinear solutions to the general relativistic three-body problem. We prove the uniqueness of the configuration for given…

General Relativity and Quantum Cosmology · Physics 2011-02-28 Kei Yamada , Hideki Asada

In this paper, we consider the elliptic relative equilibria of four-body problem. Here we prove that the corresponding linearized Hamiltonian system at such an elliptic relative equilibria of $4$-bodies splits into two independent linear…

Mathematical Physics · Physics 2021-04-27 Qinglong Zhou

Two numerical algorithms for analyzing planar central and balanced configurations in the $(n+1)$-body problem with a small mass are presented. The first one relies on a direct solution method of the $(n+1)$-body problem by using a…

Dynamical Systems · Mathematics 2022-07-12 Alexandru Doicu , Lei Zhao , Adrian Doicu

The circular restricted three body problem, which considers the dynamics of an infinitesimal particle in the presence of the gravitational interaction with two massive bodies moving on circular orbits about their common center of mass, is a…

Instrumentation and Methods for Astrophysics · Physics 2021-04-07 Cristina Blaga , Paul A. Blaga , Tiberiu Harko

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

In this paper we study the linear stability of relative equilibria in the Newtonian $n$-body problem from the viewpoint of electromagnetic systems. We first examine the effect of the ambient dimension on stability, starting from the…

Dynamical Systems · Mathematics 2026-04-10 Luca Asselle , Giorgia Testolina

In this paper, we consider the elliptic relative equilibria of the restricted $4$-body problems, where the three primaries form an Euler collinear configuration and the four bodies span $\mathbf{R}^2$. We obtain the symplectic reduction to…

Dynamical Systems · Mathematics 2022-05-24 Bowen Liu , Qinglong Zhou

The purpose of this work is to determine the location and stability of the Cassini states of a celestial body with an inviscid fluid core surrounded by a perfectly rigid mantle. Both situations where the rotation speed is either…

Earth and Planetary Astrophysics · Physics 2020-04-22 Gwenaël Boué