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The motion of a satellite around a planet can be studied by the Hill model, which is a modification of the restricted three body problem pertaining to motion of a satellite around a planet. Although the dynamics of the circular Hill model…

Earth and Planetary Astrophysics · Physics 2015-03-19 G. Voyatzis , I. Gkolias , H. Varvoglis

When dealing with satellites orbiting a central body on a highly elliptical orbit, it is necessary to consider the effect of gravitational perturbations due to external bodies. Indeed, these perturbations can become very important as soon…

Earth and Planetary Astrophysics · Physics 2016-05-26 Guillaume Lion , Gilles Métris , Florent Deleflie

The problem of describing the free motions of three gravitating bodies under each others gravitational influence is one of the oldest of unsolved problems of classical mechanics. Henry Poincare proved in his dictum that due to the nature of…

Mathematical Physics · Physics 2016-09-07 AbuBakr Mehmood , Syed Umer Abbas Shah , Ghulam Shabbir

Explicit solutions of the two-dimensional floating body problem (bodies that can float in all positions) for relative density rho different from 1/2 and of the tire track problem (tire tracks of a bicycle, which do not allow to determine,…

Classical Physics · Physics 2007-05-23 Franz Wegner

Various astrophysical processes are known, where the fly-by of a massive object affects matter initially supported against gravity by rotation. Examples are perturbations of galaxies, protoplanetary discs or planetary systems. We…

Earth and Planetary Astrophysics · Physics 2017-11-06 Andreas Breslau , Kirsten Vincke , Susanne Pfalzner

We construct a highly-symmetric periodic orbit of six bodies in three dimensions. In this orbit, binary collisions occur at the origin in a regular periodic fashion, rotating between pairs of bodies located on the coordinate axes.…

Dynamical Systems · Mathematics 2023-08-24 Skyler Simmons

Since Poincar\'e, periodic orbits have been one of the most important objects in dynamical systems. However, searching them is in general quite difficult. A common way to find them is to construct families of periodic orbits which start at…

Dynamical Systems · Mathematics 2019-10-24 Seongchan Kim

The dynamics of the Restricted 3 Body Problem in the Post Newtonian context have been, and continue to be, studied extensively and a number of characteristics such as ejections of bodies from the system, precession of orbits, chaotic…

General Relativity and Quantum Cosmology · Physics 2023-11-07 Patric de Gentile-Williams

In this article we show the crucial role of elliptic regularity theory for the development of efficient numerical methods for the solution of some variational problems. Here we focus to a class of elliptic multiobjective optimal control…

Optimization and Control · Mathematics 2021-01-27 A. Dreves , J. Gwinner , N. Ovcharova

In this article I will review some basic results on elliptic boundary value problems with applications to General Relativity.

General Relativity and Quantum Cosmology · Physics 2015-06-25 Sergio Dain

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 relative equilibria for the spherical, finite density 3 body problem are identified. Specifically, there are 28 distinct relative equilibria in this problem which include the classical 5 relative equilibria for the point-mass 3-body…

Dynamical Systems · Mathematics 2016-06-22 D. J. Scheeres

The problem of nonintegrability of the circular restricted three-body problem is very classical and important in the theory of dynamical systems. It was partially solved by Poincare in the nineteenth century: He showed that there exists no…

Dynamical Systems · Mathematics 2024-03-05 Kazuyuki Yagasaki

Using a variational method, we exhibit a surprisingly simple periodic orbit for the newtonian problem of three equal masses in the plane. The orbit has zero angular momentum and a very rich symmetry pattern. Its most surprising feature is…

Dynamical Systems · Mathematics 2016-09-07 Alain Chenciner , Richard Montgomery

We consider a two-dimensional, incompressible fluid body, together with self-induced interactions. The body is perturbed by an external particle with small mass. The whole configuration rotates uniformly around the common center of mass. We…

Analysis of PDEs · Mathematics 2026-02-25 Diego Alonso-Orán , Bernhard Kepka , Juan J. L. Velázquez

In this paper, an approach is developed to solve the three body problem involving masses which posses spherical symmetry. The problem dates back to the times of Poincare, and is undoubtedly one of the oldest of unsolved problems of…

Mathematical Physics · Physics 2007-05-23 A. B. Mehmood , U. A. Shah , G. Shabbir

In this paper we establish links between, and new results for, three problems that are not usually considered together. The first is a matrix decomposition problem that arises in areas such as statistical modeling and signal processing:…

Optimization and Control · Mathematics 2013-02-05 James Saunderson , Venkat Chandrasekaran , Pablo A. Parrilo , Alan S. Willsky

Continuing work initiated in an earlier publication [H. Asada, Phys. Rev. D {\bf 80}, 064021 (2009)], the gravitational radiation reaction to Lagrange's equilateral triangular solution of the three-body problem is investigated in an…

General Relativity and Quantum Cosmology · Physics 2018-01-22 Kei Yamada , Hideki Asada

The restricted planar three-body problem has a rich history, yet many unanswered questions still remain. In the present paper we prove the existence of a global surface of section near the smaller body in a new range of energies and mass…

Symplectic Geometry · Mathematics 2012-08-13 Peter Albers , Joel W. Fish , Urs Frauenfelder , Helmut Hofer , Otto van Koert

The Newtonian restricted three-body problem involving a positive primary point mass, $m_+$, and a negative secondary point mass, $m_-$, in a circular orbit, and a positive or negative tertiary point mass, $m_3$, with $m_+ > |m_-| \gg…

Classical Physics · Physics 2024-12-05 K. H. Thong , A. Melatos
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