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The three-body problem and the equations of dynamics: Poincaré’s foundational work on dynamical systems theory

Here is an accurate and readable translation of a seminal article by Henri Poincaré that is a classic in the study of dynamical systems popularly called chaos theory. In an effort to understand the stability of orbits in the solar system, Poincaré applied a Hamiltonian formulation to the equations o...

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Detalles Bibliográficos
Autor principal: Poincaré, Henri
Lenguaje:eng
Publicado: Springer 2017
Materias:
Acceso en línea:https://dx.doi.org/10.1007/978-3-319-52899-1
http://cds.cern.ch/record/2267301
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author Poincaré, Henri
author_facet Poincaré, Henri
author_sort Poincaré, Henri
collection CERN
description Here is an accurate and readable translation of a seminal article by Henri Poincaré that is a classic in the study of dynamical systems popularly called chaos theory. In an effort to understand the stability of orbits in the solar system, Poincaré applied a Hamiltonian formulation to the equations of planetary motion and studied these differential equations in the limited case of three bodies to arrive at properties of the equations’ solutions, such as orbital resonances and horseshoe orbits. Poincaré wrote for professional mathematicians and astronomers interested in celestial mechanics and differential equations. Contemporary historians of math or science and researchers in dynamical systems and planetary motion with an interest in the origin or history of their field will find his work fascinating. .
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spelling cern-22673012021-04-21T19:12:12Zdoi:10.1007/978-3-319-52899-1http://cds.cern.ch/record/2267301engPoincaré, HenriThe three-body problem and the equations of dynamics: Poincaré’s foundational work on dynamical systems theoryAstrophysics and AstronomyHere is an accurate and readable translation of a seminal article by Henri Poincaré that is a classic in the study of dynamical systems popularly called chaos theory. In an effort to understand the stability of orbits in the solar system, Poincaré applied a Hamiltonian formulation to the equations of planetary motion and studied these differential equations in the limited case of three bodies to arrive at properties of the equations’ solutions, such as orbital resonances and horseshoe orbits. Poincaré wrote for professional mathematicians and astronomers interested in celestial mechanics and differential equations. Contemporary historians of math or science and researchers in dynamical systems and planetary motion with an interest in the origin or history of their field will find his work fascinating. .Springeroai:cds.cern.ch:22673012017
spellingShingle Astrophysics and Astronomy
Poincaré, Henri
The three-body problem and the equations of dynamics: Poincaré’s foundational work on dynamical systems theory
title The three-body problem and the equations of dynamics: Poincaré’s foundational work on dynamical systems theory
title_full The three-body problem and the equations of dynamics: Poincaré’s foundational work on dynamical systems theory
title_fullStr The three-body problem and the equations of dynamics: Poincaré’s foundational work on dynamical systems theory
title_full_unstemmed The three-body problem and the equations of dynamics: Poincaré’s foundational work on dynamical systems theory
title_short The three-body problem and the equations of dynamics: Poincaré’s foundational work on dynamical systems theory
title_sort three-body problem and the equations of dynamics: poincaré’s foundational work on dynamical systems theory
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1007/978-3-319-52899-1
http://cds.cern.ch/record/2267301
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