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Autores principales: Cendra, Hernán, García, María Eugenia
Formato: Preprint
Publicado: 2024
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Acceso en línea:https://arxiv.org/abs/2406.01531
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author Cendra, Hernán
García, María Eugenia
author_facet Cendra, Hernán
García, María Eugenia
contents In this paper we describe optimal reduction for the system of two bodies in $\mathbb{R}^3$ whose Hamiltonian is invariant under rotations and translations. In doing this, we introduce parametrizations and charts which help giving explicit expressions in order to deal with geometric and dynamical aspects of the reduction process. For this system, the standard assumptions of the Marsden-Weinstein reduction process are only partially satisfied while optimal reduction can be readily applied, and we study a comparison between those two reduction processes. We describe potential applications to the study of Post-Newtonian Hamiltonian systems for binary systems in astronomy.
format Preprint
id arxiv_https___arxiv_org_abs_2406_01531
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle The Optimal Reduction of a 2-Body Problem in R^3
Cendra, Hernán
García, María Eugenia
Mathematical Physics
In this paper we describe optimal reduction for the system of two bodies in $\mathbb{R}^3$ whose Hamiltonian is invariant under rotations and translations. In doing this, we introduce parametrizations and charts which help giving explicit expressions in order to deal with geometric and dynamical aspects of the reduction process. For this system, the standard assumptions of the Marsden-Weinstein reduction process are only partially satisfied while optimal reduction can be readily applied, and we study a comparison between those two reduction processes. We describe potential applications to the study of Post-Newtonian Hamiltonian systems for binary systems in astronomy.
title The Optimal Reduction of a 2-Body Problem in R^3
topic Mathematical Physics
url https://arxiv.org/abs/2406.01531