The Classical N-body Problem in the Context of Curved Space
Canadian journal of mathematics, Tome 69 (2017) no. 4, pp. 790-806
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We provide the differential equations that generalize the Newtonian $N$ -body problem of celestial mechanics to spaces of constant Gaussian curvature $\kappa $ , for all $\kappa \in \mathbb{R}$ . In previous studies, the equations of motion made sense only for $\kappa \ne 0$ . The system derived here does more than just include the Euclidean case in the limit $\kappa \to 0;$ it recovers the classical equations for $\kappa =0$ . This new expression of the laws of motion allows the study of the $N$ -body problem in the context of constant curvature spaces and thus oòers a natural generalization of the Newtonian equations that includes the classical case. We end the paper with remarks about the bifurcations of the first integrals.
Diacu, Florin. The Classical N-body Problem in the Context of Curved Space. Canadian journal of mathematics, Tome 69 (2017) no. 4, pp. 790-806. doi: 10.4153/CJM-2016-041-2
@article{10_4153_CJM_2016_041_2,
author = {Diacu, Florin},
title = {The {Classical} {N-body} {Problem} in the {Context} of {Curved} {Space}},
journal = {Canadian journal of mathematics},
pages = {790--806},
year = {2017},
volume = {69},
number = {4},
doi = {10.4153/CJM-2016-041-2},
url = {http://geodesic.mathdoc.fr/articles/10.4153/CJM-2016-041-2/}
}
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