Statistics – Computation
Scientific paper
Sep 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1043..112s&link_type=abstract
EXPLORING THE SOLAR SYSTEM AND THE UNIVERSE. AIP Conference Proceedings, Volume 1043, pp. 112-115 (2008).
Statistics
Computation
Celestial Mechanics, Newtonian Mechanics, Rotational Kinematics, Computational Methods In Continuum Mechanics, Lagrangian And Hamiltonian Mechanics, Potential Energy Surfaces For Chemical Reactions, Variational And Optimizational Methods
Scientific paper
The simplest non-collision solutions of the N-body problem are the relative equilibria, in which each body follows a circular orbit around the centre of mass and the shape formed by the N bodies is constant. It is easy to see that the moment of inertia of such a solution is constant. In 1970, D. Saari conjectured that the converse is also true for the planar Newtonian N-body problem: relative equilibria are the only constant-inertia solutions. Here we review some recent results on some generalizations of Saari's Conjecture.
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