Mathematics
Scientific paper
Sep 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979crasm.289..295b&link_type=abstract
Academie des Sciences (Paris), Comptes Rendus, Serie A - Sciences Mathematiques, vol. 289, no. 4, Sept. 17, 1979, p. 295-298. In
Mathematics
1
Canonical Forms, Celestial Mechanics, Four Body Problem, Orbital Mechanics, Transformations (Mathematics), Area, Equations Of Motion, Integral Equations
Scientific paper
The Newtonian four-body problem is reduced to the 14th order by means of canonical transformations with imposed variables, including an area integral. The center of gravity in the problem is eliminated by the introduction of symmetrical variables, reducing the problem to the motion of three fictitious bodies subject to forces deriving from the Newtonian four-body potential in a Hamiltonian formulation. A canonical transformation with the imposition of a variable equal to the third area integral is performed, and a system of two invariant relations is introduced in order to project the angular momentum onto the invariable plane. The successive reductions to fourteenth order, corresponding to node elimination, are then performed by canonical changes in variables and the Jacobi method so that the variables of the reduced problem have a simple geometrical interpretation and permit the explicit calculation of the corresponding Hamiltonian.
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