Abstract
The word "average" and its variations became popular in the sixties and implicitly carried the idea that "averaging" methods lead to "average" Hamiltonians. However, given the Hamiltonian H = H0(J) + ∈R(θ, J), (∈ < < 1), the problem of transforming it into a new Hamiltonian H* (J*) (dependent only on the new actions J*), through a canonical transformation given by zero-average trigonometrical series has no general solution at orders higher than the first.
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References
Born, M.: 1926, Problems of Atomic Dynamics, M.I.T., Cambridge (US).
Brouwer, D.: 1959, Solution of the problem of artificial satellite theory without drag, Astron. J., 64, 378-397.
Charlier, C.V.L.: 1907, Die Mechanik des Himmels, De Gruyter, Leipzig, Vol. II.
Delaunay, C.: 1868, Mémoire sur la Théorie de la Lune, Acad. Sc., Paris.
Deprit, A.: 1969, Canonical transformation depending on a small parameter, Cel. Mech. & Dyn. Astr., 1, 12-30.
Hori, G.-I.: 1966, Theory of General Perturbations with Unspecified Canonical Variables, Publ. Astron. Soc. Japan, 18, 287-296.
Kolmogorov, A.N.: 1954, Preservation of conditionally periodic movements with small change in Hamiltonian function, Dokl. Akad. Nauk, 98, 527-530.
Milani, A.; Nobili, A.M. and Carpino, M.: 1987, Secular variations of the semimajor axes: theory and experiments, Astron. Astrophys., 172, 265-279.
Poincaré, H.: 1893, Les Méthodes Nouvelles de la Mécanique Celeste, Gauthier-Villars, Paris, Vol. II.
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Ferraz-Mello, S. Do Average Hamiltonians Exist?. Celestial Mechanics and Dynamical Astronomy 73, 243–248 (1999). https://doi.org/10.1023/A:1008363517421
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DOI: https://doi.org/10.1023/A:1008363517421