Abstract
This paper presents a method for constructing a transformation of coordinates in phase space yielding canonical equations. The general transformation, which does not necessarily yield a canonical system, has an arbitrary function in its right-hand members. The cases when the transformed equations may be made canonical by appropriate choice of this function are established. The method is illustrated by means of the Kustaanheimo-Stiefel Regularization and applied to the circular restricted three body problem.
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References
Kustaanheimo, P. and Stiefel, E.: 1965,J. Reine Angew Math. 218, 204.
Scheifele, G.: 1970,Celes. Mech. 2, 296.
Stiefel, E. and Scheifele, G.: 1971,Linear and Regular Celestial Mechanics, Berlin, Heidelberg, New York.
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Kurcheeva, I.V. Kustaanheimo-Stiefel Regularization and nonclassical canonical transformations. Celestial Mechanics 15, 353–365 (1977). https://doi.org/10.1007/BF01228427
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DOI: https://doi.org/10.1007/BF01228427