Abstract
A quantitative description of Hamiltonian chaos, based on a Riemannian geometrization of Newtonian dynamics, is discussed here for a model, introduced by Contopoulos, describing the dynamics of a test star in a galactic potential. A statistical treatment of the geometry of dynamics, effective in the limit of a large number N of degrees of freedom, is here applied to the N = 3 case of the Contopoulos model, discussing how the statistical model has to be modified in order to quantitatively account for the chaoticity of the dynamics.
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Ciraolo, G., Pettini, M. (2002). Geometry of Chaos in Models of Stellar Dynamics. In: Celletti, A., Ferraz-Mello, S., Henrard, J. (eds) Modern Celestial Mechanics: From Theory to Applications. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-2304-6_11
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DOI: https://doi.org/10.1007/978-94-017-2304-6_11
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