Titlebook: Ergodic Concepts in Stellar Dynamics; Proceedings of an In V. G. Gurzadyan,D. Pfenniger Conference proceedings 1994 Springer-Verlag Berlin

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lipids

Chronic

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Andrew W. Manigault,Peggy M. Zoccolaeems to be the precise definitions and hence the unique meaning of the terminology and notation often used in stellar dynamics, such as ., etc..In particular, we have seen that the term . cannot necessarily be attributed only to processes which involve exchange of energy between particles. The class

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Samuel F. Sears Jr.,Robyn L. Wallacef the main theoretical points of this research field are also briefly discussed and compared with the outcomes of recent numerical simulations..New results, obtained with a differential geometrical approach to Hamiltonian dynamics, are also presented together with a mention of their consequences for

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H. Fujii,J. Koscielniak,L. J. Berlineri.e. for galaxies of the most usual types) the systems are practically collisionless for time scales not exceeding the Hubble time. So it is necessary to follow phase trajectories not only in the 6.-D phase space but in the 6-D phase space. Studying the 6.-D space will give no new information for co

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https://doi.org/10.1007/978-90-481-2316-2systems. The system itinerates between ordered and disordered states by its deterministic dynamics. Phase space structure and existence of long-time tail reveals that the ordered state is supported by hierarchical motion around ruins of regular orbits (KAM tori and islands.

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