Titlebook: Chaos in Gravitational N-Body Systems; Proceedings of a Wor J. C. Muzzio,S. Ferraz-Mello,J. Henrard Conference proceedings 1996 Kluwer Acad

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忘恩負義的人

grability (the famous Argentine beef was, certainly, also an attraction!). All the papers of the present volume were refereed. Most were accepted after some revision, while some needed no change at all (compli- ments to their authors!) and, sadly, a few could not be included. About half a dozen authors did no978-94-010-6623-5978-94-009-0307-4

出血

A Note Concerning the 2:1 and the 3:2 Resonances in the Asteroid Belt, secular resonances. This path crosses a bridge, at moderate inclination and large amplitude of libration, between the two chaotic domains associated with these resonances..The 3:2 resonance being similar in many respects to the 2:1 resonance, one may wonder whether it contains also such a path. Ind

誘騙

Geometrodynamics, Chaos and Statistical Behaviour of N-Body Systems,are unjustified. Nevertheless, we point out that the geometrical transcription of hamiltonian systems, if carefully employed, . deep informations about the degree of stochasticity in the dynamics, and very interesting insights on its sources. To overcome some of the limitations of the approach, for

高調(diào)

Geometrodynamics on Finsler Spaces,cribed by conservative potentials and 2) Bianchi IX Cosmological Model (.). This latter example is particularly enlightening, as the introduction of Finsler Geometry overcomes the critical problems which raised some criticisms against the use of the Jacobi (Riemannian) metric to study the chaotic pr

咽下

Port Cities and Global Legacies secular resonances. This path crosses a bridge, at moderate inclination and large amplitude of libration, between the two chaotic domains associated with these resonances..The 3:2 resonance being similar in many respects to the 2:1 resonance, one may wonder whether it contains also such a path. Ind

咽下

Focus-Words

Port Cities and Global Legaciescribed by conservative potentials and 2) Bianchi IX Cosmological Model (.). This latter example is particularly enlightening, as the introduction of Finsler Geometry overcomes the critical problems which raised some criticisms against the use of the Jacobi (Riemannian) metric to study the chaotic pr

BLANK

Spectra of Stretching Numbers and Helicity Angles in Dynamical Systems,tions from a given orbit at times . and . + 1. Similarly we define a ”helicity angle” as the angle between the deviation ξ.and a fixed direction. The distributions of the stretching numbers and helicity angles (spectra) are invariant with respect to initial conditions in a connected chaotic domain.

Ambulatory

On the Measure of the Structure Around the Last KAM Torus Before and After its Break-Up,he standard map for the analysis of the hierarchical structure existing around invariant KAM tori applying two complementary methods: the Laskar’s frequency map analysis and the sup-map analysis. We recover and extend the theoretical prediction recently given by Morbidelli and Giorgilli about the ex