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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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發(fā)表于 2025-3-21 18:05:29 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Chaos in Gravitational N-Body Systems
副標題Proceedings of a Wor
編輯J. C. Muzzio,S. Ferraz-Mello,J. Henrard
視頻videohttp://file.papertrans.cn/224/223887/223887.mp4
圖書封面Titlebook: Chaos in Gravitational N-Body Systems; Proceedings of a Wor J. C. Muzzio,S. Ferraz-Mello,J. Henrard Conference proceedings 1996 Kluwer Acad
描述The Workshop on Chaos in Gravitational N -Body Systems was held in La Plata, Argentina, from July 31 through August 3, 1995. The School of Astronomy and Geophysics of La Plata National University, best known as La Plata Observatory, was the host institution. The Observatory (cover photo) was founded in 1883, and it has nowadays about 120 faculty members and 70 non-faculty members devoted to teaching and research in different areas of astronomy and geophysics. It was very nice to see how many people, from young students to well recognized authorities in the field, came to participate in the meeting. This audience success was due to the increasing understanding of the neces- sity to gather together people from Celestial Mechanics and Stellar Dynamics to explore the problems that exist at the frontier of these two disciplines and their common interest in chaotic phenomena and integrability (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 no
出版日期Conference proceedings 1996
關(guān)鍵詞Celestial mechanics; Gravity; Inflation; Population; astronomy; cosmology; dynamics; galaxies; gravitation; m
版次1
doihttps://doi.org/10.1007/978-94-009-0307-4
isbn_softcover978-94-010-6623-5
isbn_ebook978-94-009-0307-4
copyrightKluwer Academic Publishers 1996
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發(fā)表于 2025-3-21 21:06:38 | 只看該作者
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
板凳
發(fā)表于 2025-3-22 02:56:39 | 只看該作者
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
地板
發(fā)表于 2025-3-22 04:53:53 | 只看該作者
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
5#
發(fā)表于 2025-3-22 12:45:49 | 只看該作者
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
6#
發(fā)表于 2025-3-22 15:26:41 | 只看該作者
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
7#
發(fā)表于 2025-3-22 20:24:24 | 只看該作者
8#
發(fā)表于 2025-3-22 21:42:34 | 只看該作者
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
9#
發(fā)表于 2025-3-23 04:06:50 | 只看該作者
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.
10#
發(fā)表于 2025-3-23 05:53:56 | 只看該作者
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
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