EFFECTIVE POTENTIAL, HILL-TYPE STABILITY AND SUNDMAN INEQUALITY

Authors
Citation
Yc. Ge et X. Leng, EFFECTIVE POTENTIAL, HILL-TYPE STABILITY AND SUNDMAN INEQUALITY, Planetary and space science, 42(3), 1994, pp. 231-237
Citations number
27
Categorie Soggetti
Geosciences, Interdisciplinary
Journal title
ISSN journal
00320633
Volume
42
Issue
3
Year of publication
1994
Pages
231 - 237
Database
ISI
SICI code
0032-0633(1994)42:3<231:EPHSAS>2.0.ZU;2-9
Abstract
The velocity decomposition of Saari (Celest. Mech. 33, 299, 1984) is s hown to capture the best possible effective potential of the general N -body problem. This improves the effective potential inherent to Sundm an's inequality. Saari's approach is simplified by virtue of the inert ia tensor and inertia ellipsoid. The inequality stronger than Sundman' s obtained for the flat problem by Saari (Celest. Mech. 40, 197, 1987) is not only extended to the general N-body problem but is also shown to be valid under more relaxed conditions. For the spatial three-body problem, we also obtain a more explicit expression of the inequality w hich was used to plot the Hill-type surfaces by Ge and Leng (Celest. M ech. 53,233, 1992). It is proved that Hill-type stability guarantees o ne of the hierarchical stability conditions, and prevents cross-over o f orbits.