The Hamiltonian dynamics of the two gyrostats problem

被引:14
作者
Mondejar, F [1 ]
Vigueras, A [1 ]
机构
[1] Univ Murcia, Dept Matemat Aplicada, ETSII, Murcia 30203, Spain
关键词
Force Field; Explicit Form; Reduction Process; Order Approximation; Poisson Bracket;
D O I
10.1023/A:1008375820146
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The problem of two gyrostats in a central force field is considered. We prove that the Newton-Euler equations of motion are Hamiltonian with respect to a certain non-canonical structure. The system posseses symmetries. Using them we perform the reduction of the number of degrees of freedom. We show that at every stage of the reduction process, equations of motion are Hamiltonian and give explicit forms corresponding to non-canonical Poisson brackets. Finally, we study the case where one of the gyrostats has null gyrostatic momentum and we study the zero and the second order approximation, showing that all equilibria are unstable in the zero order approximation.
引用
收藏
页码:303 / 312
页数:10
相关论文
共 7 条
[1]  
ABOELNAGA MZ, 1979, ASTRON ZH+, V56, P881
[2]  
Barkin Yu. V., 1980, Pis'ma v Astronomicheskie Zhurnal, V6, P377
[3]  
CID R, 1985, CELESTIAL MECH, V36, P135
[4]  
Duboshin G.N., 1976, CELESTIAL MECH, V14, P239
[5]   Reduction, relative equilibria and potential in the two rigid bodies problem [J].
Maciejewski, AJ .
CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY, 1995, 63 (01) :1-28
[6]  
WANG L, 1995, IEEE T AUTOMATIC CON, V10, P1732
[7]  
Wang Li.-S., 1991, CELESTIAL MECH, V50, P349