Effect of Perturbations in Coriolis and Centrifugal Forces on the Non-Linear Stability of <i>L</i><sub>4</sub>in the Photogravitational Restricted Three Body Problem
Effect of Perturbations in Coriolis and Centrifugal Forces on the Non-Linear Stability of <i>L</i><sub>4</sub>in the Photogravitational Restricted Three Body Problem作者机构：Department of P. G. Department of Mathematics V.K.S. University Ara India Department of Department of Mathematics S.B. College Ara India Department of Mathematics Sri Aurobindo College University of Delhi Delhi India
出 版 物：《International Journal of Astronomy and Astrophysics》 (天文学与天体物理学国际期刊（英文）)
年 卷 期：2015年第5卷第4期
页 面：275-290页
学科分类：07[理学] 0701[理学-数学] 070101[理学-基础数学]
主 题：Restricted Three Body Problem Axis Symmetric Bodies Non-Linear Stability Libration Point L4 Double D’Alembert’s Series Method
摘 要：Effect of perturbations in Coriolis and centrifugal forces on the non-linear stability of the libration point L4 in the restricted three body problem is studied when both the primaries are axis symmetric bodies (triaxial rigid bodies) and the bigger primary is a source of radiation. Moser’s conditions are utilized in this study by employing the iterative scheme of Henrard for transforming the Hamiltonian to the Birkhoff’s normal form with the help of double D’Alembert’s series. It is found that L4 is stable for all mass ratios in the range of linear stability except for the three mass ratios μc1, μc2 and μc3, which depend upon the perturbations ε1 and ε1 in the Coriolis and centrifugal forces respectively and the parameters A1,A2,A3 and A4 which depend upon the semi-axes a1,b1,c1;a2,b2,c2 of the triaxial rigid bodies and p, the radiation parameter.
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