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作 者:Jagadish Singh Omale Solomon Okpanachi
机构地区:[1]Department of Mathematics,Faculty of Physical Sciences,Ahmadu Bello University,Zaria,Nigeria [2]Department of Engineering and Space Systems,National Space Research and Development Agency(NASRDA),Obasanjo Space Centre,Abuja,Nigeria
出 处:《Applied Mathematics(A Journal of Chinese Universities)》2023年第1期44-57,共14页高校应用数学学报(英文版)(B辑)
摘 要:The motion of a test particle within the context of the restricted four-body problem(R4BP)driven by a new kind of potential,called the generalized Manev potential,with perturbations in the Coriolis and centrifugal forces is considered in this study.The system possesses eight libration points which were distributed on its plane of motion in different manner from those of the usual Newtonian potential.Unlike the case of the perturbed R4BP under Newtonian potential,where two of these librations are stable,all of them are unstable in linear sense under Manev potential.We found that a gradual perturbation in the centrifugal force causes the trajectories of motion to drift inward but the Coriolis force was proven to have no effect on the location of the libration points of the system.Using first order Lyapunov characteristic exponents,the dynamical behavior of the system is found irregular.We experimented with a high velocity stellar system(82 G.Eridani)to establish the applicability of the model in astrophysics.
关 键 词:generalized Manev potential Coriolis force centrifugal force stability CHAOTIC 82 G.Eridani
分 类 号:O314[理学—一般力学与力学基础]
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