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- W3104378854 abstract "The aim of the present work is to reduce the secular solution around the triangular equilibrium points to periodic solution in the frame work of the generalized restricted thee-body problem. This model is generalized in sense that both the primaries are oblate and radiating as well as the gravitational potential from a belt. We show that the linearized equation of motion of the infinitesimal body around the triangular equilibrium points has a secular solution when the value of mass ratio equals the critical mass value. Moreover, we reduce this solution to periodic solution, as well as some numerical and graphical investigations for the effects of the perturbed forces are introduced. This model can be used to examine the existence of a dust particle near the triangular points of an oblate and radiating binary stars system surrounded by a belt." @default.
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- W3104378854 date "2013-12-28" @default.
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- W3104378854 title "Reduction the secular solution to periodic solution in the generalized restricted three-body problem" @default.
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- W3104378854 doi "https://doi.org/10.1007/s10509-013-1756-z" @default.
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