Normalization of Hamiltonian in the Generalized Photogravitational Restricted Three Body Problem with Poynting—Robertson Drag


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Abstract

We have performed normalization of Hamiltonian in the generalized photogravitational restricted three body problem with Poynting—Robertson drag. In this problem we have taken bigger primary as source of radiation and smaller primary as an oblate spheroid. Whittaker's method is used to transform the second order part of the Hamiltonian into the normal form.

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