Higher Order Normalizations in the Generalized Photogravitational Restricted Three Body Problem with Poynting-Robertson Drag

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dc.creatorKushvah, B. S.
dc.creatorSharma, J. P.
dc.creatorIshwar, B.
dc.date2007-09-29
dc.date.accessioned2026-07-07T08:39:23Z
dc.date.available2026-07-07T08:39:23Z
dc.descriptionHigher order normalizations are performed in the generalized photogravitational restricted three body problem with Poynting-Robertson drag. In this problem we have taken bigger primary as a source of radiation and smaller primary as an oblate spheroid. Whittaker method is used to transform the second order part of the Hamiltonian into the normal form. We have also performed Birkhoff's normalization of the Hamiltonian. For this we have tilized Henrard's method and expanded the coordinates of the infinitesimal body in double D'Alembert series. We have found the values of first and second order components. They are affected by radiation pressure, oblateness and P-R drag. Finally we obtained the third order part of the Hamiltonian zero. Keywords:Higher Order Normalization, Generalized Photogravitational, RTBP,P-R drag
dc.descriptionLatex2e paper,. BASI, 2007(Accepted)
dc.identifierhttps://arxiv.org/abs/0710.0061
dc.identifierhttp://arxiv.org/abs/0710.0061
dc.identifierBull.Astr.Soc.,India, 35,319-338(2007)
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/141052
dc.subjectDynamical Systems
dc.subject70F07;70F15
dc.titleHigher Order Normalizations in the Generalized Photogravitational Restricted Three Body Problem with Poynting-Robertson Drag
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