Normalization of Hamiltonian in the Generalized Photogravitaional Restricted Three Body Problem with Poynting-Robertson Drag

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dc.creatorKushvah, B. S.
dc.creatorSharma, J. P.
dc.creatorIshwar, B.
dc.date2006-05-18
dc.date.accessioned2026-07-07T08:32:26Z
dc.date.available2026-07-07T08:32:26Z
dc.descriptionWe 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. Wittaker method is used to transform the second order part of the Hamiltonian into the normal form. Keywords:Normalization / Generalised Photogravitational/ RTBP/P-R Drag.
dc.descriptionLaTeX2e, 9 pages
dc.identifierhttps://arxiv.org/abs/math/0605505
dc.identifierhttp://arxiv.org/abs/math/0605505
dc.identifier2007EM&P..tmp...24K
dc.identifierdoi:10.1007/s11038-007-9149-3
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/138793
dc.subjectDynamical Systems
dc.subject70F15
dc.titleNormalization of Hamiltonian in the Generalized Photogravitaional Restricted Three Body Problem with Poynting-Robertson Drag
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