On the collinear point L3 in the generalized relativistic R3BP
. The photogravitational oblate restricted three-body problem is carried out within the post-Newtonian framework. The primaries are assumed to be oblate as well as radiant sources. The perturbed location of the collinear point is computed. A series form of location is obtained as a new analytical re...
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Veröffentlicht in: | European physical journal plus 2015-11, Vol.130 (11), p.234, Article 234 |
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Hauptverfasser: | , |
Format: | Artikel |
Sprache: | eng |
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Online-Zugang: | Volltext |
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Zusammenfassung: | .
The photogravitational oblate restricted three-body problem is carried out within the post-Newtonian framework. The primaries are assumed to be oblate as well as radiant sources. The perturbed location of the collinear point
is computed. A series form of
location is obtained as a new analytical results. In order to introduce a semi-analytical view, a Mathematica program is constructed so as to draw the locations of collinear point
versus
the mass ratio
taking into account one or more of the considered perturbations. All the obtained figures are analyzed. |
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ISSN: | 2190-5444 2190-5444 |
DOI: | 10.1140/epjp/i2015-15234-x |