Relativistic orbits with gravitomagnetic corrections

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dc.creatorCapozziello, S.
dc.creatorDe Laurentis, M.
dc.creatorGarufi, F.
dc.creatorMilano, L.
dc.date2008-12-20
dc.date.accessioned2026-07-07T12:51:28Z
dc.date.available2026-07-07T12:51:28Z
dc.descriptionCorrections to the relativistic orbits are studied considering higher order approximations induced by gravitomagnetic effects. We discuss in details how such corrections come out taking into account magnetic components in the weak field limit of gravitational field and then the theory of orbits is developed starting from the Newtonian one, the lowest order in the approximation. Finally, the orbital structure and the stability conditions are discussed giving numerical examples. Beside the standard periastron corrections of General Relativity, a new nutation effect is due to the c^{-3} corrections. The transition to a chaotic behavior strictly depends on the initial conditions. The orbital phase space portrait is discussed.
dc.description16 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/0812.4063
dc.identifierhttp://arxiv.org/abs/0812.4063
dc.identifierPhys.Scripta 79:025901,2009
dc.identifierdoi:10.1088/0031-8949/79/02/025901
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/222998
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics of Galaxies
dc.titleRelativistic orbits with gravitomagnetic corrections
dc.typetext

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