The second post-Newtonian order generalized Kepler equation

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dc.creatorGergely, László Á.
dc.creatorKeresztes, Zoltán
dc.creatorMikóczi, Balázs
dc.date2006-12-13
dc.date.accessioned2026-07-07T13:15:07Z
dc.date.available2026-07-07T13:15:07Z
dc.descriptionThe radial component of the motion of compact binary systems composed of neutron stars and/or black holes on eccentric orbit is integrated. We consider all type of perturbations that emerge up to second post-Newtonian order. These perturbations are either of relativistic origin or are related to the spin, mass quadrupole and magnetic dipole moments of the binary components. We derive a generalized Kepler equation and investigate its domain of validity, in which it properly describes the radial motion.
dc.descriptionto appear in the Proceedings of the Eleventh Marcel Grossmann Meeting 2006, World Scientific, Singapore (2007)
dc.identifierhttps://arxiv.org/abs/gr-qc/0612086
dc.identifierhttp://arxiv.org/abs/gr-qc/0612086
dc.identifierProceedings of the Eleventh Marcel Grossmann Meeting 2006, Eds. H Kleinert, RT Jantzen and R Ruffini, World Scientific, Singapore, p. 2503-2505 (2008)
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/230386
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleThe second post-Newtonian order generalized Kepler equation
dc.typetext

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