On the energy integral for first post-Newtonian approximation

dc.contributor.authorO'Leary, J.
dc.contributor.authorHill, J.M.
dc.contributor.authorBennett, J.C.
dc.date.issued2018
dc.description.abstractThe post-Newtonian approximation for general relativity is widely adopted by the geodesy and astronomy communities. It has been successfully exploited for the inclusion of relativistic effects in practically all geodetic applications and techniques such as satellite/lunar laser ranging and very long baseline interferometry. Presently, the levels of accuracy required in geodetic techniques require that reference frames, planetary and satellite orbits and signal propagation be treated within the post-Newtonian regime. For arbitrary scalar W and vector gravitational potentials Wj(j= 1 , 2 , 3) , we present a novel derivation of the energy associated with a test particle in the post-Newtonian regime. The integral so obtained appears not to have been given previously in the literature and is deduced through algebraic manipulation on seeking a Jacobi-like integral associated with the standard post-Newtonian equations of motion. The new integral is independently verified through a variational formulation using the post-Newtonian metric components and is subsequently verified by numerical integration of the post-Newtonian equations of motion.
dc.identifier.citationCelestial Mechanics and Dynamical Astronomy, 2018; 130(7, article no. 44):1-9
dc.identifier.doi10.1007/s10569-018-9839-3
dc.identifier.issn0923-2958
dc.identifier.issn1572-9478
dc.identifier.urihttps://hdl.handle.net/11541.2/132870
dc.language.isoen
dc.publisherSpringer
dc.rightsCopyright 2018 Springer
dc.source.urihttps://doi.org/10.1007/s10569-018-9839-3
dc.subjectenergy
dc.subjectgeneral relativity
dc.subjectpost-Newtonian approximation
dc.titleOn the energy integral for first post-Newtonian approximation
dc.typeJournal article
pubs.publication-statusPublished
ror.mmsid9916216511401831

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