Relativistic orbital perturbations in a weak gravitational field

With the general third-order equations of motion for a test particle, Synge's third-order orbital equations at great distance in the weak gravitational field generated by a massive body are derived. The body has an axis of symmetry around which is rotating steadily. The results found for the ad...

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Veröffentlicht in:	Int. J. Theor. Phys.; (United States) 1986-02, Vol.25 (2), p.175-193
Hauptverfasser:	GAMBI, J. M, SAN MIGUEL, A
Format:	Artikel
Sprache:	eng
Schlagworte:	640106 - Astrophysics & Cosmology- Cosmology ANGULAR MOMENTUM OPERATORS AXIAL SYMMETRY CARTESIAN COORDINATES CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS Classical general relativity COORDINATES COSMOLOGICAL MODELS DIFFERENTIAL EQUATIONS EQUATIONS EQUATIONS OF MOTION Exact sciences and technology FIELD THEORIES GAUGE INVARIANCE General relativity and gravitation GENERAL RELATIVITY THEORY GRAVITATIONAL FIELDS INVARIANCE PRINCIPLES MATHEMATICAL MODELS MATHEMATICAL OPERATORS ORBITS PARTIAL DIFFERENTIAL EQUATIONS PARTICLE MODELS PERTURBATION THEORY Physics QUANTUM OPERATORS SPACE-TIME SYMMETRY
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