Quasi-Keplerian motion under the generally parameterized post-Newtonian force

DOI10.1007/s10714-020-02700-3zbMath1444.83003OpenAlexW3025182889MaRDI QIDQ776772

Bo Yang, Wenbin Lin

Publication date: 13 July 2020

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10714-020-02700-3

zbMATH Keywords

post-Newtonian approximationparameterized post-Newtonian forcequasi-Keplerian motion

Mathematics Subject Classification ID

Applications of differential geometry to physics (53Z05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar dynamics (85A05) Equations of motion in general relativity and gravitational theory (83C10) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items

The quasi-Keplerian motion in regular Bardeen spacetime ⋮ Coordinates in general relativity: orbit, velocity, and time form perihelion to aphelion ⋮ The second post-Newtonian motion in Schwarzschild spacetime

Cites Work

• Motion and gravitational wave forms of eccentric compact binaries with orbital-angular-momentum-aligned spins under next-to-leading order in spin–orbit and leading order in spin(1)–spin(2) and spin-squared couplings
• The two-body problem in the (truncated) PPN ? Theory
• The confrontation between general relativity and experiment
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