The 2PN motion of a non-spinning compact binary: the Wagoner-Will-Epstein-Haugan representation

DOI10.1134/S0202289321030075zbMath1480.85002OpenAlexW3200570740MaRDI QIDQ2054922

Yanyan Li

Publication date: 3 December 2021

Published in: Gravitation \& Cosmology (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1134/s0202289321030075

zbMATH Keywords

quasi-Keplerian motion

Mathematics Subject Classification ID

Two-body problems (70F05) Galactic and stellar dynamics (85A05) Orbital mechanics (70M20)

Related Items (1)

Coordinates in general relativity: orbit, velocity, and time form perihelion to aphelion

Cites Work

• Interacting holographic dark energy, the present accelerated expansion and black holes
• Relativistic Celestial Mechanics of the Solar System
• The two-body problem in the (truncated) PPN ? Theory
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