arXiv · 1903.03432
Post-Keplerian motion in Reissner-Nordstr\"{o}m spacetime
Abstract
We present the analytical post-Newtonian solutions for the test particle's motion in the Reissner-Nordstr\"{o}m spacetime. The solutions are formulated in the Wagoner-Will representation, the Epstein-Haugan representation, the Brumberg representation, and the Damour-Deruelle representation, respectively. The relations between the (post-)Keplerian parameters in different representations, as well as their relations to the orbital energy and angular momentum are also provided.
Explore related subjects
Keep this discovery
Bo Yang, Wenbin Lin. 2019-02-27. Post-Keplerian motion in Reissner-Nordstr\"{o}m spacetime. https://arxiv.org/abs/1903.03432
Cite the original work for its findings. Save a collection to share your selection of sources.