The Kepler equation for inspiralling compact binaries

Details The Kepler equation for inspiralling compact binaries The Kepler equation for inspiralling compact binaries

2005-10-20

arxiv.org/abs/astro-ph/0510602v1

Phys.Rev.D72:104022,2005

Astronomy and Astrophysics

Astrophysics

Scientific paper

10.1103/PhysRevD.72.104022

Compact binaries consisting of neutron stars / black holes on eccentric orbit undergo a perturbed Keplerian motion. The perturbations are either of relativistic origin or are related to the spin, mass quadrupole and magnetic dipole moments of the binary components. The post-Newtonian motion of such systems decouples into radial and angular parts. We present here for the first time the radial motion of such a binary encoded in a generalized Kepler equation, with the inclusion of all above-mentioned contributions, up to linear order in the perturbations. Together with suitably introduced parametrizations, the radial motion is solved completely.

Affiliated with

Also associated with

No associations

Rating

The Kepler equation for inspiralling compact binaries does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Kepler equation for inspiralling compact binaries, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Kepler equation for inspiralling compact binaries will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-475398