The binary black-hole dynamics at the third post-Newtonian order in the orbital motion

Details The binary black-hole dynamics at the third post-Newtonian order in the orbital motion The binary black-hole dynamics at the third post-Newtonian order in the orbital motion

2000-03-14

arxiv.org/abs/gr-qc/0003054v1

AnnalenPhys.9:378-383,2000

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Will appear in: Proceedings of the International European Conference on Gravitation "Journ\'ees Relativistes 99", September 12

Scientific paper

10.1002/(SICI)1521-3889(200005)9

The orbital dynamics of the binary point-mass systems is ambiguous at the third post-Newtonian order of approximation. The static ambiguity is known to be related to the difference between the Brill-Lindquist solution and the Misner-Lindquist solution of the time-symmetric conformally flat initial value problem for binary black holes. The kinetic ambiguity is noticed to violate in general the standard relation between the center-of-mass velocity and the total linear momentum as demanded by global Lorentz invariance.

Affiliated with

Also associated with

No associations

Rating

The binary black-hole dynamics at the third post-Newtonian order in the orbital motion 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 binary black-hole dynamics at the third post-Newtonian order in the orbital motion, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The binary black-hole dynamics at the third post-Newtonian order in the orbital motion will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-459738