High Order Relativistic Corrections To Keplerian Motion

Details High Order Relativistic Corrections To Keplerian Motion High Order Relativistic Corrections To Keplerian Motion

2004-04-13

arxiv.org/abs/gr-qc/0404057v1

J.Math.Phys. 42 (2001) 839-855

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

23 pages, LaTeX2e

Scientific paper

10.1063/1.1335556

The first terms of the general solution for an asymptotically flat stationary axisymmetric vacuum spacetime endowed with an equatorial symmetry plane are calculated from the corresponding Ernst potential up to seventh order in the radial pseudospherical coordinate. The metric is used to determine the influence of high order multipoles in the perihelion precession of an equatorial orbit and in the node line precession of a non-equatorial orbit with respect to a geodesic circle. Both results are written in terms of invariant quantities such as the Geroch-Hansen multipoles and the energy and angular momentum of the orbit.

Affiliated with

Also associated with

No associations

Rating

High Order Relativistic Corrections To Keplerian 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 High Order Relativistic Corrections To Keplerian Motion, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High Order Relativistic Corrections To Keplerian Motion will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-247194