Translational and rotational motion of a test rigid body in relativistic celestial mechanics

Details Translational and rotational motion of a test rigid body in relativistic celestial mechanics Translational and rotational motion of a test rigid body in relativistic celestial mechanics

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kfnt....3...18v&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 3, Sept.-Oct. 1987, p. 18-24. In Russian.

Statistics

Computation

Celestial Mechanics, Equations Of Motion, Relativistic Theory, Rotating Bodies, Translational Motion, Computational Astrophysics, Equivalence, Series Expansion

Scientific paper

Equations of translational and rotational motion of a test rigid body are obtained in terms of variables closely related to observable quantities. These equations are derived using two different methods. The first one is based on the equivalence principle and the equation of the second geodesic deviation, while the second involves a multipole formalism expansion.

Affiliated with

Also associated with

No associations

Rating

Translational and rotational motion of a test rigid body in relativistic celestial mechanics 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 Translational and rotational motion of a test rigid body in relativistic celestial mechanics, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Translational and rotational motion of a test rigid body in relativistic celestial mechanics will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1776007