On the energy in relativistic stellar dynamics

Details On the energy in relativistic stellar dynamics On the energy in relativistic stellar dynamics

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977gregr...8..491s&link_type=abstract

General Relativity and Gravitation, vol. 8, July 1977, p. 491-495.

Physics

10

Celestial Mechanics, Many Body Problem, Relativity, Virial Theorem, Angular Momentum, Energy Methods, Ideal Fluids, Orbital Velocity, Tensors

Scientific paper

Previously derived tensor-virial equations for post-Newtonian relativistic stellar dynamics are used to evaluate, in the post-Newtonian approximation, the energy integral for a bounded system of extended bodies with arbitrary internal structure and internal motions. The energy integral for a bounded perfect-fluid source is employed in the evalution, and an expression is obtained for the energy under secularly stationary conditions. A very simple expression for the total system energy is derived which contains only simple powers of the orbital velocities of the bodies and of their external gravitational potentials.

Affiliated with

Also associated with

No associations

Rating

On the energy in relativistic stellar dynamics 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 On the energy in relativistic stellar dynamics, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the energy in relativistic stellar dynamics will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1560502