The stationary n-body problem in general relativity
Robert Beig

TL;DR
This paper discusses the non-existence of certain stationary multi-body solutions in general relativity and compares these results with the Newtonian case, highlighting fundamental differences.
Contribution
It proves the non-existence of specific asymptotically flat, stationary solutions with multiple bodies in general relativity, extending previous results and providing detailed Newtonian analogs.
Findings
No such multi-body stationary solutions exist in general relativity under specified conditions.
The Newtonian case admits different solution structures, contrasting with the relativistic results.
The work clarifies the constraints imposed by spacetime symmetries on multi-body configurations.
Abstract
In this talk I describe recent joint works with R.Schoen and with G.Gibbons and R.Schoen which prove the non-existence of certain asymptotically flat, stationary solutions of the Einstein equations with more than one body. The basic restriction is for example satisfied when spacetime has an isometry reversing the sign of the timelike Killing vector and fixing a hypersurface in the space of Killing trajectories which is disjoint from the bodies. I also give a detailed treatment of the Newtonian situation.
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Taxonomy
TopicsCosmology and Gravitation Theories · Spacecraft Dynamics and Control · Astro and Planetary Science
