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Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
Helically symmetric N-particle solutions in scalar gravity
Robert Beig1, J Mark Heinzle, Bernd G Schmidt
1Gravitational Physics, Faculty of Physics, University of Vienna, A-1090 Vienna, Austria. Robert.Beig@univie.ac.at
Abstract:
Within a scalar model theory of gravity, where the interaction between particles is given by the half-retarded plus half-advanced solution of the scalar wave equation, we consider an N-body problem: We investigate configurations of N particles which form an equilateral N angle and are in helical motion about their common center. We prove that there exists a unique equilibrium configuration and compute the equilibrium radius explicitly in a post-Newtonian expansion.
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