Summary
The problem of two bodies with a central-force potential is treated by means of a relativistic Hamiltonian multi-time formalism. It is shown that only a Newtonian potential is compatible within this formalism, thus stating an exception of the so-called no-interaction theorems. The relativistic meaning of the Runge-Lenz vector of the classical Kepler problem is revealed.
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References
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Stickforth, J. The Kepler problem in relativistic multi-time formalism. Part I. Acta Mechanica 123, 187–193 (1997). https://doi.org/10.1007/BF01178409
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DOI: https://doi.org/10.1007/BF01178409