Solutions of the special relativistic Kepler problem with fixed energy are reparameterized as solutions to a generalized Kepler equation with a 1/r² potential term, yielding dynamics equivalent to Levi-Civita corrections up to coefficients.
Giuseppe Peano
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Reparametrizing the relativistic Kepler equation: a bridge to Levi-Civita-type models
Solutions of the special relativistic Kepler problem with fixed energy are reparameterized as solutions to a generalized Kepler equation with a 1/r² potential term, yielding dynamics equivalent to Levi-Civita corrections up to coefficients.