A modified general-relativity metric with a density-dependent medium term is used to derive an extra Mercury perihelion precession, but the derivation contains critical errors and the density is obtained by fitting the observed residual.
Dynamical friction: I
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Nonlinear Dissipative Forces in Celestial Motion Using the Method of Multiple Scales
A modified general-relativity metric with a density-dependent medium term is used to derive an extra Mercury perihelion precession, but the derivation contains critical errors and the density is obtained by fitting the observed residual.