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.
Physical Processes in the Interstellar Medium
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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.