PeterDonis
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There are no exact solutions for multiple bodies, so I'm not sure what you are basing this on.H_A_Landman said:It also works with multiple bodies.
In the weak field regime for an isolated system, you can get away with this because the non-linearities in the EFE can be assumed to be negligible. But there are still limitations with this approach, and you're still doing numerical solutions since no exact solutions are known.H_A_Landman said:You just add up the Newtonian potentials for each body and plug that in.
However, this is still limited to the weak field regime and an isolated system. You can't do it in the strong field regime, e.g., for a neutron star. And you can't do it for, e.g., FRW spacetime.
Please give a reference.H_A_Landman said:You can do a whole galaxy (minus the strong-field parts) this way.
Neither one is correct; note that I didn't say "time-only term". I said ##g_{tt}##, and I explicitly noted that it is for a particular system of coordinates.H_A_Landman said:If you're more comfortable with the phrase "time-only term" than "time-curvature term", I don't have any great objection.
It implies no such thing. There are "force-like effects" in an accelerating rocket in flat spacetime, or inside a rotating chamber in flat spacetime, for that matter.H_A_Landman said:"flat" implies no force-like effects
It implies no such thing. Spacetime curvature is geodesic deviation, which can be shown entirely from the behavior of freely falling objects that feel zero force.H_A_Landman said:"curved" implies force-like effects
All this is personal theory and you are getting very close to a warning at this point.H_A_Landman said:this clearly has force-like effects (curved geodesics). The metric is not flat, but the Minkowski part is flat. So all the non-flatness comes from the time dilation.