Assume the test body moves slowly, , and that the field is quasistatic, so time derivatives are of higher order. The spatial geodesic equation, parametrized by coordinate time, then reduces at leading order to
Defining the Newtonian potential by
gives
the Newtonian equation of motion. Terms involving , spatial velocity, or time derivatives enter beyond the stated order.
The nonrelativistic fluid assumptions give
Assume again a stationary field and asymptotic flatness. The harmonic-gauge Linearized Einstein equations become
while the other trace-reversed components are smaller. Trace reversal then gives to leading order, so
Using yields
in units , which is the Poisson equation of Newtonian gravity.

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