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 toDefining the Newtonian potential bygivesthe Newtonian equation of motion. Terms involving , spatial velocity, or time derivatives enter beyond the stated order.
The nonrelativistic fluid assumptions giveAssume again a stationary field and asymptotic flatness. The harmonic-gauge Linearized Einstein equations becomewhile the other trace-reversed components are smaller. Trace reversal then gives to leading order, soUsing yieldsin units , which is the Poisson equation of Newtonian gravity.
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