For a point mass, , and part (b) gives
The linearized Ricci tensor and scalar obey
For a static perturbation with , this becomes
Away from the source, . For , one has , so the two supplied identities give
The vacuum trace equation therefore reduces to
whose general solution for is
The scalar equation alone leaves arbitrary. Imposing the remaining vacuum components and matching the mass fixes , as in the linearized point-mass metric in radial Cartesian form.

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