Work consistently to first order in the metric perturbation, with of the same small order. Under the passive change ,
Applying this to the full metric tensor and writing with the same fixed numerical Minkowski metric gives
Indices on are lowered with . This is the gauge transformation of the perturbation relative to a fixed background. If the background were transformed as a tensor as well, the difference of those two fully transformed metrics would instead obey the homogeneous tensor transformation law. The inhomogeneous terms arise from retaining the fixed-background identification used in linearized gravity.
The trace changes by , so the trace-reversed metric perturbation changes as
Let . Commuting partial derivatives gives
Thus choose a solution of the inhomogeneous wave equation
Such a solution exists locally with suitable initial data, and can be selected with appropriate wave-equation boundary conditions. This imposes the Lorenz gauge in linearized gravity, . All the divergence terms in the supplied vacuum equation then vanish, leaving
The remaining freedom is the residual gauge symmetry of linearized gravity.
Using the old coordinates in these derivatives is consistent at the retained order. Indeed
Acting on a first-order perturbation, the correction is a product of two first-order quantities and is discarded. Similarly replacing the argument by changes by under the same perturbative ordering. This does not assert an exact equality of the two coordinate differential operators; it is the linear approximation about the fixed flat background.

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