For a perturbation , with all other components zero, the linearized Vacuum Einstein equations give . Put and choose , , , . Under the linearized coordinate gauge transformation, the mixed time/transverse and longitudinal/transverse components cancel, while the other time/longitudinal changes are proportional to . The remaining components are , , , a transverse-traceless gauge perturbation of plus polarization. This explicitly removes a nonzero affine trace without assuming it vanishes by boundary conditions. If too, all linearized curvature vanishes.

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