Retain the homogeneous lapse function , and define the physical Hubble parameter . At first order the scalar metric perturbations give , , and . Applying the passive coordinate displacement component by component gives the scalar gauge transformations with a background lapseFor example the transformation is . The spatial isotropic part acquires , explaining the positive sign in the transformation of .
Preserving synchronous gauge requires both transformed and to remain zero. The first condition is , and the second is . Integrating them givesThus fixing the lapse function and shift vector perturbations does not exhaust the scalar coordinate freedom. The functions describe residual synchronous-gauge freedom; an integration-origin change in the integral is absorbed into .
To move from synchronous gauge to Newtonian gauge, choose to set . Requiring then givesA scalar energy density transforms as . Dividing by the background energy density, which changes the contrast only at second order if perturbed in that denominator, yields the synchronous-to-Newtonian density transformation with a lapseThe last form uses background stress-energy conservation, . With cosmic time this is ; with conformal time it is , where . Keeping these clock conventions distinct is essential to the factors of .
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