Let be the uniform background dust surface density of a disk and its fractional perturbation. Here is the radial wavenumber, is the epicyclic frequency and is a real velocity amplitude. For that uniform background and late velocity , linear dust continuity equation gives . Integrating yields the displayed formula. The coherent travelling-wave fractional excess is , with validity requiring this number much smaller than one. The static term records initial density and transient displacement: drag damps velocity, but supplies no density diffusion. The long-wavelength gas wave has the same fractional density amplitude, so entrainment alone does not produce an additional dust-to-gas ratio enhancement at this order.

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