The gauge-invariant functional integral counts every gauge orbit repeatedly. Insert a gauge-orbit identity
Dividing by the gauge-group volume and averaging with a Gaussian weight produces the term . The determinant is represented by a pair of independent anticommuting scalar fields , giving the prescribed ghost density , where . The Grassmann integral gives a determinant rather than the inverse determinant of a commuting Gaussian integral; field-independent constants and overall determinant signs are absorbed in normalization.
Although the gauge group is Abelian, the determinant here is field dependent because the gauge condition contains the scalar fluctuation . Thus Abelian ghosts need not decouple in a broken-phase gauge. The fields implement gauge-orbit counting and are not physical external particles.
For the ghost coupling in a linear Cartesian Abelian Higgs gauge, the common factor in the scalar parametrization cancels from the gauge transformation. Separating real and imaginary parts gives
Consequently
For the variables and gauge function actually printed, the ghost mass and Higgs-ghost vertex are therefore
For the usual nonnegative gauge parameter, . The momentum-space ghost propagator is in this kinetic convention. There is no direct ghost-photon vertex or ghost- vertex. At the ghost becomes massless and decouples.
The scalar prefactor is incompatible with the stated canonical broken-vacuum interpretation. At it gives , whereas the potential is minimized at . In fact the printed parametrization gives
Its kinetic terms have coefficient , not , and its vector mass parameter is . The given gauge function consequently does not cancel the vector-scalar mixing in those literal variables. The ghost operator computed above nevertheless follows algebraically from that gauge function without changing the printed fields.
With a canonical Abelian Higgs shift , the expansion is about a true minimum, the vector mass is , the gauge fixing cancels the mixing, and the same ghost formulas acquire the usual interpretation . For the literal parametrization, a canonical fluctuation is , so its ghost vertex would instead be ; the non-vacuum background problem still remains. These two interpretations must not be silently mixed.

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