For the Euclidean quartic scalar field theory, expansion of gives the momentum-space rules
At one loop, the four-point one-particle-irreducible correlation function receives the three bubble diagrams in the , , and channels. If is the momentum through one channel, its contribution is
Using a Feynman parameter, shifting the loop momentum, and writing gives, up to terms caused by shifting the boundary of a hard cutoff,
Thus every channel has the logarithmic ultraviolet divergence
The complete one-loop vertex is
Let denote the bracket evaluated at the chosen on-shell kinematic point. The on-shell renormalization scheme requires , hence the perturbative solution is
The cutoff dependence of is the coupling counterterm needed to hold the measured coupling fixed.
After integration by parts, the quadratic ghost operator is . Matching its propagator to the scalar propagator after requires
Differentiating with respect to its two identical scalar fields gives the ghost-scalar vertex . Matching it to the four-scalar vertex therefore requires
The additional rules are an oriented ghost propagator , a two-scalar two-ghost vertex , and a minus sign for every closed loop of Grassmann-valued fields.
Besides the scalar bubbles from part a, each channel now has a closed heavy-ghost bubble. Its two directed internal lines cannot be interchanged, so it has no scalar bubble's factor . Consequently
If denotes the corresponding sum of heavy integrals, on-shell matching gives
The root continuously connected to is the perturbative, small positive root.
After and have been matched to the same measured coupling, the nonanalytic low-energy dependence from the light scalar loops is identical. For , a heavy loop has the local expansion
Its constant term is already absorbed into the matched quartic coupling, while the remaining terms are higher-dimensional local interactions suppressed by powers of . Dependence on the finite ultraviolet cutoff is similarly suppressed by powers of . This is heavy-field decoupling: low-energy scattering agrees up to corrections after all relevant parameters are matched. At energies comparable to , the two theories differ sharply because the second theory contains wrong-statistics heavy states.

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