Use the source action , with independent Grassmann variables used as sources and left functional derivatives. A scalar insertion is . For the odd fields the ordered rules are
The middle sign is not arbitrary: differentiating the rightmost odd source in from the left gives . Derivative ordering must consequently match the displayed order of the fields; the rightmost derivative acts first.
Expand in its power series. Replace each field in every term by its source insertion, preserving the fermion order. These derivatives can be pulled outside the free path integral. Re-exponentiation gives the unnormalized generating functional
Summation over the spinor index is understood. Normalized correlation functions require division by the same interacting , which cancels vacuum factors; that division is separate from this operator identity.
First fix the propagator kernels in a positive-sign Gaussian generating functional. From its scalar exponent, gives the contraction . The fermionic insertion rules similarly give , writing for the kernel labelled in that exponent. Thus the kernels in the question do not already include the factors of in the actual time-ordered contractions.
At order , expand the interaction operator to its second term, or equivalently apply Wick's theorem to
For a connected contribution, the external scalar insertions attach to different interaction points. The two assignments are equal after exchanging and cancel . The connected fermionic contraction is
The minus sign is the closed fermion loop sign. The alternative pairing gives two separate fermion tadpoles and belongs to disconnected external components, not the requested connected function. A free external scalar line multiplying a vacuum graph also cancels in the normalized result.
Combining with the loop minus sign gives
There are four contractions, so replacing and introduces . Therefore
This is the fermion-loop diagram in the last panel of i. The trace contracts spinor indices around the loop; it is not an additional degeneracy factor. A convention using physical contractions directly obtains the preceding formula in with the same coefficient. Mixing one convention's Gaussian kernels with another's insertion factors would change its apparent signs.
For two distinct commuting real scalar fields in place of the labelled fermion pair, with interaction , there is no anticommutation sign on closing the loop and no spinor trace. The two propagators are simply multiplied. In terms of physical time-ordered scalar contractions , the connected contribution is
The statistics and symmetry factors of a two-propagator loop determine the replacement. Relative to the fermionic formula in ii, the loop-statistics sign reverses. Scalar source kernels normalized like the stated Gaussian give the same overall minus sign after the four contraction factors are converted. There is no spin multiplicity.
If both replacement fields instead mean the same real field , the coupling normalization and the identical-line symmetry factor must be specified. With interaction , the cubic vertex is and its two-identical-line loop carries , giving coefficient . With the literal coefficient , its vertex is and the coefficient is . These cases are distinct from two separately labelled real fields; suppressing their combinatorics would hide a factor-of-two ambiguity in the replacement.

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