Use the source term and left Grassmann functional derivatives. Differentiating its exponential inserts fields according to
The sign for follows because a left derivative with respect to must cross . Keep the order when replacing these fields. Expand in the original path integral; each field monomial can now be generated by these ordered derivatives acting on the free functional. Resumming gives
The arguments refer respectively to at . The free functional arises by performing the free Gaussian field integrals, and may be chosen so that .
No additional field-integration measure remains in this differential-operator formula. Such a measure is printed outside the operator in the source even though has already integrated out those fields. At , that literal expression would contain rather than simply , which is not the free generating functional. Also, when denotes a density, the spacetime integral in the exponent is required.
At first order the Dyson expansion inserts . Contract the scalar field at the vertex with the external scalar. The four remaining fermion fields have two admissible pairings: both external fermions attach to the vertex, or the two vertex fermions contract with each other while the external pair contracts freely. Wick's theorem gives
The minus sign in the second term is the fermion sign of the closed contraction: . The first term is connected; the second is a scalar-attached fermion tadpole multiplied by a disconnected free external fermion propagator. The full time-ordered expectation includes both topologies, whereas the connected generating functional retains only the first. There is no order- contribution in this pure Yukawa expansion because the total number of scalar fields would be odd.
For a parity-preserving free propagator, the tadpole coefficient is , whose integrand contains only and . Both vanish. Thus the second term is a legitimate formal Wick contraction but is zero with a compatible regulator; normal ordering the interaction removes it from the outset.

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