Keep the mostly-plus Minkowski metric and the Fourier transform . Write , with . To fix the otherwise unspecified phase of and the Dirac adjoint, take
where are ordinary mostly-minus gamma matrices. Then , , and the fermionic time-derivative term is . In these conventions the interaction with real is Hermitian: in mostly-minus notation it is . If one instead calls the square-one chirality matrix, its coefficient must be to represent the same interaction. These phase choices leave physical relativistic scattering cross-sections unchanged.
Expanding yields the following Feynman rules with relativistically normalized external states:
Strip the overall four-momentum conservation delta function when defining the scattering amplitude. There are no further bare interaction vertices, no gauge fixing and no Faddeev-Popov ghost fields in this theory. Renormalized higher-order calculations add the required counterterms; these are additional to the rules of the displayed classical Lagrangian density.
The Dirac field has the global symmetry , , while the real scalar is unchanged. Both the free Dirac action and the pseudoscalar Yukawa interaction preserve this symmetry. Therefore Dirac fermion number conservation holds: its charge counts particles minus antiparticles.
The initial state has charge , whereas a final antiparticle and a neutral scalar have charge . Since the S-matrix commutes with that charge,
This holds at every order, not just tree level. In the Feynman rules, a continuous fermion arrow cannot connect these specified external states. Replacing only the outgoing by a in the previous expression would not give a physical amplitude. Changing both external fermions to antiparticles would instead produce an allowed process with reversed fermion flow and the appropriate spinors; moving a leg between initial and final states is a different operation governed by crossing symmetry.