A practical map from massless to massive particle amplitudes, applied to SMEFT
This paper builds a direct bridge between the simple scattering formulas you write in a theory where particles are massless and the more complicated formulas that appear after a symmetry is broken and some particles become massive. In plain terms, the authors give a systematic recipe for turning contact interactions in an unbroken (massless) theory into the corresponding contact interactions in the broken (massive) theory. They then use that recipe to relate coefficients in the Standard Model Effective Field Theory (SMEFT) before and after electroweak symmetry breaking.
The authors organize massive amplitudes using a basis called spin-transversality (ST). Roughly, this basis isolates the part of a massive particle’s amplitude that behaves like a transverse spin state and is therefore easier to compare with massless formulas. They expand amplitudes at high energy using minimal-helicity-chirality (MHC) components, which pick out the simplest spin-and-handedness combinations that survive as the energy grows. A neat technical step is to describe a massive particle with a U(2)=SU(2)×U(1)_t label so that a standard method for constructing massless Lorentz structures (the semi-standard Young-tableau) can be applied directly to the massive case.
Matching proceeds in two ways. When the leading MHC component of a massive amplitude has a smooth massless contact limit, it matches one-to-one with the corresponding ultraviolet (UV) massless amplitude. When there is no such direct limit, the authors identify five exceptional classes of ST amplitudes. In those cases they match the first nonzero descendant components to the massless contact amplitudes via conserved current couplings — that is, by using the symmetry-related currents that couple to the fields and enforce conservation laws.
As an explicit application, the paper works out the one-flavor electroweak sector of the SMEFT through dimension eight. Concretely, the authors provide formulas relating unbroken-phase Wilson coefficients — the numbers that weight effective interactions in the high-energy, massless description — to coefficients in the broken-phase ST amplitude basis for scattering processes with three to eight external particles. This gives a practical way to translate between the UV operator language and the massive-amplitude language used to describe low-energy experiments.