Higher-spin massless S-matrices in four-dimensions
David A. McGady, Laurentiu Rodina
TL;DR
This work uses on-shell, four-dimensional spinor-helicity methods to classify all massless three-point amplitudes and then tests four-point amplitudes via locality and unitarity (pole-counting). The authors show that, except for a small set of theories (phi^3, Yang–Mills, and General Relativity/Supergravity), higher-spin massless interactions cannot be consistently constructed, and no massless state with helicity >2 can couple to gravitons. Supersymmetry emerges naturally as a consistency requirement when spin-3/2 states are included, tying gravitino interactions to gravity and limiting the amount of SUSY to at most ${\cal N}=8$. The results reinforce the uniqueness of GR and YM in the massless sector and illustrate how on-shell constraints encode deep structure like the equivalence principle and SUSY, without relying on off-shell Lagrangians.
Abstract
On-shell, analytic S-matrix elements in massless theories are constructed from a finite set of primitive three-point amplitudes, which are fixed by Poincare invariance up to an overall numerical constant. We classify \emph{all} such three-point amplitudes in four-dimensions. Imposing the simplest incarnation of Locality and Unitarity on four-particle amplitudes constructed from these three-particle amplitudes rules out all but an extremely small subset of interactions among higher-spin massless states. Notably, the equivalence principle, and the Weinberg-Witten theorem, are simple corollaries of this principle. Further, no massless states with helicity larger than two may consistently interact with massless gravitons. Chromodynamics, electrodynamics, Yukawa and $φ^3$-theories are the only marginal and relevant interactions between massless states. Finally, we show that supersymmetry naturally emerges as a consistency condition on four-particle amplitudes involving spin-3/2 states, which must always interact gravitationally.
