On-shell superamplitudes in N<4 SYM
Henriette Elvang, Yu-tin Huang, Cheng Peng
TL;DR
Elvang, Huang, and Peng develop an on-shell superspace approach for pure ${\cal N}<4$ SYM using two CPT-conjugate superfields to capture the full spectrum; tree-level MHV and NMHV amplitudes are obtained by truncation from ${\cal N}=4$ and the ${\Phi}$-${\Psi}$ formalisms. They analyze the large-$z$ behavior of super-BCFW shifts, identifying a 'bad' shift that contributes to 1-loop bubble terms in ${\cal N}=0,1,2$ and derive bubble coefficients in a manifestly supersymmetric way, showing their sum for 4-point amplitudes equals $-\beta_0\, {\cal A}_{4}^{\text{tree}}$ with the standard 1-loop beta-function coefficient. The paper further solves SUSY Ward identities in ${\cal N}<4$ YM, and establishes a precise 4d–6d correspondence that relates 4d ${\cal N}^K\text{MHV}$ sectors to 6d structures, including dimensional reductions to ${\cal N}=(1,0)$ leading to ${\cal N}=2$ in 4d. Extensions to ${\cal N}<8$ supergravity are outlined, highlighting broad applicability of on-shell methods to lower-supersymmetry theories and higher-dimensional relations.
Abstract
We present an on-shell formalism for superamplitudes of pure N<4 super Yang-Mills theory. Two superfields, Phi and Phi^+, are required to describe the two CPT conjugate supermultiplets. Simple truncation prescriptions allow us to derive explicit tree-level MHV and NMHV superamplitudes with N-fold SUSY. Any N=0,1,2 tree superamplitudes have large-z falloffs under super-BCFW shifts, except under [Phi,Phi^+>-shifts. We show that this `bad' shift is responsible for the bubble contributions to 1-loop amplitudes in N=0,1,2 SYM. We evaluate the MHV bubble coefficients in a manifestly supersymmetric form and demonstrate for the case of four external particles that the sum of bubble coefficients is equal to minus the tree superamplitude times the 1-loop beta-function coefficient. The connection to the beta-function is expected since only bubble integrals capture UV divergences; we discuss briefly how the minus sign arises from UV and IR divergences in dimensional regularization. Other applications of the on-shell formalism include a solution to the N^{K}MHV N=1 SUSY Ward identities and a clear description of the connection between 6d superamplitudes and the 4d ones for both N=4 and N=2 SYM. We outline extensions to N<8 supergravity.
