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Celestial Superamplitudes

Andreas Brandhuber, Graham R. Brown, Joshua Gowdy, Bill Spence, Gabriele Travaglini

TL;DR

The paper develops a chiral spinor-helicity framework and a corresponding chiral Mellin transform to define celestial amplitudes with an explicit spin constraint $h-ar{h}=J$. Focusing on $ abla N=4$ SYM, it constructs a consistent on-shell celestial superspace and derives celestial superamplitudes, along with the full celestial superconformal algebra, showing these generators annihilate tree-level amplitudes. It provides concrete three-, four-, and five-point MHV celestial superamplitudes and outlines the general $n$-point structure, with explicit weight assignments for all celestial operators. The approach clarifies how Lorentz and superconformal symmetries act on celestial data, offering a streamlined path toward a 2D celestial SCFT interpretation and promising extensions to gravity, less-supersymmetric theories, and loop-level celestial amplitudes.

Abstract

We study celestial amplitudes in (super) Yang-Mills theory using a parameterisation of the spinor helicity variables where their overall phase is not fixed by the little group action. In this approach the spin constraint $h-\bar{h}=J$ for celestial conformal primaries emerges naturally from a new Mellin transform, and the action of conformal transformations on celestial amplitudes is derived. Applying this approach to $\mathcal{N}\!=\!4$ super Yang-Mills, we show how the appropriate definition of on-shell superspace coordinates leads naturally to a formulation of chiral celestial superamplitudes and a representation of the generators of the four-dimensional superconformal algebra on the celestial sphere, which by construction annihilate all tree-level celestial superamplitudes.

Celestial Superamplitudes

TL;DR

The paper develops a chiral spinor-helicity framework and a corresponding chiral Mellin transform to define celestial amplitudes with an explicit spin constraint . Focusing on SYM, it constructs a consistent on-shell celestial superspace and derives celestial superamplitudes, along with the full celestial superconformal algebra, showing these generators annihilate tree-level amplitudes. It provides concrete three-, four-, and five-point MHV celestial superamplitudes and outlines the general -point structure, with explicit weight assignments for all celestial operators. The approach clarifies how Lorentz and superconformal symmetries act on celestial data, offering a streamlined path toward a 2D celestial SCFT interpretation and promising extensions to gravity, less-supersymmetric theories, and loop-level celestial amplitudes.

Abstract

We study celestial amplitudes in (super) Yang-Mills theory using a parameterisation of the spinor helicity variables where their overall phase is not fixed by the little group action. In this approach the spin constraint for celestial conformal primaries emerges naturally from a new Mellin transform, and the action of conformal transformations on celestial amplitudes is derived. Applying this approach to super Yang-Mills, we show how the appropriate definition of on-shell superspace coordinates leads naturally to a formulation of chiral celestial superamplitudes and a representation of the generators of the four-dimensional superconformal algebra on the celestial sphere, which by construction annihilate all tree-level celestial superamplitudes.

Paper Structure

This paper contains 19 sections, 100 equations, 1 table.