Abstract

The operator product expansion of massless celestial primary operators of arbitrary spin is investigated. Poincaré symmetry is found to imply a set of recursion relations on the operator product expansion coefficients of the leading singular terms at tree-level in a holomorphic limit. The symmetry constraints are solved by an Euler beta function with arguments that depend simply on the right-moving conformal weights of the operators in the product. These symmetry-derived coefficients are shown not only to match precisely those arising from momentum-space tree-level collinear limits, but also to obey an infinite number of additional symmetry transformations that respect the algebra of w1+∞. In tree-level minimally-coupled gravitational theories, celestial currents are constructed from light transforms of conformally soft gravitons and found to generate the action of w1+∞ on arbitrary massless celestial primaries. Results include operator product expansion coefficients for fermions as well as those arising from higher-derivative non-minimal couplings of gluons and gravitons.

Highlights

  • Poincaré symmetry is found to imply a set of recursion relations on the operator product expansion coefficients of the leading singular terms at tree-level in a holomorphic limit

  • A more thorough investigation of this proposal is aided by working in a language in which the underlying two dimensions are rendered manifest. 2D conformal (4D Lorentz) symmetry is the basis of this two-dimensional description, so these two dimensions are more readily apparent in the scattering of particles of definite boost weight, as opposed to the standard momentum eigenstates

  • The Ward identities for infinitedimensional symmetries that follow from soft theorems are powerful and encouraging examples of this behavior

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Summary

Poincaré in celestial amplitudes

We briefly review Poincaré symmetry in the context of celestial amplitudes, studied for example in [53]. It is compatible with Poincaré to regard the translation generators as the modes of a primary operator the left, right, or both conformal weights are. Such primary operators can be constructed by taking various light or shadow transforms of the ∆ = 1 conformally soft graviton. These modes do not automatically form a closed algebra with the global conformal generators and require an additional assumption of a truncated mode expansion as presented, for example, in [24, 27]. More details on this alternative mode expansion are provided in appendix B

OPEs from Poincaré symmetry
OPEs from collinear limits
A Conventions
B Holographic symmetry algebra
Special cases

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