Split representation in celestial holography

TL;DR

This paper introduces a split representation for celestial amplitudes in celestial holography, enabling the computation of conformal block expansions and revealing novel intermediate exchanges in massless scalar amplitudes.

Contribution

It develops a split representation for celestial amplitudes by expressing bulk-to-bulk propagators as boundary integrals, facilitating conformal block analysis in celestial holography.

Findings

Derived conformal partial wave and block expansions for celestial four-point functions.

Identified novel intermediate exchanges of staggered modules in the t-channel.

Provided a new computational framework for celestial amplitudes.

Abstract

We develop a split representation for celestial amplitudes in celestial holography, by cutting internal lines of Feynman diagrams in Minkowski space. More explicitly, the bulk-to-bulk propagators associated with the internal lines are expressed as a product of two boundary-to-bulk propagators with a coinciding boundary point integrated over the celestial sphere. Applying this split representation, we compute the conformal partial wave and conformal block expansions of celestial four-point functions of massless scalars and photons on the Euclidean celestial sphere. In the $t$-channel massless scalar amplitude, we observe novel intermediate exchanges of staggered modules in the conformal block expansion.