Energy Detectors and Asymptotic Symmetries
Hernán A. González, Jakob Salzer
TL;DR
The paper develops detector operators that measure energy flux at null infinity and shows they form a universal set under collinear factorization, yielding a closed leading OPE for generalized energy operators $\mathcal{E}^{[s]}_{\Delta}$ in both gravity and Yang–Mills theories. It identifies the $\Delta=2$ detector as the particle-number operator, and demonstrates that particle counting is not independent but is determined by soft charges, expressible as bilinears of conformally soft currents in gravity (via $P_z$) and in gauge theory (via soft currents $J_z,J_{ar z}$ and their shadows). The work connects detector observables to the soft sector of celestial holography, matching bulk collinear data with celestial OPEs and revealing a unified soft–detector structure that may hint at an underlying Celestial CFT organization. These results provide a concrete framework to study infrared physics, memory effects, and asymptotic symmetries through detectors on the celestial sphere and Carrollian boundary fields, with potential extensions to other detector observables and higher-point correlators.
Abstract
We study detector operators measuring energy to a power $Δ-2$ at null infinity in four-dimensional gauge theories and gravity. These operators transform as conformal primaries on the celestial sphere and provide a natural basis for describing energy-flux observables in scattering processes. Using the collinear factorization of scattering amplitudes, we derive the universal leading structure of the operator product expansion. A key consequence of our analysis is the precise identification of the $Δ=2$ detector, the number operator. Exploiting the fact that soft charges generate symmetries of the S-matrix, we demonstrate that the number of particles is entirely determined by the product of two soft currents: in gravity, the operator is the square of the supertranslation generator, while in Yang-Mills yields a product of $SU(N)$ Kac-Moody soft currents. This work establishes thus a direct link between detector observables and the soft sector of celestial holography.
