The structure of IR divergences in celestial gluon amplitudes
Hern\'an A. Gonz\'alez, Francisco Rojas

TL;DR
This paper demonstrates that the IR divergence structure of gauge theory amplitudes persists in celestial amplitudes, revealing a universal factorization involving Wilson lines and implications for the convergence of celestial amplitudes.
Contribution
It proves the persistence of IR divergence factorization in celestial amplitudes and characterizes the soft/collinear factor as a scalar correlator of Wilson lines, extending known gauge theory structures.
Findings
IR divergence factorization persists in celestial amplitudes
Soft/collinear factor is a scalar correlator of Wilson lines
Convergence of Mellin transform is ensured by positive cusp anomalous dimension
Abstract
The all-loop resummation of SU gauge theory amplitudes is known to factorize into an IR-divergent (soft and collinear) factor and a finite (hard) piece. The divergent factor is universal, whereas the hard function is a process-dependent quantity. We prove that this factorization persists for the corresponding celestial amplitudes. Moreover, the soft/collinear factor becomes a scalar correlator of the product of renormalized Wilson lines defined in terms of celestial data. Their effect on the hard amplitude is a shift in the scaling dimensions by an infinite amount, proportional to the cusp anomalous dimension. This leads us to conclude that the celestial-IR-safe gluon amplitude corresponds to a expectation value of operators dressed with Wilson line primaries. These results hold for finite . In the large limit, we show that the soft/collinear correlator can be described in…
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