Abstract
Amplitude-level factorization for a soft gluon emission has long been understood in terms of a product of loop-expanded soft-gluon currents and hard scattering matrix elements, both of which are infrared (IR) divergent. Thus, the amplitude for multiple soft gluon emissions, ordered in their relative softness, can be written as a product of IR divergent soft gluon currents and the matrix elements. In a more recent work, Angeles-Martinez, Forshaw and Seymour [1] (AMFS) showed that the result for this amplitude can in fact be re-expressed in an ordered evolution approach, involving IR finite one-loop insertions where the virtual loop momentum is constrained in a highly non-trivial way by the kT of the adjacent real emissions. The result thus exhibits a novel amplitude level QCD coherence where the IR divergences originating only from the very last, softest, gluon emission remain, and the rest cancel. The proof of the AMFS result at one-loop in QCD, however, involves many diagrams, and only after carefully grouping and summing over all the diagrams does the correct ordering variable emerge, making the higher order extension a challenging task. Moreover, the compact, Markovian nature of the final AMFS result is suggestive of a deeper underlying physics that is obscured in the derivation using traditional diagrammatic QCD. By considering a (recursive) sequence of effective field theories (EFTs) with Glauber-SCET operators, we present an elegant derivation of this result involving only a handful of diagrams. The SCET derivation offers clean physical insights, and makes a higher order extension of the AMFS result tractable. We also show that the grouping of QCD graphs necessary to derive the AMFS result in full theory is already implicit in the Feynman rules of Glauber-SCET operators such that the same result can alternatively be derived with significantly less effort in a single EFT with multiple ordered soft gluon emissions.
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Pathak, A. A new form of QCD coherence for multiple soft emissions using Glauber-SCET. J. High Energ. Phys. 2022, 118 (2022). https://doi.org/10.1007/JHEP06(2022)118
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DOI: https://doi.org/10.1007/JHEP06(2022)118