Collinear functions for QCD resummations
Stefano Catani, Prasanna K. Dhani

TL;DR
This paper develops and analyzes collinear functions derived from splitting kernels in QCD, addressing their role in resummation of hard-scattering observables and exploring their dependence on auxiliary vectors and process-specific effects.
Contribution
It introduces a systematic way to define and compute collinear functions for QCD resummation, including their dependence on auxiliary vectors and higher-order corrections.
Findings
Time-like auxiliary vectors avoid rapidity divergences.
Computed collinear functions at ${\cal O}(\alpha_{\rm S})$ and ${\cal O}(\alpha_{\rm S}^2)$.
Identified process dependence of collinear functions beyond ${\cal O}(\alpha_{\rm S}^2)$.
Abstract
The singular behaviour of QCD squared amplitudes in the collinear limit is factorized and controlled by splitting kernels with a process-independent structure. We use these kernels to define collinear functions that can be used in QCD resummation formulae of hard-scattering observables. Different collinear functions are obtained by integrating the splitting kernels over different phase-space regions that depend on the hard-scattering observables of interest. The collinear functions depend on an auxiliary vector that can be either light-like or time-like . In the case of transverse-momentum dependent (TMD) collinear functions, we show that the use of a time-like auxiliary vector avoids the rapidity divergences, which are instead present if . The perturbative computation of the collinear functions lead to infrared (IR) divergences that can be properly…
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Taxonomy
TopicsParticle physics theoretical and experimental studies · Algorithms and Data Compression · Mathematics, Computing, and Information Processing
