Running coupling and power corrections in nonlinear evolution at the high--energy limit
Einan Gardi, Janne Kuokkanen, Kari Rummukainen, Heribert Weigert
TL;DR
This work extends nonlinear small-x QCD evolution (JIMWLK/BK) to incorporate running-coupling effects by deriving an all-orders, dispersively resummed kernel. It reveals infrared renormalon ambiguities and associated non-perturbative power corrections, and provides a PV-Borel sum to quantify their impact. Numerical BK evolution with the resummed kernel shows that both perturbative running-coupling corrections and power corrections are sizable at present energies, slowing the evolution and sharpening the saturation scale behavior. The results provide a first predictive framework for including running-coupling and power corrections in high-density QCD and highlight key directions for extending the formalism to full NLO and phenomenology.
Abstract
A main feature of high-energy scattering in QCD is saturation in the number density of gluons. This phenomenon is described by non-linear evolution equations, JIMWLK and BK, which have been derived at leading logarithmic accuracy. In this paper we generalize this framework to include running coupling corrections to the evolution kernel. We develop a dispersive representation of the dressed gluon propagator in the background of Weiszacker Williams fields and use it to compute O(beta_0^{n-1} alpha_s^n) corrections to the kernel to all orders in perturbation theory. The resummed kernels present infrared-renormalon ambiguities, which are indicative of the form and importance of non-perturbative power corrections. We investigate numerically the effect of the newly computed perturbative corrections as well as the power corrections on the evolution and find that at present energies they are both significant.
