Linear vs non-linear QCD evolution: from HERA data to LHC phenomenology
J. L. Albacete, J. G. Milhano, P. Quiroga-Arias, J. Rojo
TL;DR
The paper tests whether linear DGLAP or non-linear rcBK evolution better describes small-x DIS data from HERA, and assesses the impact on LHC predictions. It systematically compares the two formalisms by applying kinematic cuts that bias each approach and by examining extrapolations to unfitted regions. rcBK fits show stability under cuts and smaller deviations in small-x predictions, while DGLAP exhibits greater sensitivity and larger uncertainties when small-x data are removed. The results argue for a combined framework that accounts for both Q^2 evolution and small-x non-linear dynamics, with implications for precision collider phenomenology and future facilities like the LHeC or EIC.
Abstract
The very precise combined HERA data provides a testing ground in which the relevance of novel QCD regimes, other than the successful linear DGLAP evolution, in small-x inclusive DIS data can be ascertained. We present a study of the dependence of the AAMQS fits, based on the running coupling BK non-linear evolution equations (rcBK), on the fitted dataset. This allows for the identification of the kinematical region where rcBK accurately describes the data, and thus for the determination of its applicability boundary. We compare the rcBK results with NNLO DGLAP fits, obtained with the NNPDF methodology with analogous kinematical cuts. Further, we explore the impact on LHC phenomenology of applying stringent kinematical cuts to the low-x HERA data in a DGLAP fit.
