Nonlinear corrections to the DGLAP equations in view of the HERA data
K. J. Eskola, H. Honkanen, V. J. Kolhinen, Jianwei Qiu, C. A. Salgado
TL;DR
This work investigates the first nonlinear corrections to the DGLAP evolution, known as GLRMQ terms, using HERA $F_2(x,Q^2)$ data and LO PDF baselines from CTEQ5L/CTEQ6L. By fitting to H1 data and constructing nonlinear initial PDFs at $Q_0^2=1.4$ GeV$^2$, the authors show that GLRMQ corrections slow the $Q^2$ evolution and can reconcile small-$x$, low-$Q^2$ behavior with the data, yielding a power-like growth of the gluon density at small $x$ that is substantially enhanced relative to CTEQ6L at $Q_0^2$ but converges to negligible differences at $Q^2 uildrel>ar{ extstylear}{ elax} 10$ GeV$^2$. Sets with different charm thresholds (Sets 2a/2b) confirm that the nonlinear approach can maintain large-$x$ fits while improving the small-$x$/low-$Q^2 region. Overall, nonlinear GLRMQ corrections provide a plausible mechanism to account for high parton densities at small $x$ and low $Q^2$, influencing the inferred gluon PDFs and offering guidance for PDF analyses in the near-saturation regime.
Abstract
The effects of the first nonlinear corrections to the DGLAP evolution equations are studied by using the recent HERA data for the structure function $F_2(x,Q^2)$ of the free proton and the parton distributions from CTEQ5L and CTEQ6L as a baseline. By requiring a good fit to the H1 data, we determine initial parton distributions at $Q_0^2=1.4$ GeV$^2$ for the nonlinear scale evolution. We show that the nonlinear corrections improve the agreement with the $F_2(x,Q^2)$ data in the region of $x\sim 3\cdot 10^{-5}$ and $Q^2\sim 1.5$ GeV$^2$ without paying the price of obtaining a worse agreement at larger values of $x$ and $Q^2$. For the gluon distribution the nonlinear effects are found to play an increasingly important role at $x\lsim 10^{-3}$ and $Q^2\lsim10$ GeV$^2$, but rapidly vanish at larger values of $x$ and $Q^2$. Consequently, contrary to CTEQ6L, the obtained gluon distribution at $Q^2=1.4$ GeV$^2$ shows a power-like growth at small $x$. Relative to the CTEQ6L gluons, an enhancement up to a factor $\sim6$ at $x=10^{-5}$, $Q_0^2=1.4$ GeV$^2$ reduces to a negligible difference at $Q^2\gsim 10$ GeV$^2$.
