Extending the LCSR method to the electromagnetic pion form factor at low momenta using QCD renormalization-group summation
Cesar Ayala, S. V. Mikhailov, A. V. Pimikov
TL;DR
This work extends the light-cone sum rule approach to the electromagnetic pion form factor by incorporating renormalization-group summation, which, together with dispersion relations, converts the perturbative expansion into a fractional analytic perturbation theory (FAPT) framework. The method is applied to twist-2 as well as twist-4 (and twist-6) contributions, yielding an emFF description that remains well-behaved at low momentum transfers ($Q^2\sim0.5$ GeV$^2$) due to Landau-pole-free couplings. Using corrected twist-2 DA coefficients and nonperturbative twist-4/6 inputs, the RG-summed predictions agree with JLab data for $Q^2\lesssim 1$ GeV$^2$, and a hybrid NLO comparison clarifies the relative size of fixed-order corrections. The approach shows promise for extracting the leading-twist pion DA from data once the complete NLO corrections are available, highlighting the interplay between perturbative refinements and nonperturbative DA inputs in shaping the emFF. Overall, the paper demonstrates that RG-summed LCSR combined with FAPT and dispersion relations provides a robust, low-$Q^2$ description of $F_\pi$, with a clear path toward quantitative determinations of the pion's internal structure.
Abstract
We obtain the electromagnetic pion form factor (emFF) $F_π$ for spacelike mid-range of momentum transfer in QCD. We use renormalization group (RG) summation within the light cone sum rules (LCSRs) to obtain the QCD radiative corrections to the $F_π$ and involve contributions of the leading twist 2 and, twists 4, 6. The additional conditions to apply here this RG summation are discussed in details. The strong coupling constants in this approach are free of Landau singularities, which allows one to go down to the lower transferred momentum $Q^2$. The prediction of the calculations performed reproduces the experimental data below/around $Q^2= 1$~GeV$^2$ significantly better than analogous predictions based on a fixed-order power-series expansion in the standard QCD.
