On the inclusion of the pion form factor in $e^+e^- \to π^+π^-$ beyond leading order
Francesco P. Ucci
TL;DR
The paper addresses the precision challenges in predicting the hadronic vacuum-polarization contribution to $(g-2)_$, highlighting the dominance of the $pipi$ channel and the need for radiative corrections beyond the leading-order factorised $F_pi(q^2)$ treatment. It compares ab-initio lattice and dispersive approaches, emphasizing recent CMD-3 results that bring theory and experiment closer, while still requiring next-to-leading order (NLO) radiative corrections. The authors implement three strategies—generalised vector meson dominance (GVMD), a dispersive FsQED approach, and a factorised sQED baseline—within an updated version of the BabaYaga@NLO Monte Carlo to include the pion form factor inside loop amplitudes. Numerical results show sizable NLO effects (up to $\pm 8\%$ on integrated cross sections) and nontrivial forward-backward asymmetries, underscoring the importance of accounting for pion compositeness at loop level for precision hadronic predictions and MC event generation.
Abstract
The pion form factor plays a crucial role in the determination of the contribution of the hadronic vacuum polarisation to the muon anomalous magnetic moment. In order to measure this quantity, energy-scan experiments rely on Monte Carlo generator to simulate the $e^+e^- \to π^+π^-(γ)$ process. For the theoretical accuracy to match the experimental precision, next-to-leading order calculations and the resummation of multiple photon emissions are needed. In this context, the inclusion of the pion form factor beyond the leading order approximation is crucial to reproduce some observables, like the pion charge asymmetry. We present the impact of the inclusion of the pion form factor in loop diagrams with three approaches and the interplay with radiative corrections.
