Aug 3 – 7, 2026
Department of Physics, University of Connecticut
America/New_York timezone

High-precision Monte Carlo predictions for radiative return with BabaYaga@NLO

Aug 3, 2026, 4:10 PM
30m
GS117 and GS119 (Department of Physics, University of Connecticut)

GS117 and GS119

Department of Physics, University of Connecticut

196A Auditorium Rd Unit 3046, Storrs, CT 06269

Speaker

Marco Ghilardi (University of Pavia-INFN Section of Pavia)

Description

To resolve the tension between lattice QCD and data-driven evaluations of the hadronic
vacuum polarization contribution to the muon anomaly $a_\mu$, precise cross-section measurements
of the dominant $\pi^+\pi^-$ channel are highly relevant. The radiative return process
$e^+e^- \to \pi^+\pi^-\gamma$ at flavor factories is essential for extracting this
cross section below $2\,\mathrm{GeV}$, requiring tight control over theoretical systematic uncertainties.

To this end, we present the first calculation of QED
next-to-leading order (NLO) corrections to radiative pion and muon pair production in
$e^+e^-$ annihilation, matched to a QED Parton Shower (PS) algorithm for fully exclusive
simulations, achieving NLOPS accuracy. For the dipion channel, we go beyond the
factorized approach (FxsQED) to evaluate structure-dependent corrections by
including the pion form factor in the one-loop
amplitudes according to different formulations. These developments are implemented in a new version of the
BabaYaga@NLO event generator, and we present the corresponding
phenomenological results for $e^+e^- \to X^+X^-\gamma$ ($X=\mu,\pi$) in different experimental scenarios from 1 GeV to 10 GeV.

Author

Marco Ghilardi (University of Pavia-INFN Section of Pavia)

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