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Improved calculation of radiative corrections to $\boldsymbol{τ\toππν_τ}$ decays

Gilberto Colangelo, Martina Cottini, Martin Hoferichter, Simon Holz

Abstract

A reliable calculation of radiative corrections to $τ\toππν_τ$ decays is an important prerequisite for using hadronic $τ$ decays for a data-driven evaluation of the hadronic-vacuum-polarization contribution to the anomalous magnetic moment of the muon, $a_μ^\text{HVP, LO}[ππ,τ]$. In this Letter, we present an improved model-independent analysis of these radiative corrections, including, for the first time, effects beyond point-like pions in the evaluation of the loop diagrams. These structure-dependent corrections, implemented via a dispersive representation of the pion form factor, lead to significant changes compared to previous calculations due to enhancements near the $ρ(770)$ resonance. We also devise strategies for the matching to chiral perturbation theory and a stable implementation of the real corrections down to the two-pion threshold, which shows that some higher-order isospin-breaking corrections need to be kept due to a strong threshold enhancement. Finally, we perform dispersive fits to the currently available $τ\toππν_τ$ spectra and discuss the consequences for isospin-breaking corrections in the evaluation of $a_μ^\text{HVP, LO}[ππ,τ]$.

Improved calculation of radiative corrections to $\boldsymbol{τ\toππν_τ}$ decays

Abstract

A reliable calculation of radiative corrections to decays is an important prerequisite for using hadronic decays for a data-driven evaluation of the hadronic-vacuum-polarization contribution to the anomalous magnetic moment of the muon, . In this Letter, we present an improved model-independent analysis of these radiative corrections, including, for the first time, effects beyond point-like pions in the evaluation of the loop diagrams. These structure-dependent corrections, implemented via a dispersive representation of the pion form factor, lead to significant changes compared to previous calculations due to enhancements near the resonance. We also devise strategies for the matching to chiral perturbation theory and a stable implementation of the real corrections down to the two-pion threshold, which shows that some higher-order isospin-breaking corrections need to be kept due to a strong threshold enhancement. Finally, we perform dispersive fits to the currently available spectra and discuss the consequences for isospin-breaking corrections in the evaluation of .

Paper Structure

This paper contains 19 equations, 5 figures, 2 tables.

Figures (5)

  • Figure 1: Virtual photonic corrections to $\tau\to\pi\pi\nu_\tau$ in ChPT. Solid lines denote leptons, dashed lines pions, and wiggly lines photons. Not shown are self-energy diagrams and contact terms.
  • Figure 2: Box diagram in a dispersive approach. The gray blobs denote the pion form factor, in the neutral and charged channel, respectively. The short-dashed line indicates that the intermediate-state pion is taken on-shell.
  • Figure 3: Sample diagrams for the real corrections from the WZW anomaly as well as the exchange of vector and axial-vector meson resonances (indicated by the double lines). Otherwise notation as in Figs. \ref{['fig:diagrams_ChPT']} and \ref{['fig:diagrams_disp']}.
  • Figure 4: Global fit to the $\tau\to\pi\pi\nu_\tau$ spectrum, including the data sets from Belle Belle:2008xpe, ALEPH ALEPH:2005qgpDavier:2013sfa, CLEO CLEO:1999dln, and OPAL OPAL:1998rrm.
  • Figure 5: Final result for $G_\text{EM}(s)$ and comparison to previous work, Flores-Baéz et al. (2006) Flores-Baez:2006yiq, Miranda, Roig (2020) Miranda:2020wdg, and using ChPT instead of dispersion relations for the box diagram (based on Refs. Cirigliano:2001erCirigliano:2002pv).