Abstract

We address the contribution of the 3π channel to hadronic vacuum polarization (HVP) using a dispersive representation of the e+e− → 3π amplitude. This channel gives the second-largest individual contribution to the total HVP integral in the anomalous magnetic moment of the muon (g − 2)μ, both to its absolute value and uncertainty. It is largely dominated by the narrow resonances ω and ϕ, but not to the extent that the off-peak regions were negligible, so that at the level of accuracy relevant for (g − 2)μ an analysis of the available data as model independent as possible becomes critical. Here, we provide such an analysis based on a global fit function using analyticity and unitarity of the underlying γ∗ → 3π amplitude and its normalization from a chiral low-energy theorem, which, in particular, allows us to check the internal consistency of the various e+e− → 3π data sets. Overall, we obtain {a}_{mu}^{3pi } |≤1.8 GeV = 46.2(6)(6) × 10−10 as our best estimate for the total 3π contribution consistent with all (low-energy) constraints from QCD. In combination with a recent dispersive analysis imposing the same constraints on the 2π channel below 1 GeV, this covers nearly 80% of the total HVP contribution, leading to {a}_{mu}^{mathrm{HVP}} = 692.3(3.3) × 10−10 when the remainder is taken from the literature, and thus reaffirming the (g−2)μ anomaly at the level of at least 3.4σ. As side products, we find for the vacuum-polarization-subtracted masses Mω = 782.63(3)(1) MeV and Mϕ = 1019.20(2)(1) MeV, confirming the tension to the ω mass as extracted from the 2π channel.

Highlights

  • We address the contribution of the 3π channel to hadronic vacuum polarization (HVP) using a dispersive representation of the e+e− → 3π amplitude

  • We have presented a detailed analysis of the 3π contribution to HVP, including constraints from analyticity and unitarity as well as the low-energy theorem for the γ∗ → 3π amplitude

  • To the 2π analysis of the pion vector form factor [36], the main motivations are, first, to see if a global fit subject to these constraints reveals inconsistencies in the data, and, second, derive the corresponding error estimate for the contribution to (g −2)μ. Given that this method is complementary to a direct integration of the data, where potential inconsistencies are addressed by a local error inflation, such global fits that incorporate general QCD constraints should increase the robustness of the SM prediction

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Summary

Data sets and unbiased fitting

We start with a brief summary of the data sets that we will include in our analysis, see table 1. To follow the experimental documentation as closely as possible, we consider a systematic error of normalization-type origin whenever given as a percentage, otherwise, we treat that uncertainty as a diagonal error Note that this distinction mainly affects the SND data sets, while for the other energy-scan experiments all systematic errors are given as a percentage. The exception is the ISR data set from BaBar, but [68] states explicitly that the systematic errors for different mass bins are fully correlated These details are important to monitor a potential bias in the fit. We follow the iterative fit strategy proposed by the NNPDF collaboration [88] to eliminate the bias, which is based on the observation that the normalization uncertainties should be proportional to the true value rather than the measurement In this manner, the modified iterative covariance matrix is given as. We will consider both diagonal and full fits to monitor whether significant differences arise

Fits to SND
Fits to CMD-2 and BaBar
Combined fits
Extracting ω and φ masses
Consequences for the anomalous magnetic moment of the muon
Summary
A Electromagnetic mass shifts
Findings
B Estimate of the F -wave contribution
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