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Dispersion relation for hadronic light-by-light scattering: pion pole

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A bstractThe pion-pole contribution to hadronic light-by-light scattering in the anomalous magnetic moment of the muon (g − 2)μ is fully determined by the doubly-virtual pion transition form factor. Although… Click to show full abstract

A bstractThe pion-pole contribution to hadronic light-by-light scattering in the anomalous magnetic moment of the muon (g − 2)μ is fully determined by the doubly-virtual pion transition form factor. Although this crucial input quantity is, in principle, directly accessible in experiment, a complete measurement covering all kinematic regions relevant for (g −2)μ is not realistic in the foreseeable future. Here, we report in detail on a reconstruction from available data, both space- and time-like, using a dispersive representation that accounts for all the low-lying singularities, reproduces the correct high- and low-energy limits, and proves convenient for the evaluation of the (g − 2)μ loop integral. We concentrate on the systematics of the fit to e+e− → 3π data, which are key in constraining the isoscalar dependence, as well as the matching to the asymptotic limits. In particular, we provide a detailed account of the pion transition form factor at low energies in the time- and space-like region, including the error estimates underlying our final result for the pion-pole contribution, aμπ0−pole=62.6−2.5+3.0×10−11$$ {a}_{\mu}^{\uppi^0-\mathrm{pole}}={62.6}_{-2.5}^{+3.0}\times {10}^{-11} $$, and demonstrate how forthcoming singly-virtual measurements will further reduce its uncertainty.

Keywords: hadronic light; pion pole; light; light light; light scattering; pion

Journal Title: Journal of High Energy Physics
Year Published: 2018

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