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

Abstract The 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...

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Main Authors: Martin Hoferichter, Bai-Long Hoid, Bastian Kubis, Stefan Leupold, Sebastian P. Schneider
Format: Article
Language:English
Published: SpringerOpen 2018-10-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP10(2018)141
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author Martin Hoferichter
Bai-Long Hoid
Bastian Kubis
Stefan Leupold
Sebastian P. Schneider
author_facet Martin Hoferichter
Bai-Long Hoid
Bastian Kubis
Stefan Leupold
Sebastian P. Schneider
author_sort Martin Hoferichter
collection DOAJ
description Abstract The 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, a μ π 0 − 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.
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spelling doaj.art-1aee0ab73a824870baa4fb62ff8fd1da2022-12-22T00:53:28ZengSpringerOpenJournal of High Energy Physics1029-84792018-10-0120181015710.1007/JHEP10(2018)141Dispersion relation for hadronic light-by-light scattering: pion poleMartin Hoferichter0Bai-Long Hoid1Bastian Kubis2Stefan Leupold3Sebastian P. Schneider4Institute for Nuclear Theory, University of WashingtonHelmholtz-Institut für Strahlen- und Kernphysik (Theorie), Universität BonnHelmholtz-Institut für Strahlen- und Kernphysik (Theorie), Universität BonnInstitutionen för fysik och astronomi, Uppsala UniversitetHelmholtz-Institut für Strahlen- und Kernphysik (Theorie), Universität BonnAbstract The 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, a μ π 0 − 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.http://link.springer.com/article/10.1007/JHEP10(2018)141Chiral LagrangiansEffective Field TheoriesNonperturbative EffectsPrecision QED
spellingShingle Martin Hoferichter
Bai-Long Hoid
Bastian Kubis
Stefan Leupold
Sebastian P. Schneider
Dispersion relation for hadronic light-by-light scattering: pion pole
Journal of High Energy Physics
Chiral Lagrangians
Effective Field Theories
Nonperturbative Effects
Precision QED
title Dispersion relation for hadronic light-by-light scattering: pion pole
title_full Dispersion relation for hadronic light-by-light scattering: pion pole
title_fullStr Dispersion relation for hadronic light-by-light scattering: pion pole
title_full_unstemmed Dispersion relation for hadronic light-by-light scattering: pion pole
title_short Dispersion relation for hadronic light-by-light scattering: pion pole
title_sort dispersion relation for hadronic light by light scattering pion pole
topic Chiral Lagrangians
Effective Field Theories
Nonperturbative Effects
Precision QED
url http://link.springer.com/article/10.1007/JHEP10(2018)141
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