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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SpringerOpen
2018-10-01
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Series: | Journal of High Energy Physics |
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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. |
first_indexed | 2024-12-11T19:22:53Z |
format | Article |
id | doaj.art-1aee0ab73a824870baa4fb62ff8fd1da |
institution | Directory Open Access Journal |
issn | 1029-8479 |
language | English |
last_indexed | 2024-12-11T19:22:53Z |
publishDate | 2018-10-01 |
publisher | SpringerOpen |
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series | Journal of High Energy Physics |
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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