Isospin-breaking effects in the three-pion contribution to hadronic vacuum polarization

Abstract Isospin-breaking (IB) effects are required for an evaluation of hadronic vacuum polarization at subpercent precision. While the dominant contributions arise from the e + e − → π + π − channel, also IB in the subleading channels can become relevant for a detailed understanding, e.g., of the...

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Published in:Journal of High Energy Physics
Main Authors: Martin Hoferichter, Bai-Long Hoid, Bastian Kubis, Dominic Schuh
Format: Article
Language:English
Published: SpringerOpen 2023-08-01
Subjects:
Online Access:https://doi.org/10.1007/JHEP08(2023)208
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author Martin Hoferichter
Bai-Long Hoid
Bastian Kubis
Dominic Schuh
author_facet Martin Hoferichter
Bai-Long Hoid
Bastian Kubis
Dominic Schuh
author_sort Martin Hoferichter
collection DOAJ
container_title Journal of High Energy Physics
description Abstract Isospin-breaking (IB) effects are required for an evaluation of hadronic vacuum polarization at subpercent precision. While the dominant contributions arise from the e + e − → π + π − channel, also IB in the subleading channels can become relevant for a detailed understanding, e.g., of the comparison to lattice QCD. Here, we provide such an analysis for e + e − → 3π by extending our dispersive description of the process, including estimates of final-state radiation (FSR) and ρ–ω mixing. In particular, we develop a formalism to capture the leading infrared-enhanced effects in terms of a correction factor η 3π that generalizes the analog treatment of virtual and final-state photons in the 2π case. The global fit to the e + e − → 3π data base, subject to constraints from analyticity, unitarity, and the chiral anomaly, gives a μ 3 π ≤ 1.8 GeV = 45.91 53 × 10 − 10 $$ {\left.{a}_{\mu}^{3\pi}\right|}_{\le 1.8\ \textrm{GeV}}=45.91(53)\times {10}^{-10} $$ for the total 3π contribution to the anomalous magnetic moment of the muon, of which a μ FSR 3 π = 0.51 1 × 10 − 10 $$ {a}_{\mu}^{\textrm{FSR}}\left[3\pi \right]=0.51(1)\times {10}^{-10} $$ and a μ ρ − ω 3 π = − 2.68 70 × 10 − 10 $$ {a}_{\mu}^{\rho -\omega}\left[3\pi \right]=-2.68(70)\times {10}^{-10} $$ can be ascribed to IB. We argue that the resulting cancellation with ρ–ω mixing in e + e − → 2π can be understood from a narrow-resonance picture, and provide updated values for the vacuum-polarization-subtracted vector-meson parameters M ω = 782.70(3) MeV, M ϕ = 1019.21(2) MeV, Γ ω = 8.71(3) MeV, and Γ ϕ = 4.27(1) MeV.
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spelling doaj-art-e7cc8013afa94fcb9fe9a0ffb3ea7d032025-08-19T22:53:10ZengSpringerOpenJournal of High Energy Physics1029-84792023-08-012023813110.1007/JHEP08(2023)208Isospin-breaking effects in the three-pion contribution to hadronic vacuum polarizationMartin Hoferichter0Bai-Long Hoid1Bastian Kubis2Dominic Schuh3Albert Einstein Center for Fundamental Physics, Institute for Theoretical Physics, University of BernAlbert Einstein Center for Fundamental Physics, Institute for Theoretical Physics, University of BernHelmholtz-Institut für Strahlen- und Kernphysik (Theorie) and Bethe Center for Theoretical Physics, Universität BonnHelmholtz-Institut für Strahlen- und Kernphysik (Theorie) and Bethe Center for Theoretical Physics, Universität BonnAbstract Isospin-breaking (IB) effects are required for an evaluation of hadronic vacuum polarization at subpercent precision. While the dominant contributions arise from the e + e − → π + π − channel, also IB in the subleading channels can become relevant for a detailed understanding, e.g., of the comparison to lattice QCD. Here, we provide such an analysis for e + e − → 3π by extending our dispersive description of the process, including estimates of final-state radiation (FSR) and ρ–ω mixing. In particular, we develop a formalism to capture the leading infrared-enhanced effects in terms of a correction factor η 3π that generalizes the analog treatment of virtual and final-state photons in the 2π case. The global fit to the e + e − → 3π data base, subject to constraints from analyticity, unitarity, and the chiral anomaly, gives a μ 3 π ≤ 1.8 GeV = 45.91 53 × 10 − 10 $$ {\left.{a}_{\mu}^{3\pi}\right|}_{\le 1.8\ \textrm{GeV}}=45.91(53)\times {10}^{-10} $$ for the total 3π contribution to the anomalous magnetic moment of the muon, of which a μ FSR 3 π = 0.51 1 × 10 − 10 $$ {a}_{\mu}^{\textrm{FSR}}\left[3\pi \right]=0.51(1)\times {10}^{-10} $$ and a μ ρ − ω 3 π = − 2.68 70 × 10 − 10 $$ {a}_{\mu}^{\rho -\omega}\left[3\pi \right]=-2.68(70)\times {10}^{-10} $$ can be ascribed to IB. We argue that the resulting cancellation with ρ–ω mixing in e + e − → 2π can be understood from a narrow-resonance picture, and provide updated values for the vacuum-polarization-subtracted vector-meson parameters M ω = 782.70(3) MeV, M ϕ = 1019.21(2) MeV, Γ ω = 8.71(3) MeV, and Γ ϕ = 4.27(1) MeV.https://doi.org/10.1007/JHEP08(2023)208Chiral LagrangianPrecision QED
spellingShingle Martin Hoferichter
Bai-Long Hoid
Bastian Kubis
Dominic Schuh
Isospin-breaking effects in the three-pion contribution to hadronic vacuum polarization
Chiral Lagrangian
Precision QED
title Isospin-breaking effects in the three-pion contribution to hadronic vacuum polarization
title_full Isospin-breaking effects in the three-pion contribution to hadronic vacuum polarization
title_fullStr Isospin-breaking effects in the three-pion contribution to hadronic vacuum polarization
title_full_unstemmed Isospin-breaking effects in the three-pion contribution to hadronic vacuum polarization
title_short Isospin-breaking effects in the three-pion contribution to hadronic vacuum polarization
title_sort isospin breaking effects in the three pion contribution to hadronic vacuum polarization
topic Chiral Lagrangian
Precision QED
url https://doi.org/10.1007/JHEP08(2023)208
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