Pseudoscalar pole contribution to the hadronic light-by-light piece of aμ

We have studied the P → γ⋆ γ⋆ form factor in Resonance Chiral Theory, with P = π0; η, η', to compute the contribution of the pseudoscalar pole to the hadronic light-by-light piece of the anomalous magnetic moment of the muon. In this work we allow the leading U(3) chiral symmetry breaking terms...

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Main Authors: Guevara Adolfo, Roig Pablo, Sanz Cillero Juan José
Format: Article
Language:English
Published: EDP Sciences 2018-01-01
Series:EPJ Web of Conferences
Online Access:https://doi.org/10.1051/epjconf/201819200027
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spelling doaj-936f9941c0084b6d8c5056f050d33e7b2021-08-02T06:14:32ZengEDP SciencesEPJ Web of Conferences2100-014X2018-01-011920002710.1051/epjconf/201819200027epjconf_qcd2018_00027Pseudoscalar pole contribution to the hadronic light-by-light piece of aμGuevara AdolfoRoig PabloSanz Cillero Juan JoséWe have studied the P → γ⋆ γ⋆ form factor in Resonance Chiral Theory, with P = π0; η, η', to compute the contribution of the pseudoscalar pole to the hadronic light-by-light piece of the anomalous magnetic moment of the muon. In this work we allow the leading U(3) chiral symmetry breaking terms, obtaining the most general expression for the form factor of order O(m2P). The parameters of the Effective Field Theory are obtained by means of short distance constraints on the form factor and matching with the expected behavior from QCD. Those parameters that cannot be fixed in this way are fitted to experimental determinations of the form factor within the spacelike momentum region of the virtual photon. Chiral symmetry relations among the transition form factors for π0, η and η' allow for a simultaneous fit to experimental data for the three mesons. This shows an inconsistency between the BaBar π0 data and the rest of the experimental inputs. Thus, we find a total pseudoscalar pole contribution of aP,HLbLη = (8:47 ± 0:16) · 10-10 for our best fit (neglecting the BaBar π0 data). Also, a preliminary rough estimate of the impact of NLO in 1=NC corrections and higher vector multiplets (asym) enlarges the uncertainty up to aP,HLbLη = (8:47 ± 0:16stat ± 0:09NC +0:5 -0:0asym).https://doi.org/10.1051/epjconf/201819200027
collection DOAJ
language English
format Article
sources DOAJ
author Guevara Adolfo
Roig Pablo
Sanz Cillero Juan José
spellingShingle Guevara Adolfo
Roig Pablo
Sanz Cillero Juan José
Pseudoscalar pole contribution to the hadronic light-by-light piece of aμ
EPJ Web of Conferences
author_facet Guevara Adolfo
Roig Pablo
Sanz Cillero Juan José
author_sort Guevara Adolfo
title Pseudoscalar pole contribution to the hadronic light-by-light piece of aμ
title_short Pseudoscalar pole contribution to the hadronic light-by-light piece of aμ
title_full Pseudoscalar pole contribution to the hadronic light-by-light piece of aμ
title_fullStr Pseudoscalar pole contribution to the hadronic light-by-light piece of aμ
title_full_unstemmed Pseudoscalar pole contribution to the hadronic light-by-light piece of aμ
title_sort pseudoscalar pole contribution to the hadronic light-by-light piece of aμ
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2018-01-01
description We have studied the P → γ⋆ γ⋆ form factor in Resonance Chiral Theory, with P = π0; η, η', to compute the contribution of the pseudoscalar pole to the hadronic light-by-light piece of the anomalous magnetic moment of the muon. In this work we allow the leading U(3) chiral symmetry breaking terms, obtaining the most general expression for the form factor of order O(m2P). The parameters of the Effective Field Theory are obtained by means of short distance constraints on the form factor and matching with the expected behavior from QCD. Those parameters that cannot be fixed in this way are fitted to experimental determinations of the form factor within the spacelike momentum region of the virtual photon. Chiral symmetry relations among the transition form factors for π0, η and η' allow for a simultaneous fit to experimental data for the three mesons. This shows an inconsistency between the BaBar π0 data and the rest of the experimental inputs. Thus, we find a total pseudoscalar pole contribution of aP,HLbLη = (8:47 ± 0:16) · 10-10 for our best fit (neglecting the BaBar π0 data). Also, a preliminary rough estimate of the impact of NLO in 1=NC corrections and higher vector multiplets (asym) enlarges the uncertainty up to aP,HLbLη = (8:47 ± 0:16stat ± 0:09NC +0:5 -0:0asym).
url https://doi.org/10.1051/epjconf/201819200027
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