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Intermediate window observable for the hadronic vacuum polarization contribution to the muon $g-2$ from O$(a)$ improved Wilson quarks
Following the publication of the new measurement of the anomalous magnetic moment of the muon, the discrepancy between experiment and the theory prediction from the $g-2$ theory initiative has increased to $4.2\,\sigma$. Recent lattice QCD calculations predict values for the hadronic vacuum polariza...
Autores principales: | , , , , , , , , , , , , |
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Lenguaje: | eng |
Publicado: |
2022
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.22323/1.430.0321 http://cds.cern.ch/record/2847469 |
_version_ | 1780976780280070144 |
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author | Cè, Marco Gérardin, Antoine von Hippel, Georg Hudspith, Renwick J. Kuberski, Simon Meyer, Harvey Miura, Kohtaroh Mohler, Daniel Ottnad, Konstantin Paul, Srijit Risch, Andreas San José, Teseo Wittig, Hartmut |
author_facet | Cè, Marco Gérardin, Antoine von Hippel, Georg Hudspith, Renwick J. Kuberski, Simon Meyer, Harvey Miura, Kohtaroh Mohler, Daniel Ottnad, Konstantin Paul, Srijit Risch, Andreas San José, Teseo Wittig, Hartmut |
author_sort | Cè, Marco |
collection | CERN |
description | Following the publication of the new measurement of the anomalous magnetic moment of the muon, the discrepancy between experiment and the theory prediction from the $g-2$ theory initiative has increased to $4.2\,\sigma$. Recent lattice QCD calculations predict values for the hadronic vacuum polarization contribution that are larger than the data-driven estimates, bringing the Standard Model prediction closer to the experimental measurement. Euclidean time windows in the time-momentum representation of the hadronic vacuum polarization contribution to the muon $g-2$ can help clarify the discrepancy between the phenomenological and lattice predictions.
We present our calculation of the intermediate distance window contribution using $N_\mathrm{f}=2+1$ flavors of O$(a)$ improved Wilson quarks. We employ ensembles at six lattice spacings below $0.1\,$fm and pion masses down to the physical value. We present a detailed study of the continuum limit, using two discretizations of the vector current and two independent sets of improvement coefficients. Our result at the physical point displays a tension of $3.9\,\sigma$ with a recent evaluation of the intermediate window based on the data-driven method. |
id | cern-2847469 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2022 |
record_format | invenio |
spelling | cern-28474692023-10-26T05:11:36Zdoi:10.22323/1.430.0321http://cds.cern.ch/record/2847469engCè, MarcoGérardin, Antoinevon Hippel, GeorgHudspith, Renwick J.Kuberski, SimonMeyer, HarveyMiura, KohtarohMohler, DanielOttnad, KonstantinPaul, SrijitRisch, AndreasSan José, TeseoWittig, HartmutIntermediate window observable for the hadronic vacuum polarization contribution to the muon $g-2$ from O$(a)$ improved Wilson quarksParticle Physics - PhenomenologyParticle Physics - LatticeFollowing the publication of the new measurement of the anomalous magnetic moment of the muon, the discrepancy between experiment and the theory prediction from the $g-2$ theory initiative has increased to $4.2\,\sigma$. Recent lattice QCD calculations predict values for the hadronic vacuum polarization contribution that are larger than the data-driven estimates, bringing the Standard Model prediction closer to the experimental measurement. Euclidean time windows in the time-momentum representation of the hadronic vacuum polarization contribution to the muon $g-2$ can help clarify the discrepancy between the phenomenological and lattice predictions. We present our calculation of the intermediate distance window contribution using $N_\mathrm{f}=2+1$ flavors of O$(a)$ improved Wilson quarks. We employ ensembles at six lattice spacings below $0.1\,$fm and pion masses down to the physical value. We present a detailed study of the continuum limit, using two discretizations of the vector current and two independent sets of improvement coefficients. Our result at the physical point displays a tension of $3.9\,\sigma$ with a recent evaluation of the intermediate window based on the data-driven method.Following the publication of the new measurement of the anomalous magnetic moment of the muon, the discrepancy between experiment and the theory prediction from the $g-2$ theory initiative has increased to $4.2\,\sigma$. Recent lattice QCD calculations predict values for the hadronic vacuum polarization contribution that are larger than the data-driven estimates, bringing the Standard Model prediction closer to the experimental measurement. Euclidean time windows in the time-momentum representation of the hadronic vacuum polarization contribution to the muon $g-2$ can help clarify the discrepancy between the phenomenological and lattice predictions. We present our calculation of the intermediate distance window contribution using $N_\mathrm{f}=2+1$ flavors of O$(a)$ improved Wilson quarks. We employ ensembles at six lattice spacings below $0.1\,$fm and pion masses down to the physical value. We present a detailed study of the continuum limit, using two discretizations of the vector current and two independent sets of improvement coefficients. Our result at the physical point displays a tension of $3.9\,\sigma$ with a recent evaluation of the intermediate window based on the data-driven method.arXiv:2211.17083MITP-22-102DESY-22-193oai:cds.cern.ch:28474692022-11-30 |
spellingShingle | Particle Physics - Phenomenology Particle Physics - Lattice Cè, Marco Gérardin, Antoine von Hippel, Georg Hudspith, Renwick J. Kuberski, Simon Meyer, Harvey Miura, Kohtaroh Mohler, Daniel Ottnad, Konstantin Paul, Srijit Risch, Andreas San José, Teseo Wittig, Hartmut Intermediate window observable for the hadronic vacuum polarization contribution to the muon $g-2$ from O$(a)$ improved Wilson quarks |
title | Intermediate window observable for the hadronic vacuum polarization contribution to the muon $g-2$ from O$(a)$ improved Wilson quarks |
title_full | Intermediate window observable for the hadronic vacuum polarization contribution to the muon $g-2$ from O$(a)$ improved Wilson quarks |
title_fullStr | Intermediate window observable for the hadronic vacuum polarization contribution to the muon $g-2$ from O$(a)$ improved Wilson quarks |
title_full_unstemmed | Intermediate window observable for the hadronic vacuum polarization contribution to the muon $g-2$ from O$(a)$ improved Wilson quarks |
title_short | Intermediate window observable for the hadronic vacuum polarization contribution to the muon $g-2$ from O$(a)$ improved Wilson quarks |
title_sort | intermediate window observable for the hadronic vacuum polarization contribution to the muon $g-2$ from o$(a)$ improved wilson quarks |
topic | Particle Physics - Phenomenology Particle Physics - Lattice |
url | https://dx.doi.org/10.22323/1.430.0321 http://cds.cern.ch/record/2847469 |
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