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Hadronic vacuum polarization for the muon \\(g-2\\) from lattice QCD: Complete short and intermediate windows
Hadronic vacuum polarization for the muon \\(g-2\\) from lattice QCD: Complete short and intermediate windows
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Hadronic vacuum polarization for the muon \\(g-2\\) from lattice QCD: Complete short and intermediate windows
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Hadronic vacuum polarization for the muon \\(g-2\\) from lattice QCD: Complete short and intermediate windows
Hadronic vacuum polarization for the muon \\(g-2\\) from lattice QCD: Complete short and intermediate windows

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Hadronic vacuum polarization for the muon \\(g-2\\) from lattice QCD: Complete short and intermediate windows
Hadronic vacuum polarization for the muon \\(g-2\\) from lattice QCD: Complete short and intermediate windows
Paper

Hadronic vacuum polarization for the muon \\(g-2\\) from lattice QCD: Complete short and intermediate windows

2024
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Overview
We present complete results for the hadronic vacuum polarization (HVP) contribution to the muon anomalous magnetic moment \\(a_\\mu\\) in the short- and intermediate-distance window regions, which account for roughly 10% and 35% of the total HVP contribution to \\(a_\\mu\\), respectively. In particular, we perform lattice-QCD calculations for the isospin-symmetric connected and disconnected contributions, as well as corrections due to strong isospin-breaking. For the short-distance window observables, we investigate the so-called log-enhancement effects as well as the significant oscillations associated with staggered quarks in this region. For the dominant, isospin-symmetric light-quark connected contribution, we obtain \\(a^{ll,\\,{\\mathrm{SD}}}_{\\mu}(\\mathrm{conn.}) = 48.116(16)(94)[96] \\times 10^{-10}\\) and \\(a^{ll,\\,{\\mathrm{W}}}_{\\mu}(\\mathrm{conn.}) = 207.06(17)(63)[66] \\times 10^{-10}\\). We use Bayesian model averaging combined with a global bootstrap to fully estimate the covariance matrix between the individual contributions. Our determinations of the complete window contributions are \\(a^{{\\mathrm{SD}}}_{\\mu} = 69.01(2)(21)[21] \\times 10^{-10}\\) and \\(a^{{\\mathrm{W}}}_{\\mu} = 236.57(20)(94)[96] \\times 10^{-10}\\). This work is part of our ongoing effort to compute all contributions to HVP with an overall uncertainty at the few permille level.
Publisher
Cornell University Library, arXiv.org