ﻻ يوجد ملخص باللغة العربية
The leading-order hadronic contribution to the muon anomalous magentic moment, $a_mu^{rm LO,HVP}$, can be expressed as an integral over Euclidean $Q^2$ of the vacuum polarization function. We point out that a simple trapezoid-rule numerical integration of the current lattice data is good enough to produce a result with a less-than-$1%$ error for the contribution from the interval above $Q^2gtrsim 0.1-0.2 mathrm{GeV}^2$. This leaves the interval below this value of $Q^2$ as the one to focus on in the future. In order to achieve an accurate result also in this lower window $Q^2lesssim 0.1-0.2 mathrm{GeV}^2$, we indicate the usefulness of three possible tools. These are: Pad{e} Approximants, polynomials in a conformal variable and a NNLO Chiral Perturbation Theory representation supplemented by a $Q^4$ term. The combination of the numerical integration in the upper $Q^2$ interval together with the use of these tools in the lower $Q^2$ interval provides a hybrid strategy which looks promising as a means of reaching the desired goal on the lattice of a sub-percent precision in the hadronic vacuum polarization contribution to the muon anomalous magnetic moment.
We report on our computation of the leading hadronic contribution to the anomalous magnetic moment of the muon using two dynamical flavours of non-perturbatively O(a) improved Wilson fermions. The strange quark is introduced in the quenched approxima
We report on our ongoing project to calculate the leading hadronic contribution to the anomalous magnetic moment of the muon a_mu^HLO using two dynamical flavours of non-perturbatively O(a) improved Wilson fermions. In this study, we changed the vacu
We calculate the leading-order hadronic correction to the anomalous magnetic moments of each of the three charged leptons in the Standard Model: the electron, muon and tau. Working in two-flavor lattice QCD, we address essentially all sources of syst
We present results of calculations of the hadronic vacuum polarisation contribution to the muon anomalous magnetic moment. Specifically, we focus on controlling the infrared regime of the vacuum polarisation function. Our results are corrected for fi
The persistent discrepancy of about 3.5 standard deviations between the experimental measurement and the Standard Model prediction for the muon anomalous magnetic moment, $a_mu$, is one of the most promising hints for the possible existence of new ph