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Progress on computing the hadronic vacuum polarization contribution to the muon anomalous magnetic moment with staggered fermions

Vaishakhi Moningi, Christopher Aubin, Thomas Blum, Maarten Golterman, Luchang Jin, Santiago Peris

Abstract

We give an update of our calculation of the light-quark, connected, hadronic vacuum polarization contribution to the muon anomalous magnetic moment, or muon $g-2$. The update includes preliminary results on a $2 + 1 + 1$ highly-improved staggered quark (HISQ) ensemble from the MILC collaboration with physical pion mass, $0.042$ fm lattice spacing, and volume $144^3 \times 288$. We discuss code and algorithm improvements for these calculations to compute the vector-vector correlation function more efficiently.

Progress on computing the hadronic vacuum polarization contribution to the muon anomalous magnetic moment with staggered fermions

Abstract

We give an update of our calculation of the light-quark, connected, hadronic vacuum polarization contribution to the muon anomalous magnetic moment, or muon . The update includes preliminary results on a highly-improved staggered quark (HISQ) ensemble from the MILC collaboration with physical pion mass, fm lattice spacing, and volume . We discuss code and algorithm improvements for these calculations to compute the vector-vector correlation function more efficiently.
Paper Structure (9 sections, 11 equations, 5 figures, 2 tables)

This paper contains 9 sections, 11 equations, 5 figures, 2 tables.

Figures (5)

  • Figure 1: The summand in Eq. (\ref{['eq:t-m amu']}). No LMA (left), total (middle), LMA only (right). Odd-parity, excited state oscillations intrinsic to staggered fermions are readily apparent.
  • Figure 2: Comparision of the summand in Eq. \ref{['eq:t-m amu']} between our old method and new method for the $64^3$ ensemble.
  • Figure 3: Statistical errors on the summand in Eq. (\ref{['eq:t-m amu']}). Comparison between number of hits (left) and comparison between old and new method (right).
  • Figure 4: LL contribution from contracting the meson fields with, and without, sparsening the low-modes.
  • Figure 5: Summand in Eq. (\ref{['eq:t-m amu']}) for the $144^3$ ensemble (left) and uncorrected results for the intermediate window value. The new point at $a=0.042$ fm (see Table \ref{['tab:144c intermediate win']}) is compared with our earlier results Aubin:2022hgm (right). Errors shown are statistical only.