6533b82afe1ef96bd128b920
RESEARCH PRODUCT
Vacuum correlators at short distances from lattice QCD
Marco CèTim HarrisHarvey B. MeyerArianna ToniatoCsaba Töröksubject
Nuclear and High Energy PhysicsHigh Energy Physics::Latticepolecostshep-latFOS: Physical sciencesLattice QCDQC770-798nonperturbativeoperator product expansion53001 natural sciences7. Clean energythermal [correlation function]lattice [perturbation theory]High Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)Nuclear and particle physics. Atomic energy. Radioactivityprecision measurement [electroweak interaction]quantum chromodynamics0103 physical sciencesPerturbative QCDhadronic [vacuum polarization]ddc:530010306 general physicsParticle Physics - Phenomenology010308 nuclear & particles physicsscreeningComputer Science::Information RetrievalphotonHigh Energy Physics - Lattice (hep-lat)lattice field theorytemperaturehep-phParticle Physics - LatticeHigh Energy Physics - Phenomenologyelectromagnetic [coupling]flavor [quark]description
Non-perturbatively computing the hadronic vacuum polarization at large photon virtualities and making contact with perturbation theory enables a precision determination of the electromagnetic coupling at the $Z$ pole, which enters global electroweak fits. In order to achieve this goal ab initio using lattice QCD, one faces the challenge that, at the short distances which dominate the observable, discretization errors are hard to control. Here we address challenges of this type with the help of static screening correlators in the high-temperature phase of QCD, yet without incurring any bias. The idea is motivated by the observations that (a) the cost of high-temperature simulations is typically much lower than their vacuum counterpart, and (b) at distances $x_3$ far below the inverse temperature $1/T$, the operator-product expansion guarantees the thermal correlator of two local currents to deviate from the vacuum correlator by a relative amount that is power-suppressed in $(x_3\:T)$. The method is first investigated in lattice perturbation theory, where we point out the appearance of an O$(a^2 \log(1/a))$ lattice artifact in the vacuum polarization with a prefactor that we calculate. It is then applied to non-perturbative lattice QCD data with two dynamical flavors of quarks. Our lattice spacings range down to 0.049 fm for the vacuum simulations and down to 0.033 fm for the simulations performed at a temperature of 250 MeV.
year | journal | country | edition | language |
---|---|---|---|---|
2021-01-01 | Journal of High Energy Physics |