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Thrust at N3LL with Power Corrections and a Precision Global Fit for alphas(mZ)

2010/06/30 by Riccardo Abbate, Michael Fickinger, Andre H. Hoang +2 · 1 citation
Physics and Astronomy · #hep-ph #hep-ex #nucl-th

paper · pdf · doi:10.1103/physrevd.83.074021

published as Phys.Rev.D83:074021,2011 · 45 pages, 21 figures, v2: added discussion of bin integration vs. cumulant differences; comparison to Becher & Schwartz improved; typo in Eq.55 fixed

arxiv created 2010/08/25 · arxiv updated 2011/05/12

Abstract

We give a factorization formula for the e+e- thrust distribution dsigma/dtau with tau=1-T based on soft-collinear effective theory. The result is applicable for all tau, i.e. in the peak, tail, and far-tail regions. The formula includes O(alphas3) fixed-order QCD results, resummation of singular partonic alphasj lnk(tau)/tau terms with N3LL accuracy, hadronization effects from fitting a universal nonperturbative soft function defined in field theory, bottom quark mass effects, QED corrections, and the dominant top mass dependent terms from the axial anomaly. We do not rely on Monte Carlo generators to determine nonperturbative effects since they are not compatible with higher order perturbative analyses. Instead our treatment is based on fitting nonperturbative matrix elements in field theory, which are moments Omegai of a nonperturbative soft function. We present a global analysis of all available thrust data measured at center-of-mass energies Q=35 to 207 GeV in the tail region, where a two parameter fit to αs(mZ) and the first moment Omega1 suffices. We use a short distance scheme to define Omega1, called the R-gap scheme, thus ensuring that the perturbative dsigma/dtau does not suffer from an O(LambdaQCD) renormalon ambiguity. We find alphas(mZ)=0.1135 ± (0.0002)expt ± (0.0005)hadr ± (0.0009)pert, with chi2/dof=0.91, where the displayed 1-sigma errors are the total experimental error, the hadronization uncertainty, and the perturbative theory uncertainty, respectively. The hadronization uncertainty in alphas is significantly decreased compared to earlier analyses by our two parameter fit, which determines Omega1=0.323 GeV with 16% uncertainty.

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