The thrust and heavy-jet mass distributions in the two-jet region
Einan Gardi, Johan Rathsman
TL;DR
The paper develops and applies Dressed Gluon Exponentiation (DGE) to thrust and heavy-jet mass distributions in the two-jet region of e+e− annihilation, combining renormalon-resummed perturbation theory with a shape-function description of non-perturbative corrections. By expressing both observables in terms of the single-jet mass distribution, it unifies hadronization effects and includes hadron-mass schemes to enable meaningful cross-observable comparisons. The thrust distribution is described well across energies when matched to NLO, while the heavy-jet mass is reliable only for ρ_H<1/6 due to kinematic phase-space limitations, which constrains extracting α_s from this observable. Importantly, fixing α_s from the thrust analysis yields consistent power corrections for both observables, supporting a renormalon-driven, hemisphere-uncorrelated shape-function picture in the peak region.
Abstract
Dressed Gluon Exponentiation (DGE) is used to calculate the thrust and the heavy-jet mass distributions in e+e- annihilation in the two-jet region. We perform a detailed analysis of power corrections, taking care of the effect of hadron masses on the measured observables. In DGE the Sudakov exponent is calculated in a renormalization-scale invariant way using renormalon resummation. Neglecting the correlation between the hemispheres in the two-jet region, we express the thrust and the heavy-jet mass distributions in terms of the single-jet mass distribution. This leads to a simple description of the hadronization corrections to both distributions in terms of a single shape function, whose general properties are deduced from renormalon ambiguities. Matching the resummed result with the available next-to-leading order calculation, we get a good description of the thrust distribution in a wide range, whereas the description of the heavy-jet mass distribution, which is more sensitive to the approximation of the phase space, is restricted to the range rho_H<1/6. This significantly limits the possibility to determine alpha_s from this observable. However, fixing alpha_s by the thrust analysis, we show that the power corrections for the two observables are in good agreement.
