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Precision Thrust Cumulant Moments at N^3LL

Riccardo Abbate, Michael Fickinger, Andre H. Hoang, Vicent Mateu, Iain W. Stewart

TL;DR

The paper advances precision thrust analyses by leveraging a full spectrum calculation that combines ${\cal O}(\alpha_s^3)$ fixed-order results, N^3LL resummation, and renormalon-free power corrections within an SCET-inspired framework. By performing a global fit to the first thrust moment, it extracts ${\alpha_s(m_Z)}$ and the leading nonperturbative parameter ${\Omega_1}$, and demonstrates that higher moments and cumulants cleanly expose subleading power corrections ${\Omega'_n}$ and related coefficients. The study shows cumulants are less sensitive to leading power corrections and thus ideal for probing higher-order nonperturbative effects, with a nonzero ${\tilde\Omega'_2}/Q^2$ extracted from $M'_2$. Overall, the work confirms consistency with previous tail analyses, improves theoretical uncertainty via renormalon subtraction, and highlights a path to characterize subleading power corrections across a broader set of event shapes.

Abstract

We consider cumulant moments (cumulants) of the thrust distribution using predictions of the full spectrum for thrust including O(alpha_s^3) fixed order results, resummation of singular N^3LL logarithmic contributions, and a class of leading power corrections in a renormalon-free scheme. From a global fit to the first thrust moment we extract the strong coupling and the leading power correction matrix element Omega_1. We obtain alpha_s(m_Z) = 0.1141 \pm (0.0004)_exp \pm (0.0014)_hadr \pm (0.0007)_pert, where the 1-sigma uncertainties are experimental, from hadronization (related to Omega_1) and perturbative, respectively, and Omega_1 = 0.372 \pm (0.044)_exp \pm (0.039)_pert GeV. The n-th thrust cumulants for n > 1 are completely insensitive to Omega_1, and therefore a good instrument for extracting information on higher order power corrections, Omega'_n/Q^n, from moment data. We find (\tilde Omega'_2)^(1/2) = 0.74 \pm (0.11)_exp \pm (0.09)_pert GeV.

Precision Thrust Cumulant Moments at N^3LL

TL;DR

The paper advances precision thrust analyses by leveraging a full spectrum calculation that combines fixed-order results, N^3LL resummation, and renormalon-free power corrections within an SCET-inspired framework. By performing a global fit to the first thrust moment, it extracts and the leading nonperturbative parameter , and demonstrates that higher moments and cumulants cleanly expose subleading power corrections and related coefficients. The study shows cumulants are less sensitive to leading power corrections and thus ideal for probing higher-order nonperturbative effects, with a nonzero extracted from . Overall, the work confirms consistency with previous tail analyses, improves theoretical uncertainty via renormalon subtraction, and highlights a path to characterize subleading power corrections across a broader set of event shapes.

Abstract

We consider cumulant moments (cumulants) of the thrust distribution using predictions of the full spectrum for thrust including O(alpha_s^3) fixed order results, resummation of singular N^3LL logarithmic contributions, and a class of leading power corrections in a renormalon-free scheme. From a global fit to the first thrust moment we extract the strong coupling and the leading power correction matrix element Omega_1. We obtain alpha_s(m_Z) = 0.1141 \pm (0.0004)_exp \pm (0.0014)_hadr \pm (0.0007)_pert, where the 1-sigma uncertainties are experimental, from hadronization (related to Omega_1) and perturbative, respectively, and Omega_1 = 0.372 \pm (0.044)_exp \pm (0.039)_pert GeV. The n-th thrust cumulants for n > 1 are completely insensitive to Omega_1, and therefore a good instrument for extracting information on higher order power corrections, Omega'_n/Q^n, from moment data. We find (\tilde Omega'_2)^(1/2) = 0.74 \pm (0.11)_exp \pm (0.09)_pert GeV.

Paper Structure

This paper contains 16 sections, 50 equations, 16 figures, 8 tables.

Figures (16)

  • Figure 1: Theoretical computations at various orders in perturbation theory for the total hadronic cross section at the Z-pole normalized to the Born-level cross section $\sigma_0$. Here the small blue points correspond to fixed order perturbation theory, green squares to resummation without renormalon subtractions, and red triangles to resummation with renormalon subtractions.
  • Figure 2: Theoretical prediction for the first three moments at the Z-pole at various orders in perturbation theory. The blue circles correspond to fixed order perturbation theory (normalized with the total hadronic cross section) at ${\cal O}(\alpha_s)$, ${\cal O}(\alpha_s^2)$ and ${\cal O}(\alpha_s^3)$, green squares correspond to resummed predictions at NLL, NNLL, and N${}^3$LL normalized with the total hadronic cross section, and red triangles correspond to resummation normalized with the norm of the resummed distribution. For these plots we use $\alpha_s(m_Z)=0.114$.
  • Figure 3: Theory scan for uncertainties in pure QCD with massless quarks. The panels are fixed order (top-left), resummation without the nonperturbative correction (top-right), resummation with a nonperturbative function using the $\overline{\textrm{MS}}$ scheme for $\overline\Omega_1$ (bottom-left), resummation with renormalon subtraction and a nonperturbative function in the Rgap scheme for $\Omega_1$ (bottom-right).
  • Figure 4: Difference between theoretical predictions with default parameters for the first moment as function of $Q$ when varying one parameter at a time. The red solid line corresponds to varying $\Delta\alpha_s(m_Z)=\pm 0.001$ and the blue dashed lines to varying $\Delta\Omega_1=\pm 0.1$, with respect to the pure QCD best-fit values. There is a strong degeneracy of the two parameters in the region $Q>100$ GeV, which is obviously broken when considering values of $Q$ below $70$ GeV.
  • Figure 5: Evolution of the best-fit values for $\alpha_s(m_Z)$ from thrust first moment fits when including various levels of improvement with respect to fixed order QCD. Only points at the right of the vertical dashed line include nonperturbative effects.
  • ...and 11 more figures