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A Precise Determination of $α_s$ from the C-parameter Distribution

André H. Hoang, Daniel W. Kolodrubetz, Vicent Mateu, Iain W. Stewart

Abstract

We present a global fit for $α_s(m_Z)$, analyzing the available C-parameter data measured at center-of-mass energies between $Q=35$ and $207$ GeV. The experimental data is compared to a N$^3$LL$^\prime$ + $\mathcal{O}(α_s^3)$ + $Ω_1$ theoretical prediction (up to the missing 4-loop cusp anomalous dimension), which includes power corrections coming from a field theoretical nonperturbative soft function. The dominant hadronic parameter is its first moment $Ω_1$, which is defined in a scheme which eliminates the $\mathcal{O}(Λ_{\rm QCD})$ renormalon ambiguity. The resummation region plays a dominant role in the C-parameter spectrum, and in this region a fit for $α_s(m_Z)$ and $Ω_1$ is sufficient. We find $α_s(m_Z)=0.1123\pm 0.0015$ and $Ω_1=0.421\pm 0.063\,{\rm GeV}$ with $χ^2/\rm{dof}=0.988$ for $404$ bins of data. These results agree with the prediction of universality for $Ω_1$ between thrust and C-parameter within 1-$σ$.

A Precise Determination of $α_s$ from the C-parameter Distribution

Abstract

We present a global fit for , analyzing the available C-parameter data measured at center-of-mass energies between and GeV. The experimental data is compared to a NLL + + theoretical prediction (up to the missing 4-loop cusp anomalous dimension), which includes power corrections coming from a field theoretical nonperturbative soft function. The dominant hadronic parameter is its first moment , which is defined in a scheme which eliminates the renormalon ambiguity. The resummation region plays a dominant role in the C-parameter spectrum, and in this region a fit for and is sufficient. We find and with for bins of data. These results agree with the prediction of universality for between thrust and C-parameter within 1-.

Paper Structure

This paper contains 21 sections, 43 equations, 19 figures, 5 tables.

Figures (19)

  • Figure 1: Bands for the profile functions for the renormalization scales $\mu_H$, $\mu_J(C)$, $\mu_S(C)$ when varying the profile parameters.
  • Figure 2: Plots of the $r$ dependence of $g_C(r)\, \Omega_1(R_\Delta,\mu_\Delta,r)$ for different values of $\theta(R_\Delta,\mu_\Delta)$. We normalize to $\Omega_1^C(R_\Delta,\mu_\Delta)$, since it is simply an overall multiplicative factor.
  • Figure 3: Difference between the default cross section and the cross section varying only one parameter. We vary $\alpha_s (m_Z)$ by $\pm\, 0.001$ (solid red), $2\,\Omega_1$ by $\pm \,0.1$ (dashed blue) and $\Omega_2^C$ by $\pm\,0.5$ (dotted green). The three plots correspond to three different center of mass energies: (a) $Q=35$ GeV, (b) $Q=91.2$ GeV, (c) $Q=206$ GeV.
  • Figure 4: The evolution of the value of $\alpha_s(m_Z)$ adding components of the calculation. An additional $\sim 8\%$ uncertainty from not including power corrections is not included in the two left points.
  • Figure 5: The first two panels show the distribution of best-fit points in the $\alpha_s(m_Z)$-$2\Omega_1$ and $\alpha_s(m_Z)$-$2\overline\Omega_1$ planes. Panel (a) shows results including perturbation theory, resummation of large logs, the soft nonperturbative function and $\Omega_1$ defined in the Rgap scheme with renormalon subtractions. Panel (b) shows the results as in panel (a), but with $\overline\Omega_1$ defined in the $\overline{\textrm{MS}}$ scheme without renormalon subtractions. In both panels the dashed lines corresponds to an ellipse fit to the contour of the best-fit points to determine the theoretical uncertainty. The respective total (experimental + theoretical) 39% CL standard uncertainty ellipses are displayed (solid lines), which correspond to $1$-$\sigma$ (68% CL) for either one-dimensional projection. The big points represent the central values in the random scan for $\alpha_s(m_Z)$ and $2\,\Omega_1$. Likewise, the two panels at the bottom show the distribution of best-fit points in the $\alpha_s(m_Z)$-$\chi^2/{\rm dof}$ plane. Panel (c) shows the $\chi^2/{\rm dof}$ values of the points given in panel (a), whereas panel (b) shows the $\chi^2/{\rm dof}$ values of the points given in panel (b).
  • ...and 14 more figures