arXivDaily arXiv每日学术速递 周一至周五更新
arXiv 0809.3326hep-ph
收藏

非微扰对$e^+ e^-$湮灭推力分布的贡献

Non-Perturbative Contribution to the Thrust Distribution in $e^+ e^-$ Annihilation

R. A. Davison, B. R. Webber

摘要:

根据最新的实验数据和最近的NNLO微扰计算结果,我们重新评估了非微扰对$e^+e^-\to$强子推力分布的贡献。通过将计算扩展到NNLO+NLL精度,我们进行了迄今为止最详细的研究,非微扰物理对这个可观察的影响。特别是,我们调查如何以及基于低尺度QCD有效耦合的模型可以解释这样的效果。我们发现,改进的微扰分布和实验数据之间的差异是一致的$1/Q$依赖的非微扰移动的分布,预测的有效耦合模型。使用$χ^2/d.o.f.=1.09$获得了$α_s(M_Z) = 0.1164^{+0.0028}_{-0.0026}$和$α_0(2 GeV)=0.59+/-0.03$的最佳拟合值。这与NLO+NLL结果一致,但拟合质量得到改善。在$α_0$的协议是不平凡的,因为1/Q依赖的贡献(红外renormalon)的一部分,包括在NNLO微扰校正。

英文摘要:

We re-evaluate the non-perturbative contribution to the thrust distribution in $e^+e^-\to$ hadrons, in the light of the latest experimental data and the recent NNLO perturbative calculation of this quantity. By extending the calculation to NNLO+NLL accuracy, we perform the most detailed study to date of the effects of non-perturbative physics on this observable. In particular, we investigate how well a model based on a low-scale QCD effective coupling can account for such effects. We find that the difference between the improved perturbative distribution and the experimental data is consistent with a $1/Q$-dependent non-perturbative shift in the distribution, as predicted by the effective coupling model. Best fit values of $α_s(M_Z) = 0.1164^{+0.0028}_{-0.0026}$ and $α_0(2 GeV)=0.59+/-0.03$ are obtained with $χ^2/d.o.f.=1.09$. This is consistent with NLO+NLL results but the quality of fit is improved. The agreement in $α_0$ is non-trivial because a part of the 1/Q-dependent contribution (the infrared renormalon) is included in the NNLO perturbative correction.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

↑