$\mathcal{O}(\alpha_{\rm S}^2)$的QCD横向动量恢复的方位相关贡献

P. K. Dhani
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引用次数: 0

摘要

在软和共线极限下散射振幅的QCD分解产生的奇异因子在组织和计算硬散射截面的高阶微扰贡献方面起着突出的作用。在这次演讲中,我们从共线极限下散射振幅的分解结构出发,引入具有过程无关结构的共线函数。这些共线函数在全微分水平上定义,然后可以在适当的观测相关相空间上进行积分,以计算对相应观测的对数增强贡献。对于横向动量相关的可观测值,我们展示了如何在不引入文献中所谓的快速散度的情况下定义共线函数。本文给出了QCD微扰理论中次至次至上阶共线函数的显式计算结果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Azimuthally-correlated contributions to QCD transverse-momentum resummation at $\mathcal{O}(\alpha_{\rm S}^2)$
Singular factors originating from the QCD factorisation of scattering amplitudes in soft and collinear limits play a prominent role in both organising and computing high-order perturbative contributions to hard-scattering cross sections. In this talk, we start from the factorisation structure of scattering amplitudes in the collinear limit, and we introduce collinear functions that have a process-independent structure. These collinear functions, which are defined at the fully-differential level, can then be integrated over the appropriate observable-dependent phase space to compute logarithmically-enhanced contributions to the corresponding observable. For transverse-momentum dependent observables, we show how the collinear functions can be defined without introducing what is known as rapidity divergences in the literature. We present the results of explicit computations of the collinear functions up to next-to-next-to-leading order in the QCD perturbation theory.
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