论文标题
超高能量的顶级生产
Top pair production at ultra-high energies
论文作者
论文摘要
最高的夸克,是最重的夸克,也是当今所知的最重的基本粒子,它构成了夸克 - 格鲁恩相中长寿培养基的新颖探针,正如预期的那样,即使在超高能量的光核碰撞中也可以产生。在超高能域中,在顶部的颗粒产生中考虑了一些独特的特征。在量子染色体动力学和有效的现场理论方法中研究了抗top-top对的产生,用于计算总partononic横截面。所有可观察物的预测均在量子染色体动力学和LO中的NNLO计算。这些定量结果对于未来质量中心能量前沿的对撞机实验以及改进超高能域中宇宙射线级联反应的现象学模型的改进可能很重要。因此,该研究可以更好地了解重粒子的产生,并强调高能物理学对加速器和超高能宇宙射线测量的激动人心的相互关系。
The top quark, the heaviest quark and, indeed, the heaviest elementary particle known today, constitutes a novel probe of the long-lived medium in quark-gluon phase which, as expected, can be produced even in light nuclei collisions at ultra-high energies. Some distinctive features are considered for particle production in the top sector in ultra-high energy domain. The antitop-top pair production is studied within the quantum chromodynamics and effective field theory approach used for calculations of total partonic cross sections. Predictions for all observables are computed at NNLO in quantum chromodynamics and at LO in effective field theory. These quantitative results can be important for both the future collider experiments at center-of-mass energy frontier and the improvement of the phenomenological models for development of the cosmic ray cascades in ultra-high energy domain. Thus the study allows the better understanding of heavy particle production and emphasizes the exciting interrelation between the high-energy physics on accelerators and ultra-high energy cosmic ray measurements.