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下一个-到-下一个-到-领先的顺序 QCD 纠正半包罗的深不可弹性散射
Saurav Goyal1,2, Sven-Olaf Moch3, Vaibhav Pathak1,2
1<a href="https://ror.org/05078rg59">The Institute of Mathematical Sciences</a>, A CI of Homi Bhabha National Institute, Taramani, 600113 Chennai, India.
我们介绍了半包容深不可弹性散射的第一个次要次要顺序 (NNLO) 校正. 这些扰乱量子色态学计算显著降低了风味非单片子过程中的尺度依赖.
科学领域:
- 高能粒子物理学 高能粒子物理学
- 量子色态动力学 (QCD) 是一个
背景情况:
- 半包容深不可弹性散射 (SIDIS) 是探测子结构的一个关键过程.
- 扰乱性QCD计算对于高能物理学的精确理论预测至关重要.
研究的目的:
- 为了计算夸克启动的风味非单子SIDIS过程的次到次到首次顺序 (NNLO) 校正.
- 以分析的方式获得领先颜色的完整贡献.
- 评估NNLO校正对理论预测和规模依赖性的影响.
主要方法:
- 虚拟和真实发射费曼图的计算.
- 使用整合-按部分减少到主积分.
- 使用参数相位集成和微分方程的方法进行积分评估.
主要成果:
- 在领先的颜色中,分析已经获得了第一个完整的NNLO对风味非单片 SIDIS 过程的校正.
- 数字分析证实了NNLO纠正的实质性影响.
- 观察到剩余尺度依赖的显著减少.
结论:
- 在SIDIS中,NNLO校正对于准确的理论预测至关重要.
- 提出的计算为分析实验数据提供了一个更精确的理论框架.
- 缩小尺度依赖性增强了扰乱性QCD的预测能力.
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